WASP-1b explained

WASP-1b
Discoverer:Cameron et al. (SuperWASP
and SOPHIE)
South Africa
and France
Discovery Site:SAAO
Discovered:September 25, 2006
Apsis:astron
Semimajor:0.0382 (± 0.0013) AU
Eccentricity:0
Period:2.5199464 (± 8e-07) d
Inclination:88.65 (± 0.55)
Mean Radius:1.484
Mass:0.86 ± 0.07
Surface Grav:
1.27 g
Single Temperature:1,800 K

WASP-1b is an extrasolar planet orbiting the star WASP-1 located 1,300 light-years away in the constellation Andromeda.

Orbit and mass

The planet's mass and radius indicate that it is a gas giant with a similar bulk composition to Jupiter. Unlike Jupiter, but similar to many other planets detected around other stars, WASP-1b is located very close to its star, and belongs to the class of planets known as hot Jupiters.

WASP-1 b was discovered via the transit method by SuperWASP, for which the star and planet are named. Follow-up radial velocity measurements confirmed the presence of an unseen companion, and allowed for the mass of WASP-1 b to be determined.

In 2018, it was discovered via observations of the Rossiter-McLaughlin effect that the orbit of WASP-1b is strongly misaligned with rotational axis of the star by 79.0 degrees, making it a nearly "polar" orbit.[1]

See also

Further reading

External links

Notes and References

  1. 1011.5664. 10.1111/j.1365-2966.2011.18603.x. The spin-orbit angles of the transiting exoplanets WASP-1b, WASP-24b, WASP-38b and HAT-P-8b from Rossiter-Mc Laughlin observations★. 2011. Simpson. E. K.. Pollacco. D.. Cameron. A. Collier. Hébrard. G.. Anderson. D. R.. Barros. S. C. C.. Boisse. I.. Bouchy. F.. Faedi. F.. Gillon. M.. Hebb. L.. Keenan. F. P.. Miller. G. R. M.. Moutou. C.. Queloz. D.. Skillen. I.. Sorensen. P.. Stempels. H. C.. Triaud. A.. Watson. C. A.. Wilson. P. A.. Monthly Notices of the Royal Astronomical Society. 414. 4. 3023–3035. 2011MNRAS.414.3023S. 46522188.