Kepler-1649

Kepler-1649 is a red dwarf star of spectral type M5V with a radius 0.232 R, a mass 0.198 M, and a metallicity of -0.15 [Fe/H].[3][4]

Kepler-1649

Artist's impression of exoplanet Kepler-1649c with its host star in the background.
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cygnus[1]
Right ascension 19h 30m 00.9006122986s[2]
Declination 41° 49 49.513849537[2]
Characteristics
Evolutionary stage Main sequence red dwarf
Spectral type M5V[3]
Apparent magnitude (B) 19.1[2]
Apparent magnitude (R) 16.6[2]
Apparent magnitude (J) 13.379±0.023[2]
Apparent magnitude (H) 12.852±0.020[2]
Apparent magnitude (K) 12.589±0.026[2]
Astrometry
Proper motion (μ) RA: -135.842[2] mas/yr
Dec.: -99.232[2] mas/yr
Parallax (π)10.8187 ± 0.0637[2] mas
Distance301 ± 2 ly
(92.4 ± 0.5 pc)
Details[4]
Mass0.1977±0.0051 M
Radius0.2317±0.0049 R
Surface gravity (log g)5.004±0.021 cgs
Temperature3240±61 K
Metallicity [Fe/H]−0.15±0.11 dex
Other designations
Kepler-1649, KOI-3138, KIC 6444896, 2MASS J19300092+4149496[2]
Database references
SIMBADdata
Exoplanet Archivedata

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, with the 5th highest ESI as of December 2020.[5][6]

The Kepler-1649 planetary system[4]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.0514±0.0028 8.689099±0.000025 89.150+0.110
−0.079
°
1.017±0.051 R
c 19.53527±0.00010 89.339±0.056° 1.06+0.15
−0.10
 R

References


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