Status Report

NASA FY 2003 Budget Background: Office of Space Science (Code S)

By SpaceRef Editor
February 4, 2002
Filed under , ,

Office of Space Science (Code S)

Associate Administrator: Dr. Edward Weiler

Public Affairs Contacts: Donald Savage, 202/358-1727

Dolores Beasley, 202/358-1753

The total Fiscal Year 2003 budget request for the Space Science Enterprise is
$3,414.3 million; this is comprised of $3,044.5 million in direct program funding
and $369.8 million for institutional support. This represents an increase of 19
percent from FY 2002. There are an estimated 1,572 direct Full Time Equivalent
employees included within the Space Science Enterprise in Fiscal Year 2003.

SPACE SCIENCE OVERVIEW

Thousands of years ago, on a small rocky planet orbiting a modest star in an
ordinary spiral galaxy, our remote ancestors looked up and wondered about their
place between Earth and sky. At the outset of the 21
st
century, we ask the same
profound questions:

  • How did the Universe begin and evolve?
  • How did we get here?
  • Where are we going?
  • Are we alone?

    Answers to these questions will not be extracted from narrow inquiries, but will be
    built up by combining innumerable individual clues over the years to come. The
    broad outlines of much of the puzzle are discernible now, but a clear picture of the
    whole awaits years of varied research that will undoubtedly produce many
    surprises along the way. In the last 40 years, space probes and space
    obser03 bries have played a central role in this fascinating process, and NASA’s
    Space Science Enterprise will continue to be at the forefront of the search for the
    answers to these major questions.

    A summary of Space Science highlights and discoveries during calendar year
    2001 is available on the Internet at:

    http://spacescience.nasa.gov/

    New Initiatives and Other Major Features in the 2003 Budget


    A new research program announced by NASA and the Department of Energy, the
    Nuclear Systems Initiative , paves the way for an unprecedented capability in the
    next decade and beyond, to explore the far reaches of the solar system in the
    search for answers to some of the greatest questions in human history.

    Safe and proven electrical generating technologies provided by radioisotope
    power systems will enable sophisticated mobile laboratories to travel over the
    surface of Mars, drilling deep underground at promising sites where signs of life can be sought, and conduct a large variety of other experiments day and night,
    around the clock.

    Other missions will be able to speed throughout the outer reaches of the solar
    system, at speeds as much as two times faster than is possible even with the most
    sophisticated space probes available today. Such speed, coupled with numerous
    powerful scientific instruments, will allow NASA to consider more ambitious
    possibilities involving missions that could travel from one interesting planet, moon
    or comet to another for a close-up, in-depth study. The fiscal year 2003 request for
    this Initiative is $46.5 million for nuclear electric propulsion and $79 million for
    nuclear electrical power-generation systems.

    The New Frontiers Program is a new planetary exploration program, structured
    and managed along the lines of NASA’s highly successful, Discovery program,
    under which missions are selected through open peer-reviewed competitions.
    Designed to allow frequent access to space for mid-size planetary missions that
    will perform high-quality science investigations, New Frontiers will take advantage
    of advances in propulsion and power systems in the nuclear initiative. Missions
    will be cost-capped at $650 million in fiscal 2003 dollars with a launch scheduled
    48 months from the start of development. $15 million is requested for fiscal 2003.

    There is no funding for the New Horizons Pluto-Kuiper Belt mission in fiscal 2003
    and subsequent years. However, preliminary design studies on New Horizons are
    continuing through fiscal 2002. Funding for the Europa Orbiter mission was
    deleted due to significant cost growth in the missionÕs life cycle.

    Major Ongoing Programs

    As of the end of December 2001, there are 26 operating Space Science missions, in
    addition to the Enterprise’s participation in seven foreign missions. By the end of 2003
    Space Science will have 28 operating missions, in addition to participation in eight
    foreign missions.


    • The Mars Exploration Program (MEP) is a sustained series of missions to
      Mars, each of which will provide long-term, focused scientific return. The
      primary objective is to characterize and understand Mars as a dynamic
      system, including its present and past environment, climate cycles, geology
      and whether life ever arose there. The strategy includes a natural
      responsiveness to scientific discoveries that will emerge as new observations
      are made. The fiscal 2003 budget features some alterations in the strategy for
      the missions that will be launched after 2005. The fiscal 2003 request for the
      Mars Exploration program is $453.6 million.

      • The 2001 Mars Odyssey orbiter, launched April 7, 2001, is now in its
        science orbit around Mars, having just recently completed its aerobraking
        maneuvers to achieve its final orbit.
      • The twin Mars Exploration Rovers are being prepared for launch in the
        summer of 2003, and will arrive at their landing sites on the surface of the
        Red Planet about seven months later. The mission of the MER rovers is to
        find conclusive evidence of water-affected materials on the surface. They
        are designed to effectively serve as robotic field geologists, and they will
        provide the first microscopic study of rocks and soils on Mars.
      • The 2005 Mars Reconnaissance Orbiter mission is now in the formulation
        stage. The MRO will use its new observational tools, some of which could
        resolve beach ball-sized objects and their mineralogies, to search for clues
        within the Martian landscape of telltale layers and materials associated
        with action of liquid water.
      • In 2007, NASA will launch a Mars Scout mission, which will be fully
        competed and competitively selected. In addition, NASA will provide
        programmatic and technical support to international Mars missions. These
        missions are the NASA-Italian Space Agency (ASI) telecommunications
        orbiter and the French Space AgencyÕs Orbiter including NetLanders.
      • The next major step will be NASA’s 2009 Mars Smart Lander (MSL)/Mobile
        Laboratory, a long-duration roving science lab intended to confirm the
        surface presence of water-related minerals and carbonates and their
        formational histories. The MSL will be a pathfinder to those sites that offer
        the highest probability of harboring Martian ÒfossilsÓ or other forms of
        indicators of past life. It will serve as both a scientific and technological
        pathfinder for future missions, including sample return. The 2009 Smart
        Lander/Mobile Laboratory will take advantage of the advances in nuclear
        power technology. By incorporating improved nuclear power systems,
        NASA can extend the operability of the rover from months to years, greatly
        increasing the scientific return of this mission.

    • NASAÕs currently operating Great Observatories — the Hubble Space
      Telescope and the Chandra X-ray Observatory — are on the forefront of
      astronomical research. Hubble is the first scientific mission of any kind that is
      specifically designed for routine servicing by spacewalking astronauts. In
      February 2002, NASA will launch the second part of the Third Servicing
      Mission (SM-3B) to the Hubble Space Telescope . During this mission,
      astronauts will replace the failed attitude control gyros, install a new science
      instrument — the Advanced Camera for Surveys, replace the flexible solar
      arrays, restore the near-infrared imaging instrumentÕs cooling capability, and
      undertake the complex and difficult replacement of the power control unit. The
      fiscal 2003 request for Hubble development is $138.9 million.
    • NASA’s next Great Observatory, the Space Infrared Telescope Facility, or
      SIRTF , will explore the nature of the cosmos through the unique windows
      available in the infrared portion of the electromagnetic spectrum. The launch of
      SIRTF has had to be delayed to afford time to resolve software and other

      technical problems. The July 2002 launch date has been delayed to no earlier
      than December 2002. The fiscal 2003 request is $47.4 million.

    • HESSI, the High Energy Solar Spectroscopic Imager , will study the dynamics
      of solar flares, the tremendous explosions in the atmosphere of the Sun.
      HESSI will be able to produce high-resolution spectrographic movies of solar
      flares, allowing scientists to study the life cycle of a flare. HESSI is scheduled
      for launch in February 2002.
    • Albert EinsteinÕs theory of general relativity is the most accepted theory of
      gravitation and the large-scale structure of the Universe. NASAÕs Gravity
      Probe B mission is designed to verify EinsteinÕs theory, which up to now has
      only been tested through astronomical observation and Earth-based
      experiments. Whether the experiment confirms or contradicts EinsteinÕs theory,
      its results will be of the highest scientific importance. The fiscal 2003 request of
      $19.7 million supports an October 2002 launch.
    • The Galaxy Evolution Explorer (GALEX), scheduled for launch in May 2002, is
      a Small Explorer mission that will map the global history and probe the causes
      of star formation over most of the life of the Universe. GALEX will investigate
      the period over which galaxies have evolved dramatically, and the time that
      most stars, elements and galaxy disks had their origins.
    • The Comet Nucleus Tour (Contour), scheduled for launch in July 2002, will fly
      past two comets and take images of the comets’ nuclei, as well as collect and
      analyze comet dust.
    • The Space Science Research Program develops the theoretical tools and
      laboratory data needed to analyze flight data, and supplies the resources for
      future mission needs and the analysis of data returned from operating
      spacecraft in hopes to answer the fundamental questions governing the role of
      the Space Science Enterprise. The fiscal 2003 request for this program is
      $709.6 million.

    Beginning in fiscal 2003, the budget for the Deep Space Network (DSN) is
    included in Space Science, consistent with Òfull costÓ budgeting and
    management. The transfer of management responsibility for the DSN to the Office
    of Space Science has already begun. NASAÕs Jet Propulsion Laboratory is
    working with its industry contract partners to transform the DSN and associated
    mission operations system architecture into a service-provision system known as
    the Deep Space Mission System (DSMS). The DSMS will provide a customer-oriented,
    turnkey service that seamlessly integrates the facilities of the DSN and
    the Advanced Multi-Mission Operations System (AMMOS). This system will
    enable more efficient provision of currently available services as well as the
    creation of new services. The fiscal 2003 request is $385.2 million.

    Programs Under Development or Study

    The Space Science Enterprise has a number of other programs under
    development, or under study for possible future development. More information
    on these programs can be found on the Internet at

    http://spacescience.nasa.gov/

  • SpaceRef staff editor.