Q77525535

Summary

Q77525535 is a Mira variable^[1].

Key Facts

• Q77525535's instance of is recorded as Mira variable^[2].
• Q77525535's instance of is recorded as infrared source^[3].
• Q77525535's instance of is recorded as long-period variable star^[4].
• Q77525535's instance of is recorded as near-infrared source^[5].
• Q77525535's constellation is recorded as Puppis^[6].
• Q77525535's spectral class is recorded as M8^[7].
• Q77525535's catalog code is recorded as IRAS 08084-1510^[8].
• Q77525535's catalog code is recorded as IRC -20159^[9].
• Q77525535's catalog code is recorded as RAFGL 5241^[10].
• Q77525535's catalog code is recorded as 2MASS J08104310-1519469^[11].
• Q77525535's catalog code is recorded as Gaia DR2 5724674536321854208^[12].
• Q77525535's catalog code is recorded as DP Pup^[13].
• Q77525535's catalog code is recorded as TIC 422144420^[14].
• Q77525535's catalog code is recorded as Gaia DR3 5724674536321854208^[15].
• Q77525535's type of variable star is recorded as Mira variable^[16].
• Q77525535's type of variable star is recorded as long-period variable star^[17].
• Q77525535's apparent magnitude is recorded as {'unit': '1', 'amount': '+14'}^[18].
• Q77525535's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.134'}^[19].
• Q77525535's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.000'}^[20].
• Q77525535's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.348'}^[21].
• Q77525535's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.176515'}^[22].
• Q77525535's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.34'}^[23].
• Q77525535's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4979'}^[24].
• Q77525535's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+273.5978'}^[25].
• Q77525535's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+122.67951037057001'}^[26].

Body

Definition and Type

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