Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Indus |
Right ascension | 20 38 02.6870 |
Declination | −48° 27′ 43.4255″ |
Apparent magnitude (V) | 11.39 |
Characteristics | |
Evolutionary stage | main-sequence star or subgiant star |
Spectral type | F6 |
Astrometry | |
Radial velocity (Rv) | −5.1±0.6 km/s |
Proper motion (μ) | RA: 5.890 mas/yr Dec.: −4.892 mas/yr |
Parallax (π) | 1.7844 ± 0.0185 mas |
Distance | 1,830 ± 20 ly (560 ± 6 pc) |
Position (relative to WASP-88) | |
Component | WASP-88B |
Epoch of observation | 2017 |
Angular distance | 3.350±0.015″ |
Position angle | 355.5±0.5° |
Projected separation | 1877±8 AU |
Details | |
WASP-88 | |
Mass | 1.450±0.050 M☉ |
Radius | 2.08 −0.06 R☉ |
Surface gravity (log g) | 4.24±0.06 cgs |
Temperature | 6450±61 K |
Metallicity | 0.03±0.04 dex |
Rotational velocity (v sin i) | 8.4±0.8 km/s |
Age | 3.0±1.3 Gyr |
WASP-88B | |
Mass | 0.11 −0.02 M☉ |
Temperature | 2844 −209 K |
Other designations | |
Gaia DR2 6482103014085857024, 2MASS J20380268-4827434 | |
Database references | |
SIMBAD | data |
WASP-88 is a F-type main-sequence star. Its surface temperature is 6450±61 K. WASP-88 is similar to the Sun in its concentration of heavy elements, with a metallicity Fe/H index of 0.03±0.04, and is younger at an age of 3.0±1.3 billion years.
A multiplicity survey did detect a candidate red dwarf companion to WASP-88 in 2020, with a 1.65% probability of it being an unrelated background star.
Planetary system
In 2013, one planet, named WASP-88b, was discovered on a tight, circular orbit. The planet is highly inflated, and may be an easy target for atmospheric characterization. Planetary equilibrium temperature is 1775 K. The planetary atmosphere transmission spectrum is gray and featureless, probably indicating a large concentration of hazes.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.570 −0.078 MJ |
0.06438 −0.00074 |
4.954000±0.000019 | <0.13 | 88.0 −1.5° |
1.70 −0.07 RJ |
References
- ^ "WASP-88". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-01-25.
- ^ Bohn, A. J.; Southworth, J.; Ginski, C.; Kenworthy, M. A.; Maxted, P. F. L.; Evans, D. F. (2020), "A multiplicity study of transiting exoplanet host stars. I. High-contrast imaging with VLT/SPHERE", Astronomy & Astrophysics, 635: A73, arXiv:2001.08224, Bibcode:2020A&A...635A..73B, doi:10.1051/0004-6361/201937127, S2CID 210861118
- ^ Delrez, L.; Van Grootel, V.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Neveu-VanMalle, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2013), Transiting planets from WASP-South, Euler and TRAPPIST:WASP-68 b, WASP-73 b and WASP-88 b, three hot Jupiters transiting evolved solar-type stars, arXiv:1312.1827, doi:10.1051/0004-6361/201323204, S2CID 54846964
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ Andreasen, D. T.; Sousa, S. G.; Tsantaki, M.; Teixeira, G. D. C.; Mortier, A.; Santos, N. C.; Suarez-Andres, L.; Delgado-Mena, E.; Ferreira, A. C. S. (2017), "SWEET-Cat update and FASMA A new minimization procedure for stellar parameters using high-quality spectra", Astronomy & Astrophysics, A69: 600, arXiv:1703.06671, Bibcode:2017A&A...600A..69A, doi:10.1051/0004-6361/201629967, S2CID 119534579
- ^ Bonomo, A. S.; Desidera, S.; Benatti, S.; Borsa, F.; Crespi, S.; Damasso, M.; Lanza, A. F.; Sozzetti, A.; Lodato, G.; Marzari, F.; Boccato, C.; Claudi, R. U.; Cosentino, R.; Covino, E.; Gratton, R.; Maggio, A.; Micela, G.; Molinari, E.; Pagano, I.; Piotto, G.; Poretti, E.; Smareglia, R.; Affer, L.; Biazzo, K.; Bignamini, A.; Esposito, M.; Giacobbe, P.; Hébrard, G.; Malavolta, L.; et al. (2017), "The GAPS Programme with HARPS-N@TNG XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets", Astronomy & Astrophysics, A107: 602, arXiv:1704.00373, Bibcode:2017A&A...602A.107B, doi:10.1051/0004-6361/201629882, S2CID 118923163
- Kabáth, P.; Žák, Jiří; Boffin, H. M. J.; Ivanov, V. D.; Jones, D.; Skarka, M. (2019), "Detection limits of exoplanetary atmospheres with 2-m class telescopes", Publications of the Astronomical Society of the Pacific, 131 (1002): 085001, arXiv:1905.04665, Bibcode:2019PASP..131h5001K, doi:10.1088/1538-3873/ab2143, S2CID 152282971
- Spyratos, Petros; Nikolov, Nikolay; Southworth, John; Constantinou, Savvas; Madhusudhan, Nikku; Carter, Aarynn L.; De Mooij, Ernst J W.; Fortney, Jonathan J.; Gibson, Neale P.; Goyal, Jayesh M.; Helling, Christiane; Mayne, Nathan J.; Mikal-Evans, Thomas (2021), "Transmission spectroscopy with VLT FORS2: A featureless spectrum for the low-density transiting exoplanet WASP-88b", Monthly Notices of the Royal Astronomical Society, 506 (2): 2853–2870, arXiv:2106.14808, doi:10.1093/mnras/stab1847
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