Extrasolar planet | List of extrasolar planets | |
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(Celestia image) |
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Parent star | ||
Star | HD 69830 | |
Constellation | Puppis | |
Right ascension | (α) | 08h 18m 23.9s |
Declination | (δ) | -12° 37′ 55.8″ |
Apparent magnitude | (mV) | 5.95 |
Distance | 41 ly (12.6 pc) |
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Spectral type | K0V | |
Mass | (m) | 0.86 ± 0.03 M☉ |
Radius | (r) | 0.89 R☉ |
Temperature | (T) | 5385 ± 20 K |
Metallicity | [Fe/H] | −0.05 ± 0.02 |
Age | 5.1–6.1 Gyr | |
Orbital elements | ||
Semimajor axis | (a) | 0.186 AU |
Eccentricity | (e) | 0.13±0.06 |
Orbital period | (P) | 31.56±0.04 d |
Argument of periastron |
(ω) | 221±35° |
Time of periastron | (T0) | 2,453,469.6±2.8 JD |
Semi-amplitude | (K) | 2.66±0.16 m/s |
Physical characteristics | ||
Minimum mass | (m sin i) | 0.038 MJ |
Temperature | (T) | ~522 K |
Discovery information | ||
Discovery date | May 18, 2006 | |
Discoverer(s) | Lovis et al. | |
Detection method | Radial velocity | |
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia |
data | |
SIMBAD | data |
HD 69830 c is the 2nd planet orbiting HD 69830. This is likely to be a rocky planet, not a gas giant.[1] If it had formed as a gas giant, it would have stayed that way.[2]
Coordinates: 08h 18m 23.9s, −12° 37′ 55.8″
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