Q91665821
high proper-motion star in the constellation Cepheus
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Q91665821
Summary
Q91665821 is a high proper-motion star[1].
Key Facts
- Q91665821's instance of is recorded as high proper-motion star[2].
- Q91665821's instance of is recorded as astrophysical X-ray source[3].
- Q91665821's constellation is recorded as Cepheus[4].
- Q91665821's spectral class is recorded as K0[5].
- Q91665821's catalog code is recorded as 2MASS J02291316+7852285[6].
- Q91665821's catalog code is recorded as AG+78 50[7].
- Q91665821's catalog code is recorded as BD+78 85[8].
- Q91665821's catalog code is recorded as GSC 04503-00924[9].
- Q91665821's catalog code is recorded as HIC 11577[10].
- Q91665821's catalog code is recorded as HIP 11577[11].
- Q91665821's catalog code is recorded as PPM 5000[12].
- Q91665821's catalog code is recorded as SAO 4653[13].
- Q91665821's catalog code is recorded as TYC 4503-924-1[14].
- Q91665821's catalog code is recorded as Gaia DR1 561759869523423232[15].
- Q91665821's catalog code is recorded as Gaia DR2 561759873820746496[16].
- Q91665821's catalog code is recorded as 1RXS J022905.1+785157[17].
- Q91665821's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.45'}[18].
- Q91665821's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.980'}[19].
- Q91665821's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.592'}[20].
- Q91665821's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.505'}[21].
- Q91665821's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.29'}[22].
- Q91665821's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2516'}[23].
- Q91665821's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+14.6947'}[24].
- Q91665821's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-22.12'}[25].
- Q91665821's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+68.0517'}[26].
Body
Definition and Type
Recorded instance of include high proper-motion star[2] and astrophysical X-ray source[3].