astro.wikisort.org - Meteorite
SWEEPS-04 is an extrasolar planet orbiting the star SWEEPS J175853.92−291120.6 in the constellation Sagittarius approximately 27,710 light years away (based on a distance modulus of 14.1) from the Solar System, making it (along with SWEEPS-11) the most distant exoplanet(s) known.[2] This planet was found in 2006 by the Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS) program that uses the transit method.
 Size comparison of SWEEPS-04 with Jupiter. | |
| Discovery | |
|---|---|
| Discovered by | Sahu et al.[1] |
| Discovery date | October 4, 2006 |
Detection method | Transit |
| Orbital characteristics | |
Semi-major axis | 0.055 AU (8,200,000 km) |
Orbital period (sidereal) | 4.2 d |
| Inclination | >87 |
| Star | SWEEPS J175853.92−291120.6 |
| Physical characteristics | |
Mean radius | 0.81±0.1 RJ |
| Mass | <3.8 MJ |
The upper limit on the planet's mass is 3.8 times the mass of Jupiter. The best fit radius is 0.81 times that of Jupiter, but the uncertainty in this value is large, around 12%. It orbits at an average distance of 8,200,000 km (0.055 AU) from the parent star, taking 4.2 days to revolve around it.
HST SWEEPS-4 2006
Radial Velocities of SWEEPS-04 (UVES-VLT)
Artist's impression of a transiting Jupiter-mass exoplanet SWEEPS J175853.92-291120.6 b
See also
- Sagittarius Window Eclipsing Extrasolar Planet Search or SWEEPS
- SWEEPS-10
- SWEEPS-11
- List of extrasolar planets
References
- Sahu, Kailash C.; Casertano, S; Bond, HE; Valenti, J; Smith, TE; Minniti, D; Zoccali, M; Livio, M; et al. (2006). "Transiting extrasolar planetary candidates in the Galactic bulge". Nature. 443 (7111): 534–540. arXiv:astro-ph/0610098. Bibcode:2006Natur.443..534S. doi:10.1038/nature05158. PMID 17024085. (web Preprint)
- "HEC: Top 10 Exoplanets - Planetary Habitability Laboratory @ UPR Arecibo". phl.upr.edu. Retrieved 16 July 2018.
External links
- "SWEEPS-04". Exoplanets. Retrieved 2009-05-22.
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На других языках
[de] SWEEPS-04 b
SWEEPS-04 ist ein Exoplanet, der den Unterriesen SWEEPS-04 (SWEEPS J175853.92-291120.6) alle 4,2 Tage umkreist. Auf Grund seiner hohen Masse wird angenommen, dass es sich um einen Gasplaneten handelt. Er wurde im Jahr 2006 mit Hilfe der Transitmethode vom Sagittarius-Window-Eclipsing-Extrasolar-Planet-Search-Projekt entdeckt.- [en] SWEEPS-04
[ru] SWEEPS-04
SWEEPS-04 — газовый гигант, обращающийся вокруг звезды SWEEPS J175853.92-291120.6. Она расположена в созвездии Стрелец на расстоянии около 27,7 тысяч световых лет от Солнца и является одной из самых удалённых экзопланет, известных науке[2].Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
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