Q84518192
emission-line star in the constellation Sagittarius
Press Enter · cited answer in seconds
0 sources
Q84518192
Summary
Q84518192 is an emission-line star[1].
Key Facts
- Q84518192's instance of is recorded as emission-line star[2].
- Q84518192's constellation is recorded as Sagittarius[3].
- Q84518192 is part of NGC 6530[4].
- Q84518192's catalog code is recorded as GES J18025223-2411262[5].
- Q84518192's catalog code is recorded as VPHAS J180252.2-241126.2[6].
- Q84518192's catalog code is recorded as Gaia DR2 4066039667928139264[7].
- Q84518192's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.16'}[8].
- Q84518192's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.07'}[9].
- Q84518192's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.47'}[10].
- Q84518192's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.47'}[11].
- Q84518192's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.3096'}[12].
- Q84518192's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9289'}[13].
- Q84518192's metallicity is recorded as {'unit': '1', 'amount': '-0.02'}[14].
- Q84518192's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+270.71760034228400'}[15].
- Q84518192's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-24.19061030467600'}[16].
- Q84518192's epoch is recorded as J2000.0[17].
- Q84518192's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4384'}[18].
- Q84518192's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.622'}[19].
- Q84518192's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.517'}[20].
Body
Definition and Type
Q84518192's instance of is recorded as emission-line star[2].
Use and Application
Q84518192 is part of NGC 6530[4].