| Mission |
Launch |
Target |
Science / IRTF Support |
 Galileo |
Oct 1989 |
Jupiter system, asteroids |
Jovian Atm (temporal evolution, global context)Probe entry
siteIo volcanismIo flux tube |
 Near |
Feb 1996 |
Asteroid |
Thermal vs. wavelength to model thermal inertia and T for
interpreting 0.9-2.4um spectra10um spectra for minerology |
 Mars Global Surveyor |
Nov 1996 |
Mars |
Mars Surface, interior |
 Cassini |
Oct 1997 |
Saturn System, asteroid, Titan |
Mid IR spectroscopy of Saturn - temporal global
coverageTitan wind observationsTitan temporal IR
spectroscopyIcy Sats: 1-5um reflectance to plan VIMSRings -
1-5um spectra, thermal inertia |
 Neat |
ongoing |
NEOs, comets, asteroids |
Immediate followup - 1-5um spectra surface
compSize, albedo, thermal inertia within 0.25 AU |
 Deep Space 1 |
Jul 1998 |
Comet |
Nucleus/ast size, albedo, rotation to plan imagingThermal
measurements to model dust environment prior to encounter |
 Mars Climate Orbiter |
Dec 1998 |
Mars |
monitor daily weather and atmospheric conditions
record changes on the martian surface from wind measure atmospheric
temperature profiles monitor atmospheric water vapor |
 Mars Polar Lander |
Jan 1999 |
Mars Polar Regions |
IR monitoring of dust (CO band) for knowledge of
density for aerobrakingMonitor Atm. Temp for aerobraking |
 Deep Space 2 |
Jan 1999 |
Mars Probe - on Mars Polar Lander |
New Millennium Mission - sub-surface samples |
 Mars Surveyor 01 |
Mar 2001 |
Mars |
IR monitoring of dust (CO band) for knowledge of
density for aerobrakingMonitor Atm. Temp for
aerobrakingLong-term atm / weather observations - volatile
cycles |
 Mars Surveyor 03 |
May 2003 |
Mars |
IR monitoring of dust (CO band) for knowledge of
density for aerobrakingMonitor Atm. Temp for
aerobrakingLong-term atm / weather observations - volatile
cycles |
 Stardust |
Feb 1999 |
Comet sample return |
Thermal emission of dust content-Model dust
environNucleus size / rotation for mission imaging |
 NEAP |
1999-2000 |
Asteroid |
Thermal IR for size, albedo,
rotation Thermal vs. wavelength to model thermal inertia to
interpret 0.9-2.4um spectra10um spectroscopy to get minerology |
 SIRTF |
2001 |
Various |
IR Space TelescopeCharacterize classes of objects for target
selectionProvide impt. 1-5 um spectra for characterizing brown
dwarfsThermal measurements for interpretation of protoplanetary
disk data |
 SOFIA |
Future |
Developing target lists |
Airborne observatoryComplementary wavelength
coverageFollowup Observations Instrumentation development |
 CONTOUR |
Jul 2002 |
Comets |
Nucleus size, albedo, rotation for
mission imagingThermal emission of dust for dust environment
Big IRTF campaign 11/03 for Encke Earth approach of 0.2 AU |
 Europa Orbiter |
2002-2003 |
Europa |
Measure disk integrated thermal properties to
compare to Galileo missionSearch for active endogenic hotspots in
eclipse |
 Muses-C |
2002 |
Asteroid sample return |
Thermal measurments
for size, albedo, rotationThermal measurements versus wavelength
for thermal inertia10 um spectroscopy for minerology |
 Pluto Fast Flyby |
2004 |
Pluto, Charon, KB objects |
1-5um SPEX spectra to monitor decay of
atmosphere |
 Rosetta |
Jan 2003 |
Asteroids, Comet |
Nucleus physical characteristics size, albedo,
rotation - to plan imagingKnowledge of dust environment |
 Deep Space 3 |
late 2001 |
Bright astrophysical objects |
This will be a free-flying formation of 3 telescopes
in space for high resolution imaging. |
 Deep Space 4 |
2003 |
Comet |
Thermal emission for size and albedoThermal
measurements of dust as a function of time to predict s/c
environmentSearch for local active areas |
 Solar Probe |
Nov 2003 |
Sun |
Fly through the solar corona. |
 Space Interferometry |
Future |
Origins |
Space Observatory - high resolution imaging - planet search |
 Terrestrial Planet Finder |
Future |
Origins |
Space Observatory - high resolution imaging - planet search |
 Genesis |
Jan 2001 |
solar wind |
Discovery mission to study the solar wind |
 Mercury Messenger |
2004 |
Mercury |
Discovery mission 7 - global surface and atmospheric study
of the planet Mercury |
 Deep Impact |
2004 |
Comet P/Tempel 1 |
Discovery mission 8 - comet impact will study crater
formation interior structure of comet change in comet activity
|