HD 208487 b

HD 208487 b
Exoplanet List of exoplanets
Parent star
Star HD 208487
Constellation Grus
Right ascension (α) 21h 57m 19.8477s
Declination (δ) −37° 45 49.037
Distance144.4 ly
(44.30 pc)
Spectral type G2V:
Orbital elements
Semi-major axis(a) 0.524 ± 0.030[1] AU
Eccentricity (e) 0.24 ± 0.16[1]
Orbital period(P) 130.08 ± 0.51[1] d
Argument of
periastron
(ω) 113[1]°
Time of periastron (T0) 2,450,999 ± 15[1] JD
Semi-amplitude (K) 19.7 ± 3.6[1] m/s
Physical characteristics
Minimum mass(m sin i)0.520 ± 0.082[1] MJ
Discovery information
Discovery date September 16, 2004
Discoverer(s) Tinney, Butler,
Marcy et al.[2]
Discovery method Doppler spectroscopy
Discovery site  United States
Discovery status Published[2]
Database references
Extrasolar Planets
Encyclopaedia
data
SIMBADdata
Exoplanet Archivedata
Open Exoplanet Cataloguedata

HD 208487 b is an extrasolar planet located approximately 144 light-years away in the constellation of Grus, orbiting the star HD 208487. This planet has a minimum mass close to half that of Jupiter and is most probably a gas giant. The planet orbits the star in a close, eccentric orbit. One revolution takes 130 days to complete. This planet was discovered on September 16, 2004 by Tinney, Butler, and Marcy et al. using Doppler spectroscopy to measure the star's radial velocity changing over time as the planet revolves around its orbit.[2]

References

  1. 1 2 3 4 5 6 7 Butler, R. P.; et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal. 646 (1): 505–522. arXiv:astro-ph/0607493Freely accessible. Bibcode:2006ApJ...646..505B. doi:10.1086/504701.
  2. 1 2 3 Tinney, C. G.; et al. (2005). "Three Low-Mass Planets from the Anglo-Australian Planet Search". The Astrophysical Journal. 623 (2): 1171–1179. Bibcode:2005ApJ...623.1171T. doi:10.1086/428661.

External links

Coordinates: 21h 57m 19.8477s, −37° 45′ 49.037″


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