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WASP-78

Coordinates:Sky map04h 15m 01.5044s, −22° 06′ 59.1039″
From Wikipedia, the free encyclopedia
Star in the constellation Eridanus
WASP-78
Observation data
Epoch J2000      Equinox J2000
ConstellationEridanus[1]
Right ascension04h 15m 01.5043s[2]
Declination−22° 06′ 59.103″[2]
Apparent magnitude (V)12.0[3]
Characteristics
Evolutionary stagemain sequence[2]
Spectral typeF8[3]
Astrometry
Radial velocity (Rv)1.26[4] km/s
Proper motion (μ)RA: −0.367(11)mas/yr[2]
Dec.: 6.395(13)mas/yr[2]
Parallax (π)1.3851±0.0136 mas[2]
Distance2,350 ± 20 ly
(722 ± 7 pc)
Details
Mass1.33±0.09[3] M
Radius2.20±0.12[3] R
Luminosity5.2±0.1[2] L
Surface gravity (log g)3.88±0.04[3] cgs
Temperature6,100±150[3] K
Metallicity[Fe/H]−0.35±0.14[3] dex
Rotation0.4±0.4[3]
Rotational velocity (v sin i)6.63±0.16[5] km/s
Age3.4+1.5
−0.8
[5] Gyr
Other designations
Gaia DR3 5089851638095503616,TYC 5889-271-1,GSC 05889-00271,2MASS J04150149-2206591[4]
Database references
SIMBADdata

WASP-78, is a singleF-type main-sequence star about 2350 light-years away. It is likely to be younger than the Sun at 3.4+1.5
−0.8
billion years.[5] WASP-78 is depleted in heavy elements, having a 45% concentration of iron compared to the Sun.

Planetary system

[edit]

In 2012 atransitinghot Jupiter planetb was detected on a circular orbit. The planetary equilibrium temperature is 2350±80K,[3] while the nightside temperature measured in 2019 is 2200±41K.[6] The dayside planetary temperature measured in 2020 is2,560±130 K.[7]

A survey in 2016 measured aRossiter-McLaughlin effect and found the planetary orbit is well aligned with the equatorial plane of the star, misalignment equal to −6.4±5.9°[5] The planet cannot have formed in its current orbit and has likely undergone in the past a migration from the initial highly eccentric orbit.[8]

The WASP-78 planetary system[3]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b0.89±0.08 MJ0.0362±0.00082.17517632±0.0000047083.2+2.3
−1.6
°
1.70±0.11 RJ

References

[edit]
  1. ^Roman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  2. ^abcdefVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abcdefghijSmalley, B.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2012), "WASP-78b and WASP-79b: Two highly-bloated hot Jupiter-mass exoplanets orbiting F-type stars in Eridanus",Astronomy & Astrophysics,547: A61,arXiv:1206.1177,Bibcode:2012A&A...547A..61S,doi:10.1051/0004-6361/201219731,S2CID 119233646
  4. ^ab"WASP-78".SIMBAD.Centre de données astronomiques de Strasbourg.
  5. ^abcdBrown, D. J. A.; Triaud, A. H. M. J.; Doyle, A. P.; Gillon, M.; Lendl, M.; Anderson, D. R.; Collier Cameron, A.; Hébrard, G.; Hellier, C.; Lovis, C.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Smalley, B. (2016), "Rossiter–McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems",Monthly Notices of the Royal Astronomical Society,464:810–839,arXiv:1610.00600,doi:10.1093/mnras/stw2316,S2CID 53497449
  6. ^Garhart, Emily; Deming, Drake; Mandell, Avi; Knutson, Heather A.; Wallack, Nicole; Burrows, Adam; Fortney, Jonathan J.; Hood, Callie; Seay, Christopher; Sing, David K.; Benneke, Björn; Fraine, Jonathan D.; Kataria, Tiffany; Lewis, Nikole; Madhusudhan, Nikku; McCullough, Peter; Stevenson, Kevin B.; Wakeford, Hannah (2020), "Statistical Characterization of Hot Jupiter Atmospheres Using Spitzer's Secondary Eclipses",The Astronomical Journal,159 (4): 137,arXiv:1901.07040,Bibcode:2020AJ....159..137G,doi:10.3847/1538-3881/ab6cff,S2CID 119209434
  7. ^Wong, Ian; Shporer, Avi; Daylan, Tansu; Benneke, Björn; Fetherolf, Tara; Kane, Stephen R.; Ricker, George R.; Vanderspek, Roland; Latham, David W.; Winn, Joshua N.; Jenkins, Jon M.; Boyd, Patricia T.; Glidden, Ana; Goeke, Robert F.; Sha, Lizhou; Ting, Eric B.; Yahalomi, Daniel (2020), "Systematic phase curve study of known transiting systems from year one of the TESS mission",The Astronomical Journal,160 (4): 155,arXiv:2003.06407,Bibcode:2020AJ....160..155W,doi:10.3847/1538-3881/ababad,S2CID 212717799
  8. ^Valsecchi, Francesca (2014), "Planets on the Edge",The Astrophysical Journal,787 (1): L9,arXiv:1403.1870,Bibcode:2014ApJ...787L...9V,doi:10.1088/2041-8205/787/1/L9,S2CID 118451863
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