HD 136118

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HD 136118
Observation data
Epoch J2000.0
Constellation
(pronunciation)
Serpens
Right ascension 15h 18m 55.5s
Declination -1º 35' 32.6
Apparent magnitude (V) +6.94
Distance 171 ly
(52.3 pc)
Spectral type F9V
Other designations
BD-01° 3045, GC 20583, HIP 74948, SAO 140452.

HD 136118 is a star located in the constellation Serpens Cauda. It is an F-type dwarf and magnitude 7. The distance from Earth is 52.3 parsecs.

The astronomer Debra Fischer discovers a very massive planet, which was announced to other astronomers on February 7, 2002.

[edit] HD 136118 b

HD 136118 b
Extrasolar planet List of extrasolar planets
Orbital elements
Semimajor axis (a) 2.3 AU
Eccentricity (e) 0.37 ± 0.025
Orbital period (P) 1209 ± 24 d
Angular distance (θ) 44 mas
Longitude of
periastron
(ω) 315 ± 4.5°
Time of periastron (T0) 2451800.6 ± 36.6 JD
Semi-amplitude (K) 212.8 ± 5.8 m/s
Physical characteristics
Mass (m) >11.9 MJ
Discovery information
Discovery date February 7, 2002
Discoverer(s) Fischer et al.
Detection method Doppler Spectroscopy
Discovery status Published

HD 136118 b is a massive extrasolar planet, having mass of 11.9 times that of Jupiter. The lower limit on its mass is only slightly less than the deuterium-burning threshold that some astronomers use to distinguish between planets and brown dwarfs. Depending on the inclination of its orbit, the true mass could be above this limit.

The orbit of the planet is located at the average distance of 2.3 astronomical units from the parent star, taking 40 months to complete one eccentric orbit.

Due to its high mass the planet is likely to be very hot and possibly glowing faintly.

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