The 2023 Orionid Meteor Shower Ready to Rain Down on Earth This Fall—All You Need to Know

The 2023 Orionid Meteor Shower Ready to Rain Down on Earth This Fall—All You Need to Know
(Illustration - Brian Spencer/Shutterstock)
Michael Wing
10/12/2023
Updated:
10/13/2023
0:00
A little comet dust. A few shooting stars. Fireballs from above. Fall meteors are here—and it’s awe-inspiring to imagine how those infinite silver shards rain down from space like on some cosmic schedule, as they have done for eons. One group of meteors in particular faithfully returns every year around this time without fail.

The Orionids

Every mid- to late-October, we cross paths with a group of meteors called the Orionids. They seem to emanate from the same spot on our star map every year—right beside the club of the constellation Orion the Hunter, hence the name Orionids. But the meteors don’t actually come from that constellation; rather, they hail from a comet travelling along a vast loop around our sun, Halley’s Comet.

Said comet orbits once every 75-76 years, travelling in a retrograde orbit, meaning the opposite way as the planets, leaving a vast complex of dust and debris in its wake, spread across outer space. Earth collides with this enormous dust loop both on the inbound and outbound legs of its journey.

Meteors of the Orionids streak over the mountainous area of Tannourine in northern Lebanon, on Oct. 3, 2021. (IBRAHIM CHALHOUB/AFP via Getty Images)
Meteors of the Orionids streak over the mountainous area of Tannourine in northern Lebanon, on Oct. 3, 2021. (IBRAHIM CHALHOUB/AFP via Getty Images)
When our planet plows through that debris field on its inbound leg, it rains down on us and burns up in our atmosphere, causing the meteor shower, the Orionids—that’s why we have them every year. Earth also passes through the outbound leg of Halley’s Comet’s trail, causing the Eta Aquariid meteor shower in May.

Peak Orionid Season

Orionid meteors could actually be seen as early as Sept. 26 and will last as late as Nov. 22 this year. Yet their broad maximum will occur from Oct. 20-25, according to Almanac. They will reach their peak at 12:05 a.m. your local time, on the morning of Oct. 22, though the morning of Oct. 21 will present similar meteor yields. That’s less than two weeks away before they peak.
Moon conditions will be optimal for viewing, as the first quarter moon will set around 11:30 p.m. on Oct. 21, leaving dark skies thereafter. It is advisable to find a viewing location in the countryside or where there are no artificial lights to interfere with the spectacle. The Orionids tend to not be overly bright and they shoot very fast—as fast as 41 miles per second, according to EarthSky.
Orionids meteors in 2016. (Brian Spencer/Shutterstock)
Orionids meteors in 2016. (Brian Spencer/Shutterstock)
Stargazers can expect anywhere from 10-30 meteors per hour and around 25 per hour during peak, though meteors are highly unpredictable by nature. What the Orionids lack in luster is compensated for by the long streaks of light they very often leave, called persistent trains. These streaks are caused by ionized gas left behind as particles burn up in Earth’s atmosphere due to friction. The meteors can even sometimes break up into multiple pieces or explode in dramatic fireballs.

The Orionids’ Origin: The Radiant, The Constellation, and the Comet

You'll find the constellation Orion the Hunter ascending in the east around midnight during peak Orionid season. In the northeast of the constellation, near Orion’s club, the Orionids seem to radiate from a point between the ruddy, rust-colored bright star Betelgeuse and Gamma Geminorum (or Alhena). That point is called the Orionids’ radiant, yet they don’t actually emanate from between those two stars; it’s merely an optical effect, an illusion, similar to how train tracks seem to converge on the horizon but never actually meet.

When trying to spot Orion’s meteors, you ought not look to the radiant point itself. Rather, try and take in the whole sky; they will shoot from the radiant and may appear anywhere above the horizon. Actually, the Orionids don’t hail from the constellation Orion itself. They come from the distant celestial traveler called Halley’s Comet.

The Orionids' radiant point next to the constellation Orion, toward the east. (This image has been edited. Till Credner/<a href="https://commons.wikimedia.org/wiki/File:OrionCC.jpg">CC BY-SA 3.0</a>)
The Orionids' radiant point next to the constellation Orion, toward the east. (This image has been edited. Till Credner/CC BY-SA 3.0)

What are comets? Basically, hunks of frozen gas and cosmic dust, often traveling along colossal orbits around the sun. The solid, packed center of a comet is called a nucleus. The last time Halley’s nucleus was seen from Earth with the unaided eye was in 1986. As it orbits once every 75-76 years, it won’t be back until 2061.

Most comets are named after their discoverers. But Halley’s wasn’t. Instead, it was christened after the astronomer who, in 1705, first accurately predicted its return. That man was Edmund Halley.

The Orionids’ parent comet extends far beyond its nucleus, to include a vast complex of debris spread across millions of miles throughout the system. Comets constantly shed their matter—space dust, frozen gas, and debris—as they move through the universe. That shedding intensifies as they near the sun, even causing them to glow with a bright greenish hue as their icy surfaces sublimate.

As for the question whether meteors follow some cosmic schedule, one could say, yes. They really do. The Earth and Halley’s Comet have planned their yearly rendezvous long ago.

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Michael Wing is a writer and editor based in Calgary, Canada, where he was born and educated in the arts. He writes mainly on culture, human interest, and trending news.
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