HD 10180 c
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 10180 | |
Constellation | Hydrus | |
Right ascension | (α) | 01h 37m 53.5763s |
Declination | (δ) | −60° 30′ 41.499″ |
Apparent magnitude | (mV) | 7.33 |
Distance | 128 ± 3 ly (39.4 ± 1 pc) | |
Spectral type | G1V | |
Mass | (m) | 1.062 ± 0.017 M☉ |
Radius | (r) | 1.20 ± 0.318 R☉ |
Temperature | (T) | 5911 K |
Metallicity | [Fe/H] | = |
Age | 7.3 Gyr | |
Orbital elements | ||
Semi-major axis | (a) | 0.0641 ± 0.0010 AU |
Eccentricity | (e) | 0.045 ± 0.026 |
Orbital period | (P) | 5.75979 ± 0.00062 d |
Orbital speed | (υ) | 136 km/s |
Argument of periastron |
(ω) | 332 ± 43° |
Physical characteristics | ||
Minimum mass | (m sin i) | 13.10 ± 0.54 M⊕ |
Discovery information | ||
Discovery date | 24 August 2010 | |
Discoverer(s) | ||
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 10180 c is an extrasolar planet approximately 130 light-years away in the constellation Hydrus. With a minimum mass comparable to that of Neptune, it is of the class of planets known as Hot Neptunes. Dynamical simulations suggest that if the mass gradient was any more than a factor of two, the system would not be stable.
While planet c does not exist in any mean motion resonances, both planets with adjacent orbits (b and d) share near resonances with c.
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