Reorientation of the early lunar pole

被引:0
|
作者
Takahashi, Futoshi [1 ,2 ]
Tsunakawa, Hideo [2 ]
Shimizu, Hisayoshi [3 ]
Shibuya, Hidetoshi [4 ]
Matsushima, Masaki [2 ]
机构
[1] Kyushu Univ, Dept Earth & Planetary Sci, Fukuoka 8128581, Japan
[2] Tokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
[3] Univ Tokyo, Earthquake Res Inst, Tokyo 1130032, Japan
[4] Kumamoto Univ, Dept Earth & Environm Sci, Kumamoto 8608555, Japan
关键词
CORE DYNAMO; DRIVEN; MOON; MAGNETISM; ORIGIN;
D O I
10.1038/NGEO2150
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Palaeomagnetic measurements suggest that an active core dynamo operated on the Moon from 4.2 to 3.56 billion years ago(1-3). Since the Apollo era, many magnetic anomalies have been observed on the Moon. The magnetization of the lunar crust in some of these regions could preserve the signature of an early dipolar magnetic field generated by a core dynamo. Thus, the magnetic anomalies may yield information about the position of the palaeomagnetic pole during the time that the dynamo operated. Here we present a comprehensive survey of magnetic anomalies on the lunar surface using magnetometer data(4,5) obtained by the Lunar Prospector and Kaguya lunar orbiters. We extract magnetization vectors from 24 magnetic anomalies using an iterative inversion method and derive the palaeomagnetic poles. We find that the north poles, as well as the antipodal south poles, cluster in two distinct locations: one near the present rotation axis and the other at mid-latitude. The clustering is consistent with a dipole-dominated magnetic field generated in the lunar core by a dynamo that was reversing, much like that of Earth. Furthermore, the two pole clusters imply that the Moon experienced a polar wander event during its ancient history due to the reorientation of the Moon with respect to its spin axis by 45 degrees-60 degrees.
引用
收藏
页码:409 / 412
页数:4
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