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Mars Magnetic Anomalies Mars Magnetic Anomalies

Mars Magnetic Anomalies - PowerPoint Presentation

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Mars Magnetic Anomalies - PPT Presentation

Ester Aranzana 13 de Enero de 2012 Introduction Rock core Fe FeS No internal magnetic field no dynamo action but it has one in the past minimagnetospheres of crustal origin Observations ID: 462292

mars magnetic field vol magnetic mars vol field research geophysical results amp 2001 crustal martian plate tectonics 2005 faults

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Slide1

Mars Magnetic Anomalies

Ester Aranzana

13 de

Enero

de 2012Slide2

IntroductionRock core (Fe-FeS

)No internal magnetic field, no dynamo action but it has one in the past

mini-magnetospheres of crustal origin Slide3

ObservationsMars Global Surveyor(1996)

- MGS MAG: Magnetic vector data sparsely from 400-100 km - MGS ER: scalar field at 180 km

Others: Balloon magnetometer

Rover on Martian surface

Laboratory studiesSlide4

Results

EARTH

MARS

NASA

Magnetic anomalies one order of magnitude higher!! Slide5

Plate tectonics era

Results:

Dichotomy

Strong magnetization requires huge volumes (170-190 km radii, 20-30 km thicknesses)

2 faults

similar to Earth faults with E-W trending features alternating polarity

Connerney

et al. 2005Slide6

ResultsNo magnetic signatures in basins Hellas,

Isydis and Argyre => Shock demagnetization

No magnetic signature in volcanoes provinces (

T

harsis

& Elysium)=>

thermal demagnetization

by intrusions

Harkani-Hamed

2001Slide7

ResultsMini-magnetospheres

above regions with strong magnetized crust.

Brain et al. 2010

Aurorae at different latitudes, first discovered by Mars Express in 2004 above Terra

Cimmeria

(south of Mars)

ESASlide8

Discussion- Cessation of the core field around 4.1

Gyr By cooling of the planet.

- Faults,

lineations

=> Plate tectonics era in presence of a reversing dynamo

- Origin dichotomy: the new mode

is a huge impact Other explanations: Volcanic features, plate tectonics

Roberts et al. 2009

- Internal magnetic field in the past

=>

The evolution of climate and habitability

in MarsSlide9

REFERENCESConnerney,

J.E.P, Acuña, M.H. et al. 2005, Tectonic implications of Mars crustal magnetism, PNAS October 18, 2005 vol. 102 no. 42 14970-14975.

Roberts, J.H., Lillis, R.J., Manga, M. 2009

, Giant impacts an Mars cessation of the Martian dynamo,

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 114, E04009, doi:10.1029/2008JE003287, 2009

Jafar

Arkani

-Hamed 2001, A 50-degree spherical model of the magnetic

field

of Mars

,

JOURNAL OF GEOPHYSICAL RESEARCH, VOL.

106, NO.10, PAGES 23,197-23,208.

Purucker

, M.,

Ravat

, D., Frey, H.,

Voorhies

, C.,

Sabaka

,

T

. &

Acuña, M. 2000,

An altitude-normalized magnetic map of Mars and its

interpretation, GEOPHYSICAL RESEARCH LETTERS, VOL. 27, NO. 16, PAGES 2449-2452.Acuña, M. H., Connerney

,

J.E.P et al. 2001,

Magnetic

field

of Mars:

Summary

of

results

from

the

aerobraking

and

mapping

orbits

,

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 106, NO. E10, PAGES 23,403–23,417

Brain

, D.A., Baker, A.H., Briggs, J.,

Eastwood

, J.P.,

Halekas

, J.S. & Phan, T.D. 2010,

Episodic

detachment

of

Martian

crustal

magnetic

fields

leading

to

bulk

atmospheric

plasma to escape

,

GEOPHYSICAL

RESEARCH LETTERS,

VOL

.37, L14108.

Planetary

Sciences,

Imke

de Pater & Jack J.

Lissauer

, Cambridge

University

Press

2001.Slide10

THANKS

Thank you!!