WASP-75

WASP-75
Observation data; Epoch J2000 Equinox J2000
Constellation	Aquarius
Right ascension	22h 49m 32.5677s
Declination	−10° 40′ 31.9275″
Apparent magnitude (V)	11.299
Characteristics
Evolutionary stage	Main sequence[citation needed]
Spectral type	F9
Astrometry
Radial velocity (Rv)	2.7±0.8 km/s
Proper motion (μ)	RA: 45.892 mas/yr ; Dec.: 15.428 mas/yr
Parallax (π)	3.3387 ± 0.0202 mas
Distance	977 ± 6 ly ; (300 ± 2 pc)
Details
Mass	1.18 M☉
Radius	1.39 R☉
Luminosity	1.1±0.01 L☉
Surface gravity (log g)	4.233 cgs
Temperature	6090 K
Metallicity [Fe/H]	0.07±0.09 dex
Rotation	11.2±1.5 d
Age	2.9±0.2 Gyr
Other designations
	BD−11 5929, Gaia DR3 2605161444735454464, K2-40, EPIC 206154641, GSC 05816-01135, 2MASS J22493256-1040320
Database references
SIMBAD	data

WASP-75 is a F-type main-sequence star about 980 light-years away. The star is much younger than the Sun at approximately 2.9±0.2 billion years.^[5] WASP-75 is similar to the Sun in its concentration of heavy elements.^[3]

Planetary system

In 2013 a transiting hot Jupiter planet b was detected on a tight, circular orbit,^[6] and the planet was confirmed in 2018.^[3] Its equilibrium temperature is 1,688 K.^[3]

The WASP-75 planetary system^[7]
Companion (in order from star)	Mass	Semimajor axis (AU)	Orbital period (days)	Eccentricity	Inclination	Radius
b	1.08±0.05^[3] $M$ _J	0.0377±0.0006^[3]	2.484193	<0.1	81.96±0.02^[3]°	1.31±0.02^[3] $R$ _J

References

^ ^a ^b ^c "BD-11 5929", SIMBAD, Centre de données astronomiques de Strasbourg
^ ^a ^b Petigura, Erik A.; Crossfield, Ian J. M.; Isaacson, Howard; Beichman, Charles A.; Christiansen, Jessie L.; Dressing, Courtney D.; Fulton, Benjamin J.; Howard, Andrew W.; Kosiarek, Molly R.; Lépine, Sébastien; Schlieder, Joshua E.; Sinukoff, Evan; Yee, Samuel W. (2017), "Planet Candidates from K2 Campaigns 5–8 and Follow-up Optical Spectroscopy", The Astronomical Journal, 155: 21, arXiv:1711.06377, doi:10.3847/1538-3881/aa9b83, S2CID 55674757
^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j Clark, B. J. M.; Anderson, D. R.; Hellier, C.; Turner, O. D.; Močnik, T. (2018), "An Analysis of Transiting Hot Jupiters Observed with K2: WASP-55b and WASP-75b", Publications of the Astronomical Society of the Pacific, 130 (985): 034401, arXiv:1802.02132, Bibcode:2018PASP..130c4401C, doi:10.1088/1538-3873/aaa33e, S2CID 119077382
^ ^a ^b ^c ^d 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.
^ ^a ^b ^c Bonfanti, A.; Ortolani, S.; Nascimbeni, V. (2016), "Age consistency between exoplanet hosts and field stars", Astronomy & Astrophysics, 585: A5, arXiv:1511.01744, Bibcode:2016A&A...585A...5B, doi:10.1051/0004-6361/201527297, S2CID 53971692
^ Gómez Maqueo Chew, Y.; Faedi, F.; Pollacco, D.; Brown, D. J. A.; Doyle, A. P.; Collier Cameron, A.; Gillon, M.; Lendl, M.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Wheatley, P. J.; Busuttil, R.; Liebig, C.; Anderson, D. R.; Armstrong, D. J.; Barros, S. C. C.; Bento, J.; Bochinski, J.; Burwitz, V.; Delrez, L.; Enoch, B.; Fumel, A.; Haswell, C. A.; Hébrard, G.; Hellier, C.; Holmes, S.; Jehin, E.; Kolb, U.; et al. (2013), "Discovery of WASP-65b and WASP-75b: Two hot Jupiters without highly inflated radii", Astronomy & Astrophysics, 559: A36, arXiv:1307.6532, Bibcode:2013A&A...559A..36G, doi:10.1051/0004-6361/201322314, S2CID 1008674
^ Sandford, Emily; Espinoza, Néstor; Brahm, Rafael; Jordán, Andrés (2019), "Estimation of singly-transiting K2 planet periods with Gaia parallaxess", Monthly Notices of the Royal Astronomical Society, 489 (3): 3149–3161, arXiv:1908.08548, Bibcode:2019MNRAS.489.3149S, doi:10.1093/mnras/stz2348, S2CID 201645337

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[SIMBAD-1] "BD-11 5929", SIMBAD, Centre de données astronomiques de Strasbourg

[Petigura2017-2] Petigura, Erik A.; Crossfield, Ian J. M.; Isaacson, Howard; Beichman, Charles A.; Christiansen, Jessie L.; Dressing, Courtney D.; Fulton, Benjamin J.; Howard, Andrew W.; Kosiarek, Molly R.; Lépine, Sébastien; Schlieder, Joshua E.; Sinukoff, Evan; Yee, Samuel W. (2017), "Planet Candidates from K2 Campaigns 5–8 and Follow-up Optical Spectroscopy", The Astronomical Journal, 155: 21, arXiv:1711.06377, doi:10.3847/1538-3881/aa9b83, S2CID 55674757

[Clark2018-3] ^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j Clark, B. J. M.; Anderson, D. R.; Hellier, C.; Turner, O. D.; Močnik, T. (2018), "An Analysis of Transiting Hot Jupiters Observed with K2: WASP-55b and WASP-75b", Publications of the Astronomical Society of the Pacific, 130 (985): 034401, arXiv:1802.02132, Bibcode:2018PASP..130c4401C, doi:10.1088/1538-3873/aaa33e, S2CID 119077382

[EDR3-4] 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.

[Bonfanti2015-5] Bonfanti, A.; Ortolani, S.; Nascimbeni, V. (2016), "Age consistency between exoplanet hosts and field stars", Astronomy & Astrophysics, 585: A5, arXiv:1511.01744, Bibcode:2016A&A...585A...5B, doi:10.1051/0004-6361/201527297, S2CID 53971692

[Chew2013-6] Gómez Maqueo Chew, Y.; Faedi, F.; Pollacco, D.; Brown, D. J. A.; Doyle, A. P.; Collier Cameron, A.; Gillon, M.; Lendl, M.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Wheatley, P. J.; Busuttil, R.; Liebig, C.; Anderson, D. R.; Armstrong, D. J.; Barros, S. C. C.; Bento, J.; Bochinski, J.; Burwitz, V.; Delrez, L.; Enoch, B.; Fumel, A.; Haswell, C. A.; Hébrard, G.; Hellier, C.; Holmes, S.; Jehin, E.; Kolb, U.; et al. (2013), "Discovery of WASP-65b and WASP-75b: Two hot Jupiters without highly inflated radii", Astronomy & Astrophysics, 559: A36, arXiv:1307.6532, Bibcode:2013A&A...559A..36G, doi:10.1051/0004-6361/201322314, S2CID 1008674

[Sandford2019-7] Sandford, Emily; Espinoza, Néstor; Brahm, Rafael; Jordán, Andrés (2019), "Estimation of singly-transiting K2 planet periods with Gaia parallaxess", Monthly Notices of the Royal Astronomical Society, 489 (3): 3149–3161, arXiv:1908.08548, Bibcode:2019MNRAS.489.3149S, doi:10.1093/mnras/stz2348, S2CID 201645337

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Observation data Epoch J2000 Equinox J2000
Constellation	Aquarius
Right ascension	22^h 49^m 32.5677^s^[1]
Declination	−10° 40′ 31.9275″^[1]
Apparent magnitude (V)	11.299^[2]
Characteristics
Evolutionary stage	Main sequence^{[citation needed]}
Spectral type	F9^[3]
Astrometry

Radial velocity (R_v)	2.7±0.8^[4] km/s
Proper motion (μ)	RA: 45.892^[4] mas/yr Dec.: 15.428^[4] mas/yr
Parallax (π)	3.3387 ± 0.0202 mas^[4]
Distance	977 ± 6 ly (300 ± 2 pc)

Details^[2]

Mass	1.18 `M`_☉
Radius	1.39 `R`_☉
Luminosity	1.1±0.01^[5] `L`_☉
Surface gravity (log g)	4.233 cgs
Temperature	6090 K
Metallicity [Fe/H]	0.07±0.09^[3] dex
Rotation	11.2±1.5 d^[3]
Age	2.9±0.2^[5] Gyr

Other designations
BD−11 5929, Gaia DR3 2605161444735454464, K2-40, EPIC 206154641, GSC 05816-01135, 2MASS J22493256-1040320^[1]
Database references
SIMBAD	data