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evidence for a distant giant planet in the solar system
evidence for a distant giant planet in the solar system

... We estimate the statistical significance of the observed clustering by assuming that the detection biases for our clustered objects are similar to the detection biases for the collection of all objects with q>30 AU and a>50 AU. We then randomly select six objects from the sample 100,000 times and ...
Solar Nebula
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... –  i  the  inclinaEon,  which  establishes  the  Elt  of  the  orbital  plane,  relaEve   to  the  eclipEc  plane   –  Ω  the  longitude  of  the  ascending  node  (ascending  crossover  point  of   the  orbit,  measured  with  respect ...
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... What is the biggest body in our solar system? . Sun What is the largest planet? Second largest? . Jupiter . Saturn What are the next two, which are relatively close in size? . Uranus . Neptune How do the objects in our solar system compare with each other? ...
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... Its mission is to promote and safeguard the science of astronomy in all its aspects through international cooperation. ...
Our Solar System - World Book Online
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The Outer Planets - Mr. Cramer
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... Today, we know that the orbits of the planets are only slightly elliptical, but the orbits of objects such as Pluto and comets are highly elliptical. Kepler found that a planet moves slower at aphelion, sweeping out a narrow sector on the ellipse. Conversely, a planet moves faster at perihelion, swe ...
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Chapter 24 Vocabulary link - Flushing Community Schools
Chapter 24 Vocabulary link - Flushing Community Schools

... the orbit of Neptune, 30-50 AU from the Sun. It is like the asteroid belt, but it is about 200 times as massive. Like the asteroid belt, it consists of remnants from the Solar System's formation. ...
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Jovian Planet Systems (Chapter 11) Jupiter and Saturn are mostly

... Jupiter and Saturn are mostly hydrogen, with layers of gas, liquid, and metallic hydrogen above a small rock/ice (water, methane, ammonia) core. Uranus and Neptune have a thinner outer layer of hydrogen gas, a thick ice mantle, and a core. All four planets contain about 10 Earth masses of ice, rock, ...
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Scattered disc



The scattered disc (or scattered disk) is a distant region of the Solar System that is sparsely populated by icy minor planets, a subset of the broader family of trans-Neptunian objects. The scattered-disc objects (SDOs) have orbital eccentricities ranging as high as 0.8, inclinations as high as 40°, and perihelia greater than 30 astronomical units (4.5×109 km; 2.8×109 mi). These extreme orbits are thought to be the result of gravitational ""scattering"" by the gas giants, and the objects continue to be subject to perturbation by the planet Neptune.Although the closest scattered-disc objects approach the Sun at about 30–35 AU, their orbits can extend well beyond 100 AU. This makes scattered objects among the most distant and coldest objects in the Solar System. The innermost portion of the scattered disc overlaps with a torus-shaped region of orbiting objects traditionally called the Kuiper belt, but its outer limits reach much farther away from the Sun and farther above and below the ecliptic than the Kuiper belt proper.Because of its unstable nature, astronomers now consider the scattered disc to be the place of origin for most periodic comets in the Solar System, with the centaurs, a population of icy bodies between Jupiter and Neptune, being the intermediate stage in an object's migration from the disc to the inner Solar System. Eventually, perturbations from the giant planets send such objects towards the Sun, transforming them into periodic comets. Many Oort cloud objects are also thought to have originated in the scattered disc. Detached objects are not sharply distinct from scattered disc objects, and some such as Sedna have sometimes been considered to be included in this group.
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