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Kepler-160

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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.

In the Vinony graph

Vinony's link graph records 207 inbound references to Kepler-160, and connects out to list of multiplanetary systems, year and Kepler Space Telescope.

It is catalogued under topics including G-type subgiants, Kepler objects of interest and Lyra.

Vinony links it to 13 Wikipedia language editions.

Wikidata facts

Constellation
Lyra
Distance from Earth
962.92
Diameter
1450000
Radius
1.12
Variable-star type
rotating variable star
Show 15 more facts
effective temperature
5471
surface gravity
25000
parallax
1.0644
epoch
J2000.0
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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Encyclopedic overview

4 sections
Contents
  • 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.

Excerpted from Wikipedia’s “Kepler-160” article, available under the CC BY-SA 4.0 licence.

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