Q88437006
high proper-motion star in the constellation Carina
Press Enter · cited answer in seconds
0 sources
Q88437006
Summary
Q88437006 is a high proper-motion star[1].
Key Facts
- Q88437006's instance of is recorded as high proper-motion star[2].
- Q88437006's constellation is recorded as Carina[3].
- Q88437006's spectral class is recorded as G0[4].
- Q88437006's catalog code is recorded as VCA 4[5].
- Q88437006's catalog code is recorded as 1RXS J092501.0-643726[6].
- Q88437006's catalog code is recorded as CD-64 394[7].
- Q88437006's catalog code is recorded as CPD-64 1033[8].
- Q88437006's catalog code is recorded as GSC 08948-01600[9].
- Q88437006's catalog code is recorded as HD 309681[10].
- Q88437006's catalog code is recorded as PPM 357340[11].
- Q88437006's catalog code is recorded as TYC 8948-1600-1[12].
- Q88437006's catalog code is recorded as [FS2003] 0508[13].
- Q88437006's catalog code is recorded as 2MASS J09250164-6437312[14].
- Q88437006's catalog code is recorded as Gaia DR1 5248648085244411520[15].
- Q88437006's catalog code is recorded as Gaia DR2 5248648089548727552[16].
- Q88437006's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.979'}[17].
- Q88437006's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.692'}[18].
- Q88437006's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.602'}[19].
- Q88437006's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.23'}[20].
- Q88437006's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.81'}[21].
- Q88437006's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0255'}[22].
- Q88437006's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+11.5336'}[23].
- Q88437006's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+26.40'}[24].
- Q88437006's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+86.7032'}[25].
- Q88437006's SIMBAD ID is recorded as HD 309681[26].