Q87785686
star in the constellation Perseus
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Q87785686
Summary
Q87785686 is a star[1].
Key Facts
- Q87785686's instance of is recorded as star[2].
- Q87785686's constellation is recorded as Perseus[3].
- Q87785686's spectral class is recorded as F8[4].
- Q87785686's catalog code is recorded as 2MASS J03305751+3709044[5].
- Q87785686's catalog code is recorded as AG+36 353[6].
- Q87785686's catalog code is recorded as BD+36 699[7].
- Q87785686's catalog code is recorded as GSC 02354-01301[8].
- Q87785686's catalog code is recorded as HD 278697[9].
- Q87785686's catalog code is recorded as PPM 68526[10].
- Q87785686's catalog code is recorded as SAO 56503[11].
- Q87785686's catalog code is recorded as TYC 2354-1301-1[12].
- Q87785686's catalog code is recorded as Gaia DR2 222681792167925888[13].
- Q87785686's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.82'}[14].
- Q87785686's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.485'}[15].
- Q87785686's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.132'}[16].
- Q87785686's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.105'}[17].
- Q87785686's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.55'}[18].
- Q87785686's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.6220'}[19].
- Q87785686's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.5104'}[20].
- Q87785686's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+18.03'}[21].
- Q87785686's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+153.6004'}[22].
- Q87785686's SIMBAD ID is recorded as HD 278697[23].
- Q87785686's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+52.73966635744160'}[24].
- Q87785686's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.15124591316860'}[25].
- Q87785686's epoch is recorded as J2000.0[26].