The International Meteor Organization (IMO) was founded in 1988 and has more than 250 members now. IMO was created in response to an ever growing need for international cooperation of meteor amateur work. The collection of meteor observations by several methods from all around the world ensures the comprehensive study of meteor showers and their relation to comets and interplanetary dust.

You can read about the history, current aims and commissions of IMO. An additional page informs you about how to become a member the International Meteor Organization. Membership includes a subscription to WGN, the journal of the IMO.

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WGN 43:1 out now

WGN 43-1

The February 2015 issue of the IMO Journal is now in print. It will be mailed shortly and subscribers can also immediately access the journal in PDF format. The contents this month:

  • Janus (C. Verbeeck)
  • IMO's new online fireball form (M. Hankey, V. Perlerin)
  • International Meteor Conference 2015, 34th edition, August 27–30, Mistelbach, Austria (T. Weiland)
  • Various meteor scenes III: Recurrent showers and some minor showers (M. Koseki)
  • Results of the IMO Video Meteor Network — September 2014 (S. Molau, J. Kac, S. Crivello, E. Stomeo, G. Barentsen, R. Goncalves, C. Saraiva, M. Maciewski, M. Maslov)
  • Results of the IMO Video Meteor Network — October 2014 (S. Molau, J. Kac, S. Crivello, E. Stomeo, G. Barentsen, R. Goncalves, C. Saraiva, M. Maciewski, M. Maslov)

Front cover photo: Bright meteor on 2013 August 24 at 22h30m UT from Jura mountains, Switzerland. Photo courtesy: Jonas Schenker.

Fireball report form goes live!

If you see a fireball in the night sky, you can now report it to the IMO through our new fireball form! Translated into more than 25 languages, the form guides you through describing what you saw in a way that provides useful information to astronomers studying meteors. The information you provide can be combined with that of other eye-witnesses to give a good estimate of the trajectory of the fireball, and to help determine if a ground fall occurred.

Assuming no specialist astronomical knowledge or observing experience, the form easily takes you through the process of reporting a fireball sighting in detail. The information gathered from the submitted reports is collected into a public database which can be searched for particular events.

A large team of IMO volunteers has been hard at work translating the fireball form into more than 25 languages, and the IMO is now busy publicising it to local astronomical societies and observing groups around the world. Large fireball events often excite local media; if such an event happens in your region you can help by telling people about the form so that they can report what they saw.

If you would like to contribute a new translation in a language not already covered, or spot a mistake in the text of the form in your native language, please get in touch so that we can fix it, or follow the instructions to translators.

The IMO fireball report can be easily customized and branded for amateur societies, observatories, institutions or other astronomical organizations who receive fireball reports and enquiries from the public (see the Turkish Uzaybimer version for example, you may need to clear your browser cache). For more details, and to set up an account for your organization, please contact

If you would like to test the form without submitting a false event to the database, please use the test version of the form.

Happy fireball spotting!

New year starts with a bang in Romania

Never mind the new year fireworks, the start of 2015 happened with an even bigger bang, at least if you happened to be in Romania, Moldova or the Ukraine. The early hours of January 7th saw a massive fireball over the region, culminating in an explosion loud enough to wake people, and causing many to call the emergency services to report the event. In Romania reports of sightings have come in from across the country, putting the time of the explosion at 3:05 EET (01:05 UT), with people hearing the explosion in the counties of Buzau, Vrancea and Covasna.

So far over 50 recordings and eye witness reports have been collected by the IMO, many from surveillance cameras recording sudden brightening of whatever outside area was being monitored. A compilation of videos of the event, as recorded by security cameras, has been posted on youtube. The map below shows the location of the reports received so far, red dots are from surveillance cameras, the blue markers are visual reports from witnesses, and the green dots are reports from those who heard the terminal explosion.

Map of reported fireball sightings from Romania
Image by Raul Truta, compiled from online reports.
Red: detections by cameras, blue: visual observations, green: reports of sound heard.

The reports from Romania of the January 7th fireball put the maximum apparent magnitude of -16, brighter than the full Moon (-13). Roughly one in 1,200 meteors is brighter than magnitude -5, while only one on 12,000 meteors reaches magnitude -8 or brighter, so fireball events like this one are rare.

So far, information on the event is sparse. The explosion appears to have occurred at a height of roughly 55 kilometres and, although some fireballs do result in meteorite fragments reaching the ground, it is likely that in this case the meteoroid completely disintegrated.

Whether a fall occurs or not, the details of events like this can only be determined from combining the information from many eyewitness reports. If you see a bright fireball event like this, you can help researchers by reporting what you saw in as much detail as possible. You can find further information on meteors and other related events, and advice on how to observe and report them, visit the observations section of the IMO website.

WGN 42:6 out now

WGN 42-6

The December 2014 issue of the IMO Journal is now in print. It will be mailed shortly and subscribers can also immediately access the journal in PDF format. The contents this month:

  • From the Treasurer — IMO Membership/WGN Subscription Renewal for 2015 (M. Gyssens)
  • Solar Longitudes for 2015 (R. Arlt)
  • Details of the Proceedings of the International Meteor Conference, Giron, France, 18–21 September 2014 (J.-L. Rault, P. Roggemans)
  • A possible new shower on Eridanus-Orion border (D. Šegon, P. Gural, Ž. Andreić, D. Vida, I. Skokić, F. Novoselnik, L. Gržinić)
  • Observation of April alpha Capricornids (IAU#752 AAC) (SonotaCo, C. Shimoda, H. Inoue, T. Masuzawa, M. Sato)
  • Results of CMN 2013 search for new showers across CMN and SonotaCo databases III (D. Šegon, Ž. Andreić, P. Gural, I. Skokić, K. Korlević, D. Vida, F. Novoselnik, D. Gostinski)
  • Results of the IMO Video Meteor Network — July 2014 (S. Molau, J. Kac, S. Crivello, E. Stomeo, G. Barentsen, R. Goncalves, A. Igaz, C. Saraiva, M. Maciewski, M. Maslov)

Front cover photo: Bright fireball on 2014 February 24 at 01h45m UT from Milton, VT, USA. Photo courtesy: Ethan Rogati.

Geminids 2014 - the best meteor shower of the year

The nights between December 9 and 16 are marked by the best of all meteor showers – the Geminids. Up to 120 meteors per hour are visible during the shower’s peak on December 14 under dark skies, far from light pollution. This meteor shower, rich in bright, colorful meteors is also characterized by an unusually long period of relatively high activity – if you cannot observe on the peak night, you can see good numbers of meteors on December 12, 13 and 15! This year the peak of the Geminid meteor shower is expected on December 14 around 12h UT, but near-maximum rates persist for about a day, so everyone will have a good chance to see great meteor rates.

The activity graph below is updated every 15 minutes - click for details.

Geminids 2014

Unusual Geminids

But the Geminids are not remarkable only due to their strength, they are also somewhat unusual as meteor showers go. While most meteor showers are born from comets, the Geminids appear to be bits of an asteroid. The parent body of the meteor shower is asteroid 3200 Phaethon. This 5-km rocky body orbits the Sun in an elongated elliptical orbit, which carries it out to the main asteroid belt at aphelion and as close to the Sun as 0.14 astronomical units at perihelion (more than twice as close to the Sun than Mercury!). 3200 Phaethon is a B-type asteroid, but recent observations with the STEREO spacecraft have revealed cometary activity near perihelion, so it is also referred to as a “rock comet”. It is hypothesized that the dust release is caused by thermal fracturing of the surface of the comet under intense heating near the Sun. 3200 Phaethon is a very interesting body and will certainly be the target of much future research!

How to observe the Geminids?

To observe the Geminid shower at its best, try to find an observing spot far from city lights. Light pollution will greatly diminish the number of visible meteors. You need no specialized equipment to observe the Geminids! Dress warmly, bring a reclining chair and watch the sky. You will not need to wait long for the first Geminid to appear!

The Geminid radiant is located in the constellation of Gemini, near the bright stars Castor and Pollux. On the peak night the radiant is just about a degree north of Castor (the northern twin). All Geminids will appear to radiate from this point in the sky. With 35 km/s the Geminids are medium speed meteors.

On the peak night the waning gibbous Moon rises around local midnight, so the evening hours will be dark. For mid-northern latitudes the radiant rises at dusk, so some Geminids may be seen even during the early evening hours. And these Geminids are special! As the radiant is very low, meteoroids skim the upper layers of the atmosphere nearly tangentially, creating long meteors that can traverse half of the sky or more! These meteors are called Earth grazers. As the radiant rises higher in the sky, the number of meteors increases. But even in the morning hours, as the Moon rises higher in the sky, still many Geminids will be visible, right up until dawn.

If you decide to do observe the Geminids, use the IMO major meteor shower observing technique. This way your data will be in a standard format, that can readily be used for analysis. Send us your data as soon after the observations as possible.

How to photograph the Geminids?

If you are new to meteor photography, this shower will be somewhat more difficult due to the bright Moon. But photographing meteors is fun, and it is easy. You will need a good camera – a DSLR, a mirrorless cam or a good bridge camera will do, a tripod and a remote release. Set the aperture to a wide setting, depending on the lens you have this is usually anywhere between f/1.4 and f/3.5. Set the camera to Manual mode (M) or Bulb (B), depending on what your camera offers. You would usually go for a relatively high ISO value, but since the sky will be bright you can stay at about ISO 800 or so. Now focus the image. Focusing your camera is absolutely crucial! There are few things as frustrating as out of focus photos! Use live view to focus on a star manually. Shift the focus around until the image of the star on your screen reaches minimum size. You can also use autofocus on the Moon, but do check your first photo if it is really in focus. Then set your exposure to about 10 – 15 seconds and use the remote release to make the photo (if you do it on your camera shutter button your photos will be blurred due to camera motion). Then find the exposure you are most comfortable with – this will depend on how bright you allow the photos to be (do not go too far or any meteors will be drowned out in the bright background) and how bright your sky is.

WGN 42:5 out now

WGN 42-5

The October 2014 issue of the IMO Journal is now in print. It will be mailed shortly and subscribers can also immediately access the journal in PDF format. The contents this month:

  • Letter — Meteoroid streams, meteor showers (J. Rendtel)
  • From the Treasurer — IMO Membership/WGN Subscription Renewal for 2015 (M. Gyssens)
  • Letter — The CMN catalogue of orbits for 2012 (J. Rendtel)
  • International Meteor Conference 2014 report (A. Egal)
  • First announcement of the International Meteor Conference 2015 (T. Weiland)
  • Details of the Proceedings of the International Meteor Conference, Poznań, Poland, 22–25 August 2013 (M. Gyssens, P. Roggemans, P. Žołądek)
  • Various meteor scenes I: the perception and the conception of a ’meteor shower’ (M. Koseki)
  • Various meteor scenes II: Cygnid-Draconid Complex (κ-Cygnids) (M. Koseki)
  • Meteorite producing fragment on the Apophis’ orbit (A. Terentjeva, E. Bakanas)
  • Results of the IMO Video Meteor Network — June 2014 (S. Molau, J. Kac, S. Crivello, E. Stomeo, G. Barentsen, R. Goncalves, A. Igaz)

Front cover photo: Bright meteor on 2014 May 29 at 03h33m UT from Observatorio del Teide, Tenerife, Spain. Photo courtesy: Jürgen Rendtel.