Q88084095
star in the constellation Scorpius
Press Enter · cited answer in seconds
0 sources
Q88084095
Summary
Q88084095 is a star[1].
Key Facts
- Q88084095's instance of is recorded as star[2].
- Q88084095's constellation is recorded as Scorpius[3].
- Q88084095's spectral class is recorded as K7[4].
- Q88084095's catalog code is recorded as GSC 07385-00083[5].
- Q88084095's catalog code is recorded as TYC 7385-83-1[6].
- Q88084095's catalog code is recorded as CD-34 11980[7].
- Q88084095's catalog code is recorded as CPD-34 6991[8].
- Q88084095's catalog code is recorded as HD 320454[9].
- Q88084095's catalog code is recorded as Gaia DR1 4041383802549841152[10].
- Q88084095's catalog code is recorded as Gaia DR2 4041383802549841152[11].
- Q88084095's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.19'}[12].
- Q88084095's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.36'}[13].
- Q88084095's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.4334'}[14].
- Q88084095's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0981'}[15].
- Q88084095's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-16.73'}[16].
- Q88084095's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+910.6639'}[17].
- Q88084095's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+265.76647864841390'}[18].
- Q88084095's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-34.85954002336750'}[19].
- Q88084095's epoch is recorded as J2000.0[20].
- Q88084095's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.333'}[21].
- Q88084095's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+3.913'}[22].
Body
Definition and Type
Q88084095's instance of is recorded as star[2].