Q93818579
star in the constellation Cetus
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Q93818579
Summary
Q93818579 is a star[1].
Key Facts
- Q93818579's instance of is recorded as star[2].
- Q93818579's constellation is recorded as Cetus[3].
- Q93818579's spectral class is recorded as K5[4].
- Q93818579's catalog code is recorded as BD-15 63[5].
- Q93818579's catalog code is recorded as GSC 05268-00929[6].
- Q93818579's catalog code is recorded as PPM 208762[7].
- Q93818579's catalog code is recorded as SAO 147256[8].
- Q93818579's catalog code is recorded as TYC 5268-929-1[9].
- Q93818579's catalog code is recorded as YZ 105 108[10].
- Q93818579's catalog code is recorded as Gaia DR1 2374829117519446400[11].
- Q93818579's catalog code is recorded as Gaia DR2 2374829121815423104[12].
- Q93818579's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.10'}[13].
- Q93818579's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.95'}[14].
- Q93818579's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.8396'}[15].
- Q93818579's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.5893'}[16].
- Q93818579's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-32.31'}[17].
- Q93818579's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+278.6059'}[18].
- Q93818579's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+6.19449990098730'}[19].
- Q93818579's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-14.73339682507850'}[20].
- Q93818579's epoch is recorded as J2000.0[21].
- Q93818579's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.483'}[22].
- Q93818579's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.346'}[23].
Body
Definition and Type
Q93818579's instance of is recorded as star[2].