Q89725590
star in the constellation Lynx
Press Enter · cited answer in seconds
0 sources
Q89725590
Summary
Q89725590 is a star[1].
Key Facts
- Q89725590's instance of is recorded as star[2].
- Q89725590's constellation is recorded as Lynx[3].
- Q89725590's spectral class is recorded as G5[4].
- Q89725590's catalog code is recorded as 2MASS J07025413+5851387[5].
- Q89725590's catalog code is recorded as AG+58 579[6].
- Q89725590's catalog code is recorded as BD+59 1042[7].
- Q89725590's catalog code is recorded as GSC 03779-01100[8].
- Q89725590's catalog code is recorded as HD 51951[9].
- Q89725590's catalog code is recorded as PPM 30870[10].
- Q89725590's catalog code is recorded as SAO 26112[11].
- Q89725590's catalog code is recorded as TYC 3779-1100-1[12].
- Q89725590's catalog code is recorded as YZ 58 4853[13].
- Q89725590's catalog code is recorded as Gaia DR1 1002275320541252608[14].
- Q89725590's catalog code is recorded as Gaia DR2 1002275324837390336[15].
- Q89725590's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.916'}[16].
- Q89725590's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.385'}[17].
- Q89725590's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.255'}[18].
- Q89725590's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.88'}[19].
- Q89725590's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.98'}[20].
- Q89725590's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.5475'}[21].
- Q89725590's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.4407'}[22].
- Q89725590's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-39.20'}[23].
- Q89725590's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+409.7185'}[24].
- Q89725590's SIMBAD ID is recorded as HD 51951[25].
- Q89725590's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+105.72560442945060'}[26].