HD 179949 b, formally named Mastika, is an extrasolar planet discovered by the Anglo-Australian Planet Search at the Anglo-Australian Observatory, which orbits the star HD 179949. The planet is a so-called "hot Jupiter", a Jupiter-mass planet orbiting very close to its parent star. In this case, orbital distance is almost one-tenth that of Mercury from the Sun. One orbital revolution lasts only about 3 days.[3][4]
Its magnetic field induces a bright spot on its star at 30 degrees latitude, which rotates at 87 degrees inclination. If the planet orbited at 83-97 degrees, then its transit would be visible from Earth. The angle of inclination is therefore 83 degrees or less, but not much less; and its mass is about 0.92 Jupiter masses MJ. The star is not tidally locked to the planet.[5]
Assuming the planet is perfectly grey with no greenhouse or tidal effects, and a Bond albedo of 0.1, the temperature would be 1533 K. This is, like Tau Boötis b, hotter than the predicted temperature of HD 209458 b (1392K), and close to that of HD 149026 b, before they were measured.
Searches for water in the planet's atmosphere have been inconclusive at first, as have attempts to determine whether titanium and vanadium oxides are present.[6] In the meantime, both carbon monoxide and water have been found in the dayside emission of HD 179949b.[7]
HD 179949 b is a candidate for "near-infrared characterisation.... with the VLTI Spectro-Imager".[8]
The light reflected off planet could not be detected as in 2021, implying HD 179949 b has a low albedo.[9]
The planet HD 179949 b is named Mastika. The name was selected in the NameExoWorlds campaign by Brunei,[10] during the 100th anniversary of the IAU. Mastika is a Malay word, which means a gem, precious stone, jewel or the prettiest, the most beautiful.[11][12]
^Cite error: The named reference AAPS planets was invoked but never defined (see the help page).
^Brogi, M.; De Kok, R. J.; Birkby, J. L.; Schwarz, H.; Snellen, I. A. G. (2014). "Carbon monoxide and water vapor in the atmosphere of the non-transiting exoplanet HD 179949 B". Astronomy & Astrophysics. 565: A124. arXiv:1404.3769v1. Bibcode:2014A&A...565A.124B. doi:10.1051/0004-6361/201423537. S2CID 56450007.
^Cite error: The named reference Tinney2001 was invoked but never defined (see the help page).
^Cite error: The named reference Butler2006 was invoked but never defined (see the help page).
^Shkolnik and Walker; Walker, G. A. H.; Bohlender, D. A. (2003). "Evidence for Planet-induced Chromospheric Activity on HD 179949". The Astrophysical Journal. 597 (2): 1092–1096. arXiv:astro-ph/0303557. Bibcode:2003ApJ...597.1092S. doi:10.1086/378583. S2CID 15829056.
^J. R. Barnes; Barman; Jones; Leigh; Cameron; Barber; Pinfield; et al. (3 Oct 2008). "HD 179949b: a close orbiting extrasolar giant planet with a stratosphere?". Monthly Notices of the Royal Astronomical Society. 390 (3): 1258. arXiv:0806.0298. Bibcode:2008MNRAS.390.1258B. doi:10.1111/j.1365-2966.2008.13831.x. S2CID 18736260.
^Brogi, M.; Kok, R. J. de; Birkby, J. L.; Schwarz, H.; Snellen, I. A. G. (2014). "Carbon monoxide and water vapor in the atmosphere of the non-transiting exoplanet HD 179949 b". Astronomy & Astrophysics. 565: A124. arXiv:1404.3769. Bibcode:2014A&A...565A.124B. doi:10.1051/0004-6361/201423537. ISSN 0004-6361. S2CID 56450007.
^Renard, Stéphanie; Absil, Olivier; Berger, Jean-Philippe; Bonfils, Xavier; Forveille, Thierry; Malbet, Fabien (2008). "Prospects for near-infrared characterisation of hot Jupiters with the VLTI Spectro-Imager (VSI)" (PDF). Proceedings of SPIE. Optical and Infrared Interferometry. 7013: 70132Z–70132Z–10. arXiv:0807.3014. Bibcode:2008SPIE.7013E..2ZR. doi:10.1117/12.790494. S2CID 119268109.
^Bailey, Jeremy; Bott, Kimberly; Cotton, Daniel V.; Kedziora-Chudczer, Lucyna; Zhao, Jinglin; Evensberget, Dag; Marshall, Jonathan P.; Wright, Duncan; Lucas, P. W. (2021), "Polarization of hot Jupiter systems: A likely detection of stellar activity and a possible detection of planetary polarization", Monthly Notices of the Royal Astronomical Society, 502 (2): 2331–2345, arXiv:2101.07411, doi:10.1093/mnras/stab172
HD179949b, formally named Mastika, is an extrasolar planet discovered by the Anglo-Australian Planet Search at the Anglo-Australian Observatory, which...
HD179949 is a 6th magnitude star in the constellation of Sagittarius. It is a yellow-white dwarf (spectral class F8 V), a type of star hotter and more...
core. HAT-P-3b HD 209458 bHD179949b Tau Boötis b Sato, Bun'ei; et al. (2005). "The N2K Consortium. II. A Transiting Hot Saturn around HD 149026 with a...
most massive exoplanet candidate is HD 217786 b, which masses 12.98 MJ; the least massive confirmed planet is HD 10180 b, which masses 0.004 MJ or 3.1 M🜨...
Variations and Coronal Abundances of the Star-Planet Interaction Candidate HD179949 (2023) (incl. A. Acharya, V. L. Kashyap, S. H. Saar, K. P. Singh). An...
ed.). Cambridge, MA: Sky Publishing. ISBN 978-1-931559-44-7. Rumrill, H. B. (June 1936). "Star Name Pronunciation". Publications of the Astronomical...
centres. In 2003, a team of astronomers in Hawaii observing the star HD179949 detected a bright spot on its surface, apparently created by the magnetosphere...