Deep earthquakes make up approximately one-quarter of all earthquakes, yet current understanding of mechanisms for deep (300-700 km) earthquake generation fails to explain why deep range earthquakes occur. Various mechanisms have been proposed, however, there is a lack of observational constraints on the properties of deep earthquakes, which deters our understanding. In order to progress our knowledge of the deep earth, robust constraints on the mechanisms of deep earthquakes are required. The goal of this project is to explore the mechanism(s) behind deep earthquakes through studying the 2010 Moro Gulf deep earthquake sequence using a continuous back-projection technique. The Moro Gulf sequence features a 'triplet' of earthquakes with hypocentral depths between 585 and 640 km. The triplet earthquakes are particularly unusual, because they are large magnitude events (Mw7.3, 7.6, and 7.4) that occurred within an hour and a half of each other, which does not agree with the Gutenberg-Richter relationship. No other triplet sequences of this magnitude have been recorded within such a short time period. Another anomalous characteristic of these earthquakes is the emergent waveforms of the sequence. Typically, deep earthquakes have impulsive waveforms, which are thought to be associated with more rapid stress drop than shallow events, for which the stress drop occurs more gradually. The back-projection technique is an efficient method to constrain earthquake rupture properties, such as rupture direction, rupture speed, location, timing, and relative energy release of an earthquake. It requires high-quality data from a dense network of seismic stations covering a large area, and we use data from the High-Sensitivity Seismograph Network (Hi-net) in Japan and Australian Network (AU). The technique creates a grid of potential source locations around the hypocenter. The seismograms are time-shifted and stacked at each grid point. The data from the three earthquakes are filtered to a frequency range of 0.8-2 Hz in order to maximize the resolution from the back-projection, and to capture the first arriving P-waves in the waveforms. Back-projection analysis of the Moro Gulf sequence is expected to provide a detailed rupture process of these deep events with high depth and spatial resolution.