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Crucids
A minor meteor shower From Wikipedia, the free encyclopedia
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The Crucids are a group of meteor showers associated with the constellation Crux (the Southern Cross), primarily visible in the Southern Hemisphere.[1] The most notable showers within this group include the Alpha Crucids (α-Crucids), first recorded in the early 20th century,[2] and the Gamma Crucids (γ-Crucids), an unexpected meteor shower discovered in 2021.[3]The Crucids are characterized by meteors with velocities around 55.8 km/s,[4] and are believed to be linked to Halley-type comets.
They typically occur between January and February, though activity levels vary from year to year.
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Discovery
The Alpha Crucids were first observed in the 1920s and 1930s by astronomers R. McIntosh and C. Hoffmeister.[2]
The Gamma Crucids were first detected in February 2021[5] by low-light video camera networks in Australia, Chile, and New Zealand. Initially considered a previously unknown meteor shower, it was later designated as "IAU#1047" by the International Astronomical Union.
Observations suggest that the γ-Crucids may be linked to a Halley-type comet with a steeply inclined orbit.[1][3]
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Characteristics
Velocity
Crucid meteors travel at relatively slow speeds, around 55.8 km/s,[4] compared to other meteor showers.
Activity Period
Alpha Crucids
Active from January 6 to January 28, with peaks between January 12 and 20.[6]
Gamma Crucids
First detected in mid-February 2021, with peak activity on February 14.[4]
Radiant Point
- The α-Crucids radiate from a position near RA = 210.9°, Dec = -58.2°.
- The γ-Crucids radiate from RA = 192.6°, Dec = -56.0°.[7]
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Observation
The Crucid showers are best observed from southern latitudes due to their radiant location near the celestial south pole. Their low meteor rates make them a minor shower, but occasional peaks have been observed. Lunar interference can affect visibility, especially for the α-Crucids in some years.
References
External links
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