HD 39194
Three confirmed super-Earths orbit this old, inactive K-dwarf star.
Last updated
HD 39194 is a K-type main-sequence star in the southern constellation Mensa, visible in binoculars. It hosts three confirmed super-Earths in eccentric orbits, none within the habitable zone.
Quick Facts
- Apparent magnitude
- 8.07
- Distance
- 86 light years
- Mass
- 71% of the Sun
- Luminosity
- 38% of the Sun
- Iron abundance
- 24% of the Sun
Facts from the source article.
More in Planetary Systems with Three Confirmed Planets
Sources
Compiled from Wikipedia and the sources listed below. Text from Wikipedia is available under CC BY-SA 4.0; this entry is adapted from it.
- Wikipedia: HD 39194 (CC BY-SA 4.0).
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