Q80434968
high proper-motion star in the constellation Pegasus
Press Enter · cited answer in seconds
0 sources
Q80434968
Summary
Q80434968 is a high proper-motion star[1].
Key Facts
- Q80434968's instance of is recorded as high proper-motion star[2].
- Q80434968's constellation is recorded as Pegasus[3].
- Q80434968's spectral class is recorded as G5[4].
- Q80434968's catalog code is recorded as AG+22 2580[5].
- Q80434968's catalog code is recorded as BD+22 4931[6].
- Q80434968's catalog code is recorded as GSC 02252-01883[7].
- Q80434968's catalog code is recorded as HD 224236[8].
- Q80434968's catalog code is recorded as PPM 115969[9].
- Q80434968's catalog code is recorded as SAO 91590[10].
- Q80434968's catalog code is recorded as TYC 2252-1883-1[11].
- Q80434968's catalog code is recorded as YZ 22 9146[12].
- Q80434968's catalog code is recorded as uvby98 100224236[13].
- Q80434968's catalog code is recorded as 2MASS J23560796+2252567[14].
- Q80434968's catalog code is recorded as Gaia DR1 2847888910128777344[15].
- Q80434968's catalog code is recorded as GEN# +1.00224236[16].
- Q80434968's catalog code is recorded as Gaia DR2 2847888914425097856[17].
- Q80434968's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.561'}[18].
- Q80434968's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.250'}[19].
- Q80434968's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.164'}[20].
- Q80434968's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.85'}[21].
- Q80434968's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.49'}[22].
- Q80434968's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6486'}[23].
- Q80434968's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.8196'}[24].
- Q80434968's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-19.57'}[25].
- Q80434968's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+72.3610'}[26].