A comet's odd orbit hints at hidden planet. (Science News of the week).Far beyond the solar system's nine known planets, a body as massive as Mars may once have been part of our planetary system--and it might still be there. Although the proposed planet would lie too far away to be seen from Earth, its 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. tug could account for the oddball orbit of a large comet spotted in the outer 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. a year ago. Known as 2000 C[R.sub.105], the comet moves about the sun in a much more elongated e·lon·gate tr. & intr.v. e·lon·gat·ed, e·lon·gat·ing, e·lon·gates To make or grow longer. adj. or elongated 1. Made longer; extended. 2. Having more length than width; slender. pathway than originally thought, astronomers now find. Observations over the past year by Brett Gladman of the Observatoire de la Cote d'Azur in Nice, France, and his colleagues show that the comet's orbit takes it further than 200 astronomical units (AU) from the sun and as close as 44 AU. One AU equals the Earth-sun distance of about 150 million kilometers. Such an oblong orbit is usually a sign that an object has come under the gravitational influence of a massive body. But 2000 C[R.sub.105], which may be an escapee escapee A popular term for older relatives of those at risk for Huntington's disease, who didn't develop the disease. See Huntington's disease. from the distant reservoir of comets known as the Kuiper belt Kuiper belt: see comet; Kuiper, Gerard Peter. Kuiper belt or Edgeworth-Kuiper belt Disk-shaped belt of billions of small icy bodies orbiting the Sun beyond the orbit of Neptune, mostly at distances 30–50 times Earth's distance , never gets anywhere near any of the solar system's familiar team of nine planets. Even at its closest approach to the sun, the approximately 400-km-wide ball of ice comes no closer than 14 AU to Neptune, the nearest known candidate for a significant gravitational interaction gravitational interaction n. A weak, fundamental interaction between two physical objects due to their mass and energy, especially an interaction occurring between elementary particles. Noun 1. . The astronomers concede that feeble and random pushes from Neptune could have slowly nudged 2000 C[R.sub.105] into its current orbit. However, preliminary analysis suggests this scenario isn't likely, note Gladman, Matthew Holman of the Harvard-Smithsonian Center for Astrophysics The Harvard-Smithsonian Center for Astrophysics (CfA) is located in Cambridge, Massachusetts. It consists of the Harvard College Observatory and the Smithsonian Astrophysical Observatory. The Center is located at 60 Garden Street. in Cambridge, Mass., and their collaborators. In an article the researchers recently posted on the Internet (http://arXiv.org/ abs/astro-ph/0103435), they suggest that a massive body lurking among the tiny, frozen residents of the Kuiper belt could have been the culprit. That object could have been Neptune itself. According to one theory, Neptune and Uranus first formed between the orbits of Jupiter and Saturn and were then flung out to greater distances from the sun. If that kick propelled Neptune into the Kuiper belt before the planet settled into its current nearly circular orbit, its gravity could have caused the orbits of several objects like 2000 C[R.sub.105] to stretch into elongated trajectories. Alternatively, the comet's orbit could be the handiwork of an as-yet-unseen planet whose mass lies somewhere between that of Earth's moon and Mars, the researchers say. It's likely that such an object would have coalesced co·a·lesce intr.v. co·a·lesced, co·a·lesc·ing, co·a·lesc·es 1. To grow together; fuse. 2. To come together so as to form one whole; unite: in the outer solar system from the same debris that formed Neptune, Uranus, and the cores of Jupiter and Saturn, Holman notes. There's only a 1 percent chance that a planet could have survived in the Kuiper belt or its surroundings over the 4.5-billion-year age of the solar system, says Holman. If the planet found a secluded nook of the belt, however, it could remain intact today. If the proposed planet is as massive as Mars, it would have to lie some 200 AU from the sun--about 7 times Neptune's distance--Holman calculates. Were it closer, observers would have spotted it. A planet lurking in the Kuiper belt now or in the past might also explain why many members of the belt have orbits that angle away from the plane in which the nine known planets orbit the sun. "Undoubtedly, something [massive] knocked the hell out of the belt," says Harold F. Levison Harold F. "Hal" Levison is a planetary scientist specializing in planetary dynamics. He argued for a distinction between what are now called dwarf planets and the other eight planets based on their inability to "clear the neighborhood around their orbits," although his proposal of the Southwest Research Institute Southwest Research Institute (SwRI), headquartered in San Antonio, Texas, is one of the oldest and largest independent, nonprofit, applied research and development (R&D) organizations in the United States. Founded in 1947 by Thomas Slick, Jr. in Boulder, Colo. "The question is whether it's there now." The stability of the orbit of 2000 C[R.sub.105] suggests that any planet that influenced the comet's path has long since departed. If astronomers find a family of objects similar to 2000 C[R.sub.105], the nature of their orbits could indicate whether the hidden planet is in fact still there, Levison says. |
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