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Exam 1 Astronomy 100, Section 3 Select the most appropriate
Exam 1 Astronomy 100, Section 3 Select the most appropriate

... (A) kinetic energy increased by a factor of 3 (B) kinetic energy increased by a factor of 9 (C) kinetic energy decreased by a factor of 3 (D) kinetic energy decreased by a factor of 9 (E) kinetic energy did not changed 14. If the temperature of an object becomes twice as high, the wavelength where i ...
$doc.title

... In  cold  molecular  clouds.     In  warm  ionized  Hydrogen  gas  clouds.     When  a  cloud  is  massive  enough  to  collapse  under  its  own  gravity.     When   a   cloud   is   hot   enough   for   thermal   pressure   to   ...
Sample pages 1 PDF
Sample pages 1 PDF

... motion of this outermost sphere was transmitted to an outer sphere of Jupiter; and between the inner sphere of Jupiter and the outer sphere of Saturn lie three additional spheres, and so on and so on with Mars, Venus and Mercury, as well as spheres for the Moon and the Sun. and all these spheres wer ...
Chapter 2: Measuring Earth - Westmoreland Central School
Chapter 2: Measuring Earth - Westmoreland Central School

... • Lithosphere – Continuous shell of rock around Earth – Mostly covered by soil and loose rock ...
Frostburg State Planetarium presents
Frostburg State Planetarium presents

... Bright points we see at night? • Even the nearest planets appear as * (points) as we see them with our eyes; for even these objects very far away (if moon dist.=1, Venus dist.= 100) • To tell a planet from a star, all night stars twinkle and planets usually shine steady. • Also satellites (especial ...
The Origin of the Solar System
The Origin of the Solar System

... Earth has diameter 0.3 mm. Sun: ~ size of a small plum. Mercury, Venus, Earth, Mars: ~ size of a grain of salt. Jupiter: ~ size of an apple seed. Saturn: ~ slightly smaller than Jupiter’s “apple seed”. ...
Astronomy 07 Life in the Universe Final Exam Test Bank Homework
Astronomy 07 Life in the Universe Final Exam Test Bank Homework

... E) only during a short spike at the end of the Hadean 32. The late heavy bombardment occurred A) five times in the last 570 million years B) at the end of the Cretaceous, and the beginning of the Tertiary C) several times, at more or less regular intervals throughout the Hadean and Archaean D) durin ...
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... are easier to see than dim things. In particular, they can be seen farther away. Without realizing this you might draw the conclusion that most stars are brighter than the Sun, because a simple count of the stars you can see with your naked eye indicates that this is the case. However, the much more ...
Small Bodies of the Solar System
Small Bodies of the Solar System

... • Pluto’s Orbit is highly eccentric (0.250), highly inclined to the plane of the solar o system (17.2 ), and its orbit crosses Neptune’s! • Since Jan 23, 1979 and until March 15,1999 Pluto is closer to the Sun the Neptune! ...
Small Bodies of the Solar System - Astronomy
Small Bodies of the Solar System - Astronomy

... • Pluto’s Orbit is highly eccentric (0.250), highly inclined to the plane of the solar o system (17.2 ), and its orbit crosses Neptune’s! • Since Jan 23, 1979 and until March 15,1999 Pluto is closer to the Sun the Neptune! ...
Kinesthetic Astronomy: Earth`s Rotation
Kinesthetic Astronomy: Earth`s Rotation

... Many people have a hard time interpreting drawn diagrams and understanding how the earth moves in relationship to the sun. In a 2008 California Academy of Sciences Survey we discovered that many adults don’t know that the earth takes 365 days to travel around the sun. This concept was also shown in ...
XI. Astronomy: Solar-System Debris and Comets
XI. Astronomy: Solar-System Debris and Comets

... g. Being primitive objects, asteroids provide clues to the Solar System’s origin. h. Asteroids in the inner half of the asteroid belt are light-colored, like terrestrial rocks, composed of different kinds of silicate minerals and metals. (Stony = upper left figure above). Some melted and resolidifie ...
Mechanical Systems Topics 1 and 2
Mechanical Systems Topics 1 and 2

... The ancient Greeks studied the stars and the celestial bodies. They had a word that meant ‘wanderer’ to describe a celestial body that changed its position in the sky. ‘Wanderer’ is the origin for the word A. Comet B. Asteroid C. Star D. Planet ...
BBC Stargazing Live Star and Moon Guide
BBC Stargazing Live Star and Moon Guide

... The Moon is the Earth’s only natural satellite. Apart from Mercury and Venus, all the other planets in the Solar System have their own moons. Jupiter has more than 60 but only four can be seen easily through a small telescope. These are known as the Galilean moons in honour of their discovery by Gal ...
The Sun, Moon, & Earth
The Sun, Moon, & Earth

... Some people think we have different seasons on earth because of how far away the earth is from the sun. But that is not true. We have different seasons because the sun’s rays are more direct on certain parts of the earth at different times of the year. ...
AGU Fall 2011 SH34B-08
AGU Fall 2011 SH34B-08

... In rotation, the constituent particles of a body move in concentric trajectories with velocities that depend upon their position in relation to the axis of rotation In revolution, the particles of the body move in parallel trajectories with identical velocities (aside from small differences produced ...
Jupiter is 90000 miles in diameter. It is 10 times the size of the earth
Jupiter is 90000 miles in diameter. It is 10 times the size of the earth

... represent descending areas of low pressure. Jupiter radiates heat energy out to space by way of convection. The zones carry energy to the surface and then cool, and sink again. ...
Frostburg State Planetarium presents
Frostburg State Planetarium presents

... • Even the nearest planets appear as * (points) as we see them with our eyes; for even these objects far away Venus at closest 100x farther than our moon • To tell a planet from a star, all night stars twinkle and planets usually shine steady. • Also satellites (especially Space Station) shine stead ...
Final Study Guide Questions Earth Science Spring 2016 Mr. Traeger 1
Final Study Guide Questions Earth Science Spring 2016 Mr. Traeger 1

... What should you do when an earthquake strikes? What shouldn’t you do? ...
Section 5 — Earth Sciences (The Solar System) Student Edition
Section 5 — Earth Sciences (The Solar System) Student Edition

... More observations through time, and further questions that were investigated (and continue to be investigated) showed that Earth is not the center of the universe after all. In the 1500’s a Polish scientist named, Copernicus, used mathematics and his observations of the sky (without a telescope, whi ...
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The Earth in Context: Universe and Solar System

... with giant red spot visible (a) variable expanding/contracting in size (b) thought to be caused by cyclonic storm in atmosphere ...
Diapozitivul 1
Diapozitivul 1

... Saturn distinguished by its extensive ring system ...
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... – Our solar system is full of planets, moons, asteroids and comets, all of which revolve around the Sun at the center. – When a star forms from a nebula, gravity pulls most of the material into the new star, but some may also clump together to form objects in a solar system. ...
HERE
HERE

... 11. Sun contains 99.8% of Solar System mass 12. 98% of angular momentum resides in planet orbits 13. planet types/compositions depend on location (beware Moon) 14. planetary atmospheres contain ice fractions dependent on temp 15. all planets, large moons/asteroids differentiated (were warm) 16. rapi ...
Earth Science Quarter 1 Credit Recovery
Earth Science Quarter 1 Credit Recovery

... How did planets form from smaller masses such as planetesimals and protoplanets? A protoplanet is created when many asteroids collide together and create a sphere with a molten core. Planetesimals are the many small pieces of asteroid that combine to make the protoplanet. ...
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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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