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Solar System
Solar System

...  Revolve fast around the sun  Mercury, Venus, Earth, and Mars ...
Ch. 3 Sec. 4 Notes
Ch. 3 Sec. 4 Notes

... *The 4 outer planets are much bigger than Earth and do not have solid surfaces -Referred to as gas giants -Pluto is a "gas dwarf" *The gas giants are composed of mainly hydrogen and helium *Due to their large size, their gravity is much stronger and can hold in all the gas -Provides a thick atmosphe ...
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Astronomers - duerkopscience

... • Heliocentric Theory: all planets orbit the sun, only the moon orbits Earth • Assumed Earth rotated which explained the seasons • Knew of 6 planets orbiting the sun • Made a new solar system model and placed them in order ...
Chapter 17 Science Class 8
Chapter 17 Science Class 8

... 12.Why is the distance between stars expressed in light years? What do you understand by the statement that a star is eight light years away from the Earth? Answer. The Universe with millions of galaxies is so vast that speed of light is the better unit to measure distances in space because it is th ...
Mon May 27, 2013 THE VENERABLE BEDE FEAST DAY On May
Mon May 27, 2013 THE VENERABLE BEDE FEAST DAY On May

... The sun is on the move. Now this movement I’m talking about is much more subtle than the obvious sunrise-sunset stuff we get every day, due to earth’s rotation. Assuming you could make the sun dimmer so that you could see it and stars at the same time, (something that only happens in a planetarium o ...
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astronomy_SaturndayMPhysics07

... Cloud of gas and dust contracts due to gravity; conservation of angular momentum means it spins faster and faster as it contracts ...
Asteroids PP - MR D`S ICT CORNER
Asteroids PP - MR D`S ICT CORNER

... • Asteroids are large chunks of rock (but smaller than planets) left over from the formation of the Solar System. Asteroids come from the Leonid asteroid belt, between Mars and Jupiter. Asteroids orbit the sun, and some asteroids cross the Earth’s orbit. At various times during the Earth’s history, ...
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... only 1.7 times the medium distance between the Earth and the Sun. During a “red  giant phase”, the stars, after exhausting their primary fuel, hydrogen, in the core,  experience an enormous expansion (with their volume increasing by a factor of a  few millions) that can easily reach and engulf the i ...
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Solar System Study Guide

... are much smaller than the Sun. Some planets, like the Earth, only have one moon. Other planets, like Jupiter and Saturn, have as many as 30 moons traveling around them! ...
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The Sun and the Solar System

... The  circularity  of  Neptune’s  orbit,  the  outermost  and  thus  least   strongly  bound  of  all  the  major  planets  (Pluto,  Eris,  and  other   “dwarf  planets”  excepted  from  this  category),  is  especially   compelling.   •  Th ...
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Our Sidewalk Flier — in PDF format

... sent to the Moon and 12 astronauts have walked upon its surface. The presence of the Moon stabilizes Earth’s wobble. Over billions of years, the Earth’s stable spin made for a stable climate that may have influenced the development and growth of life here. From Earth, we see the same face of the Moon ...
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... • Fragments of rock made of material similar to the material that formed the planets. – More than 50,000 asteroids have been found in our solar system. ...
The Solar System - University of Sioux Falls
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... e. The tides are the daily, periodic rise and fall of water level caused by the gravitational pull of the sun and moon. f. Water occurs on Earth as a solid (ice), a liquid, or a gas (water vapor) due to its position in the solar system. g. The sun consists largely of hydrogen gas. Its energy comes f ...
Name: Date: Meteorology and Space Science Semester I 2016
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... 23. List the planets in order, starting with the Sun, which is at the center. Sun Mercury  Venus  Earth  Mars  Asteroid Belt  Jupiter  Saturn  Uranus  Neptune  Pluto 24. List characteristics of terrestrial planets. Small in size, high density, and little to no atmosphere 25. List character ...
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... Note: Venus is the hottest planet due to the composition of its atmosphere - large amounts of Co2. Note: Asteroid Belt - The area between Mars and Jupiter that contains asteroids or minor planets that orbit the Sun. ...
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Geology of the Hawaiian Islands

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Solar Nebula Theory

... - Out-gassing creates CO2 dominated atmosphere - Water vapor washes out CO2; life forms oxygenate atmosphere ...
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Pluto(2274km)- Pluto is a dwarf planet, and was classified as such in

... (the outer shell of a star) is about 10,000°F. It is composed mostly of hydrogen, some helium, and smaller quantities of heavier elements including oxygen. It is the most important source of energy for life on Earth. Solar System(9x10^9km)The solar system contains the Sun and the planets including E ...
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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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