K2-155d
K2-155d is a potentially habitable Super-Earth exoplanet in the K2-155 system. It is the outermost of three known planets orbiting around the K-type star K2-155 in the constellation Taurus. It is one of 15 new exoplanets around red dwarf stars discovered by Japanese astronomer Teruyuki Hirano of the Tokyo Institute of Technology and his team. The team used data from NASA's Kepler Space Telescope during its extended K2 "Second Light" mission. K2-155d orbits near the so-called habitable zone of its system, and has the potential to host liquid water.
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K2-155d
K2-155d is a potentially habitable Super-Earth exoplanet in the K2-155 system. It is the outermost of three known planets orbiting around the K-type star K2-155 in the constellation Taurus. It is one of 15 new exoplanets around red dwarf stars discovered by Japanese astronomer Teruyuki Hirano of the Tokyo Institute of Technology and his team. The team used data from NASA's Kepler Space Telescope during its extended K2 "Second Light" mission. K2-155d orbits near the so-called habitable zone of its system, and has the potential to host liquid water.
orbital period (μ)
temperature (K)
has abstract
K2-155d is a potentially habit ...... otential to host liquid water.
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Method of discovery
Transit method
orbital period (s)
3.5150544e+6
temperature (K)
Wikipage page ID
56,902,153
page length (characters) of wiki page
Wikipage revision ID
1,000,603,198
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apsis
astron
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discovered
March 2018
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discoverer
Teruyuki Hirano
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discovery method
discovery site
eccentricity
unknown
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inclination
unknown
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Mean radius
name
-1.3392E7
period
3515054.4000000004
semimajor
star
label
K2-155d
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name
K2-155d
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wikiPageUsesTemplate
subject
comment
K2-155d is a potentially habit ...... otential to host liquid water.
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