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PPT
PPT

... Earth’s atmosphere is a pretty turbulent place Especially the lower atmosphere – observatories are on mountains! ...
Activity 8 Tilted Globe
Activity 8 Tilted Globe

... equivalent of a 90° tilt), so that the Sun is directly overhead for someone standing at the North pole. As the Earth spins now, the illuminated half of its surface is always the Northern hemisphere, and the dark half is always the Southern hemisphere! Clearly this is not true on our Earth, though it ...
February 2013 - astronomy for beginners
February 2013 - astronomy for beginners

... above) along which the Sun, Moon and planets appear to travel across the sky. It is flanked on the ecliptic by Taurus to the west (right) and Cancer to the east (left). To the south west is Orion (lower right) and to the north west (upper right) is Auriga with its very bright white star Capella dire ...
Your World is Tilted!
Your World is Tilted!

... The reason for this variation is the fact that the Earth's axis is not, in fact, perpendicular to the line from Earth to Sun. Rather, it tilts away from perpendicular by 23.5°. In this Activity, we will investigate the effects of this tilt, and see how it can explain these variations. To clarify th ...
Activity #3 How Do Atmosphere Change Over Time? The Role of
Activity #3 How Do Atmosphere Change Over Time? The Role of

... a. Wrap, trim, and tape plastic wrap or baggie to cover bar magnets to simplify cleaning the iron filings from the magnets at the end of the experiment. b. Cut off about 1.3 cm (0.50 in) of the bottom of a 2.5 cm (1 in) diameter paper or plastic cup. Label: Mars. c. Cut off about 1.3 cm (0.50 in) of ...
Celestial Motions
Celestial Motions

... shadow, and its appearance to us is determined by the relative positions of Sun, Moon, and Earth. • What causes eclipses? – Lunar eclipse: Earth’s shadow on the Moon – Solar eclipse: Moon’s shadow on Earth – Tilt of Moon’s orbit means eclipses occur during two periods each year. © 2010 Pearson Educa ...
class slides for Chapter 7
class slides for Chapter 7

... are less than 10 km in diameter and orbit at large distances from the planet. ...
night sky a field guide to the heavens
night sky a field guide to the heavens

... things were now for the first time, if, I say, they were now suddenly presented to mortals beyond all expectation, what could have been named that would be more marvelous than these things, or that nations beforehand would less venture to believe could be? Nothing, me thinks: so wonderous strange ha ...
Asimov, Isaac - Lucky Starr 05 - and the Moons of Jupiter
Asimov, Isaac - Lucky Starr 05 - and the Moons of Jupiter

... Bigman pounded his small right fist into the open palm of his other hand. "Sands of Mars, Lucky, how long do we have to wait here?" Â They were in Lucky's ship, theShooting Starr, whichwas in an orbit about Jupiter, having matched velociÂties with Jupiter Nine, the giant planet's outermostsatellite ...
Uranus
Uranus

... elliptical (oval-shaped) orbit, which it completes in 30,685 Earth days, or just over 84 Earth years. As it orbits the sun, Uranus also rotates on its axis, an imaginary line through its center. The planet's interior (ocean and core) takes 17 hours 14 minutes to spin around once on its axis. However ...
Compartive Planetology I: Our Solar. System
Compartive Planetology I: Our Solar. System

... across—about i/. of the width of a human hair and far too small to be seen without a microscope. The planets themselves are very small compared to the distances between them. Indeed, while an airliner traveling at 1000 km/h (620 mi/h) can fly around Earth in less than two days, at this speed it woul ...
For stars
For stars

... • Even though Polaris is currently the North star, it doesn’t lie due North –and eventually will move and Vega will be our North Star, Why do you think this is happening? Discuss with your elbow partner, write down your thoughts on your white board, be ready to defend them. ...
Distant future of the Sun and Earth revisited
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... out to and including Mars are engulfed, either at the red giant branch (RGB) phase – Mercury and Venus – or at the later asymptotic giant branch (AGB) phase – the Earth and Mars. However, the Sun loses a significant amount of mass during its giant branch evolution, and that has the effect that the p ...
Venus has no ozone layer
Venus has no ozone layer

... Venus has a diameter that 95% of the Eart. Compared to Earth it is less in weight, having 81.55 of the Earth’s mass. The orbital period of Venus is 224.7 days. The winds on the top of the clouds are very strong but the same of the surface of the Venus is very low, a few kilometres speed. . Volcanic ...
Comets - LEAPShares
Comets - LEAPShares

... visible light), is the largest asteroid but is so small that it is not considered a planet. Because it does not orbit a body other than the Sun, it is also not classified as a moon. This image of Ceres suggests it has regions of ice and rock on its surface. The asteroid will be visited by the Dawn s ...
r earth - mrbernabo
r earth - mrbernabo

... The further you get from the earth, the weaker the force of gravity gets. At an infinite distance the force approaches zero If you shoot an object upward and there is no friction at 11,200 m/s. It will never fall back to earth, it will just move ...
DYNAMICS OF THE GIANT PLANETS OF THE SOLAR SYSTEM IN
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... model’’ because it was developed by an international collaboration at the Nice Observatory in France. This model argued that, if the giant planets had a more compact configuration at the end of the gas-disk phase, their subsequent migration driven by interaction with a planetesimal disk could have f ...
Astronomy Puzzle-1
Astronomy Puzzle-1

... Answers of puzzle are hidden in the box. The answers are either vertical, horizontal, diagonal or in reverse order. Sample answer is shown in the puzzle. Clues 1. The Astronomy research institute set up by the University Grant Commission. 2. The research institution set up by the Department of Spac ...
Homework #2, AST 203, Spring 2012
Homework #2, AST 203, Spring 2012

... that it is very close to the ratio of two small integers; which integers are these? Thus the two planets regularly come close to one another, in the same part of their orbits, which allows them to have a maximum gravitational influence on each other’s orbits. This is an example of an orbital resonan ...
DTU_9e_ch09 - University of San Diego Home Pages
DTU_9e_ch09 - University of San Diego Home Pages

... out compared to those of the planets. Notice how many significant events occurred on Earth during Pluto’s present orbit of the Sun. (b) Pluto’s passes inside the orbit of Neptune, but the two will never collide due to a 3:2 synchronization. ...
The ExOoS Mission - Extraterrestrial Octopus on Steroids
The ExOoS Mission - Extraterrestrial Octopus on Steroids

... changes. The spectra signature of sodium present two peaks very close to each other; at 5.890 and 5.986 µm (figure 5). To distinguish between these two peaks we would need a resolution of at least 10−3 , which is a very high value for remote sensing. However, advances in technology and the use of in ...
Jupiter`s Radio Signals
Jupiter`s Radio Signals

Uranus Fun Facts
Uranus Fun Facts

... Uranus' rotational axis is strongly tilted on its side (97.9°). Instead of rotating with its axis roughly perpendicular to the plane of its orbit (like all the other planets in our Solar System), Uranus rotates on its side (along its orbital path). This tipped rotational ___________________________ ...
PE-00-intro-course outline
PE-00-intro-course outline

... all physical phenomena. To become familiar with the scientific view of human society, social organization, and the processes of social change. To become familiar with the impact technology has had on the earth and its inhabitants, and its potential for the future. To acquire knowledge of the great s ...
SELF-TEST: True or False? 1. The Sun is a rather
SELF-TEST: True or False? 1. The Sun is a rather

... 1. The Sun is a rather normal star. HINT 2. The average density of the Sun is significantly greater than the density of the Earth. HINT 3. The Sun's diameter is about 10 times that of Earth. HINT 4. The Sun's differential rotation indicates that it is not solid. HINT 5. In the solar radiation zone, ...
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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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