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EntityQ968992· pop 17· linked from 63 articles

Also known as TOI-5797.01, TOI-5797b, TIC 374530847b

WASP-2b is an extrasolar planet orbiting the star WASP-2 located about 500 light years away in the constellation of Delphinus. It was discovered via the transit method, and then follow up measurements using the radial velocity method confirmed that WASP-2b was a planet. 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-2b is located very close to its star, and belongs to the class of planets known as hot Jupiters. A 2008 study concluded that the WASP-2b sys

Key facts

Planet.name
WASP-2b
Planet.image
Exoplanet Comparison WASP-2 b.png
Planet.caption
Size comparison of WASP-2b with Jupiter.
Planet.discoverer
Cameron et al. (SuperWASP)
Planet.discovery_site
SAAO
Planet.discovered
September 25, 2006
Planet.discovery_method
Transit
Planet.apsis
astron
Planet.semimajor
0.03138 (± 0.011) AU
Planet.eccentricity
0
Planet.period
2.15222144 (± 4e-07) d
Planet.inclination
84.73 (± 0.19)
Planet.star
WASP-2 A
Planet.mean_radius
1.079 ± 0.033
Planet.mass
0.847 ± 0.045
Planet.surface_grav
3.279 ± 0.036 g
Planet.single_temperature
1253 K

via Wikipedia infobox

Wikidata facts

Radius
1.079
Mass
0.931
Orbital period
2.15222144
Image
Exoplanet Comparison WASP-2 b.png
Show 13 more facts
catalog code
TIC 374530847b
Commons category
WASP-2 b
time of discovery or invention
2007-03-00
right ascension
307.72553300783830
declination
6.42953840608139
orbital eccentricity
0.013
semi-major axis of an orbit
0.03144
parallax
6.4980
orbital inclination
84.73
M sin i
0.927
right ascension component of proper motion
5.936
declination component of proper motion
-48.279
argument of periapsis
267
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Contents
  • See also
  • References
  • External links

WASP-2b is an extrasolar planet orbiting the star WASP-2 located about 500 light years away in the constellation of Delphinus. It was discovered via the transit method, and then follow up measurements using the radial velocity method confirmed that WASP-2b was a planet. 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-2b is located very close to its star, and belongs to the class of planets known as hot Jupiters. A 2008 study concluded that the WASP-2b system (among others) is a binary star system allowing even more accurate determination of stellar and planetary parameters.

==See also== HD 209458 b WASP-1b SuperWASP

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