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Activity 12: Solar System
Activity 12: Solar System

... composed of mostly rock and iron. Jupiter, Saturn, Uranus, and Neptune make up the outer planets, which are much larger and consist mainly of hydrogen, helium and ice. Because Pluto is the farthest planet from Earth, astronomers know very little about it. Some believe it should not even be considere ...
The Inner Planets - Library Video Company
The Inner Planets - Library Video Company

... Which is the planet closest to the Sun? The planet closest to the Sun is Mercury, a small planet with few attractions. With no atmosphere, it is constantly bombarded by meteorites, night and day last six months each, and it is either baking hot or bitterly cold. What is the first star we see at nigh ...
Content Standards/Performance Indicators: Key Pre
Content Standards/Performance Indicators: Key Pre

... Understanding the solar system helps you understand Earth’s position in space. The Sun is the star that provides energy for life on Earth. That Earth is part of the Milky Way galaxy. ...
Quick Reference - Objects in the skies
Quick Reference - Objects in the skies

... The Kuiper belt is a region of the Solar System beyond the planets, extending from the orbit of Neptune (at 30 AU) to approximately 50 AU from the Sun. It is similar to the asteroid belt, although it is far larger - 20 times as wide and 20 to 200 times as massive. Like the asteroid belt, it consists ...
Outer Space - The Reading Connection
Outer Space - The Reading Connection

... This craft requires quite a bit of prep, but it's not difficult to put together and makes an awesome take-away from the Read-Aloud. Use paper plates, yarn, and pre-cut paper circles (nine per kid, of various sizes -- these will represents the 8 planets and the sun) to make a hanging mobile model of ...
day_and_night - Primary Resources
day_and_night - Primary Resources

... Why do we have day and night? ...
PowerPoint Presentation - Small Bodies in the Solar System
PowerPoint Presentation - Small Bodies in the Solar System

... • The comet is made out of several parts: the nucleus, dust tail, and ion tail. ...
Jeopardy - University of Nebraska–Lincoln
Jeopardy - University of Nebraska–Lincoln

... universe are pretty much the same everywhere and that there are no unique vantage points in the universe. ...
SNC1PL Celestial Objects and Constellations
SNC1PL Celestial Objects and Constellations

... …maybe more… ...
Unit 3
Unit 3

... around a star. It also reflects (i.e., to throw back light, heat or sound) that star's light. Eight planets have been discovered in our solar system.  Mercury, Venus, Earth, and Mars are the planets closest to the Sun. They are called the inner planets. The inner planets are made up mostly of rock. ...
E. Sci. Astronomy Notes
E. Sci. Astronomy Notes

... retrograde orbit (clockwise), can orbit further out than Pluto Pluto – half ice/half rock, highly eccentric orbit (very oval), over 90 degree axis tilt (points south), has one moon Charon. 10th planet – UB 313 has moon ...
The Planet Hike - City of Dripping Springs
The Planet Hike - City of Dripping Springs

... Home! We are the only planet in our solar system that has 1 moon, liquid oceans and an abundance of life! That’s because we live in the “habitable zone”, where water can exist as a liquid on its surface. The Kepler Space Telescope is currently looking for earth-like planets in other solar systems. S ...
Astronomy Test Review
Astronomy Test Review

... What does the tail of a comet tell us about the direction the comet is moving? ...
Chapter One Technology, Science, and Scientific Measurement
Chapter One Technology, Science, and Scientific Measurement

... between a distance of 2.2 and 3.3 AU from the center of the solar system. Definition: a region in the solar system located between the orbits of Mars and Jupiter where there are a high number of asteroids Definition: an object orbiting the Sun that is smaller than a planet and has no atmosphere ...
The planets in the solar system
The planets in the solar system

... drawing in additional material by their gravitational attraction. These concentrations become ever denser until they collapse inward under gravity to form proto-planets. When the proto-star has grown massive enough to ignite and form a star, the rest of the disk is removed from the inside outward by ...
The Search for Extraterrestrial Life
The Search for Extraterrestrial Life

CHAPTER 9.3: The Outer Planets
CHAPTER 9.3: The Outer Planets

... cycle  vs.  a  water  cycle!!   33.  _________________________  is  the  seventh  planet  from  the  Sun.     34.  The  last  Cme  it  was  visited  by  a  probe  was  in  ______________  when  Voyager  2  flew  by.   35.  Uranus,  like ...
The Earth in Space
The Earth in Space

Outer Planets
Outer Planets

... times the diameter of Earth but much smaller than Jupiter and Saturn  Twice as far from sun as Saturn so much colder  Looks bluish because of traces of methane in atmosphere  First new planet discovered since 1781  Thought it might be a comet but when studied had an orbit just beyond Saturn  St ...
Components of Universe
Components of Universe

... Components of the Universe Note Section ...
Planet Name Origins
Planet Name Origins

... Each of the nine planets has a name taken from Roman gods and goddesses, Each of these names describes something special about the planet. Mercury: named after the Roman messenger god who was known for ...
Sample Chapter
Sample Chapter

... The sun isn’t a planet. It is a star at the centre of the solar system. It formed 5 billion years ago from a cloud of gas and dust. The sun’s diameter is 1,392,000 kilometres. It is much bigger than the Earth. ...
White Dwarf
White Dwarf

... • The lost mass comes off in helium flash explosions. ...
Document
Document

... comets make up less than 1/700 of the mass of the Solar System! ...
Geocentric vs. Heliocentric Models of the Solar System
Geocentric vs. Heliocentric Models of the Solar System

... If it fails even once must be reformulated or rejected! ...
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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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