Q87249722
star in the constellation Cepheus
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Q87249722
Summary
Q87249722 is a star[1].
Key Facts
- Q87249722's instance of is recorded as star[2].
- Q87249722's constellation is recorded as Cepheus[3].
- Q87249722's spectral class is recorded as K0[4].
- Q87249722's catalog code is recorded as 2MASS J00180174+8013108[5].
- Q87249722's catalog code is recorded as AG+79 6[6].
- Q87249722's catalog code is recorded as BD+79 4[7].
- Q87249722's catalog code is recorded as GSC 04500-00867[8].
- Q87249722's catalog code is recorded as PPM 54[9].
- Q87249722's catalog code is recorded as SAO 4077[10].
- Q87249722's catalog code is recorded as TYC 4500-867-1[11].
- Q87249722's catalog code is recorded as Gaia DR1 565088744056400640[12].
- Q87249722's catalog code is recorded as Gaia DR2 565088744056400640[13].
- Q87249722's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.88'}[14].
- Q87249722's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.221'}[15].
- Q87249722's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.739'}[16].
- Q87249722's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.648'}[17].
- Q87249722's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.84'}[18].
- Q87249722's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6381'}[19].
- Q87249722's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.0857'}[20].
- Q87249722's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+9.95'}[21].
- Q87249722's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+164.3196'}[22].
- Q87249722's SIMBAD ID is recorded as BD+79 4[23].
- Q87249722's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+4.50741260141850'}[24].
- Q87249722's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+80.21967119960060'}[25].
- Q87249722's epoch is recorded as J2000.0[26].