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November
10, 2003
The National Press Club
Remarks by Secretary of Energy Spencer Abraham
Thank you all for coming.
And thanks to the National Press Club for hosting
this event.
I’d like to welcome the directors of the
Department of Energy’s national laboratories
and the chairs of our science advisory boards
who are with us today.
They play an important role advancing science
at the Department of Energy, and I want to thank
them for their many important contributions.
I would also like to welcome Al Trivelpiece,
who led the Department’s science effort
under President Reagan.
Introduction
Ask the average American to describe the mission
of the Department of Energy and you are more
likely to hear about oil wells and gas prices
than you are about science.
That’s not surprising.
The Department of Energy makes news when oil
and gas prices spike.
But the Department of Energy makes history every
day because we sustain the enterprise of science
– the original, innovative, and risk-taking
basic research that defines our mission and
our tradition.
Most Americans don’t know that the Department
of Energy operates a network of national laboratories
where research has led to profound breakthroughs
in medicine, environmental science, biology,
and physics that have transformed – and
continue to transform – the way we all
live.
These Department of Energy labs are a national
treasure.
They are centers of scientific discovery –
as witnessed by the number of Nobel Prizes and
other honors they have produced – including
the most recent Nobel Prize in Physics that
was awarded to Alexei Abrikosov of the Argonne
National Laboratory near Chicago.
Dr. Abrikosov and his fellow researchers won
the Nobel Prize for their research into superconductivity
– a technology that will help make tomorrow’s
electric power systems more reliable and efficient.
He joins Dr. Leon Lederman, who is with us today,
as one of the 70 Nobel Prize winners who have
been funded by the Department.
Their work is just a small example of the research
being conducted by the Department of Energy
that is helping to shape the future …
research that requires sophisticated facilities
… long range planning … and …
of course … the world’s most talented
scientific minds … from universities,
industry, and the laboratories themselves.
But if we are to continue that kind of success
we need to look to the future. So I am here
today to release a 20-year roadmap for future
scientific facilities. These facilities and
upgrades to our current inventory will revolutionize
science … and society. They are needed
to extend the frontiers of science, to purse
opportunities of enormous importance, and to
maintain U.S. science primacy in the world.
Leading this effort at the Department of Energy
is the Office of Science.
Our Office of Science funding request for fiscal
year 2004 is more than $3.3 billion, and it
will fund basic research for national and energy
security, and to advance our knowledge and understanding
of the physical sciences and areas of biological,
environmental, and computational sciences.
Throughout its history, the Department of Energy
has designed, constructed, and operated many
of the world’s most advanced large-scale
research and development facilities. The facilities
are shared with the global science community
and contain technologies and instruments found
nowhere else on earth. Some 18,000 researchers
from universities, other agencies, private industry,
and foreign nations use our facilities every
year.
We are the single largest supporter of basic
research in the physical sciences, accounting
for approximately 40 percent of all federal
funds in this area over the past decade.
This research is conducted at our national laboratories
and at approximately 250 universities nationwide.
I’ve often said that the Department of
Energy could just as well be named the Department
of Energy and Science, given our world-class
research facilities and the pivotal role we
have played in supporting both basic research
and technology development.
Just consider a thin slice of our legacy.
We are the heirs to the work of Enrico Fermi
and Leo Szillard, who created the first controlled,
continuous source of nuclear energy –
and, before them, to the discoveries of Niels
Bohr and others who described the atom as a
nucleus with orbiting electrons, rather than
a solid mass.
We are the heirs to the wizardry of Robert Oppenheimer,
Edward Teller, and many others who shaped the
course of World War II and gave us a nuclear
deterrent that helped prevent global conflict
during the Cold War.
We are the heirs to the engineering and scientific
gifts of E.O. Lawrence who designed the first
machine -- his cyclotron -- to break down atomic
nuclei to understand the fundamental workings
of the atom.
And we are the heirs to the speculative genius
of Albert Einstein, whose intuition and imagination
have allowed us to describe and understand the
universe in new and important ways.
Because of our concern for and work on the effects
of radiation on human health, the Department
of Energy built on the discovery of the basic
chemistry of life by Watson and Crick and launched
the Human Genome Project in 1985.
This is a proud legacy … and the tradition
of funding world-class scientific research continues
today with the construction of the Spallation
Neutron Source that will, when completed in
less than three years, provide the world’s
most intense supply of neutrons for scientists
to study and engineer materials.
Today, our investments in nanoscience –
the science of very small things – are
making the Department of Energy a leader in
a global scientific effort that will give us
the ability to build new and better materials
from the molecular level.
It was science like this that brought us discoveries
like Kevlar, silicon chips, and flat-screen
TVs.
Imagine an aircraft wing that repairs itself
or an automobile frame twice the strength and
half the weight of current models.
Nanoscience could lead to tremendous energy
savings, vastly more efficient solar cells,
engines the size of atoms working everywhere,
including within our own bodies, and artificial
retinas that can help the blind to see.
The Department of Energy is home to some of
the world’s fastest computers, and they
are getting faster every day.
Today we measure computers in teraflops, or
the ability to perform trillions of operations
in a second.
Our supercomputer at Lawrence Livermore lab
has a peak performance of 12 teraflops.
That means it is capable of 12 million-million
operations in one second, something that would
take your handheld calculator 342,000 years
to accomplish.
There is no real way to measure the competitive
advantage this kind of computing power can give
us.
At each stage along the process of discovery,
America’s economy grows stronger, with
new tools to improve human health, generate
new industries, improve our everyday lives,
or boost efficiency – the things that
help give our nation its competitive edge.
And we need science to maintain that competitive
edge – especially in high technology,
which every day becomes more central to our
economy.
But the competitive advantage that comes to
us through America’s scientific enterprise
goes well beyond that.
If we build the required facilities and equipment,
and support the large laboratories that accelerate
discovery, America is assured of remaining the
world’s center of scientific research
for many years to come.
This is where the world will want to come to
explore the future.
This is where the world will want to come to
do science.
Facilities for the Future of Science
If we want to remain the focal point of scientific
discovery, we must look to the future.
And that is why I am here today.
Today, I am pleased to announce the Department
of Energy’s 20-year plan for building
the scientific research facilities of the future.
It is our plan to keep the United States at
the scientific frontier.
Nothing of this scope has ever been attempted
by our Department, or indeed by any other science
agency in government.
We are not only planning two decades out, but
we are prioritizing our facility needs across
all fields of science supported by the Department
of Energy.
In the 21st Century, the health and vitality
of U.S. science and technology will depend upon
the availability of the most advanced research
facilities.
Not only because science today is so complex,
but because science now requires that chemists,
physics, biologists … that all fields
of science … work together. The facilities
we propose today will bring the sciences under
one roof and give researchers the tools they
need to work their wonders.
Let me discuss the way we made our decisions
and give you some flavor of the enormous benefits
we see flowing from these new projects.
The process we followed was transparent and
interdisciplinary.
The Associate Directors of our six science divisions
– Basic Energy Sciences, Fusion Energy
Sciences, High Energy Physics, Nuclear Physics,
Advanced Scientific Computating, and Biological
and Environmental Sciences – were asked
to list in rank order the major facilities necessary
to maintain world scientific leadership in their
programs over the next 20 years.
Some 46 facilities were identified in this process.
This list was then submitted to the respective
programs’ Advisory Committees, which are
composed of top scientists from universities,
industry, and our laboratories.
We asked these committees to analyze the scientific
importance of each proposed facility and to
add or subtract as they saw fit.
The appetite for new facilities grew, and a
total of 53 new projects were recommended.
Then came the hard part.
The Director of our Office of Science, Raymond
Orbach, reviewed these proposals, ordered them
across disciplines, and recommended 28 be considered
for funding over a 20-year planning horizon.
This may appear unilateral, but the selection
was informed by the best minds in all the affected
fields.
And, frankly, the alternative of decision by
committee was not acceptable, because committees
… despite their best efforts … are
notorious for delivering compromise documents
that too often settle on the lowest common denominator.
This effort has been endorsed by the directors
of our science laboratories, who understand
the importance of modern facilities for future
scientific discovery.
In addition, the Task Force on the Future of
Science at the Department of Energy, which was
established at my direction and is chaired by
Dr. Charles Vest, President of MIT, has praised
this effort in its recent report.
It is gratifying that this effort has received
support from those who understand the enterprise
of science best.
This list of facilities is driven by science
and the Department of Energy mission, nothing
else.
Our criteria were straightforward: Which facilities
are most important for Department of Energy
science over the next two decades, taking into
account whether the prospects for construction
were in the near, mid, or far-term?
Clearly, this document has implications for
the budget. But it is not a budget document.
It will be up to Congress and the Administration
to determine how much to spend on science and
on new scientific facilities and to balance
them against other national priorities.
Once that decision is made, however, we owe
it to the American taxpayers to demonstrate
that we have thoroughly evaluated what sequence
of investment we believe best for the science
we do at DOE.
Let me stress one point here.
We believe this list of 28 facilities outlines
to an important extent the future of science
in America – and indeed the world.
These facilities cover the critical areas where
discoveries can transform our energy future,
boost economic productivity, transform our understanding
of biology, and provide revolutionary new tools
to deal with disease.
They can make major and necessary contributions
to national security – and give us the
ability to understand matter at its most fundamental
level.
They can also do something else. They can surprise
us.
The unexpected benefits of work on at these
research facilities will lead us in directions
we cannot even imagine.
And we are looking down the road far enough
to the time when facilities that are now under
construction, such as the Spallation Neutron
Source, will need enhancements.
That is the purpose of this list – to
look into the future and to be prepared.
And as with all our existing facilities, any
new projects we undertake will benefit a wide
spectrum of scientists … and will profit
from close cooperation with other agencies.
So, let me now profile some of our top priorities
… a set of facilities that not only represent
tremendous opportunities, but demonstrate the
breath of the science encompassed by the Department.
The full list of facilities, with descriptions
of the benefits each may deliver and how they
are grouped in a near, mid and long-term time
frame, is contained in the booklet we have made
available today. I urge you to review it to
understand the full scope of this effort.
First on our list is fusion. The prospect of
a limitless source of clean energy for the world
leads with our commitment to join the international
fusion energy experiment known as ITER.
This is a Presidential priority with enormous
potential. Successful negotiations among the
international partners will lead to the first-ever
fusion science experiment capable of producing
a self-sustaining fusion reaction.
If we reach agreement, ITER will be our top
facility.
Next on the list is our desire to regain global
leadership in areas of supercomputing that many
believe we have lost. Japan’s new Earth
Simulator machine is a remarkable achievement.
It has the computing power of the 20 fastest
U.S. computers – combined.
The Japanese are to be congratulated for launching
a new era in scientific computing, but the U.S.
must be part of this era.
We can create new computer architectures that
can boost computing power by 100 times over
current machines.
Such an achievement will give scientists the
ability to simulate complex reactions as never
before – and give industry the ability
to virtually prototype everything from new aircraft
engines, to super-efficient auto bodies, thus
saving hundreds of millions of dollars.
Scientific computation deserves the kind of
serious attention we believe our facilities
list gives it.
We will also look at advancing our lead in light
sources.
The Linac Coherent Light Source would provide
x-ray brightness that is 10 billion times greater
than current light sources.
That would allow researchers, for the first
time, to create real-time images of chemical
reactions at the atomic scale, leading us to
far greater understanding of how our bodies
work – indeed, how virtually all materials
are put together.
As I already mentioned, the Department of Energy
launched the human genome project nearly 20
years ago in our effort to understand how radiation
affects cells at the most fundamental level.
The Protein Production and Tags Facility can
help us build on these discoveries and make
a huge contribution to our Genomes to Life Program.
We are now taking the insights from that project
to create microbes that do everything from making
hydrogen, to sequestering carbon dioxide, to
accelerating environmental clean up.
The Protein Production and Tags Facility will
join the Molecular Machines Facility to help
create a facility to mass-produce tens of thousands
of proteins a year, code them by their DNA,
and make them available to researchers around
the country.
Using current methods, it is virtually impossible
for us to understand the thousands of proteins
that make up the microbes we want to put to
work for our energy mission. But these facilities,
together, will speed this process dramatically,
and give energy and medical science powerful
new tools.
The Rare Isotope Accelerator can help us understand
how everything from the cosmos to heavy elements
were formed.
It would allow our scientists to learn how the
chemical elements that make up the world around
us were developed, help us develop new nuclear
medicine techniques, and improve our ability
to model the explosions of nuclear weapons.
This project would be a major addition to the
Department’s nuclear physics program and
make a major contribution to stockpile stewardship.
The Joint Dark Energy Mission, a space-based
probe to be developed with NASA, will help us
understand one of the greatest mysteries in
science today – why the universe is expanding
at an accelerating rate.
By placing a new wide-angle telescope in space,
researchers will be able to see farther back
in the evolution of the universe to help unravel
this strange thing called dark energy …
a force that is apparently working against gravity
to speed up the expansion of the universe.
As we look out into this expanding universe,
we are also thinking of how best to understand
the materials that make up our day-to-day world.
A new generation of electron microscope can
help us study how atoms combine to form materials,
and how materials respond to external factors
such as electric fields.
This new instrument, the Transmission Electron
Achromatic Microscope or TEAM, will help us
design lighter, more efficient materials for
everything from automobiles to advanced fuel
cells.
In addition to launching new projects such as
these, we are also planning important upgrades
to existing facilities.
Improvements to our energy sciences computer
network – what we call E. S. Net –
which links researchers around the country to
our laboratories and research facilities, will
allow us to accommodate the huge demand for
this network.
E.S. Net puts the power and capability for our
investment in light sources and accelerators
literally at the researcher’s desktop.
To keep up with the demand, and the technology
that improves virtually by the day, we need
to upgrade our network.
And upgrades to facilities, such as the Continuous
Electron Beam Accelerator, would essentially
create new facilities by applying advanced technology
to our current stock of powerful research machines.
The upgrade to this accelerator, located at
Thomas Jefferson Lab, will double its power
and apply advanced computing power to help us
explain the properties of one of the strangest
particles yet discovered – the Quark.
From the very large, with new pictures of how
our universe evolved, to the very small, with
insights into the structure of the nucleus,
the facilities we are proposing will secure
American pre-eminence in science for the better
part of the 21st Century.
Conclusion
What I have discussed today is just a snapshot
of the detailed roadmap we have drawn for our
major science projects over the next two decades.
We recognize that, from time to time, this prioritized
list should be re-examined in light of discoveries
in science that may offer new opportunities
we cannot imagine today.
But that should not be done casually.
The American taxpayers deserve to see how we
would invest their money over the next 20 years.
More than that, the public deserves to know
what our priorities will be over that time period.
They need to see that decisions of this magnitude
are made after serious thought, and that their
government can commit to long-range planning.
We believe this list of 28 science facilities
fulfills that responsibility.
Indeed, we think it is the cornerstone for the
future of critical fields of science in America.
Now, I can’t tell precisely how or when
the projects and research I’ve discussed
today might uncover deep mysteries of science
or deliver immediate practical benefits.
But that’s the beauty of science.
It can have so many unexpected outcomes.
But even if we knew our search for Dark Energy
or our particle physics research would have
no direct impact on our every day lives, we
still would want to go forward.
We would want to go forward, because we want
to know why the universe and our planet act
the way they do.
We do basic research to understand.
And many times that’s justification enough.
But we also want to go forward because that
is what a great nation does.
It explores.
It attempts to know and to understand.
Some people have told me it would be hard to
explain why the Department of Energy’s
basic scientific research is so important. I
haven’t found that to be the case. Everyone
understands that investments in science produce
benefits for our lives.
And I think everyone is curious. Discoveries
like Dark Energy lead to deeper mysteries that,
themselves, compel us to continue our search
-- even when we know the search is not in any
normal sense practical.
To be sure, no one knows what field of science,
or what potential new science machine, will
produce the next big discovery.
But we can be certain of one thing. There will
be a big discovery. A solitary genius, or a
group of scientists from a half dozen fields
working together, will take some step, apply
some test, seek some insight, that will inevitably
lead beyond their expectations to a result as
unexpected as it is wonderful.
All we are doing is giving them the tools …
and the freedom … to work these mysteries
out.
And we don’t insist on results on some
time scale … basic research doesn’t
work that way.
We expect only that science will employ the
traditions of inquiry and curiosity that extend
in a straight line from today’s Nobel
Prize winner directly back to Aristotle.
I believe the blueprint we have presented today
will allow that tradition to grow and prosper.
And it will provide the foundation for the next
generation of scientists to work their wonders.
Thank you.
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