Title: Goddard Space Flight Center All Hands Presentation
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2New Budget Initiatives for NASA in FY04
3Aerosols provide the largest uncertainty in the
determination of the Climate Forcing Function
FY04 Presidents budget calls for accelerated
development and launch of an advanced
polarimeter to increase our understanding of
black carbon soot and other aerosols as causes of
climate change .
- Science objectives of the CCRI APS (CAPS)
- Determine the global distribution of natural and
anthropogenic aerosols with accuracy and coverage
sufficient for a reliable quantification of the
aerosol effect on climate. - Measurement approach
- Retrieval of aerosol particle microphysical
properties by inverting radiance and polarization
measurements. - The CAPS polarimeter weighs approximately 25 kg
and uses approximately 25 watts of power, while
being 10 times more accurate than present
instruments.
4Building Blocks Enable New Capabilities
- Using laser light instead of radio waveswill
dramatically increase our ability to transmit
information across the solar system - First demonstration from Mars
- Earth-based terminals
- Space or airborne or ground
- 24/7 coverage
5WHAT POWERED THE BIG BANG?
WHAT HAPPENSAT THE EDGEOF A BLACK HOLE?
WHAT ISDARK ENERGY?
http//universe.nasa.gov
National Aeronautics andSpace Administration
6Completing Einsteins Legacy
Beyond Einstein will employ a series of missions
linked by powerful new technologies and common
science goals to answer these questions and
launch the revolution of the 21st century!
- Einstein Great Observatories providing
breakthrough increases in capabilities to address
all Beyond Einstein science - LISA Gravitational waves from merging black
holes and the early Universe - Constellation-X Spectroscopy close to the event
horizon of black holes and place constraints on
dark side of the Universe - Einstein Probes to address focused science
objectives - Determine the nature of the Dark Energy
- Search for the signature of inflation in the
microwave background - Take a census of Black Holes of all sizes in the
local Universe - A technology program, theoretical studies and an
education program to inspire future generations
of scientists and engineers towards the vision - Directly detect the gravitational waves emitted
during the Big Bang - Image and resolve the event horizon of a Black
Hole
7Beyond Einstein
- Constellation-X will use X-ray spectroscopy to
observe - Black holes
- Probe close to the event horizon
- Evolution with redshift
- Dark side of the Universe
- Clusters of galaxies and large-scale structure
- Production and recycling of the elements
- Supernovae and interstellar medium
- 25-100 times sensitivity gain for high resolution
spectroscopy in the 0.25 to 10 keV band - Four satellites at L2 operating as one with
advanced X-ray spectrometers - Enable high resolution spectroscopy of faint
X-ray sources
- LISA uses a laser based Michelson interferometer
to monitor the separation between proof masses in
separate spacecraft - Three spacecraft separated by 5 million km
- Each spacecraft includes two freely falling test
masses with drag free operation - Distance changes measured with precision of 4
ppm RMS over 100 seconds
8To Inspire the Next Generation of
ExplorersEducation Initiative
- Educator Astronaut Program
- fully qualified members of NASAs Astronaut Corps
who have expertise in K-12 education. - Educator Astronauts will lead the Agency in the
development of new ways to connect space
exploration with the classroom - more information, applications, or submit a
teacher, go to http//edspace.nasa.gov - Explorer Schools
- 50 Middle Schools 5 per Center to be selected
- Commit to 3-year MOU improve math and
scienceinstruction in low performing / urban
schools - 6-member teams from each school / 6-day training
session during the summer - Pipeline Building A Pathway to NASA-related
Careers - engage Public and Parents as well as teachers and
students - emphasis on Informal (museums, science centers)
as well as Formal education community - increased partnerships with Dept. of Education on
No Child Left Behind initiatives