HD 50499 b

HD 50499 b
Exoplanet List of exoplanets
Parent star
Star HD 50499
Constellation Puppis
Right ascension (α) 06h 52m 02s
Declination (δ) −33° 54 56
Apparent magnitude (mV) 7.221
Distance154.14 ly
(47.26 pc)
Spectral type G1V
Orbital elements
Semi-major axis(a) 3.84 ± 0.04 AU
Eccentricity (e) 0.25 ± 0.20
Orbital period(P) 2458 ± 38 d
Argument of
periastron
(ω) 259 ± 36°
Time of periastron (T0) 2451220 ± 77 JD
Semi-amplitude (K) 23.0 ± 1.1 m/s
Physical characteristics
Minimum mass(m sin i)1.72 ± 0.03 MJ
Discovery information
Discovery date 5 June 2005
Discoverer(s) Vogt,
Butler,
Marcy, and
Fischer et al.
Discovery method Radial velocity
Discovery site  United States
Discovery status Confirmed
Database references
Extrasolar Planets
Encyclopaedia
data
SIMBADdata
Exoplanet Archivedata
Open Exoplanet Cataloguedata

HD 50499 b is an extrasolar planet approximately 154 light-years away in the constellation of Puppis. The planet is suspected to be a gas giant with mass of 1.7 times Jupiter. It is a long period, taking 351 weeks to orbit the star. The planet’s eccentric orbit passes through the average distance of 574 Gm.

The planet was discovered by four team members including Steve Vogt in 2005 using their radial velocity method, which used to measure changes in red- and blue-shifting of the star that indicate the presence of planets caused by gravitational tug.[1] He also indicated the existence of two additional outer planets.

See also

References

  1. Vogt, Steven S.; et al. (2005). "Five New Multicomponent Planetary Systems". The Astrophysical Journal. 632 (1): 638–658. Bibcode:2005ApJ...632..638V. doi:10.1086/432901.

Coordinates: 06h 52m 02s, −33° 54′ 56″


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