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Galileo`s telescopes Galileo (1564
Galileo`s telescopes Galileo (1564

... ’The Earth’s axis precesses in space (i.e. slowly rolls around) once in ~26,000 years. The equinoxes move round the ecliptic › this has an indirect effect on the ...
Earth at Aphelion 2015
Earth at Aphelion 2015

... elliptical in shape. Because of this the earth is slightly closer to the sun in January, at perihelion, and a bit farther away in July, at aphelion. At 3 p.m. on the 6th the earth will be 94,506,507 miles from the sun or about 1½ million miles farther than average. Some people find this a bit confus ...
THE CHEMICAL CHARACTERISTICS OF A TERRESTRIAL
THE CHEMICAL CHARACTERISTICS OF A TERRESTRIAL

... Introduction: Despite Titan’s distance from the Sun, it is characterized as Earth-like. Titan has a moderate atmosphere that is ten times more massive than Earth’s, albeit Titan is less than half the size of Earth. It also has weather patterns with rain, clouds, and wind [1], and even rivers, lakes, ...
Planets - learnfactsquick.com
Planets - learnfactsquick.com

... Tharsis - A huge bulge on the Martian surface. It's about 4000 km across and 10 km high! Though there is no water on Mars now, it is thought that large lakes or even oceans may have once existed on this planet. Clear evidence of water erosion can be seen in old river channels and floodplains. It see ...
Training Guide
Training Guide

... g. Experiment w/ sun’s energy using tools . . . UV Beads and Sun Print Paper (see SS NBs and p8 Binder) >> SS complete NBs and then collaboratively whiteboards more examples of solar energy transforming into chemical energy and showing color change (sunburn, dry grass, ripe fruit . . .) >> add to NB ...
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Document

... because the Sun is lower in winter which means the Sun’s rays aren’t directly hitting Earth and have more atmospheres to pass through. In summer the Sun is higher which means the Sun’s rays are directly hitting the Earth and have fewer atmospheres to pass through. The reason for seasons is the Sun’s ...
Lesson #6: Solar System Model - Center for Learning in Action
Lesson #6: Solar System Model - Center for Learning in Action

... Tell them they can use any notes or sketches they have taken over the past few weeks to help them accurately assemble their diagrams. They can also look at the models they made in the first lesson plan to see what they can do to make their models today more accurate. 2. Tell students that their mode ...
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11venus4s

... Venus re-surfaces itself ...
Greek Astronomy - Galileo and Einstein
Greek Astronomy - Galileo and Einstein

... the point that was describing the cycle. Mercury and Venus, as shown in the figure, had epicycles centered on the line from the earth to the sun. This picture does indeed represent fairly accurately their apparent motion in the sky—note that they always appear fairly close to the sun, and are not vi ...
1 - Alice Pevyhouse
1 - Alice Pevyhouse

... will complete one circle ‘cycle’ and point back at the same point. This is known as? 24.The Earth’s axis of tilt can vary from its current 23.5 degree tilt (T/F) 26. In another 13,000 years, Earth's axial tilt will point in the opposite direction it does now. Assuming the other astronomical influenc ...
Lecture 1
Lecture 1

... exoplanet — A moderately large object that orbits a star and shines primarily by reflecting light from its star. According to the 2006 definition of the IAU (International Astronomical Union), an object can be considered an exoplanet only if it: 1. orbits a star (or stellar remnant) 2. has a mass l ...
Days and Years
Days and Years

... The moon is Earth’s closest neighbor in space—much closer than any planet. In fact, the average distance from Earth to the moon is only about 30 times Earth’s diameter. How much time? Even so, it is quite far away. On an average, the moon is 384,400 kilometers from Earth. If there One revolution fo ...
850616SemStudyGuide_AstSns
850616SemStudyGuide_AstSns

... could have it...)? Which planet looks most like Earth’s moon? Which is the hottest planet? Which planet is on it’s side? Which planets have retrograde rotation? What is true about Mars’ surface? What is true about Venus’ atmosphere? Which planets have rocky surfaces? Which planets are gas giants? Wh ...
Link to Notes - Coweta County Schools
Link to Notes - Coweta County Schools

... moon’s gravity on different sides of the Earth  Moon matters more because it’s closer, so the difference in pull is more  Sun does help though, since it’s mass is so large  Larger tides occur when sun and moon line up (spring tides), smaller ones occur when they are in opposition (neap tides) ...
Scales in the UniverseApollo
Scales in the UniverseApollo

... Pluto and Charon - double planet (0.18 and 0.09 Earth diam 1.54 Earth diam apart at 29.7 to 49.4 AU from Sun) ...
Unit XII Study Guide
Unit XII Study Guide

... ____ 29. Much of the mass of the universe may be composed of a. electromagnetic waves. c. background radiation. b. cosmic microwaves. d. dark matter. Completion Complete each sentence or statement. 30. Because Earth’s orbit around the sun is an ellipse, and Earth is not always the same distance from ...
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... • In the 3rd Century B.C., a Greek, Aristarchus of Samos, figured out a way to measure the relative sizes and distances of the Moon and Sun. • He noticed that when the Moon was eclipsed by the Earth (월식) we can see the Earth's shadow creep across the face of the Moon. Earth's shadow is circular, and ...
Sacred Fire – Our Sun - University of Louisville
Sacred Fire – Our Sun - University of Louisville

... ● Kepler’s laws describe common features of the motions of orbiting objects, including their elliptical paths around the sun. Orbits may change due to the gravitational effects from, or collisions with, other objects in the solar system. (HSESS1-4) ● Cyclical changes in the shape of Earth’s orbit ar ...
(BAAO) Trial Paper 2015 Mark Scheme
(BAAO) Trial Paper 2015 Mark Scheme

... Also, in the question we considered the case of a total eclipse (“the eclipse is central”), while from London the eclipse on 20th March will be a partial one, with an obscuration of 85%. Therefore, the angular distance the Moon covers from first to last contact is smaller than the one we calculated. ...
3-planets-of-the-solar-system
3-planets-of-the-solar-system

... 37. How do Jupiter’s density and period of rotation compare to Earth’s? A) Jupiter is less dense and has a longer period of rotation. B) Jupiter is less dense and has a shorter period of rotation. C) Jupiter is more dense and has a longer period of rotation. D) Jupiter is more dense and has a shorte ...
Introduction Exploring the Heavens
Introduction Exploring the Heavens

... E.1 The “Obvious” View • Earth is average – we don’t occupy any special place in the universe • Universe: totality of all space, time, matter, and energy • Astronomy: study of the universe • Scales are very large: measure in light-years, the distance light travels in a year – about 10 trillion mile ...
Search for Life in the Universe
Search for Life in the Universe

... Stabilizes the Earth’s tilt at 2025, moderating the seasons How rare is a moon due to impact?: cf., Charon, Pluto’s moon Other ways to stabilize seasons: e.g., winds Can life migrate? ...
Teacher`s Show Guide
Teacher`s Show Guide

... Sun sets in our planetarium dome, we play "connect the dots" and observe a few of the more well-known constellations. But we notice that some points of light in the sky move over time. We look at our current planets visible from your yard tonight and then examine the changing phases of our Moon.. Em ...
What is the sun?
What is the sun?

... farther away from the sun and has it winter and the other part has its summer, Between wummer and winter, both halves of the earth are the same distance from the sun. Then they have spring and autumn. As the earth goes round in its orbit, we have our for seasons go on and on. ...
Multiple Choice - Secondary Science Wiki
Multiple Choice - Secondary Science Wiki

... New knowledge was revealed as new discoveries were made. Only the contributions that included all aspects of our current solar system were accepted. Scientists based the current models of the solar system primarily on the earliest discoveries. ...
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Comparative planetary science

Comparative planetary science or comparative planetology is a branch of space science and planetary science in which different natural processes and systems are studied by their effects and phenomena on and between multiple bodies. The planetary processes in question include geology, hydrology, atmospheric physics, and interactions such as impact cratering, space weathering, and magnetospheric physics in the solar wind, and possibly biology, via astrobiology.Comparison of multiple bodies assists the researcher, if for no other reason than the Earth is far more accessible than any other body. Those distant bodies may then be evaluated in the context of processes already characterized on Earth. Conversely, other bodies (including extrasolar ones) may provide additional examples, edge cases, and counterexamples to earthbound processes; without a greater context, studying these phenomena in relation to Earth alone may result in low sample sizes and observational biases.
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