Magnetic zones of Mars: Deformation-controlled origin of magnetic anomalies

Intense magnetic anomalies over Martian surface suggest preservation of large volumes of very old crust (>3 Gyr) that formed in the presence of a global magnetic field. The global distribution of the magnetic intensities observed above the Martian crust suggests a division into three zones. Zone...

Full description

Bibliographic Details
Main Authors: KLETETSCHKA, G., LILLIS, R., NESS, N. F., ACUA, M. H., CONNERNEY, J. E. P., WASILEWSKI, P. J.
Format: Article in Journal/Newspaper
Language:English
Published: Meteoritics & Planetary Science Archives 2009
Subjects:
Online Access:https://journals.uair.arizona.edu/index.php/maps/article/view/15690
id ftunivarizonaojs:oai:journals.uair.arizona.edu:article/15690
record_format openpolar
spelling ftunivarizonaojs:oai:journals.uair.arizona.edu:article/15690 2023-05-15T18:22:54+02:00 Magnetic zones of Mars: Deformation-controlled origin of magnetic anomalies KLETETSCHKA, G. LILLIS, R. NESS, N. F. ACUA, M. H. CONNERNEY, J. E. P. WASILEWSKI, P. J. 2009-01-01 application/pdf https://journals.uair.arizona.edu/index.php/maps/article/view/15690 eng eng Meteoritics & Planetary Science Archives https://journals.uair.arizona.edu/index.php/maps/article/view/15690/15678 https://journals.uair.arizona.edu/index.php/maps/article/view/15690 Meteoritics & Planetary Science Archives; Vol 44, No 1 (2009); 131-140 1945-5100 1086-9379 Magnetism;Martian origin;Martian dynamo;separation Density info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Peer-reviewed Article 2009 ftunivarizonaojs 2020-11-14T17:53:01Z Intense magnetic anomalies over Martian surface suggest preservation of large volumes of very old crust (>3 Gyr) that formed in the presence of a global magnetic field. The global distribution of the magnetic intensities observed above the Martian crust suggests a division into three zones. Zone 1 is where the magnetic signature is negligible or of relatively low intensity at Mars Global Surveyor (MGS) satellite mapping altitude (400 km). Zone 2 is the region of intermediate crustal magnetic amplitudes and zone 3 is where the highest magnetic intensities are measured. Crater demagnetization near zone 3 reveals the presence of rocks with both high magnetic intensity and coercivity. Magnetic analyses of terrestrial rocks show that compositional banding in orogenic zones significantly enhances both magnetic coercivity and thermal remanent magnetization (TRM) efficiency. Such enhancement offers a novel explanation for the anomalously large intensities inferred of magnetic sources on Mars. We propose that both large magnetic coercivity and intensity near the South Pole is indicative of the presence of a large degree of deformation. Associated compositional zoning creates conditions for large scale magnetic anisotropy allowing magnetic minerals to acquire magnetization more efficiently, thereby causing the distinct magnetic signatures in zone 3, expressed by intense magnetic anomalies. We use a simple model to verify the magnetic enhancement. We hypothesize that magnetically enhanced zone would reside over the down welling plume at the time of magnetization acquisition. Article in Journal/Newspaper South pole Journals at the University of Arizona South Pole
institution Open Polar
collection Journals at the University of Arizona
op_collection_id ftunivarizonaojs
language English
topic Magnetism;Martian origin;Martian dynamo;separation Density
spellingShingle Magnetism;Martian origin;Martian dynamo;separation Density
KLETETSCHKA, G.
LILLIS, R.
NESS, N. F.
ACUA, M. H.
CONNERNEY, J. E. P.
WASILEWSKI, P. J.
Magnetic zones of Mars: Deformation-controlled origin of magnetic anomalies
topic_facet Magnetism;Martian origin;Martian dynamo;separation Density
description Intense magnetic anomalies over Martian surface suggest preservation of large volumes of very old crust (>3 Gyr) that formed in the presence of a global magnetic field. The global distribution of the magnetic intensities observed above the Martian crust suggests a division into three zones. Zone 1 is where the magnetic signature is negligible or of relatively low intensity at Mars Global Surveyor (MGS) satellite mapping altitude (400 km). Zone 2 is the region of intermediate crustal magnetic amplitudes and zone 3 is where the highest magnetic intensities are measured. Crater demagnetization near zone 3 reveals the presence of rocks with both high magnetic intensity and coercivity. Magnetic analyses of terrestrial rocks show that compositional banding in orogenic zones significantly enhances both magnetic coercivity and thermal remanent magnetization (TRM) efficiency. Such enhancement offers a novel explanation for the anomalously large intensities inferred of magnetic sources on Mars. We propose that both large magnetic coercivity and intensity near the South Pole is indicative of the presence of a large degree of deformation. Associated compositional zoning creates conditions for large scale magnetic anisotropy allowing magnetic minerals to acquire magnetization more efficiently, thereby causing the distinct magnetic signatures in zone 3, expressed by intense magnetic anomalies. We use a simple model to verify the magnetic enhancement. We hypothesize that magnetically enhanced zone would reside over the down welling plume at the time of magnetization acquisition.
format Article in Journal/Newspaper
author KLETETSCHKA, G.
LILLIS, R.
NESS, N. F.
ACUA, M. H.
CONNERNEY, J. E. P.
WASILEWSKI, P. J.
author_facet KLETETSCHKA, G.
LILLIS, R.
NESS, N. F.
ACUA, M. H.
CONNERNEY, J. E. P.
WASILEWSKI, P. J.
author_sort KLETETSCHKA, G.
title Magnetic zones of Mars: Deformation-controlled origin of magnetic anomalies
title_short Magnetic zones of Mars: Deformation-controlled origin of magnetic anomalies
title_full Magnetic zones of Mars: Deformation-controlled origin of magnetic anomalies
title_fullStr Magnetic zones of Mars: Deformation-controlled origin of magnetic anomalies
title_full_unstemmed Magnetic zones of Mars: Deformation-controlled origin of magnetic anomalies
title_sort magnetic zones of mars: deformation-controlled origin of magnetic anomalies
publisher Meteoritics & Planetary Science Archives
publishDate 2009
url https://journals.uair.arizona.edu/index.php/maps/article/view/15690
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source Meteoritics & Planetary Science Archives; Vol 44, No 1 (2009); 131-140
1945-5100
1086-9379
op_relation https://journals.uair.arizona.edu/index.php/maps/article/view/15690/15678
https://journals.uair.arizona.edu/index.php/maps/article/view/15690
_version_ 1766202307369762816