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Goddard's
John Mather A Wise Guy
Dr. John
Mather, Senior Astrophysicist in the Infrared Astrophysics Branch,
was appointed as a Co-Investigator for the proposed Wide-field Infrared
Survey Explorer (WISE) mission.
Mather is also
Senior Project Scientist for the James Webb Space Telescope (JWST),
an infrared telescope that will be the largest ever in space, and
will explore the deep space frontier beyond what the Hubble Space
Telescope can observe. He feels perfectly suited to his new role
as a WISE Co-Investigator because the two missions will complement
each other.
"WISE will
survey the entire infrared sky with unprecedented sensitivity, finding
many new and interesting objects for a closer look by JWST,"
said Mather. He was the Project Scientist for Goddard's Cosmic Background
Explorer (COBE), which at the time provided the most detailed map
of the infrared afterglow from the Big Bang, and has extensive experience
observing celestial objects that emit infrared light, which is invisible
to the human eye but detectable by special instruments.
"I'll share
technical information where appropriate; for example, I'm making
sure the WISE team is aware of the detector technology developed
for JWST, so they can take advantage of our advances," said
Mather.
If approved
and it proceeds on schedule, WISE could be launched near the end
of 2007 for a planned six-month mission. (JWST is expected to launch
in 2010.) Once in orbit, WISE will make an all-sky infrared survey
up to 1,000 times more sensitive than previous surveys.
In addition
to picking targets for JWST, WISE is expected to find the brightest
galaxies in the universe, which are often cloaked behind veils of
dust. Since these galaxies emit as much as 100 times more infrared
light than visible light, and since infrared light can pass through
dust without being scattered as much as visible light, WISE can
reveal them.
WISE could also
find the closest stars to the Sun; faint, tiny objects called "Brown
Dwarfs". They are also known as failed stars, since they are
not massive enough to shine by nuclear fusion in their core, like
typical stars. Instead, they glow mostly in infrared with the heat
left over from their formation. These low mass stars are expected
to be more numerous than the more massive stars like red dwarfs,
and thus there should be brown dwarf stars closer to the Solar system
than Proxima Centauri, the closest known ordinary star.
Asteroid hunting
will also be in WISE's job description. Asteroids are usually detected
optically, but the typical asteroid is quite dark and usually absorbs
ten times more solar radiation than it reflects. The absorbed power
goes into heating the asteroid, and this heat is then radiated away
as infrared radiation. As a result, WISE will be able to detect
asteroids a million times fainter than Ceres, the largest asteroid.
These faint, small asteroids are not well catalogued, so WISE will
provide a vast database of new astrometric and radiometric information
on previously unknown asteroids.
Mather also
anticipates surprises, "It's likely WISE will discover things
we don't know anything about. WISE is much more sensitive than any
previous infrared survey -- a tremendous advance. From experience
with Hubble and COBE, I have faith that surprises will be found
when you have equipment that's way better than anything else."
WISE is an Explorer-class
mission, but it is still too early in the planning stages (extended
Phase A) to determine Goddard's role completely. Dr. Edward Wright
of the University of California, Los Angeles, will be the WISE Principal
Investigator. NASA's Jet Propulsion Laboratory, Pasadena, Calif.,
will manage the project, and contractors will provide the spacecraft
and instruments.
For more about
WISE, refer to: http://www.astro.ucla.edu/~wright/WISE/
For more about
John Mather, refer to: http://www.jwst.nasa.gov/Bios/ProgJMather.htm
For more about
JWST, refer to: http://jwst.gsfc.nasa.gov/
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