'Water ice' diaporamas de présentation

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Formation of the Solar System

Formation of the Solar System. Week 5 (Welcome back from Spring Break). Quick overview of the Solar System. Space School: http://www.youtube.com/watch?v=mtKNH2Y2OJM&feature=related. Theories of How the Solar System Formed. Target 1:

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C osmic Ra y T elescope for the E ffects of R adiation ( CRaTER )

C osmic Ra y T elescope for the E ffects of R adiation ( CRaTER ). Harlan E. Spence, Principal Investigator Boston University Department of Astronomy and Center for Space Physics. What do we know?

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Drawing Conclusions

Drawing Conclusions. Entailment and Implicature. (1) Tom is an undergraduate. (2) Tom is a student. (3) I have a Siamese kitten. (4) I have a cat. Entailment. A relationship between two words or sentences such that if the first is true, the second must be true. Entailment Diagnostic.

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The Solar System

The Solar System. An Interactive Learning Station. The Planets. Currently, there are nine planets which have been discovered. They include:. Mercury. Neptune. Venus. Saturn. Earth. Uranus. Mars. Pluto. Jupiter. Mercury. Closest to the sun.

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Saturn, Its Rings, and Many Moons

Saturn, Its Rings, and Many Moons. INTRODUCTION:.

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INDEX

INDEX. What is frozen dessert? Types of frozen desserts. Method for production of frozen desserts. Recipe. Conclusion. Reference. WHAT IS FROZEN DESSERT?.

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Ice in our Solar System

Ice in our Solar System. International Polar Year Web Presentation Gregory A. Neumann NASA Goddard Space Flight Center Greenbelt, MD 20771 Gregory.A.Neumann@nasa.gov. What are ices made of?. Solar system is 99% hydrogen, helium, carbon and oxygen, with >0.1% of neon, iron, and nitrogen

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Water on Mars

Remote Sensing Ices on Mars. Water on Mars. The North Arctic of Mars. The white region does not move around from day to day. The white region increases in size during the winter and decreases in size during the summer. What do you think the white areas are? What might they be made of?.

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Lunar Volatiles: New Perspectives from Diviner Observations

Lunar Volatiles: New Perspectives from Diviner Observations. Paul Hayne 1 , Oded Aharonson 2,1 , David Paige 3 , and the Diviner Lunar Radiometer Team 1 California Institute of Technology 2 Weizmann Institute of Science 3 University of California, Los Angeles June, 2012.

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Properties of Fluids

Properties of Fluids. What happens if you drop a penny into a cup of water? Why?. The nail sinks because the density of the steel is greater than the density of the water. But.. What happens when...?.

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The Bodies of the Milky Way

The Bodies of the Milky Way By: Marie, Cherianne, Patti Mercury: First Planet from the Sun 8 th largest planet Orbit: 57,910,000 kilometers from the sun Mass: 3.30e23kg No moons or satellites Surface is similar to that of the moon Venus: 2 nd Planet from the Sun

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Blizzards and Hail

Blizzards and Hail. Contents. Blizzards. hail. conclusion. Blizzards. What is a Blizzard?

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Fabrication of a Wireless Sensor Network for Extreme Environments

Fabrication of a Wireless Sensor Network for Extreme Environments. EE 496, Fall 2006 By: Faye Yuen. Project Overview. Design a network of autonomous motes to: Distinguish between water/ice Collect data on environmental factors to supplement any bio-signs found

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MERCURY

MERCURY. 10 Interesting facts about Mercury!!!. Even though it is the closest planet to the sun it is still not the hottest planet because the temperature is uneven The side of Mercury which is not facing the sun is extremely cold and the other side facing the sun is extremely hot

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Galilean Moons

Galilean Moons. By: Lavon Brown. List of all the Galilean moons. Io, europa, ganymede, callisto. Info on Galilean Moons.

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NEO -Near Earth Objects

NEO -Near Earth Objects. Sloan Digital Sky Survey (SDSS) -Experimental Astrophysics Grid Fermi National Accelerator Laboratory Batavia-Illinois Steve Kent Neha Sharma. Near Earth Objects.

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Deep Impact

Deep Impact. By: Ashley King. Visual obstruction of the edge of the comet by the ejecta. T= 0.001(s). T= 1.747(s). T= 5.482(s). T= 3.615(s). Comparing light intensity before and after impact. Line A, t= 1.747(s). Intensity after Impact . Ejecta Fit is subtracted out. W/[m^2 sr um].

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Photo Credit: www.nasa.gov

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