Q85233710
high proper-motion star in the constellation Scorpius
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Q85233710
Summary
Q85233710 is a high proper-motion star[1].
Key Facts
- Q85233710's instance of is recorded as high proper-motion star[2].
- Q85233710's constellation is recorded as Scorpius[3].
- Q85233710's spectral class is recorded as G2V[4].
- Q85233710's catalog code is recorded as Gaia DR1 5998491547689774720[5].
- Q85233710's catalog code is recorded as CD-36 10680[6].
- Q85233710's catalog code is recorded as CPC 18 8018[7].
- Q85233710's catalog code is recorded as CPD-36 6951[8].
- Q85233710's catalog code is recorded as GSC 07342-00793[9].
- Q85233710's catalog code is recorded as HD 145087[10].
- Q85233710's catalog code is recorded as HIC 79259[11].
- Q85233710's catalog code is recorded as HIP 79259[12].
- Q85233710's catalog code is recorded as PPM 294758[13].
- Q85233710's catalog code is recorded as SAO 207415[14].
- Q85233710's catalog code is recorded as TYC 7342-793-1[15].
- Q85233710's catalog code is recorded as 2MASS J16103616-3650407[16].
- Q85233710's catalog code is recorded as Gaia DR2 5998491551995630208[17].
- Q85233710's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.02'}[18].
- Q85233710's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.62'}[19].
- Q85233710's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.814'}[20].
- Q85233710's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.532'}[21].
- Q85233710's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.429'}[22].
- Q85233710's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8180'}[23].
- Q85233710's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.0424'}[24].
- Q85233710's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-21.43'}[25].
- Q85233710's metallicity is recorded as {'unit': '1', 'amount': '-0.01'}[26].
Body
Definition and Type
Q85233710's instance of is recorded as high proper-motion star[2].