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Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

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Page 1: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Seeing the Invisible

Prof. Lynn CominskySonoma State University

Director, Education and Public Outreach

Page 2: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Sources of light

• Which of these things are sources of light?

• If things are not emitting light, how do you see them?

Page 3: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Seeing the light

• Do you know of any type of light that is not visible to your eyes?

• Are people sources of light?

Page 4: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Have you ever seen the invisible?

Page 5: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

How do you detect light?

• What are common light detectors for– Visible light?– Infrared light?– X-ray light?

Page 6: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

• Radio transmission towers• TV transmission towers

• Cold objects• Planets• Collapsed stars• Radio galaxies• Intergalactic matter

Radio

Page 7: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

• microwave generator in ovens

• warm molecular clouds• Planets• Galaxies• The Universe!

Microwave

Page 8: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

• warm objects • People• Ovens

• Planets• “Normal” stars• Protostars• Galaxies

Infrared

Page 9: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

• hot objects (thousands of degrees)• Sun• Lightbulbs

• Planets• “Normal” stars, sun-like and hotter• Galaxies

Visible

Page 10: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

• hotter objects (10,000 to about 100,000 Kelvin)• UV lights (“black lights”)

• Nebulae• Aurorae• Hot stars• Galaxies

Ultraviolet

Page 11: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

• very hot objects (millions of degrees)• X-ray generators

• Solar corona• Pulsars• Black holes• Galaxy clusters

X-rays

Page 12: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Electronic light detectors

• Solid state devices that detect individual light particles (“photons”)

Digital dental x-ray

Do you know of any others?

Page 13: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

What you can see from the Earth

VLA WMAP Spitzer FUSE Chandra Fermi

Page 14: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Why study the extreme Universe?

• Universe as seen by eye is peaceful

Page 15: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

The Fermi mission…• First space-based collaboration

between astrophysics and particle physics communities

• International partners from France, Germany, Italy, Japan & Sweden

• Launched June 11, 2008• Expected duration 5-10 years

Page 16: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Before launch

• Large Area Telescope

• Gamma-ray

Burst Monitor

Page 17: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Large Area Telescope (LAT)• PI Peter Michelson (Stanford)• International Collaboration: USA NASA

and DoE, France, Italy, Japan, Sweden

• LAT is a 4 x 4 array of towers

• Each tower is a pair conversion telescope with calorimeter

Page 18: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Pair-conversion

• Anti-matter partners of e- are positrons (e+)

• When they meet, they annihilate each other!

E = mc2

m = mass of the electron or positron

E = energy of gamma ray

Page 19: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Now in reverse….

This process is called “pair conversion” as the incoming gamma-ray converts into an electron/positron pair

tungsten

Page 20: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

How does the LAT work?

• Anticoincidence Detectors – screen out charged particles

• Tungsten converts gamma rays into e+ e- pairs

• Calorimeter measures total energy

Page 21: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Launched!

• June 11, 2008

• Delta II Heavy (9 solid rocket boosters)

• Mass is 4300 kg

• 555 km circular orbit

• 1500 W total power

• 40 Mb/sec downlink

Page 22: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

What the sky looks like in gamma rays

Page 23: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

What types of things emit gamma rays?

• Really big lightning storms• Our Sun when it flares• Our Milky Way galaxy – charged particles

hitting gas between the stars• Huge explosions of stars that are dying (some

make collapsed stars)• Collapsed stars sending out jets of charged

particles• Black holes sending out jets of charged

particles

Page 24: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Gamma-ray bursts on the sky

• About 4-5 bursts per week

Page 25: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Typical strong GRB seen by GBM

• Each burst has as much energy as our Sun puts out in its entire lifetime

Page 26: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Gamma-ray Jets from Black Holes• Jets flare

dramatically in gamma rays

• Galaxies that point their jets at us are called “blazars”

• How do the black holes send out jets?

Art by Aurore Simonnet

Page 27: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Gamma rays from pulsars

• Collapsed stars – size of San Francisco, mass of our Sun

• Sending out beams of particles like lighthouses

Page 28: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

What is the Universe made of?

• Matter – what we experience in our everyday lives

• Dark matter – you can’t see it but you can feel it

• Dark Energy – a mysterious force that is tearing the Universe apart

Page 29: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach
Page 30: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Searching for dark matter

• Dark matter makes up 80% of the matter in the Universe

• The leading particle candidate for dark matter is a “WIMP” =weakly interacting massive particle

• Fermi could see gamma rays from WIMPS annihilating with each other

• More gamma rays are expected near the center of our Galaxy

Page 31: Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach

Many places to look!

All-sky map of simulated gamma ray signal from DM annihilation (Baltz

2006)

Satellite Galaxies

Galactic Center

Milky Way Halo

Spectral Lines Extra-galactic

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No detections so far, but the search continues…