'Astronomical objects' presentation slideshows

Unit 6:Life, Death and Characteristics of Stars

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Light and Telescopes

Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode (presentation mode). Light and Telescopes. Chapter 6. Guidepost.

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Course notes - reminder

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Applications of Diffraction and Interference of Light

Applications of Diffraction and Interference of Light. By: Karen Cooper. Scanning Tunneling Microscopy. Past. Gave scientists the ability to explore and manipulate solid surfaces on the size scale of atoms. Helped discover fullerenes- spherical carbon molecules.

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Light and telescopes

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Solar Data Analysis

F. Breitling, G. Mann, C. Vocks 3 nd Workshop of the Solar Key Science Project of LOFAR Astrophysikalisches Institut Potsdam 2010 July 05. Solar Data Analysis. Overview The three LOFAR data types. Dynamic spectra Single station imaging Standard imaging RCU: Receiver unit

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Low Frequency, Wide-Field Astronomy with PAPER: Precision Array to Probe the Epoch of Reionization

Low Frequency, Wide-Field Astronomy with PAPER: Precision Array to Probe the Epoch of Reionization. Nicole Gugliucci Graduate Student, UVa /NRAO Advisor: Rich Bradley. Collaborators: D. Backer, A. Parsons, J. Manley, G. Foster, M . Wright, D. Werthimer , CASPER group (UCB),

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CAPSTONE Astronomy lecture 1, 07.05.2011

CAPSTONE Astronomy lecture 1, 07.05.2011. Course introduction, models of the sky. Lect. 1: Large and ancient questions.

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The House of Wisdom

The House of Wisdom. Sixth Grade Unit 5 Week 5. Tyanna Bischoff, Hawthorne . beacon. Words to Know. manuscripts. caravans. medieval. observatory. legacy. patron. Beacon Caravans Legacy Manuscripts Medieval Observatory Patron. legacy. Something

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The Early Period

The Early Period. The Beginnings of Classical Astronomy. Early Ideas. The Ancient Greeks were the first to try and explain the workings of the heavens in a systematic manner They used models and observations made only with the naked eye

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Neutron stars and beyond

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PART III : OVERVIEW OF THE UNIVERSE

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Brightnesses , sizes and motions of stars

Brightnesses , sizes and motions of stars . Recap. Project : due Friday 11/21 Campus observatory Information from brightnesses of stars Brightness depends on: distance, temperature and size If you know two of these, brightness can be used to give you the third

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What is dark matter?

What is dark matter?. 96% of the universe is missing In fact, all of the stuff we can detect in the universe: All of the matter All of the energy Only seems to account for 4% of the total size of the universe . Scientists have been measuring the movements of millions of stars and galaxies

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Space Exploration

Space Exploration. Benchmark. SC.8.E.5.12 Summarize the effects of space exploration on the economy and culture of Florida. Essential question : How has space exploration affected Florida?. Learning goal SWBAT explain the economic and cultural impact of space exploration on Florida.

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The Electromagnetic Radiation

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History of the Solar System

History of the Solar System. William Allen. Nebular Theory. The most popular theory of the formation of the solar system is the nebular theory.

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The Electromagnetic Radiation

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Relative Sizes of Astronomical Objects

Relative Sizes of Astronomical Objects. Antares is the 15th brightest star in the sky. It is more than 1000 light years away.

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