HD96632

Summary

HD96632 is a peculiar star^[1].

Key Facts

• HD96632's instance of is recorded as peculiar star^[2].
• HD96632's instance of is recorded as high proper-motion star^[3].
• HD96632's constellation is recorded as Centaurus^[4].
• HD96632's spectral class is recorded as A2mA5-A9^[5].
• HD96632's catalog code is recorded as HD 96632^[6].
• HD96632's catalog code is recorded as CCDM J11074-4814A^[7].
• HD96632's catalog code is recorded as CPC 0 9246^[8].
• HD96632's catalog code is recorded as GSC 08204-00740^[9].
• HD96632's catalog code is recorded as IDS 11029-4742 A^[10].
• HD96632's catalog code is recorded as 2MASS J11072274-4814439^[11].
• HD96632's catalog code is recorded as PPM 316076^[12].
• HD96632's catalog code is recorded as SAO 222582^[13].
• HD96632's catalog code is recorded as WDS J11074-4815A^[14].
• HD96632's catalog code is recorded as TYC 8204-740-1^[15].
• HD96632's catalog code is recorded as Gaia DR1 5362281649901956608^[16].
• HD96632's catalog code is recorded as Gaia DR2 5362281654199753984^[17].
• HD96632's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.52'}^[18].
• HD96632's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.29'}^[19].
• HD96632's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.2599'}^[20].
• HD96632's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.877'}^[21].
• HD96632's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.862'}^[22].
• HD96632's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.799'}^[23].
• HD96632's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.8456'}^[24].
• HD96632's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+206.3728'}^[25].
• HD96632's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+166.84473700358880'}^[26].

Body

Definition and Type

Recorded instance of include peculiar star^[2] and high proper-motion star^[3].