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ÜBERSCHRIFT GRID-MAPPING MARS QUANTIFYING THE GEOGRAPHY OF LANDFORMS M. VOELKER (HRSC)

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Page 1: RID-MAPPING Ü ARS UANTIFYING THE ... - cosmos.esa.int fileINTRODUCTION 5/8/2019 2 GEOGRAPHY - Analysing the spatial distribution of objects - Analysing the relationships between geospatial

ÜBERSCHRIFTGRID-MAPPING MARS – QUANTIFYING THE

GEOGRAPHY OF LANDFORMS

M. VOELKER

(HRSC)

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INTRODUCTION

5/8/2019 2

GEOGRAPHY

- Analysing the spatial distribution of objects

- Analysing the relationships between geospatial objects

- Interdisciplinary field of science

Here: Geology, Geomorphology, Climatology, Planetary/Space Science, (Human Geography)

(Jan Vermeer, The Geographer, 1668/69)

Voelker – Grid-Mapping Mars

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INTRODUCTION

5/8/2019 3Voelker – Grid-Mapping Mars

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INTRODUCTION

5/8/2019 4

Vastitas Borealis

Tharsis

Hellas Planitia

Voelker – Grid-Mapping Mars

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INTRODUCTION

5/8/2019 5

Vastitas Borealis

Tharsis

Hellas Planitia

Voelker – Grid-Mapping Mars

warm cold

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INTRODUCTION

5/8/2019 6

Latitude → Temperature → Evolution ← Distribution ← Landforms↓

Process↙ ↓ ↘

Glacial – (Aeolian) – Fluvial

READING GEOMORPHOLOGY

Voelker – Grid-Mapping Mars

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INTRODUCTION

5/8/2019 7Voelker – Hellas Planitia10 km

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INTRODUCTION

5/8/2019 8

Latitude → Temperature → Evolution ← Distribution ← Landforms↓

Process↙ ↓ ↘

Glacial – Aeolian – Fluvial

READING GEOMORPHOLOGY

Voelker – Grid-Mapping Mars

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INTRODUCTION

5/8/2019 9Voelker – Hellas Planitia10 km

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INTRODUCTION

5/8/2019 10Voelker – Hellas Planitia10 km

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INTRODUCTION

5/8/2019 11

Latitude → Temperature → Evolution ← Distribution ← Landforms↓

Process↙ ↓ ↘

Glacial – (Aeolian) – Fluvial

READING GEOMORPHOLOGY

Voelker – Grid-Mapping Mars

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INTRODUCTION

5/8/2019 12Voelker – Hellas Planitia10 km

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INTRODUCTION

5/8/2019 13Voelker – Hellas Planitia10 km

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INTRODUCTION

5/8/2019 14

LATITUDE-DEPENDENT MANTLE – LDM SCALLOPED TERRAIN(Deposition) (Erosion)

(NASA/MSSS/CTX) (NASA/MSSS/CTX)

Voelker – Grid-Mapping Mars

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INTRODUCTION

5/8/2019 15

Global distribution of LDM (Kreslavsky and Head, 2002)

Voelker – Grid-Mapping Mars

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INTRODUCTION

5/8/2019 16Voelker – Hellas Planitia

Latitude → Temperature → Evolution ← Distribution ← Landforms↓

Process↙ ↓ ↘

Glacial – (Aeolian) – Fluvial↘ ↙

Where is the water?

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INTRODUCTION

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What is the best way to relate both parameters?

Classic geologic mapping

(Voelker et al., 2018)

Grid-mapping

(Voelker et al., 2017)

Voelker – Grid-Mapping Mars

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5/8/2019 18

<20km> <20

km>

(MOLA)

GRID MAPPING

Voelker – Grid-Mapping Mars

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5/8/2019 19

FIDPoly-gons

LTD Gullies Dunes

1 2 1 0 0

2 1 2 1 1

3 0 3 2 0

4 0 3 1 0

Categories

0 Absent

1 Possible

2 Present

3 Dominant

4 No data (MOLA)

(MOLA)

(THEMIS)

(CTX)

GRID MAPPING

Voelker – Grid-Mapping Mars

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5/8/2019 20Voelker – Grid-Mapping Mars

GRID MAPPING

(Voelker et al., 2017)

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5/8/2019 21Voelker – Grid-Mapping Mars

GRID MAPPING – PERSONAL PART!

Why not using machine learning?

- Human experience

- Human creativity

- Human intuition

- Finding new things serendipitously

- High variation of image qualities

- Too diverse selection of landforms; some landforms can be too similar or diffuse

- BUT: Machine learning can be used complementarily

- Getting a human feeling for the study area

(C. D. Friedrich, The Wanderer, 1818)

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5/8/2019 22

Key questions of this work:

- Can geography reveal information about composition/evolution of landforms?

- What climatic information can we derive from the distribution of landforms?

- Is it possible to distinguish climate zones/environments?

- What is the difference between the northern and southern hemisphere?

(ESA/DLR/FUB/Cowart)

Voelker – Grid-Mapping Mars

GRID MAPPING

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5/8/2019 23Voelker – Grid-Mapping Mars

1 2 3

1: Ramsdale et al., 20182: Orgel et al., 20183: Séjourné et al., 2018

GRID MAPPING: NORTHERN LOWLANDS

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5/8/2019 24Voelker – Grid-Mapping Mars

GRID MAPPING: NORTHERN LOWLANDS

DATASETS

- CTX, ConTeXt Camera (visual; 6 m/px)

- MOLA, Mars Orbiter Laser Altimeter

APPROACH

- Grid Mapping acc. to RAMSDALE et al. (2017)

- GIS environment

- Mapping scale 1:10,000 to 1:20,000

- Grid-size 20×20 km

- Focus on periglacial landforms

STUDY AREAS

Region Author Latitudes Landforms

ArcadiaRamsdale

et al., 201830°-80°N 17

AcidaliaOrgel

et al. 201820°-84°N 13

UtopiaSéjourné

et al., 201830°-80°N 11

(Orgel et al., 2018)

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GRID MAPPING: NORTHERN LOWLANDS

RESULTS

Region Author Results

ArcadiaRamsdale

et al., 2018

- Ground ice occurs between 35°-78°N- Volatile-loss from 35°-70°N- Support of airfall hypothesis of LDM

AcidaliaOrgel

et al. 2018

- Identification of 4 landform assemblages:1: Polar cap2: ice-related landforms3: water-related landforms4: irregularly shaped pits

UtopiaSéjourné

et al., 2018

- Identification of 3 landform assemblages:30°-38°N: Polygons, bright mounds, age: 1 Ga38°-47°N: LDM, Scalloped T., polygons (100m), age: 10 Ma47°-78°N: LDM, polygons (30m), age: 1.5 Ma

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5/8/2019 26Voelker – Grid-Mapping Mars

1 2 3

1: Ramsdale et al., 20182: Orgel et al., 20183: Séjourné et al., 2018

GRID MAPPING: SOUTHERN LOWLANDS

Terr

a Si

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No

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Terr

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a

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5/8/2019 27

DATASETS

- CTX (visual; 6 m/px)

- MOLA (elevation, slope, aspect)

- THEMIS (thermal inertia)

- DCI (Dust Cover Index)

- Albedo

METHODS

APPROACH

- Grid Mapping acc. to RAMSDALE et al. (2017)

- GIS environment

- 27 Landforms: (peri-)glacial, fluvial, aeolian

- Mapping scale 1:20,000

- 2 of 3 study areas have been mapped

Voelker – Grid-Mapping Mars

LOCATION OF LANDFORMS PARAMETERS

LARGE-SCALE SYNTHESIS

GOAL

Analysing the distribution of landforms on Mars‘ southern hemisphere by latitude,

topography, and surface properties.

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5/8/2019 28Voelker – Hellas Planitia

MAPPED LANDFORMS

(Peri-)glacial Landforms

Latitude-dependent mantle (LDM) Pedestal craters

Viscous-flow features (VFF) Palimpsests

Scalloped terrain Polygons

Gullies

Aeolian Landforms

Dunes Transversal Aeolian Ridges (TARs)

Ripples Dust

Fluvial landforms

Dendritic channels

METHODS

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5/8/2019 29Voelker – Grid-Mapping Mars

1 2 3

1: Ramsdale et al., 20182: Orgel et al., 20183: Séjourné et al., 2018

RESULTS – NOACHIS TERRA

Terr

a Si

ren

um

No

ach

isTe

rra

Terr

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imm

eri

a

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5/8/2019 30Voelker – Grid-Mapping Mars

(NASA/CTX) (NASA/CTX) (NASA/CTX) (NASA/CTX)

LDM Lower PD Upper PD Scalloped T.

RESULTS – NOACHIS TERRA

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5/8/2019 31Voelker – Grid-Mapping Mars

(NASA/CTX) (NASA/CTX) (NASA/CTX)

Dust VFF Gullies

RESULTS – NOACHIS TERRA

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5/8/2019 32Voelker – Grid-Mapping Mars

Dendritic ch. Rampart crater

(NASA/CTX) (NASA/CTX)

RESULTS – NOACHIS TERRA

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5/8/2019 33Voelker – Grid-Mapping Mars

Desiccated Zone Transition Zone Volatile-rich

Zone

ENVIRONMENTAL ZONES

Process Landforms

Aeolian Dunes, transversal aeolian ridges (TAR), ripples, dust

Fluvial Channels (dendritic)

(Peri)-glacial LDM, scalloped terrain, viscous-flow features, polygons, gullies, pedestal craters, palimpsests

Polar Polar deposits (lower, upper), polar pits, dark material

RESULTS – NOACHIS TERRA

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5/8/2019 34Voelker – Grid-Mapping Mars

RESULTS – TERRA CIMMERIA

Dry Zone Transition Zone Polar Zone

ENVIRONMENTAL ZONES

Process Landforms

Aeolian Dunes, transversal aeolian ridges (TAR), ripples, dust

Fluvial Channels (dendritic)

(Peri)-glacial LDM, scalloped terrain, viscous-flow features, polygons, gullies, pedestal craters, palimpsests

Polar Polar deposits (lower, upper), polar pits, dark material

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RESULTS – NOACHIS TERRA

Voelker – Grid-Mapping Mars

SERENDIPITIES

Funnel-like craters Palimpsests

(NASA/HiRISE) (NASA/HiRISE)

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5/8/2019 36Voelker – Grid-Mapping Mars

1 2 3

1: Ramsdale et al., 20182: Orgel et al., 20183: Séjourné et al., 2018

OUTLOOK

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5/8/2019 37

SUMMARY

Voelker – Grid-Mapping Mars

Key questions of this work:

- Can geography reveal information about composition/evolution of landforms?

→ Yes! The apparent latitude-dependence of landforms suggests a relation to climatic conditions, and hence, the existence or absence of volatiles.

- What climatic information can we derive from the distribution of landforms?

→ There are environments where water- and ice-related landforms are (1) absent (too warm and dry), (2) under erosion (metastable), and stable (cold and “wet” enough)

- Is it possible to distinguish climate zones/environments?

→ There are three environments; Desiccated Zone (0°-30°S), Transition Zone (30°-60°S), and a stable Volatile-rich Zone (60°-90°S)

(ESA/DLR/FUB/Cowart)

QUESTIONS?