Exploring Habitability, Hydrology, and Climate Change on Mars at ...

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Exploring Habitability, Hydrology, and Climate Change on Mars at Columbus Crater Abstract #1041 Kennda Lynch 1 and James Wray 2 1 Depart of Civil & Environmental Engineering, Colorado School of Mines 2 School of Earth and Atmospheric Sciences, Georgia Tech

Transcript of Exploring Habitability, Hydrology, and Climate Change on Mars at ...

Page 1: Exploring Habitability, Hydrology, and Climate Change on Mars at ...

Exploring  Habitability,  Hydrology,  and  Climate  Change  on  Mars  at  Columbus  

Crater    Abstract  #1041  

Kennda  Lynch1  and  James  Wray2  1  Depart  of  Civil  &  Environmental  Engineering,  Colorado  School  of  Mines  

2School  of  Earth  and  Atmospheric  Sciences,  Georgia  Tech  

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Columbus  Crater:  Overview  1st  EZ  Workshop  for  Human  Missions  to  Mars  

Ground-­‐water  filled  paleolake basin~110  km  in  diameter  Estimated  1.5  km  depth  of  sedimentary  and/or  volcanic  infill  Excellent  crater  retention  for   age  dating  Diversity  of  Noachian  &   Hesperian  aged  deposits  and  outcrops  High  diversity  of  aqueous   mineral  deposits  

     Polyhydrated  sulfates  

     Al-­‐phyllosilicate  

     Fe/Mg-­‐phyllosilicate  

     Jarosite,  alunite  

     Monohydrated  sulfate  

     Unknown  hydrated  phase  

b  

CAB2  5AA4  

750A  

13D1F  

13FF5  

16F13  

1663B  

ABF2  

16CFE  

7D87  

12C19  

1212A  

5483  

62B6  

13EEF  

8565  

167FA  

Columbus  Crater   Wray  et  al.,  2011   2  

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

Columbus  Crater  

Analog  Studies  

Lynch  et  al.,  2015   3  

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Columbus  Crater  

LZ  &  Field  Station   Latitude:  194.0194  E  Longitude:  29.2058  S  Altitude:  +910  m  

SROI  #1  

SROI  #2  

SROI  #5  

SROI  #4  

RROI  #1  LZ/HZ  

22  KM  

4  

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

Science  ROI(s)  Rubric  

Site Factors

SR

OI1

SR

OI2

SR

OI3

SR

OI4

SR

OI5

RR

OI1

EZ S

UM

Sci

ence

Sit

e C

rite

ria

Ast

robi

o

Threshold

AN

D/

OR

Potential for past habitability ●   ●   ●   ● ●     ● (6,0) Potential for present habitability/refugia  ? ? ?     ? ? (0,0)

Qualifying Potential for organic matter, w/ surface exposure ● ○ ● ● ● ●   (5,1)

Atm

osph

eric

Sci

ence

Threshold Noachian/Hesperian rocks w/ trapped atmospheric gases ●     ●   ●   ●   ●   ●   (6,0)

Qualifying

Meteorological diversity in space and time ●     ●     ●     ●     (4,0) High likelihood of surface-atmosphere exchange ● ● ●     (3,0)

Amazonian subsurface or high-latitude ice or sediment ○   ○     ○   ○   ○   ○     (0,6) High likelihood of active trace gas sources ? ? ? ? ? ? (0,0)

Geo

scie

nce

Threshold

Range of martian geologic time; datable surfaces ●     ●   ●   ●   ●   (5,0) Evidence of aqueous processes ●   ●   ●   ●  ●   ● (6,0)

Potential for interpreting relative ages ●     ●   ● ●   ●   ●   (6,0)

Qualifying

Igneous Rocks tied to 1+ provinces or different times ● ● ● (3,0) Near-surface ice, glacial or permafrost ? ? ? ? ? ? (0,0)

Noachian or pre-Noachian bedrock units ○     ○   (0,2) Outcrops with remnant magnetization ○   ○   (0,2)

Primary, secondary, and basin-forming impact deposits ● ● ● (3,0) Structural features with regional or global context   ● (1,0) Diversity of aeolian sediments and/or landforms ● ● ● (3,1)

Key

●   Yes

○   Partial Supportor Debated

No

? Indeterminate

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

Resource  ROI(s)  Rubric  Site Factors

RR

OI1

LZ/

HZ

EZ S

UM

ISR

U a

nd

Civ

il En

gin

eeri

ng

Cri

teri

a

Engineering Meets First Order Criteria (Latitude, Elevation, Thermal Inertia)  ●   ●   (2,0)

Wat

er R

esou

rce

Threshold

AN

D/

OR

Potential for ice or ice/regolith mix (0,0)Potential for hydrated minerals ● (1,0)

Quantity for substantial production ?     (0,0)Potential to be minable by highly automated systems ?   (0,0)

Located less than 3 km from processing equipment site ○   (0,1)Located no more than 3 meters below the surface ● (0,1)

Accessible by automated systems  ○   (0,1)

Qualifying

Potential for multiple sources of ice, ice/regolith mix and hydrated minerals (0,0)Distance to resource location can be >5 km ●   (1,0)

Route to resource location must be (plausibly) traversable  ●   (1,0)

Civ

il En

gine

erin

g

Threshold

~50 sq km region of flat and stable terrain with sparse rock distribution ○   (0,1)1–10 km length scale: <10° ○   (0,1)

Located within 5 km of landing site location ○   (0,1)

Qualifying Located in the northern hemisphere (0,0)

Evidence  of  abundant  cobble  sized  or  smaller  rocks  and  bulk,  loose  regolith    ●   (1,0)Utilitarian terrain features ? (0,0)

Food

Pr

oduc

tion

Qualifying

Low latitude  ● (1,0)No local terrain feature(s) that could shadow light collection facilities   (0,0)

Access to water (0,0)Access to dark, minimally altered basaltic sands ○ (0,1)

Met

al/S

ilico

n Re

sour

ce

Threshold

Potential for metal/silicon ●   (1,0)Potential to be minable by highly automated systems ○ (0,1)

Located less than 3 km from processing equipment site (0,0)Located no more than 3 meters below the surface  ●   (1,0)

Accessible by automated systems ○     (0,1)

Qualifying

Potential for multiple sources of metals/silicon ● (1,0)Distance to resource location can be >5 km ● (1,0)

Route to resource location must be (plausibly) traversable  ●   (1,0)

Key

●   Yes

○   Partial Supportor Debated

No

? Indeterminate

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

Columbus  Crater  

LZ  &  Field  Station  

500  m  

7  

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

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Columbus  Crater  

Science  ROI  1  

Northeastern  Shore  194.2591°  E,  -­‐28.883°  N  Most  exposed  light  toned  units  &  highest  diversity  of  aqueous  mineral  deposits  

Wray  et  al.,  2011   8  

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

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Columbus  Crater  

Science  ROI  2  

D11  Crater  194.2591°  E,  29.581°  S  Stratigraphic  context    Possible  RSL  

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

Columbus  Crater  

Science  ROI  3  

Wray  et  al.,  2011  

Bathtub  Ring  

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

Columbus  Crater  

Science  ROI  4  

Pedestal  Crater  193.603°  E,  29.345°  S  

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

Columbus  Crater  

Science  ROI  5  

Dual  Craters  • 193.599°  E,  29.973°  S    

12  

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

Columbus  Crater  

Central  Peak  193.865°  E,  29.101°  S  •

 

Resource  ROI  1  

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1st  EZ  Workshop  for  Human  Missions  to  Mars  

Columbus  Crater  

Data  Coverage  

CRISM  Coverage       HiRISE  Coverage      14  

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Columbus  Crater  

Highest  Priority  EZ  Data  Needs  1st  EZ  Workshop  for  Human  Missions  to  Mars  

Science  CoverageHRSC  coverage  of  crater  rim  &  basin  floorCRISM  coverage  of  the  Northwest  crater  RimGeneral  HiRISE  coverage  of  the  crater  rim  and basin  floor

Resource  CoverageGeneral  HiRISE  coverage  of  basin  floor  

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