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Star · G7V

Kepler-37

Kepler-37 is a main-sequence star of spectral type G7V in the constellation Lyra, 208.7 light-years from the Sun. It is orbited by 4 confirmed exoplanet(s).

ConstellationLyra
Distance208.7 light-years (64.0 pc)
Apparent magnitudemagnitude 9.85
Absolute magnitudemagnitude 5.82
Spectral typeG7V
Surface temperature5,360 K
Luminosity0.477 L☉
Radius0.789 R☉
Mass0.79 M☉
Age7.6 billion years
Metallicity [Fe/H]-0.36
Right ascension (J2000)18h 56m 14.3s
Declination (J2000)+44° 31′ 05″
Space velocity (relative to the Sun)38.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.85. Visible from the whole Northern Hemisphere and south to latitude 45° S. North of latitude 45° N it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1817. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.7 million years.

The Sun seen from there

From a planet around Kepler-37, the Sun would look like a star of magnitude 8.86, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.

Planets

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

  • HIP 92291 10.4 light-years
  • HIP 92714 14.6 light-years
  • Kepler-1651 16.2 light-years
  • HIP 90813 17.7 light-years
  • HIP 92269 18.5 light-years

Open in the simulation

Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.