WASP-95
Sign in to saveWASP-95 is a star away in the constellation Grus. With an apparent magnitude of 10.1, it is not visible to the naked eye. Its spectral type of G2 means it is a yellow sunlike star.
In the Vinony graph
Within Vinony's link graph, WASP-95 is referenced by 77 other articles, and connects out to year, Durchmusterung and star.
It is catalogued under topics including Durchmusterung objects, Grus (constellation) and G-type main-sequence stars.
Its subject is documented across 6 Wikipedia language editions.
Wikidata facts
- Instance of
- eclipsing binary star
- Constellation
- Grus
- Distance from Earth
- 138.087
- Radius
- 1.13
- Mass
- 1.11
- Variable-star type
- eclipsing binary star
Show 15 more facts
- radial velocity
- 6.37
- apparent magnitude
- 9.940329
- parallax
- 7.2379
- epoch
- J2000.0
- catalog code
- TOI-105
- surface gravity
- 21400
- spectral class
- G2
- effective temperature
- 5630
- luminosity
- 1.5059582
- right ascension component of proper motion
- 92.151
- declination component of proper motion
- -6.905
- metallicity
- 0.3
- right ascension
- 337.45723129495
- declination
- -48.00306907894
- age estimated by a dating method
- 2.4
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Encyclopedic overview
2 sectionsContents
- Planetary system
- References
WASP-95 is a star away in the constellation Grus. With an apparent magnitude of 10.1, it is not visible to the naked eye. Its spectral type of G2 means it is a yellow sunlike star.
==Planetary system== In 2013, a planet was discovered around WASP-95. The planet, WASP-95b, is a hot Jupiter about 10% more massive than Jupiter, and completes an orbit round its star every two days. It was discovered by its transit of the star in 2013. The planet's equilibrium temperature is 1692.6 K.
Excerpted from Wikipedia’s “WASP-95” article, available under the CC BY-SA 4.0 licence.