Q90958275
high proper-motion star in the constellation Eridanus
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Q90958275
Summary
Q90958275 is a high proper-motion star[1].
Key Facts
- Q90958275's instance of is recorded as high proper-motion star[2].
- Q90958275's constellation is recorded as Eridanus[3].
- Q90958275's spectral class is recorded as G6V[4].
- Q90958275's catalog code is recorded as 2MASS J04301481-1747250[5].
- Q90958275's catalog code is recorded as BD-18 853[6].
- Q90958275's catalog code is recorded as CCDM J04302-1747AB[7].
- Q90958275's catalog code is recorded as GSC 05894-00089[8].
- Q90958275's catalog code is recorded as HD 28637[9].
- Q90958275's catalog code is recorded as IDS 04258-1800 AB[10].
- Q90958275's catalog code is recorded as PPM 214420[11].
- Q90958275's catalog code is recorded as SAO 149684[12].
- Q90958275's catalog code is recorded as TYC 5894-89-1[13].
- Q90958275's catalog code is recorded as YZ 0 6168[14].
- Q90958275's catalog code is recorded as YZ 107 1234[15].
- Q90958275's catalog code is recorded as WDS J04302-1747AB[16].
- Q90958275's catalog code is recorded as Gaia DR2 3170985216611124992[17].
- Q90958275's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.23'}[18].
- Q90958275's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.94'}[19].
- Q90958275's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.042'}[20].
- Q90958275's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.774'}[21].
- Q90958275's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.672'}[22].
- Q90958275's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0587'}[23].
- Q90958275's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.2847'}[24].
- Q90958275's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-28.43'}[25].
- Q90958275's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+107.7041'}[26].
Body
Definition and Type
Q90958275's instance of is recorded as high proper-motion star[2].