WASP-13
Sign in to saveAlso known as BD+34 1976, Gloas
WASP-13, also named Gloas, is a star in the Lynx constellation. The star is similar, in terms of metallicity and mass, to the Sun, although it is hotter and most likely older. The star was first observed in 1997, according to the SIMBAD database, and was targeted by SuperWASP after the star was observed by one of the SuperWASP telescopes beginning in 2006. Follow-up observations on the star led to the discovery of planet Cruinlagh in 2008; the discovery paper was published in 2009.
Astronomical data · SIMBAD
- Object type
- V*
- Spectral type
- G1V
- Distance
- 753 light-years
- Redshift
- z = 0.00003268981564152895
- Coordinates
- RA 140.1030° · Dec 33.8824°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Distance from Earth
- 156
- Radius
- 1.5753999
Show 15 more facts
- spectral class
- G1V
- catalog code
- TIC 8767448
- effective temperature
- 5826
- apparent magnitude
- 10.382959
- radial velocity
- 10.3591
- parallax
- 4.331
- metallicity
- 0.007
- stellar rotational velocity
- 5.97
- surface gravity
- 13152
- name
- Gloas
- luminosity
- 2.7312114
- right ascension component of proper motion
- -2.275
- declination component of proper motion
- -20.072
- right ascension
- 140.10297724525
- declination
- 33.88241556661
via Wikidata · CC0
~4 min read
Article
5 sectionsContents
- Observational history
- Naming
- Characteristics
- Planetary system
- References
WASP-13, also named Gloas, is a star in the Lynx constellation. The star is similar, in terms of metallicity and mass, to the Sun, although it is hotter and most likely older. The star was first observed in 1997, according to the SIMBAD database, and was targeted by SuperWASP after the star was observed by one of the SuperWASP telescopes beginning in 2006. Follow-up observations on the star led to the discovery of planet Cruinlagh in 2008; the discovery paper was published in 2009.
==Observational history== 175px|thumb|left|The telescope, housed at the Haute-Provence Observatory, which was used to collect radial velocity measurements According to SIMBAD, WASP-13 was first observed in 1997, when it was catalogued by astronomers measuring the proper motion of stars in regions of the sky where galaxies are detected. Between November 27, 2006, and April 1, 2007, the SuperWASP-North telescope in the Canary Islands observed WASP-13; analysis of the data suggested that a planet could be in the orbit of the star.