Scientific Colloquium
June 13, 2014
MICHAEL
WERNER
JET PROPULSION
LABORATORY/CALIFORNIA INSTITUTE OF TECHNOLOGY
"10 Years of Infrared
Exploration with the Spitzer Space Telescope"
In March of 2004, within a few
months of the start of the scientific mission of the Spitzer
Space Telescope, I talked here at GSFC about the scientific
results that were only just starting to emerge from NASA’s Great
Observatory for infrared exploration of the Universe. Ten years
later, we are awash in Spitzer data, and exciting new results
continue to pour in from the observatory, which has now
completed about a quarter of a revolution around the sun as seen
from Earth. In this talk, I will summarize the latest scientific
results from the Spitzer warm mission, which started in mid-2009
and relies totally on the 3.6 and 4.5um arrays of the IRAC
camera built here at GSFC. I will highlight results on
exoplanets and on the early Universe, two of the prime areas of
study from Spitzer in recent years. In addition, I will present
results from a selection of the many investigations which
Spitzer has carried out in other scientific areas, including
results of particular interest from the cryogenic mission.
About the Speaker:
Dr. Michael Werner is the Project Scientist for the Spitzer
Space Telescope and also the Chief Scientist for Astronomy and
Physics at the Jet Propulsion Laboratory, California Institute
of Technology. He has been an active researcher in infrared
astronomy for over 35 years, studying star formation, the
interstellar medium and the central regions of our Galaxy. He
has served as Spitzer Project Scientist since 1984 and was one
of the leaders of the evolution of Spitzer from a
shuttle-attached payload into the elegant free-flying
observatory now operating successfully in an Earth-trailing
solar orbit. Werner was named the 2006 George Darwin lecturer by
the Royal Astronomical Society in recognition of the success of
Spitzer and is also the recipient of two NASA Outstanding
Leadership medals. He graduated from Haverford College in 1963
with a B.A. in physics and received a PhD in Astronomy from
Cornell University in 1968.
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