CoRoT-9b
Discovery
CoRoT-9b was discovered by combining observations from the CoRoT satellite, which looks for a small dip in starlight as a planet passes in front of its parent star, and radial velocity measurements from the European Southern Observatory's High Accuracy Radial velocity Planet Searcher (HARPS) instrument on the 3.6 m Telescope. Its presence was confirmed by observations from several telescopes from the ESO. This discovery was announced in 2010 on St. Patrick's Day, after 145 days of continuous observations in summer 2008.
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Artist's impression of the transiting exoplanet CoRoT-9b. Credit: ESO/L. Calçada.
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Animation of an artist's impression.
Mass and size
CoRoT-9b has a mass of 0.84 times that of Jupiter (MJ) as determined from HARPS spectroscopy, and has a radius of 1.05 times that of Jupiter (RJ) as determined from photometry of the transit light curve. This implies that this planet has a density of 96% that of water, and surface gravity 1.93 times that of Earth. A search for rings and satellites around this planet with the Spitzer space telescope was negative.
Atmosphere and interior
Since CoRoT-9b is the first temperate giant exoplanet found by the transit method, astronomers will be able to study the atmosphere of a temperate giant planet for the first time, examining the composition of clouds, the composition of the atmosphere, temperature distributions, and even some details of the interior of the planet. The atmosphere of this planet is presumably dominated by hydrogen and helium (like Jupiter and Saturn), with up to 20 Earth masses of other elements including water, as well as rock at high temperatures and pressures. The authors of the CoRoT-9b discovery paper refer to the planet as a class II ("water cloud") or class III ("clear") atmosphere planet, as described by the Sudarsky extrasolar planet classification.
See also
- CoRoT is a CNES space mission to discover planets using the photometric transit method. It is in polar orbit around the Earth.
- CoRoT-7b is a rocky super-Earth.
- HD 80606 b is the longest period (but much more eccentric than CoRoT-9b) transiting planet.
- GJ 1214 b is a transiting super-Earth found by MEarth Project.
References
- ^ Deeg, H. J; et al. (2010). "A transiting giant planet with a temperature between 250 K and 430 K". Nature. 464 (7287): 384–387. Bibcode:2010Natur.464..384D. doi:10.1038/nature08856. hdl:2268/76653. PMID 20237564. S2CID 4307611.
- ^ New exoplanet like 'one of ours' (BBC, March 17, 2010)
- ^ "First temperate exoplanet sized up". 2010-03-17. Retrieved 2010-03-18.
- ^ Lecavelier Des Etangs, A.; et al. (2017). "Search for rings and satellites around the exoplanet CoRoT-9b using Spitzer photometry". Astronomy and Astrophysics. 603. A115. arXiv:1705.01836. Bibcode:2017A&A...603A.115L. doi:10.1051/0004-6361/201730554. S2CID 119041929.
External links
Media related to CoRoT-9 b at Wikimedia Commons
- "Cool Jupiter exoplanet found". University of Oxford. March 18, 2010. Archived from the original on 2010-03-24. Retrieved 2010-03-18.
- "CoRoT-9b, a temperate exoplanet" - DLR Portal, 2010.march.17