Jump to content

WASP-18

Coordinates: Sky map 01h 37m 25s, −45° 40′ 41″
From Wikipedia, the free encyclopedia
This is an old revision of this page, as edited by Mike s (talk | contribs) at 03:25, 27 October 2013 (add starbox astrometry and ref). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
WASP-18
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Phoenix[1]
Right ascension 01h 37m 25.034s[2]
Declination –45° 40′ 40.39″[2]
Apparent magnitude (V) 9.3[3]
Characteristics
Spectral type F6[3]
Astrometry
Proper motion (μ) RA: 26.52 ± 0.95[2] mas/yr
Dec.: 18.79 ± 1.06[2] mas/yr
Parallax (π)10.06±1.07 mas[2]
Distanceapprox. 320 ly
(approx. 100 pc)
Details
Mass1.256 ± 0.13[3] M
Radius1.216 +0.067
−0.054
[3] R
Surface gravity (log g)4.37 ± 0.03[4] cgs
Temperature6368 ± 66[4] K
Metallicity [Fe/H]0.11 ± 0.08[4] dex
Rotational velocity (v sin i)11.9 ± 1.2[4] km/s
Age0.5–1.5[3] Gyr
Other designations
HD 10069, HIP 7562, PPM 306061, SAO 215585
Database references
SIMBADdata
Exoplanet Archivedata

WASP-18 is a magnitude 9 star located in the Phoenix constellation of the southern hemisphere.[1] It has a mass of 1.25 solar masses.[5]

Planetary system

In 2009 SuperWASP project announced that a large hot Jupiter type extrasolar planet, WASP-18b, was orbiting very close to this star.[3]

The WASP-18 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ~10[3] MJ 0.020206 0.94145299[1] 0.0092

References

  1. ^ a b c "WASP-18b". Exoplanet Transit Database. Retrieved 2009-08-29.
  2. ^ a b c d e van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.Vizier catalog entry
  3. ^ a b c d e f g Hellier, Coel; et al. (2009). "An orbital period of 0.94days for the hot-Jupiter planet WASP-18b" (PDF). Nature. 460 (7259): 1098–1100. Bibcode:2009Natur.460.1098H. doi:10.1038/nature08245.
  4. ^ a b c d Torres, Guillermo; et al. (2012). "Improved Spectroscopic Parameters for Transiting Planet Hosts". The Astrophysical Journal. 757 (2). 161. arXiv:1208.1268. Bibcode:2012ApJ...757..161T. doi:10.1088/0004-637X/757/2/161.
  5. ^ PlanetQuest: WASP-18 b

See also