Mira B

Summary

Mira B is a white dwarf^[1]. It draws 155 Wikipedia views per month (white_dwarf category, ranking #3 of 16).^[2]

Key Facts

• Mira B's instance of is recorded as white dwarf^[3].
• Mira B's instance of is recorded as variable star^[4].
• Mira B's instance of is recorded as astrophysical X-ray source^[5].
• Mira B's constellation is recorded as Cetus^[6].
• Mira B's spectral class is recorded as DA^[7].
• Mira B is part of Mira^[8].
• Mira B's companion of is recorded as Mira A^[9].
• Mira B's catalog code is recorded as VZ Cet^[10].
• Mira B's catalog code is recorded as WDS J02193-0259Ab^[11].
• Mira B's catalog code is recorded as CCDM J02194-0258P^[12].
• Mira B's right ascension is recorded as {'unit': 'Q28390', 'amount': '+34.836667'}^[13].
• Mira B's declination is recorded as {'unit': 'Q28390', 'amount': '-2.977778'}^[14].
• Mira B's epoch is recorded as J2000.0^[15].

Body

Geography

Mira B is part of Mira^[8].

Designation and Status

Recorded instance of include white dwarf^[3], variable star^[4], and astrophysical X-ray source^[5].

History and Context

Catalog codes include VZ Cet^[10], WDS J02193-0259Ab^[11], and CCDM J02194-0258P^[12].

Why It Matters

Mira B draws 155 Wikipedia views per month (white_dwarf category, ranking #3 of 16).^[2] It has Wikipedia articles in 6 language editions, a strong signal of global cultural recognition.^[16] It is known by 27 alternative names across languages and contexts.^[17]