WASP-60

WASP-60 is a F-type main-sequence star about 1420 light-years away. The stars age is much younger than the Sun's at 1.7±0.5 billion years. WASP-60 is enriched in heavy elements, having 180% of the solar abundance of iron. The star does not have noticeable starspot activity, an unexpected observation for a relatively young star.[2] The age of WASP-60 determined by different methods is highly discrepant though, and it may actually be an old star which experienced an episode of spin-up in the past.[4]

WASP-60 / Morava
Observation data
Epoch J2000      Equinox J2000
Constellation Pegasus
Right ascension 23h 46m 39.9747s[1]
Declination 31° 09′ 21.3721″[1]
Apparent magnitude (V) 12.18
Characteristics
Evolutionary stage Main sequence
Spectral type F9[2]
Astrometry
Radial velocity (Rv)-26.604[1] km/s
Proper motion (μ) RA: 30.262[1] mas/yr
Dec.: −5.852[1] mas/yr
Parallax (π)2.2916 ± 0.0397 mas[1]
Distance1,420 ± 20 ly
(436 ± 8 pc)
Details[2]
Mass1.229±0.026 M☉
Radius1.401±0.066 R☉
Surface gravity (log g)4.31±0.11 cgs
Temperature6105±50 K
Metallicity [Fe/H]0.26±0.07 dex
Rotation34.8±2.7 d
Rotational velocity (v sin i)3.8±0.6 km/s
Age1.7±0.5 Gyr
Other designations
Morava, Gaia DR2 2868528637464028160, TYC 2767-1746-1, 2MASS J23463997+3109213[3]
Database references
SIMBADdata

The star was named Morava in 2019 by Serbian amateur astronomers as part of the NameExoWorlds contest, after the Morava River in Serbia.[5]

A multiplicity survey in 2015 did not detect any stellar companions to WASP-60.[6]

Planetary system

In 2012 a transiting hot Jupiter planet b was detected on a tight, circular orbit.[7] The planet was named Vlasina by Serbian astronomers in December 2019, after the Vlasina River, a tributary of the Morava.[8]

Its equilibrium temperature is 1479±35 K.[2]

Measurement of the Rossiter–McLaughlin effect in 2018 revealed WASP-60b is on a retrograde orbit relative to the equatorial plane of the star, orbital obliquity equal to 129±17°.[2]

The WASP-60 planetary system[2]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b (Vlasina) 0.560±0.036 MJ 0.05548±0.00040 4.3050040 0 86.05±0.57° 1.225±0.069 RJ

References
  1. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. Mancini, L.; et al. (2018), "The GAPS programme with HARPS-N at TNG", Astronomy & Astrophysics, 613: A41, arXiv:1802.03859, doi:10.1051/0004-6361/201732234, S2CID 73565379
  3. "WASP-60". SIMBAD. Centre de données astronomiques de Strasbourg.
  4. Brown, D. J. A. (2014), "Discrepancies between isochrone fitting and gyrochronology for exoplanet host stars?", Monthly Notices of the Royal Astronomical Society, 442 (2): 1844–1862, arXiv:1406.4402, Bibcode:2014MNRAS.442.1844B, doi:10.1093/mnras/stu950
  5. Star Facts Stars: A guide to the night sky Home Brightest Stars Star Names Star Names
  6. Wöllert, Maria; Brandner, Wolfgang; Bergfors, Carolina; Henning, Thomas (2015), "A Lucky Imaging search for stellar companions to transiting planet host stars", Astronomy & Astrophysics, 575: A23, arXiv:1507.01938, Bibcode:2015A&A...575A..23W, doi:10.1051/0004-6361/201424091, S2CID 119250579
  7. Hébrard, G.; et al. (2012), "WASP-52b, WASP-58b, WASP-59b, and WASP-60b: Four new transiting close-in giant planets", Astronomy & Astrophysics, 549: A134, arXiv:1211.0810, doi:10.1051/0004-6361/201220363, S2CID 54502046
  8. Srbija je dobila zadatak da predloži i izglasa novo ime za zvezdu WASP-60 i njenu planetu WASP-60b


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