Q88893717
high proper-motion star in the constellation Auriga
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Q88893717
Summary
Q88893717 is a high proper-motion star[1].
Key Facts
- Q88893717's instance of is recorded as high proper-motion star[2].
- Q88893717's constellation is recorded as Auriga[3].
- Q88893717's spectral class is recorded as F5[4].
- Q88893717's catalog code is recorded as 2MASS J07010844+4001069[5].
- Q88893717's catalog code is recorded as AG+40 831[6].
- Q88893717's catalog code is recorded as BD+40 1771[7].
- Q88893717's catalog code is recorded as GSC 02947-01214[8].
- Q88893717's catalog code is recorded as HD 51930[9].
- Q88893717's catalog code is recorded as HIC 33806[10].
- Q88893717's catalog code is recorded as HIP 33806[11].
- Q88893717's catalog code is recorded as PPM 49520[12].
- Q88893717's catalog code is recorded as SAO 41499[13].
- Q88893717's catalog code is recorded as TYC 2947-1214-1[14].
- Q88893717's catalog code is recorded as uvby98 100051930[15].
- Q88893717's catalog code is recorded as GEN# +1.00051930[16].
- Q88893717's catalog code is recorded as Gaia DR2 947435945451648640[17].
- Q88893717's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.702'}[18].
- Q88893717's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.424'}[19].
- Q88893717's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.393'}[20].
- Q88893717's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.59'}[21].
- Q88893717's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.08'}[22].
- Q88893717's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.4846'}[23].
- Q88893717's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+10.2515'}[24].
- Q88893717's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-1.64'}[25].
- Q88893717's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+97.5467'}[26].
Body
Definition and Type
Q88893717's instance of is recorded as high proper-motion star[2].