WASP-19b

WASP-19b is an extrasolar planet, notable for possessing one of the shortest orbital periods of any known planetary body: 0.7888399 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. At the time of discovery it was the shortest period hot Jupiter discovered as planets with shorter orbital periods had a rocky, or metallic composition.

WASP-19b
Size comparison of WASP-19b with Jupiter.
Discovery
Discovered byHebb et al. (SuperWASP)[1]
Discovery dateDecember 10, 2009[1]
Transit[1]
Orbital characteristics
0.01655 ± 0.00013 AU (2,476,000 ± 19,000 km)
Eccentricity0.0046+0.0044
−0.0028[2]
0.78884 ± 0.0000003 d (18.9321600 ± 7.2×10−6 h; 68,155.776 ± 0.026 s)[1]
Inclination79.4±0.4[2]
StarWASP-19
Physical characteristics
Mean radius
1.386±0.032[2] RJ
Mass1.168±0.023[2] MJ
Mean density
680 kg/m3 (1,150 lb/cu yd)
Albedo<0.26 [3]
0.16±0.04[4]
Temperature2350+168
−314[5]
2240±40[4]

    The study in 2012, utilizing a Rossiter–McLaughlin effect, have determined the planetary orbit is well aligned with the equatorial plane of the star, misalignment equal to -15±11°.[6]

    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.[3]

    In 2019 the planet was observed with TESS and the eclipse of the planet was measured. The broad variations caused by the changing aspect of the heated face of the planet were measured. The study deduced that the dayside has a temperature of 2240 ± 40 K (1967 ± 40 °C) and that the planet reflects 16 ± 4 percent of the light that falls on it.The last value is relatively high compared to other planets.[7][4]

    Despite of the short orbital period, orbital decay of the WASP-19b was not detected as in 2019.[8]

    Atmosphere

    In December 2013, scientists working with the Hubble Space Telescope reported detecting water in the atmosphere of the exoplanet.[9][10]

    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.[11] They also detected a strongly scattering haze in the atmosphere as well as the element sodium, and additionally confirmed the presence of water.[5]

    A study using TESS data concluded that the atmosphere of WASP-19b is moderately efficient at transporting heat from the dayside to the nightside.[4]

    Comparison of "hot Jupiter" exoplanets (artist concept).

    From top left to lower right: WASP-12b, WASP-6b, WASP-31b, WASP-39b, HD 189733b, HAT-P-12b, WASP-17b, WASP-19b, HAT-P-1b and HD 209458b.

    References
    1. Hebb, L.; et al. (2010). "WASP-19b: The Shortest Period Transiting Exoplanet Yet Discovered". The Astrophysical Journal. 708 (1): 224–231. arXiv:1001.0403. Bibcode:2010ApJ...708..224H. doi:10.1088/0004-637X/708/1/224.
    2. "Notes for planet WASP-19b". The Extrasolar Planets Encyclopaedia. Retrieved 2009-12-10.
    3. Abe, L.; Gonçalves, I.; Agabi, A.; Alapini, A.; Guillot, T.; Mékarnia, D.; Rivet, J.-P.; Schmider, F.-X.; Crouzet, N.; Fortney, J.; Pont, F.; Barbieri, M.; Daban, J.-B.; Fanteï-Caujolle, Y.; Gouvret, C.; Bresson, Y.; Roussel, A.; Bonhomme, S.; Robini, A.; Dugué, M.; Bondoux, E.; Péron, S.; Petit, P.-Y.; Szulágyi, J.; Fruth, T.; Erikson, A.; Rauer, H.; Fressin, F.; Valbousquet, F.; et al. (2013). "The secondary eclipses of WASP-19b as seen by the ASTEP 400 telescope from Antarctica". Astronomy & Astrophysics. 553: A49. arXiv:1303.0973. Bibcode:2013A&A...553A..49A. doi:10.1051/0004-6361/201220351.
    4. Wong, Ian; Benneke, Björn; Shporer, Avi; Fetherolf, Tara; Kane, Stephen R.; Ricker, George R.; Vanderspek, Roland; Seager, Sara; Winn, Joshua N.; Collins, Karen A.; Mireles, Ismael; Morris, Robert; Tenenbaum, Peter; Ting, Eric B.; Rinehart, Stephen; Villaseñor, Jesus Noel (2019-12-13). "TESS Phase Curve of the Hot Jupiter WASP-19b". arXiv:1912.06773 [astro-ph.EP].
    5. Sedaghati, Elyar; et al. (2017). "Detection of titanium oxide in the atmosphere of a hot Jupiter". Nature. 549 (7671): 238–241. arXiv:1709.04118. Bibcode:2017Natur.549..238S. doi:10.1038/nature23651.
    6. Obliquities of Hot Jupiter host stars: Evidence for tidal interactions and primordial misalignments, 2012, arXiv:1206.6105
    7. waspplanets (2019-12-19). "TESS phase curve of WASP-19b". WASP Planets. Retrieved 2020-01-01.
    8. Discarding orbital decay in WASP-19b after one decade of transit observations, 2019, arXiv:1910.11930
    9. Staff (3 December 2013). "Hubble Traces Subtle Signals of Water on Hazy Worlds". NASA. Retrieved 4 December 2013.
    10. Mandell, Avi M.; et al. (2013). "Exoplanet Transit Spectroscopy Using WFC3: WASP-12 b, WASP-17 b, and WASP-19 b". Astrophysical Journal. 779 (2). 128. arXiv:1310.2949. Bibcode:2013ApJ...779..128M. doi:10.1088/0004-637X/779/2/128.
    11. "Inferno World with Titanium Skies" (Press release). European Southern Observatory. September 13, 2017. Retrieved December 24, 2017.

    Media related to WASP-19b at Wikimedia Commons

    This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.