HD136150
star
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HD136150
Summary
HD136150 is a star[1].
Key Facts
- HD136150's instance of is recorded as star[2].
- HD136150's instance of is recorded as Alpha² Canum Venaticorum variable[3].
- HD136150's instance of is recorded as infrared source[4].
- HD136150's constellation is recorded as Lupus[5].
- HD136150's spectral class is recorded as ApSi[6].
- HD136150's catalog code is recorded as HD 136150[7].
- HD136150's catalog code is recorded as GSC 08298-01704[8].
- HD136150's catalog code is recorded as 2MASS J15205036-4731423[9].
- HD136150's catalog code is recorded as SAO 225674[10].
- HD136150's catalog code is recorded as CD-47 9901[11].
- HD136150's catalog code is recorded as CPC 0 13214[12].
- HD136150's catalog code is recorded as CPD-47 7060[13].
- HD136150's catalog code is recorded as PPM 320484[14].
- HD136150's catalog code is recorded as TYC 8298-1704-1[15].
- HD136150's catalog code is recorded as Gaia DR1 5902991403674220032[16].
- HD136150's catalog code is recorded as Gaia DR2 5902991407994010240[17].
- HD136150's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.92'}[18].
- HD136150's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.83'}[19].
- HD136150's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.8418'}[20].
- HD136150's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.674'}[21].
- HD136150's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.691'}[22].
- HD136150's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.660'}[23].
- HD136150's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9594'}[24].
- HD136150's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1042.3181'}[25].
- HD136150's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+230.20982111382910'}[26].
Body
Definition and Type
Recorded instance of include star[2], Alpha² Canum Venaticorum variable[3], and infrared source[4].