PPT-Estimate of the Age of the Universe Through Time

Author : phoebe-click | Published Date : 2016-06-08

By Dr Harold Williams of Montgomery College Planetarium httpmontgomerycollegeeduDepartmentsplanet Just Goggle Montgomery College Planetarium First given on

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Estimate of the Age of the Universe Through Time: Transcript


By Dr Harold Williams of Montgomery College Planetarium httpmontgomerycollegeeduDepartmentsplanet Just Goggle Montgomery College Planetarium First given on Creation day celebration . For more information see HUDs Special Information Booklet on settlement charges your TruthinLending Disclosures and other consumer information at wwwhudgovrespa If you decide you would like to proceed with this loan contact us Purpose Summary of you Expanding Universe – consistent w/ a Big Bang?. Olber’s Paradox. Large Scale Structure and relation to Dark Matter. Evidence for the Big Bang. The Cosmic Microwave Background. The abundances of the elements. Lecture . 10; . May . 14 2013. Previously… on astro-2. If the universe is homogenous and isotropic and correctly described by General Relativity:. At any given time the universe is a 3D space. It could be open/close/flat. w. here does it end?. Chris North. Cardiff University. The speed of light. c = 299,792,458 m/s. . or 670,616,629 miles per hour. . or 2 million . million. furlongs per fortnight. or ~300,000 km/s. The Milky Way Galaxy. When you look into the hazy band of light across the sky, you are actually looking at our galaxy from the inside. While an awesome sight, you can only truly begin to see it if you get away from city lights on a moonless night. . http://www.pa.uky.edu. I will add 5 points on your final exam if you complete the evaluation.. Edwin Hubble’s next project.. Having established in 1925 that galaxies were not in the Milky Way, Hubble used the Mt Wilson telescope to obtain spectra of galaxies.. Lecture . 11; . May . 21 2013. Previously… on astro-2. In an expanding universe the relationship between redshift and distance depends on the cosmological parameters (i.e. the geometry and expansion of the universe). Why?. b. -values for Three Different Tectonic Regimes. Christine . Gammans. What is the . b. -value and why do we care?. Earthquake occurrence per magnitude follows a power law introduced by Ishimoto and Iida (1939) and Guten. Hubble Expansion and the Big Bang . The fact that more distant galaxies. have higher . redshifts. . indicates that the universe is expanding. This implies that the universe was born in a huge explosion, or . You want your answer to BE IN PLAY!. Close to the correct answer.. You don’t want to be OUT IN LEFT FIELD!. I Can Make a Ballpark Estimate. Remember. When you make a Ballpark Estimate you change the numbers to close but EASIER numbers that you can easily add in your head.. If the universe was 1 year old . . .. Science/religion – either/or?. How do we predict the conditions of the early universe?. What are the different eras in the early universe?. What key lines of evidence support the Big Bang model?. The Snowflake Universe Overview of Snowflake Universe Model for Bahamas Conference May 13, May 17, 2018 Printed May 11, 2018 (Reprinted/edited for PowerPoint Distribution May 29)  By John M. Kulick (B.S.E.) NOTE: A health risk assessment or appraisal includes questions on medical history, health status, and lifestyle and is designed to identify the health risks of the person being assessed.. SOURCE: Kaiser/HRET Survey of Employer-Sponsored Health Benefits, 2009-2016.. Astro. Ch. 11-1. Cosmology. The . study of the nature, origin, and evolution (how it changes) of the universe. Basically . the study of the universe as a whole. Cosmology . is an attempt to understand how the universe works.

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