Q85431820
star in the constellation Telescopium
Press Enter · cited answer in seconds
0 sources
Q85431820
Summary
Q85431820 is a star[1].
Key Facts
- Q85431820's instance of is recorded as star[2].
- Q85431820's constellation is recorded as Telescopium[3].
- Q85431820's spectral class is recorded as G6/8III[4].
- Q85431820's catalog code is recorded as CD-54 8079[5].
- Q85431820's catalog code is recorded as CPC 19 7526[6].
- Q85431820's catalog code is recorded as CPD-54 9178[7].
- Q85431820's catalog code is recorded as GSC 08759-01659[8].
- Q85431820's catalog code is recorded as HD 175327[9].
- Q85431820's catalog code is recorded as PPM 347299[10].
- Q85431820's catalog code is recorded as SAO 245827[11].
- Q85431820's catalog code is recorded as TYC 8759-1659-1[12].
- Q85431820's catalog code is recorded as 2MASS J18575066-5414024[13].
- Q85431820's catalog code is recorded as RAVE J185750.7-541403[14].
- Q85431820's catalog code is recorded as Gaia DR1 6650328701156283776[15].
- Q85431820's catalog code is recorded as Gaia DR2 6650328705456363392[16].
- Q85431820's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.990'}[17].
- Q85431820's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.476'}[18].
- Q85431820's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.380'}[19].
- Q85431820's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.96'}[20].
- Q85431820's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.900'}[21].
- Q85431820's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.169'}[22].
- Q85431820's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.5908'}[23].
- Q85431820's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.6215'}[24].
- Q85431820's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-9.16'}[25].
- Q85431820's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+616.7129'}[26].