Q78449608
high proper-motion star in the constellation Pegasus
Press Enter · cited answer in seconds
0 sources
Q78449608
Summary
Q78449608 is a high proper-motion star[1].
Key Facts
- Q78449608's instance of is recorded as high proper-motion star[2].
- Q78449608's constellation is recorded as Pegasus[3].
- Q78449608's spectral class is recorded as K5[4].
- Q78449608's catalog code is recorded as AG+13 2292[5].
- Q78449608's catalog code is recorded as BD+12 4639[6].
- Q78449608's catalog code is recorded as DO 7428[7].
- Q78449608's catalog code is recorded as GSC 01131-01658[8].
- Q78449608's catalog code is recorded as HD 204661[9].
- Q78449608's catalog code is recorded as IRAS 21273+1303[10].
- Q78449608's catalog code is recorded as PPM 140212[11].
- Q78449608's catalog code is recorded as SAO 107177[12].
- Q78449608's catalog code is recorded as TYC 1131-1658-1[13].
- Q78449608's catalog code is recorded as YZ 13 8522[14].
- Q78449608's catalog code is recorded as 2MASS J21294702+1316412[15].
- Q78449608's catalog code is recorded as Gaia DR1 1770281615562814848[16].
- Q78449608's catalog code is recorded as Gaia DR2 1770281615562814848[17].
- Q78449608's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.090'}[18].
- Q78449608's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.131'}[19].
- Q78449608's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.19'}[20].
- Q78449608's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.79'}[21].
- Q78449608's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.592'}[22].
- Q78449608's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.4724'}[23].
- Q78449608's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2694'}[24].
- Q78449608's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-120.26'}[25].
- Q78449608's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+787.7738'}[26].