Q79284545
long period variable
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Q79284545
Summary
Q79284545 is a long-period variable star[1].
Key Facts
- Q79284545's instance of is recorded as long-period variable star[2].
- Q79284545's constellation is recorded as Taurus[3].
- Q79284545's spectral class is recorded as M3[4].
- Q79284545's catalog code is recorded as 2MASS J05453362+1626560[5].
- Q79284545's catalog code is recorded as GSC 01299-00591[6].
- Q79284545's catalog code is recorded as IRAS 05426+1625[7].
- Q79284545's catalog code is recorded as SV* SON 3737[8].
- Q79284545's catalog code is recorded as Gaia DR2 3396422518061798400[9].
- Q79284545's catalog code is recorded as EH Tau[10].
- Q79284545's type of variable star is recorded as slow irregular variables of late spectral types[11].
- Q79284545's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.033'}[12].
- Q79284545's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.060'}[13].
- Q79284545's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.703'}[14].
- Q79284545's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.2658'}[15].
- Q79284545's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2083'}[16].
- Q79284545's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+15.65'}[17].
- Q79284545's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+86.39011127607510'}[18].
- Q79284545's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+16.44888142766800'}[19].
- Q79284545's epoch is recorded as J2000.0[20].
- Q79284545's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.339'}[21].
- Q79284545's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.930'}[22].
Body
Definition and Type
Q79284545's instance of is recorded as long-period variable star[2].