HAT-P-5

HAT-P-5[1][2]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lyra
Right ascension 18h 17m 37.311s[3]
Declination +36° 37 17.12[3]
Apparent magnitude (V) +11.95
Characteristics
Spectral type G
Variable type planetary transit
Astrometry
Proper motion (μ) RA: 14.0 ± 2.1[3] mas/yr
Dec.: 4.1 ± 0.8[3] mas/yr
Distanceapprox. 1,100 ly
(340 ± 30 pc)
Details
Mass1.16 ± 0.062 M
Radius1.167 ± 0.049 R
Surface gravity (log g)4.37 ± 0.03[4] cgs
Temperature5863 ± 80[4] K
Metallicity [Fe/H]0.10 ± 0.10[4] dex
Rotational velocity (v sin i)2.8 ± 1.0[4] km/s
Age2.6 ± 1.8 Gyr
Other designations
GSC 02634-01087, 2MASS J18173731+3637170, TYC 2634-1087-1
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia
data

HAT-P-5 is a 12th magnitude star in the constellation Lyra, approximately 1,100 light years away from Earth. It is a spectral type G star, about 1.16 solar masses and radii greater than our Sun, and only 200 Kelvins hotter. It is estimated to be 2.6 billion years old.[1][2]

Planetary system

On October 9, 2007, a report was submitted to The Astrophysical Journal Letters telling of the discovery of an exoplanet transiting HAT-P-5. The planet was described as a Jupiter-like hot Jupiter, with a radius about one and one quarter times that of Jupiter, and nearly the same mass. Its density was reported as 0.66 ± 0.11 g/cm3, and its inclination 86.75 ± 0.44°.[5]

The HAT-P-5 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 1.06 ± 0.11 MJ 0.04075 ± 0.00076 2.788491 ± 2.5e-05 0

See also

References

  1. 1.0 1.1 "Notes for Planet HAT-P-5 b". Extrasolar Planets Encyclopaedia. Retrieved October 16, 2007.
  2. 2.0 2.1 "Simbad Query Result". Simbad. Retrieved October 16, 2007.
  3. 3.0 3.1 3.2 3.3 Zacharias, N. et al. (2013). "The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)". The Astronomical Journal 145 (2). 44. arXiv:1212.6182. Bibcode:2013AJ....145...44Z. doi:10.1088/0004-6256/145/2/44.Vizier catalog entry
  4. 4.0 4.1 4.2 4.3 Torres, Guillermo et al. (2012). "Improved Spectroscopic Parameters for Transiting Planet Hosts". The Astrophysical Journal 757 (2). 161. arXiv:1208.1268. Bibcode:2012ApJ...757..161T. doi:10.1088/0004-637X/757/2/161.
  5. Bakos, G. Á. et al. (2007). "HAT-P-5b: A Jupiter-like Hot Jupiter Transiting a Bright Star". The Astrophysical Journal Letters 671 (2): L173–L176. arXiv:0710.1841. Bibcode:2007ApJ...671L.173B. doi:10.1086/525022.

External links

Coordinates: 18h 17m 37.299s, +36° 37′ 16.88″