Q86949680
high proper-motion star in the constellation Piscis Austrinus
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Q86949680
Summary
Q86949680 is a high proper-motion star[1].
Key Facts
- Q86949680's instance of is recorded as high proper-motion star[2].
- Q86949680's constellation is recorded as Piscis Austrinus[3].
- Q86949680's spectral class is recorded as G0V[4].
- Q86949680's catalog code is recorded as Gaia DR1 6598318880585396224[5].
- Q86949680's catalog code is recorded as CD-36 15307[6].
- Q86949680's catalog code is recorded as CPC 18 11430[7].
- Q86949680's catalog code is recorded as CPD-36 9555[8].
- Q86949680's catalog code is recorded as GSC 07502-01141[9].
- Q86949680's catalog code is recorded as HD 211484[10].
- Q86949680's catalog code is recorded as HIC 110087[11].
- Q86949680's catalog code is recorded as HIP 110087[12].
- Q86949680's catalog code is recorded as PPM 302419[13].
- Q86949680's catalog code is recorded as SAO 213710[14].
- Q86949680's catalog code is recorded as TYC 7502-1141-1[15].
- Q86949680's catalog code is recorded as Gaia DR2 6598318884880520448[16].
- Q86949680's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.07'}[17].
- Q86949680's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.70'}[18].
- Q86949680's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9645'}[19].
- Q86949680's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.2842'}[20].
- Q86949680's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-11.90'}[21].
- Q86949680's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+137.2834'}[22].
- Q86949680's SIMBAD ID is recorded as HD 211484[23].
- Q86949680's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+334.50718145365200'}[24].
- Q86949680's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-36.21556018651640'}[25].
- Q86949680's epoch is recorded as J2000.0[26].