Clever Geek Handbook
📜 ⬆️ ⬇️

Kepler-20 d

Kepler-20 d (KOI-70 c, KIC 6850504 s, 2MASS J19104752 + 4220194 s [2] ) is one of the five exoplanets of the star Kepler-20 in the constellation Lyra. [3] [4] The exoplanet belongs to the class of Hot Neptunes with an estimated surface temperature of 369 Kelvin.

Kepler-20 d
Exoplanet
Parent star
StarKepler-20 (KOI-070)
ConstellationLyra
Right Ascension ( α )19 h 10 m 47.524 s
Declination ( δ )+ 42 ° 20 ′ 19.30 ″
Visible magnitude ( m V )12.51
Distance945 St. years old
( 290 ± 30 pc )
Spectral classG8
Weight ( m )0.912 ± 0.035 M ☉
Radius ( r )0.944 +0.06
−0.095 R ☉
Temperature ( T )5,466 ± 93 K
Metallicity ([Fe / H])0.02 ± 0.04
Age8.8 +4.7
−2.7 billion years
Elements of the orbit
Semimajor axis ( a )0.3453 a. e.
Eccentricity ( e )<0.60
Orbital Period ( P )77.61184 d.
Inclination ( i )89.570 °
physical characteristics
Weight ( m )<20.1 M ⊕
Radius ( r )2.75 +0.17
−0.30 R ⊕
Density ( ρ )<4.07 g / cm 3
Temperature ( T )369 K
Discovery Information
opening dateDecember 20, 2011
Detection methodTransit
Opening placeKepler telescope
Opening statusPublished [1]
Other designations
KOI-70 d, KIC 6850504 d, 2MASS J19104752 + 4220194 d [2]

The existence of this exoplanet was announced on December 20, 2011 . [1] [4]

Content

Native Star

The star Kepler-20, also known as GSC 03129-01902, belongs to the stars of the spectral class G8. The star is located 945 light-years from Earth in the constellation Lyra. At least five planets revolve around the star, two of which are comparable in size to the Earth [3] [4]

The star in its characteristics resembles our Sun. Its mass and radius are 91% and 94% of the solar, respectively. The surface temperature is about 5466 Kelvin , which is comparable to the temperature of our daylight. The luminosity of a star is 85% of the sun. The star was named Kepler-20 , because it was discovered using planetary telescope Kepler planetary companions. [3] [4]

See also

  • Kepler-20
  • List of exoplanets discovered in 2011
  • List of exoplanets discovered by the Kepler telescope
  • Kepler (telescope)

Notes

  1. ↑ 1 2 1201.5424v1, 2012 .
  2. ↑ 1 2 NASA Exoplanet Archive .
  3. ↑ 1 2 3 1112.4514v2, 2012 .
  4. ↑ 1 2 3 4 1102.0541v2, 2011 .

Literature

  • Michael Perryman Part 6. Transits // The Exoplanet Handbook . - Cambridge University Press , 2011 .-- pp. 103-114. - 424 p. - ISBN 9780521765596 . Archived July 21, 2013 to Wayback Machine

Articles

  • Thomas N. Gautier III et all. Kepler-20: A Sun-like Star with Three Sub-Neptune Exoplanets and Two Earth-size Candidates . - 2012. - arXiv : 1112.4514v2 .
  • William J. Borucki. Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data . - 2011 .-- arXiv : 1102.0541v2 .
  • Stephen R. Kane, Dawn M. Gelino. Decoupling Phase Variations in Multi-Planet Systems (Eng.) // The Astrophysical Journal . - 2012. - arXiv : 1211.6747v1 .
  • Jack J. Lissauer. Almost All of Kepler's Multiple Planet Candidates are Planets . - 2012. - arXiv : 1201.5424v1 .

Links

  • NASA's Kepler announces 11 planetary systems hosting 26 planets Ames Research Center. Archived July 10, 2013.

Directories

  • Kepler-20 d (English) . exoplanets.org. Archived July 10, 2013.
  • Kepler-20 d (English) (inaccessible link) . Open Exoplanet Catalog. Archived July 10, 2013.
  • Kepler-20 d (English) . Ames Research Center. Archived July 10, 2013.
  • Kepler-20 d (English) . NASA Exoplanet Archive. Archived July 10, 2013.
  • Kepler-20 d (English) . SIMBAD Archived July 10, 2013.

  19 h 10 m 47.52 s , + 42 ° 20 ′ 19.4 ″

Source - https://ru.wikipedia.org/w/index.php?title=Kepler-20_d&oldid=100954349


More articles:

  • Strikili
  • Kurbune, Jürgen
  • Pasarell, Charlie
  • Russian Bryzgovo
  • Rheology
  • Karl Friedrich August Mecklenburg-Strelitz
  • Shefcovic, Maroš
  • Terry Mills
  • Smith, Bruce
  • Clemens Brummer

All articles

Clever Geek | 2019