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PowerPoint file - High Point University
PowerPoint file - High Point University

... Leonid meteor storms happen when Earth plows through clouds of dusty debris shed by comet 55/P Tempel-Tuttle. Right now Earth is heading for two such clouds. "We'll collide with both of them on Tuesday morning, Nov. 19th," says Cooke. "The first cloud will cause a flurry of meteors over Europe at ab ...
Explain. How is Copernicus`s description of the system of planets
Explain. How is Copernicus`s description of the system of planets

... • The theory of the moon's origin that best fits the evidence is called the collision theory. • Material from the object and Earth's outer layers was thrown into orbit around Earth. • Eventually, this material combined to form the ...
PowerPoint Presentation - AST121 Introduction to Astronomy
PowerPoint Presentation - AST121 Introduction to Astronomy

... Leonid meteor storms happen when Earth plows through clouds of dusty debris shed by comet 55/P Tempel-Tuttle. Right now Earth is heading for two such clouds. "We'll collide with both of them on Tuesday morning, Nov. 19th," says Cooke. "The first cloud will cause a flurry of meteors over Europe at ab ...
Lecture - Faculty
Lecture - Faculty

... • The current layout of our solar system may bear little resemblance to its original form • This view is more in line with the “planetary migration” thought to occur even more dramatically in many extrasolar planet systems • It may be difficult to prove or disprove these models of our early solar sy ...
Inner Planets Mercury
Inner Planets Mercury

... planet from the sun at a distance of about 150 million km (93 million miles). ...
Mercury - alexanderscience8
Mercury - alexanderscience8

... structures. Uranus has a faint ring system and 27 known moons. The plain aquamarine face of Uranus confirms the fact that Uranus is covered with clouds. The sameness of the planet's appearance shows that the planet's atmosphere is mostly composed of one thing, methane. The planet appears to be blue- ...
planet
planet

... – is in orbit around the Sun, – has sufficient mass to assume hydrostatic equilibrium (a nearly round shape), and – has "cleared the neighborhood" around its orbit. ...
Document
Document

... More violent and rapid impact accretion. The final stage of accretion has been described as 'runaway accretion'. Planetesimals are swept up into well defined zones around the sun which approximate to the present orbits of the terrestrial planets. The process leads eventually to a small number of lar ...
February 6
February 6

... of the Sun's apparent path (the ecliptic), that includes the apparent paths of the Moon and the planets Mercury, Venus, Mars, Jupiter, Saturn, Uranus, and Neptune. ...
Shape of Earth?
Shape of Earth?

... establish the size of the earth. Study the diagram on P 551 1. Who is credited with the first successful measurement of the earth’s circumference? 2. When did he do this? 3. What two variables did he need to measure in order to calculate the circumference of the earth? 4. Why do you think he chose t ...
http://circle.adventist.org/files/nadspiritual/earthsci/saearthscilabs.pdf
http://circle.adventist.org/files/nadspiritual/earthsci/saearthscilabs.pdf

... These Earth Science labs are numbered according to the chapter that they relate to. I’ve included the chapter titles of the book I currently use (Feather, Snyder, Zike, 2005, Earth Science, Glencoe McGraw Hill). The numbering of the labs I use is as follows: The first number in the triplet indicates ...
1 - TECC Science
1 - TECC Science

... (b) Explain why there could be no liquid water on the surface of: (i) Mars ............................................................................................................................. ................................................................................................... ...
venus_transit - University of Glasgow
venus_transit - University of Glasgow

... observations were published. e.g. Thomas Hornsby (1771): 1 A.U. = 93,726,900 miles (between 90 Captain James Cook ...
Astronomy Comprehensive Test
Astronomy Comprehensive Test

... the spectra of most galaxies shifted toward the red end of the spectrum. Another American astronomer, Edwin Hubble, later interpreted this discovery as evidence that __________________________________ ...
The Earth in Space
The Earth in Space

... to 90,000 degrees F. The Sun has a period of high activity of solar storms, also called sunspots, every eleven years. ...
Meteoroids! Asteroids! Comets!
Meteoroids! Asteroids! Comets!

... •  Q: Which is larger, asteroid or meteoroid? •  Asteroids are larger than meteoroids. ...
Meteoroids-Asteroids-Comets
Meteoroids-Asteroids-Comets

... • Q: Which is larger, asteroid or meteoroid? • Asteroids are larger than meteoroids. ...
Meteroroids! Asteroids! Comets!
Meteroroids! Asteroids! Comets!

... • Q: Which is larger, asteroid or meteoroid? • Asteroids are larger than meteoroids. ...
Science 9 Unit 5: Space Name
Science 9 Unit 5: Space Name

... unit is used for measuring ‘local’ distances in the solar system. It is equal to the distance from the center of the Sun to the center of the Earth (approximately 149,599,000 kms). Light year is equal to the distance light travels in 1 year (approximately 9.5 trillion kms). It is used for longer di ...
astrophysics 2009
astrophysics 2009

... Earth, Mars, Jupiter, Saturn, Uranus, Neptune and Pluto. -make up a mnemonic to remember the order eg: Most Very Eminent Men Just Sleep Under New Planets (MVEMJSUNP) -in order of increasing size, they are Pluto, Mercury, Mars, Venus, Earth, Uranus, Neptune, Saturn and Jupiter. -the moons or natural ...
Formation of the Solar System The Solar System
Formation of the Solar System The Solar System

... – Planets all revolve in the same direction. ü – Most planets and the Sun rotate in the same direction that the planets revolve. ü – Planets have almost all of the angular momentum of the Solar System. ü – Spacing between planets follows a regular pattern (Bode’s Law). ? ...
Lesson 2_GoingSolar
Lesson 2_GoingSolar

... Even Sol needs a little help sometimes  It takes more than just heat to keep our planet warm  Earth’s atmosphere (the particles in the air above ...
Test 2 review session
Test 2 review session

... Inner parts of Solar Nebula hotter (due to forming Sun): mostly gas. Accretion of gas atoms onto dust grains relatively inefficient. Jovian planets: Outer parts cooler: ices form (but still much gas), also ice "mantles" on dust grains => much more solid material for accretion => larger planetesimals ...
Lecture (Powerpoint)
Lecture (Powerpoint)

... Even more objects in early solar system; many have been swept up/accreted/kicked out since then Earth's atmosphere protects against smaller objects ...
Earth, Moon, Sun Sort
Earth, Moon, Sun Sort

... The moon is a small rocky satellite. It is about ¼ the size of the Earth. It is about 1/8 the mass of the Earth. It has extreme temperatures and virtually no atmosphere, water, and life. ...
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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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