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[[File:PIA23690-Exoplanet-Kepler1649c-20200415.jpg|thumb|Exoplanet Kepler-1649c with star at the background]]
Kepler-1649 is a red dwarf star of spectral type M5V with a radius 0.252 Sun radii, a mass 0.219 Solar masses, and a metallicity of -0.15 [Fe/H].<ref></ref>
Two confirmed planets orbit the star: [[Kepler-1647b|Kepler-1649 b]] and [[Kepler-1649c|Kepler-1649 c]]. Kepler-1649 b is similar to [[Venus]], whereas Kepler-1649 c is considered th 5th most potentially habitable exoplanet as of December 2020.<ref></ref><ref></ref>
== References ==
Kepler-1649 is a red dwarf star of spectral type M5V with a radius 0.252 Sun radii, a mass 0.219 Solar masses, and a metallicity of -0.15 [Fe/H].<ref></ref>
Two confirmed planets orbit the star: [[Kepler-1647b|Kepler-1649 b]] and [[Kepler-1649c|Kepler-1649 c]]. Kepler-1649 b is similar to [[Venus]], whereas Kepler-1649 c is considered th 5th most potentially habitable exoplanet as of December 2020.<ref></ref><ref></ref>
== References ==
from Wikipedia - New pages [en] https://ift.tt/2W4Ue3J
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