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Flexure model The flexure of an elastic plate in two dimensions obeys Equation 1 4 4 + โˆ’ = 0 Equation 1. where = 4 โˆ’ 1/4 is the flexural parameter, = โˆ—โ„Ž 3 12(1โˆ’ 2 ) is the flexural rigidity, is the density of the underlying layer of the ice shell, is the density of the ice shell. g is the gravity on Pluto, E is the Youngโ€™s modulus of water ice, h is the elastic thickness, and is Poissonโ€™s ratio For a single vertical load at =0 , the boundary conditions are 3 3 = 1 2 0 and =0 The deflection due to several line loads is found by superposition: = ฯƒ 3 8 sin โˆ’ + cos โˆ’ exp โˆ’ โˆ’ Equation 2. Where { } is the magnitude of the loads at position { } Inversion The load vector that produces topography , is found by least squares optimization: = โ€ฒ + โˆ’1 โ€ฒ where M is the operator matrix that links a load at position to deflection at a point = 3 8 sin โˆ’ + cos โˆ’ exp โˆ’ โˆ’ and = โˆ’2 is the covariance matrix, whose components are linked to the noise of the topographic data, Synthetic Model The inversion method was tested using two synthetic profiles generated by Dr. Montesi. I inverted the profiles using many test values of and recorded the misfit. The smallest misfit was found for = 45 ยฑ 32 (1 value) when the synthetic profile was built with = 45 and for = 224 ยฑ 160 (1 value) when the synthetic profile was built with = 225 (shown in figure below). Motivation Sputnik Planitia Flexural modeling Plans for GEOL 394 Left image. The top panel displays an elastic flexure signal under a line load along with the curve of best fit that was produced with the misfit test. The bottom panel displays the mass distribution. The model is unitless. Right image. The flexural parameter, alpha, and misfit values displayed as a graph with the best misfit value highlight with a dot. โ€ข Conduct the analysis of the inverse theory on the 20 profiles tracked for Sputnik Planitia and its surrounding. โ€ข Find if the elastic thicknesses and load magnitude for all 20 profiles are consistent. โ€ข Time permitting, create a 2D finite element model that uses the geometry of Sputnik Planitia to also find the best elastic thickness and load magnitude. โ€ข The values for elastic thickness and load size will indicate if the interior is warm or cold, which helps constrain the timing of the load. This model may also allow the evaluation if a subsurface ocean is needed as that will change the flexibility of Plutoโ€™s ice shell. False-color elevation map of Sputnik Planitia with twenty 600 km long tracks approximately perpendicular to the edge of the basin. Selected topographic profiles across the edge of Sputnik Planitia. Each profile is offset for clarity. Some profiles show a clear topographic bulge while others show apparently random variations. Sputnik Planitia โ€ข Large teardrop-shaped basin located on Pluto at 20ยฐN 180ยฐE โ€ข Size: 1300 km by 900 km โ€ข Depth: 3-4 km (basin) โ€ข Deposit of nitrogen ice โ€ข Water ice basement Formation Hypotheses โ€ข An ancient impact basin created by an impactor later filled with N 2 ice. The feature would have moved to the current location through polar wander. โ€ข Runaway deposition of N 2 ice due to albedo feedback at the ยฑ30ยฐ. The depression is due to elastic flexure under the load of a thick N 2 ice cap. Most of the cap has since sublimated away. Hypothesis โ€ข The topography of Pluto around Sputnik Planitia matches the prediction of an elastic plate flexed by a large load. Expected results and implications โ€ข What elastic thickness would explain the observe topography around Sputnik Planitia? โ€ข Was the interior relatively warm or cold? Did the deformation happen early or late in the history of Pluto? โ€ข Was the ice as flexible as expected if there is a water ocean? โ€ข What load distribution and amplitude can explain the observed topography? โ€ข Is there evidence of a much larger N 2 ice layer as inferred today? Example of plate flexure on Earth โ€ข The Hawaiian islands act as line load on the Pacific Plate. โ€ข Flexure is expressed as a moat around the islands surrounded by a bulge. โ€ข A similar signal may be present around Sputnik Planitia. โ€ข Topographic map and profile taken from GeoMapApp. Theoretical model of elastic flexure โ€ข An elastic plate subjected to a line load is deflected downward, forming a moat. โ€ข A bulge develop due to the restoring force acting against the deflected plate.
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Motivation Sputnik Planitia Flexural modelingย ยท Motivation Sputnik Planitia Flexural modeling Plans for GEOL 394 Left image. The top panel displays an elastic flexure signal under

Jul 25, 2020

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Page 1: Motivation Sputnik Planitia Flexural modelingย ยท Motivation Sputnik Planitia Flexural modeling Plans for GEOL 394 Left image. The top panel displays an elastic flexure signal under

Flexure modelThe flexure of an elastic plate in two dimensions obeys Equation 1

๐ท๐‘‘4๐‘ค

๐‘‘๐‘ฅ4+ ๐œŒ๐‘š โˆ’ ๐œŒ๐‘ ๐‘”๐‘ค = ๐‘‰0 Equation 1.

where ๐›ผ =4๐ท

๐œŒ๐‘šโˆ’๐œŒ๐‘ ๐‘”

1/4is the flexural parameter, ๐ท =

๐ธโˆ—โ„Ž3

12(1โˆ’๐‘ฃ2)is the flexural rigidity, ๐œŒ๐‘š is the

density of the underlying layer of the ice shell, ๐œŒ๐‘ is the density of the ice shell. g is the gravity on Pluto, E is the Youngโ€™s modulus of water ice, h is the elastic thickness, and ๐œˆ is Poissonโ€™s ratio

For a single vertical load at ๐‘ฅ = 0 , the boundary conditions are ๐ท๐‘‘3๐‘ค

๐‘‘๐‘ฅ3=

1

2๐‘‰0 and

๐‘‘๐‘ค

๐‘‘๐‘ฅ= 0

The deflection due to several line loads is found by superposition:

๐‘ค = ฯƒ๐‘–๐‘‰๐‘– ๐›ผ

3

8๐ทsin

๐‘ฅโˆ’๐‘ฅ๐‘–

๐›ผ+ cos

๐‘ฅโˆ’๐‘ฅ๐‘–

๐›ผexp โˆ’

๐‘ฅโˆ’๐‘ฅ๐‘–

๐›ผEquation 2.

Where {๐‘‰๐‘–} is the magnitude of the loads at position {๐‘ฅ๐‘–}

InversionThe load vector ๐• that produces topography ๐ฐ, is found by least squares optimization:

๐• = ๐Œโ€ฒ๐Œ+ ๐‚๐’Žโˆ’1 ๐Œโ€ฒ๐ฐ

where M is the operator matrix that links a load at position ๐‘ฅ๐‘— to deflection at a point ๐‘ฅ๐‘–

๐Œ๐‘–๐‘— =๐›ผ3

8๐ทsin

๐‘ฅ๐‘– โˆ’ ๐‘ฅ๐‘—

๐›ผ+ cos

๐‘ฅ๐‘– โˆ’ ๐‘ฅ๐‘—

๐›ผexp โˆ’

๐‘ฅ๐‘– โˆ’ ๐‘ฅ๐‘—

๐›ผand ๐‚๐‘š = ๐œŽ๐‘ก

โˆ’2 ๐›ฟ๐‘–๐‘— is the covariance matrix, whose components are linked to the noise of the

topographic data, ๐œŽ๐‘ก

Synthetic Model The inversion method was tested using two synthetic profiles generated by Dr. Montesi. I inverted the profiles using many test values of and recorded the misfit. The smallest misfit was found for ๐›ผ =45 ยฑ 32 (1๐œŽ value) when the synthetic profile was built with ๐›ผ = 45 and for ๐›ผ = 224 ยฑ 160 (1๐œŽvalue) when the synthetic profile was built with ๐›ผ = 225 (shown in figure below).

Motivation Sputnik Planitia Flexural modeling

Plans for GEOL 394

Left image. The top panel displays an elastic flexure signal under a line load along with the curve of best fit that was produced with the misfit test. The bottom panel displays the mass distribution. The model is unitless. Right image. The flexural parameter, alpha, and misfit values displayed as a graph with the best misfit value highlight with a dot.

โ€ข Conduct the analysis of the inverse theory on the 20 profiles tracked for Sputnik Planitia and its surrounding.

โ€ข Find if the elastic thicknesses and load magnitude for all 20 profiles are consistent.โ€ข Time permitting, create a 2D finite element model that uses the geometry of Sputnik Planitia to

also find the best elastic thickness and load magnitude.โ€ข The values for elastic thickness and load size will indicate if the interior is warm or cold, which

helps constrain the timing of the load. This model may also allow the evaluation if a subsurface ocean is needed as that will change the flexibility of Plutoโ€™s ice shell.

False-color elevation map of Sputnik Planitia with twenty 600 km long tracks approximately perpendicular to the edge of the basin.

Selected topographic profiles across the edge of Sputnik Planitia. Each profile is offset for clarity. Some profiles show a clear topographic bulge while others show apparently random variations.

Sputnik Planitiaโ€ข Large teardrop-shaped basin

located on Pluto at 20ยฐN 180ยฐEโ€ข Size: 1300 km by 900 kmโ€ข Depth: 3-4 km (basin)โ€ข Deposit of nitrogen iceโ€ข Water ice basement

Formation Hypothesesโ€ข An ancient impact basin created

by an impactor later filled with N2 ice. The feature would have moved to the current location through polar wander.

โ€ข Runaway deposition of N2 ice due to albedo feedback at the ยฑ30ยฐ. The depression is due to elastic flexure under the load of a thick N2 ice cap. Most of the cap has since sublimated away.

Hypothesisโ€ข The topography of Pluto around Sputnik Planitia matches the prediction of an

elastic plate flexed by a large load.

Expected results and implicationsโ€ข What elastic thickness would explain the observe topography around Sputnik Planitia?

โ€ข Was the interior relatively warm or cold? Did the deformation happen early or late in the history of Pluto?

โ€ข Was the ice as flexible as expected if there is a water ocean?โ€ข What load distribution and amplitude can explain the observed topography?

โ€ข Is there evidence of a much larger N2 ice layer as inferred today?

Example of plate flexure on Earthโ€ข The Hawaiian islands act as line load

on the Pacific Plate.โ€ข Flexure is expressed as a moat around

the islands surrounded by a bulge.โ€ข A similar signal may be present

around Sputnik Planitia.โ€ข Topographic map and profile taken

from GeoMapApp.

Theoretical model of elastic flexureโ€ข An elastic plate subjected to a line

load is deflected downward, forming a moat.

โ€ข A bulge develop due to the restoring force acting against the deflected plate.