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THE EARTH
THE EARTH

... known to exist (although similar systems are likely to be common in the universe). Like that of all planets and stars, the earth's shape is approximately spherical, the result of mutual gravitational attraction pulling its material toward a common center. Unlike the much larger outer planets, which ...
Chapter 2
Chapter 2

... Questions and Exercises This content can also be found in your book following the chapter Summary of Key Concepts Surprising Discoveries? Suppose we make the discoveries described below. (These are not real discoveries.) Decide whether each discovery should be considered reasonable or surprising. Ex ...
The mass of the Moon is 1/81 of the mass of the Earth. Compared to
The mass of the Moon is 1/81 of the mass of the Earth. Compared to

... the radius. This means that compared to the amount of energy required to move an object from the Earth’s surface to infinity, the amount of energy required to move that same object from Planet X’s surface to infinity is A. 4 times as much. B. twice as much. C. the same. D. 1/2 as much. E. 1/4 as muc ...
Space_Review_Coelho
Space_Review_Coelho

... The Sun for $300 They are all spheres, have gravity (but of course different amounts of gravity), all have atmospheres (Earth’s atmosphere is the only one to support life and the Moon’s atmosphere isn’t very sustainable though)… ...
The mass of the Moon is 1/81 of the mass of the Earth. Compared to
The mass of the Moon is 1/81 of the mass of the Earth. Compared to

... the radius. This means that compared to the amount of energy required to move an object from the Earth’s surface to infinity, the amount of energy required to move that same object from Planet X’s surface to infinity is A. 4 times as much. B. twice as much. C. the same. D. 1/2 as much. E. 1/4 as muc ...
File - Mr. Bogdon`s Website
File - Mr. Bogdon`s Website

... Millions to billions of miles, or astronomical units (AU). (An AU is the average distance from Earth to the sun, or 93 million miles.) ...
speed
speed

... the radius. This means that compared to the amount of energy required to move an object from the Earth’s surface to infinity, the amount of energy required to move that same object from Planet X’s surface to infinity is A. 4 times as much. B. twice as much. C. the same. D. 1/2 as much. E. 1/4 as muc ...
Frostburg State Planetarium presents
Frostburg State Planetarium presents

... Bright steady points at night? • Even the nearest planets appear as * (points) as we see them with our eyes; for even these objects very far away (moon=1 unit). Venus 100x farther. • To tell a planet from a star, all night stars twinkle and planets usually shine steady. • Also satellites (especiall ...
Sample pages 1 PDF
Sample pages 1 PDF

... Mars, have similar rocky surfaces and the four together are collectively known as the “terrestrial planets”. The rocky nature of Mars is most vividly illustrated by the landscape images sent back by the Martian rovers Spirit, Opportunity, and Curiosity. In contrast, the other four planets in the out ...
Document
Document

... Facts and photos used in the slideshow taken from: Sun: http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sun&Display=OverviewLong Mercury: http://solarsystem.nasa.gov/planets/profile.cfm?Object=Mercury&Display=OverviewLong Venus: http://solarsystem.nasa.gov/planets/profile.cfm?Object=Venus&Dis ...
winter
winter

... By an incredible coincidence, Polaris is almost directly over the North Pole. So it can be used to help us navigate. This is a temporary situation, however. Since the Earth is wobbling like a top, the pole slowly moves. This is called precession. ...
chapter01 - California State University, Long Beach
chapter01 - California State University, Long Beach

... 5. The Andromeda galaxy has an angular diameter of 5 degrees at a distance of 2.2x106 ly. We can find its true size by using the angular diameter formula L = 2DA/360, where D = distance, A = angle subtended, and L = linear diameter. Thus, L = 2 x 2.2x106 ly x 5 degrees / 360 degrees = 1.92x105 ly ...
The
The

... orbit around the Sun sometimes the Moon comes directly between the Earth and the Sun. This is called a solar eclipse; if the alignment is slighly imperfect then the Moon covers only part of the Sun's disk and the event is called a partial eclipse. When it lines up perfectly the entire solar disk is ...
CH 26 PPT
CH 26 PPT

... particles ** called the solar wind. These particles travel in all directions at a speed of about 450 kilometers per second (reaching Earth in a few days). Earth’s magnetic field deflects most of the solar wind particles around the planet. Solar flares (outbursts of light that rise up suddenly in are ...
Astro history 1
Astro history 1

... • With no street lights and no alarm clocks… • The Night sky was a great glowing question… • Who are we? (no answer yet?) • Why are we here (not clear on that one either…?) • Where are we? • Humans have been working on that one for a long time! ...
Exercise set five
Exercise set five

... Using each pair of observations, calculate the length of the sidereal day. (Hint: start by calculating how much earlier, in seconds, the later occultation occurred, then divide that by the number of days between the observations. This gives you how many seconds shorter a sidereal day is than a solar ...
Measuring the Sky - Physics and Astronomy and more!
Measuring the Sky - Physics and Astronomy and more!

...  True, they emit light, but it’s not a fluid ...
Earth`s Internal Structure I
Earth`s Internal Structure I

... depth. But, how can we obtain a more detailed picture of the variation of density with depth? ...
FREE Sample Here
FREE Sample Here

... © 2014 by McGraw-Hill Education. This is proprietary material solely for authorized instructor use. Not authorized for sale or distribution in any manner. This document may not be copied, scanned, duplicated, forwarded, distributed, or posted on a website, in whole or part ...
Introduction: Gravity
Introduction: Gravity

... -Gather, record, and organize data using appropriate units, tables, graphs or maps (4-5 INQD) -Explain the need for additional trials (INQE) -Create simple models, use the model to learn something, explain how the model is similar and different to the thing being modeled (4-5 INQF) -Generate a concl ...
FREE Sample Here
FREE Sample Here

... 1. The moon appears larger when it rises than when it is high in the sky because A. You are closer to it when it rises (angular-size relation). B. You are farther from it when it rises (angular-size relation). C. It's an illusion from comparison to objects on the horizon. D. It's brighter when it ri ...
Comparing the Chemical Compositions of the Sun and Earth
Comparing the Chemical Compositions of the Sun and Earth

... within about 4 AU (the snowline) and a more refractory solid beyond 4 AU. Similar consideration of the ices NH3 and CH4 explain why H, C and N are only partially depleted. Fe, Mg Ni,Ca, Al, Cr, Ti, V, Sr and Zr are refractory elements and have relative abundances that have not changed since the Eart ...
Formation of the Solar System Chapter 8
Formation of the Solar System Chapter 8

... because of the initially hot conditions. (some were supplied by comets) • Satellites like Ganymede have similar structures but have an ice layer on top (volatiles are more common in the outer nebula) ...
CHAPTER 4 PRECESSION OF THE EARTH`S AXIS
CHAPTER 4 PRECESSION OF THE EARTH`S AXIS

... The constant term of this speed corresponds to one full precession circle in 25,771.58 years. The precession rate is not a constant, but is (at the moment) slowly increasing over time, as indicated by the linear (and higher order) terms in T. In any case it must be stressed that this eqauation is on ...
Meteoroid/Meteor/Meteorite Facts
Meteoroid/Meteor/Meteorite Facts

... 1. A meteoroid is a small rock or particle of debris in our Solar System. They range in size from dust to around 33 feet in diameter (larger objects are usually referred to as asteroids). 2. A meteoroid that burns up as it passes through the Earth’s atmosphere is known as a meteor. If you’ve ever lo ...
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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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