Q88395193
star in the constellation Puppis
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Q88395193
Summary
Q88395193 is a star[1].
Key Facts
- Q88395193's instance of is recorded as star[2].
- Q88395193's constellation is recorded as Puppis[3].
- Q88395193's spectral class is recorded as G5V[4].
- Q88395193's catalog code is recorded as BD-17 2500[5].
- Q88395193's catalog code is recorded as GSC 06002-01042[6].
- Q88395193's catalog code is recorded as HD 71455[7].
- Q88395193's catalog code is recorded as PPM 220127[8].
- Q88395193's catalog code is recorded as SAO 154269[9].
- Q88395193's catalog code is recorded as TYC 6002-1042-1[10].
- Q88395193's catalog code is recorded as YZ 107 3360[11].
- Q88395193's catalog code is recorded as 2MASS J08265998-1809385[12].
- Q88395193's catalog code is recorded as Gaia DR2 5707985118043148032[13].
- Q88395193's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.83'}[14].
- Q88395193's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.273'}[15].
- Q88395193's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.872'}[16].
- Q88395193's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.783'}[17].
- Q88395193's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.73'}[18].
- Q88395193's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6384'}[19].
- Q88395193's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2995'}[20].
- Q88395193's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-7.00'}[21].
- Q88395193's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+769.5267'}[22].
- Q88395193's SIMBAD ID is recorded as HD 71455[23].
- Q88395193's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+126.74996247617290'}[24].
- Q88395193's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-18.16070027098790'}[25].
- Q88395193's epoch is recorded as J2000.0[26].