Extrasolar planet | List of extrasolar planets | |
---|---|---|
Parent star | ||
Star | HD 73256 | |
Constellation | Pyxis | |
Right ascension | (α) | 08h 36m 23.0155s |
Declination | (δ) | −30° 02′ 15.456″ |
Distance | 119 ly (36.5 pc) |
|
Spectral type | G9V | |
Orbital elements | ||
Semimajor axis | (a) | 0.037 AU |
Periastron | (q) | 0.036 AU |
Apastron | (Q) | 0.038 AU |
Eccentricity | (e) | 0.029±0.02 |
Orbital period | (P) | 2.54858±0.00016 d |
Orbital speed | (υ) | 160 km/s |
Argument of periastron |
(ω) | 337±46° |
Time of periastron | (T0) | 2452500.18±0.28 JD |
Semi-amplitude | (K) | 269±8 m/s |
Physical characteristics | ||
Minimum mass | (m sin i) | 1.87 MJ |
Discovery information | ||
Discovery date | 2003 | |
Discoverer(s) | Udry et al. | |
Detection method | Doppler spectroscopy (CORALIE) |
|
Discovery site | La Silla Observatory, Chile | |
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia |
data | |
SIMBAD | data |
HD 73256 b is an 1.87 MJ hot Jupiter orbiting at 0.037 AU taking 2.55 days to orbit around HD 73256.
Assuming the planet is perfectly grey with no greenhouse or tidal effects, and a Bond albedo of 0.1, the temperature would be about 1300 K. This is close to 51 Pegasi b; between the predicted temperatures of HD 189733 b and HD 209458 b (1180-1392K), before they were measured. It is a candidate for "near-infrared characterisation with the VLTI Spectro-Imager".[1]