astro.wikisort.org - Meteorite

Search / Calendar

OGLE-TR-56b is an extrasolar planet located approximately 1500 parsecs away in the constellation of Sagittarius, orbiting the star OGLE-TR-56. This planet was the first known exoplanet to be discovered with the transit method. The object was discovered by the OGLE project, announced on July 5, 2002[2] and confirmed on January 4, 2003 by the Doppler technique.[3] The period of this confirmed planet was the shortest until the confirmed discovery of WASP-12b on April 1, 2008.[4] The short period and proximity of the OGLE-TR-56 b to its host mean it belongs to a class of objects known as hot Jupiters.

OGLE-TR-56b
Size comparison of OGLE-TR-56b with Jupiter.
Discovery
Discovered byKonacki et al.[1]
Discovery date3 November 2002
confirmed: 4 January 2003
Detection method
Transit
Orbital characteristics
Apastron0.0225 AU (3,370,000 km)
Periastron0.0225 AU (3,370,000 km)
Semi-major axis
0.0225 ± 0.0004 AU (3,366,000 ± 60,000 km)
Eccentricity0
Orbital period (sidereal)
1.211909 ± 0.000001 d
29.08582 h
Average orbital speed
203
Inclination78.8 ± 0.5
StarOGLE-TR-56
Physical characteristics
Mean radius
1.30 ± 0.05 RJ
Mass1.29 ± 0.12 MJ
Mean density
779 kg/m3 (1,313 lb/cu yd)
Surface gravity
19.8 m/s2 (65 ft/s2)
2.02 g
Temperature~1973


    The radial velocity trend of OGLE-TR-56, caused by the presence of OGLE-TR-56 b.
    The radial velocity trend of OGLE-TR-56, caused by the presence of OGLE-TR-56 b.

    The planet is thought to be only 4 stellar radii from its star, and hot enough to have iron rain.[5]


    See also



    References


    1. Konacki, Maciej; et al. (2003). "An extrasolar planet that transits the disk of its parent star" (PDF). Nature. 421 (6922): 507–509. Bibcode:2003Natur.421..507K. doi:10.1038/nature01379. PMID 12556885.
    2. Udalski, A.; et al. (2002). "The Optical Gravitational Lensing Experiment. Search for Planetary and Low-Luminosity Object Transits in the Galactic Disk. Results of 2001 Campaign - Supplement". Acta Astronomica. 52 (2): 115–128. arXiv:astro-ph/0207133. Bibcode:2002AcA....52..115U.
    3. Konacki, Maciej; et al. (2003). "High-Resolution Spectroscopic Follow-up of OGLE Planetary Transit Candidates in the Galactic Bulge: Two Possible Jupiter-Mass Planets and Two Blends". The Astrophysical Journal. 597 (2): 1076–1091. arXiv:astro-ph/0306542. Bibcode:2003ApJ...597.1076K. doi:10.1086/378561.
    4. Hebb, L.; et al. (2009). "WASP-12b: THE HOTTEST TRANSITING EXTRASOLAR PLANET YET DISCOVERED". The Astrophysical Journal. 693 (2): 1920–1928. arXiv:0812.3240. Bibcode:2009ApJ...693.1920H. doi:10.1088/0004-637X/693/2/1920.
    5. Harvard University and Smithsonian Institution (2003-01-08). "New World of Iron Rain". Astrobiology Magazine. Archived from the original on 2010-01-10. Retrieved 2010-01-25.


    Media related to OGLE-TR-56 b at Wikimedia Commons


    This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it.

    • v
    • t
    • e

    На других языках

    - [en] OGLE-TR-56b

    [es] OGLE-TR-56b

    OGLE-TR-56b es un planeta extrasolar, que se encuentra a unos 5 000 años luz de distancia, en la constelación de Sagitario, orbitando la estrella OGLE-TR-56. Fue descubierto en 2002 por el proyecto OGLE,[1] usando el método de tránsito astronómico, y confirmado en 2003 por la técnica de espectroscopia de efecto Doppler.[2]

    [ru] OGLE-TR-56 b

    OGLE-TR-56b — экзопланета класса «горячий юпитер», вращающаяся вокруг жёлтого карлика OGLE-TR-56.


    Текст в блоке "Читать" взят с сайта "Википедия" и доступен по лицензии Creative Commons Attribution-ShareAlike; в отдельных случаях могут действовать дополнительные условия.

    Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.

    2019-2025
    WikiSort.org - проект по пересортировке и дополнению контента Википедии