Q85442817
star in the constellation Ophiuchus
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Q85442817
Summary
Q85442817 is a star[1].
Key Facts
- Q85442817's instance of is recorded as star[2].
- Q85442817's constellation is recorded as Ophiuchus[3].
- Q85442817 is part of Messier 10[4].
- Q85442817's catalog code is recorded as Cl* NGC 6254 CGW 105[5].
- Q85442817's catalog code is recorded as 2MASS J16562614-0357472[6].
- Q85442817's catalog code is recorded as Gaia DR2 4365640884081656064[7].
- Q85442817's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.284'}[8].
- Q85442817's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.719'}[9].
- Q85442817's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.571'}[10].
- Q85442817's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2015'}[11].
- Q85442817's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8993'}[12].
- Q85442817's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+9.32'}[13].
- Q85442817's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1111.9760'}[14].
- Q85442817's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+254.10895869542670'}[15].
- Q85442817's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-3.96310783172770'}[16].
- Q85442817's epoch is recorded as J2000.0[17].
- Q85442817's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.81'}[18].
- Q85442817's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.810'}[19].
- Q85442817's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.557'}[20].
Body
Definition and Type
Q85442817's instance of is recorded as star[2].
Use and Application
Q85442817 is part of Messier 10[4].