Evolution of Backarc Rifting: Mariana Trough, 20-24šN Fernando Martinez and Patricia Fryer Hawaii Institute of Geophysics and Planetology School of Ocean and Earth Science and Technology University of Hawaii, Honolulu Nancy A. Baker Department of Geology and Geophysics School of Ocean and Earth Science and Technology University of Hawaii, Honolulu Toshitsugu Yamazaki Geological Survey of Japan, Tsukuba, Japan

Abstract. The Mariana Trough is an actively opening backarc basin in the western Pacific. The trough formed by extension which longitudinally split an earlier arc massif creating a crescent-shaped basin between the remnant West Mariana Ridge and eastern active volcanoes of the Mariana Arc. Opening increases southward from the Volcano Islands near 24^šN where the two arcs join. At 18^šN in the central Mariana Trough the basin is widest and may be opening primarily by seafloor spreading. We present a synthesis of closely spaced shipboard gravity, magnetic, and bathymetry measurements from the northern basin (20-24^šN), an area that undergoes a significant progress ive southward increase in extension. We have identified three stages in the evolution of rifting in this area: (1) asymmetric rifting from 24^šN to 22^š15'N where faulting and magmatism have migrated laterally to remain near the active volcanic arc side of the basin, (2) a "localization" of rifting from 22^š15'N to ~21^šN where the primary zone of rifting separates from the active volcanic arc, and (3) a further concentration of rifting from 21^šN to 20^šN leading to the formation of deep tectonic grabens near the center of the basin. This last stage may be a precursor to (or incipient) seafloor spreading. We describe a new type of magnetic lineation resolved in a three-dimensional seafloor magnetization inversion of the trough between 20^š and 24^šN. The detailed character of these lineations, their association with tectonic structures, and other geophysical observations indicate that they are not seafloor spreading lineations but rather result from magnetic intrusions and volcanism emplaced within preexisting, less magnetic rifted arc crust. The development of these well-defined magnetization bands indicates that the zone of magmatism remains relatively narrow at any one time throughout the opening of the trough, although tectonic deformation appears to be more widely distributed. In addition, the geometry of the magnetization bands with respect to the remnant arc border faults indicates that rifting propagated rapidly northward.

Image: Satellite-derived gravity image of the Izu-Bonin-Mariana area

Image: Bathymetry of the northern Mariana trough 20š-24^šN

Image: Perspective view of the northern Mariana arc and backarc

Image: SeaMARC II sidescan sonar image of the northern Mariana trough.