How Do You Find an Exoplanet?
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The Big Bang: New Light on an Old Theory
Physics The Big Bang: New light on an old theory This lesson explores the evidence for the Big Bang theory of the origin of the Universe. In it, you will learn about the following: • Using the electromagnetic spectrum (EMS) to define radiation. • The Big Bang origin of the Universe theory. • What is the cosmic microwave background and how does this support the Big Bang theory? • Universe or Multiverse? Get ready for extragalactic time travel as we squeeze and bend our way through this space-time lesson. This is a print version of an interactive online lesson. To sign up for the real thing or for curriculum details about the lesson go to www.cosmosforschools.com Introduction: The Big Bang (P1) Scientists say they have just made a discovery that will help explain how our Universe began. If they are right, it could be the biggest, most exciting event in physics ever. Looking through a telescope into the clear skies over the South Pole, scientists spotted what they say is evidence of gravitational waves, or ripples in space-time, from the split second after the birth of the Universe – what scientists call the Big Bang. What’s got everyone so excited by this is that Albert Einstein predicted the existence of gravitational waves when he described how space and time were related and could be bent by huge forces of gravity. What the scientists at the South Pole think they saw was not gravitational waves – they would be invisible – but the effect of the waves on the light left over from the Big Bang. -
Intelligent Design: Is It Really Worth It?
Leaven Volume 17 Issue 2 Theology and Science Article 6 1-1-2009 Intelligent Design: Is It Really Worth It? Chris Doran [email protected] Follow this and additional works at: https://digitalcommons.pepperdine.edu/leaven Part of the Biblical Studies Commons, Christianity Commons, and the Religious Thought, Theology and Philosophy of Religion Commons Recommended Citation Doran, Chris (2009) "Intelligent Design: Is It Really Worth It?," Leaven: Vol. 17 : Iss. 2 , Article 6. Available at: https://digitalcommons.pepperdine.edu/leaven/vol17/iss2/6 This Article is brought to you for free and open access by the Religion at Pepperdine Digital Commons. It has been accepted for inclusion in Leaven by an authorized editor of Pepperdine Digital Commons. For more information, please contact [email protected], [email protected], [email protected]. Doran: Intelligent Design: Is It Really Worth It? Intelligent Design: Is It Really Worth It? CHRIS DORAN imaginethatwe have all had occasion to look up into the sky on a clear night, gaze at the countless stars, and think about how small we are in comparison to the enormity of the universe. For everyone except Ithe most strident atheist (although I suspect that even s/he has at one point considered the same feeling), staring into space can be a stark reminder that the universe is much grander than we could ever imagine, which may cause us to contemplate who or what might have put this universe together. For believers, looking up at tJotestars often puts us into the same spirit of worship that must have filled the psalmist when he wrote, "The heavens declare the glory of God; the skies proclaim the work of his hands" (Psalms 19.1). -
Planet Formation
3. Planet form ation Frontiers of A stronom y W orkshop/S chool Bibliotheca A lexandrina M arch-A pril 2006 Properties of planetary system s • all giant planets in the solar system have a > 5 A U w hile extrasolar giant planets have semi-major axes as small as a = 0.02 A U • planetary orbital angular momentum is close to direction of S un’s spin angular momentum (w ithin 7o) • 3 of 4 terrestrial planets and 3 of 4 giant planets have obliquities (angle betw een spin and orbital angular momentum) < 30o • interplanetary space is virtually empty, except for the asteroid belt and the Kuiper belt • planets account for < 0.2% of mass of solar system but > 98% of angular momentum Properties of planetary system s • orbits of major planets in solar system are nearly circular (eMercury=0.206, ePluto=0.250); orbits of extrasolar planets are not (emedian=0.28) • probability of finding a planet is proportional to mass of metals in the star Properties of planetary system s • planets suffer no close encounters and are spaced fairly n regularly (Bode’s law : an=0.4 + 0.3×2 ) planet semimajor axis (A U ) n an (A U ) Mercury 0.39 −∞ 0.4 V enus 0.72 0 0.7 Earth 1.00 1 1.0 Mars 1.52 2 1.6 asteroids 2.77 (Ceres) 3 2.8 Jupiter 5.20 4 5.2 S aturn 9.56 5 10.0 U ranus 19.29 6 19.6 N eptune 30.27 7 38.8 Pluto 39.68 8 77.2 Properties of planetary system s • planets suffer no close encounters and are spaced fairly n regularly (Bode’s law : an=0.4 + 0.3×2 ) planet semimajor axis (A U ) n an (A U ) Mercury+ 0.39 −∞ 0.4 V enus 0.72 0 0.7 Earth 1.00 1 1.0 *predicted -
Planets of the Solar System
Chapter Planets of the 27 Solar System Chapter OutlineOutline 1 ● Formation of the Solar System The Nebular Hypothesis Formation of the Planets Formation of Solid Earth Formation of Earth’s Atmosphere Formation of Earth’s Oceans 2 ● Models of the Solar System Early Models Kepler’s Laws Newton’s Explanation of Kepler’s Laws 3 ● The Inner Planets Mercury Venus Earth Mars 4 ● The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects Beyond Neptune Why It Matters Exoplanets UnderstandingU d t di theth formationf ti and the characteristics of our solar system and its planets can help scientists plan missions to study planets and solar systems around other stars in the universe. 746 Chapter 27 hhq10sena_psscho.inddq10sena_psscho.indd 774646 PDF 88/15/08/15/08 88:43:46:43:46 AAMM Inquiry Lab Planetary Distances 20 min Turn to Appendix E and find the table entitled Question to Get You Started “Solar System Data.” Use the data from the How would the distance of a planet from the sun “semimajor axis” row of planetary distances to affect the time it takes for the planet to complete devise an appropriate scale to model the distances one orbit? between planets. Then find an indoor or outdoor space that will accommodate the farthest distance. Mark some index cards with the name of each planet, use a measuring tape to measure the distances according to your scale, and place each index card at its correct location. 747 hhq10sena_psscho.inddq10sena_psscho.indd 774747 22/26/09/26/09 111:42:301:42:30 AAMM These reading tools will help you learn the material in this chapter. -
How the Universe Works an Attempt at Dealing with the Big Questions of Science and Philosophy in Light of 21’St Century Knowledge
How the Universe Works An attempt at dealing with the big questions of science and philosophy in light of 21’st century knowledge. By Theodore A. Holden Copyright © 2015 Theodore A. Holden. All rights reserved. Other than as permitted under the Fair Use section of the United States copyright act of 1976, no part of this publication shall be reproduced or distributed in any form or by any means, or stored in a database or retrieval system without the prior written permission of the authors. Quoting of this work must be attributed to this book, and not in a manner which would indicate any sort of endorsement. No derivative works are permitted without express permission of the author. Reproduction of artwork contained in this book must be properly attributed to this book. Information, discussion, related links at: http://www.cosmosincollision.com/. ISBN # 978-0-9891787-3-0 Version 5/2/15 Contents Forward: Part I, Ancient Realities and Some Background Chapter 1. Gravity in prehistoric times. Animal and Human Sizes of Past Ages The Weightlifter and the Witch How Much Attenuation of Gravity was Needed to Account for Dinosaur Sizes? Sauropod Necks and the Problem of Torque Ancient Flying Creatures Ancient Humans and their Sizes Antediluvian Lifespans Chapter 2. The Fermi Paradox and the Realities of Interstellar Distances Chapter 3. Telepathy and Pre-Flood Language The Evidence for Telepathy in Today’s World Telepathy in the Ancient World Talking to the Animals… Chapter 4. The Mars Images Cities and villages Walls and fitted stones Mechanical junk and debris (A few samples) Gateways to Subterranean areas. -
Meteorites and the Origin of the Solar System
Meteorites and the origin of the solar system STEPHEN G. BRUSH University of Maryland, College Park, MD 20742, USA (e-mail: [email protected]) Abstract: During the past two centuries, theories of the origin of the solar system have been strongly influenced by observations and theories about meteorites. I review this history up to about 1985. During the 19th century the hypothesis that planets formed by accretion of small solid particles ('the meteoritic hypothesis') competed with the alternative 'nebular hypothesis' of Laplace, based on condensation from a hot gas. At the beginning of the 20th century Chamberlin and Moulton revived the meteoritic hypothesis as the 'planetesimal hypothesis' and joined it to the assumption that the solar system evolved from the encounter of the Sun with a passing star. Later, the encounter hypothesis was rejected and the planetesimal hypothesis was incorporated into new versions of the nebular hypothesis. In the 1950s, meteorites provided essential data for the establishment by Patterson and others of the pre- sently accepted 4500 Ma age of the Earth and the solar system. Analysis of the Allende meteorite, which fell in 1969, inspired the 'supernova trigger' theory of the origin of the solar system, and furnished useful constraints on theories of planetary formation developed by Urey, Ringwood, Anders and others. Many of these theories assumed condensation from a homogeneous hot gas, an assumption that was challenged by astrophysical calculations. The meteoritic-planetesimal theory of planet formation was developed in Russia by Schmidt and later by Safronov. Wetherill, in the United States, established it as the preferred theory for formation of terrestrial planets. -
Saturday in the Park One for the Ladies?
SUNDAY, OCTOBER 2, 2011 732-747-8060 $ TDN Home Page Click Here SATURDAY IN THE PARK ONE FOR THE LADIES? Yesterday=s card at Belmont Park was dubbed as With Sarafina (Fr) (Refuse To Bend {Ire}), Galikova ASuper Saturday,@ and it sure lived up to the billing (Fr) (Galileo {Ire}), Snow Fairy (Ire) (Intikhab) and despite wet conditions. Last Danedream (Ger) (Lomitas {GB}) in the line-up, today=s year=s champion juvenile renewal of the G1 Qatar Prix de l=Arc de Triomphe could Uncle Mo (Indian Charlie) be all about the females. Few have managed to overhaul proved to be one of the the colts in this feature, but the strengthening and brightest stars on the day, upgrading of Europe=s distaff program may be bringing a getting back on track against return to the era of Allez France, Ivanjica, Three Troikas older horses with a sharp (Fr), Detroit (Fr), Gold River (Fr), Akiyda (GB) and All three-length win over Along (Fr), who all triumphed here from 1974-1983. Jackson Bend (Hear No Evil) Sarafina represents the powerful axis of His Highness in the GII Kelso H. The The Aga Khan and Alain de Royer-Dupre, who Uncle Mo Repole Stable colorbearer has masterminded the success of the best filly in Adam Coglianese his sights set on the generations Zarkava (Ire) (Zamindar) here in 2008, and GI Breeders= Cup Classic some may suggest she is unlucky not to have already next. Fox Hill Farm=s Havre de Grace (Saint Liam) captured Europe=s feature. Hampered before rallying into apparently has plenty left in the tank after defeating the third behind Workforce (GB) (King=s Best) 12 months boys in the GI Woodward S. -
Allowed Planetary Orbits
RELATIONSHIPS OF PARAMETERS OF PLANETARY ORBITS IN SOLAR---TYPE-TYPE SYSTEMS FACULTY OF SCIENCE, PALACKÝ UNIVERSITY, OLOMOUC RELATIONSHIPS OF PARAMETERS OF PLANETARY ORBITS IN SOLAR-TYPE SYSTEMS DOCTORAL THESIS PAVEL PINTR OLOMOUC 2013 VYJÁD ŘENÍ O PODÍLNICTVÍ Prohlašuji, že všichni auto ři se podíleli stejným dílem na níže uvedených článcích: Pintr P., Pe řinová V.: The Solar System from the quantization viewpoint. Acta Universitatis Palackianae, Physica, 42 - 43 , 2003 - 2004, 195 - 209. Pe řinová V., Lukš A., Pintr P.: Distribution of distances in the Solar System. Chaos, Solitons and Fractals 34 , 2007, 669 - 676. Pintr P., Pe řinová V., Lukš A.: Allowed planetary orbits. Chaos, Solitons and Fractals 36 , 2008, 1273 - 1282. Pe řinová V., Lukš A., Pintr P.: Regularities in systems of planets and moons. In: Solar System: Structure, Formation and Exploration . Editor: Matteo de Rossi, Nova Science Publishers, USA (2012), pp. 153-199. ISBN: 978-1-62100-057-0. Pintr P.: Závislost fotometrických parametr ů hv ězd na orbitálních parametrech exoplanet. Jemná Mechanika a Optika 11 - 12 , 2012, 317 - 319. Pintr P., Pe řinová V., Lukš A.: Areal velocities of planets and their comparison. In : Quantization and Discretization at Large Scales . Editors: Smarandache F., Christianto V., Pintr P., ZIP Publishing, Ohio, USA (2012), pp. 15 - 26. ISBN: 9781599732275. Pintr P., Pe řinová V., Lukš A., Pathak A.: Statistical and regression analyses of detected extrasolar systems. Planetary and Space Science 75 , 2013, 37 - 45. Pintr P., Pe řinová V., Lukš A., Pathak A.: Exoplanet habitability for stellar spectral classes F, G, K and M. 2013, v p říprav ě. -
Intensity Frontier
Intensity Frontier 38th International Conference on High Energy Physics DOE-PI Meeting Session • Sheraton Grand Chicago August 5, 2016 Alan L. Stone Office of High Energy Physics Office of Science, U.S. Department of Energy Chicago, IL – ICHEP – Intensity Frontier PI Meeting Outline • HEP Overview • Budget • LBNF/DUNE • Intensity Frontier Overview • Comparative Review • Early Career • Workforce Development • Last Word • Q&A Aug 5, 2016 Chicago, IL – ICHEP – Intensity Frontier PI Meeting 2 The High Energy Physics Program Mission …is to understand how the universe works at its most fundamental level: • Discover the most elementary constituents of matter and energy • Probe the interactions between them • Explore the basic nature of space and time Office of High Energy Physics (HEP) fulfills its mission by: • Building projects that enable discovery science • Operating facilities that provide the capability to perform discovery science • Supporting a balanced research program that produces discovery science Our program is formally advised by: • High Energy Physics Advisory Panel (HEPAP) – Jointly chartered by DOE and NSF to advise both agencies • Astronomy and Astrophysics Advisory Committee (AAAC) 0 – Advises DOE, NASA, and NSF on selected issues in astronomy & astrophysics of mutual interest and concern • National Academy of Sciences (NAS) – Established by Congress in 1863 to advise the government and any department thereof on the arts and sciences Aug 5, 2016 Chicago, IL – ICHEP – Intensity Frontier PI Meeting 3 The Next Big Discovery in -
Formation and Evolution of Planetary Systems
Specialist Topics in Astrophysics: Lecture 2 Formation and Evolution of Planetary Systems Ken Rice ([email protected]) FormationFormation ofof PlanetaryPlanetary SystemsSystems Lecture 2: Main topics • Solar System characteristics • Origin of the Solar System • Building the planets Most theories of planet formation have been carried out in the context of explaining our Solar System • Any theory must first explain the data/observables OriginOrigin ofof ourour SolarSolar SystemSystem To have a successful theory we must explain the following: • Planets revolve in mostly circular orbits in same direction as the Sun spins OriginOrigin ofof ourour SolarSolar SystemSystem • Planetary orbits nearly lie in a single plane (except Pluto [no longer a planet!!] and Mercury), close to the Sun’s equator • Planets are well spaced, and their orbits do not cross or come close to crossing (except Neptune/Pluto) OriginOrigin ofof ourour SolarSolar SystemSystem • All planets (probably) formed at roughly the same time • Meteorites suggest inner portions of the Solar System were heated to ~1500 K during meteorite/planet formation period OriginOrigin ofof ourour SolarSolar SystemSystem • Planet composition varies in a systematic way throughout the Solar System Terrestrial planets are rocky Outer planets are gaseous OriginOrigin ofof ourour SolarSolar SystemSystem • Jupiter/Saturn are dominated by H and He; Neptune/ Uranus have much less H and He (mainly ices, methane, carbon dioxide and ammonia) OriginOrigin ofof OurOur SolarSolar SystemSystem • Planetary satellites -
The List: All Primetime Series on Television Calendar Year 2015
The List: All Primetime Series on Television Calendar Year 2015 Source: Nielsen, Live+7 data provided by FX Networks Research. 12/29/14-12/27/15. Original telecasts only. Excludes repeats, specials, movies, news, sports, programs with only one telecast, and Spanish language nets. Cable: Mon-Sun, 8-11P. Broadcast: Mon-Sat, 8-11P; Sun 7-11P. "<<" denotes below Nielsen minimum reporting standards based on P2+ Total U.S. Rating to the tenth (0.0). Important to Note: This list utilizes the TV Guide listing service to denote original telecasts (and exclude repeats and specials), and also line-items original series by the internal coding/titling provided to Nielsen by each network. Thus, if a network creates different "line items" to denote different seasons or different day/time periods of the same series within the calendar year, both entries are listed separately. The following provides examples of separate line items that we counted as one show: %(7 V%HLQJ0DU\-DQH%(,1*0$5<-$1(6DQG%(,1*0$5<-$1(6 1%& V7KH9RLFH92,&(DQG92,&(78( 1%& V7KH&DUPLFKDHO6KRZ&$50,&+$(/6+2:3DQG&$50,&+$(/6+2: Again, this is a function of how each network chooses to manage their schedule. Hence, we reference this as a list as opposed to a ranker. Based on our estimated manual count, the number of unique series are: 2015³1,415 primetime series (1,524 line items listed in the file). 2014³1,517 primetime series (1,729 line items). The List: All Primetime Series on Television Calendar Year 2015 Source: Nielsen, Live+7 data provided by FX Networks Research. -
Here Non-Majors Can Undertake Focused Reading, Discussion, and Writing, Delving Deeply Into Some of the Most Exhilarating Mysteries of Our Universe
Cover image Reprinted by permission. ScienceCartoonsPlus.com. www.kendallhunt.com Send all inquiries to: 4050 Westmark Drive Dubuque, IA 52004-1840 Copyright © 2013 by David Toback ISBN 978-1-4652-2578-8 Kendall Hunt Publishing Company has the exclusive rights to reproduce this work, to prepare derivative works from this work, to publicly distribute this work, to publicly perform this work and to publicly display this work. All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopy- ing, recording, or otherwise, without the prior written permission of the copyright owner. Printed in the United States of America 10 9 8 7 6 5 4 3 2 1 Contents Foreword ........................................................................................................... v Preface ............................................................................................................. vii Instructor Notes ............................................................................................. xiii Suggested Reading ..........................................................................................xvi UNIT 1: Introduction: Big and Small Stuff .................................................... 1 Chapter 1: Introduction ........................................................................... 3 Chapter 2: Going Big .............................................................................. 7 Chapter 3: Going Small........................................................................