| 词条 | OGLE-TR-113b |
| 释义 |
| name = OGLE-TR-113b | image = Exoplanet Comparison OGLE-TR-113 b.png | caption = Size comparison of OGLE-TR-113b with Jupiter | discoverer = Konacki et al.[1] | discovery_site = {{flag|Poland}}[1] | discovered = transit found in 2002, proved to be a planet on 14 April 2004[1] | discovery_method = Transit[1] | apsis = astron | semimajor = {{convert|0.0229|±|0.0002|AU|km|abbr=on}} | eccentricity = 0 | period = 1.4324757 ± 0.0000013 d | inclination = 88.8 | star = OGLE-TR-113 | mean_radius = 1.09 ±0.03 {{Jupiter radius|link=y}} | mass = 1.32 ±0.19 {{Jupiter mass|link=y}} }} OGLE-TR-113b is an extrasolar planet orbiting the star OGLE-TR-113. In 2002 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object.[9] 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.[1] The planet has a mass 1.32 times that of Jupiter. Since the planet's inclination is known, the value is exact. It orbits the star (OGLE-TR-113) in an extremely close orbit, even closer than the famous planets 51 Pegasi b and HD 209458 b. The planet races around the star every 1.43 days. The radius of the planet is only 9% larger than Jupiter's, despite the heating effect by the star. Planets of its kind are sometimes called "super-hot Jupiters". See also
References1. ^1 2 3 4 5 {{cite journal | title=The Transiting Extrasolar Giant Planet around the Star OGLE-TR-113 | url=http://iopscience.iop.org/1538-4357/609/1/L37/fulltext/ | last1=Konacki | first1=Maciej | last2=Torres | first2=Guillermo | last3=Sasselov | first3=Dimitar D. | last4=Pietrzynski | first4=Grzegorz | last5=Udalski | first5=Andrzej | last6=Jha | first6=Saurabh | last7=Ruiz | first7=Maria Teresa | last8=Gieren | first8=Wolfgang | last9=Minniti | first9=Dante | display-authors=1 | journal=The Astrophysical Journal Letters | volume=609 | issue=1 | pages=L37–L40 | date=2004 | arxiv=astro-ph/0404541 | bibcode=2004ApJ...609L..37K | doi=10.1086/422600 }} [1][2]2. ^1 {{cite journal| title=The Optical Gravitational Lensing Experiment. Planetary and Low-Luminosity Object Transits in the Carina Fields of the Galactic Disk | url=http://acta.astrouw.edu.pl/Vol52/n4/a_52_4_1.html | last1=Udalski | first1=A. | last2=Szewczyk | first2=O. | last3=Zebrun | first3=K. | last4=Pietrzynski | first4=G. | last5=Szymanski | first5=M. | last6=Kubiak | first6=M. | last7=Soszynski | first7=I. | last8=Wyrzykowski | first8=L. | display-authors=1 | journal=Acta Astronomica | volume=52 | issue=4 | pages=317–359 | date=2002 | arxiv=astro-ph/0301210 | bibcode=2002AcA....52..317U }} }} External links{{commonscat-inline|OGLE-TR-113 b}}
6 : Exoplanets|Hot Jupiters|Transiting exoplanets|Exoplanets discovered in 2002|Giant planets|Carina (constellation) |
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