Q85014509
high proper-motion star in the constellation Aquila
Press Enter · cited answer in seconds
0 sources
Q85014509
Summary
Q85014509 is a high proper-motion star[1].
Key Facts
- Q85014509's instance of is recorded as high proper-motion star[2].
- Q85014509's constellation is recorded as Aquila[3].
- Q85014509's spectral class is recorded as K4[4].
- Q85014509's catalog code is recorded as StKM 1-1730[5].
- Q85014509's catalog code is recorded as 2MASS J19541497-0715487[6].
- Q85014509's catalog code is recorded as Gaia DR2 4196022210256933504[7].
- Q85014509's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.5'}[8].
- Q85014509's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.147'}[9].
- Q85014509's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.549'}[10].
- Q85014509's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.379'}[11].
- Q85014509's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.9563'}[12].
- Q85014509's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+17.0842'}[13].
- Q85014509's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-34.21'}[14].
- Q85014509's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+58.5336'}[15].
- Q85014509's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+298.56241468800900'}[16].
- Q85014509's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-7.26348650746420'}[17].
- Q85014509's epoch is recorded as J2000.0[18].
- Q85014509's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.429'}[19].
- Q85014509's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+50.548'}[20].
Body
Definition and Type
Q85014509's instance of is recorded as high proper-motion star[2].