HD 60532 c
From Infogalactic: the planetary knowledge core
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 60532 | |
Constellation | Puppis | |
Right ascension | (α) | 07h 34m 03.1805s |
Declination | (δ) | –22° 17′ 45.841″ |
Apparent magnitude | (mV) | 4.458 |
Distance | 83.8 ly (25.7 pc) |
|
Spectral type | F6V | |
Orbital elements | ||
Semi-major axis | (a) | 1.58 AU (236 Gm) |
Periastron | (q) | 1.52 AU (227 Gm) |
Apastron | (Q) | 1.64 AU (245 Gm) |
Eccentricity | (e) | 0.038 ± 0.008 |
Orbital period | (P) | 607.06 ± 2.1 d (1.6620 y) |
Inclination | (i) | ~20° |
Argument of periastron |
(ω) | 119.49 ± 9.14° |
Time of periastron | (T0) | 2454000 JD |
Physical characteristics | ||
Mass | (m) | 7.46 MJ |
Discovery information | ||
Discovery date | September 22, 2008 | |
Discoverer(s) | Desort et al. | |
Discovery method | Doppler spectroscopy | |
Discovery site | La Silla Observatory | |
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia |
data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 60532 c is an extrasolar planet located approximately 84 light-years away in the constellation of Puppis, orbiting the star HD 60532. This planet has a true mass of 7.46 times more than Jupiter which orbits at 1.58 AU and takes 607 days to revolve in an eccentric orbit. This planet was discovered on September 22, 2008 in La Silla Observatory using the HARPS spectrograph. On this same day, the second planet in this system, HD 60532 b, was discovered in a 3:1 orbital resonance.
References
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External links
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Coordinates: 07h 34m 03.1805s, −22° 17′ 45.841″
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