Title: Modeling of major martian magnetic anomalies: Further evidence for polar reorientations during the Noachian

Author(s): Hood LL, Young CN, Richmond NC, Harrison KP

Source: ICARUS 177 (1): 144-173 SEP 2005

Document Type: Article

Language: English

Abstract: Maps of the vector components of the Mars crustal magnetic field are constructed at the mapping altitude (360 to 410 km) using a selected set of data obtained with the Mars Global Surveyor magnetometer during 2780 orbits of the planet in 1999. Forward modeling calculations are then applied to six relatively strong and isolated, dominantly dipolar, magnetic anomalies for the primary purpose of estimating bulk directions of magnetization. Assuming that the magnetizing field was a (dipolar) core dynamo field centered in the planet, paleomagnetic pole positions are calculated for the six primary source bodies together with that for a seventh anomaly analyzed earlier. In agreement with several previous studies, it is found that six of the seven pole positions are clustered in what is now the northern lowlands in a region centered northwest of Olympus Mons (mean pole position: 34 degrees +/- 10 degrees N, 202 degrees +/- 58 degrees E). Assuming that the dynamo dipole moment vector was approximately parallel to the rotation axis, the modeling results therefore suggest a major reorientation of Mars relative to its rotation axis after magnetization was acquired. Such a reorientation may have been stimulated by internal mass redistributions associated with the formation of the northern lowlands and Tharsis, for example. A comparison of the mean paleo (magnetic) equator to the global distribution of crustal fields shows that magnetic anomalies tend to occur at low paleolatitudes. The same appears to be true for the Noachian-aged valley networks, which exhibit a broad spatial correlation with the magnetic anomalies. A possible interpretation is that the formation of magnetic anomalies and the valley networks was favored in the tropics where melting of water ice and snow was a stronger source of both surface valley erosion and groundwater recharge during the earliest history of the planet. This would be consistent with models in which hydrothermal alteration of crustal rocks played a role in producing the unusually strong martian magnetic anomalies. (c) 2005 Elsevier Inc. All rights reserved.

Author Keywords: Mars, magnetic fields; Mars, interior; Mars, surface

KeyWords Plus: EARLY MARS; FIELD; CRUST; CONSTRAINTS; VOLATILE; BODIES

Addresses: Hood LL (reprint author), Univ Arizona, Lunar & Planetary Lab, 1629 E Univ Blvd, Tucson, AZ 85721 USA
Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
SW Res Inst, Boulder, CO 80309 USA

E-mail Addresses: lon@lpl.arizona.edu

Publisher: ACADEMIC PRESS INC ELSEVIER SCIENCE, 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA

Subject Category: ASTRONOMY & ASTROPHYSICS

IDS Number: 958XL