Q94027886
high proper-motion star in the constellation Crater
Press Enter · cited answer in seconds
0 sources
Q94027886
Summary
Q94027886 is a high proper-motion star[1].
Key Facts
- Q94027886's instance of is recorded as high proper-motion star[2].
- Q94027886's constellation is recorded as Crater[3].
- Q94027886's spectral class is recorded as G8/K0V[4].
- Q94027886's catalog code is recorded as CD-23 9690[5].
- Q94027886's catalog code is recorded as CPD-23 5043[6].
- Q94027886's catalog code is recorded as GSC 06636-01136[7].
- Q94027886's catalog code is recorded as HD 95714[8].
- Q94027886's catalog code is recorded as PPM 258452[9].
- Q94027886's catalog code is recorded as SAO 179460[10].
- Q94027886's catalog code is recorded as TYC 6636-1136-1[11].
- Q94027886's catalog code is recorded as YZ 114 8581[12].
- Q94027886's catalog code is recorded as 2MASS J11023720-2416568[13].
- Q94027886's catalog code is recorded as RAVE J110237.2-241657[14].
- Q94027886's catalog code is recorded as Gaia DR1 3537037887608468864[15].
- Q94027886's catalog code is recorded as Gaia DR2 3537037891905801728[16].
- Q94027886's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.90'}[17].
- Q94027886's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.506'}[18].
- Q94027886's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.126'}[19].
- Q94027886's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.054'}[20].
- Q94027886's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.78'}[21].
- Q94027886's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7142'}[22].
- Q94027886's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+14.3637'}[23].
- Q94027886's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+15.97'}[24].
- Q94027886's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+69.6199'}[25].
- Q94027886's SIMBAD ID is recorded as HD 95714[26].