OGLE-TR-113

OGLE-TR-113
OGLE-TR-113
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Carina
Right ascension 10h 52m 24.40s [1]
Declination –61° 26′ 48.5″ [1]
Apparent magnitude (V) 16.08[1]
Characteristics
Spectral type K
Apparent magnitude (V) ~16.08[1]
Apparent magnitude (I) ~14.42[1]
Apparent magnitude (K) 13.0 ±0.1[1]
Variable type SB*[1]
Astrometry
Distance 1800 ± 100 ly
(550 ± 30 [2] pc)
Absolute magnitude (MV) 15.55
Details
Mass 0.78 (± 0.02) M
Radius 0.77 (± 0.02) R
Metallicity 0.15 (± 0.10) [3]
Age > 0.7 billion years
Other designations
SBC9 2451
Database references
SIMBAD data
Extrasolar Planets
Encyclopaedia
data

OGLE-TR-113 is a dim, distant magnitude 16 binary star in the star fields of the constellation Carina. Because of its distance of about 1800 light years,[2] and location in a crowded field it was not notable in any way. Spectral type of the star is type K dwarf star, slightly cooler and less luminous than the Sun.[1]

Contents

Planetary system

However, in 2002 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object.[4] Since low-mass red dwarfs and brown dwarfs may mimic a planet radial velocity measurements were necessary to calculate the mass of the body. In 2004 the object was proved to be a new transiting extrasolar planet, OGLE-TR-113b.[5]

The OGLE-TR-113 system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity
b 1.32 ± 0.19 MJ 0.0229 ± 0.0002 1.4324757 ± 0.0000013 0

See also

References

  1. ^ a b c d e f g h "SIMBAD query result: SBC9 2451 -- Spectroscopic binary". Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=OGLE-TR+113. Retrieved 2009-04-30. 
  2. ^ a b Díaz et al.; Ramirez, Sebastian; Fernandez, Jose Miguel; Gallardo, Jose; Gieren, Wolfgang; Ivanov, Valentin D.; Mauas, Pablo; Minniti, Dante et al. (2007). "Millimagnitude Photometry for Transiting Extrasolar Planetary Candidates. II. Transits of OGLE-TR-113-b in the Optical and Near-IR". The Astrophysical Journal 660 (1): 850–857. arXiv:astro-ph/0701345. Bibcode 2007ApJ...660..850D. doi:10.1086/512721. http://www.iop.org/EJ/article/0004-637X/660/1/850/70886.html. 
  3. ^ Santos et al.; Ecuvillon, A.; Israelian, G.; Mayor, M.; Melo, C.; Queloz, D.; Udry, S.; Ribeiro, J. P. et al. (2006). "Chemical abundances for the transiting planet host stars OGLE-TR-10, 56, 111, 113, 132, and TrES-1". Astronomy and Astrophysics 458 (3): 997–1005. arXiv:astro-ph/0606758. Bibcode 2006A&A...458..997S. doi:10.1051/0004-6361:20065683. http://www.aanda.org/articles/aa/abs/2006/42/aa5683-06/aa5683-06.html. (web Preprint)
  4. ^ Udalski et al.; Szewczyk, O.; Zebrun, K.; Pietrzynski, G.; Szymanski, M.; Kubiak, M.; Soszynski, I.; Wyrzykowski, L. (2002). "The Optical Gravitational Lensing Experiment. Planetary and Low-Luminosity Object Transits in the Carina Fields of the Galactic Disk". Acta Astronomica 52: 317–359. arXiv:astro-ph/0301210. Bibcode 2002AcA....52..317U. (web Preprint)
  5. ^ Bouchy et al.; Pont, F.; Santos, N. C.; Melo, C.; Mayor, M.; Queloz, D.; Udry, S. (2004). "Two new "very hot Jupiters" among the OGLE transiting candidates". Astronomy and Astrophysics 421: L13–L16. arXiv:astro-ph/0404264. Bibcode 2004A&A...421L..13B. doi:10.1051/0004-6361:20040170. http://cds.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aa/abs/2004/25/aagd142/aagd142.html. (web Preprint)

External links

Coordinates: Sky map 10h 52m 24.40s, −61° 26′ 48.5″



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  • OGLE-TR-113 b — ist ein Exoplanet, der den Hauptreihenstern OGLE TR 113 alle 1,432 Tage umkreist. Auf Grund seiner hohen Masse wird angenommen, dass es sich um einen Gasplaneten handelt. Inhaltsverzeichnis 1 Entdeckung 2 Umlauf und Masse 3 …   Deutsch Wikipedia

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  • OGLE-TR-113b — Comparación del tamaño de OGLE TR 113b con Júpiter. Descubrimiento Descubridor Bouchy et al …   Wikipedia Español

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  • OGLE — El Experimento de lente óptica gravitacional, u OGLE, por su sigla en inglés (Optical Gravitational Lensing Experiment) es un proyecto astronómico polaco, iniciado en la Universidad de Varsovia, que está dedicado principalmente al descubrimiento… …   Wikipedia Español

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