Q88959037
high proper-motion star in the constellation Sagittarius
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Q88959037
Summary
Q88959037 is a high proper-motion star[1].
Key Facts
- Q88959037's instance of is recorded as high proper-motion star[2].
- Q88959037's constellation is recorded as Sagittarius[3].
- Q88959037's spectral class is recorded as G8/K0+G[4].
- Q88959037's catalog code is recorded as CD-31 15326[5].
- Q88959037's catalog code is recorded as CPC 17 9810[6].
- Q88959037's catalog code is recorded as CPD-31 5465[7].
- Q88959037's catalog code is recorded as GSC 07396-00020[8].
- Q88959037's catalog code is recorded as HD 167364[9].
- Q88959037's catalog code is recorded as PPM 297479[10].
- Q88959037's catalog code is recorded as SAO 209936[11].
- Q88959037's catalog code is recorded as TYC 7396-20-1[12].
- Q88959037's catalog code is recorded as 2MASS J18161340-3153510[13].
- Q88959037's catalog code is recorded as Gaia DR2 4045903757412808704[14].
- Q88959037's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.160'}[15].
- Q88959037's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.948'}[16].
- Q88959037's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.853'}[17].
- Q88959037's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.24'}[18].
- Q88959037's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.83'}[19].
- Q88959037's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0842'}[20].
- Q88959037's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.9448'}[21].
- Q88959037's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+143.9926'}[22].
- Q88959037's SIMBAD ID is recorded as HD 167364[23].
- Q88959037's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+274.05582596625520'}[24].
- Q88959037's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-31.89753779501990'}[25].
- Q88959037's epoch is recorded as J2000.0[26].