Q89095756
star in the constellation Lyra
Press Enter · cited answer in seconds
0 sources
Q89095756
Summary
Q89095756 is a star[1].
Key Facts
- Q89095756's instance of is recorded as star[2].
- Q89095756's constellation is recorded as Lyra[3].
- Q89095756's spectral class is recorded as K0[4].
- Q89095756's catalog code is recorded as AG+38 1821[5].
- Q89095756's catalog code is recorded as BD+38 3526[6].
- Q89095756's catalog code is recorded as DO 17626[7].
- Q89095756's catalog code is recorded as GSC 03121-00151[8].
- Q89095756's catalog code is recorded as HD 181208[9].
- Q89095756's catalog code is recorded as PPM 82654[10].
- Q89095756's catalog code is recorded as SAO 68099[11].
- Q89095756's catalog code is recorded as TYC 3121-151-1[12].
- Q89095756's catalog code is recorded as 2MASS J19175837+3844006[13].
- Q89095756's catalog code is recorded as Gaia DR1 2099432000570241920[14].
- Q89095756's catalog code is recorded as Gaia DR2 2099432004870517248[15].
- Q89095756's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.224'}[16].
- Q89095756's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.688'}[17].
- Q89095756's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.538'}[18].
- Q89095756's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.31'}[19].
- Q89095756's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.53'}[20].
- Q89095756's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.9502'}[21].
- Q89095756's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.8773'}[22].
- Q89095756's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-16.08'}[23].
- Q89095756's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+205.0315'}[24].
- Q89095756's SIMBAD ID is recorded as HD 181208[25].
- Q89095756's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+289.49331523528140'}[26].