- OGLE2-TR-L9b
-
OGLE2-TR-L9b Extrasolar planet List of extrasolar planets
Size comparison of OGLE2-TR-L9b with Jupiter. Parent star Star OGLE2-TR-L9 Constellation Carina Right ascension (α) 11h 07m 55s Declination (δ) –61° 08′ 46″ Distance 2935 ly
(900 pc)Spectral type F3 Orbital elements Orbital period (P) 2.4855335 ± 0.0000007 d (59.6528 h) Time of transit (Tt) 2,454,492.79765 JD Physical characteristics Mass (m) 4.5 ± 1.5 MJ Radius (r) 1.61 ± 0.04 RJ Discovery information Discovery date December 2, 2008 Discoverer(s) Meta de Hoon
Remco van der Burg
Francis VuijsjeDetection method Tansit Discovery status Published Database references Extrasolar Planets
Encyclopaediadata SIMBAD data OGLE2-TR-L9b is an extrasolar planet discovered by three undergraduate students from Leiden University, Netherlands. The planet is about 4.5 times as massive as Jupiter and is the first discovered planet orbiting a fast rotating hot star.[1]
Initially discovered while testing a method for investigating light fluctuations in the OGLE database, the planet's existence was later confirmed by follow up observations from the ESO's Very Large Telescope in Chile.[1]
See also
References
- ^ a b Snellen et al.; Koppenhoefer, J.; Van Der Burg, R. F. J.; Dreizler, S.; Greiner, J.; De Hoon, M. D. J.; Husser, T. O.; Krühler, T. et al. (2009). "OGLE2-TR-L9b: an exoplanet transiting a rapidly rotating F3 star". Astronomy and Astrophysics 497: 545–550. Bibcode 2009A&A...497..545S. doi:10.1051/0004-6361/200810917. http://www.aanda.org/index.php?option=article&access=doi&doi=10.1051/0004-6361:20078949.
External links
Media related to OGLE2-TR-L9 b at Wikimedia Commons
- "OGLE2-TR-L9". Exoplanets. http://media4.obspm.fr/exoplanets/base/etoile.php?nom=OGLE2-TR-L9.
- ESO 45/08 Science Release from the European Southern Observatory
- "Students find planet outside our solar system". MSNBC. 2008-12-04. http://www.msnbc.msn.com/id/28058012/. Retrieved 2008-12-04.
Coordinates: 11h 07m 55s, −61° 08′ 46″
This extrasolar planet related article is a stub. You can help Wikipedia by expanding it.