Misplaced Pages

Kepler-37: Difference between revisions

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Browse history interactively← Previous editNext edit →Content deleted Content addedVisualWikitext
Revision as of 21:26, 20 February 2013 editMichał Rosa (talk | contribs)104 editsm pl:Kepler-37Tag: Addition of interwiki link← Previous edit Revision as of 22:22, 20 February 2013 edit undoAlphachimera (talk | contribs)239 editsm bad sourceNext edit →
Line 13: Line 13:
Kepler-37c is similar in size to ]. Kepler-37c is similar in size to ].


Kepler-37d is about three times the size of Earth and was the first exoplanet discovered to be "unquestionably rocky." Kepler-37d is about three times the size of Earth.


==References== ==References==
Line 20: Line 20:
* Bad Astronomy, * Bad Astronomy,
* NASA, * NASA,
* WIRED,
* *



Revision as of 22:22, 20 February 2013

Kepler-37
Diagram showing star positions and boundaries of the constellation and its surroundingsLocation of Kepler-37 in (circled)

Kepler-37 is a star in the constellation Lyra that is host to exoplanets Kepler-37b, Kepler-37c and Kepler-37d.

Planetary system

Kepler-37b is the smallest known exoplanet, at 3865 kilometers in diameter, as of February 2013. It orbits Kepler-37 once every 13 days and is too small and too close to its star to maintain an atmosphere.

Kepler-37c is similar in size to Venus.

Kepler-37d is about three times the size of Earth.

References

  • Nature,
  • Bad Astronomy,
  • NASA,
  • JPL

See also

Stub icon

This extrasolar-planet-related article is a stub. You can help Misplaced Pages by expanding it.

Stub icon

This star-related article is a stub. You can help Misplaced Pages by expanding it.

Categories: