Wilkinson Microwave Anisotropy Probe

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Wilkinson Microwave Wilkinson Microwave Anisotropy Probe Anisotropy Probe AST 403 Jimmy Jones WMAP: WMAP:

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WMAP:. Wilkinson Microwave Anisotropy Probe. AST 403 Jimmy Jones. WMAP:. Cosmic Microwave Background Radiation (CMB). CMB. Big Bang predicts early universe was very hot – photons produced As universe expands, the gas within cools and photons lose energy - PowerPoint PPT Presentation

Transcript of Wilkinson Microwave Anisotropy Probe

Page 1: Wilkinson Microwave Anisotropy Probe

Wilkinson Microwave Wilkinson Microwave Anisotropy ProbeAnisotropy Probe

AST 403Jimmy Jones

WMAP:WMAP:

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WMAP:WMAP:

Cosmic Cosmic Microwave Microwave Background Background Radiation Radiation

(CMB)(CMB)

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CMBCMB• Big Bang predicts

early universe was very hot – photons produced

• As universe expands, the gas within cools and photons lose energy

• Implies universe should be filled with radiation left over from Big Bang - CMB

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CMB DiscoveryCMB Discovery

• Initially predicted by George Gamow in 1948 and by Ralph Alpher and Robert Herman in 1950

• Inadvertently observed by Arno Penzias and Robert Wilson in 1965

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COBECOBE• Cosmic Background

Explorer• Launched November

1989• Designed to measure

cosmic background radiation

• Possessed three instruments:– DIRBE – infrared– DMR – microwave– FIRAS – spectrum

analysis

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COBE DataCOBE Data

• COBE helped to determine average temperature of CMB as 2.725 kelvins

• This temperature is very uniform

• However, COBE was able to detect slight variations

Red areas .0002 degrees Red areas .0002 degrees warmer than black areaswarmer than black areas

Milky WayMilky Way

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Why Study CMBs?Why Study CMBs?• CMBs provide

information on the universe as early as 400,000 years after Big Bang

• (as opposed to studying visible light sources in the million year range)

• Studying fluctuations can provide insight into origin of galaxies and measure the basic parameters of the Big Bang theory.

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How?How?

• The Big Bang can account for background radiation and the formation of light elements but not galaxies

• One theory is:– Large objects potentially grew out of small

fluctuations in the background radiation– Areas of greater density expand slower

allowing for build up of even greater densities

– Further study of these anomalies can help to prove the validity of this theory

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WMAPWMAP

Microwave Microwave Anisotropy Probe:Anisotropy Probe:

The MissionThe Mission

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Satellite TimelineSatellite Timeline

• Launched June 30, 2001

• Completed prime 2 years of mission operations September 2003

• Extensions granted to September 2009

• Orbits in L2 with back to Sun and Earth

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Satellite ComponentsSatellite Components

• Uses differential microwave radiometers that measure temperature differences between two points on the sky.

• To facilitate rejection of foreground signals from our own Galaxy, WMAP uses five separate frequency bands from 22 to 90 GHz.

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Measurement Error Measurement Error ControlControl

• Sensitivity better than 20 microkelvins per 0.3 degree square pixel

• Measures temp. differences rather than absolute temp (implies most spurious signals will cancel)

• Spins and precesses like a top allowing an observing pattern that covers 30% of sky during each 1 hour precession.

• Five frequency bands (as compared to COBE’s three)

• The L2 Lagrange point offers exceptionally stable environment and unobstructed view of deep space.

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Data AcquisitionData Acquisition

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WMAPWMAP

DataData

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Universes’ ‘Baby Universes’ ‘Baby Picture’Picture’

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Universes’ FingerprintUniverses’ Fingerprint

• Universes’ baby picture provides unique ‘fingerprint’ that can be analyzed to determine characteristics of the universe, past and present

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Composition of Composition of UniverseUniverse

• Although the data is still be analyzed a wealth of information has already been discovered

• Based on analysis a composition of the primordial universe has been proposed

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How?How?

• WMAP measured temperature fluctuations in term of their ‘angular fluctuation spectrum’.

• Graphing this data produced features generated by the various physical processes that produce different amounts of energy (temperature) at the different angular scales.

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How IIHow II

Variations due to Variations due to gravity?gravity?

Dark Matter?Dark Matter?

Variations due to Variations due to sound waves? sound waves?

Atoms?Atoms?

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Shape of the UniverseShape of the Universe• The vertical peaks and

angular scale in the previous graph provide information to the density as well

• If the density is greater than the critical density a closed universe is produced

• If the density is less than the critical density an open universe is produced

• If the density is equal to the critical density a flat universe is produce

• Findings of the WMAP mission appear consistent with a flat universe geometry

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Rapid Inflation Rapid Inflation

• Measures of the fluctuations on the angular scale seem to support the theory that the universe underwent a period of extremely rapid (exponential) expansion

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More DataMore Data

• The universe is 13.7 billion ± 200 million years old

• The Hubble constant is 70 (km/sec)/Mpc, +2.4/-3.2

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ReferencesReferences

• General Information– http://map.gsfc.nasa.gov/m_mm.html– http://en.wikipedia.org/wiki/WMAP

• CMB– http://www.astro.ubc.ca/people/scott/faq_basic.html

Missions

• Results– http://www.cnn.com/2003/TECH/space/02/11/cosmic.p

ortrait/

• COBE– http://lambda.gsfc.nasa.gov/product/cobe/