Kepler-160
Sign in to saveKepler-160 is a G-type subgiant star approximately the width of our Galactic arm away in the constellation Lyra, first studied in detail by the Kepler Mission, a NASA-led operation tasked with discovering terrestrial planets. The star, which is very similar to the Sun in mass and radius, has three confirmed planets and one unconfirmed planet orbiting it.
Wikidata facts
- Distance from Earth
- 962.92
- Diameter
- 1450000
- Radius
- 1.12
Show 14 more facts
- effective temperature
- 5471
- surface gravity
- 25000
- parallax
- 1.0644
- metallicity
- 0.15
- apparent magnitude
- 14.688
- catalog code
- SPOCS 3679
- stellar rotational velocity
- 1.7
- luminosity
- 1.0084367
- declination component of proper motion
- -5.233
- right ascension component of proper motion
- 3.477
- right ascension
- 287.77355258164994
- declination
- 42.86929798738
- radial velocity
- -26.48
- spectral class
- G5
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Article
4 sectionsContents
- Characteristics
- Planetary system
- See also
- References
Kepler-160 is a G-type subgiant star approximately the width of our Galactic arm away in the constellation Lyra, first studied in detail by the Kepler Mission, a NASA-led operation tasked with discovering terrestrial planets. The star, which is very similar to the Sun in mass and radius, has three confirmed planets and one unconfirmed planet orbiting it.
== Characteristics == The star Kepler-160 is rather old, having no detectable circumstellar disk. The star's metallicity is unknown, with conflicting values of either 40% or 160% of solar metallicity reported.