Q88726546

Summary

Q88726546 is a star^[1].

Key Facts

• Q88726546's instance of is recorded as star^[2].
• Q88726546's constellation is recorded as Ophiuchus^[3].
• Q88726546's spectral class is recorded as F5V^[4].
• Q88726546's catalog code is recorded as AG+04 2049^[5].
• Q88726546's catalog code is recorded as BD+04 3305^[6].
• Q88726546's catalog code is recorded as GSC 00406-03317^[7].
• Q88726546's catalog code is recorded as HD 153587^[8].
• Q88726546's catalog code is recorded as PPM 163367^[9].
• Q88726546's catalog code is recorded as TYC 406-3317-1^[10].
• Q88726546's catalog code is recorded as Gaia DR1 4392295515535422080^[11].
• Q88726546's catalog code is recorded as Gaia DR2 4392295519832731648^[12].
• Q88726546's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.68'}^[13].
• Q88726546's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.33'}^[14].
• Q88726546's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.5748'}^[15].
• Q88726546's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.8593'}^[16].
• Q88726546's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-36.77'}^[17].
• Q88726546's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+205.7910'}^[18].
• Q88726546's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+255.05897857056000'}^[19].
• Q88726546's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+4.40728983039780'}^[20].
• Q88726546's epoch is recorded as J2000.0^[21].
• Q88726546's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+19.249'}^[22].
• Q88726546's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.720'}^[23].

Body

Definition and Type

Q88726546's instance of is recorded as star^[2].