Q90760603
long period variable
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Q90760603
Summary
Q90760603 is a long-period variable star[1].
Key Facts
- Q90760603's instance of is recorded as long-period variable star[2].
- Q90760603's instance of is recorded as near-infrared source[3].
- Q90760603's instance of is recorded as spectroscopic binary[4].
- Q90760603's constellation is recorded as Ophiuchus[5].
- Q90760603's catalog code is recorded as 2MASS J17533711+0425532[6].
- Q90760603's catalog code is recorded as Gaia DR2 4472762247521413248[7].
- Q90760603's catalog code is recorded as V1078 Oph[8].
- Q90760603's catalog code is recorded as TIC 324905143[9].
- Q90760603's catalog code is recorded as Gaia DR3 4472762247521413248[10].
- Q90760603's type of variable star is recorded as semiregular variable star[11].
- Q90760603's type of variable star is recorded as long-period variable star[12].
- Q90760603's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.856'}[13].
- Q90760603's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.005'}[14].
- Q90760603's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.739'}[15].
- Q90760603's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.771072'}[16].
- Q90760603's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3313'}[17].
- Q90760603's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.60'}[18].
- Q90760603's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3018.412'}[19].
- Q90760603's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+268.40465472864'}[20].
- Q90760603's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+4.4314422584'}[21].
- Q90760603's epoch is recorded as J2000.0[22].
- Q90760603's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.333'}[23].
- Q90760603's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.236'}[24].
Body
Definition and Type
Recorded instance of include long-period variable star[2], near-infrared source[3], and spectroscopic binary[4].