Template:Short description Template:Infobox meteor shower

The Geminids are a prolific meteor shower with 3200 Phaethon (which is thought to be an Apollo asteroid<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> with a "rock comet" orbit.<ref name="Jewitt2010" />) being the parent body.<ref name=IAUC3881>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> Because of this, it would make this shower, along with the Quadrantids, the only major meteor showers not originating from a comet. The meteors from this shower are slow, they can be seen in December and usually peak around December 4–16, with the date of highest intensity being the morning of December 14. Current showers produce up to 120–160 meteors per hour under optimal conditions, peaking around 2:00 or 3:00. Geminids were first observed in 1862,<ref name="Kronk"/> much later than other showers such as the Perseids (36 AD) and Leonids (902 AD).

Based on data from the Parker Solar Probe, a 2023 study suggested that the Geminids may have been formed by the catastrophic breakup of a comet that formed asteroids 2005 UD and 1999 YC in addition to Phaethon.<ref>Template:Cite journal</ref><ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

BackgroundEdit

The Geminid meteor shower is unique among celestial events as it originates not from a comet but from the asteroid 3200 Phaethon, discovered on Oct. 11, 1983, by the Infrared Astronomical Satellite (IRAS). Phaethon's 1.4-year orbit around the Sun and its comet-like elliptical trajectory have led scientists to speculate if it is a "dead comet" or a distinct celestial entity known as a "rock comet." Despite its comet-like orbit, Phaethon lacks a cometary tail and exhibits spectra resembling a rocky asteroid. The Geminid meteoroids formed from Phaethon are denser (2–3 g/cm3) than typical cometary dust flakes (0.3 g/cm3). Named after the Greek mythological figure who drove the Sun-god Helios' chariot, Phaethon's discovery was attributed to astronomer Fred Whipple.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

RadiantEdit

File:Geminids-2025-EN.jpg
Appearance of the Geminids on 13 December 2025 at 21:00 local winter time
File:Geminid 121407 1.jpg
A Geminid meteor in 2007, seen from San Francisco
File:Asteroid Phaethon 25dec2010 stack.jpg
Asteroid (3200) Phaethon, parent body of the Geminids, imaged on December 25, 2010, with the 37 cm F14 Cassegrain telescope of Winer Observatory, Sonoita (MPC 857)

The meteors in this shower appear to come from the radiant in the constellation Gemini (hence the shower's name). However, they can appear almost anywhere in the night sky, and often appear yellowish in hue. Well north of the equator, the radiant rises about sunset, reaching a usable elevation from the local evening hours onwards. In the southern hemisphere, the radiant appears only around local midnight or so. Observers in the northern hemisphere will see higher Geminid rates as the radiant is higher in the sky.<ref name="Meteorwatch2"/> The meteors travel at medium speed in relation to other showers, at about Template:Convert, making them fairly easy to spot. They usually fall apart while at heights above Template:Convert.<ref name="Meteorwatch"/>

File:Meteor falling courtesy NASA.gif
Animated GIF of a Geminid meteor falling earthwards

TimelineEdit

Year Peak of shower ZHRmax Lunar phase<ref>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

2006 December 14 115<ref name=IMO2006>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

33% waning crescent
2007 December 15 122<ref name=IMO2007>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

30% waxing crescent
2008 December 14 139<ref name=IMO2008>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

95% full moon
2009 December 13 120<ref name=IMO2009>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

9% new moon
2010 December 14 127<ref name=IMO2010>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

59% first quarter
2011 December 14 198<ref name=IMO2011>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

86% waning gibbous
2012 December 14<ref name=IMO2012P>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

109<ref name=IMO2012>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

2% new moon
2013 December 14<ref name=IMO2013>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

134<ref name=IMO2013b>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

92% full moon
2014 December 14<ref name=IMO2014>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

253<ref name=IMO2014b>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

50% last quarter
2015 December 14 120<ref>Template:Cite news</ref> 10% waxing crescent
2016 December 13 25<ref>Template:Cite news</ref> 100% full moon
2017 December 14 145<ref>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

13% waning crescent
2018 December 14 Template:Value<ref>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

41% waxing crescent
2019 December 14 120<ref>Template:Cite news</ref> 94% waning gibbous
2020 December 13 120<ref>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

2% waning crescent
2021 December 13 Template:Value<ref>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

73% waxing gibbous
2022 December 14 120 72% waning gibbous
2023 December 13 150<ref>{{#invoke:citation/CS1|citation CitationClass=web

}}</ref>

0% waxing crescent

See alsoEdit

ReferencesEdit

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External linksEdit

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Template:Meteor showers