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: http://star.arm.ac.uk/press/2014/geminids2014_pr.html
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The Geminid meteor shower is the last, and one of the best, major meteor showers of the year. The meteors, or "shooting stars", can be seen at any time from late evening onwards during the period 7тАУ17 December and with a broad maximum in activity on the night of the 13/14 December. The Geminid shower usually includes a number of bright meteors, or fireballs, and because they are also relatively slow-moving compared to those from many other meteor showers, they are easily observed. For those who have never seen a meteor, provided the sky is clear the Geminids provide a perfect opportunity.
Shower meteors appear to come from a point in the sky known as the radiant. In the case of the Geminids, this is roughly the same direction as the two bright stars Castor and Pollux, the so-called "twins" of the constellation Gemini. In mid-December, the Geminid radiant rises around 7.00pm, and by 10pm it has reached a moderately high altitude in the East. Around this time, the stars Castor and his distinctly orange "twin" Pollux can be seen standing one above the other towards the East, along with the familiar winter constellation Orion lying at about the same altitude towards the South-East, that is, slightly to the right of Gemini.
The number of meteors that may potentially be observed during the maximum of the shower on the evening of the 13/14 December, and from a clear, dark site with no light pollution and little moonlight, can range up to as many as 100 or more per hour. However, most observers will see fewer than this, perhaps around 30 per hour from a moderately clear site with no light pollution and shaded from moonlight.
These Geminid meteors are produced by the collision of small particles, debris from the unusual near-Earth asteroid (3200) Phaethon, with the EarthтАЩs upper atmosphere. The asteroid is approximately 5 kilometres across, and orbits the Sun once every 1.43 years. It is currently more than 100 million kilometres from Earth. The small rocky particles, or meteoroids, from the asteroid move in roughly the same elliptical orbit as their parent body and are spread nearly evenly around the whole orbit. They collide with our planet at speeds of around 35 kilometres per second (approximately 80,000 miles per hour). This is a relatively slow velocity compared to that of many other shower meteors, but is nevertheless high enough to cause the meteoroids to burn up in the EarthтАЩs atmosphere in the region known as the mesosphere, at a height of around 80 kilometres (50 miles). It is the burning up of the meteoroid that produces the observed fast-moving streak of light called a meteor.
In order to observe meteors, the main rules are always the same. That is, find a place as far as possible from any light pollution or the interfering light of the Moon. Wrap up well against the freezing cold and make yourself comfortable. Allow plenty of time for your eyes to become adapted to the dark; and look at a convenient angle, perhaps 45 or 90 degrees away from the radiant, ready to catch the meteors when they appear.
FOR FURTHER INFORMATION PLEASE CONTACT: Mark Bailey at the Armagh Observatory, College Hill, Armagh, BT61 9DG. Tel.: 028-3752-2928; FAX: 028-3752-7174; meb
arm.ac.uk.
See also: Observations of (3200) Phaethon made with the Faulkes Telescope
Last Revised: 2014 December 15th |