David E. King Field Work Award
The David E. King Field Work Award is given annually to one or more full-time graduate students in the Department of Geosciences to support their research. Preference is given to projects that require support for field work. This Award was made possible by a generous gift from former graduate student Mr. David E. King (MS '84). In creating this Award, Mr. King noted that external funding had made it possible for him to conduct field work for his dissertation research. This Award provides a similar benefit for current graduate students.
Applications are available in March with a submission deadline in April. Recipient announced at department convocation in May.
Past Recipients of the David E. King Field Work Award:
The paleoenvironment of Late Cretaceous methane seeps in Western Interior Seaway: A new perspective from carbonate clumped isotope thermometry - Yang Gao (Faculty Advisor - Gregory Henkes)
The so-called “Tepee Buttes” are fossiliferous authigenic carbonate mounds formed around ancient methane seeps preserved within the Pierre Shale Formation of Western Interior Seaway (WIS) during the Late Cretaceous. Previous research had reported extreme depletion of δ 13C in carbonate cements and Ammonite shell fossils at several different locations within the Tepee zone. Such negative δ 13C values in carbonate cements and shells may indicate a high temperature methane-derived carbon source is present during the formation of those carbonates and seep-inhabiting Ammonites. This implies that dissolved inorganic carbon (DIC) generated by anaerobic oxidation of methane, along with ambient seawater DIC, act as significant carbon sources for shell growth in these seep environments. My interest is applying carbonate clumped isotope thermometry to well-preserved authigenic carbonate samples and fossils of Ammonites (Baculites) to better understand the paleoenvironment and paleobiology of the WIS methane seeps.
In order to collect suitable samples for my study, I worked in the field along with the AMNH 2018 paleontology expedition team in South Dakota and eastern Montana. In our team, researchers from five different institutes worked collaboratively to collect well-preserved Ammonite shell fossils and rock samples for paleontological and geochemical studies. We stopped at AMNH excavation sites in Red Shirt, Wall, Hill City, Rapid City in South Dakota, and Glendive in Montana to research different morphologies and fossil types of the region. Most of the sites are very fossiliferous and are in B Compressus zone. After ten days of intense excavation and collection, we accumulated over 30 boxes of usable shell fossils, rock, and sediment samples, which will be stored in the museum and become a valuable resource for collaborating research groups around the country.
Observation of microbial life in modern and Precambrian formations on the Western Australian coast & implications in the search for extraterrestrial life - Ella Holme (Faculty Advisor - Joel Hurowitz)
Understanding the conditions in which microbial life developed on the early Earth is an important step in determining the potential pathways for life to develop on other planetary bodies. Investigating Precambrian rock formations, which are host to some of the oldest traces of life on Earth, can provide crucial insight into the environment and fluid chemistry of the earliest fluid bodies and the microbes they were able to sustain; it is also important to illustrate the evolution of fluid chemistry over geologic time in order to characterize the conditions which allow sustained habitability on long timescales. Several excellent examples of Precambrian formations can be found in Western Australia, including the stromatolite-bearing Fortescue Group and the Dresser Formation, the latter of which houses a newly-discovered geyserite that is the oldest potential evidence of terrestrial life. The coast of Western Australia is also host to the living stromatolites of Shark Bay, which can help to provide context for the formation of stromatolites in ancient rock and create further constraints on the evolution of microbial life from the Precambrian to the modern Earth. Thus, a traverse through the formations of Western Australia has the potential to better inform the astrobiological community on the processes in which habitable environments can be created and maintained through geologic time.
The 2018 Astrobiology Grand Tour, hosted by the Australian Center for Astrobiology at the University of New South Wales, spans approximately 1,700 km of the Western Australian coast, starting with the living stromatolites of Shark Bay and ending in the Pilbara Craton. Other sites of interest include the 1.8 Ga Duck Creek Dolomite, the 2.4 Ga Turee Creek Group, and 2.5 Ga banded iron formation (BIF). This backward hike through Australia’s geologic history will illustrate how depositional environments changed through the Precambrian and the effect of those changes on early life. The focus of this field campaign was providing context for my primary research project, which is concerned with the evolution of Fe-rich water bodies in the Precambrian using the Gunflint Iron Formation. Observing fossil-bearing rocks from a similar time period and deposited from a similar water body is extremely important for interpretation of my own samples and for painting a broader picture of Precambrian ocean chemistry.
This study is aligned with Goal 4 of the NASA Astrobiology Roadmap, which seeks to understand the evolution and persistence of life on Earth, paying specific attention to the response of life to environmental change on a planetary scale. Iron formations such as the Gunflint are associated with oscillation of O2 concentration in seawater, and the effect of these fluctuations on pH in Paleoproterozoic seawater could have had important implications for microbial life in aquatic environments on early Earth. The Gunflint Iron Formation is an example of a banded iron formation, characterized by chert-iron mineral laminations deposited during alternating periods of anoxia and oxygenation in seawater. Its depositional age is 1.88 Ga, as determined by U-Pb dating of zircons from ash beds deposited within the Gunflint. It is well exposed in the Kakabeka Falls region outside of Thunder Bay, Ontario, where our field work was conducted. With the successful completion of the field work, the focus of my work is now on sample characterization and preparation for isotopic analyses. Samples have been and continue to be prepared for petrographic and spectroscopic analysis using thin section equipment available in the SBU Geosciences Sedimentary Petrography Lab. This task is being undertaken with the help of undergraduate student Natalie Crnosija. Thin sections are ground to standard thickness (~30 microns) and are then polished sequentially using Al2O3 grit in grain sizes 15µm, 5µm, 3µm, and 1µm in order to ensure uniform smoothness of the section for Raman analysis. Preliminary results from Raman confirm that siderite is the most abundant carbonate phase, with ankerite appearing as a product of early diagenesis. LA-ICP-MS measurements continue to be collected from a suite of collected samples; primary focus has been on boron concentration and its correlation to major elements Ca, Fe, and Mg, as well as with other trace elements such as Sr and Ce. Initial results indicate that B is generally positively correlated with Fe, indicating that either siderite is a primary carbonate phase that has not experienced diagenetic B loss or that siderite incorporates B very strongly into its mineral.
Our knowledge of Mars and the Moon depends heavily on interpretation of remote data
sets, acquired by satellites and rovers. Making sense of these data sets often requires
comparison with terrestrial locations that exemplify the processes that we observe
on the surfaces of those bodies. Funding by the David E. King Award made it possible
for three graduate students and an undergraduate to travel with me to several world-class
locations in Utah to study planetary analog geological landforms.
The first site explored was inverted channel features near Green River, Utah. These features represent sandstones deposited some 115 million years ago on the floor of a meandering river. The more erosionally-resistant channel sandstones now form narrow, winding ridges that stand above the surrounding shale plains. Similar deposits have been spotted in multiple places locations on Mars, and interpreting them is important for understanding the history of water on the Red Planet’s surface. Walking the outcrop allowed us to correlate large-scale morphologies that are visible from orbit to lithologic boundaries within the inverted channel feature. We also collected samples that will let us study the thermophysical properties of the rocks within these deposits, which will allow us to better identify and characterize Martian inverted channels using the THEMIS instrument onboard the Mars Odyssey orbiter.
We then visited the Upheaval Dome structure in Canyonlands National Park, a heavily eroded example of a complex crater. The deep erosion experienced by this crater allows us to study the processes that occur deep underneath the impact that are generally out of reach in better preserved craters. Complex craters are a common landform on the Moon and Mars, but no landed mission has had the opportunity to study these features up close. In addition to these valuable field sites, we also conducted a geological tour near St. George, UT, to study a range of sedimentary, volcanic, and tectonic processes that may be relevant to the Moon and Mars.
Sedimentary environments explored by rover and orbiter missions provide compelling evidence for liquid water shaping the ancient surface of Mars. However, two conflicting climate models have been proposed to support these findings, (1) a warm and wet environment, and (2) a cold and icy Mars. The argument for the first scenario is supported by the identification of valley networks that are associated with hydrous clays, which on Earth would be comparable to a temperate climate like that of northwestern Idaho. In contrast, climate modelers propose seasonal melting of glaciers as a likely mechanism to produce these sedimentary features. This type of climate is characteristic of Iceland, which was the destination of the 2015 David E. King field award. Honored to receive the award in back-to-back years, the combination of our previous work in Idaho on the Columbia River Basalts (see below for more detailed explanation of our work for the 2014 field season) and the currently funded trip to Iceland will provide a necessary comparison of basaltic sedimentation in varying climates.
The trip to Iceland consisted of a week of exploring the Southwestern region of the country, starting at the glacially fed Lake Hvítárvatn and tracking the outlet of Hvítá River for over 70 km. Sedimentary deposits at point bars, tributary deltas and flood plains were the targets for our sampling locations. The focal point of this research is to determine the chemical and mineralogical changes that occur as you break the source rock down, transport it down stream and then separate it into various grain sizes. This sedimentation process is well known for granitic provenances, but is less understood in basaltic terrains. At the conclusion of our field campaign, we shipped approximately 50 lbs. of sample back to Stony Brook. The analytical work has begun and the main techniques employed will be optical emission spectroscopy and x-ray diffraction. Results from this work will not only fill a knowledge gap in basaltic sedimentation processes but also serve as a valuable terrestrial analog for comparison to ancient Mars.
Source-to-Sink Variations in the Geochemistry and Mineralogy of the Columbia River Basalts: Implications for Chemical and Physical Processes Affecting Planetary Surfaces - Michael Thorpe (Faculty Advisor - Professor Joel Hurowitz)
The surface of Mars is dominated by basalt and its sedimentary record appears to have been strongly influenced by fluvial processes that have resulted in the generation of clastic sedimentary rocks with basaltic compositions. However, basaltic sedimentation is an understudied process on Earth, and as a result, we lack an adequate reference frame to interpret the sedimentary rock record of Mars. Therefore, the objective of this field campaign was to collect samples along the path of a small creek in order to track the geochemical and mineralogical variations that occur during the production of clastic basaltic sediment and sedimentary rocks.
For my field study, I examined the Columbia River Basalts (CRB) by tracing the process of sedimentation in a fluvial system from the rock source to the site of sediment deposition. The CRB is a flood basalt covering 210,000 km2 of the Pacific Northwest, ranging from the Columbia Basin to the Oregon Plateau. Basalts from this region were formed during the Miocene (~16.7 Ma) and experienced episodic pulses of lava flow. The specific area of interest for this investigation was the Lawyer Creek watershed, which carves through the CRB and eventually discharges into the Clearwater River at Kamiah, ID. The Lawyer Creek watershed presents an ideal location to investigate basaltic sedimentation in a relatively short drainage system from its headwaters to its terminus, approximately 40 miles away. Samples collected during my field investigation will be analyzed for bulk geochemistry and mineralogy, in order to generate the first detailed examination of the changes that occur in a source-to-sink basaltic system.
Isotope Systematics of Shocked Feldspar: Implications for Planetary Chronology - Steven
Jaret (Faculty Advisors - Professor Timothy Glotch and Professor Troy Rasbury)
A critical aspect of geochronology is understanding what event measured date reflect. For rocks with complex histories, post-formation processes such as deep burial, tectonics, or contact metamorphism often obscure the original age. For extraterrestrial samples, many samples have been affected by another process, shock metamorphism, which has an unclear affect on radiogenic isotope systems. This study is designed to compare the behavior of argon isotopes after impact events. I will compare 40Ar/39Ar ages of naturally shocked feldspar with impact melt and unaffected target rocks. The goal is to learn whether or not argon ages of highly shocked feldspar can be used as a reliable chronometer for martian, lunar, or meteorite samples.
The purpose of field work at the Ries impact crater, Germany, is primarily to collect crystalline breccias containing feldspar of various composition and shock level. Shock metamorphism is progressive and therefore a key component of this study is comparing the behavior of argon at multiple shock levels.
Ries is a 24-km diameter, complex crater, with a large volume of moderately to highly shocked crystalline material. Ries is one of the most heavily studied terrestrial craters, having a literature base spanning nearly 60 years. It has been well mapped, and both target and impactites have been well characterized petrologically. Furthermore, Ries is the type locality of “suevite,” (aka “impact breccia”) and much of the initial work on terrestrial shocked feldspar was conducted on samples from Ries (von Engelhardt and Stöffler, 1968). Ries also has the advantage of containing both melt-bearing breccias and melt-free breccias. One possibility is that significant heating is required to reset argon isotopes. This can be tested by comparing shocked feldspars in association with melt to those that remained isolated from the melt, because melt-breccias were substantially hotter after impact. Equally important, the impact age is of 15 Ma is significantly younger than the Cretaceous target so it will be obvious if shocked feldspar are reset by the impact.
Developing a more detailed record of sea level shifts by radiometric dating of tuff layers within a well-resolved coral reef stratigraphy in the Late Miocene, Mallorca, Spain - Andrew Kay (Faculty advisor - Professor Troy Rabury)
Significant shifts in Earth's climate took place during the Miocene (ca. 5 – 23 Ma),
particularly in the area of the modern Mediterranean due to the closing of the Tethys
Ocean. These changes culminated in the Messinian Salinity Crisis (ca. 5-7 Ma) during
which the Mediterranean Basin experienced a series of changes in water level resulting
in the deposition of thick layers of evaporites. These sediments have been interpreted
as indicating that during this period the Mediterranean Sea largely dried up and was
refilled with water in a cyclic manner before finally refilling permanently prior
to the modern era. The detailed timing of these events is not well established.
A carbonate platform is the ideal setting for establishing the ages and timing of events because the living component of the reef responds to changes in sea level that result from climatic changes. Volcanic tuffs are present in the sediments associated with the coral reefs of the platform and they can be used for high precision dating to establish a chronostratigraphy. These data will then be used to determine the duration and timing of the different phases of coral reef growth in response to changing sea level.
The field location in Mallorca was selected for this research because there are two Miocene carbonate platforms exposed and their facies architecture and structure are well studied. Samples of tuffs have been collected to permit dating of biotite, sanidine, and zircon, using Ar-Ar and U-Pb dating methods.
The goal of this research project is to explore the mineral physics and petro physics
of upper mantle derived rocks, specifically comparing natural deformation textures
with those produced in laboratory experiments. The Western Gneiss Region of Norway
is one of the best exposed and most extensive ultrahigh-pressure (UHP) metamorphic
terranes in the world. The thermobarometry and thermochronology of the region have
been well characterized. Eclogite ages indicate that there was a major episode of
subduction into the mantle followed by exhumation from UHP conditions during the Caledonian
orogeny roughly 400-420 million years ago. It is inferred that minerals such as garnets,
widespread in the eclogite facies, formed well within the mantle, probably up to depths
of 500 km. The fabrics in these garnet-bearing bodies would be direct indicators of
the rheological mechanisms at depth. This project encompasses collection of peridotite
and eclogite samples located in the coastal areas of the Western Gneiss Region in
Norway, followed by examination of fabrics and textures for direct comparison with
those produced during deformation experiments.
Companion laboratory deformation experiments provide deformation textures in lithologcally similar samples under controlled conditions. Such experiments, however, are limited by their small scale and the difficulty of reproducing slow strain rates that operate inside the earth. Using synchrotron radiation we can simultaneously probe the preferred orientation and strain response during sample deformation in a multi-anvil D-DIA apparatus. Preferred orientation is observed dynamically as changes in peak intensities of various crystallographic planes. The samples are mapped after each experiment using SEM to identify grain boundary development and evidence of recrystallization. These measurements are then combined to help constrain the conditions and mechanisms of plastic flow in the mantle.
Submarine Groundwater Discharge on Long Island's North Shore - Caitlin Young (Faculty
advisor - Professor Gilbert Hanson)
Contributions of submarine groundwater discharge (SGD) to coastal embayments are estimated at ≥ 20% of total surface water inputs. Groundwater nitrogen, a non-point pollution source, discharges into embayments via SGD and may contribute a significant fraction of total nitrogen to surface water bodies such as Long Island Sound. Fresh groundwater traverses the bottom sediments of the embayments and interacts with the overlying saltwater in a zone defined as a subterranean estuary. Investigations in other coastal areas conclude that the subterranean estuary is a highly reactive zone where nitrogen attenuation can occur over 10-50 meter distances during SGD. The aim of this study was to use dissolved N2/Ar measurements to quantify groundwater denitrification during SGD through two subterranean estuaries of Long Island Sound embayments. This study also aimed to determine the spatial extent of SGD in an embayment by combing aerial infrared imagining and 222Radon measurements, which when combined, provide a robust estimate of the fresh fraction (i.e nitrogen rich) inputs of SGD. Results from year 1, which investigated Stony Brook Harbor, indicate that 0-50% of groundwater sourced nitrogen is denitrified during transit through the subterranean estuary when SGD exits at or near the low tide mark. Conversely, a smaller portion of SGD exits through the carbon rich muddy harbor floor, and experiences 80-100% denitrification.
Preliminary year 2 results, using a combination nitrogen porewater profiles, infrared imaging (IR) and 222Radon, indicate maximum discharge rates of nutrient rich groundwater occur along the east and southeast harbor shoreline. Current data analysis yields daily nitrogen discharge rates from SGD into Port Jefferson Harbor exceeds daily nitrogen inputs from sewage treatment plant outfall. Our findings underline the importance of including SGD derived nitrogen inputs in nitrogen mass balance models, utilized to make land management planning decisions that protect coastal waters.
Analysis of Lava Flow Inflation Features and Chemical Weathering Patterns at the Mauna
Iki Vent, Hawaii – Jessica Arnold (Faculty advisor – Professor Timothy Glotch)
Mauna Iki is a small shield volcano on Kilauea's southwest rift zone formed during an eruption spanning from December 1919 to August 1920. The eruptions produced predominantly pāhoehoe lavas, however, 'a'ā and toothpaste lavas were produced as well. Other features observed in the lava field include collapsed lava tubes and sheet collapse pits. This area has several characteristics commonly associated with lava inflation features, including low, but constant effusion rates and shallow slope surfaces. Inflation usually takes the form of either plateaus, which can span hundreds of meters to kilometers, or rounded mounds called tumuli, which are roughly tens of meters in diameter and 1-10 meters in height. Inflation plateaus form extensive sheets without well developed channels or tubes, while tumuli might correspond to lava pathways or tubes, which form beneath the surface and partially inflate. Why one form or another predominates is not well understood and tumuli happen to be the prevalent form at Mauna Iki.
In this project we will collect Differential Global Positioning System (DGPS) topographic data across both types of inflation features and map contacts between different flow textures. These measurements will provide a better understanding of the factors that determine which type of inflationary feature is expressed at a given site and the degree of connectivity between inflation features within the overall flow field. Additionally, this topographic information can aid in identifying and interpreting inflation features on Mars and other planetary surfaces based on remote sensing data.
An additional project goal is to understand the effect that surface textures and weathering rinds have on remotely sensed visible/near-infrared (VIS/NIR) and mid-IR spectra of surfaces. There is evidence from the Alpha Particle–X-Ray Spectrometer on-board the Spirit rover that rocks within Gusev crater on Mars have undergone minor aqueous alteration. Such alteration would be similar to that seen in basaltic lavas within semi-arid regions on Earth, like Mauna Iki's location within the Ka'u desert. Many of the rocks in this region have a very thin (12-18 μm) yellow/orange coating, making the site ideal for VIS/NIR and mid-IR studies of alteration rinds, volcanic glass and their comparison to observed spectra of Martian rocks. Surfaces with the colored coating have markedly different composition from the regular volcanic glass surface. The mid-IR reflectance and emissivity spectra of the collected samples were compared with both Thermal Emission Spectrometer (TES) and Mars Pathfinder data. The Mauna Iki glass was not a good spectral match for Martian basalt as observed by either TES or Pathfinder, with coated surfaces showing a greater dissimilarity. Although the coatings are chemically distinct from the underlying glass, it is not known how much their presence alters estimates of mineralogy based on remote sensing data. The aim of fieldwork at Mauna Iki will be the collection of VIS/NIR, mid-IR and XRF/XRD field data of both coated and non-coated surfaces with varying degrees of weathering from multiple lava flows.
187Re-187 Os Dating of Black Shales from Late Pennsylvanian Cyclothems – Lynnette
Pitcher (Faculty advisor – Professor Troy Rasbury)
The Late Paleozoic experienced one of the most extensive periods of glaciation recognized in Earth's history, and its geologic record illustrates many comparisons to the present-day climate system. It is the only pre-Pleistocene record of extensive glaciations in a vegetated world, sea level was low, it was a time of aragonite seas, and there were high-frequency, high-amplitude cycles (cylothems). Since there is a record of the Late Permian and Mesozoic emerging from this icehouse into the greenhouse world, researchers have turned to this interval to better understand our current climate situation and particularly to more fully address the role of pCO2 on global warming. Recent work on the glacial sedimentary record from Australia and Antarctica is demonstrating that during the late Paleozoic, there were ice-free periods punctuated with intervals of glaciation. It is thought that during the Pennsylvanian (Missourian) the Earth was nearly ice-free; however, some of the best-developed cyclothems from this interval are of Missourian age. Of these Missourian cyclothems the Kansas-type cylothems, located in Kansas, are the most extensively studied alternating stratigraphic sequences of marine and non-marine sediments to date.
This presents us with a conundrum, as most geologists accept that the waxing and waning of Gondwana glaciers is responsible for the changes in sea level, which resulted in the construction of these cyclothems. Currently the age constraints for these deposits are based on global correlation of conodont fossils. Some volcanic ashes have been recognized through this succession, and none are known from the Missourian strata. The 187Re-187Os system in black shales has been shown to be an effective means of dating; recent advances in the technique demonstrate that uncertainties of better than 1% of the age can be obtained. The project under consideration here is for field work in Kansas, through collaboration with Dr. Lynn Watney and Dr. Even Franseen from the Kansas Geological Survey, to sample black shales in cores from the extensive core repository and to examine the black shales in outcrops to obtain a better understanding of the geological setting. The ultimate goal of this research is to be able to estimate the cycle periods and to tie into a global framework with reliable ages. The Master's thesis work will be to establish techniques at Stony Brook for Re-Os dating of black shales and to test the potential for dating core black shales from Kansas.
The Assessment of a Solar Disinfection Method for Water in the Kondoa Region, Tanzania
– Rob Wallace (Faculty advisor – Professor Martin Schoonen)
In sub-Saharan Africa, water-borne diseases pose a serious public health burden because of the lack of safe drinking water. In countries such as Tanzania, E. coli and other bacteria account for as much as 18% of infant deaths. Simple solutions are desperately needed that will provide safe drinking water. One simple, albeit imperfect, solution practiced in countries like Tanzania is solar disinfection. It is common for rural communities in Tanzania to collect water in clear plastic bottles and leave them exposed to the sun for a good part of the day before consumption. The solar exposure has been proven to promote the disinfection of the water, but the role of mineral particulates in the unfiltered water is unknown. My research project seeks to investigate the role of minerals in this solar disinfection process and possibly increase the efficiency of the process by adding specific minerals. As demonstrated in earlier work by Prof. Schoonen's group at Stony Brook, mineral slurries may spontaneously generate hydroxyl radicals, which are known to kill pathogens. By adding specific minerals, it may possible to generate sufficient amounts of OH radical to kill off most of the harmful bacteria.
The first task is to observe the solar disinfection method in practice. Besides observing, I plan to conduct a field count of E. coli bacteria on several waters before and after solar disinfection using the current practice. Although these field counts can be done in situ, it would be preferable to return the samples to Stony Brook University for counting, as it would allow more time to collect samples. We will also measure solar intensity over the duration of the protocol. The field trip will occur winter time in the southern hemisphere. This is when solar intensity is lowest; hence, this is when the efficiency of the disinfection process may be at its lowest and addition of supplemental minerals might be most useful. Samples will be taken of sediment in a hand-dug well to assay which minerals are common in the soil. This will be performed by filtering a sufficient amount of water to collect about 500 mg of material. The filtering will be done by hand over a 0.45 micron filter. The filters will be collected and taken back to Stony Brook for analysis by X-ray fluorescence to determine elemental composition. If sufficient material is available we will also use non-destructive techniques (XRD, FTIR and Raman) to determine the mineral content.
I also plan to collect samples from local rock outcrops to evaluate what other minerals might be available as supplemental materials to boost the efficiency of the process. The focus is on freely available materials that could be easily collected, ground and added to the water. For example, earlier work in Schoonen's group has shown that forsterite and fayalite, as well as freshly ground quartz spontaneously produce OH radicals. If possible, we would take small samples of materials back to Stony Brook for characterization and use in laboratory studies that simulate the solar disinfection process in Schoonen's lab. These laboratory experiments will be conducted using benign strains of E. coli to investigate their viability under conditions similar to those of rural Tanzania.
The Origin of the Calverton Ponds, Long Island – Shungtao Zhang (Faculty advisor –
Prof. Gilbert Hanson)
The Calverton Ponds in Long Island's Pine Barrens are examples of coastal plain ponds. These are small, shallow (only a few feet deep), groundwater-fed ponds that occur on the siliciclastic sands of the Atlantic Coastal Plain. The Calverton Ponds serve as important habitats for rare and endangered Pinelands flora and fauna and contain the highest concentration of endangered and rare species in New York State. Wetlands and ponds are a critical part of the Pine Barrens landscape.
Several studies have focused on the origin of Coastal Plain ponds located in New Jersey (in New Jersey these ponds are called spunges) and in South and North Carolina (Carolina Bays). Proposed explanations for their origin include: freezing and thawing in a periglacial climate during the Late Wisconsinan, with subsequent modification by wind action, mass wastage, and erosion; thermokarst lakes or basins; periglacial wind-action; and even excavation by an extraterrestrial air burst over Canada near the end of the Wisconsinan some 12,900 years ago (as suggested by the discovery of charcoal, vitreous carbon, magnetic spherules and excess iridium in the sediments in the rims of the depressions).
There is no careful study of the origin of the Calverton Ponds located on Long Island. My project will study the origin of these ponds. The method to be used is grain size analysis of sediment collected from the rim of the ponds on Long Island and in New Jersey. For this study I will collect samples in both New Jersey and Long Island and carry out a detailed analysis of grain size. Results will be compared with a grain size analysis of the rim sediments of some of the Carolina Bays from previous studies. If the sediments are well sorted sands then the ponds could represent blow outs formed during the periglacial times after the Wisconsinan glacier receded from Long Island.