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Envisioning arcs of moondust at Neptune.


Envisioning arcs of moondust at Neptune

As Voyager 2 approaches its Aug. 24 rendezvous with Neptune, scientists wait eagerly to see whether the spacecraft will confirm that the planet possesses the strangest set of rings known in the solar system solar system, the sun and the surrounding planets, natural satellites, dwarf planets, asteroids, meteoroids, and comets that are bound by its gravity. The sun is by far the most massive part of the solar system, containing almost 99.9% of the system's total mass. .

About a decade ago, in studying the way a star's light blinked off and on as Neptune got in the way, Peter Goldreich Peter Goldreich (born July 14, 1939) is an American astrophysicist whose research focuses on planetary rings, helioseismology and neutron stars.[1] He is currently the Lee DuBridge Professor of Astrophysics and Planetary Physics at California Institute of Technology.  and Scott Tremaine Scott Tremaine (born 1950)[1] is a Canadian-born astrophysicist. He is a fellow of the Royal Society of London, the Royal Society of Canada and the National Academy of Sciences.  of the California Institute of Technology California Institute of Technology, at Pasadena, Calif.; originally for men, became coeducational in 1970; founded 1891 as Throop Polytechnic Institute; called Throop College of Technology, 1913–20.  in Pasadena concluded that the planet has rings--but that unlike the rings of Jupiter This article is included in the list of featured articles.

The rings of Jupiter is a system of planetary rings around the planet Jupiter.
, Saturn and Uranus, Neptune's might consist of short, unconnected arcs. Now Goldreich heads a research group proposing that if the arcs actually exist, as Voyager's photos should show, they may consist of debris left over from the destruction of some of Neptune's moons.

The source of this moon wreckage would be Neptune's big satellite Triton, say Goldreich and Caltech colleagues Norman Murray, Pierre-Yves Longaretti and Donald Banfield in the Aug. 4 SCIENCE. They propose that Triton originally formed in an orbit around the sun and was later gravitationally grav·i·ta·tion  
n.
1. Physics
a. The natural phenomenon of attraction between physical objects with mass or energy.

b. The act or process of moving under the influence of this attraction.

2.
 captured by Neptune as the result of a collision with another of the planet's moons. This left Triton in an orbit that gradually became more steeply tilted. In such an orbit, Triton circled Neptune and collided with a number of the planet's smaller satellites.

Triton could have gone around this path as many as 100 million times, picking off lesser moons all the while, says Goldreich. As a result, the researchers calculate, Triton "cannibalized" most of the satellites then orbiting Neptune at distances between about five and 200 times the planet's radius, which spans approximately 15,000 miles.

"Close to the planet, in the region where Triton never penetrated, regular satellites might still survive," the group concludes. "If comparison with the satellite systems of other giant planets is an accurate guide, several satellites must have formed in this region."

By Aug. 1, Voyager 2 scientists had identified only one moon other than the pair (Triton and Nereid) detected from Earth. But the craft had discovered no more moons at the other giant planets while at a similar distance from them.

The debris resulting from Triton's collisions would be confined con·fine  
v. con·fined, con·fin·ing, con·fines

v.tr.
1. To keep within bounds; restrict: Please confine your remarks to the issues at hand. See Synonyms at limit.
 in individual arcs, rather than a continuous ring, by "resonances" located at the balance points of the gravitational grav·i·ta·tion  
n.
1. Physics
a. The natural phenomenon of attraction between physical objects with mass or energy.

b. The act or process of moving under the influence of this attraction.

2.
 attractions of Neptune, Triton and perhaps several other satellites, say Goldreich and his colleagues. They base this whole idea on observations of stellar light blockages, or occultations, during only two occasions. Nonetheless, the group estimates from the limited data that Neptune may possess 10 to 100 arcs. The arcs would measure from a few tens of miles to thousands of miles long, laid out like segments of what would otherwise be a continuous ring. Holding them in place might require "a large number" of additional satellites, the researchers suggest.

On the other hand, the group also suggests that all the arcs might be held in position by resonances associated with a single moon, which they call Satellite X. If one Satellite X is indeed responsible, they speculate, its orbit is most likely tilted or elliptical el·lip·tic   or el·lip·ti·cal
adj.
1. Of, relating to, or having the shape of an ellipse.

2. Containing or characterized by ellipsis.

3.
a.
. Tides caused on Triton by Neptune could have made Triton almost entirely molten during most of its unusual orbital evolution, they conclude.
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Copyright 1989, Gale Group. All rights reserved. Gale Group is a Thomson Corporation Company.

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Author:Eberhart, J.
Publication:Science News
Date:Aug 5, 1989
Words:538
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