Q85506030
long period variable
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Q85506030
Summary
Q85506030 is a long-period variable star[1].
Key Facts
- Q85506030's instance of is recorded as long-period variable star[2].
- Q85506030's constellation is recorded as Monoceros[3].
- Q85506030's spectral class is recorded as M4[4].
- Q85506030's catalog code is recorded as 2MASS J07115143-0839461[5].
- Q85506030's catalog code is recorded as AN 102.1936[6].
- Q85506030's catalog code is recorded as GSC 05394-03521[7].
- Q85506030's catalog code is recorded as SV* P 2985[8].
- Q85506030's catalog code is recorded as Gaia DR2 3048362388487522688[9].
- Q85506030's catalog code is recorded as FL Mon[10].
- Q85506030's type of variable star is recorded as slow irregular variables of late spectral types[11].
- Q85506030's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.103'}[12].
- Q85506030's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.072'}[13].
- Q85506030's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.734'}[14].
- Q85506030's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.7831'}[15].
- Q85506030's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4201'}[16].
- Q85506030's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+33.06'}[17].
- Q85506030's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+107.96430660479860'}[18].
- Q85506030's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-8.66281622463500'}[19].
- Q85506030's epoch is recorded as J2000.0[20].
- Q85506030's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.902'}[21].
- Q85506030's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.907'}[22].
Body
Definition and Type
Q85506030's instance of is recorded as long-period variable star[2].