Aldebaran
red giant star in the constellation Taurus
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Aldebaran
Summary
Aldebaran is a red giant[1].
Key Facts
- Aldebaran's image is recorded as Occultation.jpg[2].
- Aldebaran's image is recorded as Taurus - Prodromus astronomiae 1690 (5590444).jpg[3].
- Aldebaran's image is recorded as Aldebaran.jpg[4].
- Aldebaran's instance of is recorded as red giant[5].
- Aldebaran's instance of is recorded as variable star[6].
- Aldebaran's instance of is recorded as near-infrared source[7].
- Aldebaran's instance of is recorded as high proper-motion star[8].
- Aldebaran's instance of is recorded as ultraviolet source[9].
- Aldebaran's instance of is recorded as double star[10].
- Aldebaran's constellation is recorded as Taurus[11].
- Aldebaran's spectral class is recorded as K5III[12].
- Aldebaran's part of is recorded as Winter Hexagon[13].
- Aldebaran's part of is recorded as Aldebaran[14].
- Aldebaran's Commons category is recorded as Aldebaran[15].
- Aldebaran's child astronomical body is recorded as Aldebaran b[16].
- Aldebaran's catalog code is recorded as 2MASS J04355524+1630331[17].
- Aldebaran's catalog code is recorded as GSC 01266-01416[18].
- Aldebaran's catalog code is recorded as HD 29139[19].
- Aldebaran's catalog code is recorded as HIP 21421[20].
- Aldebaran's catalog code is recorded as HR 1457[21].
- Aldebaran's catalog code is recorded as IRAS 04330+1624[22].
- Aldebaran's catalog code is recorded as SAO 94027[23].
- Aldebaran's catalog code is recorded as GJ 171.1 A[24].
- Aldebaran's catalog code is recorded as GJ 9159 A[25].
- Aldebaran's catalog code is recorded as α Tau[26].
Body
Geography
Part of include Winter Hexagon[13], an asterism[27] and Aldebaran[14], a binary star[28].
Designation and Status
Recorded instance of include red giant[5], variable star[6], near-infrared source[7], high proper-motion star[8], ultraviolet source[9], and double star[10].
History and Context
Catalog codes include 2MASS J04355524+1630331[17], GSC 01266-01416[18], HD 29139[19], HIP 21421[20], HR 1457[21], and IRAS 04330+1624[22].