2013 Orionids Forecast
This year the Orionids will peak during the early morning hours of 20 and 21 of October. A bright and waning gibbous moon will make this year less than favorable for viewing the Orionids. However, as these meteors are known for their brightness, it still may be possible to view them during the hours between midnight and dawn.
- Comet of Origin: 1P/Halley
- Radiant: Just to the north of constellation Orion's bright star Betelgeuse
- Active: 2 Oct. - 7 Nov. 2013
- Peak Activity: 20-21 Oct. 2013
- Peak Activity Meteor Count: Approximately 20 meteors per hour in moonless skies.
- Meteor Velocity: 66 km (41 miles) per second
About the Meteor Shower
The Orionids, which peak during mid-October each year, are considered to be one of the most beautiful showers of the year. Orionid meteors are known for their brightness and for their speed. These meteors are fast -- they travel at about 148,000 mph (66 km/s) into the Earth's atmosphere. Fast meteors can leave glowing "trains" (incandescent bits of debris in the wake of the meteor) which last for several seconds to minutes. Fast meteors can also sometimes become fireballs: Look for prolonged explosions of light when viewing the Orionid meteor shower.
The Orionids are also framed by some of the brightest stars and planets in the night sky, which lend a spectacular backdrop for theses showy meteors.
The Orionids are viewable in both the Northern and Southern hemispheres during the hours after midnight. Find an area well away from city or street lights. Come prepared with a sleeping bag, blanket or lawn chair. Lie flat on your back with your feet facing southeast if you are in the Northern Hemisphere or northeast if you are in the Southern Hemisphere, and look up, taking in as much of the sky as possible. In less than 30 minutes in the dark, your eyes will adapt and you will begin to see meteors. Be patient -- the show will last until dawn, so you have plenty of time to catch a glimpse.
Where Do Meteors Come From?
Meteors come from leftover comet particles and bits from broken asteroids. When comets come around the sun, the dust they emit gradually spreads into a dusty trail around their orbits. Every year the Earth passes through these debris trails, which allows the bits to enter our atmosphere where they disintegrate to create fiery and colorful streaks in the sky.
The pieces of space debris that interact with our atmosphere to create the Orionids originate from comet 1P/Halley. Each time that Halley returns to the inner solar system its nucleus sheds ice and rocky dust into space. The dust grains eventually become the Orionids in October and the Eta Aquarids in May if they collide with Earth's atmosphere.
Comet Halley takes about 76 years to orbit the sun once. The last time comet Halley was seen from the Earth was in 1986. Comet Halley will not enter the inner solar system again until 2061.
The comet is named for Edmond Halley, who discovered in 1705 that three previous comets seemed to return every 76 years or so and suggested that these sightings were in fact all the same comet. The comet returned as he predicted (after his death) and it was named in Halley's honor. Comet Halley is perhaps the most famous comet -- it has been sighted for millennia. It is featured on the Bayeux tapestry, which chronicles the Battle of Hastings in 1066.
Comet Halley's dimensions are 16 x 8 x 8 km. It is one of the darkest, or least reflective, objects in the solar system, with an albedo of 0.03.
Their radiant -- the point in the sky from which the Orionids appear to come from -- is the constellation Orion. The constellation of Orion is also where we get the name for the shower: Orionids. Note: The constellation for which a meteor shower is named only serves to aid viewers in determining which shower they are viewing on a given night. The constellation is not the source of the meteors.
Also, you need not look only to the constellation of Orion to view the Orionids -- they are visible throughout the night sky. It is actually better to view the Orionids at least 90 degrees away from the radiant. They will appear longer and more spectacular from this perspective. If you do look directly at the radiant, you will find that the meteors will be short -- this is called foreshortening.
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