Astronomy:HD 154857 b

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Short description: Extrasolar planet orbiting HD 154857
HD 154857 b
Discovery
Discovered byMcCarthy et al.
AAT
 Australia
Discovery siteAAPS
Discovery date2004
Radial velocity
Orbital characteristics
astron|astron|helion}}1.8 AU (270,000,000 km)
astron|astron|helion}}0.64 AU (96,000,000 km)
1.2 ± 0.2 AU (180,000,000 ± 30,000,000 km)
Eccentricity0.47±0.02
Orbital period409±1 d
1.12 y
astron|astron|helion}}2450346±5
59±4
Semi-amplitude50.4±1
StarHD 154857
Physical characteristics
Mass>1.8±0.4 ||J}}}}}}
(>570±100 M)


HD 154857 b is an extrasolar planet approximately 224 light years away in the constellation of Ara. This is a gas giant mass that orbits the star in an eccentric orbit. This planet was detected by using Anglo-Australian Telescope (AAT) UCLE spectrometer.[1][2]

References

  1. McCarthy, Chris et al. (2004). "Multiple Companions to HD 154857 and HD 160691". The Astrophysical Journal 617 (1): 575–579. doi:10.1086/425214. Bibcode2004ApJ...617..575M. 
  2. O'Toole, Simon J. et al. (2007). "New Planets around Three G Dwarfs". The Astrophysical Journal 660 (2): 1636–1641. doi:10.1086/513563. Bibcode2007ApJ...660.1636O. 

External links

Coordinates: Sky map 17h 11m 15.7219s, −56° 40′ 50.865″