HD 88133

HD 88133
Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 10h 10m 07.68s
Declination +18° 11′ 12.74″
Apparent magnitude (V) 8.06
Distance 242.7 ly
(74.46 pc)
Spectral type G5IV
Other designations
BD+18°2326, GC 13963, HIP 49813, LTT 12725, NLTT 23562, SAO 98978
Database references
SIMBAD data
ARICNS data
Extrasolar Planets
Encyclopaedia
data

HD 88133 is an 8th magnitude star in the constellation of Leo. It is classified as a yellow subgiant star (spectral type G5IV). It is slightly more massive than our Sun, cooler and more luminous. As a subgiant, it has left the main sequence and started to evolve towards red gianthood. Located at a distance of 240 light years from Earth it is not in our immediate neighbourhood and thus not visible to the unaided eye. With a small telescope it should be easily visible.

In 2004 a planet was found to orbit the star.[1]

The HD 88133 system[2]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity
b >0.229 ± 0.033 MJ 0.0472 ± 0.0027 3.41587 ± 0.00059 0.133 ± 0.072

See also

References

  1. ^ Fischer et al.; Laughlin, Greg; Butler, Paul; Marcy, Geoff; Johnson, John; Henry, Greg; Valenti, Jeff; Vogt, Steve et al. (2005). "The N2K Consortium. I. A Hot Saturn Planet Orbiting HD 88133". The Astrophysical Journal 620 (1): 481–486. Bibcode 2005ApJ...620..481F. doi:10.1086/426810. http://www.iop.org/EJ/article/0004-637X/620/1/481/61277.html. 
  2. ^ Butler et al.; Wright, J. T.; Marcy, G. W.; Fischer, D. A.; Vogt, S. S.; Tinney, C. G.; Jones, H. R. A.; Carter, B. D. et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646 (1): 505–522. arXiv:astro-ph/0607493. Bibcode 2006ApJ...646..505B. doi:10.1086/504701. http://www.iop.org/EJ/article/0004-637X/646/1/505/64046.html. 

External links

Coordinates: 10h 10m 07.68s, +18° 11′ 12.74″