Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lyra |
Right ascension | 18h 56m 14.30760s[1] |
Declination | +44° 31′ 05.3896″[1] |
Apparent magnitude (V) | 9.710[2] |
Characteristics | |
Spectral type | G8V |
Astrometry | |
Radial velocity (Rv) | −30.92±0.20[1] km/s |
Proper motion (μ) | RA: −60.396 mas/yr[1] Dec.: 48.657 mas/yr[1] |
Parallax (π) | 15.6253 ± 0.0105 mas[1] |
Distance | 208.7 ± 0.1 ly (64.00 ± 0.04 pc) |
Details | |
Mass | 0.79+0.033 −0.03[3] M☉ |
Radius | 0.789+0.0064 −0.0056[3] R☉ |
Temperature | 5357±68[3] K |
Metallicity [Fe/H] | −0.36±0.05[3] dex |
Rotational velocity (v sin i) | 1.1 (± 1.1)[4] km/s |
Age | 7.6+3.4 −3.1[3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
KIC | data |
Kepler-37, also known as UGA-1785,[6][7][8] is a G-type main-sequence star located in the constellation Lyra 209 light-years (64 parsecs) from Earth. It is host to exoplanets Kepler-37b, Kepler-37c, Kepler-37d and possibly Kepler-37e, all of which orbit very close to it. Kepler-37 has a mass about 80.3 percent of the Sun's and a radius about 77 percent as large.[4] It has a temperature similar to that of the Sun, but a bit cooler at 5,357 K. It has about half the metallicity of the Sun. With an age of roughly 6 billion years,[9] it is slightly older than the Sun, but is still a main-sequence star. Until January 2015, Kepler-37 was the smallest star to be measured via asteroseismology.[10]
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