Misplaced Pages

Kepler-438b: 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 11:38, 8 January 2015 editArtman40 (talk | contribs)2,039 editsNo edit summary← Previous edit Revision as of 17:03, 8 January 2015 edit undoDrbogdan (talk | contribs)Autopatrolled, Extended confirmed users, Pending changes reviewers, Rollbackers90,408 edits External links: added relevant data links - re NASA Exoplanet Archive & Extrasolar Planets Encyclopaedia.Next edit →
Line 77: Line 77:
== External links == == External links ==
{{Commons category|Kepler Mission}} {{Commons category|Kepler Mission}}
*. * .
*. * .
* at ].
* at ].
{{portal bar|Astrobiology|Astronomy}} {{portal bar|Astrobiology|Astronomy}}
{{Sky|18|46|35.000|+|41|57|03.93}} {{Sky|18|46|35.000|+|41|57|03.93}}

Revision as of 17:03, 8 January 2015

Template:Planetbox begin Template:Planetbox image Template:Planetbox star Template:Planetbox character Template:Planetbox orbit Template:Planetbox discovery Template:Planetbox catalog Template:Planetbox end Kepler-438b (also known by its Kepler Object of Interest designation KOI-3284.01) is a confirmed near-Earth-sized exoplanet, likely rocky, orbiting within the habitable zone of a sun-like star Kepler-438, about 470 light-years (145 pc) from the Earth in the constellation Lyra. The planet was discovered by NASA's Kepler spacecraft using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. NASA announced the discovery of the exoplanet on 6 January 2015.

Confirmed exoplanet

Kepler-438b, a near-Earth-sized exoplanet, has a radius 1.12 times that of Earth. The planet orbits a sun-like star, named Kepler-438, once every 35.2 days.

Habitability

The planet was announced as being located within the star's "habitable zone", a region where liquid water could exist on the surface of the planet. It was described as being one of the most Earth-like planets, in terms of size and temperature, yet found.

See also

References

  1. ^ Cite error: The named reference NASA-20150106 was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference TG-20150107-IS was invoked but never defined (see the help page).

External links

Portal:
Exoplanets
Main topics
Sizes
and
types
Terrestrial
Gaseous
Other types
Formation
and
evolution
Systems
Host stars
Detection
Habitability
Catalogues
Lists
Other
Astrobiology
Disciplines
Main topics
Planetary
habitability
Space
missions
Earth orbit
Mars
Comets and
asteroids
Heliocentric
Planned
Proposed
Cancelled and
undeveloped
Institutions
and programs
Extraterrestrial life
Events and objects
Signals of interest
Misidentified
Stars
Other
Life in the Universe
Planetary
habitability
Space missions
Interstellar
communication
Types of alleged
extraterrestrial beings
Hypotheses
Fermi paradox solutions
Related topics
2015 in space
Space probe launches Space probes launched in 2015
Space probes
Space observatories
  • DSCOVR (weather satellite; Feb 2015)
  • Astrosat (space telescope; Sep 2015)


Impact events
Selected NEOs
Exoplanets Exoplanets discovered in 2015
Discoveries
Comets Comets in 2015
Space exploration
Categories: