Extrasolar planet | List of extrasolar planets | |
---|---|---|
Parent star | ||
Star | HD 101930 | |
Constellation | Centaurus | |
Right ascension | (α) | 11h 43m 30.11s[1] |
Declination | (δ) | –58° 00′ 24.79″[1] |
Distance | 95 ± 2[1] ly (29.2 ± 0.7[1] pc) | |
Spectral type | K1V | |
Orbital elements | ||
Semimajor axis | (a) | 0.302 AU |
Periastron | (q) | 0.077 AU |
Apastron | (Q) | 0.335 AU |
Eccentricity | (e) | 0.11 ± 0.02 |
Orbital period | (P) | 70.46 ± 0.18 d (0.1929 y) |
Orbital speed | (υ) | 46.8 km/s |
Argument of periastron |
(ω) | 251 ± 11° |
Time of periastron | (T0) | 2,453,145.0 ± 2.0 JD |
Semi-amplitude | (K) | 18.1 ± 0.4 m/s |
Physical characteristics | ||
Mass | (m) | >0.30 MJ (>95 M⊕) |
Discovery information | ||
Discovery date | 14 February 2005 | |
Discoverer(s) | Lovis, Mayor, Pepe et al.[2] | |
Discovery method | Doppler spectroscopy (HARPS) | |
Discovery site | La Silla Observatory | |
Discovery status | Published[2] | |
Other designations | ||
GJ 3683 b, HIP 57172 b
| ||
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data |
HD 101930 b is an extrasolar planet orbiting the star HD 101930. It has a minimum mass a third of Jupiter's, nearly the same as Saturn's so it is thought to be a gas giant. It orbits the star closer than Mercury, and the orbit is slightly eccentric.[2]
References[]
- ↑ 1.0 1.1 1.2 1.3 (2007). Validation of the new Hipparcos reduction. Astronomy and Astrophysics 474 (2): 653–664.Vizier catalog entry
- ↑ 2.0 2.1 2.2 (2005). The HARPS search for southern extra-solar planets III. Three Saturn-mass planets around HD 93083, HD 101930 and HD 102117. Astronomy and Astrophysics 437 (3): 1121–1126.
External links[]
- HD 101930. Exoplanets.
Coordinates: Sky map 11h 43m 30.11s, −58° 00′ 24.793″
File:Iota-draconis-b.jpg | This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it. |
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