WASP-62: Difference between revisions
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'''WASP-62''' was named Naledi in 2019.<ref name="Methodology"/> |
'''WASP-62''' was named Naledi in 2019.<ref name="Methodology"/> |
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==Planetary system== |
==Planetary system== |
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A [[Astronomical transit|transiting]] [[hot Jupiter]] [[exoplanet]] orbiting WASP-62 was discovered by [[Wide Angle Search for Planets|WASP]] in 2012.<ref name=Hellier2012>{{citation|arxiv=1204.5095|title=Seven transiting hot-Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b & WASP-67b|year=2012}}</ref> The planet's equilibrium temperature is 1440{{±|30}} [[Kelvin|K]], but the measured average temperature is colder at 1329.6{{±|44.8}} K.<ref name=Kilpatrick2016/>. In 2020, a transmission spectrum indicated the atmosphere of WASP-62b is free of clouds. It contains sodium and possibly silicon hydrides.<ref>{{citation|arxiv=2011.06424|title=Evidence of a Clear Atmosphere for WASP-62b: the Only Known Transiting Gas Giant in the JWST Continuous Viewing Zone|year=2020}}</ref> |
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The planetary orbit is slightly misaligned to the equatorial plane of the star, misalignment angle equals to 19.4{{±|5.1|4.9}}°.<ref name=Brown2016>{{citation|arxiv=1610.00600|title=Rossiter–McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems|year=2016}}</ref> |
The planetary orbit is slightly misaligned to the equatorial plane of the star, misalignment angle equals to 19.4{{±|5.1|4.9}}°.<ref name=Brown2016>{{citation|arxiv=1610.00600|title=Rossiter–McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems|year=2016}}</ref> |
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Revision as of 22:22, 13 November 2020
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Dorado |
| Right ascension | 05h 48m 33.5938s[1] |
| Declination | −63° 59′ 18.3868″[1] |
| Apparent magnitude (V) | 10.21 |
| Characteristics | |
| Evolutionary stage | main-sequence star |
| Spectral type | F |
| Apparent magnitude (B) | 10.73 [1] |
| Apparent magnitude (G) | 10.0721 [1] |
| Apparent magnitude (R) | 9.93 [1] |
| Astrometry | |
| Radial velocity (Rv) | 15.47 km/s |
| Proper motion (μ) | RA: -15.641[2] mas/yr Dec.: 26.046[2] mas/yr |
| Parallax (π) | 5.6649 ± 0.0189 mas[2] |
| Distance | 576 ± 2 ly (176.5 ± 0.6 pc) |
| Details[3] | |
| Mass | 1.250±0.05 M☉ |
| Radius | 1.280±0.05 R☉ |
| Surface gravity (log g) | 4.45±0.1 cgs |
| Temperature | 6230±80 K |
| Metallicity [Fe/H] | 0.04±0.06 dex |
| Rotational velocity (v sin i) | 8.7±0.4 km/s |
| Age | 0.8±0.6[4] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | 484 data |
WASP-62 is a single star about 575 light-years away. It is a F class main-sequence star, orbited by a planet WASP-62b. The age of WASP-62 is much younger than the Sun at 0.8±0.6 billion years,[4] and it has a metal abundance similar to the Sun.
WASP-62 was named Naledi in 2019.[5]
Planetary system
A transiting hot Jupiter exoplanet orbiting WASP-62 was discovered by WASP in 2012.[6] The planet's equilibrium temperature is 1440±30 K, but the measured average temperature is colder at 1329.6±44.8 K.[3]. In 2020, a transmission spectrum indicated the atmosphere of WASP-62b is free of clouds. It contains sodium and possibly silicon hydrides.[7]
The planetary orbit is slightly misaligned to the equatorial plane of the star, misalignment angle equals to 19.4+5.1
−4.9°.[4]
WASP-62b was named "Krotoa" in 2019 by amateur astronomers from South Africa as part of the NameExoWorlds contest.[5]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 0.562±0.042 MJ | 0.0567±0.0007[6] | 4.4119530±0.000003 | <0.21[6] | 88.3+0.9 −0.6° |
1.390±0.060 RJ |
References
- ^ a b c d e f "CPD-64 484". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c 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.
- ^ a b c Spitzer secondary eclipse depths with multiple intrapixel sensitivity correction methods observations of WASP-13b, WASP-15b, WASP-16b, WASP-62b, and HAT-P-22b, 2016, arXiv:1611.08708
- ^ a b c Rossiter–McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems, 2016, arXiv:1610.00600
- ^ a b "International Astronomical Union Approves Names For New Stars And Exoplanets". Space in Africa. Retrieved 2020-11-12.
- ^ a b c Seven transiting hot-Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b & WASP-67b, 2012, arXiv:1204.5095
- ^ Evidence of a Clear Atmosphere for WASP-62b: the Only Known Transiting Gas Giant in the JWST Continuous Viewing Zone, 2020, arXiv:2011.06424
