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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The Perseids, one of the finest and the most-observed annual meteor shower peaks on August 12/13. This year the very impressive meteor shower, rich in bright trained meteors and fireballs coincides almost perfectly with the Full Moon. The bright moonlight will drown out all but the brightest of Perseids, diminishing the visual rates by 3-5 times. Still, those willing to persevere under the bright skies may be rewarded with a sprinkling of bright and colorful Perseids.
The activity graph below is updated every 15 minutes - click for details.
Perseids 2014 in detail
The Perseid meteor shower is caused by meteoroids, dust particles from the well-known, bright periodic comet 109P/Swift-Tuttle. The shower is active from mid-July to late-August, although the latest work by Molau (2013) indicates the shower may commence even earlier. It peaks on August 13 with the zenithal hourly rate usually reaching 80 – 100 meteors per hour. Under dark skies this translates to about 1 to 2 meteors per minute. This year, however, a waning gibbous Moon is high in the sky most of the peak night. The peak is expected late on August 12 to early on August 13 (Aug 12 19h UT to Aug 12 08h UT), although work by Jeremie Vaubaillon suggests the peak may occur earlier, during the second half of August 12.
Looking east at 45° N on August 13, 3:00 local time. The radiant is high in the northeast, the nearly full Moon (92% phase) is in the constellation Pisces.
Observing meteor showers under a nearly full Moon is difficult. Moonlight is scattered on haze and aerosols, producing a bright sky and greatly diminishing the number of visible meteors. By taking some additional steps, however, this effect may be mitigated to some extent. The most important step to take is to choose an observing spot at a higher elevation. Usually the most dramatic improvement occurs up to about 1500 m high, but if it is possible try to go even higher. By going above the haze the sky darkens quite dramatically and the number of visible meteor increases significantly. While observing, face away from the Moon. If possible, place it behind an object (house, tower, mountain, …). Some observers use an umbrella, to good effect. Even by taking all these steps you probably will not see nearly as many meteors as under a dark moonless sky, unless something completely unexpected happens. But strong meteor showers are fairly rare, so why not make the most of it?
Perseid radiant drift from mid July to late August. Radiant positions are marked for every 5 days.
On the peak night the radiant of the Perseids is located at the northern tip of Perseus. With 59 km/s members of this meteor shower are swift. The radiant of the shower is at its lowest early in the night and rises steadily towards the morning. Consequently the number of Perseids is the lowest in the evening hours and highest in the morning hours. This year on the peak night the Moon rises during evening twilight and is at its highest in the morning hours, somewhat diminishing the increase in the number of visible meteors by brightening the sky.
To observe the Perseids, you need to dress warm, bring a reclining chair and watch the sky. You need no other equipment. If you decide to do so, 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.
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.
When things go right. Jure Atanackov captured this brilliant -9 magnitude Perseid fireball in constellation Cetus on August 12, 2010 with a Nikon D80 camera set to ISO 1600 and an 18-mm f/3.5 lens (100 sec exposure). Such meteors are rare, but the excitement of catching a brilliant fireball is tremendous!
The June 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:
Front cover photo: Frame-by-frame development of a Camelopardalid on 2014 May 24 at 01h58m08s UT. Original recording by Peter C. Slansky; compilation by Jim Albers and Peter Jenniskens.
The sky may erupt on May 24 in one of the strongest meteor showers of the past decade. On May 24 the Earth intersects a number of dust trails by comet 209P/LINEAR. Such an encounter would usually promise an exceptionally strong meteor shower, but things are much more complicated with this meteor shower.
On May 24 around 7-8h UT the Earth intersects a large number of dust trails released by comet 209P/LINEAR. This event is expected to result in a potentially significant meteor shower, which may be one of the strongest in the past decade. But very little is known about the meteoroid stream that may produce the shower and anything is possible, from a barely detectable shower to a very strong outburst. The radiant of the shower, the point from which the meteors apparently radiate from is in the large, but inconspicuous constellation of Camelopardalis. The radiant is located about 10° southwest of Polaris, nearly halfway between the brightest star in Ursa Major (Big Dipper) – Dubhe and Cassiopea (RA 125°, Dec +79°). Contrary to well known annual meteor showers, such as the Perseids, Orionids and Geminids, the Camelopardalids will be very slow with their velocity being only 18 km/s.
View towards the north on May 24, 7:30 UT from Toronto. The radiant is marked with the red circle. Note the rising waning crescent Moon.
The timing of the peak, May 24 7-8h UT (2-3h EST, 1-2h CST) favours the North American continent. The radiant is circumpolar – it never sets – for latitudes above 11 °N. The best conditions will be found where the radiant is highest in a dark sky. The best locations will be near the USA-Canada border east of North Dakota. Locations further west and south will have the radiant lower in the sky and will consequently see less meteors. Locations further north will never have a fully dark sky as the Sun never goes deep enough below the horizon. Any early or late activity of the meteor shower may be visible over European and Pacific longitudes, respectively. At the time of the peak, the constellation of Camelopardalis will be at its lowest in the sky, directly below Polaris.
Visibility of the Camelopardalids. Image courtesy: Geert Barentsen.
The April 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:
Front cover photo: September ε-Perseids fireball photographed on 2013 September 9 from Gahberg observatory in Austria. Photo courtesy: Erwin Filimon.
The Eta Aquariids reach peak activity over the next few nights, providing one of the best meteoric displays for the southern hemisphere and a special treat for observers in the northern hemisphere. The activity graph below is updated every 15 minutes - click for details.
The period May 4 – 8 sees the peak of activity of the Eta Aquariid meteor shower. This is the strongest meteor shower of the south celestial hemisphere and is also best observed from the southern hemisphere. The shower is caused by meteoroids (small crumbs) of the most famous of all periodic comets - 1P/Halley. This shower's radiant, the apparent point where the meteors fly out or radiate from (hence the name) is in constellation Aquarius. More precisely the radiant is located close to the conspicuous ''Mercedes'' asterism of four 3rd magnitude stars. While Eta Aquariids can appear anywhere in the sky, tracing their paths backwards will intersect the radiant. At 66 km/s the Eta Aquariids are very fast meteors which often leave persistent trains.
Position of the Eta Aquariid radiant as listed in the IMO meteor shower calendar.
Being a southern hemisphere meteor shower the Eta Aquariids are best seen from the southern hemisphere. The radiant rises in the morning, so only in the final two hours or so before dawn will any Eta Aquariids be visible. Evening and midnight hours will be devoid of Eta Aquariids. The shower’s peak ZHR (Zenithal Hourly Rate) is somewhat variable, ranging from 50 to 80 meteors per hour. In 2013, however, there was a significant activity outburst as the ZHR reached approximately 130 meteors per hour with a high proportion of bright meteors.
Preliminary ZHR (activity) graph of Eta Aquariids in 2013. More information on the 2013 shower on the "live" page.
Higher northern latitudes will see low activity from the Eta Aquariids as the radiant never rises high above the horizon. However, active meteor showers with their radiant near the horizon provide a special visual treat for observers – the so-called “Earth grazers”. These are meteors that strike our atmosphere nearly tangentially, skimming its higher parts. Such meteors are exceptionally long, stretching halfway or nearly across the entire sky and lasting for several seconds. While only a few of these will be visible when the radiant is low, each will be spectacular! Good luck with your observations!
To observe the Eta Aquariids, you need to dress warm, bring a reclining chair and watch the sky. You need no other equipment. If you decide to do so, 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 posssible.
The 2013 outburst of the Eta Aquariids was caused by several old dust trails the Earth encountered. Mikiya Sato posted a warning for observers on "meteorobs" mailing list two days before the peak about the possible increase in activity. The Earth encountered dust trails released in 1197 and 970 BC with additional meteoroids from 1403, 1333, 1265, 1128, 985 and 835 BC. No predictions are available for 2014 at this time.