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Secondary Science Documents: Grade 6 – Earth/Space Science
Secondary Science Documents: Grade 6 – Earth/Space Science

... b. Develop the topic with relevant, well-chosen facts, definitions, concrete details, quotations, or other information and examples. c. Use appropriate and varied transitions to create cohesion and clarify the relationships among ideas and concepts. d. Use precise language and domain-specific vocabu ...
Milankovitch cycles
Milankovitch cycles

"Inner Oort cloud" -
"Inner Oort cloud" -

... Comets can also shift their orbits due to jets of gas and dust that rocket from their icy surface as they approach the sun. Although they get off course, comets do have initial orbits with widely different ranges, from 200 years to once every million years or more. Comets entering the planetary regi ...
ES Chapter 30
ES Chapter 30

... together and that orbit a common center of mass. – More than half of the stars in the sky are either binary stars or members of multiple-star systems. – Astronomers are able to identify binary stars through several methods. • Accurate measurements can show that its position shifts back and forth as ...
Larger, high-res file, best for printing
Larger, high-res file, best for printing

Lecture14.v1 - Lick Observatory
Lecture14.v1 - Lick Observatory

... occurred every few thousand years. Now they only occur over tens or hundreds of millions of years (so the lunar surface hasn’t changed too much). ...
Earths Moon and Solar System Test Prep-2
Earths Moon and Solar System Test Prep-2

... 23.Most scientists believe the Milky Way Galaxy is ...
Planet formation Abstract Megan K Pickett and Andrew J Lim
Planet formation Abstract Megan K Pickett and Andrew J Lim

... is from this disk that the planets somehow coalesced. Close to the forming Sun, where the temperatures were high enough to vaporize most volatiles, the terrestrial planets formed by the accumulation of silicon, iron, nickel and other refractory grains into progressively larger bodies. Far from the S ...
8-4.4 - S2TEM Centers SC
8-4.4 - S2TEM Centers SC

... Sun, where it can receive the most light, and that a new moon occurs when the Earth blocks the Sun’s light from reaching the moon. (Phases are the result of the Moon’s relative position to Earth.)  Gravity is selective about what it affects when it does, and that gravity must be stronger at great d ...
Power Point Presentation
Power Point Presentation

... where they burn hydrogen in nuclear reactions in their cores Burning rate is higher for more massive stars - hence their lifetimes on the main sequence are much shorter and they are rather rare Red dwarf stars are the most common as they burn hydrogen slowly and live the longest Often called dwarfs ...
An “Asteroid Garden” for the Gainesville Solar Walk And an Asteroid
An “Asteroid Garden” for the Gainesville Solar Walk And an Asteroid

... (Lagrangian Points L4 and L5). Another family (“Hildas”) orbits between 3.5 and 4.2 Aus. Diagram based on data in JPL DE-405 ephemeris and Minor Planet Center database of asteroids (2006 July 6).Rendered by custom software written for Wikipedia. Diagram redrawn by author using Wikipedia image. ...
Cosmic Influence on the Sun-Earth Environment
Cosmic Influence on the Sun-Earth Environment

... CME glances along the magnetic shield, local disturbances in the atmosphere of the Earth have been noticed. During the monsoon of 2003 there were continuous CME glances with the magnetic shield from a group of sunspots, which are responsible for the abnormal record rainfall in northern parts of Indi ...
How the Sun Shines
How the Sun Shines

... Why was there so much fuss about this scientific puzzle? The nineteenth-century astronomer John Herschel described eloquently the fundamental role of sunshine in all of human life in his 1833 Treatise on Astronomy: The sun’s rays are the ultimate source of almost every motion which takes place on th ...
arXiv:astro-ph/0009259 v3 12 Dec 2000
arXiv:astro-ph/0009259 v3 12 Dec 2000

... Why was there so much fuss about this scientific puzzle? The nineteenth-century astronomer John Herschel described eloquently the fundamental role of sunshine in all of human life in his 1833 Treatise on Astronomy: The sun’s rays are the ultimate source of almost every motion which takes place on th ...
How the Sun Shines
How the Sun Shines

... Why was there so much fuss about this scientific puzzle? The nineteenth-century astronomer John Herschel described eloquently the fundamental role of sunshine in all of human life in his 1833 Treatise on Astronomy: The sun’s rays are the ultimate source of almost every motion which takes place on th ...
solar system - National Geographic Society
solar system - National Geographic Society

... Explain that you are going to play a game of “Revolve! Rotate!” Students will either “revolve” or “rotate” to travel to the other side of the map. The first student to the other side of the map is the winner. Remind students that there is no running on the map. This game has the similar rules to Red ...
Problem 1. Marking scheme Lagrange Point
Problem 1. Marking scheme Lagrange Point

... THEORETICAL TEST 15 short problems page 3 from 30 ...
Natural Satellite - Mr. Gray`s Class
Natural Satellite - Mr. Gray`s Class

... people saw pictures of the Far Side. It wasn’t until 1968 that people saw it first hand. Apollo 8 was able to orbit the moon and view the far side. Astronauts Frank Borman, Jim Lovell and William Anders were able to see it. ...
How the Sun Shines
How the Sun Shines

... In 1938, C. F. von Weizsäcker came close to solving the problem of how some stars shine. He discovered a nuclear cycle, now known as the carbon-nitrogen-oxygen (CNO) cycle (see Appendix A), in which hydrogen nuclei could be burned using carbon as a catalyst. However, von Weizsäcker did not investi ...
an all-sky extrasolar planet survey with multiple object, dispersed
an all-sky extrasolar planet survey with multiple object, dispersed

How the Sun Shines - School of Natural Sciences
How the Sun Shines - School of Natural Sciences

... In 1938, C. F. von Weizsäcker came close to solving the problem of how some stars shine. He discovered a nuclear cycle, now known as the carbon-nitrogen-oxygen (CNO) cycle (see Appendix A), in which hydrogen nuclei could be burned using carbon as a catalyst. However, von Weizsäcker did not investi ...
Uranus and its Moons
Uranus and its Moons

Jupiter Maddie Hunt
Jupiter Maddie Hunt

... 46 of them are less than 3 km wide They were all discovered between 1610-2004 Four Biggest moons are called the Galilean moons because he discovered them Galilean moons: Io, Europa, Ganymede and Callisto These are about the same size as Earths moon ...
Updated IAA RAS Planetary Ephemerides
Updated IAA RAS Planetary Ephemerides

... The motion of the barycenter of the Earth-Moon system is appreciably perturbed by the Moon itself. The Moon’s orbit is subject to perturbations from the asphericity of the gravitational potentials of the Earth and the Moon, which makes it necessary to characterize the positions of the equators of t ...
Astonomy-Space The Final Frontier
Astonomy-Space The Final Frontier

...  Explain how Kepler’s laws allow us to construct a scale model of the solar system, and explain the technique used to determine the actual size of the planetary orbits.  Be able to state Newton’s laws of gravitation and explain how they account for Kepler’s laws.  Explain how the law of gravitati ...
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Orrery



An orrery is a mechanical model of the solar system that illustrates or predicts the relative positions and motions of the planets and moons, usually according to the heliocentric model. It may also represent the relative sizes of these bodies; but since accurate scaling is often not practical due to the actual large ratio differences, a subdued approximation may be used instead. Though the Greeks had working planetaria, the first orrery that was a planetarium of the modern era was produced in 1704, and one was presented to Charles Boyle, 4th Earl of Orrery — whence came the name. They are typically driven by a clockwork mechanism with a globe representing the Sun at the centre, and with a planet at the end of each of the arms.
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