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Encyclopedia > Epsilon Tauri
ε Tauri
Observation data
Equinox J2000.0
Constellation Taurus
Right ascension 04h 28m 37.0s
Declination +19° 10' 49"
Apparent magnitude (V) +3.53
Distance 155 ± 6 ly
(48 ± 2 pc)
Spectral type K0III
Other designations
Ain, Oculus Borealus,
74 Tauri, HR 1409,
HD 28305, BD+18 640,
FK5 164, HIP 20889,
SAO 93954, GC 5430,
CCDM 04286+1911

Epsilon Tauri (ε Tau / ε Tauri) is a star in the constellation Taurus and a member of the Hyades open cluster. It has the traditional names Ain (Arabic عين), or Oculus Borealus, both of which mean "eye". Another traditional name is Coronis (Greek Κορωνις), referring to one of the Hyades sisters. From the Glossary of Astronomical Terms by the Harvard-Smithsonian Center for Astrophysics: Either of the two points (vernal, autumnal) on the celestial sphere where the ecliptic (which is the apparent path of the sun on the sky) intersects the celestial equator. ... It has been suggested that this article or section be merged into Julian epoch. ... This article or section does not cite its references or sources. ... For other uses of the word Taurus see Taurus. ... Equatorial Coordinates Right ascension (abbrev. ... In astronomy, declination (abbrev. ... // Headline text HEY!! HOW ARE YOU ALL?? Its nice of you to come read this page. ... This article is in need of attention from an expert on the subject. ... A light-year or lightyear, symbol ly, is a unit of length. ... Stellar parallax motion The parsec (symbol pc) is a unit of length used in astronomy. ... In astronomy, stellar classification is a classification of stars based initially on photospheric temperature and its associated spectral characteristics, and subsequently refined in terms of other characteristics. ... In astronomy, many stars are referred to simply by catalogue numbers. ... In astronomy, many stars are referred to simply by catalogue numbers. ... The Henry Draper Catalogue is an astronomy catalogue with astrometric and spectroscopic data about more than 225,000 stars. ... In astronomy, many stars are referred to simply by catalogue numbers. ... In astronomy, many stars are referred to simply by catalogue numbers. ... In astronomy, many stars are referred to simply by catalogue numbers. ... This article is about the astronomical object. ... This article or section does not cite its references or sources. ... For other uses of the word Taurus see Taurus. ... The Hyades (‘Υάδες) are an open star cluster located in the constellation Taurus. ... The Pleiades is one of the most famous open clusters. ... Arabic ( or just ), is the largest member of the family of Semitic branch of the Afro-Asiatic language family (classification: South Central Semitic) and is closely related to Hebrew, Amharic, and Aramaic. ...


ε Tau belongs to the spectral class K0 and has apparent magnitude +3.6. It is 155 light years away from the Sun, has a luminosity of 90 times that of the Sun and a radius of 13 times solar. The surface temperature of this star is measured at 4925 kelvins. It has an 11th magnitude companion 182 arcseconds from the primary. In astronomy, stellar classification is a classification of stars based initially on photospheric temperature and its associated spectral characteristics, and subsequently refined in terms of other characteristics. ... // Headline text HEY!! HOW ARE YOU ALL?? Its nice of you to come read this page. ... A light-year or lightyear, symbol ly, is a unit of length. ... The Sun is the star at the center of the Solar System. ... Luminosity has different meanings in several different fields of science. ... The Kelvin scale is a thermodynamic (absolute) temperature scale where absolute zero—the lowest possible temperature where nothing could be colder and no heat energy remains in a substance—is defined as zero kelvin (0 K). ... A second of arc or arcsecond is a unit of angular measurement which comprises one-sixtieth of an arcminute, or 1/3600 of a degree of arc or 1/1296000 ≈ 7. ...


Since ε Tau lies near the plane of the ecliptic, it is sometimes occulted by the Moon and (very rarely) by planets. The plane of the ecliptic is well seen in this picture from the 1994 lunar prospecting Clementine spacecraft. ... In this July, 1997 still frame captured from video, the bright star Aldebaran has just reappeared on the dark limb of the waning crescent moon in this predawn occultation. ... Apparent magnitude: up to -12. ... For the astrological concept, see Planets in astrology. ...


Refences

  • HD 28305 -- Star in double system. SIMBAD Astronomical Database. Retrieved on 2007-01-25.

2007 (MMVII) is the current year, a common year starting on Monday of the Gregorian calendar and the AD (or CE) era. ... January 25 is the 25th day of the year in the Gregorian calendar. ...

External Links

  • Star Names

  Results from FactBites:
 
T Tauri - Wikipedia, the free encyclopedia (274 words)
T Tauri is a variable star in the constellation Taurus, the prototype of the T Tauri stars.
Through VLA radio observations, it was found that the young star (the "T Tauri star" itself) dramatically changed its orbit after a close encounter with one of its companions and may have been ejected from the system.
The nebula NGC 1554 was likewise associated with T Tauri and was observed in 1968 by Otto Struve, but soon disappeared or perhaps never existed, and is known as "Struve's Lost Nebula".
AAVSO: T Tauri, February 2001 Variable Star Of The Month (2432 words)
This spectral feature is seen in the atmospheres of the T Tauri stars, which implies, in the astronomical sense, that T Tauri stars are a young, low-mass stars that are contracting as they evolve toward the main sequence stage of stellar evolution.
He chose T Tauri to be the protoype of the class since "it is best known, is among the brightest, and represents the group with respect to both emission and absorption spectra." Up to this point, these stars had been classified as irregular variables.
While T Tauri variations may result from instabilities within and interactions with the surrouding accretion disk, FU Orionis (also known as FUors) activity results from a dramatic increase in instability and the dumping of large amounts of matter on the accompanying star (Kaler 1999).
  More results at FactBites »


 
 

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