Q93879397
high proper-motion star in the constellation Camelopardalis
Press Enter · cited answer in seconds
0 sources
Q93879397
Summary
Q93879397 is a high proper-motion star[1].
Key Facts
- Q93879397's instance of is recorded as high proper-motion star[2].
- Q93879397's constellation is recorded as Camelopardalis[3].
- Q93879397's spectral class is recorded as G5[4].
- Q93879397's catalog code is recorded as 2MASS J13001889+8415073[5].
- Q93879397's catalog code is recorded as PLX 2993[6].
- Q93879397's catalog code is recorded as AG+84 275[7].
- Q93879397's catalog code is recorded as BD+85 214[8].
- Q93879397's catalog code is recorded as GCRV 7781[9].
- Q93879397's catalog code is recorded as GSC 04633-00705[10].
- Q93879397's catalog code is recorded as HD 113826[11].
- Q93879397's catalog code is recorded as PPM 2251[12].
- Q93879397's catalog code is recorded as SAO 2131[13].
- Q93879397's catalog code is recorded as TYC 4633-705-1[14].
- Q93879397's catalog code is recorded as PLX 2993.00[15].
- Q93879397's catalog code is recorded as Gaia DR1 1726231984298617856[16].
- Q93879397's catalog code is recorded as WEB 11230[17].
- Q93879397's catalog code is recorded as Gaia DR2 1726231988594763520[18].
- Q93879397's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.962'}[19].
- Q93879397's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.679'}[20].
- Q93879397's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.577'}[21].
- Q93879397's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.21'}[22].
- Q93879397's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.89'}[23].
- Q93879397's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0711'}[24].
- Q93879397's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+12.9298'}[25].
- Q93879397's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-26.44'}[26].
Body
Definition and Type
Q93879397's instance of is recorded as high proper-motion star[2].