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In the Spring of 2007 two of us began planning a new course in
In the Spring of 2007 two of us began planning a new course in

... d. mass e. chemical makeup 15. Current evidence about how the universe is changing tells us that a. We are near the center of the universe. b. Galaxies are expanding into empty space. c. Groups of galaxies appear to move away from each other d. Nearby galaxies are younger than distant galaxies. 16. ...
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... nanometers. But at high redshifts, that line passed not just into the visible but all the way through to the infrared, and for the newly discovered galaxy, GN-z11, its whopping redshift of 11.1 pushed that line all the way out to 1471 nanometers, more than double the limit of visible light! Hubble i ...
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... It is believed that our solar system began similar to a galaxy…(or a hurricane). A cloud of gas (nebula) collapsed to form the sun, which began rotating. As time when on, the heavier dust fell toward the sun, creating the rocky inner planets, and the ...
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... Most of the Sun’s hydrogen is too far from the core and too cool to participate in fusion reactions. Photons in the Sun travel such short distances that many absorptions and reemissions must occur before radiative diffusion can carry the Sun’s energy to the surface. It is at that distance from the c ...
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... The second demonstration concerns the relative sizes of planetary orbits. You will need pieces of string or ribbon to represent the orbital radii (strictly, the orbital semi-major axes). I use a scale in which the Sun's radius is 1 mm: this is handy because you can say that you have ...
Exploring the Solar System - Rourke Publishing eBook Delivery
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... different rates. Mercury travels quickly around the Sun in just 88 Earth days, but it rotates very slowly. One Mercurian day is 176 Earth days long. It takes Venus 225 Earth days to orbit the Sun, but it rotates very slowly. It takes 243 Earth days for Venus to rotate once. Since a day is the time ...
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Copy rights – www.SJJeyanth.yolasite.com 01.Our Solar system

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... Scientists try to predict when comets will come too close to Earth Sometimes comets collide with planets and their moons Haley’s Comet is the most famous comet, it passes by Earth every 76 years – the last time it passed by Earth was in 1986 When Earth crosses the path of a comet, leftover dust and ...
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... • You need “metals” to make planets –Metals are elements heavier in mass than helium ...
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... By contrast, the Moon moves across the star background a distance equal to its width every hour as it orbits Earth. The Moon is our closest neighbor. The planets are farther away, but you can see their gradual movements among the constellations over a period of weeks or months. ...
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How did our solar system get here?

... • Third largest planet in our solar system. It is about four times the diameter of Earth. • Uranus’s atmosphere is made up of mostly hydrogen, helium, and methane. The methane causes the planet to have a bluish green appearance. The planet is also a gas giant so it has no solid surface. Under the at ...
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Solar System



The Solar System comprises the Sun and the planetary system that orbits it, either directly or indirectly. Of those objects that orbit the Sun directly, the largest eight are the planets, with the remainder being significantly smaller objects, such as dwarf planets and small Solar System bodies such as comets and asteroids. Of those that orbit the Sun indirectly, two are larger than the smallest planet.The Solar System formed 4.6 billion years ago from the gravitational collapse of a giant interstellar molecular cloud. The vast majority of the system's mass is in the Sun, with most of the remaining mass contained in Jupiter. The four smaller inner planets, Mercury, Venus, Earth and Mars, are terrestrial planets, being primarily composed of rock and metal. The four outer planets are giant planets, being substantially more massive than the terrestrials. The two largest, Jupiter and Saturn, are gas giants, being composed mainly of hydrogen and helium; the two outermost planets, Uranus and Neptune, are ice giants, being composed largely of substances with relatively high melting points compared with hydrogen and helium, called ices, such as water, ammonia and methane. All planets have almost circular orbits that lie within a nearly flat disc called the ecliptic.The Solar System also contains smaller objects. The asteroid belt, which lies between Mars and Jupiter, mostly contains objects composed, like the terrestrial planets, of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc, populations of trans-Neptunian objects composed mostly of ices, and beyond them a newly discovered population of sednoids. Within these populations are several dozen to possibly tens of thousands of objects large enough to have been rounded by their own gravity. Such objects are categorized as dwarf planets. Identified dwarf planets include the asteroid Ceres and the trans-Neptunian objects Pluto and Eris. In addition to these two regions, various other small-body populations, including comets, centaurs and interplanetary dust, freely travel between regions. Six of the planets, at least three of the dwarf planets, and many of the smaller bodies are orbited by natural satellites, usually termed ""moons"" after the Moon. Each of the outer planets is encircled by planetary rings of dust and other small objects.The solar wind, a stream of charged particles flowing outwards from the Sun, creates a bubble-like region in the interstellar medium known as the heliosphere. The heliopause is the point at which pressure from the solar wind is equal to the opposing pressure of interstellar wind; it extends out to the edge of the scattered disc. The Oort cloud, which is believed to be the source for long-period comets, may also exist at a distance roughly a thousand times further than the heliosphere. The Solar System is located in the Orion Arm, 26,000 light-years from the center of the Milky Way.
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