Paleomagnetism and paleothermometry of the Sydney Basin .1. Thermoviscous and chemical overprinting of the Milton Monzonite

被引:21
作者
Dunlop, DJ
Schmidt, PW
Ozdemir, O
Clark, DA
机构
[1] CSIRO, DIV EXPLORAT & MIN, N RYDE, NSW 2113, AUSTRALIA
[2] UNIV TORONTO, DEPT PHYS, GEOPHYS LAB, TORONTO, ON M5S 1A7, CANADA
关键词
D O I
10.1029/97JB02479
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 [地球物理学]; 070902 [地球化学];
摘要
The Early Triassic (similar to 245 Ma) Milton Monzonite of the Sydney Basin, Australia, has four distinct components of natural remanent magnetization (NRM) with only slightly overlapping ranges of unblocking temperatures. The low-temperature (LT) component, the first to be thermally demagnetized, is thought to be a Late Cretaceous (approximate to 100 Ma) thermoviscous overprint acquired in slow cooling during uplift. The high-temperature (HT) component, the second to be demagnetized, is probably the primary thermoremanent magnetization (TRM) of the Milton intrusion but could possibly be a Jurassic overprint. LT and HT are usually carried by magnetite and occasionally by pyrrhotite. Samples from nine sites have a further NRM component which unblocks at higher temperatures than HT but below the magnetite Curie temperature of 580 degrees C. This component is argued to be a chemical remanent magnetization (CRM) because of its discrete range of high unblocking temperatures, above those of the thermal components HT and LT, and is called CRM1. CRM1 has almost the same direction as LT and is likely carried by authigenic magnetite produced during uplift similar to 100 Ma. Samples from five sites have a fourth NRM component, with a direction resembling that of HT but carried by hematite. This fourth component could be a primary TRM but is more likely a CRM and is therefore called CRM2. The HT-CRM2 mean direction is D= 50 degrees, I= 75.5 degrees, defining a pareopole at 16 degrees S, 172 degrees E. The HT-CRM2 paleopole falls near 150 Ma on the Australian apparent polar wander path but is a considerable distance from paleopoles of Permian and Early Triassic age. There is no known tectonic or other remagnetizing event in the Sydney Basin around 150 Ma. For this reason, we propose that the HT-CRM2 paleopole defines a new Triassic segment of the Australian polar wander path. The LT-CRM1 mean direction is D= 348 degrees, I= -79 degrees, with a paleopole falling at 56 degrees S, 158 degrees E, near 100 Ma on the polar wander path. This age is consistent with uplift and cooling related to initial rifting of the Tasman Sea.
引用
收藏
页码:27271 / 27283
页数:13
相关论文
共 47 条
[1]
[Anonymous], J GEOL SOC AUST
[2]
BOLSHAKOV AS, 1979, B ACAD SCI USSR PHYS, V15, P111
[3]
Branagan D. F., 1976, OUTLINE GEOLOGY GEOM
[4]
ORIGIN OF SECONDARY MAGNETIZATION OF OLD RED SANDSTONES OF ANGLO-WELSH CUVETTE [J].
CHAMALAUN, FH .
JOURNAL OF GEOPHYSICAL RESEARCH, 1964, 69 (20) :4327-+
[5]
THEORETICAL-ANALYSIS OF THERMOMAGNETIC PROPERTIES, LOW-TEMPERATURE HYSTERESIS AND DOMAIN-STRUCTURE OF TITANOMAGNETITES [J].
CLARK, DA ;
SCHMIDT, PW .
PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 1982, 30 (04) :300-316
[6]
CLARK DA, 1996, EOS T AGU S, V77
[7]
CLARK DA, 1996, 318R CSIRO EXPL MIN
[8]
CONNOLLY JR, 1971, AAPG BULL, V55, P2018
[9]
HYSTERESIS PROPERTIES OF TITANOMAGNETITES - GRAIN-SIZE AND COMPOSITIONAL DEPENDENCE [J].
DAY, R ;
FULLER, M ;
SCHMIDT, VA .
PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 1977, 13 (04) :260-267
[10]
HYSTERETIC PROPERTIES OF SYNTHETIC AND NATURAL MONODOMAIN GRAINS [J].
DUNLOP, DJ .
PHILOSOPHICAL MAGAZINE, 1969, 19 (158) :329-&