Q93864245
Press Enter · cited answer in seconds
0 sources
Q93864245
Summary
Q93864245 is a high proper-motion star[1].
Key Facts
- Q93864245's instance of is recorded as high proper-motion star[2].
- Q93864245's instance of is recorded as astrophysical X-ray source[3].
- Q93864245's constellation is recorded as Volans[4].
- Q93864245's spectral class is recorded as F0IV/V[5].
- Q93864245's catalog code is recorded as CD-65 456[6].
- Q93864245's catalog code is recorded as CPC 21 1237[7].
- Q93864245's catalog code is recorded as CPD-65 647[8].
- Q93864245's catalog code is recorded as GSC 08907-01345[9].
- Q93864245's catalog code is recorded as HD 49172[10].
- Q93864245's catalog code is recorded as PPM 355566[11].
- Q93864245's catalog code is recorded as TYC 8907-1345-1[12].
- Q93864245's catalog code is recorded as uvby98 100049172[13].
- Q93864245's catalog code is recorded as 2MASS J06420923-6605393[14].
- Q93864245's catalog code is recorded as Gaia DR1 5283545244280380288[15].
- Q93864245's catalog code is recorded as GEN# +1.00049172[16].
- Q93864245's catalog code is recorded as Gaia DR2 5283545248579599232[17].
- Q93864245's catalog code is recorded as 1RXS J064209.1-660536[18].
- Q93864245's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.00'}[19].
- Q93864245's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.39'}[20].
- Q93864245's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.286'}[21].
- Q93864245's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.213'}[22].
- Q93864245's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.107'}[23].
- Q93864245's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9394'}[24].
- Q93864245's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.9824'}[25].
- Q93864245's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+21.56'}[26].
Body
Definition and Type
Recorded instance of include high proper-motion star[2] and astrophysical X-ray source[3].