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HD 49674 - Wikipedia, the free encyclopedia

HD 49674

From Wikipedia, the free encyclopedia

HD 49674
Observation data
Epoch 2000
Constellation
(pronunciation)
Auriga
Right ascension 6h 51m 30.52s
Declination +40° 52' 3.92"
Apparent magnitude (V) 8.10
Distance 133.8 ly
(40.73 pc)
Spectral type G5 V
Other designations
BD+41°1544, HIP 32916,
SAO 41390

HD 49674 is an 8th magnitude yellow dwarf star (spectral type G5 V) 133 light years from Earth in the constellation of Auriga. It has a very similar mass to our Sun. It is orbited by a recently discovered planet.


[edit] HD 49674 b

HD 49674 b
Extrasolar planet List of extrasolar planets
Orbital elements
Semimajor axis (a) 0.0580±0.0034 AU
Eccentricity (e) 0.087±0.095
Orbital period (P) 4.94737±0.00098 d
Angular distance (θ) 1.425 mas
Longitude of
periastron
(ω) 264°
Time of periastron (T0) 2,451,882.38±0.88 JD
Semi-amplitude (K) 13.7±0.21 m/s
Physical characteristics
Mass (m) >0.105±0.011 MJ
Discovery information
Discovery date June 13, 2002
Discoverer(s) Butler, Marcy,
Vogt, et al.
Detection method Radial velocity
Discovery site California
Discovery status Published

HD 49674 b is a planet discovered orbiting the star in 2002. At the time of discovery, it was the least massive extrasolar planet known, being less than half the mass of Saturn, but smaller planets were discovered in 2004. The planet is a gas giant and orbits extremely close to its star. Surface temperatures would be very high, and the planet probably has a faint red glow.


[edit] References

[edit] External links


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