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Probing the Edge of the Solar System: Formation of an
Probing the Edge of the Solar System: Formation of an

... We are located in the middle of the Milky Way Galaxy 28,000 light years from the center One of 200 billion stars in our Galaxy ...
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star chart - Ontario Science Centre

... AUG 10 * Second Supermoon of the year; This will be the largest full Moon of the year as the Moon will only be 356,896km away from the Earth AUG 12 Perseid meteor shower peaks; Unfortunately, the Moon will be bright and high in the sky AUG 18 * Conjunction between Venus and Jupiter; These two planet ...
Article - public.iastate.edu
Article - public.iastate.edu

... Now he said he is working on furthering debate by encouraging online discussions on what the characteristics of a planet should be with the goal of creating a definition more effective than the union's. Pluto's planet status has eroded since its discovery in 1930, and it has been found to be far les ...
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WORD - hrsbstaff.ednet.ns.ca
WORD - hrsbstaff.ednet.ns.ca

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... Aside: observations of other planetary systems In most other stellar (extrasolar) systems, all we know about are the stars, because they are overwhelmingly bright. – But, planets have been detected around other stars, with surprising properties (high eccentricities, small radii from star, sparse an ...
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... 2.  Earth does not orbit Sun; it is the center of the universe and stationary. With rare exceptions (Aristarchus), the Greeks rejected the correct explanation (1) because they did not think the stars could be that far away. Set the stage for a long controversy about Earth-centered and Sun-centered t ...
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... While the sun is often referred to as the most important star within our solar system, it is certainly not the only one. There are too many stars for us to even begin to count. See how many you can count while gazing up at the sky on a clear night. Not only are there too many stars to count but, the ...
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...  Comets whose orbit brings them close to the Sun more frequently than every 200 years are considered to be short period comets, the most famous of which is probably Comet Halley, named after the British astronomer Edmund Halley, which has an orbital period of roughly 76 years. ...
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... The model is unrealistic in one respect, however. All of the planets have been arranged roughly in a straight line on the same side of the Sun, and hence the separation from one planet to the next is as small as it can possibly be. The last time all nine planets were lined up this well in the real s ...
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Supplemental Resources - Morehead Planetarium and Science

Time runs out for Herschel
Time runs out for Herschel

... eye of the storm is about 2000 km across – ten times the typical size on Earth – and clouds at the outer edge of the hurricane on Saturn are moving at more than 500 kph – rather faster than on Earth! One difference from terrestrial hurricanes is that this storm is locked into the weather system at t ...
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Formation and evolution of the Solar System



The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.
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