Aldebaran
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- For the Fallen Angel Aldebaran, see Aldebaran (demon); and distinguish from Alderaan.
| Observation data Equinox J2000.0 |
|
|---|---|
| Constellation | Taurus |
| Right ascension | 04h 35m 55.2s |
| Declination | +16° 30' 33" |
| Apparent magnitude (V) | +0.85 / +13.50 |
| Characteristics | |
| Spectral type | K5III / M2V |
| U-B color index | 1.90 / ? |
| B-V color index | 1.54 / ? |
| Variable type | Suspected / ? |
| Astrometry | |
| Radial velocity (Rv) | +53.8 km/s |
| Proper motion (μ) | RA: 62.78 mas/yr Dec.: −189.36 mas/yr |
| Parallax (π) | 50.09 ± 0.95 mas |
| Distance | 65 ± 1 ly (20 ± 0.4 pc) |
| Absolute magnitude (MV) | −0.63 / 11.98 |
| Details | |
| Mass | 2.5 / 0.15 M☉ |
| Radius | 25 / 0.04 R☉ |
| Luminosity | 150 / 0.00014 L☉ |
| Temperature | 4,100 / 3,050 K |
| Metallicity | 70% Sun / ? |
| Rotation | |
| Age | years |
| Other designations | |
| Database references | |
| SIMBAD | data |
Aldebaran from the Arabic (الدبران al-dabarān) meaning "the follower", (α Tau / α Tauri / Alpha Tauri) is the brightest star in the constellation Taurus and one of the brightest stars in the nighttime sky. Because of its location in the head of Taurus, it has historically been called the Bull's Eye.
Its name refers to the way the star follows the Pleiades star cluster in its nightly journey across the sky. Aldebaran has the appearance of being the brightest member of the more scattered Hyades cluster, which is the closest star cluster to Earth. However, it is merely located in the line of sight between the Earth and the Hyades, and is actually an independent star.
It is known as 畢宿五 (Bìxiùwŭ, the Fifth Star of the Net) in Chinese.
Aldebaran is a K5 III star, which means it is orangish, large, and has moved off of the main sequence by using all its hydrogen fuel. It has a minor companion (a dim M2 dwarf orbiting at several hundred AU). Now primarily fusing helium, the main star has expanded to a diameter of approximately 5.3 × 107 km, or about 38 times the diameter of the Sun. The Hipparcos satellite has measured it as 65.1 light years away, and it shines with 150 times the Sun's luminosity. Taken together this distance and brightness makes it the 14th brightest star, having an apparent magnitude of 0.87. It is slightly variable, of the irregular variable type, by about 0.2 magnitude.
In 1997, a possible large planet (or small brown dwarf) companion was reported, with a mass equalling that of 11 Jupiters and orbiting at a distance of 1.35 AU. However, see below.
Aldebaran is one of the easiest stars to find in the night sky, partly due to its brightness and partly due to its spatial relation to one of the more noticeable asterisms in the sky. If one follows the three stars of Orion's belt from left to right (in the Northern Hemisphere) or right to left (in the Southern), the first bright star found by continuing that line is Aldebaran.
Contents |
[edit] Radial velocity variations
| Discovery | |
|---|---|
| Discovered by: | Hatzes et al. |
| Discovery date: | 1997 |
| Detection method(s): | Doppler Spectroscopy |
| Orbital characteristics | |
| Semi-major axis: | ~2 AU |
| Eccentricity: | 0.182±0.065 |
| Orbital period: | 653.8±10.1 d |
| Longitude of the periastron: | 290.2±4.9° |
| Time of periastron: | 2,447,625.4±7.8 JD |
| Physical characteristics | |
| Mass: | ~11 MJ |
In 1993, radial velocity measurements of Aldebaran A, Arcturus and Pollux showed that Aldebaran A exhibited a long-period radial velocity oscillation, which could be interpreted as a substellar companion with a minimum mass 11.4 times that of Jupiter in a 643-day orbit at a separation of 2.0 AU in an eccentric orbit (eccentricity 0.147) [1]. However, all three stars surveyed showed similar oscillations yielding similar companion masses, and the authors concluded that the variation was likely to be intrinsic to the star rather than due to the gravitational effect of a companion.
An analysis of the spectrum of Aldebaran A [2] did not show any variation correlated to the 643-day radial velocity oscillation, which would be expected if the cause was intrinsic. The best orbital solution was found to be around 653.8 days with an eccentricity of 0.182, and a lower mass limit of 11 Jupiter masses. The high value for the minimum mass means that it is likely that the object, if it exists, exceeds 13 Jupiter masses and is therefore a brown dwarf. However the possibility that the oscillation is due to a pulsation or combination of pulsations still exists, and as of 2006, this companion has not been confirmed.
[edit] Aldebaran in mythology
For the Dakotas (a branch of the Native American Sioux tribe), Aldebaran took on a heroic aspect. The young star was the child of the sun and the lady Blue Star. One day he desired to hunt the white buffalo (the Pleiades). After he pulled up a sapling to make a spear, a hole was made in the ground and he could see all the people of earth down below. The white buffalo took this chance to push him through. He was found by an old woman and was to be known as Old Woman's Grandson. On earth he killed many strange monsters which had been troubling the Native Americans; one monster of which was a serpent that caused drought; he killed it releasing a great stream of water that became the Mississippi River. In time, Old Woman's Grandson remembered the white buffalo and returned to hunting him in the sky to fulfill his destiny.
For the Seris of northwestern Mexico, this star is providing light for the seven women giving birth (Pleiades). It has three different names: Hant Caalajc Ipápjö, Queeto, and Azoj Yeen oo Caap ("star that goes ahead"). The lunar month corresponding to October is called Queeto yaao "Aldebaran's path".[1]
In the religion of Stregheria, Aldebaran is a fallen angel and quarter guardian of the eastern gate.
Aldebaran was thought to be a possible origin point for the Übermenschen in Nazi mysticism. The Rolling Stones refer to this star by name in the song "2,000 Light Years From Home".
[edit] References
- ^ Moser, Mary B.; Stephen A. Marlett (2005). Comcáac quih yaza quih hant ihíip hac: Diccionario seri-español-inglés (in Spanish and English). Hermosillo, Sonora and Mexico City: Universidad de Sonora and Plaza y Valdés Editores.
[edit] See also
[edit] External links
- Gl 171.1A. ARICNS. Retrieved on 14 November, 2005.
- Aldebaran 2. SolStation. Retrieved on 14 November, 2005.
