*** Welcome to piglix ***

51 Pegasi b

51 Pegasi b
Exoplanet List of exoplanets
Artist impression of the exoplanet 51 Pegasi b.jpg
An artist's impression of 51 Pegasi b (center) and its star (right).
Parent star
Star 51 Pegasi
Constellation Pegasus
Right ascension (α) 22h 57m 28.0s
Declination (δ) +20° 46′ 08″
Apparent magnitude (mV) 5.49
Distance 50.9 ± 0.3 ly
(15.61 ± 0.09 pc)
Spectral type G2.5IVa or G4-5Va
Mass (m) 1.06 M
Radius (r) 1.237 ± 0.047 R
Temperature (T) 5571 ± 102 K
Metallicity [Fe/H] 0.20 ± 0.07
Age 6.1-8.1 Gyr
Orbital elements
Semi-major axis (a) 0.0527 ± 0.0030 AU
(7.89 Gm)
Periastron (q) 0.0520 AU
(7.79 Gm)
Apastron (Q) 0.0534 AU
(7.99 Gm)
Eccentricity (e) 0.013 ± 0.012
Orbital period (P) 4.230785 ± 0.000036 d
    (101.5388 h)
Orbital speed (υ) 136 km/s
Argument of
periastron
(ω) 58°
Time of periastron (T0) 2,450,001.51 ± 0.61 JD
Semi-amplitude (K) 55.94 ± 0.69 m/s
Physical characteristics
Minimum mass (m sin i) 0.472 ± 0.039 MJ
Stellar flux (F) 480
Rotation period (ω) Synchronous
Temperature (T) 1284 ± 19
Discovery information
Discovery date 6 October 1995
Discoverer(s) Michel Mayor and
Didier Queloz
Discovery method Radial velocity (ELODIE)
Discovery site OHP, France
Discovery status Published
Other designations
Dimidium, Bellerophon
Database references
Extrasolar Planets
Encyclopaedia
data
SIMBAD data
Exoplanet Archive data
Open Exoplanet Catalogue data

51 Pegasi b (abbreviated 51 Peg b), unofficially dubbed Bellerophon, later named Dimidium, is an extrasolar planet approximately 50 light-years away in the constellation of Pegasus. It was the first exoplanet to be discovered orbiting a main-sequence star, the Sun-like 51 Pegasi, and marked a breakthrough in astronomical research. It is the prototype for a class of planets called hot Jupiters.

51 Pegasi is the Flamsteed designation of the host star. The planet was originally designated 51 Pegasi b by Michel Mayor and Didier Queloz, who discovered the planet. The following year it was unofficially dubbed Bellerophon by astronomer Geoffrey Marcy, who followed the convention of naming planets after Greek and Roman mythological figures (Bellerophon was a figure from Greek mythology who rode the winged horse Pegasus).

In July 2014, the International Astronomical Union launched a process for giving proper names to certain exoplanets and their host stars. The process involved public nomination and voting for the new names. In December 2015, the IAU announced the winning name for this planet was Dimidium. The name was submitted by the Astronomische Gesellschaft Luzern (German for Astronomical Society of Lucerne), Switzerland. 'Dimidium' is Latin for 'half', referring to the planet's mass of at least half the mass of Jupiter.


...
Wikipedia

...