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WASP-16

Coordinates:Sky map14h 18m 44s, −20° 16′ 32″
From Wikipedia, the free encyclopedia
Star in constellation of Virgo
WASP-16
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationVirgo[1]
Right ascension14h 18m 43.9225s[2]
Declination−20° 16′ 31.844″[2]
Apparent magnitude (V)11.309[3]
Characteristics
Spectral typeG3V[4]
Apparent magnitude (B)12.51±0.32[5]
Apparent magnitude (R)~11.00[5]
Apparent magnitude (I)10.49±0.02[5]
Apparent magnitude (J)9.984±0.024[5]
Apparent magnitude (H)9.659±0.022[5]
Apparent magnitude (K)9.589±0.023[5]
Astrometry
Proper motion (μ)RA: 0.088(27)mas/yr[2]
Dec.: 17.350(21)mas/yr[2]
Parallax (π)5.1912±0.0262 mas[2]
Distance628 ± 3 ly
(192.6 ± 1.0 pc)
Details
Mass1.022±0.101[4] M
Radius0.946±0.054[4] R
Surface gravity (log g)4.5±0.2[4] cgs
Temperature5700±150[4] K
Metallicity [Fe/H]0.01±0.10[4] dex
Rotational velocity (v sin i)3.0±1.0[4] km/s
Age5+3.1
−0
[4][6] Gyr
Other designations
TYC 6147-229-1,GSC 06147-00229,SDSS J141843.92-201631.8,2MASS J14184392-2016317, Gaia DR2 6283723285046532864[5]
Database references
SIMBADdata
Exoplanet Archivedata

WASP-16 is amagnitude 11yellow dwarfmain sequencestar, with characteristics similar to theSun,[5] located in theVirgoconstellation.[1]

Planetary system

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In 2009, a planet of the star was announced by theSuperWASP project. It appears to be anotherhot Jupiter type exoplanet.[4]

In 2024, a candidatemini-neptune was detected, also using thetransit method. Further observations are needed to confirm its existence. The planet takes ten days to fully orbit WASP-16 and has anequilibrium temperature of 810 K (537 °C).[7]

The WASP-16 planetary system
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b0.855±0.059 MJ0.0421+0.001
−0.0018
3.1186009+0.0000146
−0.0000131
01.008 RJ
c(unconfirmed)10.457+0.018
−0.028
2.2±0.23 R🜨

See also

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References

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  1. ^ab"WASP-16b".Exoplanet Transit Database. Retrieved2009-08-28.
  2. ^abcdVallenari, 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. ^Maxted, P. F. L.; et al. (2011)."UBV(RI)C photometry of transiting planet hosting stars".Monthly Notices of the Royal Astronomical Society.418 (2):1039–1042.arXiv:1108.0349.Bibcode:2011MNRAS.418.1039M.doi:10.1111/j.1365-2966.2011.19554.x.S2CID 117056033.
  4. ^abcdefghiLister, T. A.; et al. (2009). "WASP-16b: A New Jupiter-Like Planet Transiting a Southern Solar Analog".The Astrophysical Journal.703 (1):752–756.arXiv:0908.0297.Bibcode:2009ApJ...703..752L.doi:10.1088/0004-637X/703/1/752.S2CID 15203701.
  5. ^abcdefgh"TYC 6147-229-1 -- Star".Centre de Données astronomiques de Strasbourg. Retrieved2009-08-20.
  6. ^Brown, D. J. A.; Cameron, A. Collier; Anderson, D. R.; Enoch, B.; Hellier, C.; Maxted, P. F. L.; Miller, G. R. M.; Pollacco, D.; Queloz, D.; Simpson, E.; Smalley, B.; Triaud, A. H. M. J.; Boisse, I.; Bouchy, F.; Gillon, M.; Hébrard, G. (2012)."Rossiter-McLaughlin effect measurements for WASP-16, WASP-25 and WASP-31★".Monthly Notices of the Royal Astronomical Society.423 (2):1503–1520.arXiv:1203.4971.Bibcode:2012MNRAS.423.1503B.doi:10.1111/j.1365-2966.2012.20973.x.S2CID 53445367.
  7. ^Dévora-Pajares, Martín; Pozuelos, Francisco J.; Thuillier, Antoine; Timmermans, Mathilde; Van Grootel, Valérie; Bonidie, Victoria; Mota, Luis Cerdeño; Suárez, Juan C. (2024)."The SHERLOCK pipeline: new exoplanet candidates in the WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 systems".Monthly Notices of the Royal Astronomical Society.arXiv:2407.14602.doi:10.1093/mnras/stae1740.

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