WASP-78

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WASP-78
Observation data
Epoch J2000      Equinox J2000
Constellation Eridanus
Right ascension 04h 15m 01.5044s[1]
Declination −22° 06′ 59.1039″[1]
Apparent magnitude (V) 12.0[2]
Characteristics
Evolutionary stage
main-sequence star[citation needed
]
Spectral type F8[2]
Distance
2,520 ± 60 ly
(770 ± 20 pc)
Details
Gyr
TYC 5889-271-1, GSC 05889-00271, 2MASS J04150149-2206591[1]
Database references
SIMBADdata

WASP-78, is a single F-type main-sequence star about 2500 light-years away. It is likely to be younger than the Sun at 3.4+1.5
−0.8
billion years.[4] WASP-78 is depleted in heavy elements, having a 45% concentration of iron compared to the Sun.

Planetary system

In 2012 a

b was detected on a circular orbit. The planetary equilibrium temperature is 2350±80 K,[2] while the nightside temperature measured in 2019 is 2200±41 K.[5] The dayside planetary temperature measured in 2020 is 2560±130 K.[6]

A survey in 2016 measured a

Rossiter-McLaughlin effect and found the planetary orbit is well aligned with the equatorial plane of the star, misalignment equal to −6.4±5.9°[4] The planet cannot have formed in its current orbit and has likely undergone in the past a migration from the initial highly eccentric orbit.[7]

The WASP-78 planetary system[2]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b
0.89±0.08 MJ 0.0362±0.0008 2.17517632±0.0000047 0 83.2+2.3
−1.6
°
1.70±0.11 RJ

References

  1. ^ a b c d e f "WASP-78". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. ^
    S2CID 119233646
  3. ^ .
  4. ^