HD 80606 b
|Exoplanet||List of exoplanets|
to scale with Jupiter
|Right ascension||(α)||09h 22m 37.5679s|
|Declination||(δ)||+50° 36′ 13.397″|
|Semimajor axis||(a)||0.453 ± 0.015 AU
|Eccentricity||(e)||0.9336 ± 0.0002|
|Orbital period||(P)||111.436 ± 0.003 d
|Orbital speed||(υ)||31.7[notes 1] km/s|
|Inclination||(i)||89.285 ± 0.023°|
|(ω)||300.4977 ± 0.0045°|
|Time of periastron||(T0)||2,454,424.857 ± 0.05 JD|
|Time of transit||(Tt)||2,454,876.344 ± 0.011 JD|
|Time of eclipse||(Te)||2,454,424.736 ± 0.003 JD|
|Semi-amplitude||(K)||472 ± 5 m/s|
|Mass||(m)||4.0 ± 0.3 MJ|
|Radius||(r)||0.921 ± 0.036 RJ|
|Density||(ρ)||4440 ± 240 kg m−3|
|Surface gravity||(g)||9.6 g|
|Temperature||(T)||at periastron: 1500|
|Discovery date||April 4, 2001|
|Discoverer(s)||Geneva Extrasolar Planet Search|
|Discovery method||Radial velocity|
|Other detection methods||Orbital phase reflected light variations
|Discovery site||Haute-Provence Observatory|
Struve 1341 B b, HIP 45982 b
|Open Exoplanet Catalogue||data|
HD 80606 b (also Struve 1341 B b or HIP 45982 b) is an eccentric Jupiter 190 light-years from the Sun in the constellation of Ursa Major. HD 80606 b was discovered orbiting the star Struve 1341 B in April 2001 by a team led by Michel Mayor and Didier Queloz. With a mass 4 times that of Jupiter, it is a gas giant. Because the planet transits the host star its radius can be determined using the transit method and was found to be slightly smaller than Jupiter's. Its density is slightly less than Earth's.
HD 80606 b has the most eccentric orbit of any known planet after HD 20782 b. Its eccentricity is 0.9336, comparable to Halley's Comet. The eccentricity may be a result of the Kozai mechanism, which would occur if the planet's orbit is significantly inclined to that of the binary stars. This interpretation is supported by measurements of the Rossiter–McLaughlin effect, which indicate that the planet's orbit may be significantly inclined (by approximately 50 degrees) to the rotational axis of the star, a configuration which would be expected if the Kozai mechanism were responsible for the orbit.
As a result of this high eccentricity, the planet's distance from its star varies from 0.03 to 0.88 AU. At apastron it would receive an insolation similar to that of Earth, while at periastron the insolation would be around 800 times greater, far more than that experienced by Mercury in the Solar System. In 2009, the eclipse of HD 80606 b by its parent star was detected, allowing measurements of the planet's temperature to be made as the planet passed through periastron. These measurements indicated that the temperature rose from around 800 K (500 °C / 1000 °F) to 1500 K (1200 °C / 2200 °F) in just 6 hours.
The transit was detected using a Celestron 35-cm Schmidt–Cassegrain telescope. Prior to the large data release of the Kepler Mission in February 2011, HD 80606 b has the longest orbital period of any known transiting planet. It takes 12.1 hours to transit its star.
The transit of 14 January 2010 was partially observed by MOST; but there were equipment failures over part of this time, and the 8 January secondary transit was entirely lost. The midpoint of the next transit is 1 February 2013 11:37 UT.
The planet has wild variations in its weather as it orbits its parent star. Computer models predict the planet heats up 555 °C (1,000 °F) in just a matter of hours triggering "shock wave storms" with winds that move faster than the speed of sound, at 3 miles per second.
- From perimeter of the orbit divided by orbital period.
- Moutou, C.; et al. (April 2009). "Photometric and spectroscopic detection of the primary transit of the 111-day-period planet HD 80606 b". Astronomy and Astrophysics 498 (5): L5–L8. arXiv:0902.4457. Bibcode:2009A&A...498L...5M. doi:10.1051/0004-6361/200911954.
- Fossey, S. J.; Waldman, I. P.; Kipping, D. M. (2009). "Detection of a transit by the planetary companion of HD 80606". Monthly Notices of the Royal Astronomical Society: Letters 396: L16–L20. arXiv:0902.4616. Bibcode:2009MNRAS.396L..16F. doi:10.1111/j.1745-3933.2009.00653.x.
- Laughlin, G.; et al. (2009). "Rapid heating of the atmosphere of an extrasolar planet". Nature 457 (7229): 562–564. Bibcode:2009Natur.457..562L. doi:10.1038/nature07649. PMID 19177124.
- Hidas, M. G.; et al. (2010). "An ingress and a complete transit of HD 80606 b". arXiv:1002.1052 [astro-ph.EP].
- "Exoplanets: The Hunt Continues!" (Press release). Garching, Germany: European Southern Observatory. April 4, 2001. Retrieved December 27, 2012.
- Naef, D.; et al. (2001). "HD 80606 b, a planet on an extremely elongated orbit". Astronomy and Astrophysics 375 (2): L27–L30. arXiv:astro-ph/0106256. Bibcode:2001A&A...375L..27N. doi:10.1051/0004-6361:20010853.
- PONT; et al. "Spin-orbit misalignment in the HD 80606 planetary system". Astronomy & Astrophysics. Retrieved 7 February 2013.
- Robert Massey and Anita Heward (2009-04-21). "RAS PN 09/23 (NAM 10): London students find Jupiter-sized oddball planet". The Royal Astronomical Society. Retrieved 2009-07-15.
- Jessica E. Roberts, Jason W. Barnes, Jason F. Rowe, Jonathan F. Fortney (2012). "MOST Space Telescope Photometry of the 2010 January Transit of Extrasolar Planet HD80606b". arXiv:1212.0285. Bibcode:2013ApJ...762...55R. doi:10.1088/0004-637X/762/1/55.
- HD 80606 Transit Times - Variable Star and Exoplanets
- "Exoplanet Sees Extreme Heat Waves". Space.com. January 28, 2009.
Media related to HD 80606 b at Wikimedia Commons