HD174595
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HD174595
Summary
HD174595 is a star[1].
Key Facts
- HD174595's instance of is recorded as star[2].
- HD174595's instance of is recorded as infrared source[3].
- HD174595's constellation is recorded as Sagittarius[4].
- HD174595's spectral class is recorded as B9II[5].
- HD174595's catalog code is recorded as HD 174595[6].
- HD174595's catalog code is recorded as 2MASS J18520450-2036171[7].
- HD174595's catalog code is recorded as BD-20 5297[8].
- HD174595's catalog code is recorded as GSC 06289-00201[9].
- HD174595's catalog code is recorded as CPD-20 7244[10].
- HD174595's catalog code is recorded as PPM 269008[11].
- HD174595's catalog code is recorded as TYC 6289-201-1[12].
- HD174595's catalog code is recorded as YZ 110 7945[13].
- HD174595's catalog code is recorded as Gaia DR1 4085145189972146944[14].
- HD174595's catalog code is recorded as Gaia DR2 4085145194298893440[15].
- HD174595's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0367'}[16].
- HD174595's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.819'}[17].
- HD174595's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.856'}[18].
- HD174595's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.850'}[19].
- HD174595's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.16'}[20].
- HD174595's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.07'}[21].
- HD174595's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.3309'}[22].
- HD174595's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+751.3713'}[23].
- HD174595's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+283.01875398050910'}[24].
- HD174595's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-20.60474929581440'}[25].
- HD174595's epoch is recorded as J2000.0[26].
Body
Definition and Type
Recorded instance of include star[2] and infrared source[3].