The NASA-funded Origins Program
a comprehensive effort to study the
origins of galaxies, stars, planets, and even life itself. Such engrossing
questions can best be answered through studies conducted at infrared
wavelength
and at high spatial resolution. As NASA's center of excellence for infrared
and sub-millimeter astrophysics, and as the institutional home for the Spitzer
Science Center and the Michelson Science Center, IPAC eagerly anticipates
an exciting future.
The Spitzer Science Center (SSC) at IPAC provides development and
operations support for NASA's last Great Observatory, which was launched
in August 2003. The SSC is responsible for soliciting and reviewing Spitzer research
proposals, and in selecting and scheduling observations aboard the
observatory. It also provides scientific and technical support for scientists
planning observations, and will process Spitzer data for archiving and
dissemination to the broader scientific community.
The European successor to the Infrared Space Observatory will be the
Herschel Space Observatory (nee FIRST), scheduled for launch in 2008. IPAC
will
again serve as the lead US-based science support center for the European Space
Agency's fourth Cornerstone Mission. A second payload will be launched with
Herschel. The
Planck mission will study the cosmic microwave
background radiation and conduct an all-sky sub-millimeter survey. IPAC will
serve as the lead US science support center and will process the
sub-millimeter
data.
When the Galaxy Evolution Explorer (GALEX) was launched in 2003, IPAC
began processing the ultraviolet data from this NASA
Small Explorer
program.
As NASA astronomers continue to become increasingly adept at designing and
utilizing ground-based telescope arrays, they will also begin planning and
developing space-borne facilities. The
Michelson Science Center
(MSC) at
IPAC, in association with the Jet Propulsion Laboratory, will provide the
needed scientific and technical support for the
SIM PlanetQuest
(SIM) and the
Terrestrial Planet Finder
(TPF) missions.
In addition to these missions and programs, IPAC will continue its development
and maintenance of rich databases of long-wavelength astronomical data, along
with the associated development of useful analysis tools. IPAC-based
databases, including the
NASA/IPAC Infrared Science Archive (IRSA) and the
NASA/IPAC Extragalactic Database
(NED), will continue to expand
their
contents, sophistication, and general utility for both the professional
astronomer and the general public alike.
For the foreseeable future, IPAC will continue to provide NASA and the nation
with unparalleled capabilities and expertise in support of long-wavelength
astrophysics and of astronomical studies conducted with interferometers.