KOI-204

звезда в созвездии Лебедя

In the Vinony graph

Within Vinony's link graph, KOI-204 is referenced by 307 other articles, and connects out to year, apparent magnitude and stellar rotation.

It sits within the topics Cygnus (constellation), G-type subgiants and Kepler objects of interest.

Its subject is documented across 7 Wikipedia language editions.

Astronomical data · SIMBAD

Object type: Er*
Distance: 3,741 light-years
Redshift: z = -0.00011857500582690417
Coordinates: RA 300.1024° · Dec 45.7622°

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via SIMBAD · CDS Strasbourg

Wikidata facts

Constellation: Cygnus
Distance from Earth: 1229.15
Radius: 1.35
Mass: 1.12
Variable-star type: rotating variable star

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catalog code: TIC 239277658
surface gravity: 14000
luminosity: 1.6339194
effective temperature: 5800
parallax: 0.8719
apparent magnitude: 14.781
epoch: J2000.0
metallicity: 0.15
right ascension component of proper motion: -0.956
declination component of proper motion: 8.241
spectral class: G2 IV
right ascension: 300.10235707385
declination: 45.76215627641999
radial velocity: -35.55
age estimated by a dating method: 5.8

Sources (1)

ru.wikipedia.org

via Wikidata · CC0

Article · Русский

KOI-204 (или Kepler-44) — звезда в созвездии Лебедя. Находится на расстоянии около 7338 световых лет от Солнца. Вокруг звезды обращается, как минимум, одна планета.

Abstract from DBpedia / Wikipedia · CC BY-SA