Q85040633
high proper-motion star in the constellation Cygnus
Press Enter · cited answer in seconds
0 sources
Q85040633
Summary
Q85040633 is a high proper-motion star[1].
Key Facts
- Q85040633's instance of is recorded as high proper-motion star[2].
- Q85040633's constellation is recorded as Cygnus[3].
- Q85040633's spectral class is recorded as G8III[4].
- Q85040633's catalog code is recorded as AG+29 2082[5].
- Q85040633's catalog code is recorded as BD+28 3375[6].
- Q85040633's catalog code is recorded as GSC 02137-00172[7].
- Q85040633's catalog code is recorded as HIC 96059[8].
- Q85040633's catalog code is recorded as HIP 96059[9].
- Q85040633's catalog code is recorded as LF 2 +29 72[10].
- Q85040633's catalog code is recorded as PPM 109163[11].
- Q85040633's catalog code is recorded as SAO 87322[12].
- Q85040633's catalog code is recorded as TYC 2137-172-1[13].
- Q85040633's catalog code is recorded as YZ 29 10070[14].
- Q85040633's catalog code is recorded as 2MASS J19315464+2908309[15].
- Q85040633's catalog code is recorded as Gaia DR1 2026517337225273728[16].
- Q85040633's catalog code is recorded as Gaia DR2 2026517341547283584[17].
- Q85040633's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.665'}[18].
- Q85040633's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.028'}[19].
- Q85040633's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.934'}[20].
- Q85040633's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.68'}[21].
- Q85040633's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.80'}[22].
- Q85040633's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.3370'}[23].
- Q85040633's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.8760'}[24].
- Q85040633's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+3.99'}[25].
- Q85040633's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+347.7051'}[26].