HD 73526 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 73526 | |
Constellation | Vela | |
Right ascension | (α) | 08h 37m 16.4839s |
Declination | (δ) | −41° 19′ 08.767″ |
Apparent magnitude | (mV) | 9 |
Distance | 322.9 ly (99.0 pc) | |
Spectral type | G6V | |
Mass | (m) | 1.02 M☉ |
Radius | (r) | 1.49 R☉ |
Temperature | (T) | 5470 K |
Metallicity | [Fe/H] | 0.28 |
Age | 5.59 Gyr | |
Orbital elements | ||
Semi-major axis | (a) | 0.66±0.05 AU |
Eccentricity | (e) | 0.39±0.05 |
Orbital period | (P) | 187.5±0.3 d |
Argument of periastron |
(ω) | 172±11° |
Time of periastron | (T0) | 2,450,037±15 JD |
Semi-amplitude | (K) | 76.1±5.1 m/s |
Physical characteristics | ||
Minimum mass | (m sin i) | 2.07±0.16 MJ |
Discovery information | ||
Discovery date | Jun 13, 2002 | |
Discoverer(s) | Tinney et al. | |
Discovery method | Radial velocity | |
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 73526 b is an extrasolar planet orbiting about 61 million miles (0.66 AU) away from its parent star.[1] This planet is more massive than Jupiter in the Solar System, so is most likely a gas giant. Based on its orbit and the stellar luminosity, the planet probably receives insolation 61% that of Mercury.
See also
References
- ↑ Tinney, C. G.; et al. (2003). "Four New Planets Orbiting Metal-enriched Stars". The Astrophysical Journal 587 (1): 423–428. arXiv:astro-ph/0207128. Bibcode:2003ApJ...587..423T. doi:10.1086/368068.
External links
Coordinates: 08h 37m 16.4839s, −41° 19′ 08.767″
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