Q89302257
star in the constellation Leo
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Q89302257
Summary
Q89302257 is a star[1].
Key Facts
- Q89302257's instance of is recorded as star[2].
- Q89302257's constellation is recorded as Leo[3].
- Q89302257's spectral class is recorded as K0[4].
- Q89302257's catalog code is recorded as AG+27 1027[5].
- Q89302257's catalog code is recorded as BD+27 1805[6].
- Q89302257's catalog code is recorded as GSC 01963-00305[7].
- Q89302257's catalog code is recorded as PPM 99825[8].
- Q89302257's catalog code is recorded as SAO 80997[9].
- Q89302257's catalog code is recorded as TYC 1963-305-1[10].
- Q89302257's catalog code is recorded as YZ 27 5080[11].
- Q89302257's catalog code is recorded as 2MASS J09445793+2718399[12].
- Q89302257's catalog code is recorded as Gaia DR2 647955503762505472[13].
- Q89302257's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.48'}[14].
- Q89302257's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.456'}[15].
- Q89302257's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.804'}[16].
- Q89302257's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.668'}[17].
- Q89302257's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.66'}[18].
- Q89302257's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.1536'}[19].
- Q89302257's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1935'}[20].
- Q89302257's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-16.01'}[21].
- Q89302257's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+837.8718'}[22].
- Q89302257's SIMBAD ID is recorded as BD+27 1805[23].
- Q89302257's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+146.24139660409160'}[24].
- Q89302257's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+27.31107172476400'}[25].
- Q89302257's epoch is recorded as J2000.0[26].