350 likes | 523 Views
The UW Observational Cosmology Laboratory. A Brief Tour. Our Focus. The Cosmic Microwave Background (as viewed by WMAP). What is the CMB?. …A remnant from the BIG BANG. Discovery of the CMB. Robert Wilson and Arno Penzias, 1964. The CMB and the Early Universe.
E N D
The UWObservational Cosmology Laboratory A Brief Tour
Our Focus The Cosmic Microwave Background (as viewed by WMAP)
What is the CMB? …A remnant from the BIG BANG
Discovery of the CMB Robert Wilson and Arno Penzias, 1964
The CMB and the Early Universe The CMB provides clues as how the Universe expanded, or inflated to its current size
The CMB and the Early Universe The CMB also provides clues about the composition of the universe…
The Structure of the Universe Early perturbations in the density of matter later give rise to the formation of galaxies…
CMB Detection • Ground-Based Experiments • Wilson & Penzias • COMPASS http://cmb.physics.wisc.edu/compass.html • POLAR http://cmb.physics.wisc.edu/polar/ • Balloons • MSAM/TopHat http://topweb.gsfc.nasa.gov/ • Satellites • COBE http://lambda.gsfc.nasa.gov/product/ • WMAP http://map.gsfc.nasa.gov/m_mm/ms_status.html
CMB Detection:Satellites • COBE • WMAP
WMAP Over Many Frequencies K-Band
WMAP Over Many Frequencies Ka-Band
WMAP Over Many Frequencies Q-Band
WMAP Over Many Frequencies V-Band
WMAP Over Many Frequencies W-Band • 75-110 GHz • CMB peaks in this band
Wisconsin Experiments Missions: • Compass • POLAR • MBI MBI Instrumentation • Beam Mapping • Device Design • Mount & Pointing Structure • Phase Shifters • SQUIDS
Our Fearless Leader Professor Peter Timbie