Q80603788
high proper-motion star in the constellation Ursa Major
Press Enter · cited answer in seconds
0 sources
Q80603788
Summary
Q80603788 is a high proper-motion star[1].
Key Facts
- Q80603788's instance of is recorded as high proper-motion star[2].
- Q80603788's constellation is recorded as Ursa Major[3].
- Q80603788's spectral class is recorded as G0[4].
- Q80603788's catalog code is recorded as ADS 7698 AB[5].
- Q80603788's catalog code is recorded as AG+48 882[6].
- Q80603788's catalog code is recorded as BD+49 1933[7].
- Q80603788's catalog code is recorded as CCDM J10162+4844AB[8].
- Q80603788's catalog code is recorded as GSC 03438-00192[9].
- Q80603788's catalog code is recorded as HIC 50296[10].
- Q80603788's catalog code is recorded as HIP 50296[11].
- Q80603788's catalog code is recorded as IDS 10099+4914 AB[12].
- Q80603788's catalog code is recorded as PPM 51777[13].
- Q80603788's catalog code is recorded as SAO 43252[14].
- Q80603788's catalog code is recorded as TYC 3438-192-1[15].
- Q80603788's catalog code is recorded as 2MASS J10160942+4844288[16].
- Q80603788's catalog code is recorded as WDS J10162+4844AB[17].
- Q80603788's catalog code is recorded as Gaia DR2 846753150300401920[18].
- Q80603788's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.76'}[19].
- Q80603788's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.622'}[20].
- Q80603788's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.361'}[21].
- Q80603788's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.306'}[22].
- Q80603788's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.35'}[23].
- Q80603788's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6152'}[24].
- Q80603788's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.4331'}[25].
- Q80603788's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-18.81'}[26].
Body
Definition and Type
Q80603788's instance of is recorded as high proper-motion star[2].