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Infrared Mars: Activities at the Mars Space Flight Facility

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Title: Infrared Mars: Activities at the Mars Space Flight Facility


1
Infrared Mars Activities at the Mars Space
Flight Facility
  • Joshua L. Bandfield
  • Arizona State University

THEMIS infrared image of the Martian limb
2
Spacecraft Instruments
  • TES on Mars Global Surveyor
  • THEMIS on 2001 Mars Odyssey
  • Mini-TES on the Mars Exploration Rovers

3
Mars Global SurveyorThermal Emission
Spectrometer (TES)
  • 143 infrared colors from 6-50 mm
  • 3 km resolution
  • 6 spectra every two seconds almost continuously
    from 1997-2005

4
TES Data
5
Mars OdysseyThermal Emission Imaging System
(THEMIS)
  • 9 infrared colors from 7-15 mm wavelengths
  • 100 m resolution
  • Also 18 m resolution visible camera

6
THEMIS Data
Band 654 Radiance
Surface Unit Emissivity
1.00
0.98
0.96
0.94
0.92
Emissivity
0.90
0.88
0.86
6
7
8
9
10
11
12
13
Wavelength (mm)
7
Mars Exploration Rovers mini-TES
  • 167 infrared colors from 5-28 mm
  • 20 mrad resolution (several cm and larger)
  • Similar to the TES instrument

8
Mini-TES Data
9
Science Activities
  • Three basic questions we try to answer
  • What is the composition of the Martian surface?
  • What are the physical properties of
    rocky/sandy/dusty surfaces and ices?
  • How does the Martian atmosphere work?

10
Spectroscopy
  • Most rock forming minerals have distinctive
    absorptions (colors) in the thermal infrared

11
Hematite
  • Mars spectral fingerprint from TES matches
    laboratory data of hematite in Sinus Meridiani
  • Hematite forms in water!

TES Data
Laboratory Hematite
12
  • The discovery of hematite led to the selection of
    the primary Mars Exploration Rover landing site

TES Hematite Concentrations
13
TES and THEMIS show that Mars has a variety of
igneous compositions
THEMIS Band 875 DCS
Granite in Syrtis Major
Basalt and dacite in Nili Patera
14
THEMIS Data from the Southern Highlands
15
Looking at Mars with Different THEMIS Images
16
Why are nighttime temperatures useful?
Dusty
Sandy
Rocky
  • Determining surface properties using thermophysics

Rocky
Sandy
THEMIS Night IR
Dusty
17
Mapping Water Ice
  • By observing seasonal temperatures we can sense
    buried water ice

Water Ice Depth
Shallow
Deep
18
Atmospheric Monitoring
NASA/JPL/MSSS
19
NASA/JPL/MSSS
20
Temperatures and Season
NASA/JPL/GSFC
21
(No Transcript)
22
E/PO Activities
  • Mars Student Imaging Project
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