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WASP-19b
Exoplanet List of exoplanets

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Parent star

under construction


WASP-19b is an extrasolar planet, notable for possessing one of the shortest orbital periods of any known planetary body: Template:Val days or approximately 18.932 hours. It has a mass close to that of Jupiter (1.15 Jupiter masses), but by comparison has a much larger radius (1.31 times that of Jupiter, or 0.13 Solar radii); making it nearly the size of a low-mass star.[1] It orbits the star WASP-19 in the Vela constellation. It is currently the shortest period hot Jupiter discovered as planets with shorter orbital periods have a rocky, metallic or degenerate matter composition.

In 2013, secondary eclipse and orbital phases were barely observed from the data gathered with ASTEP telescope, making it the first detection of such kind through ground-based observations. This was possible due to large size of the planet and its small semi-major axis.[2]

AtmosphereEdit

In December 2013, scientists working with the Hubble Space Telescope reported detecting water in the atmosphere of the exoplanet.[3][4]

In September 2017, astronomers using the Very Large Telescope at the European Southern Observatory reported the detection of titanium oxide (TiO) in WASP-19b's atmosphere.[5] This was the first time titanium oxide had been detected in an exoplanet atmosphere.[6] They also detected a strongly scattering haze in the atmosphere as well as the element sodium, and additionally confirmed the presence of water.[5]

ReferencesEdit

  1. Hebb, L.; Collier Cameron, A.; Triaud, A. H. M. J.; Lister, T. A.; Smalley, B.; Maxted, P. F. L.; Hellier, C.; Anderson, D. R.; et al. (2010). "WASP-19b: The Shortest Period Transiting Exoplanet Yet Discovered". The Astrophysical Journal 708 (1): 224–231. doi:10.1088/0004-637X/708/1/224. Bibcode2010ApJ...708..224H. http://iopscience.iop.org/article/10.1088/0004-637X/708/1/224. 
  2. Cite error: Invalid <ref> tag; no text was provided for refs named arxiv.org
  3. Staff (3 December 2013). "Hubble Traces Subtle Signals of Water on Hazy Worlds". NASA. http://www.nasa.gov/content/goddard/hubble-traces-subtle-signals-of-water-on-hazy-worlds/. Retrieved on 4 December 2013. 
  4. Mandell, Avi M.; Haynes, Korey; Sinukoff, Evan; Madhusudhan, Nikku; Burrows, Adam; Deming, Drake (2013). "Exoplanet Transit Spectroscopy Using WFC3: WASP-12 b, WASP-17 b, and WASP-19 b". Astrophysical Journal 779: 128. doi:10.1088/0004-637X/779/2/128. Bibcode2013ApJ...779..128M. http://iopscience.iop.org/article/10.1088/0004-637X/779/2/128. 
  5. 5.0 5.1 Sedaghati, Elyar; Boffin, Henri M. J.; MacDonald, Ryan J.; Gandhi, Siddharth; Madhusudhan, Nikku; Gibson, Neale P.; Oshagh, Mahmoudreza; Claret, Antonio; et al. (2017). "Detection of titanium oxide in the atmosphere of a hot Jupiter". Nature 549: 238-241. doi:10.1038/nature23651. Bibcode2017Natur.549..238S. 
  6. European Southern Observatory (September 13, 2017). "Inferno World with Titanium Skies". Press release. https://www.eso.org/public/news/eso1729/. Retrieved on December 24, 2017. 
Cite error: <ref> tag with name "Wong2016" defined in <references> is not used in prior text.

External linksEdit

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