HAT-P-24 b
Sign in to saveHAT-P-24b is an extrasolar planet discovered by the HATNet Project in 2010 orbiting the F8 dwarf star HAT-P-24. It is a hot Jupiter, with a mass three quarters that of Jupiter and a radius 20% larger.
Astronomical data · SIMBAD
- Object type
- Pl
- Distance
- 1,348 light-years
- Coordinates
- RA 108.8251° · Dec 14.2626°
via SIMBAD · CDS Strasbourg
Exoplanet data
- Host star
- HAT-P-24
- Discovered
- 2010
- Discovered by
- HATNet
- Orbital period
- 3.36 days
- Radius
- 14.57 × Earth
- Mass
- 238.37 × Earth
- Equilibrium temp
- 1637 K
- Distance
- 415.34 pc
via NASA Exoplanet Archive
Wikidata facts
- Constellation
- Gemini
- Parent body
- HAT-P-24
- Radius
- 1.3
- Mass
- 0.75
- Orbital period
- 3.35524439
- Image
- Exoplanet Comparison HAT-P-24 b.png
Show 15 more facts
- catalog code
- TIC 440777904b
- time of discovery or invention
- 2010-12-00
- Commons category
- HAT-P-24 b
- right ascension
- 108.82508088479875
- declination
- 14.26261379265194
- epoch
- J2000.0
- argument of periapsis
- 197
- orbital inclination
- 90
- orbital eccentricity
- 0.07
- discovery method
- transit method
- angular distance
- 0.000152
- right ascension component of proper motion
- 8.152
- declination component of proper motion
- -1.716
- semi-major axis of an orbit
- 0.0465
- parallax
- 2.3795
via Wikidata · CC0
~1 min read
Encyclopedic overview
2 sectionsContents
- References
- External links
HAT-P-24b is an extrasolar planet discovered by the HATNet Project in 2010 orbiting the F8 dwarf star HAT-P-24. It is a hot Jupiter, with a mass three quarters that of Jupiter and a radius 20% larger.
The study in 2012, utilizing a Rossiter–McLaughlin effect, have determined the planetary orbit is probably aligned with the equatorial plane of the star, misalignment equal to 20°.
Excerpted from Wikipedia’s “HAT-P-24 b” article, available under the CC BY-SA 4.0 licence.