Lecture Description
10/14/2009
Fermi-LAT Observing the Universe With High-Energy Gamma-Ray Eyes
Dr. Stefan Funk, Assistant Professor, Department of Physics, Stanford University
The Fermi Gamma-ray Space Telescope, formerly called GLAST, is a satellite mission designed to measure gamma-rays in the energy range 20 MeV to >300 GeV, with supporting measurements for gamma-ray bursts from 8 keV to 30 MeV. In addition to breakthrough capabilities in energy coverage and localization, the very large field of view enables observations of 20% of the sky at any instant, and the entire sky on a timescale of a few hours. With its recent launch on 11 June 2008, Fermi now opens a new and important window on a wide variety of phenomena, including pulsars, black holes and active galactic nuclei, gamma-ray bursts, the origin of cosmic rays and supernova remnants, and searches for hypothetical new phenomena such as supersymmetric dark matter annihilations. Dr. Funk will discuss early results and science opportunities of investigations of the Universe with high-energy eyes.
- Slides
Course Index
- David Morrison: Mission to a Potentially Threatening Asteroid
- Laura T. Iraci: Laboratory Studies of Water Ice Cloud formation under Martian Conditions
- Jeffrey Van Cleve: The Race to Detect the First Earth-sized Planet
- Ron Greeley: Surface modifications by winds on Earth, Mars, Venus, and Titan
- JoAnne Hewett: The Hunt for Hidden Dimensions
- Franck Marchis: Multiple Asteroid Systems: New Techniques to Study New Worlds
- Interstellar and Early Solar System Organics in Samples from Comet Wild 2
- Ross A. Beyer: Google Earth, now with Mars!
- Jeffrey Scargle: Tools for Probing the Universe
- Richard Muller: Discovery of Strong Cycles in Fossil Diversity
- Rachel Mastrapa: Weathering on Icy Satellites: Probing the Near Surface Using Infrared Spectroscopy
- John McCarthy: Convergent evolution of our own and extra-terrestrial intelligence
- Jasper Halekas: The Dynamic Lunar Environment
- Tom Abel: First Things in the Universe
- Julie Chittenden: Experimental determination of the effect of salts, regolith, and wind
- Philip Russell: Aerosol particle roles in climate change
- Edwin Kite: True Polar Wander and Climate on Late Hesperian/Amazonian Mars
- Robert Landis: NEOs Ho!! The Asteroid Option
- Terry Fong: Field Testing of Utility Robots for Lunar Surface Operations
- Mikhail Kreslavsky: Geological record of recent climate change on Mars
- Amos Nur: Apocolypse: Earthquakes, Archeology and the the Wrath of God
- Robert Lillis: Death of the Martian Dynamo
- Brian Jeffs: Progress in phased array feed development for radio astronomy
- Ray Kurzweil: The Implications of the Law of Accelerating Returns for the Search for ETI
- The impact and recovery of asteroid 2008 TC3
- Dr. Beth Ann Hockey: How to Speak to Your Computer
- Janice Bishop: The Surface of Mars
- John Balboni: How do You Qualify Heat Shields on Earth?
- Kevin Zahnle: Earth After the Moon-forming Impact
- Dave Brain: Atmospheric Escape and Aurora on Mars
- Michael Carr: Mars - The Water Story and Prospects for Life
- Risa Wechsler: Connecting Galaxies, Halos, and Star Formation Rates Across Cosmic Time
- Natalie Batalha: Kepler's First Peek
- Darlene Lim: Pavilion Lake - Diving Deep to Get Us to the Moon and Mars
- Paul Kalas: HST Imaging of Fomalhaut
- Reid Parsons: Where is Mars' Ice?
- Markus Aschwanden: Solar Flares and Coronal Mass Ejections Observed with STEREO
- Nathan Bramall: Detecting Organics Using Fluorescence Spectroscopy
- Dr. Stefan Funk: Fermi-LAT Observing the Universe With High-Energy Gamma-Ray Eyes
- Special Panel: LCROSS Mission - The First Results of the Impact
- Elmar Fuchs: The Inner Structure of a Floating Water Bridge
- Ben Zuckerman: The Search for Intelligent Life in the Universe - Some Great Challenges for SETI
- David Hollenbach: Water, Molecular Oxygen and Ice in Star-Forming Molecular Clouds
- Linda Spilker: The Rings of Saturn as seen by Cassini CIRS
- Claudio Maccone: Deep Space Flight and Communications
- Lauren Wye: Titan's Ontario Lacus
- Steven S. Vogt: Finding Planets Around Nearby Stars
- Gerry Harp: Exploring Alternative SETI Search Algorithms with the ATA
Course Description
The colloquiums are free and open to the public, and run from noon to 1 pm on Wednesdays at the SETI Institute, 515 N. Whisman Road, Mountain View, California.