T13A-2973
Revised Macquarie-Antarctic plate motion during the last 6 Ma using magnetic anomalies of Australian-Antarctic Ridge near 156°-161°E

Monday, 14 December 2015
Poster Hall (Moscone South)
Hakkyum Choi1, Seung-Sep Kim2 and Sung-Hyun Park1, (1)Korea Polar Research Institute, Incheon, South Korea, (2)Chungnam National University, Daejeon, South Korea
Abstract:
The longest segment of Australian-Antarctic Ridge (AAR), located near 156°-161°E, is the tectonic boundary between the Australian and the Antarctic plates, and meets the Macquarie Triple Junction of Australian-Antarctic-Pacific plates at the eastern end of the segment. In 2011 and 2013, the multidisciplinary mid-ocean ridge program of Korea Polar Research Institute (KOPRI) conducted a series of geological, geochemical, geophysical, and hydrothermal studies at the segment. Especially, in order to determine the detailed location of the ridge axis, a number of short magnetic cross lines were observed in 2013. In 2015, we additionally collected the magnetic data and the high-resolution shipboard bathymetric data for two 400-km long lines across the ridge segment. Here we utilize the observed magnetic data to estimate spreading rates and its temporal changes along the ridge segment. The half-spreading rates computed using MODMAG with our magnetic data range mostly between 28~34 mm/yr. The southern flank of this ridge segment, which has been added to the Antarctic plate as a trailing side between the Australian and the Antarctic plate, tends to have faster spreading rates compared to the northern flank. According to the previous studies, the Macquarie plate, which is regarded as the intra-plate inside the Australian plate and bounded by the northern flank of the ridge segment in this study, has been rotated relative to the Antarctic plate since about 6 Ma. We revised rotation poles between the Macquarie-Antarctic plates for the chron C2Ay (2.58 Ma), chron C3Ay (6.04 Ma) and the other ages additionally, using Hellinger. In this study, we employed the observed magnetic data with additional constraints from the available shipboard measurements. The synthetic flow-line of Balleny Fracture Zone is used as an input to Hellinger, because the region between the Tasman Fracture Zone and the Macquarie Triple Junction is supposed to be included to the Macquarie plate. We examine relevant tectonic adjustments, if any, near the AAR and Macquarie plate using the revised rotation poles.