Kepler-186b

from Wikipedia, the free encyclopedia
Exoplanet
Kepler-186b

Simulation of the Kepler-186 system, the innermost planet is Kepler-186b.

Simulation of the Kepler-186 system, the innermost planet is Kepler-186b.
Constellation swan
Position
equinox : J2000.0
Right ascension 19h 54m 36.65s
declination + 43 ° 57 ′ 18.1 ″
Orbit data
Central star Kepler-186
Major semi-axis 0.0343 ± 0.0046 AU
Period of circulation 3.8867907  +0.0000062−0.0000063 d
Further data
radius 1.07 ± 0.12 R
distance 151 ± 18 pc
history
Date of discovery 2014
Catalog names
KOI-571.01, Kepler-186 b, KOI-571 b, K00571.01, 2MASS J19543665 + 4357180 b, KIC 8120608 b, WISE J195436.65 + 435717.9 b

Kepler-186b is an exoplanet orbiting the red dwarf Kepler-186 . The planet was discovered in 2014 by the Kepler space telescope.

Parent star

The parent star Kepler-186 is very faint, but also very active. It is a so-called flare star that tends to have strong prominences . The system is about 500 light years from Earth .

Location in the system

The planet is very close to its star in the star system and is the innermost planet of the star system. It is clearly not in the habitable zone , as it would be much too hot on the planet. It takes Kepler-186b less than four days to orbit its parent star.

Individual evidence

  1. ^ A b Elisa V. Quintana, Thomas Barclay, Jason F. Rowe [u. a.]: An Earth-Sized Planet in the Habitable Zone of a Cool Star . In: Science . April 18, 2014, Vol. 344, No. 6181, pp. 277–280, DOI: 10.1126 / science.1249403 .
  2. a b c NASA Exoplanet Archives: Kepler-186. Retrieved May 6, 2015 .