Gliese 22
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Gliese 22, also catalogued V547 Cassiopeiae or ADS 440, is a hierarchical star system approximately 33 light-years away in the constellation of Cassiopeia. The system consists of pair of red dwarf stars, Gliese 22A and Gliese 22C, orbited by a third red dwarf Gliese 22B in an outer orbit of about 223 years.
The discovery of flare activity on Gliese 22A was announced by Bjørn Ragnvald Pettersen in 1975,[1] which led to it being given a variable star designation, V547 Cassiopeiae, in 1977.[12]
Planetary system
As of 2008, it was announced that a possible extrasolar planet, Gliese 22B b, orbits Gliese 22B but this is currently unconfirmed. The study in 2011 has indicated the orbit of the purported planet is stable.[13]
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References
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External links
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- Pages with script errors
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- Binary stars
- Brown dwarfs
- Cassiopeia (constellation)
- Durchmusterung objects
- Flare stars
- Gliese and GJ objects
- Hipparcos objects
- M-type main-sequence stars
- Objects with variable star designations
- Hypothetical planetary systems
- TIC objects
- Long stubs with short prose