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Orionids

Orionids (ORI)
Orionid12n.jpg
An Orionid meteor (center right) streaking across the sky below the Milky Way and to the right of Venus. The zodiacal light can also be seen in the image.
Discovery date October 1839
Parent body 1P/Halley
Radiant
Constellation Orion (near Betelgeuse)
Right ascension 06h 24m
Declination +15°
Properties
Occurs during October 16 – October 27
Date of peak October 21
Velocity 66.9 km/s
Zenithal hourly rate typically 20–25
See also: List of meteor showers

The Orionid meteor shower, usually shortened to the Orionids, is the most meteor shower associated with Halley's Comet. The Orionids are so-called because the point they appear to come from, called the radiant, lies in the constellation Orion, but they can be seen over a large area of the sky. Orionids are an annual meteor shower which last approximately one week in late October. In some years, meteors may occur at rates of 50–70 per hour.

Meteor showers first designated "shooting stars" were connected to comets in the 1800s. E.C. Herrick made an observation in 1839 and 1840 about the activity present in the October night skies. A. S. Herschel produced the first documented record that gave accurate forecasts for the next meteor shower. The Orionid meteor shower is produced by the well known Halley's Comet, which was named after the astronomer Edmund Halley and last passed through the inner solar system in 1986 on its 75- to 76-year orbit. When the comet passes through the solar system, the sun sublimates some of the ice, allowing rock particles to break away from the comet. These particles continue on the comet's trajectory and appear as meteors ("falling stars") when they pass through Earth's upper atmosphere. Halley's comet is also responsible for creating the Eta Aquariids, which occur each May.

* This meteor shower may give double peaks as well as plateaus, and time periods of flat maxima lasting several days.

The radiant of the Orionids is located between the constellations Orion and Gemini (in the south-eastern sky before dawn, as viewed from mid-northern latitudes. The most active time of the meteor shower was stated by Telegraph.uk.co to be in the early morning of October 21, 2009 6 a.m. Eastern Standard Time in the United States or 11 a.m. in the United Kingdom. Tweets and user news articles were shared on Social networking and micro-blogging services such as Twitter and Yahoo! Buzz. Photos and videos of the event were posted on photo and video sharing websites such as YouTube and Flickr. Universe Today reported that the meteor shower arrived at 140,000 miles (230,000 km) per hour on the morning of the 21 when showing was predicted to be at its height, however compared to previous showers in years past, the trail of 2009 appeared narrower without branching out. Observers observing the small meteor "Halleyids" at Alabama's Space Flight Center saw streaks radiating in all directions with the naked eye.


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Wikipedia

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