Q88248021
star in the constellation Sextans
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Q88248021
Summary
Q88248021 is a star[1].
Key Facts
- Q88248021's instance of is recorded as star[2].
- Q88248021's constellation is recorded as Sextans[3].
- Q88248021's catalog code is recorded as [LPP2003] 741[4].
- Q88248021's catalog code is recorded as [WMO2009] Sex-348[5].
- Q88248021's catalog code is recorded as [KGS2010] Sex 741[6].
- Q88248021's catalog code is recorded as Gaia DR2 3829157373826735232[7].
- Q88248021's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.68'}[8].
- Q88248021's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.768'}[9].
- Q88248021's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.800'}[10].
- Q88248021's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.5678'}[11].
- Q88248021's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1360'}[12].
- Q88248021's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+212.0'}[13].
- Q88248021's metallicity is recorded as {'unit': '1', 'amount': '-2.04'}[14].
- Q88248021's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+153.25779406990290'}[15].
- Q88248021's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-1.59009267856600'}[16].
- Q88248021's epoch is recorded as J2000.0[17].
- Q88248021's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4882'}[18].
- Q88248021's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+93'}[19].
- Q88248021's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.781'}[20].
- Q88248021's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.118'}[21].
Body
Definition and Type
Q88248021's instance of is recorded as star[2].