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Jupiter by Jessie Ann and Rosalyn
Jupiter by Jessie Ann and Rosalyn

... Jupiter is the largest of the nine planets, more than 10 times the diameter of Earth and more than 300 times its mass. In fact, the mass of Jupiter is almost 2.5 times that of all the other planets combined. Being composed largely of the light elements hydrogen and helium, its mean density is only 1 ...
December 2015 - Hermanus Astronomy
December 2015 - Hermanus Astronomy

... the Sun. However, earlier studies that proposed giant planets could possibly eject one another did not consider the effect such violent encounters would have on minor bodies, such as the known moons of the giant planets and their orbits. So, Cloutier and his colleagues turned their attention to moon ...
Pistol Star - University of Dayton
Pistol Star - University of Dayton

... • The big bang was initially suggested because it explains why distant galaxies are traveling away from us at great speeds. The theory also predicts the existence of cosmic background radiation (the glow left over from the explosion itself). • The Big Bang Theory received its strongest confirmation ...
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Approaching a black hole

... horizon to the outside world). However, this is an hypothesis, not proven, so it is conceivable that so-called "Naked Singularities" might exist, not clothed by an event horizon. ...
The length of an Earth day is determined by the time required for
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The Hidden Lives of Galaxies NSTA 2001
The Hidden Lives of Galaxies NSTA 2001

... Helium fuses: All elements larger than helium (up to iron) begin to be produced now. Stage 7 Helium fuses to form Carbon. The star shines less brightly. Energy sustains the expanded outer layers. Star is called a red giant of the Red Giant ...
Title of Lesson Sequence: “The Earth`s Seasons”
Title of Lesson Sequence: “The Earth`s Seasons”

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NGSS Alignment - University of Louisville
NGSS Alignment - University of Louisville

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Gravity - Indiana University Astronomy

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Solo - Net Start Class
Solo - Net Start Class

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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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