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Outline of Lecture on Copernican Revolution: 1. Source of word
Outline of Lecture on Copernican Revolution: 1. Source of word

... Both Ptolemy and Copernicus had to explain the nonuniform motion of the planets in their orbits. Planets move faster when they are closer to the sun. Ptolemy “explained” this by a nonuniform motion of the guiding center of the epicycle about the guiding center circle. Copernicus, perhaps rediscover ...
The Sun
The Sun

... The largest spots in this image are over 20,000 km across—twice the diameter of Earth. Typical sunspots are only about half this size. ...
The Sun
The Sun

... The largest spots in this image are over 20,000 km across—twice the diameter of Earth. Typical sunspots are only about half this size. ...
Designing Curriculum and Instruction in Elementary School
Designing Curriculum and Instruction in Elementary School

... The Asteroid Belt, The Kuiper Belt, And The Oort Cloud You have probably heard about the Asteroid Belt. This band of asteroids sits between the orbits of the planets Jupiter and Mars. It is made up of thousands of objects too small to be considered planets. Some of them no larger than a grain of dus ...
The Ceres Connection - MIT Lincoln Laboratory
The Ceres Connection - MIT Lincoln Laboratory

... generally between Mars and Jupiter, were first noticed by astronomers observing the night sky through a telescope. The search for minor planets continues today, with astronomers using computerassisted methods that pair highly sensitive image sensors with powerful telescopes. While these new methods ...
Chapter 1: Introduction to Earth Science Indiana State Standards 1
Chapter 1: Introduction to Earth Science Indiana State Standards 1

... Describe the relationships among evaporation, precipitation, ground water, surface water, and glacial systems in the water cycle. Discuss the effect of human interactions with the water cycle. SCI.ES.4.3 2010 Explain the importance of heat transfer between and within the atmosphere, land masses, and ...
Section 4 Orbits and Effects
Section 4 Orbits and Effects

... The precession of Earth’s axis is one part of the precession cycle. Another part is the precession of Earth’s orbit. As Earth moves around the Sun in its elliptical orbit, the major axis of Earth’s orbital ellipse is rotating about the Sun. In other words, the orbit itself rotates around the Sun. Th ...
SOLAR SYSTEM
SOLAR SYSTEM

... Its axis point toward Sun most of the time. Spins on side. • Bright blue green color comes from methane in atmosphere. • Has 11 known rings • Uranus has 27 moons most very small. – Largest: Miranda, Ariel, Umbriel, Oberon, Titania (small large) ...
Meet the Planets - Arbordale Publishing
Meet the Planets - Arbordale Publishing

... The layout, and general look, of the Venus page illustration is based on Botticelli’s “Birth of Venus.” Compare and contrast the two. A set of 1,670 on-off pulses ...
ess 102: space and space travel
ess 102: space and space travel

... engineering students interested in the space environment around the Earth, its control by solar activity, and potential opportunities for the exploration of the solar system. In this course we will describe the filling of space with hot ionized gases called plasmas that are ejected from the Sun, the ...
early earth
early earth

... Collapsed disk not shown  Sun is about 5 billion years old  5 billion years until a red giant is formed ...
Earth & Space - Stars - Students, Teachers and Resources
Earth & Space - Stars - Students, Teachers and Resources

angular size - Particle and Astroparticle Physics
angular size - Particle and Astroparticle Physics

... If you draw lines from your eye to each of two stars, the angle between these lines is the angular distance between these two stars ...
Earth & Space
Earth & Space

... • The earth has over time had an increasingly longer day • The original length of one day, when the earth was new, is actually closer to 21 hours • This phenomenon is due to the tides raised by the Moon (tidal acceleration) which slows the Earth's rotation – During the Pennsylvanian Period a day was ...
Physivd Preliminary Module 8.5 The Cosmic Engine
Physivd Preliminary Module 8.5 The Cosmic Engine

... Thales of Miletus (640-546 BC) The earth was a disc floating on a vast body of water Anaximander (611-547 BC) The earth was a free floating cylinder in space The heavens formed sphere about the earth The moon was self-luminous ie the earth is the unsupported centre of the universe Pythagoras (580-50 ...
Earth
Earth

... measure distance B. Astronomical Units (AU) measure distances between planets C. Neither are big enough to measure outside of our solar system, scientists use a unit based on the speed of light ...
Modeling the Orbits of the Outer Planets
Modeling the Orbits of the Outer Planets

... of the ancient, icy mini-worlds in that vast region, at least a billion miles beyond Neptune’s orbit. Sending a spacecraft on this long journey will help us answer basic questions about the surface properties, geology, interior makeup and atmospheres on these bodies. ...
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 ...
Asteroids4 Feb Asteroids, Comets, Minor Planets • Understanding composition of solar system
Asteroids4 Feb Asteroids, Comets, Minor Planets • Understanding composition of solar system

... • Small, rocky objects in orbit around the Sun. – Sizes up to 940 km. (Detroit to Boston) – 26 known with sizes > 200 km (width of MI). ...
Rotation and Revolution
Rotation and Revolution

... elliptical, or oval shaped. This means that each planet is sometimes closer to and sometimes farther from the Sun. The diagram titled “Seasons in the Northern Hemisphere,” below, shows an example of an elliptical orbit. ...
Starlight and What it Tells Us
Starlight and What it Tells Us

File
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... the comet melts, sometimes large chunks of ice break off in a hurry and large amounts of gases escape at once and cause a bright “outburst”. The gas and dust are released and form an atmosphere around the comet called the coma. ...
Time and Diurnal Motion
Time and Diurnal Motion

... defines 0 RA ...
ph507lecnote06
ph507lecnote06

... Absolute wavelength calibration and stability over long timescales is achieved by: • passing stellar light through a cell containing iodine, imprinting large number of additional lines of known wavelength into the spectrum • with the calibrating data suffering identical instrumental distortions as t ...
Visitor`s Guide to the Planets edit done
Visitor`s Guide to the Planets edit done

... no oxygen, so you will have to bring your own oxygen. The air is made out of poison and plus there are temperatures that average -185˚C. Saturn is -119˚C colder than Earth. The most memorable thing about Saturn is its tremendous rings. We want to see them up close. An interesting thing about the rin ...
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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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