WASP-3b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | WASP-3 | |
Constellation | Lyra | |
Right ascension | (α) | 18h 34m 31.6241s[1] |
Declination | (δ) | +35° 39′ 41.488″[1] |
Apparent magnitude | (mV) | 10.64 |
Distance | ±60 800[1] ly (±20 250[1] pc) | |
Spectral type | F7V | |
Orbital elements | ||
Semi-major axis | (a) | 0.0317+0.0006 −0.001 AU |
Eccentricity | (e) | 0 |
Orbital period | (P) | 1.8468372 ± 6e-07 d |
Inclination | (i) | 85.06+0.15 −0.16° |
Time of transit | (Tt) | 2454605.55915 ± 0.00023 JD |
Physical characteristics | ||
Mass | (m) | 2.06 ± 0.13 MJ |
Radius | (r) | 1.454 ± 0.084 RJ |
Density | (ρ) | 1040 kg m−3 |
Surface gravity | (g) | 2.71 m/s² (26.6 g) |
Temperature | (T) | 1983 |
Discovery information | ||
Discovery date | October 31, 2007 | |
Discoverer(s) | Pollacco et al. (SuperWASP) | |
Discovery method | Transit | |
Discovery site | ORM | |
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
WASP-3b is an extrasolar planet orbiting the star WASP-3 located approximately 800 light-years away in the constellation Lyra. It was discovered via the transit method by SuperWASP, and follow up radial velocity observations confirmed that WASP-3b is a planet. The planet's mass and radius indicate that it is a gas giant with a similar bulk composition to Jupiter. WASP-3b has such an orbital distance around its star to classify it in the class of planets known as hot Jupiters and has an atmospheric temperature of approximately 1983 K.[2]
WASP-3b undergoes no detectable gravitational tugging from other bodies in this system.[3]
See also
References
- 1 2 3 4 Brown, A. G. A; et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy and Astrophysics. 595. A2. arXiv:1609.04172. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512. Gaia Data Release 1 catalog entry
- ↑ Pollacco, D.; et al. (2008). "WASP-3b: a strongly irradiated transiting gas-giant planet". Monthly Notices of the Royal Astronomical Society. 385 (3): 1576–1584. arXiv:0711.0126. Bibcode:2008MNRAS.385.1576P. doi:10.1111/j.1365-2966.2008.12939.x.
- ↑ M Montalto; et al. (Nov 2, 2012). "A new analysis of the WASP-3 system: no evidence for an additional companion". MNRAS. 427 (4): 2757. arXiv:1211.0218. Bibcode:2012MNRAS.427.2757M. doi:10.1111/j.1365-2966.2012.21926.x.
External links
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