HAT-P-24
Sign in to saveHAT-P-24 is an F8 dwarf star about 413 parsecs away. A planet was discovered with the transit method by the HATNet Project in 2010. HAT-P-24b, is a typical hot Jupiter orbiting in only 3 days.
Wikidata facts
- Instance of
- eclipsing binary star
- Constellation
- Gemini
- Child body
- HAT-P-24 b
- Distance from Earth
- 405
- Diameter
- 1750000
- Radius
- 1.317
- Mass
- 1.191
- Variable-star type
- eclipsing binary star
Show 16 more facts
- catalog code
- HAT-P-24
- epoch
- J2000.0
- stellar rotational velocity
- 11.4
- luminosity
- 2.8472667
- right ascension component of proper motion
- 8.193
- metallicity
- -0.232
- declination component of proper motion
- -1.595
- right ascension
- 108.8250806903
- declination
- 14.26261334028
- surface gravity
- 19953
- radial velocity
- -1.19
- parallax
- 2.4202
- spectral class
- F8IV-V
- effective temperature
- 6373
- apparent magnitude
- 10.543
- age estimated by a dating method
- 2.8
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Encyclopedic overview
3 sectionsContents
- Planetary system
- References
- External links
HAT-P-24 is an F8 dwarf star about 413 parsecs away. A planet was discovered with the transit method by the HATNet Project in 2010. HAT-P-24b, is a typical hot Jupiter orbiting in only 3 days.
==Planetary system== In 2010 the HATNet Project announced the discovery of a hot jupiter type gas giant extrasolar planet in orbit around this star. Following the designation scheme used by the HATNet Project, the star is designated as HAT-P-24, and the planet itself HAT-P-24b.
Excerpted from Wikipedia’s “HAT-P-24” article, available under the CC BY-SA 4.0 licence.