Q89870165
Sign in to saveKepler-1649 is a red dwarf star of spectral type M5V with a radius , a mass , and a metallicity of -0.15 [Fe/H].
Wikidata facts
- Instance of
- rotating variable star
- Constellation
- Cygnus
- Distance from Earth
- 92.757
- Radius
- 0.23
- Mass
- 0.2
- Variable-star type
- rotating variable star
- Image
- PIA23690-Exoplanet-Kepler1649c-20200415.jpg
Show 12 more facts
- epoch
- J2000.0
- catalog code
- Gaia DR3 2125699062780742016
- right ascension component of proper motion
- -135.831
- parallax
- 10.7808
- apparent magnitude
- 16.243011
- effective temperature
- 3240
- declination component of proper motion
- -99.524
- spectral class
- M5V
- declination
- 41.83042176362001
- right ascension
- 292.5037525135
- metallicity
- -0.15
- Commons category
- Kepler-1649
via Wikidata · CC0
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Encyclopedic overview
2 sectionsContents
- Planetary system
- References
Kepler-1649 is a red dwarf star of spectral type M5V with a radius , a mass , and a metallicity of -0.15 [Fe/H].
==Planetary system== thumb|left|Artist's impression and size comparison of the two planets in the Kepler-1649 system with Earth Two confirmed planets orbit the star: Kepler-1649b and Kepler-1649c. Kepler-1649b is similar to Venus, whereas Kepler-1649c is a potentially habitable exoplanet similar to Earth.
Excerpted from Wikipedia’s “Q89870165” article, available under the CC BY-SA 4.0 licence.
Gallery (2)
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