Q84010174

Summary

Q84010174 is a Mira variable^[1].

Key Facts

• Q84010174's instance of is recorded as Mira variable^[2].
• Q84010174's instance of is recorded as infrared source^[3].
• Q84010174's instance of is recorded as near-infrared source^[4].
• Q84010174's instance of is recorded as variable star^[5].
• Q84010174's constellation is recorded as Sagittarius^[6].
• Q84010174's spectral class is recorded as Me^[7].
• Q84010174's catalog code is recorded as IRAS 19007-2703^[8].
• Q84010174's catalog code is recorded as ASAS J190349-2659.0^[9].
• Q84010174's catalog code is recorded as 2MASS J19034876-2659012^[10].
• Q84010174's catalog code is recorded as GCRV 6460 E^[11].
• Q84010174's catalog code is recorded as WEB 16259^[12].
• Q84010174's catalog code is recorded as Gaia DR2 6763549575305981696^[13].
• Q84010174's catalog code is recorded as QY Sgr^[14].
• Q84010174's catalog code is recorded as Gaia DR3 6763549575305981696^[15].
• Q84010174's catalog code is recorded as TIC 108906826^[16].
• Q84010174's type of variable star is recorded as long-period variable star^[17].
• Q84010174's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.291'}^[18].
• Q84010174's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.406'}^[19].
• Q84010174's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.011'}^[20].
• Q84010174's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.488909'}^[21].
• Q84010174's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4063'}^[22].
• Q84010174's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+78.77'}^[23].
• Q84010174's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+285.95320626090995'}^[24].
• Q84010174's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-26.98368903437'}^[25].
• Q84010174's epoch is recorded as J2000.0^[26].

Body

Definition and Type

Recorded instance of include Mira variable^[2], infrared source^[3], near-infrared source^[4], and variable star^[5].