WASP-2
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Delphinus |
| A[1] | |
| Right ascension | 20h 30m 54.1300s[2] |
| Declination | +06° 25′ 46.37″[2] |
| Apparent magnitude (V) | +11.98[2] |
| Ca | |
| Right ascension | ~20h 30m 54s[1] |
| Declination | ~+06° 25′ 46″[1] |
| Apparent magnitude (V) | 15.38[1] |
| Characteristics | |
| Spectral type | K1V[3]/M[1] |
| Apparent magnitude (B) | ~13[2] |
| Apparent magnitude (V) | ~11.98[2] |
| Apparent magnitude (J) | 10.166±0.027[2] |
| Apparent magnitude (H) | 9.752±0.026[2] |
| Apparent magnitude (K) | 9.632±0.024[2] |
| Astrometry | |
| Proper motion (μ) | RA: 3.0[2] mas/yr Dec.: -53.1[2] mas/yr |
| Distance | 469 ly (144 pc) |
| Details | |
| Mass | 0.77[1]/0.48[1] M☉ |
| Radius | 0.834 ±0.08 R☉ |
| Temperature | 5200 ±200 K |
| Other designations | |
| GSC 00522-01199, 1SWASP J203054.12+062546.4, | |
| Database references | |
| SIMBAD | data |
WASP-2 is a magnitude 12 orange dwarf star located about 469 light-years away in the Delphinus constellation.[2]
Planetary system
This star has one extrasolar planet WASP-2b, detected by the SuperWASP project in 2006.[3]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 0.914 ±0.092[1] MJ | 0.03138 ±0.00142[1] | 2.152226 ±4e-05 | 0 | — | — |
Binary star
In 2008 a study was undertaken of fourteen stars with exoplanets that were originally discovered using the transit method through relatively small telescopes. These systems were re-examined with the 2.2 m (87 in) reflector telescope at the Calar Alto Observatory in Spain. This star system, along with two others, was determined to be a previously unknown binary star system. The previously unknown secondary star is a dim magnitude 15 M-type star separated by about 111 AU from the primary, appearing offset from the primary by about one arc second in the images. This discovery resulted in a recalculation of parameters for both the planet and the primary star.[1]
Notes
- Note b: The secondary star is identified with a "C" suffix so as to not confuse it with the planetary designation suffix "b".[1]
See also
References
- ^ a b c d e f g h i j k Daemgen; Hormuth, F.; Brandner, W.; Bergfors, C.; Janson, M.; Hippler, S.; Henning, T.; et al. (2009). "Binarity of transit host stars - Implications for planetary parameters" (PDF). Astronomy and Astrophysics. 498: 567–574. doi:10.1051/0004-6361/200810988.
{{cite journal}}: Explicit use of et al. in:|author=(help) - ^ a b c d e f g h i j k "SIMBAD query result: GSC 00522-01199 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-04.
- ^ a b Cameron; Bouchy, F.; Hébrard, G.; Maxted, P.; Pollacco, D.; Pont, F.; Skillen, I.; Smalley, B.; Street, R. A.; et al. (2007). "WASP-1b and WASP-2b: two new transiting exoplanets detected with SuperWASP and SOPHIE". Monthly Notices of the Royal Astronomical Society. 375: 951–957. doi:10.1111/j.1365-2966.2006.11350.x.
{{cite journal}}: Explicit use of et al. in:|author=(help) (web Preprint)
External links
- "WASP-2". Exoplanets. Retrieved 2009-05-04.