'Big bang model' diaporamas de présentation

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Distance is the separation between two points in space.

The Cosmic Redshift. Distance is the separation between two points in space. Time is the separation between two events. . The Cosmic Redshift.

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Vorlesung 6:

Vorlesung 6:. Roter Faden: Cosmic Microwave Background radiation (CMB). Zum Mitnehmen. Pfeiler der Urknalltheorie: Hubble Expansion CMB Kernsynthese 1) beweist dass es Urknall gab und 2,3) beweisen,dass Univ. am Anfang heiss war. Bisher: Ausdehnung und Alter des Universums berechnet.

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Vorlesung 6+7

Vorlesung 6+7. Roter Faden: Cosmic Microwave Background radiation (CMB) Akustische Peaks Universum ist flach Baryonic Acoustic Oscillations (BAO) Energieinhalt des Universums.

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GECH119 A Brief History of Chemistry

GECH119 A Brief History of Chemistry. Dr. Ralph C. Gatrone Virginia State University Department of Chemistry and Physics. Fall, 2010. 1. Chapter Objectives. Introduce Origins of Universe Introduce Origins of Science Introduce History of Chemistry. Fall, 2010. 2.

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The beginning of the Universe as we know it began about 13.7 billion years ago.

The beginning of the Universe as we know it began about 13.7 billion years ago. What is Cosmology?. Cosmology is the study of the origin, structure, and evolution of the Universe. The Universe itself is defined as all matter, energy, and spacetime.

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The beginning of the Universe as we know it began about 13.7 billion years ago.

The beginning of the Universe as we know it began about 13.7 billion years ago. What is Cosmology?. Cosmology is the study of the origin, structure, and evolution of the Universe. The Universe itself is defined as all matter, energy, and spacetime.

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Chapter 17 Cosmology and Big Bang

Chapter 17 Cosmology and Big Bang. COSMOLOGY. How the Universe got started. The Big Bang Model Basis of the Big Bang model ? v = H d Other supporting evidence Consequences of the Big Bang model Universe is finite. Yes -- Quasars

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Large Scale Structure in the Universe

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The Standard Model of Fundamental Interactions Achievements and Prospects

The Standard Model of Fundamental Interactions Achievements and Prospects. Gilles Cohen-Tannoudji. Introduction. The scope of the Standard Model.

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Welcome to ESC 102 Evolution of Earth and Life Historical Geology Fall 2014

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Particles, Nuclei, and the Cosmos

Particles, Nuclei, and the Cosmos. Where Have Your Atoms Been? The Big Bang The Creation of the Elements. Gary D. Westfall Michigan State University. History of the Universe. Where Have Your Atoms Been?. The universe was created in the big bang 13 to 15 billion years ago

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What can we learn from CMB in the Planck area? (Planck is going to be launch May 6)

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HOT Big Bang

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Cornell Notes...

Cornell Notes. TITLE. This column gets filled out LATER! Can be key questions about notes used as study questions for test Can also be questions about things you did not understand. Notes will go here from my PowerPoints Bulleted or outlined information works best

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EXPANDING UNIVERSE

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30.3 Big Bang Theory

30.3 Big Bang Theory. Doppler Effect. Doppler effect = apparent shift in the wavelengths of energy emitted by an energy source moving away from or towards an observer. Spectroscope. Scientists used a spectroscope to study what elements were in stars

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Thursday August 30, 2012

Thursday August 30, 2012. (The Big Bang Theory and General Relativity; The Doppler Effect and Red Shift). The Launch Pad Thursday, 8/30/12. Which of the following best describes the Big Bang Theory?. The Universe has always existed as it is today, and always will.

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The Evidence for the Big Bang

The Evidence for the Big Bang. Student Resource Sheet 5 Science and Religion in Schools: Unit 4a. Evidence for the Big Bang. The Big Bang model is a concise explanation for 3 independent observations: The red shift of light from distant galaxies

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