Q93041219
long period variable
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Q93041219
Summary
Q93041219 is a long-period variable star[1].
Key Facts
- Q93041219's instance of is recorded as long-period variable star[2].
- Q93041219's instance of is recorded as infrared source[3].
- Q93041219's instance of is recorded as near-infrared source[4].
- Q93041219's constellation is recorded as Perseus[5].
- Q93041219's spectral class is recorded as M7[6].
- Q93041219's catalog code is recorded as IRAS 02570+5602[7].
- Q93041219's catalog code is recorded as 2MASS J03004842+5614100[8].
- Q93041219's catalog code is recorded as Gaia DR2 459803157014082816[9].
- Q93041219's catalog code is recorded as QR Per[10].
- Q93041219's catalog code is recorded as TIC 251492245[11].
- Q93041219's catalog code is recorded as Gaia DR3 459803157014082816[12].
- Q93041219's type of variable star is recorded as semiregular variable star[13].
- Q93041219's type of variable star is recorded as long-period variable star[14].
- Q93041219's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.06'}[15].
- Q93041219's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.78'}[16].
- Q93041219's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.19'}[17].
- Q93041219's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.686366'}[18].
- Q93041219's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4717'}[19].
- Q93041219's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-38.78'}[20].
- Q93041219's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+45.20177815199'}[21].
- Q93041219's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+56.23606063783'}[22].
- Q93041219's epoch is recorded as J2000.0[23].
- Q93041219's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.415'}[24].
- Q93041219's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.704'}[25].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].