Jupiter Polar Orbiter (Juno)
Juno will fly to Jupiter and orbit its polar regions in order to understand the planet's gross size and structural properties, as well as measure Jupiter's atmospheric composition, temperature and deep wind profiles.

Microwave Instrument for the Rosetta Orbiter (MIRO)
MIRO (Microwave Instrument for the Rosetta Orbiter) is a scientific instrument on the ROSETTA Spacecraft that will measure temperatures and abundances of asteroids and comets.

Mars Reconnaissance Orbiter (MRO)
NASA's Mars Reconnaissance Orbiter (MRO) launched in 2005 and is on a search for evidence that water persisted on the surface of Mars for a long period of time.

Vehicle Cabin Atmosphere Monitor (VCAM)
VCAM, made up of a gas chromatograph and a mass spectrometer, will monitor the air in the International Space Station for trace amounts of organic molecules.

InSAR Working Group
The role of an Interferometric Synthetic Aperture Radar observational capability spans a broad spectrum of end uses.

Spitzer Space Telescope (SST)
The Spitzer Space Telescope has unprecedented infrared sensitivity that will allow astronomers to study the most distant, coldese, and most dust-obscured objects and processes in the universe.

Physical Oceanography Data Archive (PO.DAAC)
The Physical Oceanography Distributed Active Archive Center is responsible for archiving and distributing data relevant to the physical state of the ocean.

Deep Space Network (DSN)
The NASA Deep Space Network is an international network of antennas that supports interplanetary spacecraft missions and radio and radar astronomy observations for the exploration of the solar system and the universe.

Terrestrial Planet Finder Interferometer (TPF-I)
The Terrestrial Planet Finder Interferometer (TPF-I) will search for habitable worlds around nearby stars and look for indicators of the presence of life. TPF-I works in the infrared wavelengths.

Terrestrial Planet Finder Coronagraph (TPF-C)
The Terrestrial Planet Finder Coronagraph (TPF-C) will search for habitable worlds around nearby stars and look for indicators of the presence of life. TPF-C works in the visible wavelengths.

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