HD 168746

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HD 168746
Observation data
Epoch 2000
Constellation
(pronunciation)
Serpens
Right ascension 18h 21m 49.78s
Declination -11° 55' 21.66"
Apparent magnitude (V) 7.95
Distance 140.6 ly
(43.12 pc)
Spectral type G5
Other designations
BD-11°4606, HIP 90004

HD 168746 is an 8th magnitude star in the constellation of Serpens. It is very similar to our Sun, a yellow dwarf star (spectral class G5 V). It is not visible to the unaided eye, but is easily visible with binoculars or a small telescope. In 2000 a planet was announced orbiting it.


[edit] HD 168746 b

HD 168746 b
Orbital elements
Semi-major axis a: 0.065 AU
Eccentricity e: 0.081 ± 0.029
Orbital period P: 6.403 ± 0.001 d
Inclination i:  ?°
Angular distance θ: 2 mas
Longitude of
periastron ω:
16.30 ± 20.88°
Time of periastron τ: 2,451,994.7 ± 0.4 JD
Semi-amplitude K: 28.6 ± 1.7 m/s
Physical characteristics
Mass: >0.23 MJ
Radius:  ? RJ
Density:  ? kg/
Gravity:  ? g
Temperature:  ? K
Discovery
Discovery date: 2000
Discovery site:
Detection method(s): CORALIE
Discoverer(s): Pepe, Mayor,
Galland et al.
Other catalogue


HD 168746 b is an extrasolar planet orbiting the star. It has a minimum mass about one fourth that of Jupiter, so it is most likely a low mass gas giant. It orbits very near the star in a so-called "torch orbit" completing one revolution in only about six and half days.


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[edit] External links