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Marine Resources Assessment for the Marianas Operating ... - SPREP

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AUGUST 2005 FINAL REPORT<br />

During La Niña, Guam experiences a deficit in rain during <strong>the</strong> dry and rainy season (86% and 87% of<br />

historical averages, respectively) (Pacific ENSO Applications Center 1995). During June to September<br />

rainfall amounts exceed historical averages (104% of average). The Nor<strong>the</strong>rn Mariana Islands also<br />

experience a surplus of rainfall throughout <strong>the</strong> year during La Niña (104 to 139% of historical averages<br />

with excess rainfall peaking in March, April and May) (Pacific ENSO Applications Center 1995).<br />

2.1.3 Pacific Decadal Oscillation<br />

The PDO is a long-term climatic pattern capable of altering SST, surface wind, and sea level pressure<br />

(SLP) (Mantua 2002; Mantua and Hare 2002). The PDO is a long-lived El Niño-like pattern of Pacific<br />

climate variability and experiences both warm and cool phases. However, <strong>the</strong> PDO has three main<br />

characteristics separating it from ENSO events. First, PDO events can persist <strong>for</strong> 20 to 30 years which<br />

contrasts with <strong>the</strong> relatively short duration of ENSOs (up to 18 months). Second, climatic effects of <strong>the</strong><br />

PDO are more prominent in ecosystems outside <strong>the</strong> tropics. Third, <strong>the</strong> mechanisms controlling <strong>the</strong> PDO<br />

are unknown, while those <strong>for</strong>ces creating ENSO variability have been resolved (Mantua and Hare 2002).<br />

During warm phases of <strong>the</strong> PDO, <strong>the</strong> western tropical Pacific experiences periods of increased SLP while<br />

<strong>the</strong> opposite is true during cold periods of <strong>the</strong> PDO. However, <strong>the</strong> effect of <strong>the</strong> PDO is weak in tropical<br />

areas, such as <strong>the</strong> <strong>Marianas</strong> OPAREA, and thus climatic anomalies are most likely due to ENSO <strong>for</strong>cings<br />

(Mantua 2002; Mantua and Hare 2002).<br />

2.2 MARINE GEOLOGY<br />

The study area is located at <strong>the</strong> intersection of <strong>the</strong> Philippine and Pacific crustal plates, atop what is<br />

believed to be <strong>the</strong> oldest seafloor on <strong>the</strong> planet dating to <strong>the</strong> Jurassic era (Handschumacher et al. 1988).<br />

The collision of <strong>the</strong> two plates has resulted in <strong>the</strong> subduction of <strong>the</strong> Pacific Plate beneath <strong>the</strong> Philippine<br />

Plate <strong>for</strong>ming <strong>the</strong> Mariana Trench (Kennett 1982; Figure 2-1). The Mariana Trench is over 2,270 km long<br />

and 114 km wide. The deepest point in <strong>the</strong> trench and on Earth, Challenger Deep (11,034 m; 11°22’N,<br />

142°25’E), is found 544 km southwest of Guam in <strong>the</strong> southwestern extremity of <strong>the</strong> trench (Fryer et al.<br />

2003).<br />

The seafloor of <strong>the</strong> study area region is characterized by <strong>the</strong> Mariana Trench, <strong>the</strong> Mariana Trough, ridges,<br />

numerous seamounts, hydro<strong>the</strong>rmal vents, and volcanic activity. Two volcanic arcs, <strong>the</strong> West Mariana<br />

Ridge (a remnant volcanic arc than runs from approximately 21°N 142°E to 11°30’N 141°E) and <strong>the</strong><br />

Mariana Ridge (an active volcanic arc) are separated by <strong>the</strong> Mariana Trough (Baker et al. 1996; Figure 2-<br />

1). The Mariana Trough <strong>for</strong>med when <strong>the</strong> oceanic crust in this region began to spread between <strong>the</strong> ridges<br />

as recently as four million years ago. Currently <strong>the</strong> Mariana Trough is spreading at a rate of less than 1<br />

centimeter per year (cm/yr) in <strong>the</strong> nor<strong>the</strong>rn region and at rates up to 3 cm/yr in <strong>the</strong> center of <strong>the</strong> trough<br />

(Yamazaki et al. 1993). The Mariana archipelago is located on <strong>the</strong> Mariana Ridge, 160 to 200 km west of<br />

<strong>the</strong> Mariana Trench subduction zone. The Mariana archipelago is comprised of fifteen volcanic islands:<br />

Guam, Rota, Tinian, Saipan, FDM, Aguijan, Anatahan, Sarigan, Guguan, Alamagan, Pagan, Agrigan,<br />

Asuncion, Maug, and Farallon de Pajaros (listed from south to north) (Figure 2-2). Approximately 800 km<br />

separate Guam from Farallon de Pajaros (Eldredge 1983; DoN 1998; DoN 2003a).<br />

The islands north of FDM are located on an active volcanic arc ridge axis and were <strong>for</strong>med between 1.3<br />

and 10 million years ago (Randall 1985, 1995, 2003; Fryer personal communication). The six sou<strong>the</strong>rn<br />

islands (Guam to FDM) are on <strong>the</strong> old Mariana <strong>for</strong>e-arc ridge axis and <strong>for</strong>med about 43 million years ago<br />

(Eocene) (Randall 1985, 2003; Birkeland 1997). The young volcanic active ridge axis is offset 25 to 35 km<br />

west of <strong>the</strong> sou<strong>the</strong>rn arc ridge axis (Randall 1995). The islands on <strong>the</strong> sou<strong>the</strong>rn ridge consist of a volcanic<br />

core covered by thick coralline limestone (up to several hundreds of meters) (DoN 2003a). The<br />

subsidence of <strong>the</strong> original volcanoes in <strong>the</strong> sou<strong>the</strong>rn islands allowed <strong>for</strong> <strong>the</strong> capping of <strong>the</strong> volcanoes by<br />

limestone. Limestone covers <strong>the</strong> nor<strong>the</strong>rn half of Guam (limestone plateau height: 90 to 180 m above<br />

mean sea level [MSL]) while volcanic rock and clay are exposed on <strong>the</strong> sou<strong>the</strong>rn half of <strong>the</strong> island (DoD<br />

1999). Tinian consists of rocky shoreline cliffs and limestone plateaus with no apparent volcanic rock<br />

(DoD 1999). Similar to Tinian, <strong>the</strong> uplifted limestone substrate of FDM is bordered by steep cliffs (DoN<br />

2004).<br />

2-3

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