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... from the harmful effects of the solar wind, these highenergy particles that the Sun is constantly bombarding us with, and this shield is really essential for us for our ...
Tides on Earth
Tides on Earth

... http://www.5min.com/Video/Learn-about-Ocean-Tides117529562 ...
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The Crust

... •Volcanism continually produces highly differentiated continental crust on Earth. •Venus surface appears to be all basalt. •Plate tectonics & volcanism do not appear to be happening on Venus (or Mars, Moon). •So Earth may be unique in Solar System. And plate tectonics & volcanism likely critical in ...
The Sun and the Origin of the Solar System
The Sun and the Origin of the Solar System

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Slide 1 - MrMrsCase

... Planets, their moons, asteroids, comets, dwarf planets. ...
Article - Iowa State University
Article - Iowa State University

... If you were traveling in a spaceship at 10 miles per second (36,000 miles per hour) it would take you 70,000 years to get to the next closest one. Could Earth be hit by an asteroid or meteor? For the most part, our atmosphere protects us by burning up the majority of space material as it enters. In ...
Essay One - Physics & Astronomy
Essay One - Physics & Astronomy

... Constellations are recognizable patterns of stars in the sky. (Based on stories and named in honor of them)  There are 88 constellations. (e.g. Orion) ...
Genetics: The Science of Heredity
Genetics: The Science of Heredity

... 15. If you are in a car that stops suddenly, your body keeps moving because it has ____________________. ...
Genetics: The Science of Heredity
Genetics: The Science of Heredity

... b. how much of the sunlit side of the moon faces Earth. c. how much of the moon’s surface is lit by the sun. d. whether or not an eclipse is occurring. ______ 9. When a meteoroid enters Earth’s atmosphere, it produces a streak of light called a(n) a. meteor. c. meteorite. b. asteroid. d. comet. ____ ...
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lecture9 Solar System1

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Please jot down or ponder your answers. 1. What causes seasons
Please jot down or ponder your answers. 1. What causes seasons

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b. Compare the similarities and differences of planets to the stars in
b. Compare the similarities and differences of planets to the stars in

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Objective or GLE: 6.1.A.a: Classify celestial bodies in the solar

... Most meteors are dissipated ( they are burned up) in flight and fall to the earth as dust; a meteor that reaches the surface of the earth or another planet is called a meteorite. ...
Space - mrhandley.co.uk
Space - mrhandley.co.uk

... are very dark and very faint. Scientists still haven't figured out what they are made of yet. ...
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Old Sample Exam #2

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... reactions that typically last mere seconds during the explosion of the supernova core. Scatters elements into cosmos into giant clouds. All elements heavier than Lithium are formed in the heart of stars. ...
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Some facts and concepts to have at your fingertips.

... maximum intensity is related to the temperature of the material. Example: cannon ball at 3000 deg K. Peak intensity is in the near-infrared. • A low density gas excited to emit gives an emission line spectrum. Example: neon light. • Cool gas in between the observer and a source of a continuous spect ...
Theories of the solar system
Theories of the solar system

... The word retrograde applies to the apparent backward motion of a planet. An old encyclopedia of astrology describes this retrograde motion as "…the effect of a slow-moving train as viewed from another train traveling parallel to it but at a more rapid rate, wherein the slower train appears to be mov ...
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Ecliptic 1 2 3 Three tell tale visual characteristics a planet:

... When Mercury or Venus move between the Earth and the sun or when they orbit on the sun’s far side, they appear near it in our day sky and can’t be seen. ...
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PLANETARY ATMOSPHERES HOMEWORK

... which is the total energy output of today’s Sun per second? (ans. 1x1038 reactions/sec). 1 Watt=1 Joule/sec. (5) (d) Calculate the total mass which should be burned/lost in one second? (ans: 6.68x1011 kg/sec) (5) (e) Assume that the present processes within the Sun will continue (not true) and the h ...
Answer Key - Science NetLinks
Answer Key - Science NetLinks

... 1. Planets that have calculated temperatures close to (but not exactly the same as) the real average surface temperatures are Mercury, Earth, and Mars. Answers may vary as to why. Some possibilities include: we assume that there is nothing impeding the radiation on its way through the interplanetary ...
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PPT, 13.2 Mb

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Friends of the Planetarium Newsletter September

... reaches of the solar system." Several senior members of the New Horizons science team were young members of Voyager's science team in 1989. Many remember how Voyager 2's approach images of Neptune and its planetsized moon Triton fueled anticipation of the discoveries to come. They share a similar, g ...
Solar system
Solar system

... Gravity is the force that pulls you toward other bodies or objects. For example the gravity on Earth pulls us and other things to itself. Gravity helps us because we would float out of Earth’s atmosphere and there is no oxygen in space so we would die. Our weight would be different on other planets ...
Astronomy Midterm Review Sheet
Astronomy Midterm Review Sheet

... the same direction as viewed from Earth. 20. Visible from the Northern Hemisphere all year long, and appear to rotate around Polaris. 21. Observed brightness as seen from Earth. 22. Occurs at 0 degrees declination, from the observer’s position. 23. Circle where the Earth’s equator, if extended outwa ...
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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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