HD 217580
Star HD 217580 |
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AladinLite | |||||||||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
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Constellation | Aquarius | ||||||||||||
Right ascension | 23 h 01 m 51.54 s | ||||||||||||
declination | -03 ° 50 ′ 55.4 ″ | ||||||||||||
Apparent brightness | 7.48 likes | ||||||||||||
Typing | |||||||||||||
Spectral class | K4 V | ||||||||||||
Astrometry | |||||||||||||
Radial velocity | (−44.1 ± 0.4) km / s | ||||||||||||
parallax | (58.70 ± 0.92) mas | ||||||||||||
distance | (55.6 ± 0.9) ly (17.0 ± 0.3) pc |
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Visual absolute brightness M vis | +6.3 mag | ||||||||||||
Proper movement | |||||||||||||
Rec. Share: | (+396.20 ± 0.93) mas / a | ||||||||||||
Dec. portion: | (−207.68 ± 0.73) mas / a | ||||||||||||
Physical Properties | |||||||||||||
radius | 0.96 R ☉ | ||||||||||||
Effective temperature | 4590 K | ||||||||||||
Other names and catalog entries |
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HD 217580 is a main sequence star of spectral class K in the constellation Aquarius, about 56 light years from Earth . With an apparent brightness of 7.48 mag, it can no longer be seen with the naked eye, even under optimal observation conditions. The star has a spectroscopic companion that is believed to be a red dwarf .
Spectroscopic companion
HD 217580 is orbited by a spectroscopic companion with a period of (454.7 ± 0.9) days and an eccentricity of (0.520 ± 0.022). Based on the mass determination of (0.161 ± 0.013) M ☉ , it is very likely a stellar object.
Sources and individual references
- ↑ a b c Hipparcos catalog (ESA 1997)
- ↑ Pulkovo radial velocities for 35493 HIP stars
- ↑ a b c Hipparcos, the New Reduction (van Leeuwen, 2007)
- ↑ Halbwachs et al .: Exploring the brown dwarf desert with Hipparcos ; in: Astronomy and Astrophysics, Vol. 355, pp. 581ff. (2000), bibcode : 2000A & A ... 355..581H
- ↑ Ribas, Ignasi; Jordi, Miralda-Escudé: The eccentricity-mass distribution of exoplanets: signatures of different formation mechanisms? ; in: Astronomy and Astrophysics, Vol. 464, Issue 2, pp. 779ff. (2007), bibcode : 2007A & A ... 464..779R