COROT-Exo-1b

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COROT-Exo-1b
Extrasolar planet List of extrasolar planets
Parent star
Star COROT-Exo-1
Constellation Monoceros
Right ascension (α) 6h 48m 19.17s[1]
Declination (δ) −3° 06′ 07.78″[1]
Distance 1560 ly (480 pc)
Spectral type G0V[1]
Orbital elements
Semimajor axis (a) 0.025 ± 0.001[1][2] AU
Eccentricity (e) 0 (assumed)[1]
Orbital period (P) 1.5089557 ± 0.0000064[1] d
Inclination (i) 85.1 ± 0.5[1]°
Time of transit (Tt) 2454159.4532 ± 0.0001[1] JD
Physical characteristics
Mass (m) 1.03 ± 0.12[1] MJ
Radius (r) 1.49 ± 0.08[1] RJ
Density (ρ) 380 ± 50[1] kg/m3
Surface gravity (g) 11.5[3] m/s²
Temperature (T) 1898 ± 50[1] K
Discovery information
Discovery date 2007-05-01,
announced 2007-05-03
Discoverer(s) COROT mission
Detection method Transit method
Discovery site Earth's orbit
Discovery status Confirmed
Planet Jupiter

COROT-Exo-1b is the first extrasolar planet to be detected by the French-led COROT Mission, in May 2007. It is about 1,560 light years away in the constellation Monoceros and orbits a yellow dwarf star.

The planet, one of the largest ever known is an enormous hot jupiter, about 1.49 times the radius of Jupiter and approximately 1.03 times as massive, based on ground observations of the star. Its huge size is due to its low density combined with the intense heating of its parent star causing the outer layers of the atmosphere to bloat.

COROT-exo-1b orbits its star approximately once every 1.5 days, which would make it an extremely hot planet: the discoverers estimate around 1900 K.

[edit] References

  1. ^ a b c d e f g h i j k l Barge, P.; Baglin, A.; Auvergne, M.; Rauer, H.; Léger, A.; Schneider, J.; Pont, F.; Aigrain, S.; Almenara, J.-M.; Alonso, R.; Barbieri, M.; Bordé, P.; Bouchy, F.; Deeg, H. J.; La Reza, De; Deleuil, M.; Dvorak, R.; Erikson, A.; Fridlund, M.; Gillon, M.; Gondoin, P.; Guillot, T.; Hatzes, A.; Hebrard, G.; Jorda, L.; Kabath, P.; Lammer, H.; Llebaria, A.; Loeillet, B.; Magain, P.; Mazeh, T.; Moutou, C.; Ollivier, M.; Pätzold, M.; Queloz, D.; Rouan, D.; Shporer, A.; Wuchterl, G. (2008). "Transiting exoplanets from the CoRoT space mission. I. CoRoT-Exo-1b: a low-density short-period planet around a G0V star". Astronomy and Astrophysics 482 (3): L17–L20. 
  2. ^ The paper gives the semimajor axis as 4.92 ± 0.08 times the radius of the star, which is estimated at 1.11 ± 0.05 solar radii
  3. ^ Calculated using Newtonian gravity: \textstyle g=\frac{GM}{R^2}

[edit] External links