Q93894434
long period variable
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Q93894434
Summary
Q93894434 is a long-period variable star[1].
Key Facts
- Q93894434's instance of is recorded as long-period variable star[2].
- Q93894434's constellation is recorded as Pavo[3].
- Q93894434's catalog code is recorded as CRTS J185243.0-710446[4].
- Q93894434's catalog code is recorded as IRAS 18470-7108[5].
- Q93894434's catalog code is recorded as AKARI-IRC-V1 J1852430-710446[6].
- Q93894434's catalog code is recorded as RAVE J185243.1-710446[7].
- Q93894434's catalog code is recorded as UCAC4 095-077204[8].
- Q93894434's catalog code is recorded as Gaia DR2 6418752452631285760[9].
- Q93894434's type of variable star is recorded as long-period variable star[10].
- Q93894434's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.76'}[11].
- Q93894434's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.718'}[12].
- Q93894434's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.9701'}[13].
- Q93894434's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-712.65'}[14].
- Q93894434's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+283.17958141250050'}[15].
- Q93894434's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-71.07955631609430'}[16].
- Q93894434's epoch is recorded as J2000.0[17].
- Q93894434's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+3200'}[18].
- Q93894434's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+31600'}[19].
- Q93894434's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-7.497'}[20].
- Q93894434's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.781'}[21].
Body
Definition and Type
Q93894434's instance of is recorded as long-period variable star[2].