Q92175326
star in the constellation Perseus
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Q92175326
Summary
Q92175326 is a star[1].
Key Facts
- Q92175326's instance of is recorded as star[2].
- Q92175326's constellation is recorded as Perseus[3].
- Q92175326's spectral class is recorded as G0[4].
- Q92175326's catalog code is recorded as 2MASS J03364206+3656102[5].
- Q92175326's catalog code is recorded as AG+36 361[6].
- Q92175326's catalog code is recorded as BD+36 729[7].
- Q92175326's catalog code is recorded as GSC 02367-01723[8].
- Q92175326's catalog code is recorded as HD 278779[9].
- Q92175326's catalog code is recorded as PPM 68624[10].
- Q92175326's catalog code is recorded as SAO 56578[11].
- Q92175326's catalog code is recorded as TYC 2367-1723-1[12].
- Q92175326's catalog code is recorded as Gaia DR2 222534182732093440[13].
- Q92175326's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.51'}[14].
- Q92175326's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.180'}[15].
- Q92175326's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.883'}[16].
- Q92175326's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.780'}[17].
- Q92175326's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.14'}[18].
- Q92175326's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.3042'}[19].
- Q92175326's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.8033'}[20].
- Q92175326's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-26.45'}[21].
- Q92175326's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+208.1902'}[22].
- Q92175326's SIMBAD ID is recorded as HD 278779[23].
- Q92175326's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+54.17527383068900'}[24].
- Q92175326's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+36.93615724019760'}[25].
- Q92175326's epoch is recorded as J2000.0[26].