WASP-16

WASP-16 is a magnitude 11 yellow dwarf main sequence star, with characteristics similar to our Sun,[5] located in the Virgo constellation.[1]

WASP-16
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Virgo[1]
Right ascension  14h 18m 43.9227s[2]
Declination −20° 16 31.8422[2]
Apparent magnitude (V) 11.309[3]
Characteristics
Spectral type G3V[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: −0.040±0.082[2] mas/yr
Dec.: 17.257±0.061[2] mas/yr
Parallax (π)5.1230 ± 0.0507[2] mas
Distance637 ± 6 ly
(195 ± 2 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
Extrasolar Planets
Encyclopaedia
data

Planetary system

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

The WASP-16 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.855±0.059 MJ 0.0421+0.001
−0.0018
3.1186009+0.0000146
−0.0000131
0
gollark: Apiocity is basically bee-ness.
gollark: It's a much more complex procedure involving invocation of the dark bee gods, [REDACTED]-65, several orbs of apiocity (μ-class and up), the ███ ████████ ████ █████ arrays, and direct memory access.
gollark: And tell them that they're being impossible.
gollark: Really? You'll have to talk to our physics disabling department.
gollark: Your claim is irrelevant.

See also

References

  1. "WASP-16b". Exoplanet Transit Database. Retrieved 2009-08-28.
  2. 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.
  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.
  4. Lister, 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.
  5. "TYC 6147-229-1 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-08-20.
  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-Mc Laughlin 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.

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