Love shooting stars? Then you’ll love the Orionid Meteor Shower, the second meteor shower of October, which peaks October 21-22 each year.
What Are the Orionids?
The Orionids are an annual meteor shower caused by debris from the most famous of all comets, Halley’s Comet. The comet last visited Earth in 1986 and will return next in 2061. Each time that famous comet passed around the Sun, it would leave in its wake a trail of cosmic dust and grit along its orbit. Our Earth passes closest to Halley’s orbit every mid-to-late October, and in the process, encounters this comet debris. The particles ram into our atmosphere at speeds in excess of 40 miles per second, and thanks to friction, they are raised to white heat in the span of a heartbeat, creating the effect of a “shooting star” in our sky.
They are called Orionids because the meteors seem to emerge or radiate from the constellation Orion, near the Orion-Gemini border in Orion’s upraised club.
When To View The Orionids
The Orionids shower will be visible from October 16th-24th, with the highest period of activity on the 21st. The meteors can be seen with the naked eye. The best time to observe any meteor shower is during the early morning hours, from 4 to 5 a.m. local daylight time, with the numbers of meteors increasing until morning twilight interferes. Generally, observers can expect to see anywhere from 10 to more than 30 meteors per hour. A few Orionids may appear as early as the start of October and as late as November 7th.
An observer who plots these meteors on a star chart will notice that they seem to radiate or spray outward from northeastern Orion, between Betelgeuse and Gamma (γ) Geminorum, also known as Alhena; this region of the sky will be about two-thirds up from the southern horizon when morning twilight begins.
These meteors travel at around 42 miles per second when they enter the Earth’s atmosphere, twice as fast as the more prolific Geminids of December. Some bright ones may leave pretty trains. Enjoy the show!