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Profile Documents Logout
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Solar System PowerPoint
Solar System PowerPoint

... heat does not make many particles in the atmosphere move fast enough to escape.  This planet has an atmosphere dominated by H and He. ...
Moon Obs #1 Due!
Moon Obs #1 Due!

... Why Does Everything Rotate and Spin in the ...
27-1 Objectives
27-1 Objectives

... • solar nebula: a rotating cloud of gas and dust from which the sun and planets formed; also any nebular from which stars and exoplanets may form • In 1796, French mathematician Pierre Simon, advanced a hypothesis now known as the nebular hypothesis. • Modern scientific calculations support this the ...
White Dwarf
White Dwarf

... • The core of a giant star collapses as helium fuses. – Outer layers continue to expand – Loses over half its mass ...
Dead Earth – Lesson 4 – Life on other worlds
Dead Earth – Lesson 4 – Life on other worlds

... • The Earth’s magnetic field also protects us from harmful particles and radiation from the Sun ...
The Inner Planets
The Inner Planets

... because it has very little gravity. Gases escape out into space as they heat up. Mercury has extreme temperature difference (-170 °C to 430 °C) . ...
Powers of ten notation
Powers of ten notation

... Diurnal motion – daily motion from east to west staying close to ecliptic Direct motion – as with the Sun and Moon, move west to east as compared to the stars, each at a ...
the inner planets - Horace Mann Webmail
the inner planets - Horace Mann Webmail

... • There is some solid water at the north pole of Mars. This is covered with solid carbon dioxide in the winter. • Mars is tilted on its axis so it has seasons. During the change of seasons many dust storms exist. • Mars has two very small moons called Phobos and Deimos. ...
Moon Match
Moon Match

... The Solar System contains 1 star (the Sun), 8 planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune), 10’s of satellites that orbit the planets, dwarf planets (Pluto, Ceres, and Eris), 1000’s of asteroids that orbit the Sun, and billions of comets. For our Solar System the planets o ...
Document
Document

... the Gas Giants. Large – 88,000 miles to 30,000 miles. Short days – 10 hours to 17 hours. ...
Ch 13 PP
Ch 13 PP

... rocky material, metallic nickel and iron  Mercury ...
Review Lecture 5
Review Lecture 5

... Moon during a lunar eclipse. Hipparchus ~ 130 B.C., discovered the precession of the north celestial pole. Ptolemy ~ 150 A.D., explained motion of the Sun, planets, and Moon with Epicycle Theory. This is the Earth at center of universe theory = geocentric world view. Copernicus ( 1473-1543) publishe ...
Transcript - Cheap Astronomy
Transcript - Cheap Astronomy

... punishable by death – and often a fairly grisly death. Presumably to avoid any such complications, Copernicus arranged for the posthumous publication of his book On the Revolutions of the Heavenly Spheres in 1543, being the same year in which he died. Not so lucky was Giordano Bruno who was burned a ...
User guide 2 - Finding celestial treasures
User guide 2 - Finding celestial treasures

... 4. Find star patterns that you already know, such as the Big Dipper or Orion. Then, triangulate to the brighter stars that you don’t know. ...
Word doc - UC-HiPACC - University of California, Santa Cruz
Word doc - UC-HiPACC - University of California, Santa Cruz

... Indeed, the team of 15 astronomers from seven institutions on four continents had picked Tau Ceti specifically because meticulous observations strongly suggested the star had no planetary system. From the earliest days of the hunt for exoplanets almost 20 years ago, astronomers suspected that eviden ...
Solar System Review
Solar System Review

... Chunks of rock or metal orbiting the Sun that may be underdeveloped parts of planets or pieces of planets that have broken off are called a. stars. b. asteroids. c. comets. d. meteorites. ...
Science test study guide for the last week in January 2011[1]
Science test study guide for the last week in January 2011[1]

... 29. Jupiter has a thick atmosphere made up of hydrogen and helium. It has a giant red spot that is a large storm larger than planet Earth. 30. Uranus is different from most other planets because it rotates on its side. 31.Pluto is different from the other outer planets because it is rocky and has a ...
Final Review Sheet - Astronomy Part 2
Final Review Sheet - Astronomy Part 2

... 24.What units do I use to describe distance in space? List them from smallest to ...
The Solar System
The Solar System

... Jupiter • Jupiter is a giant gas planet made up of about 90% hydrogen and 10% helium. • Jupiter was first visited by Pioneer II in 1973. • It is thought that Jupiter’s ‘Great Red Spot’ is a storm of swirling gas that has lasted for hundreds of years. • Jupiter has 16 moons. • Jupiter is the fifth p ...
Final Exam Earth science
Final Exam Earth science

... Main sequence stars. Hertzsprung-Russell diagram, a graph used by astronomers. It shows a relationship between surface temperature and brightness. Most stars (90%) form a diagonal band called the main sequence stars. In the main sequence, surface temperature increases as brightness increases. Our su ...
document
document

... Earth at about 43,000mph in the Arizona desert near Flagstaff 40,000 years ago. ...
Test #2
Test #2

... c) we are doomed, d) it will burn up in the atmosphere 24. Why is Mars red? a) Dust storms on the planet have blasted the planet so fiercely that the rocks have reddened. b) The planet's surface undergoes a process by which rust forms. c) Sulfuric acid rain etched a reddish color into surface rocks. ...
Scale
Scale

... planets in our solar system. Voyager II, traveling at nearly 50,000 mph took 12 years to reach the planet Neptune! This gives you an idea of just how far our planets are from each other. However, we can make a scale model of the distances between the planets using almost anything as our reference. I ...
Unit 8: Space Study Guide
Unit 8: Space Study Guide

... Venus: – This planet was once considered a twin planet to earth. But later scientists discovered that the surface of this planet has a lead-melting temperature of 480°C. Venus has no moons or rings. Mars: – This planet shows signs of liquid water flowing on its surface in the past. Atmosphere of Mar ...
Space Unit - Questions and Answers
Space Unit - Questions and Answers

... (this rubbing is called friction), it becomes hot and vaporizes and the air glows. This produces a bright streak of light across the sky (shooting star) that you can see at night. A comet is a chunk of frozen matter that travels in a very long orbit around the sun. The glowing tail of a comet is the ...
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History of Solar System formation and evolution hypotheses



Ideas concerning the origin and fate of the world date from the earliest known writings; however, for almost all of that time, there was no attempt to link such theories to the existence of a ""Solar System"", simply because almost no one knew or believed that the Solar System, in the sense we now understand it, existed. The first step towards a theory of Solar System formation was the general acceptance of heliocentrism, the model which placed the Sun at the centre of the system and the Earth in orbit around it. This conception had been gestating for thousands of years, but was only widely accepted by the end of the 17th century. The first recorded use of the term ""Solar System"" dates from 1704.
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