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Life in the Atacama Project Workshop

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Title: Life in the Atacama Project Workshop


1
Life in the AtacamaProject Workshop
  • Science Objectives and InvestigationJuly 28-30,
    2003
  • Nathalie A. CabrolNASA Ames

2
How do we Perceive the World through Hyperion ?
  • Is the payload right? (Improve/drastic changes)
  • Ability at finding life
  • Ability at finding and characterizing habitats
  • Ability at capturing transitions and subtle
    changes in habitats
  • Are the science exploration strategies adequate?
  • (Very) preliminary observations
  • Goals reached
  • Go beyond our mindsets!
  • Bio I want white rocks (the tree hiding the
    forest.
  • I want an image of that hill! (to know what it
    is a spectra could have been acquired from
    distance instead and composition known.
  • We need to make sure that our strategies will
    allow to limit the weight of mindsets on overall
    results.

3
Summary of Presented Material
  • Overall Science Goals
  • Review of Science Questions and Methods
  • Science Payload
  • Science Activities since 12/02
  • Remote Science Operations FY03 Framework
  • FY03 Science Objectives and Exploration
    Strategies Tested during the Field Campaign
  • Post Field Experiment Science Activities

4
Overall Science Goals
  • A real science question on Earth with critical
    applications to Mars
  • Understand the Atacama as a habitat for life
  • Document the limits of life on Earth
  • Test the capacity of a science payload to detect
    and characterize life in one of the most desertic
    environments of Earth for application to the
    exploration of Mars
  • Test astrobiological exploration strategies and
    train science teams to benefit future Mars
    missions. remote science
  • Test astrobiological exploration strategies for
    the exploration of extreme terrestrial
    environments. telepresence
  • Make genuine discoveries and contribute to the
    body of knowledge about the Atacama and life in
    terrestrial extreme environments.

5
Science Method and Questions
  • Unambiguous Signature of Life?
  • Goal Establish in situ the presence of life
  • No speculation
  • Converging evidence from instruments data
  • Is unambiguous realistic? Increasing the
    probability of detecting life signature?
  • Map Habitats (morphology, geology, mineralogy,
    texture, physical and elemental properties of
    rock and soil)
  • Document how life modifies its environment
    (geo-bio)
  • Derive survival strategies
  • Develop science protocols on what should
    constitute a life discovery claim
    (extinct/extant)
  • Identify biosignatures (and life geosignatures)

6
Science Payload
7
Science Activity since 12/02
8
First Campaign Remote Science
  • Location NASA Ames Research Center
  • Science Ops Room in Space Science Division
  • SST Computer rooms 1 station in the science
    ops room and 3 laptops computer projector.
  • Pre-Mission Data Set
  • ASTER Orbital image (pre-mission)
  • DEM from orbital image GPS points

9
Orbital Images ASTER
Resolution relevant to Mars Express
  • Used for
  • Context
  • pre-mssion
  • mission
  • Base Mapping
  • Topography (DEM)

10
First Campaign Remote Science
  • Data from the field during Mission
  • Imagery (visible) SPI (PanCam equivalent)
  • Microscopic Images Fluo Dyes
  • Some Vis/NIR spectra (ground)
  • Environmental data
  • Post-Mission Data
  • Vis/NIR set of samples spectra
  • Hyperion Orbiter spectral imagery (post-mission)
  • Data stored on Science Ops. Website (_at_CMU)

11
High-Resolution Imagery/SPI
Resolution Equivalent MER PanCam
  • Detailed science interpretation
  • Used for geology and biology
  • Data Products
  • High-res. single images
  • Mosaics
  • Panoramas

12
SPI/Mosaic and Panoramas
  • Color adjustments needed at the beginning of the
    mission. Inproved after. Panorama were most of
    the time of excellent quality.
  • Camera alignment problematic. Was visible when
    trying to build anaglyphs

13
Example Derived Products Anaglyphs 3D world for
SPIYr2 MI?
14
Biology Microscopy and Fluorescence
vis
530-570
450-660
15
First Campaign Framework
  • Component testing ?
  • Limited integration of science instruments
  • SPI, EnviS onboard
  • Vis/NIR, Fluor. Microscope in the field
  • XRD/XRF at Ames for further sample anal.
  • Limited Remote Science Team
  • 2 geologists, 2 biologists, 2 mineralogists
    (consultants), 2 support data managers.
  • Science Team with limited to no experience in
    rover field experiment (1 exception). On purpose

16
First Campaign Framework
  • Field Science Team Instruments Support
  • Jeff Moersch, Alan Waggoner, Guillermo Chong
  • No Limit on Bandwidth
  • Focus on testing exploration strategies
  • Implications
  • Strategies immediately applicable to terrestrial
    exploration
  • Strategies need to be now calibrated and scaled
    for Mars (bandwidth/communications) Real mission
    sols number?
  • Data came through emails and web
  • Pan/image Processing via CMU

17
First Campaign Framework)
  • Limited Communications
  • Simulation of Orbital Pass (1 uplink and 1
    downlink/day)
  • Eventscope tools use beyond E/PO
  • Support Science Team Data Analysis
  • Need to explore promising potential unraveled
    during the mission (e.g., triangulation,
    embedding information in pans, etc.)
  • Importance to use Mars missions tools
    (discussed on Wednesday).

18
Year 1 Exploration Strategies (1)
  • How to obtain a comprehensive understanding of
    life and habitat?
  • Random Sampling (large-scale mapping)
  • Along a traverse from A to B, rover stops every
    determined n-meters, deploys a set number of
    instruments and always acquire same type of data
    (e.g., 1 mosaic Vis/NIR spectra microscopic
    image)
  • Efficient way of mapping fast
  • Good statistical chance of discovery. Need a way
    to call home if discovery or to develop methods
    of finding our way back to the find if rover
    continues and only calls at set times. Dvlpt
  • Directly applicable to remote-sensing
    terrestrial astrobiology. Bandwith constraints
    for Mars. Adpt

19
Year 1 Exploration Strategies (2)
  • Random Sampling (large-scale mapping, cont.)
  • Maybe too large scale to grasp the fine-scale
    changes of habitats as observed in the
    Atacama/Mars.
  • That could make the difference between finding
    life or not
  • Or will allow to find life (good statistical
    coverage) but will not allow to understand subtle
    changes in habitats.
  • What is important at this stage? Finding Life!
    So, this is a valid search strategy for Mars.
  • It must be used as an exploratory mode. Great
    tool for developing background information on a
    site.

20
Year 1 Exploration Strategies (3)
  • Targeted Sampling
  • Thorough investigation of science targets of
    interest identified in the scene.
  • Similar to what is currently used (MPF/MER)
    However, payload differs
  • Allows a reasoned search
  • Time consuming (approach, positioning). Time
    spent there is not used to cover ground and learn
    more environment.
  • However, excellent tool to obtain
    high-resolution information on specific
    important targets compared to Random Sampling.
  • Not an exploratory mode in the broad sense. It is
    an in-depth analysis tool.
  • Convey all the good and bad of current Mars
    exploration

21
Year 1 Science Numbers
22
Post Field Experiment Science Activities
  • Extended Mission Data Analysis
  • May to July 28th
  • Addition of Vis/NIR spectra
  • Hyperion Orbital imagery
  • Remote Science Team Year 1 Final Report
  • Assessment of Science Interpretation Success
    Rate
  • November 2003 Site Selection Year 2 Campaign
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