Kepler-24
Sign in to savethumb | right | alt=Comparative sizes of Sun and Kepler-24. | Comparative sizes of Sun and Kepler-24. Kepler-24 is a star in the northern constellation of Lyra. It is located at the celestial coordinates: Right Ascension , Declination . With an apparent visual magnitude of 15.5, this star is too faint to be seen with the naked eye.
In the Vinony graph
Vinony's link graph records 192 inbound references to Kepler-24, and connects out to list of multiplanetary systems, star and Lyra.
Vinony files it under G-type main-sequence stars, Kepler-24 and Kepler objects of interest.
Vinony links it to 9 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- Er*
- Distance
- 3,924 light-years
- Redshift
- z = 0.00001845510420839247
- Coordinates
- RA 290.4133° · Dec 38.3437°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Instance of
- rotating variable star
- Constellation
- Lyra
- Distance from Earth
- 1195.99
- Diameter
- 2370000
- Radius
- 1.29
- Mass
- 1.03
- Variable-star type
- rotating variable star
- Image
- Kepler-24.jpg
Show 15 more facts
- Commons category
- Kepler-24
- parallax
- 0.8361
- catalog code
- KIC 3231341
- effective temperature
- 5897
- surface gravity
- 24500
- apparent magnitude
- 14.787
- epoch
- J2000.0
- stellar rotational velocity
- 4.3
- metallicity
- -0.02
- luminosity
- 1.1846913
- right ascension component of proper motion
- -2.153
- declination component of proper motion
- -1.822
- right ascension
- 290.41327389827
- declination
- 38.34373616450001
- radial velocity
- 3
Sources (1)
via Wikidata · CC0
~1 min read
Encyclopedic overview
2 sectionsContents
- Planetary system
- References
thumb | right | alt=Comparative sizes of Sun and Kepler-24. | Comparative sizes of Sun and Kepler-24. Kepler-24 is a star in the northern constellation of Lyra. It is located at the celestial coordinates: Right Ascension , Declination . With an apparent visual magnitude of 15.5, this star is too faint to be seen with the naked eye.
==Planetary system== Two planetary candidates b and c were discovered in 2011, and were confirmed in 2012 together with d and e.
Excerpted from Wikipedia’s “Kepler-24” article, available under the CC BY-SA 4.0 licence.
Available in 9 languages
via Wikidata sitelinks · CC0