Sand!
Sand! is a 1920 American silent Western film directed by Lambert Hillyer and written by Lambert Hillyer based upon the Russell A. Boggs short story "Dan Kurrie’s Inning." The film stars William S. Hart, Mary Thurman, G. Raymond Nye, Patricia Palmer, Bill Patton, and S.J. Bingham. The film was released on June 20, 1920, by Paramount Pictures.
Cast
Survival status
Copies of the film are in the Library of Congress and George Eastman House Motion Picture Collection.
References
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Sand (Herrndorf novel)
Sand is a 2011 novel by the German writer Wolfgang Herrndorf. It won the Leipzig Book Fair Prize in 2012.
See also
References
External links
Sand (film)
Sand is 2000 thriller comedy film, directed and written by Matt Palmieri. Starring Michael Vartan, Norman Reedus, Kari Wührer, Harry Dean Stanton, Emilio Estevez, Denis Leary, Jon Lovitz and Julie Delpy.
Plot
The Briggs family comes together for the first time in over 20 years to attend the funeral and read the will of Marina (Kayle Martin). It is a very uneasy experience for Tyler (Michael Vartan), her son.
Having been abandoned by his father Gus (Marshall Bell) when he was an infant, Tyler grew up only with his mother Marina and felt no real ties to Gus or his two stepbrothers Barker (Rodney Eastman) and Hardy (John Hawkes), who were not only alcoholic cocaine addicts but also very ill-mannered and an embarrassment.
Tyler disliked Gus' good friend and travel companion "Boston" Teddy (Denis Leary), whose obsession with the Kennedy family of Hyannis Port, Massachusetts, as well as John F. Kennedy's sexual exploits in and out of the White House even disturbed Gus.
Marina left her son Tyler everything that she had. Tyler, in a show of good faith, only took the White 1972 Ford LTD and a photo album and left everything else, the house and $6,000, to his father Gus. Tyler then took off for the coast to where Marina was born and raised to get away from the "family" in solitude.
The Witch (ballet)
The Witch is a ballet made by John Cranko to Maurice Ravel's Piano Concerto No. 2 in G Major (1931). The premiere took place Friday, 18 August 1950 at the Royal Opera House, Covent Garden, London.
Original Cast
External links
Hag
A hag is a wizened old woman, or a kind of fairy or goddess having the appearance of such a woman, often found in folklore and children's tales such as Hansel and Gretel. Hags are often seen as malevolent, but may also be one of the chosen forms of shapeshifting deities, such as the Morrígan or Badb, who are seen as neither wholly beneficent nor malevolent.
Etymology
The term appears in Middle English, and was a shortening of hægtesse, an Old English term for witch, similarly the Dutch heks and German Hexe are also shortenings, of the Middle Dutch haghetisse and Old High German hagzusa respectively. All these words derive from the Proto-Germanic *hagatusjon- which is of unknown origin, however the first element may be related to the word "hedge". As a stock character in fairy or folk tale, the hag shares characteristics with the crone, and the two words are sometimes used as if interchangeable.
Using the word "hag" to translate terms found in non-English (or non-modern English) is contentious, since use of the word is often associated with a misogynistic attitude.
Araotes lapithis
The Witch, Araotes lapithis, is a small butterfly found in India that belongs to the Lycaenids or Blues family.
References
Parallax
Parallax is a displacement or difference in the apparent position of an object viewed along two different lines of sight, and is measured by the angle or semi-angle of inclination between those two lines. The term is derived from the Greek word παράλλαξις (parallaxis), meaning "alteration". Due to foreshortening, nearby objects have a larger parallax than more distant objects when observed from different positions, so parallax can be used to determine distances.
Astronomers use the principle of parallax to measure distances to the closer stars. Here, the term "parallax" is the semi-angle of inclination between two sight-lines to the star, as observed when the Earth is on opposite sides of the Sun in its orbit. These distances form the lowest rung of what is called "the cosmic distance ladder", the first in a succession of methods by which astronomers determine the distances to celestial objects, serving as a basis for other distance measurements in astronomy forming the higher rungs of the ladder.
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