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Miranda: shattering an old image.


Measuring a mere 470 kilometers across, Uranus Uranus - Hideyuki Nakashima , 1993. A logic-based knowledge representation language. An extension of Prolog written in Common Lisp, with Lisp-like syntax. Extends Prolog with a multiple world mechanism, plus term descriptions to provide functional programming.

ftp://etlport.etl.go.jp/pub/uranus/ftp.
" moon Miranda (language) Miranda - (From the Latin for "admirable", also the heroine of Shakespeare's Tempest) A lazy purely functional programming language and interpreter designed by David Turner at the University of Kent in the early 1980s. It is sold by his company, Research Software Limited. It combines the main features of KRC and SASL with strong typing similar to that of ML. Implemented for Unix by Allan Grimeley, Computer Lab., UKC. has barely enough gravity to maintain its spherical shape. Yet its scarred surface seems more appropriate for a planet 10 times that size. When astronomers get their first close-up view of this icy moon, in images from the Voyager 2 spacecraft in 1986, they were struck by a strange feature--three ovoid o·voi·dal (-voidl)
n.
Something that is shaped like an egg.
adj.
Shaped like an egg; oviform.
 regions, now known as coronas
corona glan´dis pe´nis  the rounded proximal border of the glans penis.
corona radia´ta 
1. the radiating crown of projection fibers passing from the internal capsule to every part of the cerebral cortex.
2. an investing layer of radially elongated follicle cells surrounding the zona pellucida.
, that contain sets of parallel ridges, troughs, and scraps.

Researchers initially proposed that the rough-hewn surface formed because Miranda, after being struck by a comet or other large object early in the history of the solar system, shattered and then influence of Uranus' gravity. That scenario has appeared in several textbooks as well as popular accounts of Mirandahs evolution. But in reanalyzing the Voyager images, Robert T. Pappalardo, Ronald Greeley, and Stephen J. Reynolds of Arizona State University in Tempe say they have found evidence to demolish that notion.

Pappalardo and others note that if the breakup theory were correct, the moon's rocky, denser chunks would have sunk toward the reassembled core if the satellite. Internal currents created by the sinking would have formed the coronas by compressing the surface, and the ridges and troughs would represent compressional folds within the coronas. But when he and his colleagues exmained the Voyager images using a filter that highlighted Miranda's unusual topography, they found no evidence of compression.

Instead, says Pappalardo, the coronas appear to have formed atop giant upwellings of material from the moon's interior. The alternating ridges anf troughs were created when internal forces pulled the surface apart--in much the same way that such features were formed in the American Soutwest and on Jupiter's moon Ganymede

Ganymede, in astronomy

Ganymede (găn`ēmēd'), in astronomy, one of the moons, or natural satellites, of Jupiter; the largest natural satellite in the solar system, it is larger than the planet Mercury.

Ganymede, in Greek mythology

Ganymede, in Greek mythology, a youth of great beauty.
, he notes.

Images of Miranda's Arden and Inverness coronas indicate that giant blocks material, some more than 10 kilometers dominoes to create fault scraps, Pappalardo says. He suggests that tidal stretching and distortion by Uranus' gravity could have supplied the heat source necessary to fuel such uprisings.
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Copyright 1993, Gale Group. All rights reserved. Gale Group is a Thomson Corporation Company.

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Title Annotation:coronas of Uranus' Miranda formed when internal forces pulled the satellite apart
Author:Cowen, Ron
Publication:Science News
Article Type:Brief Article
Date:Nov 6, 1993
Words:328
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