Wilkinson Microwave Anisotropy Probe (WMAP) Timeline June 30, 2001: launched aboard a Delta II-7425-10 launch vehicle October 1, 2001: arrival at L2 April.

Slides:



Advertisements
Similar presentations
Chapter 18: Cosmology For a humorous approach to quarks, check out the Jefferson Lab’s game.  In Looking for the Top Quark, each player receives six quarks.
Advertisements

The complete history of the Universe (abridged) The Big Bang and the Cosmic Microwave Background (With thanks to Angela Taylor)Sutton Trust Summer School.
Planck 2013 results, implications for cosmology
UNIVERSE CHAPTER BIG BANG The big bang theory is the main cosmological model for the earliest known time of the Universe. It shows us how the universe.
Origin & Evolution of the Universe
LECTURE 25, DECEMBER 2, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Thursday, April 8 th Agenda  Finish Section 18.1: The Universe  Origin of the universe, red shift, big bang theory  In-Class Assignments Section 18.1.
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.
“PLANET AND GALAXY WE LIVE…” Presentation M. Filonenko K. Tusov School 1173, Form 9E GUIDANCE – Markova S.A.
Titel The Oldest Memory: The Echo of the Big Bang.
Objectives Distinguish the different models of the universe.
WMAP. The Wilkinson Microwave Anisotropy Probe was designed to measure the CMB. –Launched in 2001 –Ended 2010 Microwave antenna includes five frequency.
Observing the Cosmic Microwave Background 1. Penzias and Wilson with their Horn Antenna. Penzias and Wilson were astronomers, from Bell Labs, who built.
The Birth Of Our Universe The Big Bang And Inflation
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.
J. Goodman – May 2003 Quarknet Symposium May 2003 Neutrinos, Dark Matter and the Cosmological Constant The Dark Side of the Universe Jordan Goodman University.
© 2010 Pearson Education, Inc. Chapter 23 The Beginning of Time.
X What is the shape of our universe? By Sandro Berndt.
Evidence to Support the Theory
The Big Bang Theory By James L. Barker. Big Bang Theory Today the Big Bang Theory is the dominant scientific theory about the origin of the universe.
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.
Cosmology. Some important questions Did the universe have a beginning or has it always existed? Will the universe end? If it ends, what will happen at.
Modern Physics: Part 2. ALL Galaxies have redshifts – farther from us greater redshifts! Many other scientists made observations similar to Slipher’s.
Lecture 11: The Big Bang. Galaxies: islands of stars making up the universe.
© 2010 Pearson Education, Inc. Chapter 23 The Beginning of Time.
MAPping the Universe ►Introduction: the birth of a new cosmology ►The cosmic microwave background ►Measuring the CMB ►Results from WMAP ►The future of.
PHY306 1 Modern cosmology 4: The cosmic microwave background Expectations Experiments: from COBE to Planck  COBE  ground-based experiments  WMAP  Planck.
How the Universe got its Spots Edmund Bertschinger MIT Department of Physics.
Hubble’s galaxy classes Spheroid Dominates Disk Dominates.
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.
The theory of the universe. Expanding of our universe In the 1920s, astronomers had the technology to see more Celestial bodies with advance telescope.
OUR UNIVERSE : AN EXPANDING MYSTERY Supratik Pal Indian Statistical Institute, Kolkata.
The Big Bang Theory Not this one…. The Theory The Big Bang describes how: – a massive explosion created the universe – the cooling and expansion of.
Chapter 18: Chapter 18: Cosmology. WHAT DO YOU THINK? What does the universe encompass? Is the universe expanding, fixed in size, or contracting? Will.
Formation of the Universe The Big Bang Theory. The Big Bang All matter & energy in the universe was compressed into a tiny volume 13.7 billion years ago,
Cosmology (Chapter 14) NASA. Student Learning Objectives Describe the Big Bang theory Analyze possible fates of our universe.
Salient Features of the Universe Homogeneity and isotropy for 6000 Mpc > x > 100 Mpc Universe expanding uniformly ordinary matter is more abundant than.
The Planck Satellite Matthew Trimble 10/1/12. Useful Physics Observing at a redshift = looking at light from a very distant object that was emitted a.
The Planck Mission: Looking into the Past to Learn about Our Future Courtney Nickle, Stephanie Clark and Taylor Phillips Astronomy, Spring 2011 Abstract.
WMAP The Wilkinson Microwave Anisotropy Probe Universe.
The Universe Through Time: The Big Bang. The Universe Through Time: The Curvature of Space.
The Expanding Universe  When light or sound moves toward or away from an observer, its frequency/wavelength changes (Known as Doppler effect)  Can be.
Jim Sullivan.  Scientist: Dr. Chris Jillings, SNOLAB.
#23 Big Bang Theory The expanding universe and a quick galaxy review.
THE BIG BANG THEORY. HOW IT ALL BEGAN Scientists hypothesize that approximately 13.7 billion years ago, a rapid expansion created the universe, producing.
Wilkinson Microwave Anisotropy Probe (WMAP) By Susan Creager April 20, 2006.
CMB physics Zong-Kuan Guo 《现代宇宙学》
Harrison B. Prosper Florida State University YSP
Chapter 23 The Beginning of Time
Evidence for The Big Bang
Astrophysics II: Cosmology
Origin of the Universe.
Wilkinson Microwave Anisotropy Probe
The Cosmic Microwave Background and the WMAP satellite results
The expanding universe and a quick galaxy review
Cosmology: SNC 1D.
The Universe.
The Formation of the.
Evidence for the Big Bang Theory
Big Bang.
of Montgomery College Planetarium
The Big Bang Theory.
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
Formation of the Universe
Evidence for the Big Bang Theory
Hubbles Law.
CMB Anisotropy 이준호 류주영 박시헌.
What observed feature of the universe motivated scientists to propose the “Big Bang” theory? There is lots of debris in space, as would be expected from.
Presentation transcript:

Wilkinson Microwave Anisotropy Probe (WMAP) Timeline June 30, 2001: launched aboard a Delta II launch vehicle October 1, 2001: arrival at L2 April 2002: completed first full sky scan October 2002: completed second full sky scan February 2003: first data released April 2003: third full sky scan due to be completed …

Wilkinson Microwave Anisotropy Probe (WMAP) Instrumentation Radiometer: Differential pseudo-correlation with polarization Optics: Dual Gregorian, 1.4 m x 1.6 m primary reflectors Thermal: Passive radiative cooling to < 95 kelvins Frequencies (GHz): 22, 30, 40, 60, 90 Angular Resolution: 0.25 o – 0.93 o Sensitivity: ~ 35 x K per 0.3 o square pixel

Wilkinson Microwave Anisotropy Probe (WMAP) Mission Results to Date Age of Universe: 13.7 billion years +/- 1% margin of error First stars ignited: 200 million years after Big Bang Content of the Universe: 4% atoms, 23% Cold Dark Matter, 73% Dark Energy Geometry of the Universe: flat Expansion Rate (Hubble Constant) Value: H 0 = 71 km/s/Mpc +/- 5% Inflation: New evidence (from polarized signal) to support theory Fate of the Universe: it will expand forever