Kepler-174
Kepler-174 is a K-type main-sequence star located in the Milky Way Galaxy at a distance of 1269.0 light-years (389.1 parsecs) away from the Sun. It is located inside the boundaries of the Lyra constellation, but it is too dim to be visible to the unaided eye and is not part of the main outline.
Planetary System
Kepler-174 has three confirmed Super-Earth planets orbiting it, Kepler-174b, Kepler-174c and Kepler-174d. Kepler-174d is notable as it is within the star's habitable zone, meaning it is potentially habitable.[1][2]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 4.5 M🜨 | — | 14 | 0 | — | 1.96 R🜨 |
| c | 2.83 M🜨 | — | 33.4 | 0 | — | 1.49 R🜨 |
| d | 5.43 M🜨 | — | 247.4 | 0 | — | 2.19 R🜨 |
References
- "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System.
- "Kepler's Tally of Planets". www.nytimes.com.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.