Global Meteor Network report 2025

By Paul Roggemans, Peter Campbell-Burns, Milan Kalina, Mark McIntyre, James M. Scott, Damir Šegon, and Denis Vida

Abstract: A status report is presented for the Global Meteor Network. Since the start of the network, 2847823 meteoroid orbits have been collected up to the end of 2025 and 418 different meteor showers have been identified among these orbits. During 2025, more than 236 new GMN cameras started contributing successfully paired meteors. 966063 orbits were collected in 2025. The development of the Global Meteor Network in different regions is described. The coverage of the camera fields of view is shown on maps.

 

1  Introduction

Over the past 20 years many video camera networks were created, both regional and national, with the aim of obtaining meteor trajectories through multi-station registrations. Most of these networks specialize in fireballs and meteorite droppers, others are dedicated to a fainter magnitude range comparable to what visual observers used to cover. The orbit data obtained by these networks brought a tremendous progress in our knowledge of meteoroid streams.

The Global Meteor Network is the most recent development in this domain. Its success builds on the many years of expertise of the Croatian Meteor Network, one of the pioneers in the field of video meteor observations and the origin of GMN (Gural and Šegon, 2009). Based on RMS, the significantly improved Raspberry Pi solution introduced by Zubović et al. (2015) and Vida et al. (2016), the Global Meteor Network began its operation at the end of 2018; its first six cameras located in New Mexico used IP cameras controlled by a Raspberry running its own dedicated software and reduction pipeline (Vida et al., 2021). GMN became the fastest growing meteor video network with 76 operational cameras at the end of 2019, 172 at the end of 2020, 390 at the end of 2021, 700 at the end of 2022, 1066 in 2023, 1213 by the end of 2024 and 1365 in 2025. In 2025 236 new cameras got operational, 12 non-active in 2024 resumed capturing, 96 cameras active in 2024 did no longer contribute in 2025, bringing the total number of decommissioned cameras at 254.

2  Joining the Global Meteor Network

More information about this project can be found in Vida et al. (2020a; 2020b; 2021; 2022) and on the GMN website. An informative video presentation about the Global Meteor Network project can be watched online. Many sites and participants are still waiting to find partners to improve the coverage on their cameras. New participants are welcome to expand the network.

To obtain a camera for participation you can either buy it plug&play from Istrastream, or you buy the components and build your own camera for about 250 US$ or ~200 €. The RMS cameras are easy to build and operate. If you are interested in building your own camera you can find detailed instructions online.

The daily status of most (not all) meteor stations can be followed on the GMN weblog or on the GMN status pages per country. The GMN results and data are publicly available and daily updated online. The UK meteor network maintains a comprehensive archive and daily update which may inspire others. Their Wiki-page may be helpful to people outside the UK as well as their github repos, see also here.

The meteor map is an online tool for visualizing meteor cameras and ground tracks of observed meteors. Each participant can check the results obtained with each camera, check the location of the meteor trajectories and combinations with other camera stations. The tool has been described in an article (Dijkema, 2022). Milan Kalina developed another tool, “Meteorview” to map meteor trajectories with several extra functionalities described in an article (Kalina, 2024). Steve Matheson generated the GMN Status viewer that rapidly summarizes the nightly activity.

As the static maps of camera FoVs presented in this report sometimes become overcrowded, the aggregated kml files valid for end of 2025 can be downloaded. The individual up-to-date kml-files for all GMN cameras can be downloaded from the GMN website. Camera operators are encouraged to point new cameras in function of optimal coverage with other cameras. Opening the kml files in Google Earth allows to toggle cameras on and off to get a better view on the actual coverage. Make sure to compare kml files at the same elevation (e.g. 100 km) and prevent 3D perspective by changing the properties in the Google Earth graphical interface to “clamped to ground” instead of the default setting “absolute”.

If you have a dark site with a free view and if you are looking to make a scientifically useful contribution, with just five RMS cameras with 3.6 mm lenses (FoV 88° × 47°) pointed at azimuths 0° (North), 70°, 140°, 220° and 290°, between 35° and 40° elevation, you cover all the sky except your zenith. Avoid pointing a camera at the meridian (180° azimuth) as the transit of the Full Moon will take full effect in this position. Also do not point lower than 35° elevation; there are no meteors in the local scenery, trees or buildings. If you use 6 mm lenses, recommended where light pollution is an issue, you need six RMS to cover the sky with a royal overlap between the camera edges. Six cameras with 6 mm lenses (FoV 54° × 30°) pointed at azimuths 30°, 90°, 150°, 210°, 270° and 330°, between 35° and 40° elevation, would make you a key video meteor hub in the network. Building the cameras at the cost of the purchased components, or bought plug & play, both remain a low-cost project, affordable to many amateurs, observatories and societies.

The unavailability of Raspberry Pi because of production limitations due to Covid in former years has been meanwhile solved, but inspired people to explore alternative systems for unavailable RPi’s. A cheap Linux PC can handle multiple cameras and a system has been developed to operate multiple GMN cameras using a single PC. Read the article written by Harman et al. (2023) and check the Wiki pages for the latest updates.

3 Annual GMN meeting 2025 (online)

The annual meeting of the Global Meteor Network got more than 100 people participating online from around the globe. The meeting took place in two sessions on February 8–9, 2025 in order to allow people from all time zones to participate. 23 presentations were given with enough time for questions and discussions; each session ended with a Q&A workshop session. Both sessions can be viewed online:

• Session 1 – February 8, 16^h00^m – 21^h00^m UTC
• Session 2 – February 9, 00^h00^m – 03^h00^m UTC

4 GMN camera coverage

The aim of the GMN is to cover all latitudes and longitudes to assure a global coverage of meteor activity in order to let no unexpected meteor event pass unnoticed. This is an ambitious goal especially for a project that depends for most efforts entirely on volunteers’ work. In this report we describe the progress that was made by GMN during 2025 in different regions of the world. The status of the camera coverage is illustrated with maps showing the fields of view intersected at an elevation of 100 km in the atmosphere, projected and clamped to the ground. This way the actual overlap between the camera fields is shown without any effects of 3D perspectives. Where possible the camera ID has been mentioned on the plots.

Many RMS cameras with 4 mm optics have the horizon at the bottom of their field of view, which results in a huge camera field at 100 km elevation. Rather few meteors will be bright enough to get registered near the horizon. The large distance between the camera station and the meteor also reduces the chances to obtain a useable triangulation. The number of paired meteors at the outskirts of these large camera fields is very small. However, cameras pointing so low towards the horizon turn out to be very useful regarding obtaining coverage at lower heights where meteorite dropping fireballs end their visible path. When looking for camera overlap, it is strongly recommended to look for an optimized overlap between cameras. An interesting study on this topic for the New Mexico Meteor Array has been published by Mroz (2021). Camera operators are encouraged to optimize their camera overlap.

The number of multi-station events mentioned per country corresponds to the number of orbits, unless an orbit was based on camera data from different countries, then it was counted once for each country. This can also be visualized on the MeteorMap (Dijkema, 2022) or with MeteorView (Kalina, 2024). The current camera coverage is presented per country or per region for reason of readability. To consider the real overlap for most European countries it is necessary to look at the camera coverage of neighboring countries. In several regions the camera coverage is too dense to visualize it in a single map. We strongly recommend to view the camera FoVs in Google Earth. The required kml-files have been grouped per country and can be downloaded for: Asia, Europe, North America, Africa and Southern hemisphere.

4.1 AQ – Antarctica

On 11 March 2025 the first seven cameras were installed on Antarctica. No multiple station meteors and thus no orbits were obtained yet as there isn’t yet a partner station for coverage (Figure 1).

4.2 AT – Austria

Austria got its first RMS (AT0002), generating orbits since August 2024, and the second camera (AT0004) had its first orbits in October 2024, good for 1701 orbits in 2024. The two Austrian GMN cameras contributed 4819 orbits in 2025, most of which combined with GMN cameras in neighboring countries, see Figure 2.

 

4.3 AU – Australia

The first 31 meteor orbits by Australian RMS cameras were registered in September 2021 when the first five cameras got ready to harvest meteors. By the end of 2021, twelve cameras managed to obtain 1871 orbits in the final 4 months of 2021. A first breakthrough was achieved in 2022 as the number of RMS cameras in Australia increased to 29, good for 12460 orbits in 2022. The expansion of the network accelerated even more in 2023 with 66 operational cameras contributing 40712 orbits making Australia one of the major contributors to GMN. Nine cameras active in 2023 were decommissioned, but 31 new cameras were added in 2024. This resulted in a major breakthrough in 2024 with 88 cameras contributing as many as 100044 orbits (see Table 5). Eleven cameras stopped capturing, while four new were installed and one resumed capture in 2025. With 82 cameras 111155 orbits were obtained. The all-time number of orbits is 266242 for Australia, twenty cameras were decommissioned so far.

 

Most cameras were installed in Western Australia (Figure 4) but there is also a dense network in the eastern states of Australia with more cameras in Victoria, Queensland and New South Wales (Figure 5). Australia being a very large country, describing its camera networks as a single network is a bit unfair as it is like considering all European countries as a single EU network.

4.4 BA – Bosnia and Herzegovina

In August 2025, five GMN cameras were installed in Bosnia and Herzegovina with a lot of overlap with cameras in Croatia and other countries in the region (Figure 6). In the final months of the year, these cameras contributed 6153 orbits to GMN.

4.5 BE – Belgium

Belgium had its first RMS cameras operational in early 2019. Figure 7 shows the GMN coverage at the end of 2025 for Belgium. The map can be compared with the situation end of 2024 in the previous GMN annual report (Roggemans et al., 2025).

Most of the Belgian RMS cameras were installed for the reinforcement of the CAMS-BeNeLux. For this purpose, the 6 mm lenses are preferred which have less distortion than the 3.6 mm and detect more fainter meteors. GMN started in Belgium with four cameras in 2019 recording 921 orbits in 2019 and 5500 orbits in 2020. Six more cameras were installed in 2021, when 8582 orbits were collected. The network expanding to twenty cameras in 2022 when exceptional favorable weather resulted in 23174 orbits. In 2023, 23 cameras were active and had 25443 orbits. Although the weather was significantly less favorable in 2024, 34049 orbits were collected with 28 operational cameras. As many as 15 extra cameras were installed in 2025 and with 43 cameras, 53244 orbits were collected. The all-time number of orbits for Belgium is 150913. The only two decommissioned cameras so far will be hopefully reinstalled in 2026. Belgian cameras have many paired meteors with those in neighboring countries, France, Germany, Netherlands and the United Kingdom. Especially the overlap from cameras of the largest and most successful network in the UK result in many good combinations. Some cameras in Belgium have been installed to improve the coverage on Northern France.

4.6 BR – Brazil

The BRAMON network had its first two RMS cameras getting paired meteors in October 2020 good for 40 orbits with two cameras in the last quarter of 2020. The network expanded to 13 operational cameras, good for 1645 orbits in 2021. In 2022 the number of cameras increased to 20 and 2760 orbits were obtained. In 2023 the number of cameras increased to 34 but the number of paired meteors dropped to 2331. With 37 cameras contributing to orbits in 2024, 4753 orbits were collected. In 2025, nine cameras were decommissioned and eight new cameras were installed. With 36 cameras 9949 meteoroid orbits were obtained, a record for Brazilian GMN cameras so far. The all-time number of orbits is 21478 for Brazil. This is a huge country and most RMS cameras are installed in the southern part (Figure 8). Some cameras are installed waiting for coverage from other cameras. Further optimization of the network could increase the number of orbits a lot as these longitudes need more observing capacity to cover southern hemisphere meteor activity.

4.7 BG – Bulgaria

Bulgaria had its first RMS camera operational in June 2021 and got three cameras installed by the end of 2021 of which two had 419 multi-station events. In April 2022 a 4^th RMS and in July 2022, two extra cameras were installed. With 6 cameras in 2022, 3877 orbits could be collected. Seven operational cameras had 3530 orbits in 2023. As many as ten extra cameras were installed in 2024, good for 15058 meteor orbits. One camera was decommissioned in 2025, and with 16 cameras 12297 orbits were recorded. The Bulgarian RMS cameras also get paired meteors with cameras in Greece and in Romania (Figure 8).

4.8 CA – Canada

The Canadian GMN network had its first five operational RMS cameras providing orbits in June 2019 and expanded to 11 cameras by the end of 2019, good for 3599 orbits. The number of cameras increased to 17 by the end of 2020 with 10815 orbits registered. During 2021, 15 new camera IDs appeared in the list and 8809 orbits were recorded with 29 cameras in 2021, less than the year before despite the extra cameras. The number of cameras doubled from 29 to 58 in 2022 resulting in 16232 orbits. In 2023 the number of contributing cameras increased to 67, resulting in 15023 orbits. The number of operating cameras dropped to 51 in 2024, good for 18508 orbits. In 2025, 13 cameras were decommissioned, one resumed and ten new installed. With 49 cameras, 20576 meteoroid orbits were collected. In total 50 Camera IDs that worked in previous years have been decommissioned since the start of the project.

Two smaller sub-networks existed, CAWE (Elginfield) and CAWT (Tavistock). Each of both networks had eight cameras, but Tavistock stopped observing in 2023. Six new cameras were added at Elginfield in 2025. A small network in the Calgary region of Alberta had its first orbits in 2022 (Figure 12) and continued in 2025. Most cameras are installed in Quebec and Southern Ontario, ideal for volunteers south of the Canadian border in the US. Some cameras in New Found Land still wait for a multi-station partner (Figure 10).

 

4.9 HR – Croatia

Croatia was the first European country in May 2019 to harvest orbits with three RMS cameras. By the end of 2019 Croatia had already 23 cameras successfully contributing in triangulations, good for 12221 multi-station events. The number of cameras increased to 32 in 2020 resulting in 35099 orbits that year. 38370 multi-station events were recorded in 2021 with 48 cameras. 2022 was slightly less successful with 31329 orbits and 45 operational cameras. In 2023 the number of cameras slightly decreased at 41 contributing to 27721 orbits. In 2024, 35726 orbits were collected with 43 operational cameras. In 2025 six cameras were decommissioned, but 12 new installed and 13 inactive cameras from 2024 resumed capturing. With 50 cameras in 2025, 57060 orbits were collected. In total Croatia contributed 237526 orbits to the GMN orbit database. 22 cameras have been decommissioned since the start.

Croatia plays a major role in the coordination of GMN, maintaining the IstraStream service to produce and deliver new cameras for many countries and providing technical assistance to participants in the GMN project worldwide. The Croatian cameras provide a huge overlap on the neighboring countries (Figure 13). A number of Croatian cameras have a very small FoV to register fainter meteors with higher positional accuracy. To view these camera fields in detail we refer to the online KML files for consultation in Google Earth.

 

4.10 CK – Cook Island

The Cook Islands is a nation in the South Pacific and its 15 islands are scattered over a vast area. The Global Meteor Network got the first camera installed at this geographically interesting location. So far, we wait for multi station coverage.

4.11 CL – Chile

In June 2025, two GMN cameras were installed in Chile to cover strategic longitudes in the Southern Hemisphere. Thanks to a favorable climate, 1907 orbits were collected by these two cameras at observatories La Silla and El Sauce. Further camera enhancement and FOV optimization is planned in 2026.

4.12 CZ – Czech Republic

The first three RMS in the Czech Republic scored 163 orbits in 2020, with four cameras in 2021, 464 orbits were recorded and 2490 orbits with six cameras in 2022. A major breakthrough happened in 2023 as the number of cameras increased to twenty, good for 11269 orbits. In 2024, five more cameras were installed and a total of 18248 orbits were collected. In 2025 one camera was decommissioned and four new added, 28 cameras harvested 25668 orbits. In total Czech GMN cameras captured 58302 orbits.

Since the end of 2022, the Czech and Slovak GMN camera operators are grouped in the CSMON (Czech & Slovak Meteor Observation Network), which helps the new and current meteor enthusiasts to get on board. In addition to individual amateur astronomers, there is an increasing number of public observatories getting equipped by RMS cameras, thanks to public funding. Latest advances in the SBC (Pi5) technology allows to multiply the numbers of cameras on the same PC, i.e. make it even more accessible for low budgets.

 

4.13 DK – Denmark

In October 2022 a first GMN camera was operational in Denmark, good for 55 orbits that year. In 2023 four cameras were active in Denmark, and these obtained 1386 orbits. A fifth camera was added in 2024 and 3360 orbits were collected. The GMN network underwent a spectacular expansion in Denmark in 2025 with 22 new GMN cameras being added and the establishment of the Nordic Meteor Network. With 27 cameras, 20522 orbits were collected bringing the all-time total to 25323 orbits for Danish cameras. These northern cameras create possibilities for further camera coverage in southern Norway and Sweden as well as in Northern Germany (Figure 17).

4.14 FI – Finland

In October 2022 the first GMN cameras became operational at two sites in Finland, with 41 orbits as a first result. In 2023 there were five cameras active which resulted in 90 orbits and in 2024 three more cameras were installed and 204 orbits obtained. In 2025 one new camera was added and with 8 of the 9 cameras 407 orbits were obtained (Figure 18).

4.15 FR – France

The number of RMS cameras in France increased gradually from 10 in 2020 with 3176 orbits registered, to 14 devices in 2021 with 5601 orbits and 16 cameras in 2022 with 11990 orbits. More new cameras were installed in 2023 and 16682 orbits were obtained with 18 cameras. In 2024 there were 19 operational cameras in France contributing 20592 orbits to the GMN dataset. In 2025, 27617 orbits were collected with 20 cameras.  In total 28 RMS cameras were installed since March 2020, but eight of them did not function anymore in 2025.  The all-time total of orbits is 85658 for France. A large part of France, the entire south-western, is still without GMN coverage (Figure 19).

4.16 DE – Germany

The first GMN camera in Germany had its first orbits in August 2019 with Belgian GMN cameras. By the end of 2019 there were four GMN cameras in Germany, good for 200 orbits. The number of cameras increased to 10 and the numbers of orbits to 3963 in 2020. With 12 cameras in 2021, 7009 orbits were collected, in 2022, with 18 cameras 9128 orbits were collected. In 2023 as many as 12194 orbits were recorded with 19 cameras. In 2024 the number of cameras in Germany increased with 11 to 30, good for 23240 orbits. 32 cameras in 2025 resulted in 37570 orbits, bringing the total score at 93304 orbits for Germany. Two cameras were decommissioned so far. Some GMN cameras in the North-Western part of Germany also participate in the CAMS-BeNeLux network, supporting both GMN and CAMS (Figure 20).

4.17 GR – Greece

In September 2022 the first GMN camera got operational in Greece, ideally pointed to overlap with some Bulgarian GMN cameras and it was good for 977 paired meteors in the four last months of 2022. Three extra cameras were installed and with four cameras 3375 orbits were obtained in 2023. Four more cameras were installed in 2024 and with eight operational cameras 8998 orbits were obtained. The same number of cameras resulted in 16865 orbits in 2025 bringing the all-time total at 30215 orbits for Greece (Figure 21).

4.18 – Greenland

The most northern GMN camera, GL0001, installed in the North West of Greenland at 77°28’ northern latitude. During the late autumn and winter months, this site has almost permanent night time. A second camera was installed in 2025. The possibilities are being considered to install more cameras at favorable distances for triangulations.

4.19 – Hungary

A first GMN camera was operational in March 2022 in Hungary and by end of 2022, two Hungarian cameras had obtained 2114 orbits. One new camera was added in 2023 and the Hungarian cameras contributed 7872 orbits. The number of cameras remained status quo in 2024 and produced 9626 orbits, mainly paired meteors with Croatian and Czech cameras. A break-through happened in 2025 when nine new cameras got installed and 19870 meteors were recorded bringing the all-time total for Hungary at 39482 orbits.

4.20 IE – Ireland

Ireland got a first GMN operational in October 2020 and a second one a month later, good for 120 orbits in 2020. With three cameras in 2021 the number of orbits increased to 424. 3490 orbits were recorded in 2022 with five GMN cameras. In 2023 the number of cameras remained unchanged but the number of orbits dropped to 1954. In 2024 two new cameras were added and one previously active RMS stopped uploading data. With six available cameras, 3706 orbits were obtained. In 2025 the number of cameras remained at six, but 6692 orbits were obtained, the best year so far for Ireland. The all-time total of orbits is 16386 for Ireland. Most of the paired meteors were obtained thanks to the overlap provided by GMN cameras in the UK.

4.21 IL – Israel

Israel had its first three GMN cameras installed in November 2020, good for 553 orbits that year. In 2021 with three extra cameras 2009 orbits were obtained. In 2022 the cameras did not provide orbits during some periods of time and one camera was discontinued, resulting in 975 orbits. In 2023, 1096 orbits were collected using six cameras. In 2024 an extra camera was installed and with seven cameras, 991 orbits were collected. In 2025 six cameras had 681 orbits. In total three cameras were decommissioned, the all-time number of orbits for Israel is 6305.

4.22 IT – Italy

Italy had its first GMN camera installed and contributed to orbits in October 2019, and was good for 862 orbits. Italy remained with one GMN camera in 2020, which had as many as 5384 paired meteors with Croatian and Slovenian cameras. Italy increased its number of cameras to five and these cameras were involved in 5447 multi-station events in 2021. An extra camera was added in Bologna in 2022 and 4943 orbits were collected. With seven cameras in 2023, 5064 orbits were obtained. In 2024, 6603 orbits were obtained with seven cameras. The number of cameras remained unchanged in 2025 and 9249 orbits were collected, so far the best year.  Three cameras were decommisioned before 2025 and the all-time number of orbits is 37489 for Italy. More cameras in Italy would allow to cover much more of the atmosphere over the Mediterranean Sea.

 

4.23 JP – Japan

A first GMN camera was installed in Japan in 2022, waiting for some multi-station partners at suitable distance for triangulation. In 2023 a second camera was installed which allowed to obtain 629 orbits. The network remained status quo in 2024 with two cameras and 606 orbits. In 2025 a third camera was installed and 147 orbits recorded. The all-time number of orbits for GMN in Japan is 1382. Japan has the very active SonotaCo network which, uses analog Watec cameras. RMS cameras deliver UFO capture output which may offer opportunities for the SonotaCo network to include GMN cameras in its network.

4.24 KR – Korea (South)

A most impressive deployment of GMN cameras took place in 2022 in South Korea with a first few cameras obtaining orbits in September and as many as 47 GMN cameras installed in November and December 2022. The cameras were installed and pointed to obtain an optimal overlap resulting in 7711 orbits during the first year. In 2023 the number of cameras rapidly increased to 125 (!) collecting 34044 orbits. This fast deployment made the RMS network in South Korea a major contributor at a strategic geo-location at the northern hemisphere for a 24 on 24-hour monitoring of meteor activity.

In 2024 three cameras were decommissioned, 122 operational cameras captured 42477 orbits. 123 operational cameras obtained 63284 orbits in 2025, the best year so far for South Korea. The all-time number of orbits stands at 147516. The dense coverage of overlapping camera fields in 2025 can be compared to the situation end of 2022 in Figure 28. If any RMS cameras are installed in South-Western Japan, these would generate many paired meteors with the Korean cameras.

4.25 – Luxembourg

In October 2022 a first GMN camera was installed in Luxembourg in combination contributing to 622 orbits with Belgian, Dutch, French, German and even Czech GMN cameras (Figure 29). In 2023 this camera had 2018 paired meteors with orbits and in 2024, 2194 orbits were obtained. In 2025 a second camera was installed in Luxembourg and 4133 orbits were recorded. The all-time number of orbits for Luxembourg stands at 8967. With many cameras in Belgium, France and Germany, extra cameras in Luxembourg can score many multi-station events.

4.26 MY – Malaysia

A first GMN camera was installed in Malaysia in 2021 but waited for coverage from cameras installed at suitable distances to get good triangulations. Some extra cameras were installed in 2022, and in June 2022 the first orbits were obtained. In total 50 orbits were collected in 2022 with three cameras. In 2023 a ten-fold of orbits, 501, were collected with five cameras. In 2024, 246 orbits were obtained with six cameras, two new cameras were added and two cameras were decommissioned. With 10 cameras, 258 orbits were obtained in 2025. The all-time total of orbits stands at 1055 for Malaysia. Further extensions of the Malaysian network are very welcome. Extra cameras in the western part of Malaysia could give coverage on the camera in Singapore.

4.27 MX – Mexico

An impressive deployment of GMN cameras took place in Mexico in 2022. The first few installed cameras obtained the first orbits in February 2022 and soon twelve cameras were installed with a good overlap. A total of 1769 meteor orbits were collected in 2022. The number of cameras increased to 15 in 2023 with 2953 orbits as a result. In 2024 13 cameras recorded 2871 orbits, two cameras were decommissioned. Eleven cameras remained in 2025 and recorded 1134 orbits. The all-time number of orbits is 8727 for Mexico. The efforts in Mexico are crucial in getting coverage for both the northern and especially the southern hemisphere at these longitudes (Figure 31).

4.28 MA – Morocco

The first two GMN cameras obtained their first meteor orbits in May 2024, and a third camera was added in July. The Moroccan GMN cameras collected 851 orbits in 2024 and 1312 in 2025, despite frequent technical issues that prevented recording meteors much of the time (Figure 32).

4.29 NL – Netherlands

The Netherlands started collecting orbits within GMN in August 2019 with two cameras and had 278 orbits in this first year. The number of GMN cameras increased to eleven in 2020 with 4337 orbits as a result. The number of cameras remained unchanged in 2021 but the better overlap from neighboring countries resulted in 7605 orbits. Some cameras dropped off in 2022 and a few new ones were installed, resulting in 9139 orbits from 13 cameras. In 2023, 14 Dutch RMS cameras had 9421 orbits. In 2024 four new RMS cameras were installed, with a total of 18 cameras 17409 orbits were collected. A major breakthrough came in 2025 when 13 new GMN cameras were added, most of them built during a workshop where interested people could assemble their camera under supervision of experienced GMN camera operators. 33566 orbits were obtained with 31 cameras in 2025, the best year so far.  The Netherlands have five decommissioned RMS cameras. Dutch cameras get mainly multi-station coverage from cameras in Belgium, Germany, the UK and Denmark (Figure 33). The all-time total number of orbits is 81755 for the Netherlands.

4.30 NZ – New Zealand

The first two GMN cameras were installed in July 2021 in New Zealand and 1146 orbits were obtained that year. From March 2022 more cameras were installed month by month with an impressive deployment of strategically placed well pointed cameras covering the huge surface of the country. With 28 active cameras at the end of 2022, 6280 orbits were recorded. The New Zealand GMN network, known as Fireballs Aotearoa, was further expanded in 2023 and with a total of 111 cameras 47436 orbits were obtained, making New Zealand one of the most important providers of orbit data for the Southern Hemisphere. The density of the camera coverage can be seen in Figure 34 and compared to the situation three years earlier. In 2024, 44 extra cameras became operational and three older cameras decommissioned. With a total of 152 cameras, 147831 meteor orbits were collected. In 2025, five cameras were decommissioned, one older camera resumed capturing, and 36 new cameras were added to the network. 182324 orbits were collected with the 184 available cameras. This makes New Zealand the greatest orbit contributor within the Global Meteor Network, doing better than the GMN network in the USA that covers a much larger volume of atmosphere to intercept meteoroids. The all-time number of collected orbits is 385017 for New Zealand, with seven cameras decommissioned.

4.31 NO – Norway

The two first GMN cameras were installed in Norway in December 2024, but so far without paired meteors as calibration failed. The cameras are pointed south and should combine well with cameras in Denmark, Germany and the United Kingdom (Figure 35). Unfortunately, the cameras are currently listed as decommissioned.

4.32 PL – Poland

The first GMN camera was installed in September 2020 and remained long the only Polish GMN camera with 35 orbits in 2020 and 67 orbits in 2021. In March 2022 two extra Polish GMN cameras got their first 35 orbits. The cameras didn’t function all the time but the number of orbits obtained increased to 398 in 2022. In 2023 only two cameras were active and 456 orbits were collected. In 2024 two new cameras were installed and 1759 orbits obtained. Eight new cameras were added in 2025 and 7486 orbits collected with eleven operational cameras. The all-time number of orbits is 10201. Polish GMN cameras get mainly paired meteors with cameras installed in Czechia and Germany (Figure 36).

4.33 PT – Portugal

A first GMN camera got meteor orbits in September 2022 in Portugal. A vast coverage from GMN cameras in Spain guarantees many paired meteors (Figure 37). In 2022, 327 orbits were recorded, in 2023 the total increased to 3322 orbits. A second camera was installed in January 2024 and with two cameras, 4413 orbits were obtained. The two Portuguese cameras collected 4067 orbits in 2025, bringing the all-time total at 12129 for Portugal.

 

4.34 RO – Romania

Romania had its first three RMS cameras installed in 2023. Operational since October 2023 and despite unfavorable weather, 417 orbits were collected. The network in Romania remained status quo in 2024, but RO0003 failed functioning in February. With only two functioning cameras, 4361 meteor orbits were collected. In December 2025 three new cameras got installed and 4426 orbits were collected this year. The all-time number of orbits is 9204 for Romania. These cameras had many paired meteors with Bulgarian, Croatian, Czech and Hungarian cameras. Several new camera systems have been commissioned for installation in 2026.

4.35 RU – Russia

The first two GMN cameras in Russia had orbits in July 2019 in Southern Russia (Figure 39). The first year had already 5715 orbits with 10 cameras. In 2020 the number of cameras increased to 21, good for as many as 13438 orbits. The number of RMS cameras having paired meteors remained stable at 21, but the number of orbits decreased to 6208 in 2021. Problems with the maintenance of some meteor stations reduced the number of paired observations. In 2022, 19 cameras in Russia had 5437 orbits. The number of Russian GMN cameras decreased further to 15 in 2023 and the number of paired meteors dropped to 1992. In 2024 seven new cameras were installed and with 22 cameras, 10939 meteor orbits were obtained. In 2025 two cameras were decommissioned and one new added, good for 10553 orbits in 2025. The all-time number of orbits for Russia is 54282. In total 14 of the formerly active cameras were decommissioned.

Some single RMS devices were installed elsewhere in Russia, like near St. Petersburg and Kazan, some other cameras are still waiting for coverage from other sites at a suitable distance. Some cameras are installed in the far east of Russia at longitude ~132° east and 50° north (Figure 40).

 

4.36 SG – Singapore

A first camera was installed in 2022 and is waiting for multi-station partners, no orbits could be obtained yet in 2025. Multi-station work should be possible with nearby cameras in Malaysia (Figure 41).

4.37 SK – Slovakia

Slovakia got its first camera in November 2021 with 37 paired meteors. In 2022, three GMN cameras got operational good for 2026 orbits. The number of cameras increased to four in 2023 and 5535 paired meteors with orbits were recorded by Slovakian cameras. In March 2024 a fifth camera was installed and 7532 orbits were obtained. The five cameras recorded 6943 orbits in 2025 bringing the all-time number of orbits at 22073 for Slovakia (Figure 42). Since the end of 2022, the Czech and Slovak GMN camera operators are grouped in the CSMON (Czech & Slovak Meteor Observation Network), which helps the new and current meteor enthusiasts to get on board.

4.38 SI – Slovenia

Slovenia had its first RMS contributing in August 2019 and a second RMS in August 2021. The coverage with mainly cameras in neighboring Croatia, resulted in 2753 orbits in 2019, 3999 in 2020 and 6001 in 2021. The two Slovenian cameras contributed to 5887 orbits in 2022. In 2023, four extra cameras were installed and 6789 orbits were collected. The number of cameras remained status quo in 2024 with six, and 12209 orbits were obtained. A new camera was added in 2025 and 14741 orbits were collected. The all-time total of orbits for Slovenia is 52379 (Figure 43).

4.39 ES – Spain

The GMN had its first orbits collected in Spain in April 2020. End of 2020, eight GMN cameras had collected 1207 orbits. A lot of progress was made in Spain in 2021 when the number of cameras increased from eight to 23. The 23 Spanish cameras were involved in 15113 multi-station events in 2021. The number of GMN cameras increased further to 30 in 2022 and resulted in 19301 orbits. In 2023, 22610 orbits were obtained with 35 cameras. In 2024 three new cameras were installed but six older cameras were decommissioned so that the number of operational cameras decreased to 32. 16771 meteor orbits were recorded in 2024. One camera was decommissioned and two new installed in 2025, resulting in 12599 orbits. Four cameras are installed at the Canary Islands (Figure 45). The all-time total of orbits is 87601 for Spain.

4.40 CH – Switzerland

The first orbits were obtained in August 2021 but it took until May 2022 before extra cameras were installed and more orbits recorded. With five operational cameras 3439 orbits were obtained in 2022. The central location of Switzerland is ideal to obtain multi-station events with GMN cameras in the neighboring countries. The number of cameras remained unchanged in 2023 and the number of paired meteors increased to 4352. In 2024 one camera was decommissioned and with the remaining four cameras, 2383 meteor orbits were obtained. In 2025 four cameras collected 3808 orbits. The all-time number of orbits is 13985 for Switzerland.

4.41 TJ – Tajikistan

The country has a long tradition in meteor astronomy and observations. In June 2024 two GMN cameras installed in Tajikistan had their first paired meteors. In total 411 meteor orbits were obtained despite technical issues that limited the time both cameras were operational. In 2025 the cameras collected 794 orbits. The all-time total of orbits stands at 1205 for Tajikistan (Figure 47).

4.42 UA – Ukraine

A first RMS camera contributes meteor data to Global Meteor Network in Ukraine in 2024 but no paired meteors were recorded. In 2025 five more cameras joined GMN and 1896 orbits were recorded. This is an amazing achievement in a country that suffers under war conditions.

4.43 UK – United Kingdom

The GMN started with 13 cameras in 2020 in the UK, which contributed 1889 orbits. These numbers rapidly grew in 2021 to 97 cameras and 27430 orbits. The largest expansion came in 2022 when 191 cameras contributed 78652 paired meteors. The network continued to grow throughout 2023 when 261 cameras contributed 84688. In 2024 the UK had 95730 orbits with 283 cameras. 30 cameras quit, 24 new were installed and 2 resumed operations, with 279 cameras 139838 orbits were obtained in 2025, best result for the UK so far. The all-time total number of orbits for the U.K. is 428227, 56 cameras were decommissioned in past years. The vast majority of the UK cameras are part of the UK Meteor Network which now provides complete coverage of the UK and Eire (Figure 49), see also the kml file.

 

Cameras

UK camera numbers have now more or less stabilized, with 279 different cameras contributing to trajectories during the year, slightly down from 2024. There were 242 active cameras in January and while around 40 new cameras came online during the year, the same number were decommissioned for various reasons.  Almost all the cameras are contributing to UKMON.

The cameras along the eastern side of the UK overlap well with cameras in Europe, and 134 different non-UK cameras contributed to matches with UK cameras with the number per month increasing from around 50 to over 100 by the end of the year (Figure 50). There were contributions from cameras in Belgium, the Czech Republic, Croatia, Germany, Denmark, France, Ireland, Luxembourg and the Netherlands.

Matches

UK cameras contributed to 132530 trajectories in 2025, about 14% of the total reported by GMN.  As might be expected, the latter half of the year was more active, with December, November and August being the most active months.

As noted above, many UK stations’ data matched with stations in Europe – 23708 trajectories also involved cameras from other countries. This shows the importance of a global network as many of these meteors might have been missed, or been analyzed less robustly, without contributions from across Europe.

On average, five stations were involved in each match, and generally there were more stations involved in each match than in prior years, with 90% of trajectories involving up to ten stations. Furthermore, 99 trajectories involved twenty or more stations, and the maximum number of involved stations was 36. Figure 51 shows the number of detections on the left axis, and the number of involved stations on the horizontal axis for up to 15-station matches.

 

Geographic coverage

Geographic range was roughly similar to 2024, with trajectories obtained for events between 45.6 and 60.5 North, and between 12.7 West and 10.5 East, covering an area of about two million square kilometers.  This equates to about six meteors per year, per ten-kilometer square. When viewed in this context, it is perhaps less surprising that two fireballs were seen a few months apart over the same general area.

Fireballs

Although only 46 fireballs were recorded by UKMON (defining a fireball as having a visual magnitude of brighter than –4), around 1000 detections had an absolute magnitude between –4 and –5, and a further 400 were brighter than this. Many of these were offshore or very distant from cameras and hence with a lower visual magnitude. Nonetheless its likely there were more meteorite-dropping events than we thought. From analysis of trajectories at least three or four of the 46 visual fireballs probably dropped meteorites, though searches were unsuccessful.

Showers

41336 meteors were classified as members of 270 separate showers. 9382 of these were Geminids, 6119 were Perseids, 2711 were Quadrantids and 2123 were Orionids. Other showers had fewer than 1000 meteors each, with 120 showers having fewer than 100 detections.

Looking forward

UK camera growth seems to have peaked south of the Edinburgh-Glasgow line, where every part of the island is covered by at least two cameras, and cameras pointing offshore cover Europe, Eire and the seas around the UK.

We’d like to see more in the West and Highlands of Scotland, though the terrain makes pointing cameras more challenging, and low-elevation detections and matches are less likely. The further north regions of the UK are also a challenge due to lack of darkness in the summer, and generally less clement weather in the winter.

4.44 US – United States

The American New Mexico Meteor Array was the pioneering network of the GMN as it started to harvest meteors in December 2018 with six cameras, producing the first 497 orbits for GMN. It remained the only data provider for GMN until May 2019 when the first 3 Croatian cameras started to deliver orbits. At the end of 2019, the number of US cameras had increased to 20 when the network collected 27643 orbits that year. In 2020, the 33 operational cameras in the US collected as many as 50537 orbits. With 72 RMS cameras registering paired meteors in the US, a total of 91637 orbits were obtained in 2021.

The number of GMN cameras involved in orbit determinations had increased to 100 in 2022, good for 114054 orbits. 2023 saw a further increase in cameras resulting in 120162 orbits. With 141 operational cameras in 2024, 135819 meteor orbits were collected. In 2025 five cameras had been decommissioned, 35 new systems were installed, two resumed capturing, with 173 operational cameras 181237 orbits were collected in 2025. The all-time number of orbits for the USA is 721920. Until 2025 the USA had 17 decommissioned GMN cameras.

Figure 52 shows the GMN status like it was at the end of 2025 with 173 GMN cameras in the US, most of which belong to the New Mexico Camera Array and the Lowell Observatory in Arizona. Both networks are independent in neighboring states but have a large overlap. Figure 54 shows the situation for the Lowell network in Arizona. The Lowell Observatory cameras also benefit coverage from other GMN cameras in the state as well as in California (Figure 53).

GMN camera networks are emerging at several other sites in the US (Figure 52). The network reaches till Alaska at 65° northern latitude. Several cameras installed near the East Coast, south of the Canadian border connect to the existing GMN network in Canada (Figure 55). The maps show where cameras in the US still wait for multi-station partners to set up cameras (Figure 56). The density of the overlap of the camera fields of view is better consulted in Google Earth with the kml file aggregated for all North American cameras.

4.45 ZA – South Africa

The first two GMN cameras were installed at the end of 2022 but no paired meteors were obtained then. In 2023 the number of cameras increased to four and the first 200 orbits were obtained in South Africa. Major progress was made in 2024 when the number of operational cameras doubled and 2294 meteor orbits were recorded. In 2025 four new cameras were installed and 11396 orbits were collected (Figure 57). Four cameras were stationed at two schools and there is interest from several more schools giving hope to expand the number of cameras in South Africa further in 2026. The all-time total of orbits is 13890 for South Africa. The geographical position of South Africa makes this network of strategic interest for the coverage of southern hemisphere meteor activity.

 

5 GMN statistics 2025

When a first GMN status report was published, including all data until end October 2020, 140 operational cameras were involved and 144950 orbits had been collected (Roggemans, 2021). Now, we can compare seven years of GMN work. Figure 58 shows the accumulated number of orbits obtained and the number of contributing cameras during each calendar month. The rapid growth of the Global Meteor Network is obvious. The number of cameras involved in collecting orbits for GMN increased from 390 in 2021 to 700 in 2022, 1066 in 2023, 1213 in 2024 and 1365 in 2025.

In 2025 GMN has installed 236 new cameras while 96 cameras that were active in 2024 did no longer have paired meteors. Twelve cameras that had stopped in 2024 resumed contributing to multi-station events. Since 2018 there have been 1621 cameras contributing to paired meteors of which 254 were decommissioned.

Table 2 shows that only 32% of all orbits are collected during the first six months of each year, while 68% is obtained in the period July to December. The fast expansion of the Global Meteor Network also means that more cameras were available towards the end of each year than at the beginning of each year, what also influenced the number of orbits obtained. The most important cause for the difference in number of orbits between the first and last six months is the meteor activity itself. Apart from the most active major meteor showers like the Perseids, Taurids, Orionids, Leonids and Geminids, the overall meteor activity is much higher during the second half of the year. This can be seen very well in Figure 58 where the blue curve has a much steeper increase each second half of the year.

Although 1365 different cameras contributed paired meteors during 2025, only 1115 or 82% were successfully contributing during December (Table 3). The explanation is that this report is based on the camera IDs which occur in the orbit dataset and thus successfully recorded paired meteors. Apart from the 1115 successful cameras in December there were also a number of cameras functioning without having any paired meteors and thus not listed in the orbit dataset. Persistent unfavorable weather in winter with ice and snow sometimes prevent some cameras from getting paired meteors at the Northern Hemisphere. If a camera somehow has no calibration, no trajectories can be calculated.

Occasionally some hardware or network problem occur, if the connection with the camera board gets lost, the system may ping its camera unsuccessfully until the camera owner fixes the problem. Another frequent hardware problem is when the sd card crashes and needs replacement. To prevent loss of valuable observing data, it is strongly recommended

to look regularly at the weblog page to check if all cameras report correctly to GMN. The GMN status page is another handy tool that shows all cameras per country color coding the status of all cameras in a single view. This page has additional features, including fields of view, sorting of data, presentation of daily data etc.

Table 4 lists the number of orbits obtained by the cameras per country. Meteors don’t care about borders and many multi-station events are recorded by stations in different countries. In that case the orbit has been counted for each different country that provided camera data for the trajectory solution.

Table 5 lists the number of cameras active per country for each year since 2018. The number of camera IDs that contributed no paired meteors in 2025 has been also listed per country. In some cases, old devices were replaced by new, in other cases the camera owner somehow was unable to solve technical issues, had lack of time or lost interest. Unfortunately, some camera operators have died.

The number of operational devices tend to stabilize above 1100 active cameras. New cameras compensate the loss of older devices. There are still critical longitudes where global coverage of meteor activity requires more cameras, mainly at the Southern Hemisphere in South America and Southern Africa.

Table 2 – Total number of orbits obtained by the Global Meteor Network per calendar month for each year.

	2018	2019	2020	2021	2022	2023	2024	2025	Totals
January	–	564	7539	9919	23727	23972	45613	62373	173707
February	–	1284	5330	6529	14910	18602	31316	49527	127498
March	–	537	5101	8767	15409	16310	33960	64809	144893
April	–	876	7213	9655	15658	22713	38029	55227	149371
May	–	1242	5654	10217	16951	22050	39834	67921	163869
June	–	1523	5700	7954	13463	23125	38336	55659	145760
July	–	1961	10973	11325	25226	35109	67402	88341	240337
August	–	5387	19422	31292	47300	65155	112442	125815	406813
September	–	6058	14012	21189	29984	44174	62041	88586	266044
October	–	11978	13097	31501	48360	59134	81356	96024	341450
November	–	7710	13228	30381	37895	54030	67862	93761	304867
December	497	11143	17826	33059	45785	67520	89364	118020	383214
Totals	497	50263	125095	211788	334668	451894	707555	966063	2847823

 

Table 3 – Total number of operational cameras with paired meteors within the Global Meteor Network per calendar month.

	2018	2019	2020	2021	2022	2023	2024	2025	Totals
January		9	75	152	363	591	910	1025	1303
February		9	80	161	380	583	911	1038	1302
March		9	86	182	410	609	940	1072	1342
April		10	91	200	418	648	942	1070	1366
May		15	101	216	458	665	956	1077	1393
June		22	111	232	466	680	953	1064	1394
July		29	117	239	483	720	969	1091	1432
August		52	122	285	507	806	1016	1144	1495
September		55	131	304	510	821	1007	1128	1497
October		65	122	316	542	842	990	1137	1499
November		71	142	326	571	873	1000	1132	1495
December	6	73	155	341	571	896	1000	1115	1518
Totals	6	76	172	390	700	1066	1213	1365	1621

Table 4 – Total number of multi-station events contributing to an orbit result, recorded in each country for each year. The list is sorted on the country ID used in the camera ID. Subnetworks for some countries are counted in the grand total for the country.

	2018	2019	2020	2021	2022	2023	2024	2025	Totals
Austria (AT)	0	0	0	0	0	0	1702	4819	6521
Australia (AU)	0	0	0	1871	12460	40712	100044	111155	266242
Bosnia and Herzegovina (BA)	0	0	0	0	0	0	0	6153	6153
Belgium (BE)	0	921	5500	8582	23174	25443	34049	53244	150913
Bulgaria (BG)	0	0	0	419	3877	3530	15058	12297	35181
Brazil (BR)	0	0	40	1645	2760	2331	4753	9949	21478
Canada (CA)	0	3599	10815	8809	16232	15023	18508	20576	93562
Switzerland (CH)	0	0	0	3	3439	4352	2383	3808	13985
Chile (CL)	0	0	0	0	0	0	0	1907	1907
Czech Republic (CZ)	0	0	163	464	2490	11269	18248	25668	58302
Germany (DE)	0	200	3963	7009	9128	12194	23240	37570	93304
Denmark (DK)	0	0	0	0	55	1386	3360	20522	25323
Spain (ES)	0	0	1207	15113	19301	22610	16771	12599	87601
Finland (FI)	0	0	0	0	41	90	204	407	742
France (FR)	0	0	3176	5601	11990	16682	20592	27617	85658
Greece (GR)	0	0	0	0	977	3375	8998	16865	30215
Croatia (HR)	0	12221	35099	38370	31329	27721	35726	57060	237526
Hungary (HU)	0	0	0	0	2114	7872	9626	19870	39482
Ireland (IE)	0	0	120	424	3490	1954	3706	6692	16386
Israel (IL)	0	0	553	2009	975	1096	991	681	6305
Italy (IT)	0	862	5384	5447	4943	5064	6603	9249	37552
Japan (JP)	0	0	0	0	0	629	606	147	1382
South Korea (KR)	0	0	0	0	7711	34044	42477	63284	147516
Luxembourg (LU)	0	0	0	0	622	2018	2194	4133	8967
Morocco (MA)	0	0	0	0	0	0	851	1312	2163
Mexico (MX)	0	0	0	0	1769	2953	2871	1134	8727
Malasia (MY)	0	0	0	0	50	501	246	258	1055
Netherlands (NL)	0	278	4337	7605	9139	9421	17409	33566	81755
New Zealand (NZ)	0	0	0	1146	6280	47436	147831	182324	385017
Poland (PL)	0	0	35	67	398	456	1759	7486	10201
Portugal (PT)	0	0	0	0	327	3322	4413	4067	12129
Romania (RO)	0	0	0	0	0	417	4361	4426	9204
Russia (RU)	0	5715	13438	6208	5437	1992	10939	10553	54282
Slovenia (SI)	0	2753	3999	6001	5887	6789	12209	14741	52379
Slovakia (SK)	0	0	0	37	2026	5535	7532	6943	22073
Tajikistan (TJ)	0	0	0	0	0	0	411	794	1205
Ukraine (UA)	0	0	0	0	0	0	0	1896	1896
United Kingdom (UK)	0	0	1889	27430	78652	84688	95730	139838	428227
USA (US)	497	27643	50607	91901	114054	120162	135819	181237	721920
Erroneous entry (XX)	0	0	0	8	28	0	123	0	159
South Africa (ZA)	0	0	0	0	0	200	2294	11396	13890

 

 

 

 

Table 5 – Total number of operational cameras with paired meteors in each country for each year. Inactive devices and cameras without orbits are not counted. The list is sorted on the country ID used in the camera ID. Subnetworks for some countries are counted in the grand total for the country. The column ‘Quit’ lists the number of cameras which had paired meteors before 2025 but did not appear in the 2025 data and are therefore considered as decommissioned.

	2018	2019	2020	2021	2022	2023	2024	2025	Totals	Quit
Austria (AT)	0	0	0	0	0	0	2	2	2	0
Australia (AU)	0	0	0	12	29	66	88	82	102	20
Bosnia and Herzegovina (BA)	0	0	0	0	0	0	0	5	5	0
Belgium (BE)	0	4	4	10	20	23	28	43	45	2
Bulgaria (BG)	0	0	0	2	6	7	17	16	18	2
Brazil (BR)	0	0	2	13	20	34	37	36	52	16
Canada (CA)	0	11	17	29	51	51	46	43	77	34
Canada (CAWE)	0	0	0	0	7	8	4	6	14	8
Canada (CAWT)	0	0	0	0	0	8	1	0	8	8
Switzerland (CH)	0	0	0	1	5	5	4	4	5	1
Chile (CL)	0	0	0	0	0	0	0	2	2	0
Czech Republic (CZ)	0	0	3	4	6	20	25	28	29	1
Germany (DE)	0	4	10	12	18	19	30	32	34	2
Denmark (DK)	0	0	0	0	1	4	5	27	27	0
Spain (ES)	0	0	8	23	30	35	32	33	41	8
Finland (FI)	0	0	0	0	4	5	7	8	8	0
France (FR)	0	0	10	14	16	18	19	20	28	8
Greece (GR)	0	0	0	0	1	4	8	8	8	0
Croatia (HR)	0	23	32	48	45	41	43	50	72	22
Hungary (HU)	0	0	0	0	2	3	3	12	12	0
Ireland (IE)	0	0	2	3	5	5	6	6	9	3
Israel (IL)	0	0	3	6	5	6	7	6	9	3
Italy (IT)	0	1	1	5	5	7	7	7	10	3
Japan (JP)	0	0	0	0	0	2	2	3	3	0
South Korea (KR)	0	0	0	0	47	125	122	123	128	5
Luxembourg (LU)	0	0	0	0	1	1	1	2	2	0
Morocco (MA)	0	0	0	0	0	0	3	3	3	0
Mexico (MX)	0	0	0	0	12	15	13	11	15	4
Malasia (MY)	0	0	0	0	3	5	6	10	11	1
Netherlands (NL)	0	2	11	11	13	14	18	31	36	5
New Zealand (NZ)	0	0	0	2	28	111	152	184	191	7
Poland (PL)	0	0	1	1	3	2	4	11	13	2
Portugal (PT)	0	0	0	0	1	1	2	2	2	0
Romania (RO)	0	0	0	0	0	3	3	5	6	1
Russia (RU)	0	10	21	21	19	15	22	21	35	14
Slovenia (SI)	0	1	1	2	2	6	6	7	7	0
Slovakia (SK)	0	0	0	1	3	4	5	5	5	0
Tajikistan (TJ)	0	0	0	0	0	0	2	2	2	0
Ukraine (UA)	0	0	0	0	0	0	0	5	5	0
United Kingdom (UK)	0	0	13	97	191	261	283	279	335	56
USA (US)	6	20	33	72	100	128	141	173	190	17
USA (US0)	6	20	24	36	51	78	97	124	133	9
USA (USL)	0	0	9	36	47	45	41	41	48	7
USA (USN)	0	0	0	0	0	3	1	5	6	1
USA (USV)	0	0	0	0	2	2	2	3	3	0
Erroneous entry (XX)	0	0	0	1	1	0	1	0	1	1
South Africa (ZA)	0	0	0	0	0	4	8	12	12	0

 

6   Meteor showers covered by GMN

Using the Working List of Meteor Showers (Jenniskens et al., 2020; Jopek and Kaňuchová, 2017; Jopek and Jenniskens, 2011; Neslušan et al., 2020) as a reference, 387 of the showers listed could be associated with orbits collected by the Global Meteor Network. The number of orbits recorded for each of these showers is listed in
Table 6 for each year since 2018.

The GMN meteor shower association was originally based on the table of Sun-centered ecliptic shower radiant positions given in Jenniskens et al. (2018). However, in May 2023 it was concluded that the list had some imperfections and therefore it was decided to make GMN’s own meteor shower list and redo the meteor shower associations from the past. The new reference list contained 387 meteor showers instead of the 425 in the previous list. Meanwhile, new discovered activities and known showers that were missing in the list have been added bringing the total number of meteor showers monitored by GMN at 418. Still, many entrees of the IAU MDC Working List of Meteor Showers have no matching orbits in the GMN database and most of these meteor showers are not included in the GMN list for reasons explained below. Some of the showers are periodic and display only some activity once every few years, some showers have been detected by radar in a fainter range of magnitudes than what GMN cameras cover and others are known as daylight meteor showers. While GMN is getting better coverage at the southern hemisphere, more of the low declination meteor showers are getting covered. For many of the listed meteoroid streams their absence in the GMN orbit database can be explained because the evidence for the existence of the shower is still missing. One of the goals of the GMN project is to help to identify ghost meteor showers that should be removed from the Working List.

Table 6 serves as an inventory of what the GMN orbit database has available until end 2025. Of course, the number of shower members detected depends on the criteria used to associate a meteor with a known meteor shower radiant. The GMN shower association criterion assumes that meteors within 1° in solar longitude, within 3° in radiant, and within 10% in geocentric velocity of a shower reference location are members of that shower. Further details about the shower association are explained in Moorhead et al. (2020). This is a rather strict criterion since meteor showers often have a larger dispersion in radiant position and velocity. Therefore, using the orbit similarity criteria (Drummond, 1981; Southworth and Hawkins, 1963; Jopek, 1993) will certainly detect more shower candidates but at the risk of including sporadic orbits that fulfil similarity criteria by pure chance.

In 2025 a number of case studies on GMN meteoroid orbit data to document meteor shower activities have been published:

• New meteor shower in Cassiopeia, 4 September 2024
• New meteor shower in Ursa Minor, 23–24 September 2024
• New meteor shower in Lyra, 26–27 October 2024
• New meteor shower in Puppis
• New meteor shower in Octans
• New meteor shower in Equuleus
• New meteor shower in Indus
• June delta Pavonids (JDP#835) in 2025
• Two meteor shower outbursts with potential connection to comet 73P/Schwassmann-Wachmann
• New meteor shower in Eridanus
• Outburst of a new meteor shower in Aries
• New meteor shower in Delphinus (M2025-S1)
• M2024-S1 activity confirmed in 2025
• Epsilon-Ursae Minorids (EPU#1044) enhanced activity in 2025
• New meteor shower in Hydrus (M2025-S2)
• Delta-Horologiids (DHO#1146) in 2025
• October epsilon-Carinids (OEC#1172)
• A Carinids (842#CRN) outburst in 2025
• New meteor shower in Pegasus (M2025-U1)
• New meteor shower in Monoceros (M2025-V1)
• 29-Piscids (PIS#1046) return in 2025
• M2024-H1 activity confirmed in 2025
• M2024-N1 activity confirmed in 2025
• Eccentrids in the GMN orbit dataset

The main goal of the GMN, not to let any meteor shower activity pass unnoticed, is being achieved. Whenever some unexpected meteor activity occurs, the Global Meteor Network has good chances to cover it. Many of the existing showers monitored by GMN are still awaiting independent confirmation to be nominated by the IAU-MDC staff to get the status of an established shower.

More case studies on poorly known meteor showers are possible thanks to the statistically relevant numbers of shower meteors recorded by GMN for many of these meteoroid streams that wait to be better documented. Therefore, it is most important to keep as many cameras operational around the globe.

More information and detailed documentation about meteor showers can be found in the new reference work “Atlas of Earth’s Meteor Showers” that appeared in October 2023 (Jenniskens, 2023).

Table 6 – Total number of orbits according to the meteor shower association (IAU number + code) for each year.

		2018	2019	2020	2021	2022	2023	2024	2025	Total
Spo#-1	Sporadics	294	35624	88579	145663	231788	318794	519521	707068	2047331
CAP#1	alpha-Capricornids	0	94	604	451	1147	1840	3845	4740	12721
STA#2	Southern Taurids	0	765	838	1934	2178	3575	4564	5765	19619
SIA#3	Southern iota-Aquariids	0	11	27	39	52	116	267	271	783
GEM#4	Geminids	130	2117	5959	9968	15800	19655	13814	37342	104785
SDA#5	Southern delta-Aquariids	0	269	1271	1225	3190	4138	10056	13999	34148
LYR#6	April Lyrids	0	30	531	743	1066	1451	1235	2703	7759
PER#7	Perseids	0	1231	6192	11407	15126	22003	35890	32234	124083
ORI#8	Orionids	0	2045	2501	4556	9576	10417	10664	12708	52467
DRA#9	October Draconids	0	2	4	7	11	6	295	19	344
QUA#10	Quadrantids	0	13	561	1216	1070	1017	2798	5535	12210
EVI#11	eta-Virginids	0	2	38	283	241	82	139	1562	2347
KCG#12	kappa-Cygnids	0	15	78	1773	85	107	180	222	2460
LEO#13	Leonids	0	272	683	953	1548	2362	2281	3443	11542
URS#15	Ursids	4	84	244	169	325	402	745	832	2805
HYD#16	sigma-Hydrids	4	356	488	1613	1263	2737	4287	3456	14204
NTA#17	Northern Taurids	0	344	579	965	1053	2397	2161	2902	10401
AND#18	Andromedids	0	40	71	920	175	216	226	333	1981
MON#19	December Monocerotids	8	118	239	593	531	1291	1438	1712	5930
COM#20	Comae Berenicids	13	259	574	680	1660	1686	2347	3169	10388
AVB#21	alpha-Virginids	0	10	107	123	142	368	394	673	1817
LMI#22	Leonis Minorids	0	83	103	193	357	436	539	789	2500
EGE#23	epsilon-Geminids	0	100	116	347	510	624	753	920	3370
NOA#25	Northern October delta-Arietids	0	115	159	183	294	437	392	725	2305
NDA#26	Northern delta-Aquariids	0	99	393	476	774	1265	1792	2300	7099
KSE#27	kappa-Serpentids	0	2	12	29	26	54	76	78	277
SOA#28	Southern October delta-Arietids	0	73	143	318	124	576	706	360	2300
ETA#31	eta-Aquariids	0	162	503	1321	2446	2575	7948	10243	25198
NIA#33	Northern iota-Aquariids	0	64	132	215	230	382	623	740	2386
ZCY#40	zeta-Cygnids	0	10	120	203	303	347	357	636	1976
DLI#47	mu-Virginids	0	4	56	33	143	205	214	188	843
TAH#61	tau-Herculids	0	0	0	1	1243	1	3	2	1250
GDE#65	gamma-Delphinids	0	1	6	27	26	36	45	72	213
SSG#69	Southern mu-Sagittariids	0	16	48	67	81	354	674	974	2214
SLY#81	September Lyncids	0	11	76	104	75	197	214	228	905
ODR#88	omicron-Draconids	0	3	18	17	46	31	53	71	239
PVI#89	January pi-Virginids	0	1	19	48	89	105	208	196	666
NCC#96	Northern delta-Cancrids	0	26	77	86	245	204	388	490	1516
SCC#97	Southern delta-Cancrids	2	47	121	104	278	272	498	674	1996
PIH#101	pi-Hydrids	0	79	127	290	469	649	1196	1437	4247
ACE#102	alpha-Centaurids	0	0	0	0	29	40	319	382	770
BTU#108	beta-Tucanids	0	0	0	0	1	28	29	3	61
AAN#110	alpha-Antliids	0	3	20	10	61	48	76	159	377
DPA#120	delta-Pavonids	0	0	0	0	0	0	0	128	128
DME#130	delta-Mensids	0	0	0	0	5	57	215	259	536
ELY#145	eta-Lyrids	0	7	39	148	209	181	289	368	1241
NOP#149	Northern May Ophiuchids	0	4	22	12	18	61	110	146	373
SOP#150	Southern May Ophiuchids	0	3	9	25	15	70	144	151	417
EAU#151	epsilon-Aquilids	0	23	76	109	230	303	563	588	1892
NOC#152	Northern Daytime omega-Cetids	0	2	4	8	9	12	13	31	79
OCE#153	Southern Daytime omega-Cetids	0	0	0	0	0	0	0	16	16
SSC#161	Southern omega-Scorpiids	0	10	7	38	21	50	102	70	298
NZC#164	Northern June Aquilids	0	63	331	304	709	1005	1966	2368	6746
SZC#165	Southern June Aquilids	0	19	74	93	226	408	1287	1229	3336
JBO#170	June Bootids	0	1	3	0	35	5	0	2	46
ARI#171	Daytime Arietids	0	6	14	32	34	46	90	113	335
JPE#175	July Pegasids	0	24	145	221	404	669	960	1048	3471
PHE#176	July Phoenicids	0	1	0	11	49	221	650	940	1872
OCY#182	omicron-Cygnids	0	1	20	20	31	34	41	67	214
PAU#183	Piscis Austrinids	0	5	33	40	52	104	352	191	777
GDR#184	July gamma-Draconids	0	8	124	66	175	127	322	413	1235
EUM#186	epsilon-Ursae Majorids	0	0	13	6	14	22	33	25	113
PCA#187	psi-Cassiopeiids	0	4	19	33	56	80	71	87	350
BPE#190	beta-Perseids	0	8	27	33	96	75	151	186	576
ERI#191	eta-Eridanids	0	49	117	183	328	642	1614	1464	4397
UCE#194	upsilon-Cetids	0	28	56	114	200	272	393	443	1506
AUD#197	August Draconids	0	92	237	320	460	714	858	1014	3695
ADC#199	August delta-Capricornids	0	0	0	0	0	0	0	1	1
AUR#206	Aurigids	0	29	50	128	152	157	265	371	1152
SPE#208	September epsilon-Perseids	0	85	220	411	310	833	865	882	3606
BAU#210	beta-Aurigids	0	41	118	159	250	340	374	609	1891
KLE#212	Daytime kappa-Leonids	0	2	4	6	7	24	12	29	84
NPI#215	Northern delta-Piscids	0	58	114	123	253	237	386	643	1814
SPI#216	Southern delta-Piscids	0	26	52	52	96	175	156	386	943
NDR#220	nu-Draconids	0	28	58	51	91	169	165	312	874
DSX#221	Daytime Sextantids	0	5	3	22	42	34	66	89	261
SOR#225	sigma-Orionids	0	43	76	118	218	310	394	463	1622
XDR#242	xi-Draconids	0	9	24	66	72	136	131	139	577
ZCN#243	zeta-Cancrids	0	1	9	22	15	26	25	23	121
NHD#245	November Hydrids	0	7	24	81	66	131	154	152	615
AMO#246	alpha-Monocerotids	0	25	22	40	73	80	138	138	516
NOO#250	November Orionids	0	232	273	821	1047	953	2127	1797	7250
ALY#252	alpha-Lyncids	0	1	6	10	16	8	15	31	87
CMI#253	December Canis Minorids	1	33	60	100	158	189	298	343	1182
PHO#254	Phoenicids	0	0	0	0	0	0	53	12	65
ORN#256	Northern chi-Orionids	3	112	127	233	376	423	611	828	2713
ORS#257	Southern chi-Orionids	2	183	247	525	688	971	1330	1671	5617
OCT#281	October Camelopardalids	0	28	9	55	149	55	163	129	588
FTA#286	omega-Taurids	0	87	66	156	492	206	537	1162	2706
DSA#288	Southern December delta-Arietids	1	38	76	111	220	259	355	579	1639
DNA#289	Northern December delta-Arietids	0	17	22	126	96	96	237	251	845
TPU#307	tau-Puppids	0	1	0	3	11	31	86	91	223
PIP#308	January pi-Puppids	1	18	16	36	66	108	321	300	866
MVE#318	mu-Velids	0	8	19	35	49	107	200	251	669
JLE#319	January Leonids	0	0	9	5	24	13	33	56	140
LBO#322	lambda-Bootids	0	1	15	29	70	56	86	81	338
XCB#323	xi-Coronae Borealids	0	0	17	31	41	65	92	54	300
EPR#324	epsilon-Perseids	0	0	12	3	12	17	17	27	88
EPG#326	epsilon-Pegasids	0	8	25	33	52	59	104	126	407
SSE#330	sigma-Serpentids	0	3	4	0	8	4	8	5	32
AHY#331	alpha-Hydrids	0	6	32	43	161	62	405	496	1205
OCU#333	October Ursae Majorids	0	41	52	150	139	295	176	296	1149
DAD#334	December alpha-Draconids	2	99	169	406	481	606	817	940	3520
XVI#335	December chi-Virginids	0	54	82	115	163	289	352	400	1455
DKD#336	December kappa-Draconids	0	106	35	293	149	423	668	309	1983
NUE#337	nu-Eridanids	0	234	423	850	1309	1849	2746	3678	11089
OER#338	omicron-Eridanids	0	132	146	308	435	718	946	1147	3832
PSU#339	psi-Ursae Majorids	0	30	25	124	62	150	291	129	811
TPY#340	theta-Pyxidids	1	22	39	63	154	194	400	451	1324
XUM#341	January xi-Ursae Majorids	0	0	22	31	50	133	135	152	523
HVI#343	h-Virginids	0	10	148	6	2	7	116	505	794
FHE#345	f-Herculids	0	1	13	30	75	49	77	157	402
XHE#346	x-Herculids	0	3	33	53	96	84	123	193	585
BPG#347	beta-Pegasids	0	0	1	7	4	5	8	19	44
ARC#348	April rho-Cygnids	0	7	84	119	232	205	175	488	1310
LLY#349	lambda-Lyrids	0	0	3	2	4	6	7	15	37
DTR#351	Daytime Triangulids	0	0	0	0	0	0	0	12	12
JMC#362	June mu-Cassiopeiids	0	3	23	56	66	44	69	81	342
PPS#372	phi-Piscids	0	66	286	354	841	952	1301	2189	5989
ALN#376	August Lyncids	0	5	11	19	31	45	49	105	265
OLP#384	October Leporids	0	12	14	36	50	74	102	109	397
OBC#386	October beta-Camelopardalids	0	21	24	71	117	115	155	177	680
CTA#388	chi-Taurids	0	61	62	195	202	288	377	394	1579
THA#390	November theta-Aurigids	8	105	202	507	387	693	947	1026	3875
NID#392	November i-Draconids	0	16	39	74	79	126	136	177	647
ACA#394	alpha-Canis Majorids	1	23	15	51	77	107	203	190	667
GCM#395	gamma-Canis Majorids	1	27	60	39	130	132	323	363	1075
GUM#404	gamma-Ursae Minorids	0	0	30	19	54	162	103	165	533
DPI#410	delta-Piscids	0	2	12	17	54	98	69	355	607
CAN#411	c-Andromedids	0	18	130	205	411	439	652	882	2737
SIC#416	September iota-Cassiopeiids	0	5	32	43	42	82	108	111	423
SOL#424	September-October Lyncids	0	16	62	77	181	178	245	439	1198
FED#427	February eta-Draconids	0	1	7	3	27	11	31	106	186
DSV#428	December sigma-Virginids	2	60	120	222	407	395	711	805	2722
ACB#429	alpha-Coronae Borealids	0	6	23	18	103	115	71	161	497
JIP#431	June iota-Pegasids	0	2	15	11	60	106	68	138	400
ZCS#444	zeta-Cassiopeiids	0	22	139	262	392	624	644	613	2696
KUM#445	kappa-Ursae Majorids	0	21	55	125	111	154	161	141	768
DPC#446	December phi-Cassiopeiids	0	12	11	71	89	40	357	54	634
AAL#448	April alpha-Librids	0	3	19	26	54	52	94	173	421
AED#450	April epsilon-Delphinids	0	3	15	27	48	49	93	127	362
CAM#451	Camelopardalids	0	3	1	2	6	6	2	7	27
MPS#456	May psi-Scorpiids	0	28	89	139	211	390	493	935	2285
JEC#458	June epsilon-Cygnids	0	5	41	61	43	128	107	99	484
JEO#459	June epsilon-Ophiuchids	0	39	28	10	47	110	90	154	478
AXC#465	August xi-Cassiopeiids	0	6	20	57	74	96	106	97	456
AOC#466	August omicron-Cetids	0	0	11	16	25	52	109	83	296
LAQ#473	lambda-Aquariids	0	9	22	23	44	104	56	189	447
ICE#476	iota-Cetids	0	11	42	32	36	60	68	128	377
TCA#480	tau-Cancrids	0	68	87	233	371	439	502	661	2361
NZP#486	November zeta-Perseids	0	8	20	17	50	43	55	80	273
NSU#488	November sigma-Ursae Majorids	0	11	16	25	53	45	77	72	299
DEL#494	December Lyncids	0	20	36	127	93	169	214	207	866
DAB#497	December alpha-Bootids	0	5	13	20	47	52	31	75	243
FPL#501	February pi-Leonids	0	2	21	30	31	52	100	99	335
DRV#502	December rho-Virginids	2	35	47	129	140	173	263	281	1070
AIC#505	August iota-Cetids	0	52	118	159	312	439	635	1035	2750
FEV#506	February epsilon-Virginids	0	5	83	115	302	360	473	532	1870
UAN#507	upsilon-Andromedids	0	17	64	87	265	211	299	420	1363
JRC#510	June rho-Cygnids	0	1	15	44	55	98	116	142	471
RPU#512	rho-Puppids	0	12	36	47	56	185	192	232	760
OMC#514	omega-Capricornids	0	0	13	16	34	120	223	358	764
OLE#515	omicron-Leonids	0	28	46	87	193	189	350	389	1282
FMV#516	February mu-Virginids	0	1	22	32	105	116	149	225	650
ALO#517	April lambda-Ophiuchids	0	1	5	25	45	30	54	106	266
AHE#518	April 102-Herculids	0	1	11	4	19	27	18	39	119
BAQ#519	beta-Aquariids	0	4	8	28	53	31	109	145	378
MBC#520	May beta-Capricornids	0	5	16	25	32	90	108	201	477
AGC#523	August gamma-Cepheids	0	15	54	72	169	103	260	363	1036
LUM#524	lambda-Ursae Majorids	0	13	12	66	108	35	148	184	566
SLD#526	Southern lambda-Draconids	0	15	18	67	68	92	101	106	467
EHY#529	eta-Hydrids	2	56	97	241	287	473	632	616	2404
ECV#530	eta-Corvids	0	5	31	47	130	211	362	434	1220
GAQ#531	gamma-Aquilids	0	6	18	60	73	94	114	188	553
JXA#533	July xi-Arietids	0	9	41	60	134	212	418	445	1319
THC#535	theta-Cetids	0	1	4	11	20	29	91	46	202
TTB#543	22-Bootids	0	4	8	9	22	16	27	52	138
JNH#544	January nu-Hydrids	0	3	14	10	33	20	58	86	224
XCA#545	xi-Cassiopeiids	0	1	6	10	29	13	24	49	132
FTC#546	43-Cassiopeiids	0	12	57	63	83	149	167	232	763
KAP#547	kappa-Perseids	0	33	171	266	462	689	900	1212	3733
FAN#549	49-Andromedids	0	3	56	77	112	156	132	248	784
PSO#552	pi6-Orionids	0	27	85	221	270	361	428	403	1795
OCP#555	October gamma-Camelopardalids	0	14	18	51	83	85	136	147	534
PTA#556	phi-Taurids	0	14	8	50	78	81	147	116	494
SFD#557	64-Draconids	0	29	53	101	111	191	202	252	939
MCB#559	beta-Canis Majorids	0	11	12	10	42	42	65	87	269
SSX#561	6-Sextantids	1	8	20	31	61	64	77	136	398
DOU#563	December omega-Ursae Majorids	1	22	33	26	96	88	177	182	625
SUM#564	61-Ursae Majorids	0	16	14	13	40	23	81	78	265
OHY#569	omicron-Hydrids	0	9	22	34	128	225	511	679	1608
FBH#570	February beta-Herculids	0	3	9	11	48	48	58	157	334
TSB#571	26-Bootids	0	2	9	11	29	28	48	108	235
SAU#575	63-Aurigids	0	6	18	19	41	60	56	79	279
CHA#580	chi-Andromedids	0	7	34	16	73	67	97	169	463
NHE#581	90-Herculids	0	5	66	88	130	190	160	304	943
JBC#582	January beta-Craterids	0	0	15	36	60	80	182	216	589
GCE#584	Cepheids-Cassiopeiids	0	11	28	50	84	102	169	193	637
THY#585	33-Hydrids	1	5	13	20	41	73	56	81	290
FNC#587	59-Cygnids	0	3	15	24	45	25	47	49	208
FCA#589	50-Cancrids	0	6	21	49	81	62	131	138	488
VCT#590	10-Canum Venaticids	0	1	5	2	14	5	30	26	83
ZBO#591	zeta-Bootids	0	3	20	28	52	49	92	102	346
PON#592	91-Piscids	0	3	10	18	30	39	61	44	205
TOL#593	28-Lyncids	0	16	19	62	77	126	117	157	574
RSE#594	Serpentids-Coronae Borealids	0	0	3	4	4	27	11	30	79
POS#599	72-Ophiuchids	0	4	44	89	156	173	256	355	1077
ICT#601	iota-Craterids	1	3	8	10	27	28	86	98	261
KCR#602	kappa-Craterids	0	0	1	21	36	37	104	85	284
FAR#608	14-Aurigids	0	2	13	38	52	64	86	49	304
TLY#613	31-Lyncids	0	1	12	61	56	104	97	84	415
THD#618	12-Hydrids	0	2	6	16	30	12	64	55	185
XCS#623	xi2-Capricornids	0	20	78	99	248	814	499	878	2636
XAR#624	xi-Arietids	0	83	156	138	370	523	286	882	2438
LTA#625	lambda-Taurids	0	50	130	132	454	492	286	1646	3190
LCT#626	lambda-Cetids	0	54	19	126	191	42	271	477	1180
NPS#627	nu-Piscids	0	51	21	158	226	122	402	463	1443
STS#628	s-Taurids	0	123	62	208	3172	258	388	5156	9367
ATS#629	A2-Taurids	0	84	124	176	326	706	228	883	2527
TAR#630	tau-Arietids	0	132	115	411	352	537	698	584	2829
DAT#631	delta-Arietids	0	167	58	374	553	227	877	1207	3463
NET#632	November eta-Taurids	0	61	161	377	179	774	682	542	2776
PTS#633	p-Taurids	2	115	76	262	246	401	692	551	2345
TAT#634	tau-Taurids	0	99	157	210	487	606	670	1096	3325
ATU#635	A1-Taurids	0	44	263	471	260	1090	969	1407	4504
MTA#636	m-Taurids	0	60	33	172	121	182	432	267	1267
FTR#637	f-Taurids	0	120	156	404	1248	663	760	3745	7096
DZT#638	December zeta-Taurids	1	14	18	39	47	97	66	150	432
AOA#640	August omicron-Aquariids	0	62	251	328	547	1117	2296	1567	6168
JLL#644	January lambda-Leonids	4	37	83	107	134	231	249	397	1242
BCO#647	beta-Comae Berenicids	0	8	40	69	99	82	117	234	649
TAL#648	22-Aquilids	0	6	82	113	216	317	431	610	1775
OAV#651	68-Virginids	0	18	32	67	128	385	273	374	1277
OSP#652	omicron-Serpentids	0	4	10	21	30	36	96	99	296
RLY#653	R-Lyrids	0	4	34	33	88	71	94	201	525
APC#655	April phi-Capricornids	0	1	2	4	4	29	63	73	176
GSG#657	gamma-Sagittariids	0	0	2	12	13	27	60	66	180
EDR#658	epsilon-Draconids	0	2	14	22	30	19	44	100	231
EPS#660	epsilon-Scorpiids	0	3	15	30	25	61	143	209	486
OTH#661	110-Herculids	0	0	11	28	32	25	45	72	213
MUC#665	May upsilon-Cygnids	0	2	22	27	35	64	58	89	297
JMP#668	June mu-Pegasids	0	3	20	16	36	52	38	61	226
MCY#671	mu-Cygnids	0	0	3	9	20	9	32	33	106
MUA#679	mu-Aquariids	0	5	6	33	32	56	91	99	322
JEA#680	June epsilon-Arietids	0	6	9	12	19	22	33	29	130
OAQ#681	omicron-Aquariids	0	4	17	17	21	48	56	120	283
JTS#683	June theta-Serpentids	0	0	8	6	5	20	21	48	108
JPS#685	June beta-Pegasids	0	4	11	9	39	37	42	74	216
JRD#686	June rho-Draconids	0	0	1	7	17	26	15	17	83
KDP#687	kappa-Delphinids	0	0	9	5	7	8	19	7	55
TAC#689	tau-Capricornids	0	8	41	31	100	160	468	510	1318
ZCE#691	zeta-Cetids	0	1	0	13	29	15	49	57	164
EQA#692	epsilon-Aquariids	0	15	119	239	373	159	1243	1056	3204
ANP#693	August nu-Perseids	0	17	44	65	158	147	208	317	956
OMG#694	omicron-Geminids	0	32	73	111	180	217	283	342	1238
APA#695	August psi-Aurigids	0	4	14	27	36	34	46	89	250
OAU#696	omicron-Aurigids	0	5	26	36	63	79	96	135	440
AET#698	August eta-Taurids	0	1	22	30	48	81	48	152	382
BCE#701	beta-Cepheids	0	2	8	7	24	37	93	91	262
ASP#702	August 78-Pegasids	0	1	12	9	17	13	23	41	116
OAN#704	omicron-Andromedids	0	18	83	107	135	197	250	316	1106
ZPI#706	zeta-Piscids	0	24	51	80	132	174	210	326	997
BPX#707	beta-Pyxidids	0	0	2	4	19	15	102	121	263
RLM#708	R-Leonis Minorids	0	0	4	24	31	46	86	61	252
FDC#712	February delta-Cygnids	0	1	8	12	19	21	20	46	127
CCR#713	chi-Cancrids	0	5	10	9	19	25	13	43	124
RPI#714	rho-Piscids	0	34	62	89	143	181	250	368	1127
ACL#715	alpha-Camelopardalids	0	60	162	286	401	557	607	758	2831
OCH#716	October chi-Andromedids	0	25	29	67	108	109	154	204	696
NGB#720	November gamma-Bootids	0	7	3	16	16	16	50	64	172
DAS#721	December alpha-Sextantids	0	13	6	38	19	23	73	49	221
FLE#722	15-Leonids	0	14	11	42	36	45	112	64	324
DEG#726	December epsilon-Geminids	3	15	37	12	85	76	119	177	524
ISR#727	iota-Serpentids	0	2	2	0	16	6	12	44	82
PGE#728	phi-Geminids	0	10	15	11	46	26	65	71	244
DCO#729	delta-Corvids	0	2	9	2	17	13	48	53	144
ATV#730	April theta-Virginids	0	1	6	1	4	7	22	26	67
FGV#732	February gamma-Virginids	0	3	12	14	33	41	27	123	253
MOC#734	March omicron-Cygnids	0	1	12	14	17	11	23	49	127
XIP#736	xi-Perseids	0	3	8	15	32	27	60	53	198
FNP#737	59-Perseids	0	1	4	2	15	4	25	25	76
RER#738	rho-Eridanids	0	3	13	31	47	78	238	119	529
LAR#739	lambda-Arietids	0	7	11	26	57	36	81	132	350
OSD#745	October 6-Draconids	0	7	18	40	66	83	84	115	413
EVE#746	e-Velids	0	11	13	123	195	942	1710	1408	4402
JKL#747	January kappa-Leonids	0	8	23	44	101	52	153	197	578
JTL#748	January theta-Leonids	0	0	22	14	95	92	139	203	565
SMV#750	Southern March gamma-Virginids	0	6	50	94	186	229	397	691	1653
KCE#751	kappa-Cepheids	0	17	42	39	78	87	109	172	544
MID#755	May iota-Draconids	0	0	4	3	11	6	5	18	47
CCY#757	chi-Cygnids	0	12	380	16	23	47	57	1209	1744
SCO#771	sigma-Columbids	0	1	2	9	9	27	25	41	114
ILU#783	iota-Lupids	0	0	0	0	0	0	0	26	26
KVE#784	kappa-Velids	0	0	2	28	103	99	404	353	989
TCD#785	theta-Carinids	0	0	0	9	41	75	343	360	828
SXP#786	6-Puppids	0	2	4	1	13	10	34	29	93
KVO#787	kappa-Volantids	0	0	0	0	0	0	0	324	324
MBE#792	March beta-Equuleids	0	0	0	2	4	6	9	4	25
KCA#793	kappa-Cancrids	0	0	8	10	30	14	53	59	174
SED#796	September epsilon-Draconids	0	6	5	29	41	34	63	78	256
ADS#802	June Aquariids	0	0	8	9	18	46	68	84	233
LSA#803	lambda-Sagittariids	0	2	5	27	54	69	200	169	526
FLO#807	February Leonids	0	7	57	61	98	126	180	405	934
XCD#810	October Cetids	0	10	7	29	63	62	62	97	330
NAA#812	November alpha-Aurigids	0	5	20	27	32	64	59	76	283
CVD#814	January Canum Venaticids	0	0	6	6	34	48	24	72	190
UMS#815	August Ursae Majorids	0	0	10	9	15	16	16	36	102
CVT#816	February Canum Venaticids	0	1	5	13	15	23	20	44	121
OAG#818	October Aurigids	0	6	9	10	21	30	28	49	153
NUT#822	nu-Taurids	0	0	4	9	18	52	108	131	322
FCE#823	56-Cetids	0	10	20	26	54	85	129	165	489
DEX#824	December Sextantids	0	3	17	13	35	45	66	77	256
XIE#825	xi-Eridanids	0	14	12	22	25	69	111	42	295
ILI#826	iota1-Librids	0	4	36	42	69	126	282	347	906
NPE#827	nu-Pegasids	0	1	17	16	31	52	90	107	314
JSP#829	July 77-Pegasids	0	7	18	54	46	113	121	130	489
SCY#830	63-Cygnids	0	2	27	20	46	46	65	84	290
GPG#831	gamma-Pegasids	0	5	8	14	30	44	61	63	225
LEP#832	Leporids	0	3	1	5	12	27	85	84	217
KOR#833	kappa-Orionids	0	5	3	13	30	34	54	43	182
ACU#834	April theta-Centaurids	0	1	1	6	6	9	57	43	123
JDP#835	June delta-Pavonids	0	0	0	0	0	0	0	79	79
ABH#836	April beta-Herculids	0	0	2	8	17	22	30	48	127
CAE#837	Caelids	0	2	0	2	19	30	20	77	150
PSR#839	phi-Serpentids	0	1	9	17	22	29	53	27	158
TER#840	tau4-Eridanids	0	0	4	8	3	17	31	37	100
DHE#841	delta-Herculids	0	0	5	16	46	25	46	79	217
CRN#842	A-Carinids	0	0	0	0	0	0	0	229	229
DMD#843	December mu-Draconids	0	1	5	5	9	13	25	37	95
DTP#844	December theta-Pyxidids	0	15	6	45	36	61	151	100	414
TSC#846	tau-Sculptorids	0	0	0	0	0	0	0	46	46
BEL#847	beta-Leonids	0	4	0	13	10	12	19	23	81
OPE#848	omicron-Perseids	0	2	4	4	9	8	2	17	46
SZE#849	September zeta-Eridanids	0	1	15	17	22	48	60	99	262
PCY#854	psi-Cygnids	0	1	17	25	67	69	71	93	343
ATD#855	August tau-Draconids	0	0	3	8	8	18	19	12	68
EMO#856	epsilon-Monocerotids	0	4	8	15	25	17	43	54	166
FPB#858	February phi-Bootids	0	3	20	15	75	81	62	113	369
MTB#859	March 12-Bootids	0	2	1	17	35	21	45	105	226
PAN#860	psi-Andromedids	0	0	3	12	28	22	15	24	104
JXS#861	June xi1-Sagittariids	0	1	9	4	15	33	26	89	177
SSR#862	16-Scorpiids	0	1	9	16	37	48	61	123	295
TLR#863	12-Lacertids	0	1	5	12	12	26	17	15	88
JSG#864	June 66-Pegasids	0	2	1	10	8	20	24	22	87
JES#865	June epsilon-Serpentids	0	4	4	3	15	25	25	40	116
ECB#866	epsilon-Coronae Borealids	0	2	5	9	8	6	17	12	59
FPE#867	52-Pegasids	0	3	10	2	38	17	44	52	166
PSQ#868	psi3-Aquariids	0	1	5	2	8	23	29	38	106
UCA#869	upsilon1-Cassiopeiids	0	0	10	5	25	29	65	98	232
JPG#870	July eta-Pegasids	0	0	11	8	11	10	27	45	112
DCD#871	delta-Cepheids	0	0	9	5	11	11	18	43	97
ETR#872	epsilon-Triangulids	0	2	9	16	32	39	84	42	224
OMI#873	omicron-Cetids	0	5	8	12	26	21	39	91	202
PXS#874	September xi-Perseids	0	13	44	45	75	113	82	186	558
TEI#875	tau9-Eridanids	0	4	2	13	19	24	42	42	146
ROR#876	rho-Orionids	0	9	11	20	49	43	79	131	342
OHD#877	omega-Hydrids	0	5	7	21	25	41	19	45	163
OEA#878	October epsilon-Aurigids	0	2	5	2	9	23	21	33	95
ATI#879	alpha-Taurids	0	7	11	28	35	58	56	64	259
YDR#880	Y-Draconids	0	12	13	28	40	50	42	87	272
TLE#881	theta-Leonids	0	1	1	21	19	9	19	22	92
PLE#882	phi-Leonids	0	3	7	10	20	20	25	21	106
NBP#884	November beta-Pyxidids	0	1	3	1	15	29	61	49	159
DEV#885	December epsilon-Virginids	0	4	11	7	32	16	69	74	213
ACV#886	alpha-Corvids	1	0	7	11	48	24	104	135	330
DZB#887	December zeta-Bootids	0	3	13	15	25	13	37	85	191
SCV#888	6-Corvids	0	0	2	10	10	21	43	46	132
YOP#889	Y-Ophiuchids	0	0	1	2	8	6	10	14	41
ESU#890	eta-Scutids	0	1	5	3	6	10	5	19	49
FSL#891	February sigma-Leonids	0	2	17	9	55	44	38	184	349
MCN#892	March Centaurids	0	0	0	3	9	5	22	24	63
EOP#893	eta-Ophiuchids	0	0	19	25	42	71	100	173	430
OTA#896	130-Taurids	0	11	21	11	42	61	41	119	306
OUR#897	October alpha-UrsaeMinorids	0	9	2	21	28	10	49	31	150
SGP#898	September gamma-Piscids	0	5	10	19	10	30	50	43	167
EMC#899	epsilon-Microscopiids	0	1	0	3	13	29	72	109	227
BBO#900	beta-Bootids	0	0	18	40	109	44	155	105	471
TLC#901	34-Lyncids	0	3	8	7	19	21	22	37	117
DCT#902	delta-Cetids	0	15	13	24	36	86	83	104	361
OAT#903	October alpha-Triangulids	0	8	12	7	25	35	51	61	199
OCO#904	omicron-Columbids	0	2	2	14	5	50	56	26	155
MXD#905	March xi-Draconids	0	0	7	6	7	11	7	22	60
ETD#906	eta-Draconids	0	0	13	18	34	27	17	99	208
MCE#907	mu-Cepheids	0	1	5	11	21	17	26	12	93
BTC#910	beta2-Cygnids	0	1	14	19	32	26	35	91	218
TVU#911	21-Vulpeculids	0	2	11	29	57	49	80	141	369
BCY#912	beta-Cygnids	0	1	17	23	39	46	74	92	292
DNO#915	delta-Normids	0	0	1	2	6	41	45	167	262
TAG#918	theta-Aurigids	0	4	10	17	41	18	37	70	197
ICN#919	iota-Centaurids	0	0	2	4	3	17	126	223	375
XSC#920	xi-Scorpiids	0	4	10	25	43	53	137	163	435
JLC#921	July lambda-Capricornids	0	3	15	6	22	27	48	116	237
SAN#924	62-Andromedids	0	1	3	20	5	26	16	6	77
EAN#925	eta-Andromedids	0	2	4	4	23	23	14	31	101
OCR#1033	omega-Carinids	0	0	0	0	0	6	19	14	39
EPU#1044	epsilon-Ursae Minorids	0	0	0	0	0	0	0	150	150
PIS#1046	29-Piscids	0	0	0	0	0	0	0	0	0
TVL#1055	35-Vulpeculids	0	0	0	0	0	0	0	13	13
SCE#1070	77-Cetids	0	0	0	0	0	0	0	244	244
IHD#1071	iota-Hydrusids	0	0	0	0	0	0	0	60	60
GAD#1106	gamma-Draconids	0	0	0	0	0	0	0	51	51
IHR#1108	July iota-Hydrusids	0	0	0	0	0	0	0	17	17
ARD#1130	Arids	0	0	0	6	0	1	2	0	9
OZP#1131	October zeta-Perseids	0	0	0	6	1	0	0	0	7
OEC#1172	October epsilon-Carinids	0	0	0	0	0	0	0	161	161
M23K1	M2023-K1	0	0	0	0	0	0	0	21	21
M24H1	M2024-H1	0	0	0	0	0	0	0	17	17
M24N1	M2024-N1	0	0	0	0	0	0	0	42	42
M24S1	M2024-S1	0	0	0	0	0	0	0	28	28
M25F1	M2025-F1	0	0	0	0	0	0	0	124	124
M25K1	M2025-K1	0	0	0	0	0	0	0	35	35
M25L1	M2025-L1	0	0	0	0	0	0	0	55	55
M25L2	M2025-L2	0	0	0	0	0	0	0	46	46
M25O1	M2025-O1	0	0	0	0	0	0	0	69	69
M25O2	M2025-O2	0	0	0	0	0	0	0	48	48
M25P1	M2025-P1	0	0	0	0	0	0	0	70	70
M25S1	M2025-S1	0	0	0	0	0	0	0	132	132
M25S2	M2025-S2	0	0	0	0	0	0	0	466	466
M2025U1	M2025-U1	0	0	0	0	0	0	0	152	152
M25Y1	M2025-Y1	0	0	0	0	0	0	0	395	395
	Totals	497	50263	125095	211788	334668	451894	707555	966063	2847823

 

Acknowledgments

This report is based on the data of the Global Meteor Network which is released under the CC BY 4.0 license. We thank all the participants in the Global Meteor Network project for their contribution and perseverance, operators whose cameras provided the data used in this work and contributors who made important code contributions The Global Meteor Network results were obtained thanks to the efforts of the following volunteers. (list cut-off date as it was at the end of 28 January 2026).

In memory of Global Meteor Network members:

Dr. Daniel A. Klinglesmith III (d. 2019)

Martin Richmond-Hardy (d. 2023)

Rajko Susanj (d. 2023)

Zoran Dragic (d. 2025)

Romke Schievink (d. 2025)

Seppe Canonaco (d. 2025)

Memento mori

Each of us, a fleeting flame

Yet our paths remain.

Campbell, Adam Mullins, Aden Walker, Adrian Bigland, Adriana Roggemans, Adriano Fonseca, Aksel Askanius, Al Foster, Alain Marin, Alaistar Brickhill, Alan Beech, Alan Maunder, Alan Pevec, Alan Pickwick, Alan Decamps, Alan Cowie, Alan Kirby, Alan Senior, Alastair Emerson, Aled Powell, Alejandro Barriuso, Aleksandar Merlak, Aleksei Blokhin, Alex Bell, Alex Haislip, Alex Hodge, Alex Jeffery, Alex Kichev, Alex McConahay, Alex Pratt, Alex Roig, Alex Aitov, Alex McGuinness, Alexander Wiedekind-Klein, Alexander Kasten, Alexandre Alves, Alexandru Tudorica, Alfredo Dal’ Ava Júnior, Alison Scott, Amy Barron, Anatoly Ijon, Andre Rousseau, Andre Bruton, Andrea Storani, Andrei Marukhno, Andres Fernandez, Andrew Campbell-Laing, Andrew Challis, Andrew Cooper, Andrew Fiamingo, Andrew Heath, Andrew Moyle, Andrew Washington, Andrew Fulher, Andrew Robertson, Andy Stott, Andy Sapir, Andy Shanks, Ange Fox, Angel Sierra, Angélica López Olmos, Anna Johnston, Anne van Weerden, Anoop Chemencherry, Ansgar Schmidt, Anthony Hopkinson, Anthony Pitt, Anthony Kesterton, Anton Macan, Anton Yanishevskiy, Antony Crowther, Anzhari Purnomo, Ari Paulechen Jr, Arie Blumenzweig, Arie Verveer, Arnaud Leroy, Arne Krueger, Artem Oskolkov, Attila Nemes, Barry Findley, Bart Dessoy, Bela Szomi Kralj, Ben Poulton, Bence Kiss, Bernard Côté, Bernard Hagen, Bev M. Ewen-Smith, Bill Cooke, Bill Wallace, Bill Witte, Bill Carr, Bill Thomas, Bill Kraimer, Bob Evans, Bob Greschke, Bob Hufnagel, Bob Marshall, Bob Massey, Bob Zarnke, Bob Guzik, Branko Zubić, Brenda Goodwill, Brendan Cooney, Brendon Reid, Brian Chapman, Brian Murphy, Brian Rowe, Brian Hochgurtel, Wyatt Hochgurtel, Brian Mitchell, Bridgend Astronomical Society, Bruno Bonicontro, Bruno Casari, Callum Potter, Carl Elkins, Carl Mustoe, Carl Panter, Cesar Domingo Pardo, Charles Thody, Charlie McCormack, Chris Baddiley, Chris Blake, Chris Dakin, Chris George, Chris James, Chris Ramsay, Chris Reichelt, Chris Chad, Chris O’Neill, Chris White, Chris Jones, Chris Sale, Chris Raynerd, Christian Wanlin, Christine Ord, Christof Zink, Christophe Demeautis, Christopher Coomber, Christopher Curtis, Christopher Tofts, Christopher Brooks, Christopher Matthews, Chuck Goldsmith, Chuck Pullen, Ciaran Tangney, Claude Boivin, Claude Surprenant, Clive Sanders, Clive Hardy, Colin Graham, Colin Marshall, Colin Nichols, Con Stoitsis, Craig Young, Creina Beaman, Daknam Al-Ahmadi, Dale Hooper, Damien Lemay, Damien McNamara, Damir Matković, Damir Šegon, Damjan Nemarnik, Dan Klinglesmith, Dan Pye, Daniel Duarte, Daniel J. Grinkevich, Daniela Cardozo Mourão, Danijel Reponj, Danko Kočiš, Dario Zubović, Dave Jones, Dave Mowbray, Dave Newbury, Dave Smith, David Akerman, David Attreed, David Bailey, David Brash, David Castledine, David Hatton, David Leurquin, David Price, David Rankin, David Robinson, David Rollinson, David Strawford, David Taylor, David Rogers, David Banes, David Johnston, David Rees, David Cowan, David Greig, David Hickey, David Colthorpe, David Straer, David Harding, David Furneaux, David Teissier, David Lynch, David M. Goldie, Dean Moore, Debbie Godsiff, Denis Bergeron, Denis St-Gelais, Dennis Behan, Derek Poulton, Derek Baker, Didier Walliang, Dimitris Georgoulas, Dino Čaljkušić, Dmitrii Rychkov, Dominique Guiot, Don Anderson, Don Hladiuk, Dorian Božičević, Dougal Matthews, Douglas Sloane, Douglas Stone, Dustin Rego, Dylan O’Donnell, Ed Breuer, Ed Harman, Edd Stone, Edgar Mendes Merizio, Edison José Felipe Pérezgómez Álvarez, Edson Valencia Morales, Eduardo Fernandez Del Peloso, Eduardo Lourenço, Edward Cooper, Egor Gustov, Ehud Behar, Eleanor Mayers, Emily Barraclough, Enrico Pettarin, Enrique Arce, Enrique Chávez Garcilazo, Eric Lopez, Eric Toops, Eric O’ Toole, Eric Ronney, Errol Balks, Erwin van Ballegoij, Erwin Harkink, Eugene Potapov, Ewan Richardson, Fabricio Borges, Fabricio Colvero, Fabrizio Guida, Felipe P. Leitzke, Felix Bettonvil, Ferenc-Levente Juhos, Fernando Dall’Igna, Fernando Jordan, Fernando Requena, Filip Matković, Filip Mezak, Filip Parag, Fiona Cole, Firuza Rahmat, Florent Benoit, Francis Rowsell, François Simard, Frank Lyter, Frans Lowiessen, Frantisek Bilek, Gabor Sule, Gaétan Laflamme, Gareth Brown, Gareth Lloyd, Gareth Oakey, Garry Dymond, Gary Parker, Gary Eason, Gavin Martin, Gene Mroz, Geoff Scott, Georges Attard, Georgi Momchilov, Gerald Engwell, Gerard Van Os, Germano Soru, Gert Jan Netjes, Gilberto Sousa, Gilton Cavallini, Gino Robert, Glen Shennan, Gordon Hudson, Graeme Hanigan, Graeme McKay, Graham Stevens, Graham Winstanley, Graham Henstridge, Graham Atkinson, Graham Palmer, Graham Cann, Graham Mallin, Grant Salmond, Greg Michael, Greg Parker, Guillaume Poulizac, Gulchehra Kokhirova, Gustav Frisholm, Gustavo Silveira B. Carvalho, Guy Létourneau, Guy Williamson, Guy Lesser, Hamish Barker, Hamish McKinnon, Hanson Du, Haris Jeffrey, Harri Kiiskinen, Hartmut Leiting, Heather Petelo, Henk Bril, Henning Letmade, Heriton Rocha, Hervé Lamy, Herve Roche, Holger Pedersen, Horst Meyerdierks, Howard Edin, Hugo González, Iain Drea, Ian Enting Graham, Ian Lauwerys, Ian Parker, Ian Pass, Ian A. Smith, Ian Williams, Ian Hepworth, Ian Collins, Ian Cattermole, Igor Duchaj, Igor Henrique, Igor Macuka, Igor Pavletić, Ilya Jankowsky, Ioannis Kedros, Ivan Gašparić, Ivan Sardelić, Ivica Ćiković, Ivica Skokić, Ivo Dijan, Ivo Silvestri, Jack Barrett, Jacques Masson, Jacques Walliang, Jacqui Thompson, Jake Turner, James Davenport, James Farrar, James Scott, James Stanley, James Dawson, James Lloyd, James Malley, Jamie Allen, Jamie Cooper, Jamie McCulloch, Jamie Olver, Jamie Shepherd, Jan Hykel, Jan Wisniewski, Jan Tromp, Janis Russell, Janusz Powazki, Jasminko Mulaomerović, Jason Burns, Jason Charles, Jason Gill, Jason van Hattum, Jason Sanders, Javor Kac, Jay Shaffer, Jayce Dowell, Jean Francois Larouche, Jean Vallieres, Jean Brunet, Jean-Baptiste Kikwaya, Jean-Bruno Desrosiers, Jean-Fabien Barrois, Jean-Louis Naudin, Jean-Marie Jacquart, Jean-Paul Dumoulin, Jean-Philippe Barrilliot, Jeff Holmes, Jeff Huddle, Jeff Wood, Jeff Devries, Jeffrey Legg, Jenifer Millard, Jeremy Taylor, Jeremy Spink, Jesse Stayte, Jesse Lard, Jessica Richards, Jim Blackhurst, Jim Cheetham, Jim Critchley, Jim Fordice, Jim Gilbert, Jim Rowe, Jim Seargeant, Jim Fakatselis, João Mattei, Joaquín Albarrán, Jochen Vollsted, Jocimar Justino, Joe Zender, Joe Farragher, Johann Swanepoel, John W. Briggs, John Drummond, John Hale, John Kmetz, John Maclean, John Savage, John Thurmond, John Tuckett, John Waller, John Wildridge, John Bailey, John Thompson, John Martin, John Yules, John Burrin, John Huberd, Jon Bursey, Jonathan Alexis Valdez Aguilar, Jonathan Eames, Jonathan Mackey, Jonathan Whiting, Jonathan Wyatt, Jonathan Pettingale, Jonathon Kambulow, Jorge Augusto Acosta Bermúdez, Jorge Oliveira, Jose Carballada, Jose Galindo Lopez, José María García, José-Luis Martín, Josef Scarantino, Joseph Jones, Josip Belas, Josip Krpan, Jost Jahn, Juan Luis Muñoz, Juergen Neubert, Julián Martínez, Julien Roy, Jure Zakrajšek, Jürgen Dörr, Jürgen Ketterer, Justin Zani, Kamel Nechma, Karen Smith, Karl Browne, Kath Johnston, Kees Habraken, Keith Maslin, Keith Biggin, Keith Christie, Keith Scorrar, Keith Butterworth, Kelvin Richards, Ken Jamrogowicz, Ken Lawson, Ken Gledhill, Ken Kirvan, Ken Whitnall, Kevin Gibbs-Wragge, Kevin Morgan, Kevin Faure, Kevin Nielsen, Klaas Jobse, Korado Korlević, Kyle Francis, Lachlan Gilbert, Larry Groom, Lars Rombi, Laurent Brunetto, Laurent Reix, Laurie Stanton, Lawrence Saville, Lee Hill, Lee Brady, Leith Robertson, Len North, Les Rowe, Leslie Kaye, Lev Pustil’Nik, Lexie Wallace, Lisa Holstein, Llewellyn Cupido, Logan Carpenter, Lorna McCalman, Louw Ferreira, Lovro Pavletić, Lubomir Moravek, Luc Turbide, Luc Busquin, Lucia Dowling, Luciano Miguel Diniz, Ludger Börgerding, Luis Fabiano Fetter, Luis Santo, Maciej Reszelsk, Maciej Kwinta, Magda Wisniewska, Manel Colldecarrera, Marc Corretgé Gilart, Marcel Berger, Marcelo Domingues, Marcelo Zurita, Marcio Malacarne, Marco Verstraaten, Marcus Rigo, Margareta Gumilar, Marián Harnádek, Mario Sandri, Mariusz Adamczyk, Mark Fairfax, Mark Gatehouse, Mark Haworth, Mark McIntyre, Mark Phillips, Mark Robbins, Mark Spink, Mark Suhovecky, Mark Williams, Mark Ward, Mark Bingham, Mark Fechter, Mark Severance, Marko Šegon, Marko Stipanov, Marshall Palmer, Marthinus Roos, Martin Breukers, Martin Richmond-Hardy, Martin Robinson, Martin Walker, Martin Woodward, Martin Connors, Martin Kobliha, Martyn Andrews, Martyn Kinder, Martyn Hunter-Wyatt, Mary Waddingham, Mary Hope, Mason McCormack, Mat Allan, Máté Pintér, Matej Mihelčić, Matt Cheselka, Matt McMullan, Matthew Howarth, Matthew Finch, Matthew Terracciano, Max Schmid, Megan Gialluca, Megan Spencer-Young, Mia Boothroyd, Michael Cook, Michael Mazur, Michael O’Connell, Michael Krocil, Michael Camilleri, Michael Kennedy, Michael Lowe, Michael Atkinson, Michael Rainbow, Michał Warchoł, Michel Saint-Laurent, Mielke Sarkol, Miguel Diaz Angel, Miguel Preciado, Miguel Ángel Rapado, Mike Breimann, Mike Hutchings, Mike Read, Mike Shaw, Mike Ball, Mike Youmans, Milan Kalina, Milen Nankov, Miles Eddowes, Minesh Patel, Miranda Clare, Mirjana Malarić, Motohito Mizusaw, Muhammad Luqmanul Hakim Muharam, Murray Forbes, Murray Singleton, Murray Thompson, Myron Valenta, Nalayini Brito, Nawaz Mahomed, Ned Smith, Nedeljko Mandić, Nedim Mujić, Neil Graham, Neil Papworth, Neil Waters, Neil Petersen, Neil Allison, Nelson Moreira, Neville Vann, Nial Bruce, Nicholas Hill, Nicholas Ruffier, Nick Howarth, Nick James, Nick Moskovitz, Nick Norman, Nick Primavesi, Nick Quinn, Nick Russel, Nick Powell, Nick Wiffen, Nicola Masseroni, Nigel Bubb, Nigel Evans, Nigel Owen, Nigel Harris, Nigen Harris, Nikola Gotovac, Nikolay Gusev, Nikos Sioulas, Noah Simmonds, Norman Izsett, Olaf Jakubzik Reinartz, Ole Alexander, Ollie Eisman, Pablo Canedo, Pablo Domingo Escat, Paraksh Vankawala, Pat Devine, Patrick Franks, Patrick Poitevin, Patrick Geoffroy, Patrick Onesty, Patrik Kukić, Paul Cox, Paul Dickinson, Paul Haworth, Paul Heelis, Paul Kavanagh, Paul Ludick, Paul Prouse, Paul Pugh, Paul Roche, Paul Roggemans, Paul Stewart, Paul Huges, Paul Breck, Paul Volman, Paul Jenkinson, Paul D. Clarke, Pedro Augusto de Jesus Castro, Penko Yordanov, Pete Graham, Pete Lynch, Peter G. Brown, Peter Campbell-Burns, Peter Davis, Peter Eschman, Peter Gural, Peter Hallett, Peter Jaquiery, Peter Kent, Peter Lee, Peter McKellar, Peter Meadows, Peter Stewart, Peter Triffitt, Peter Leigh, Peter Felhofer, Péter Molnár, Peter Murray, Peter Watts, Pető Zsolt, Phil James, Philip Gladstone, Philip Norton, Philippe Schaak, Phillip Wilhelm Maximilian Grammerstorf, Pierre Gamache, Pierre de Ponthière, Pierre-Michael Micaletti, Pierre-Yves Pechart, Pieter Dijkema, Predrag Vukovic, Przemek Nagański, Radim Stano, Rajko Sušanj, Raju Aryal, Ralph Brady, Raoul van Eijndhoven, Raul Truta, Raul Elias-Drago, Raymond Shaw, Rebecca Starkey, Reinhard Kühn, Reinier Ott, Rembert Melman, Remi Lacasse, Renato Cássio Poltronieri, René Tardif, Richard Abraham, Richard Bassom, Richard Croy, Richard Davis, Richard Fleet, Richard Hayler, Richard Johnston, Richard Kacerek, Richard Payne, Richard Stevenson, Richard Severn, Richard Bates, Rick Fischer, Rick Hewett, Rick James, Rick Olupot, Ricky Bassom, Rob Agar, Rob de Corday Long, Rob Saunders, Rob Smeenk, Rob Musquetier, Robert Longbottom, Robert McCoy, Robert Saint-Jean, Robert D. Steele, Robert Veronneau, Robert Peledie, Robert Haas, Robert Kiendl, Robert Vallone, Robert Bungener, Robert Lucas, Robin Boivin, Robin Earl, Robin Rowe, Robin Leadbeater, Roel Gloudemans, Roger Banks, Roger Morin, Roger Conway, Roland Idaczyk, Rolf Carstens, Roman Moryachkov, Romke Schievink, Romulo Jose, Ron James Jr, Ron Paine, Ronal Kunkel, Roslina Hussain, Ross Skilton, Ross Dickie, Ross Welch, Ross Hortin, Russell Jackson, Russell Brunton, Ruud Oskam, Ryan Frazer, Ryan Harper, Ryan Kinnett, Ryan Thompson, Salvador Aguirre, Sam Green, Sam Hemmelgarn, Sam Leaske, Sandy Allan, Sarah Tonorio, Scott Kaufmann, Sean Lavigne, Sebastiaan de Vet, Sebastian Klier, Seppe Canonaco, Seraphin Feller, Serge Bergeron, Sergei Pavlov, Sergio Mazzi, Sergiy Ivanchenko, Sevo Nikolov, Simon Cooke-Willis, Simon Holbeche, Simon Maidment, Simon McMillan, Simon Minnican, Simon Parsons, Simon Saunders, Simon Fidler, Simon Oosterman, Simon Peterson, Simon lewis, Simon Lewis, Simon van Leverink, Simon Andersson, Slava Ilyin, Sofia Ulrich, Srivishal Sudharsan, Stacey Downton, Stan Nelson, Stanislav Korotkiy, Stanislav Tkachenko, Stef Vancampenhout, Stefan Frei, Stephane Zanoni, Stephen Grimes, Stephen Nattrass, Stephen M. Pereira, Steve Berry, Steve Bosley, Steve Carter, Steve Dearden, Steve Homer, Steve Kaufman, Steve Lamb, Steve Rau, Steve Tonkin, Steve Trone, Steve Welch, Steve Wyn-Harris, Steve Matheson, Steve Daniels, Steven Shanks, Steven Tilley, Stewart Doyle, Stewart Ball, Stewart Clark, Stuart Brett, Stuart Land, Stuart McAndrew, Sue Baker Wilson, Sylvain Cadieux, Tammo Jan Dijkema, Ted Cline, Terry Pundiak, Terry Richardson, Terry Simmich, Terry Young, Terry Meldrum, Theodor Feldbaumer, Thiago Paes, Thilo Mies, Thomas Blog, Thomas Schmiereck, Thomas Stevenson, Thomas Duff, Tihomir Jakopčić, Tim Burgess, Tim Claydon, Tim Cooper, Tim Gloudemans, Tim Havens, Tim Polfliet, Tim Frye, Tioga Gulon, Tobias Westphal, Tobias Hinse, Tom Warner, Tom Bell, Tomi Simola, Tommy McEwan, Tommy B. Nielsen, Torcuill Torrance, Tosh White, Tracey Snelus, Travis Shao, Trevor Clifton, Ubiratan Borges, Urs Wirthmueller, Uwe Glässner, Vasilii Savtchenko, Ventsislav Bodakov, Victor Acciari, Viktor Toth, Vincent McDermott, Vitor Jose Pereira, Vladimir Jovanović, Vladimir Usanin, Waily Harim, Warley Souza, Warwick Latham, Washington Oliveira, Wayne Metcalf, Wenceslao Trujillo, William Perkin, William Schauff, William Stewart, William Harvey, William Hernandez, Wullie Mitchell, Yakov Tchenak, Yanislav Ivanov, Yfore Scott, Yleana Ceballos, Yohsuke Akamatsu, Yong-Ik Byun, Yozhi Nasvadi, Yuri Stepanychev, Zach Steele, Zané Smit, Zbigniew Krzeminski, Željko Andreić, Zhuoyang Chen, Zoran Dragić, Zoran Knez, Zoran Novak, Zouhair Benkhaldoun, Łukasz Sanocki, Łukasz Łyjak, Alexander-von-Humboldt-Gymnasium (Germany), Asociación de Astronomía de Marina Alta (Spain), Costa Blanca Astronomical Society (Spain), Friedrich-Schiller-Gymnasium Preetz (Germany), HUN-REN Institute of Earth Physics and Space Science (Hungary), Haagar Observatory (Norway), Laingsburg High School (South Africa), Perth Observatory Volunteer Group (Australia), Phillips Academy Andover (United States), Royal Astronomical Society of Canada Calgary Centre (Canada), Touwsrivier Primary School (South Africa).

The following cameras contributed to triangulations with a valid meteor trajectory and meteoroid orbit in 2025. The camera id is given with the total number of orbits in brackets:

AT0002 (878), AT0004 (3989), AU0001 (470), AU0002 (7836), AU0003 (5143), AU000A (5061), AU000B (2012), AU000C (4557), AU000D (11267), AU000F (4425), AU000G (4080), AU000J (5), AU000K (13), AU000L (767), AU000Q (1187), AU000R (3936), AU000S (2948), AU000T (2316), AU000U (3705), AU000V (6323), AU000W (6099), AU000X (8008), AU000Y (6024), AU000Z (1886), AU0010 (3586), AU001A (10930), AU001B (7427), AU001C (1760), AU001D (1523), AU001E (4760), AU001F (5387), AU001G (167), AU001K (4424), AU001L (7449), AU001M (103), AU001N (2744), AU001P (8722), AU001Q (9180), AU001R (5897), AU001S (11719), AU001T (154), AU001U (4342), AU001V (5236), AU001W (8368), AU001X (4360), AU001Y (4658), AU001Z (2877), AU0028 (1409), AU0029 (2561), AU002A (1157), AU002B (3630), AU002C (829), AU002D (1249), AU002E (1047), AU002F (769), AU0030 (7805), AU0031 (42), AU0034 (62), AU0035 (4), AU003C (507), AU003E (5454), AU003F (37), AU003G (2397), AU003H (6387), AU003J (4762), AU003K (2), AU0040 (642), AU0041 (1354), AU0042 (1755), AU0043 (960), AU0044 (11), AU0045 (756), AU0046 (2696), AU0047 (2851), AU0048 (2277), AU004A (283), AU004B (1220), AU004H (541), AU004J (1207), AU004K (1080), AU004L (3167), AU004M (501), AU004Q (1646), AU004R (216), BA0001 (959), BA0002 (1401), BA0003 (2499), BA0004 (2095), BA0005 (1122), BE0001 (3017), BE0002 (1553), BE0003 (1155), BE0004 (1549), BE0005 (2843), BE0006 (3183), BE0007 (2208), BE0008 (2342), BE0009 (2028), BE000A (1600), BE000B (2456), BE000C (3814), BE000D (2220), BE000E (2739), BE000G (3825), BE000H (675), BE000J (1014), BE000K (2750), BE000L (5110), BE000M (1826), BE000P (4408), BE000Q (5525), BE000R (3275), BE000S (3295), BE000T (4492), BE000U (2594), BE000V (5168), BE000W (4090), BE000X (2380), BE000Y (652), BE000Z (1463), BE0010 (1884), BE0011 (1742), BE0012 (1774), BE0013 (1823), BE0014 (2607), BE0015 (1778), BE0016 (1487), BE0017 (2072), BE0018 (2313), BE0019 (1576), BE001A (1326), BE001B (103), BG0001 (1759), BG0002 (620), BG0003 (5772), BG0004 (632), BG0005 (1002), BG0008 (321), BG0009 (970), BG000A (674), BG000B (4213), BG000C (2525), BG000E (67), BG000F (220), BG000G (3027), BG000H (576), BG000J (569), BG000K (1116), BR0001 (45), BR0002 (924), BR0003 (89), BR0004 (85), BR0005 (137), BR000A (149), BR000F (1463), BR000G (2815), BR000H (1), BR000M (93), BR000Q (1260), BR000R (85), BR000S (537), BR000T (825), BR000Y (726), BR0013 (65), BR0015 (244), BR0016 (68), BR0019 (6), BR001F (390), BR001G (41), BR001H (245), BR001M (1320), BR001Q (313), BR001R (2365), BR001S (9), BR001T (992), BR001U (514), BR001W (808), BR001X (12), BR001Z (188), BR0021 (1), BR0029 (983), BR002A (906), BR002B (933), BR002C (1367), CA0003 (1), CA000C (10), CA000E (888), CA000L (836), CA000P (977), CA000Q (2200), CA000R (1939), CA000U (1679), CA000V (1511), CA000Y (983), CA001F (205), CA001G (925), CA001H (607), CA001J (401), CA001N (66), CA001R (2508), CA001Z (251), CA0022 (2185), CA0023 (1110), CA0026 (1007), CA002F (1435), CA002H (73), CA002J (720), CA002K (1900), CA002L (1792), CA002N (797), CA002P (269), CA002Q (4), CA002R (2164), CA002U (2296), CA002V (2064), CA0031 (3077), CA0032 (1590), CA0035 (3421), CA0036 (66), CA0037 (406), CA003A (2055), CA003B (199), CA003C (253), CA003D (1921), CA003E (37), CA003V (559), CA003W (269), CAWEC1 (68), CAWEC2 (147), CAWEC3 (34), CAWEC4 (16), CAWEC5 (22), CAWEC6 (36), CH0002 (1244), CH0003 (1335), CH0004 (939), CH0005 (2084), CL0002 (1907), CL0003 (1907), CZ0001 (552), CZ0002 (1985), CZ0003 (827), CZ0004 (1019), CZ0006 (929), CZ0007 (1470), CZ0008 (1029), CZ0009 (1508), CZ000A (2518), CZ000B (1139), CZ000C (1228), CZ000E (2190), CZ000F (900), CZ000G (1108), CZ000H (4056), CZ000J (1054), CZ000K (2966), CZ000L (1960), CZ000M (3380), CZ000N (1310), CZ000P (2187), CZ000Q (2926), CZ000R (2428), CZ000U (784), CZ000V (815), CZ000W (1091), CZ000X (833), CZ000Y (1472), DE0001 (3034), DE0002 (86), DE0003 (111), DE0004 (1746), DE0005 (2263), DE0006 (1638), DE0007 (1370), DE0008 (1863), DE0009 (1205), DE000B (4307), DE000C (651), DE000G (146), DE000H (213), DE000J (1922), DE000K (1846), DE000M (1009), DE000P (727), DE000Q (2474), DE000R (835), DE000S (4216), DE000V (486), DE000W (4043), DE000X (3370), DE000Y (1995), DE0011 (2860), DE0012 (1650), DE0013 (4422), DE0014 (1598), DE0015 (1698), DE0016 (3136), DE0017 (650), DE0018 (40), DK0001 (2882), DK0002 (1539), DK0003 (2957), DK0004 (2327), DK0005 (711), DK0006 (2015), DK0007 (3689), DK0008 (2611), DK0009 (2120), DK000A (1919), DK000B (1248), DK000C (2233), DK000D (3168), DK000E (481), DK000F (2201), DK000G (2406), DK000H (300), DK000J (1592), DK000K (2330), DK000L (859), DK000M (710), DK000N (295), DK000P (1358), DK000Q (1662), DK000R (2244), DK000S (2021), DK000T (2020), ES0001 (299), ES0002 (1), ES0003 (39), ES0004 (455), ES0005 (532), ES0006 (125), ES0009 (589), ES000C (1420), ES000D (1250), ES000E (484), ES000F (345), ES000H (695), ES000L (147), ES000M (128), ES000N (25), ES000P (36), ES000Q (1691), ES000T (852), ES000U (1794), ES000V (603), ES000W (34), ES000X (143), ES000Z (443), ES0011 (61), ES0013 (1149), ES0016 (1891), ES0019 (1368), ES001A (1722), ES001B (2), ES001D (690), ES001F (2113), ES001G (934), ES001H (392), FI0001 (20), FI0002 (63), FI0003 (61), FI0004 (158), FI0005 (231), FI0007 (128), FI0008 (25), FI0009 (46), FR0003 (758), FR0006 (3172), FR000A (1998), FR000G (787), FR000L (21), FR000M (129), FR000P (140), FR000R (1878), FR000U (588), FR000V (1338), FR000X (3820), FR000Y (5187), FR000Z (4077), FR0011 (3287), FR0012 (2396), FR0013 (3704), FR0014 (1279), FR0015 (381), FR0016 (2393), FR0017 (214), GR0002 (4050), GR0003 (4054), GR0004 (2926), GR0005 (1032), GR0006 (6275), GR0007 (3246), GR0008 (3319), GR0009 (7218), HR0001 (1849), HR0002 (2132), HR0004 (95), HR0006 (2186), HR0007 (5452), HR0008 (1431), HR000D (326), HR000H (989), HR000J (653), HR000K (58), HR000M (61), HR000P (1839), HR000Q (998), HR000S (2061), HR000U (295), HR000V (1672), HR000W (389), HR000Z (54), HR0015 (1298), HR0016 (687), HR001D (1312), HR001E (4162), HR001J (768), HR001K (550), HR001L (208), HR001M (230), HR001N (294), HR001P (336), HR001Q (789), HR001R (346), HR001X (1575), HR001Z (8740), HR0021 (10), HR0024 (1524), HR0025 (1859), HR0027 (2143), HR002D (8307), HR002E (4313), HR002F (5247), HR002G (5106), HR002H (5892), HR002J (9308), HR002K (2729), HR002M (2031), HR002T (3184), HR002U (99), HR002V (5715), HR002W (4021), HR002X (5033), HR002Y (1754), HU0001 (2309), HU0002 (5181), HU0003 (5869), HU0004 (2753), HU0005 (3786), HU0006 (1481), HU0007 (1402), HU0008 (819), HU0009 (1736), HU000A (2966), HU000B (5935), HU000C (373), IE0004 (3259), IE000G (654), IE000H (445), IE000J (1340), IE000M (794), IE000N (848), IL0001 (61), IL0002 (613), IL0003 (16), IL0004 (295), IL0009 (82), IL000A (332), IT0001 (2650), IT0004 (3801), IT0007 (57), IT0008 (2409), IT000A (240), IT000B (1034), IT000C (7), JP0001 (147), JP0002 (58), JP0003 (89), KR0001 (479), KR0002 (5616), KR0003 (354), KR0004 (6333), KR0005 (1203), KR0006 (502), KR0007 (584), KR0008 (409), KR0009 (1745), KR000A (5252), KR000B (4154), KR000C (2244), KR000D (3339), KR000E (3680), KR000F (2392), KR000G (1995), KR000H (5112), KR000J (4585), KR000K (4050), KR000L (2840), KR000M (3173), KR000N (4895), KR000P (3349), KR000Q (1779), KR000R (3030), KR000S (3048), KR000Y (2), KR000Z (2603), KR0010 (2764), KR0011 (2829), KR0012 (1900), KR0013 (2434), KR0014 (366), KR0015 (819), KR0016 (864), KR0017 (1417), KR0018 (1328), KR0019 (3947), KR001A (1526), KR001B (3200), KR001C (3134), KR001D (2470), KR001E (2386), KR001F (1338), KR001G (1969), KR001H (2573), KR001J (1761), KR001K (909), KR001L (486), KR001M (783), KR001N (573), KR001P (957), KR001Q (1371), KR001R (463), KR001S (707), KR001T (974), KR001U (1980), KR001V (1301), KR001W (1633), KR001X (1066), KR001Y (716), KR001Z (741), KR0020 (1333), KR0021 (1149), KR0022 (3294), KR0023 (3184), KR0024 (3651), KR0025 (2320), KR0026 (2006), KR0027 (2305), KR0028 (2826), KR0029 (2412), KR002A (1183), KR002B (1455), KR002C (2354), KR002D (2353), KR002E (2056), KR002F (1892), KR002G (1947), KR002H (1168), KR002J (1387), KR002K (499), KR002L (1739), KR002M (1527), KR002N (1182), KR002P (1433), KR002Q (1489), KR002R (997), KR002S (1377), KR002T (1344), KR002U (50), KR002V (31), KR002W (22), KR002X (13), KR002Y (18), KR002Z (45), KR0030 (32), KR0036 (2793), KR0037 (1841), KR0038 (863), KR0039 (2398), KR003A (1748), KR003B (1412), KR003C (987), KR003D (793), KR003E (359), KR003F (429), KR003G (1335), KR003H (1399), KR003J (3386), KR003K (2327), KR003L (2598), KR003M (3385), KR003N (4903), KR003P (3579), KR003Q (3275), KR003R (3312), KR003S (3481), KR003T (4507), KR003U (2186), KR003V (1723), KR003W (2791), KR003X (3531), LU0001 (2423), LU0002 (1783), MA0001 (862), MA0002 (540), MA0003 (1312), MX0001 (53), MX0003 (76), MX0004 (3), MX0006 (165), MX0009 (92), MX000A (1), MX000B (41), MX000C (20), MX000D (775), MX000E (221), MX000F (88), MY0001 (4), MY0002 (106), MY0004 (26), MY0005 (15), MY0006 (82), MY0008 (122), MY000B (8), MY000C (93), MY000D (5), MY000E (62), NL0001 (1835), NL0006 (1226), NL0009 (3363), NL000A (1197), NL000B (623), NL000C (3383), NL000D (1287), NL000G (1425), NL000K (1811), NL000L (90), NL000M (2518), NL000N (2711), NL000P (2752), NL000Q (2907), NL000R (3295), NL000S (3774), NL000T (2494), NL000U (3429), NL000W (1290), NL000Z (3807), NL0010 (2853), NL0011 (2421), NL0013 (3183), NL0014 (2908), NL0017 (2244), NL0019 (1962), NL001A (704), NL001B (644), NL001D (427), NL001E (441), NL001F (475), NZ0001 (3274), NZ0002 (4674), NZ0003 (3427), NZ0004 (5571), NZ0007 (4955), NZ0008 (1970), NZ0009 (4333), NZ000A (67), NZ000B (2443), NZ000C (477), NZ000D (5158), NZ000F (661), NZ000G (2531), NZ000H (2708), NZ000J (432), NZ000K (1564), NZ000L (776), NZ000M (2989), NZ000N (2598), NZ000P (396), NZ000Q (1248), NZ000R (1272), NZ000S (3854), NZ000T (887), NZ000U (1712), NZ000V (2364), NZ000W (2560), NZ000X (1107), NZ000Y (2727), NZ000Z (4586), NZ0010 (2312), NZ0011 (4920), NZ0012 (7040), NZ0013 (1238), NZ0014 (6484), NZ0015 (2999), NZ0016 (2153), NZ0017 (4886), NZ0018 (7676), NZ0019 (4572), NZ001A (3513), NZ001B (57), NZ001C (324), NZ001D (1326), NZ001E (1701), NZ001G (3814), NZ001H (2632), NZ001J (3084), NZ001K (296), NZ001L (2872), NZ001N (2625), NZ001P (5617), NZ001Q (2235), NZ001R (3674), NZ001S (5356), NZ001V (4951), NZ001W (1878), NZ001X (2908), NZ001Y (1312), NZ001Z (2407), NZ0020 (4256), NZ0021 (2656), NZ0022 (4850), NZ0023 (4973), NZ0024 (3626), NZ0025 (359), NZ0026 (5438), NZ0027 (6888), NZ0028 (1266), NZ0029 (5926), NZ002C (10194), NZ002D (2191), NZ002E (3430), NZ002F (5798), NZ002G (3377), NZ002H (3621), NZ002J (1772), NZ002K (4193), NZ002L (2649), NZ002M (94), NZ002N (7437), NZ002P (4959), NZ002Q (5316), NZ002R (7191), NZ002S (4250), NZ002T (6121), NZ002U (2095), NZ002V (3058), NZ002W (4518), NZ002X (7571), NZ002Y (2861), NZ002Z (5709), NZ0030 (7998), NZ0032 (4195), NZ0033 (7503), NZ0034 (6610), NZ0035 (2794), NZ0036 (6766), NZ0037 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UK0073 (993), UK0074 (1118), UK0077 (1106), UK0078 (2204), UK0079 (3085), UK007A (4125), UK007B (3582), UK007C (377), UK007G (1773), UK007H (2904), UK007J (1007), UK007P (4090), UK007Q (3772), UK007R (4188), UK007U (2294), UK007V (1099), UK007Y (4676), UK007Z (2537), UK0080 (2067), UK0081 (1948), UK0082 (693), UK0083 (2962), UK0084 (4633), UK0085 (832), UK0086 (1125), UK0087 (2118), UK0088 (1447), UK0089 (2980), UK008A (1761), UK008B (3149), UK008C (3130), UK008D (1906), UK008E (3), UK008F (6420), UK008G (3355), UK008H (902), UK008J (2635), UK008K (394), UK008M (790), UK008Q (3330), UK008R (638), UK008S (2452), UK008T (3398), UK008U (2321), UK008V (2360), UK008X (4475), UK008Z (2382), UK0090 (1542), UK0092 (3459), UK0096 (812), UK0098 (5740), UK0099 (5489), UK009A (553), UK009B (405), UK009C (2774), UK009D (3855), UK009F (1342), UK009G (4546), UK009J (3472), UK009K (4778), UK009L (4245), UK009M (2139), UK009P (5657), UK009Q (1980), UK009R (1470), UK009S (4078), UK009T (666), UK009U 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