Q90859707

Summary

Q90859707 is a star^[1].

Key Facts

• Q90859707's instance of is recorded as star^[2].
• Q90859707's constellation is recorded as Virgo^[3].
• Q90859707's spectral class is recorded as G^[4].
• Q90859707's catalog code is recorded as Pul -3 940021^[5].
• Q90859707's catalog code is recorded as AG+05 1712^[6].
• Q90859707's catalog code is recorded as BD+06 2585^[7].
• Q90859707's catalog code is recorded as GPM 184.661190+05.360625^[8].
• Q90859707's catalog code is recorded as GSC 00287-00541^[9].
• Q90859707's catalog code is recorded as PPM 158706^[10].
• Q90859707's catalog code is recorded as SAO 119320^[11].
• Q90859707's catalog code is recorded as TYC 287-541-1^[12].
• Q90859707's catalog code is recorded as YZ 5 6076^[13].
• Q90859707's catalog code is recorded as 2MASS J12183868+0521384^[14].
• Q90859707's catalog code is recorded as Gaia DR1 3894395865468591104^[15].
• Q90859707's catalog code is recorded as Gaia DR2 3894395869764448768^[16].
• Q90859707's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.1'}^[17].
• Q90859707's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.267'}^[18].
• Q90859707's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.033'}^[19].
• Q90859707's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.980'}^[20].
• Q90859707's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.13'}^[21].
• Q90859707's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.81'}^[22].
• Q90859707's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.1783'}^[23].
• Q90859707's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.7489'}^[24].
• Q90859707's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+6.20'}^[25].
• Q90859707's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+266.7449'}^[26].

Body

Definition and Type

Q90859707's instance of is recorded as star^[2].