Q87903753
long period variable
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Q87903753
Summary
Q87903753 is a long-period variable star[1].
Key Facts
- Q87903753's instance of is recorded as long-period variable star[2].
- Q87903753's instance of is recorded as infrared source[3].
- Q87903753's instance of is recorded as near-infrared source[4].
- Q87903753's constellation is recorded as Cygnus[5].
- Q87903753's spectral class is recorded as M4.5[6].
- Q87903753's catalog code is recorded as GSC 03137-01721[7].
- Q87903753's catalog code is recorded as IRAS 19538+3807[8].
- Q87903753's catalog code is recorded as 2MASS J19554114+3816043[9].
- Q87903753's catalog code is recorded as Gaia DR2 2072513864297647488[10].
- Q87903753's catalog code is recorded as PR Cyg[11].
- Q87903753's catalog code is recorded as TIC 171415301[12].
- Q87903753's catalog code is recorded as Gaia DR3 2072513864297647488[13].
- Q87903753's type of variable star is recorded as slow irregular variables of late spectral types[14].
- Q87903753's type of variable star is recorded as long-period variable star[15].
- Q87903753's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.560'}[16].
- Q87903753's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.134'}[17].
- Q87903753's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.146'}[18].
- Q87903753's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.738'}[19].
- Q87903753's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.111308'}[20].
- Q87903753's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1154'}[21].
- Q87903753's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-2.96'}[22].
- Q87903753's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+298.9214783318'}[23].
- Q87903753's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+38.26790672812'}[24].
- Q87903753's epoch is recorded as J2000.0[25].
- Q87903753's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.955'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].