Cosmic Microwave Background The 2006 Nobel Prizes.

Slides:



Advertisements
Similar presentations
Cosmology How did our universe form?. The study of the universe – its nature, origin and its evolution.
Advertisements

Astrophysics from Space Lecture 7: Infrared astronomy Prof. Dr. M. Baes (UGent) Prof. Dr. C. Waelkens (KUL) Academic year
10.1 EXPLAINING THE EARLY UNIVERSE SCIENCE 9 BLOCK C LIZ PEREJILO.
The Nobel prize in Physics 2006: Cosmology becomes precision science Hans Kristian Eriksen Institute of Theoretical Astrophysics Onsala, June 2012.
The Universe By Noah Gray Science 9. Mr. Horton Feb 20 th 2015.
Evidence to support the.... But first, what’s a scientific theory? The term “theory” in science has a different meaning than in our everyday language.
3K background radiation by Roman Werpachowski and Peter Holrick.
The Mathematics of General Relativity, Black holes, and Cosmology Chad A. Middleton Brown Bag Seminar Mesa State College February 12, 2010.
The Evidence for the Big Bang Student Resource Sheet 5 Science and Religion in Schools: Unit 4a.
Objectives Distinguish the different models of the universe.
11/25/03Prof. Lynn Cominsky1 Class web site: Office: Darwin 329A (707) Best way to reach me:
April 1, 2003Lynn Cominsky - Cosmology A3501 Professor Lynn Cominsky Department of Physics and Astronomy Offices: Darwin 329A and NASA EPO (707)
Announcements Homework 13 due Wednesday Projects due Friday No office hour tomorrow (Tuesday) at 10 am; I will be available after 1 pm.
Parvaneh, Shelby & Marleena Microwave Telescopes Visit For 100’s of free powerpoints.
Recent advances in physics and astronomy --- our current understanding of the Universe Lecture 4: Big Bang, the origin of the Universe April 23 th, 2003.
Recent advances in physics and astronomy --- our current understanding of the Universe Lecture 4: Big Bang, the origin of the Universe April 23 th, 2003.
The Nobel prize in Physics 2006 piet mulders VU October 4, 2006
Lecture 1: Basics of dark energy Shinji Tsujikawa (Tokyo University of Science) ``Welcome to the dark side of the world.”
Cosmology Physics CSG Day at Southampton University 5/6/7 13.7Gyr ABB Steve King.
The Big Bang: Fact or Fiction? The Big Bang Fact or fiction? Dr Cormac O’Raifeartaigh.
From the Big Bang to the Nobel Prize: Cosmic Background Explorer (COBE) and Beyond Goddard Space Flight Center Lecture John Mather Nov. 21, 2006.
Evidence to Support the Theory
Olbers paradox Why is the sky dark at night? Of course, the Sun’s gone down! But more careful consideration of this simple fact led early astronomers to.
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.
By: Andrew Cheung Teacher: Mr. Horton
ASTR Fall Semester Joel E. Tohline, Alumni Professor Office: 247 Nicholson Hall [Slides from Lecture23]
P olarized R adiation I maging and S pectroscopy M ission Probing cosmic structures and radiation with the ultimate polarimetric spectro-imaging of the.
PHY306 1 Modern cosmology 4: The cosmic microwave background Expectations Experiments: from COBE to Planck  COBE  ground-based experiments  WMAP  Planck.
THE BIG BANG THEORY A video on the Big Bang theory click here.
By: Tony Strazzara.  Why might our universe be finite?  medieval philosophers gave the first logical arguments supporting a finite universe  during.
Cosmology, Inflation & Compact Extra Dimensions Chad A. Middleton Mesa State College March 1, 2007 Keith Andrew and Brett Bolen, Western Kentucky University.
Chapter IV Science and Technology. I. Federal Government’s Policy and Support 1.Federal investment in science and technology has played a critical role.
MAPping the Universe ►Introduction: the birth of a new cosmology ►The cosmic microwave background ►Measuring the CMB ►Results from WMAP ►The future of.
How the Universe got its Spots Edmund Bertschinger MIT Department of Physics.
A new view of the Universe VI Fred Watson April 2005.
Whisper of Creation By Dr. Harold Williams of Montgomery College Planetarium
April 17, 2001Lynn Cominsky - Cosmology A3501 Answer to last week’s Question How do we know that the Milky Way is at the outer edge of the Virgo cluster?
The measurement of q 0 If objects are observed at large distances of known brightness (standard candles), we can measure the amount of deceleration since.
Big Bang Theory. Cosmology Study of deep space and the dynamics of universe other galaxies stars (nebula, supernova…) origin of the universe black holes.
Cosmic Microwave Background Carlo Baccigalupi, SISSA CMB lectures at TRR33, see the complete program at darkuniverse.uni-hd.de/view/Main/WinterSchoolLecture5.
The theory of the universe. Expanding of our universe In the 1920s, astronomers had the technology to see more Celestial bodies with advance telescope.
The Cosmic Microwave Background Based partly on slides Joe Mohr ( University of Chicago)
Galaxies and Cosmology / Types of Galaxies Spiral –Including Barred Spiral Elliptical Irregular.
Planck Report on the status of the mission Carlo Baccigalupi, SISSA.
Salient Features of the Universe Homogeneity and isotropy for 6000 Mpc > x > 100 Mpc Universe expanding uniformly ordinary matter is more abundant than.
Cosmology -- the Origin and Structure of the Universe Cosmological Principle – the Universe appears the same from all directions. There is no preferred.
Cosmic Background Explorer: COBE
The Universe Through Time: The Big Bang. The Universe Through Time: The Curvature of Space.
Cosmology : a short introduction Mathieu Langer Institut d’Astrophysique Spatiale Université Paris-Sud XI Orsay, France Egyptian School on High Energy.
Wilkinson Microwave Anisotropy Probe (WMAP) By Susan Creager April 20, 2006.
CMB physics Zong-Kuan Guo 《现代宇宙学》
Cosmic Microwave Background
Unmanned Space Probes.
The Science of Creation
Planck mission All information and images in these slides can be found browsing through
Wilkinson Microwave Anisotropy Probe
The Cosmic Microwave Background and the WMAP satellite results
The Science of Creation
Main Evidence for the Big Bang
Cosmology.
The Formation of the.
Evidence for the Big Bang Theory
Big Bang.
SMP: Active Galactic Nuclei Supeluminal Motions etc.
of Montgomery College Planetarium
Whisper of Creation with Psalm 19
of Montgomery College Planetarium
Evidence for the Big Bang Theory
Presentation transcript:

Cosmic Microwave Background The 2006 Nobel Prizes

This year’s laureates  John C. Mather, Senior Astrophysicist at NASA’s Goddard Space Flight Center, MD  George F. Smoot, Professor of Physics at the University of California, Berkeley  “For their discovery of the basic form of the cosmic microwave background radiation as well as its small variations in different directions. The very detailed observations that the Laureates have carried out from the COBE satellite have played a major role in the development of modern cosmology into a precise science.”

Memoirs  J. C. Mather and J. Boslough, “The Very First Light,” 1996  G. Smoot and K. Davidson, “Wrinkles in Time,” 1993

Outline  Introduction  The cosmic microwave background  The COBE project  Further work – The Wilkinson Microwave Asymmetry Probe  A quick survey of modern cosmology  The origin of microwave anisotropies  Interpretation of data  The concordant picture

COBE Instrumentation  Differential Microwave Radiometer (DMR) – Maps variations in the CMB  Far-InfraRed Absolute Spectrophotometer (FIRAS) – Measures the spectrum of the CMB  Diffuse InfraRed Background Experiment (DIRBE) – Maps dust emission

2.73 degrees Not with a whimper

Composition of the Universe

Yes!