HD15476
star in the constellation Cetus
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HD15476
Summary
HD15476 is a star[1].
Key Facts
- HD15476's instance of is recorded as star[2].
- HD15476's instance of is recorded as infrared source[3].
- HD15476's constellation is recorded as Cetus[4].
- HD15476's spectral class is recorded as A1/2mA5-F0[5].
- HD15476's catalog code is recorded as HD 15476[6].
- HD15476's catalog code is recorded as BD-07 440[7].
- HD15476's catalog code is recorded as 2MASS J02292303-0704131[8].
- HD15476's catalog code is recorded as SAO 129934[9].
- HD15476's catalog code is recorded as GSC 04697-00198[10].
- HD15476's catalog code is recorded as PPM 184680[11].
- HD15476's catalog code is recorded as RAVE J022923.0-070413[12].
- HD15476's catalog code is recorded as TYC 4697-198-1[13].
- HD15476's catalog code is recorded as YZ 97 551[14].
- HD15476's catalog code is recorded as Gaia DR1 5178403207923272192[15].
- HD15476's catalog code is recorded as Gaia DR2 5178403212218764928[16].
- HD15476's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.44'}[17].
- HD15476's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.23'}[18].
- HD15476's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2572'}[19].
- HD15476's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.980'}[20].
- HD15476's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.953'}[21].
- HD15476's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.906'}[22].
- HD15476's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.2039'}[23].
- HD15476's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+53.82'}[24].
- HD15476's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+453.7411'}[25].
- HD15476's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.34598183303850'}[26].
Body
Definition and Type
Recorded instance of include star[2] and infrared source[3].