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The Mars Dichotomy

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Topographic profiles across the Mars dichotomy are not consistent with ancient ... It is unlikely a giant impact resurfaced the N hemisphere of Mars. ... – PowerPoint PPT presentation

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Title: The Mars Dichotomy


1
The Mars Dichotomy
  • Evidence for Plate Tectonics or Erosion?

2
Theories of the Dichotomy Formation
  • Giant Impact
  • One major collision resurfaced the region.
  • Multiple Impacts
  • Several large impacts caused resurfacing.
  • Ancient Ocean
  • An ancient ocean existed in the northern
    hemisphere. The ocean eroded away the surface
    erasing the craters observed in the southern
    hemisphere.
  • Plate tectonics
  • Erosion
  • Out flow channels

3
Impacts
  • Wilhems and Squyres (1984) suggested a single
    impact hypothesis.
  • The geology of the northern lowlands (Vastitas
    Borealis) is not consistent with a one impact
    hypothesis. (Frey et. al., 1986a)
  • The lowlands are not radial in shape (Smith et.
    al. 1999), and there is no evidence of a crater
    rim.

4
Several Impacts
  • The lowland geology could have formed through
    several large impacts.
  • Impact basins on mercury and the moon roughly
    follow a the D-? distribution curves,
  • Frey and Schultz (1988) concluded that the
    largest impact basins on Mars (Fig 2A) roughly
    follow this curve, but the proposed Borealis
    impact does not.
  • But is the 2A curve really a good fit?

5
Ocean erosion
  • Topographic profiles across the Mars dichotomy
    are not consistent with ancient shoreline
    (Withers and Neumann, 2001).
  • Possible shoreline slopes are not orientated in
    the correct direction
  • Concluded shorelines were most likely created
    by compressive tectonic stress.
  • Suggested volcanism and impact craters.

6
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7
Utopia
Utopia
-Inferred shorelines slope down to the
North. -However, the slopes appear to be impact
related.
North facing slopes
  • Alba Patera
  • -Inferred shorelines
  • slope down to the south.
  • This is opposite of the expected slope
  • direction, if formed by an ocean shore.
  • -Slopes are most likely due to volcanic
    compression.

Note shoreline reversal
Alba Patera
South facing slopes
(Withers and Neumann, 2001)
8
Plate Tectonics
  • The differences between the Northern and Southern
    hemisphere's can be interpreted using analogs to
    earths plate tectonics.
  • Crustal thickness, volcanoes, and contraction
    features.
  • Sea floor spreading continuously forms new
    crust at rift margins.
  • New crust will be smother and thinner then old
    crust.
  • Subduction destroys the new crust, which provides
    the fuel for volcanic activity.
  • Tharsis?
  • Convergence will produce contraction features
    along the plate boundary

9
Contraction Features
  • Watters (1993) mapped contraction features on the
    surface of Mars.
  • Wrinkle ridges, lobate scarps, and high relief
    ridges.
  • Wrinkle ridges are regularly spaced landforms
    generally caused by thrust faulting and/or
    folding.
  • Wrinkle ridges accounted for 80 of the mapped
    contraction features.
  • Watters found that contractional features are
    generally parallel to the dichotomy boundary in
    the eastern hemisphere.
  • Suggests the influence of regional stresses
    related to dichotomy formation.
  • Whereas the pattern in the western hemisphere
    reflects the Tharsis volcanic province.
  • The geometry of the inferred stress was analyzed
    by fitting great circles to each mapped segment,
    and plotting them on a Schmidt net to create a
    Beta diagram (an equal area stereonet
    projection). (Watters, 1993)

10
East
West
Above Beta Diagram showing the concentration of
great circle intersections to inferred maximum
principle stress direction. -Note the general E-W
trend of the contraction features. -Two
clusters dominate at Tharsis and Hesperia
Planum. (Watters, 1993)
Wrinkle Ridges
11
Mars Tectonics
  • The northern hemisphere of Mars was formed during
    sea floor spreading along a ridge axis that
    broke away from Terra Cimmeria.
  • Terra Cimmeria then acted as a passive margin.
  • Subduction initiated along Arabia Terra and the
    eastern edge of the Tharsis volcanic province.

(Sleep, 1994)
12
Not to scale
13
Not to scale
Plate motion ceases when the rift margin is
subducted.
14
Plates and Margins
15
1
2
-Yellow outline shows the plate margin at the
time of the break up.
-The singular plate breaks into 2 plates,
possibly due to subduction angle and different
plate velocities.
(Sleep, 1994)
16
4
3
-New plate geometry after the break up. -Note
the transform fault between the two plates.
-Plate geometry at the time plate motion is
inferred to have ceased.
(Sleep, 1994)
17
Fast vs. Slow Spreading Rates
  • On earth a fast spreading center produces smooth
    topography, and virtually no vertical scarps.
  • Slow spreading centers build up topography, and
    have a large number of high angle scarps.

East Pacific Rise
Mid-Atlantic Ridge
18
Summary of Martian Tectonics(Sleep, 1994)
  • Due to the smooth nature of the northern lowlands
    sea floor spreading must have occurred
    relatively fast.
  • A quantitative estimate of a full plate spreading
    rate is 80 mm/yr.
  • This is fast, but comparable to places on earth,
    such as the East Pacific Rise.
  • The northern lowland crust would have formed
    rather quickly, and plate tectonics may not have
    lasted that long.
  • Plate tectonics could aid in cooling the interior
    of Mars.

19
Magnetic Stripes
  • Magnetic field observations acquired by the MGS
    suggest Mars possessed a periodically reversing
    dynamo

(Acuna et. al., 1999).
20
Dynamo
  • On earth the dynamo occurs due to convection in
    the outer core. Convection in the core occurs
    because it is being cooled by the mantle.
  • Plate tectonics can drive core convection.
  • Absence of crustal magnetism near large impacts
    basins suggests the dynamo was only active early
    in Mars history during the Naochian epoch 4
    billion years ago. (Acuna et. al., 1999)
  • It is proposed that cessation of plate tectonics
    is linked to the cessation of the Mars dynamo
    (Nimmo and Stevenson, 2000).
  • i.e. Plate tectonics allows the planet to cool
    from the inside out.

21
Summary
  • It is unlikely a giant impact resurfaced the N
    hemisphere of Mars.
  • It is possible multiple large impacts resurfaced
    the N hemisphere.
  • However, this is not supported geological or
    statistically.
  • There is no evidence of an ocean shore line, only
    tectonic features and impact ridges.
  • Plate tectonics provides a possible mechanism for
    N hemisphere resurfacing.
  • Magnetic stripes are present on Mars, therefore
    a dynamo may have existed early in Mars history.

22
Future Work
  • Photo mapping of the dichotomy boundary would
    reveal subtle details required for an accurate
    geologic analysis.
  • Detailed N-S gravity profiles across the
    dichotomy to analyze the details of the crustal
    thickness variation.
  • Send a geologist to Mars to map the boundary!
    Well figure it out.....

23
References
  • Acuna, M.H. et. al., Global distribution of
    crustal magnetization discovered by the Mars
    Global Surveyor MAG/ER experiment, Science, 284,
    790-793, 1999.
  • Frey et. al., The martian crustal dichotomy
    product of accretion and not a specific event?
    (abstract) Lunar and Planet. Sci., 27, 241-242,
    1986a.
  • Frey, H. and R.A. Schultz, Large impact basins
    and the mega-impact origin for the crustal
    dichotomy on Mars, Geophys. Res. Lett., 15,
    229-232, 1988.
  • Nimmo F. and D.J. Stevenson, Influence of early
    plate tectonics on the thermal evolution and
    magnetic field of Mars, J. Geophys. Res., 105,
    11,969-11,979, 2000.
  • Sleep, N.H., Martian plate tectonics, J Geophys.
    Res., 99, 5639-5655, 1994.
  • Smith, D.E. et. al., The global topography of
    Mars and implications for surface evolution,
    Science, 284, 1495-1502, 1999.
  • Watters, T. R., Compressional tectonics on Mars,
    J. Geophys. Res., 98, 17,049-17,060, 1993.
  • Wilhems D.E. and S.W. Squyres, The martian
    hemisphere dichotomy may be due to a giant
    impact, Letters to Nature, 309, 138-140, 1984.
  • Withers P. and G.A. Neumann, Enigmatic northern
    plains of Mars, Nature brief communications,
    410, p.651, 2001.

24
Outflow channels
  • Images from Mars show distinct valley networks
    that flow across the dichotomy from S to N.
  • These outflow channels may have carried water (or
    even volcanic materials) into the northern plains
  • But it would take a large standing body of water
    to physically form the dichotomy.
  • Implies episodic flooding.

25
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26
Valles Marineris Linear shape implies it was
formed tectonically.
27
Increase in crustal thickness to the south must
have formed by internal processes.However, the
Northern lowlands may have been resurfaced
through water/volcanic outflow.
Arabia Terra
(Zuber, 2001)
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