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Lecture13
Lecture13

... takes place on approximately the free-fall timescale, which can be as short as a few hundred years. ...
Fulltext PDF - Indian Academy of Sciences
Fulltext PDF - Indian Academy of Sciences

... known as Kepler’s Laws. The first of these is that planets move in elliptical, not circular orbits, around the Sun. Ellipses are curves which are at the bottom of a right circular cone which is sliced (without cutting the base) along a plane not parallel to the base. With their sister figures, the p ...
Chapter03
Chapter03

... I’ve found that many students think anyone who lived before 1900 (or perhaps even 1980) was hopelessly ignorant and dull. I love to use the accomplishments of the later Greek astronomers to teach them otherwise. Students seem impressed by Aristarchus’s work showing the enormous size of the solar sys ...
The Certification Exam
The Certification Exam

... 1.4 The four innermost planets from the Sun (terrestrial planets) are  Jupiter, Saturn, Uranus and Neptune  Mercury, Uranus, Earth and Mars Incorrect  x Missing   Mercury, Venus, Earth and Mars  Earth, Venus, Jupiter and Pluto ...
Problems 4 File
Problems 4 File

... ”I see myself as a huge fiery comet, a shooting star. Everyone stops, points up and gasps ”Oh look at that!” Then whoosh, and I’m gone... and they’ll never see anything like it ever again... and they won’t be able to forget me ever.” Jim Morrison (a) The asteroid 2060 Chiron is 8.5 astronomical unit ...
Integrative Studies 410 Our Place in the Universe
Integrative Studies 410 Our Place in the Universe

... • Different quantities will change by different factors! • Typical example: how does the circumference, surface, volume of a sphere change when its radius changes? ...
LAB1_1SEP09
LAB1_1SEP09

... to pole passing through Greenwich England ...
The Night Sky
The Night Sky

... • path in sky depends on location on CS and latitude of observer • some always above horizon, some always below, and some are above horizon for part of day; latter are observable during part of the year, when Sun’s position on CS places it below the horizon while the star is above it ...
Exploring the Universe, Test #3, Summer 97
Exploring the Universe, Test #3, Summer 97

... 27. Cassini’s division is a) a new form of math b) imaginary line which divides a planet into Eastern and Western hemispheres c) a gap in Saturn’s rings d) the space between Mars and Jupiter where there is no planet 28. The many ringlets which compose planetary ring systems are caused by a) gravitat ...
celestial si ghtseeing
celestial si ghtseeing

... themselves. They're suspended in space like weightless jewels. Of the planets, most have moons. Of the moons, some are bigger than planets. Both moons and planets can have tenuous atmospheres, or incredibly thick ones, or none at all. Much of the solar system’s awesome scenery has been photographed, ...
PowerPoint 2.6Mb
PowerPoint 2.6Mb

... use "daylight savings time" to make it get dark later (Sun hits meridian at 1pm) (but nothing astronomical happens; this is an arbitrary convention) ...
Grade 3: Solar System
Grade 3: Solar System

... Upon completion of all strings being put into place, each student group will choose one member to stand on their orbit strings in a straight line away from the sun. Students who are not participating will stand outside the solar system and observe the planets’ rotations and revolutions. The teacher ...
Words
Words

... Include a description of what the planet looks like. ...
Planet Nine
Planet Nine

... Include a description of what the planet looks like. ...
Chapter 7 Powerpoint - ftgms-Mock
Chapter 7 Powerpoint - ftgms-Mock

... -27.3 days to orbit the Earth -27.3 days to rotate once on its axis ...
Lecture PDF
Lecture PDF

... core; the lighter silicates and aluminum compounds rose to the surface to form a crust. Earth became density stratified – that is layered by density. The ocean formed as soon as Earth was cool enough for water to remain liquid. Life followed soon thereafter. ...
Fun Facts: Sunshine
Fun Facts: Sunshine

... The sun is by far the largest object in the Solar System. In fact it is so big that over one million earths could fit inside it! The sun is 93 million miles away but we receive just the right amount of sunlight to keep our planet habitable. ...
PPT - El Camino College
PPT - El Camino College

... – Students know how the differences and similarities among the sun, the terrestrial planets, and the gas planets may have been established during the formation of the solar system ...
Chapter 04
Chapter 04

... direction around the Sun. b. Inner planets orbit the Sun faster and pass outer planets as they orbit around the Sun. c. Each planet moves on an epicycle, that in turn moves on a deferent that circles around Earth. d. The Sun and Moon orbit Earth, whereas all the other planets orbit the Sun. e. None ...
Introduction to Astronomy
Introduction to Astronomy

The Origin of Modern Astronomy(Seeds)
The Origin of Modern Astronomy(Seeds)

... direction around the Sun. b. Inner planets orbit the Sun faster and pass outer planets as they orbit around the Sun. c. Each planet moves on an epicycle, that in turn moves on a deferent that circles around Earth. d. The Sun and Moon orbit Earth, whereas all the other planets orbit the Sun. e. None ...
Outer Solar System Exploration - Lunar and Planetary Institute
Outer Solar System Exploration - Lunar and Planetary Institute

... Weather more akin to earth: Earth is at the mercy of processes today that are taken to extremes on Saturn’s moon Titan: a thick greenhouse atmosphere with violent rainstorms, desertification, and seas with coastline erosion and climate impact. Atmospheric chemistry and astrobiology - The reducing at ...
Planets
Planets

... around it. Saturn's diameter at its equator is 74,600 miles which is almost ten times that of Earth. The planet can be seen from Earth with the unaided eye, but its rings cannot. Saturn was the farthest planet from the earth that the ancient astronomers knew about. They named Saturn after the Roman ...
Universal Gravitation
Universal Gravitation

... • Uranus had an orbit that Newton’s law of gravity did not correctly predict • Proposed that another planet was attracting Uranus in addition to the sun (Giant: Neptune) ...
16.6 NOTES How do astronomers measure distance? Objective
16.6 NOTES How do astronomers measure distance? Objective

... distance light travels in one year (about 10 trillion km). Light from the Sun reaches Earth in a little more than 8 minutes. Light from the North Star (Polaris), reaches earth in about 700 years. Astronomers can use parallax to find out distances to the closer stars. Parallax is the apparent change ...
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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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