Q91570850
star in the constellation Puppis
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Q91570850
Summary
Q91570850 is a star[1].
Key Facts
- Q91570850's instance of is recorded as star[2].
- Q91570850's constellation is recorded as Puppis[3].
- Q91570850's spectral class is recorded as K1III[4].
- Q91570850's catalog code is recorded as BD-12 2058[5].
- Q91570850's catalog code is recorded as GSC 05409-00467[6].
- Q91570850's catalog code is recorded as HD 61179[7].
- Q91570850's catalog code is recorded as PPM 218952[8].
- Q91570850's catalog code is recorded as SAO 153165[9].
- Q91570850's catalog code is recorded as TYC 5409-467-1[10].
- Q91570850's catalog code is recorded as YZC 11 2751[11].
- Q91570850's catalog code is recorded as 2MASS J07373296-1318247[12].
- Q91570850's catalog code is recorded as Gaia DR2 3030721823932934528[13].
- Q91570850's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.679'}[14].
- Q91570850's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.104'}[15].
- Q91570850's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.940'}[16].
- Q91570850's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.71'}[17].
- Q91570850's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.82'}[18].
- Q91570850's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.3522'}[19].
- Q91570850's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5835'}[20].
- Q91570850's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+25.67'}[21].
- Q91570850's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+631.5125'}[22].
- Q91570850's SIMBAD ID is recorded as HD 61179[23].
- Q91570850's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+114.38733329460410'}[24].
- Q91570850's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-13.30683692835420'}[25].
- Q91570850's epoch is recorded as J2000.0[26].