Q24049348
Sign in to save| eccentricity = ~0 | period = 86.829 d | inclination = ~89.5 | star = Kepler-1229 (KOI-2418) | mean_radius = | mass = ~2.7 | single_temperature =
Key facts
- Planet.name
- Kelper Circular
- Planet.caption
- An artistic simulation of the potentially habitable exoplanet Kepler-1229b, with its star (center). The Milky Way can be seen in the background.
- Planet.discoverer
- Kepler spacecraft
- Planet.discovered
- May 12, 2016
- Planet.discovery_method
- transit
- Planet.apsis
- astron
- Planet.semimajor
- {{#tag:ref|Kepler's Third Law, assuming a circular orbit: \begin{smallmatrix}\frac{4 \pi^2}{T^2} = \frac{G M}{R^3}\end{smallmatrix} Mass and the period are known, so the equation can be written with semimajor axis as the subject: \begin{smallmatrix}R = \sqrt[3]{\frac{GMT^2}{4\pi^2}}\end{smallmatrix}.
- Planet.group
- "nb"
via Wikipedia infobox
~5 min read
Encyclopedic overview
9 sectionsContents
- Physical characteristics
- Mass, radius and temperature
- Host star
- Orbit
- Habitability
- Discovery and follow-up studies
- See also
- Notes
- References
{{Infobox planet | name = Kepler-1229b | image = | caption = An artistic simulation of the potentially habitable exoplanet Kepler-1229b, with its star (center). The Milky Way can be seen in the background.
| discoverer = Kepler spacecraft | discovered = May 12, 2016 | discovery_method = transit
Excerpted from Wikipedia’s “Q24049348” article, available under the CC BY-SA 4.0 licence.