HAT-P-5

From Wikipedia, the free encyclopedia

HAT-P-5[1][2]
Observation data
Epoch J2000.0
Constellation
(pronunciation)
Lyra
Right ascension 18h 17m 37.299s
Declination +36° 37′ 16.88″
Apparent magnitude (V) +11.95
Astrometry
Proper motion (μ) RA: 2.6 mas/yr
Dec.: -2.5 mas/yr
Distance approx. 1,100 ly (340 ± 30 pc)
Details
Mass 1.16 ± 0.062 M
Radius 1.167 ± 0.049 R
Temperature 5960 ± 100 K
Metallicity 0.24 ± 0.15
Age 2.6 ± 1.8 Giga years
Other designations
GSC 02634-01087, 2MASS J18173731+3637170, HAT-P-5, TYC 2634-1087-1

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, only about 0.16 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]

[edit] 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°.[3]

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

[edit] References

  1. ^ a b Notes for Planet HAT-P-5 b. Extrasolar Planets Encyclopaedia. Retrieved on October 16, 2007.
  2. ^ a b Simbad Query Result. Simbad. Retrieved on October 16, 2007.
  3. ^ HAT-P-5b: A Jupiter-like hot Jupiter Transiting a Bright Star. fr.arxiv.org. Retrieved on October 16, 2007.

[edit] External links


Languages