sounding the ganymede’s crust with a gpr

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Sounding the Ganymede’s crust with a GPR V. Ciarletti 1 , A. Le Gall 1 , M. Biancheri- Astrier 2 , J-J. Berthelier 1 , S.M. Clifford 3 , D. Plettemeier 4 , M. Hamelin 1 1 LATMOS, Guyancourt, France 2 IDES, Orsay, France 3 LPI, Houston, TX, USA 4 TUD, Dresden, Germany national Colloquium and Workshop “Ganymede Lander: scientific goals and experime

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Sounding the Ganymede’s crust with a GPR. V. Ciarletti 1 , A. Le Gall 1 , M. Biancheri -Astrier 2 , J-J. Berthelier 1 , S.M. Clifford 3 , D. Plettemeier 4 , M. Hamelin 1 1 LATMOS, Guyancourt, France 2 IDES, Orsay, France 3 LPI, Houston, TX, USA 4 TUD, Dresden , Germany . - PowerPoint PPT Presentation

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Page 1: Sounding the Ganymede’s crust  with a GPR

Sounding the Ganymede’s crust with a GPR

V. Ciarletti1, A. Le Gall1, M. Biancheri-Astrier2, J-J. Berthelier1, S.M. Clifford3, D. Plettemeier4 , M. Hamelin1

1LATMOS, Guyancourt, France2IDES, Orsay, France

3LPI, Houston, TX, USA 4TUD, Dresden, Germany

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 2: Sounding the Ganymede’s crust  with a GPR

Scientific Objectives

• Characterize the 3D compositional (ice purity) and physical (porosity, structure) properties of the Ganymede Landing Site down to a depth of ~100m to a few km

• Identify potential shallow (<1 m depth) and deep (up to ~1+ km) structures

• Clues to understand the large-scale geologic evolution of the Landing Site

• Characterize the electromagnetic environment and potential activity of the thin atmosphere (ambient Jovian HF background noise, potential atmospheric discharges )

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 3: Sounding the Ganymede’s crust  with a GPR

Overview

A stationary, impulse, multiband HF GPR operated from the surface

• designed to conduct geologic investigations of planetary environments in both the near and deep subsurface (~1m – few km)

An enhanced version of the low-frequency GPRs developed for

• The original Mars NetLander (CNES) • The original ExoMars mission (mono and bi-static

operations)

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

valerie ciarletti
10m? 1m?
Page 4: Sounding the Ganymede’s crust  with a GPR

The instrument main features

Frequency bands • 2-4 MHz deep soundings (from 100 m to a few kms with a resolution of ~50m)

3D mapping• 3 components of the magnetic field + 2 for the electrical field • Retrieval of the direction of arrival of the echoes - 3D mapping of the reflecting

structures

Modes of operation• Active• Antenna impedance measurement• Passive

Detection of weak echoes• Deployment on the surface• Coherent additions up to 228 (in monostatic operation) to improve the SNR

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 5: Sounding the Ganymede’s crust  with a GPR

Mono-static configuration (NetLander)

Magnetic sensor

Electrical antennas

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 6: Sounding the Ganymede’s crust  with a GPR

Mono & Bi-static configuration (former ExoMars mission)

Magnetic sensor

Electrical antennas

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 7: Sounding the Ganymede’s crust  with a GPR

Coherent additions efficiency

0 1 2 3 4 5 6 7 8 9 10

-10

0

10

nbcoh=1

0 1 2 3 4 5 6 7 8 9 10

-10

0

10

nbcoh=8nbcoh=64

0 1 2 3 4 5 6 7 8 9 10

-10

0

10

nbcoh=64nbcoh=4096

Tens

ion

mes

urée

(mV

)

0 1 2 3 4 5 6 7 8 9 10

-10

0

10

nbcoh=512

0 1 2 3 4 5 6 7 8 9 10

-10

0

10

nbcoh=4096

Retard (s)

nbcoh=4194304

nbcoh=65536

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 8: Sounding the Ganymede’s crust  with a GPR

• Electrical antennas deployed on the surface (transmission and reception)• 2 perpendicular dipoles (2 X 35 m long resistively loaded ribbon

monopoles)

The antennas system

Electrical antennas deployment system

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

valerie ciarletti
Mass : ~100 g (for one antenna and its deployment system)Deployement validated by perfomances experimentaly observed on Earth and extrapolated by simulation to the Martian conditions
Page 9: Sounding the Ganymede’s crust  with a GPR

Magnetic antennas (reception)• 10 cm long search coil magnetic antenna

The antennas system

Magnetic sensor

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 10: Sounding the Ganymede’s crust  with a GPR

Demonstration of 3D investigation

Mono-Static Investigations of the Subsurface in Antarctic

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 11: Sounding the Ganymede’s crust  with a GPR

Demonstration of 3D investigation

Mono-Static Investigations of the Subsurface in Antarctic

Topography reconstruction

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 12: Sounding the Ganymede’s crust  with a GPR

Application to Ganymede

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

In active mode: Assessing the stratigraphy of a grooved terrain, a crater or a putative cryo-volcanic features on Ganymede will significantly help to determine and describe the geological processes that have shaped the moon’s surface and bring new constraints on its age.

Page 13: Sounding the Ganymede’s crust  with a GPR

Application to Ganymede

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

In active mode: could contribute greatly to the understanding of the relationship between this subsurface ocean and the surface by revealing compositional boundaries between different ice sheets.

Page 14: Sounding the Ganymede’s crust  with a GPR

Application to Ganymede

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

In the antenna impedance measurement mode: will help to characterize Ganymede’s crust composition and in particular the proportion of non-ice components in the near surface.

εr=3 σ=10 -5S/m

Simulation

εr~3 σ~10-5 S/m

MeasurementSimulation

Electrical HF antenna impedance measurement

Page 15: Sounding the Ganymede’s crust  with a GPR

Application to Ganymede

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Passive mode: will monitor Jupiter radiation and its variations with time.

Better to operate on the anti-Jupiter side of Ganymede!

Page 16: Sounding the Ganymede’s crust  with a GPR

Summary

The data acquired by such low-frequency GPR will provide local information about the geology of the Landing site:

• at a scale (~100 m – a few kms) and resolution (~10 – 100 m) • including its composition, stratigraphy and structure.

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

valerie ciarletti
1m? 10m?
valerie ciarletti
1m? 10m?
Page 17: Sounding the Ganymede’s crust  with a GPR

Back up slides

Page 18: Sounding the Ganymede’s crust  with a GPR

Mono-Static HF measurementsPassive measurements Impedance measurements

Magnetic sensor Electrical antenna

Bi-Static HF measurements

Mono & Bi-static configuration (former ExoMars mission)

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”

Page 19: Sounding the Ganymede’s crust  with a GPR

Demonstration of 3D investigation

Bi-Static Investigations of the Subsurface

1st interface

2nd interface

3rd interface

TxIn profile:

International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments”