Catherine Walker | |
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Thesis | Fracture of Antarctic Ice Shelves and Implications for the Icy Satellites of the Outer Solar System |
Doctoral advisor | Jeremy N. Bassis |
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Catherine Walker (Catherine Colello Walker) is an American Earth and planetary scientist [1] at the Woods Hole Oceanographic Institution, where she is on the scientific staff in the Department of Applied Ocean Physics and Engineering. [2] Her research spans fracture mechanics and dynamics in ice, cryosphere change, physical oceanography, and geomorphology on Earth and other planets and moons using a variety of methodologies including remote sensing. [3] [4] [5] [6]
Her scientific contributions include studies of ice shelf rifting [7] and iceberg calving, [8] oceanic drivers of Antarctic ice loss, [9] [10] [11] [12] and the formation of ice fracture and collapse features on Europa and Enceladus. [13] [14] In 2022, she was part of the team that observed the collapse of the Conger-Glenzer Ice Shelf, a first in East Antarctica. [15] [16] [17] She was educated at Mount Holyoke College and the University of Michigan, followed by postdoctoral positions at Georgia Institute of Technology and Caltech/NASA Jet Propulsion Laboratory and a senior fellowship at NASA Headquarters.
Catherine Walker was born in High Point, North Carolina with her twin sister, Cynthia, to parents Cheryl (née Colello), an early childhood educator, and George Walker II, a surgeon. The family moved to North Andover, Massachusetts in the late 1980s. Walker attended North Andover Public Schools, where she developed an interest in science and becoming an astronaut at an early age. [1]
Walker attended Mount Holyoke College, one of the Seven Sisters, and was advised by planetary geologist Darby Dyar. [3] Walker graduated with her B. A. in Astronomy and a minor in Geology magna cum laude. During her undergraduate years, she conducted research at University of New Hampshire, working with space physicist Vania Jordanova analyzing magnetospheric substorms using the NASA/ESA Cluster spacecraft, and space physicist Antoinette Galvin on the pre- and post-launch analyses for the Plasma and SupraThremal Ion Composition (PLASTIC) instrument on NASA's Solar TErrestrial RElations Observatory (STEREO) mission that launched in 2006. [18] In 2007, Walker joined the NASA Academy at Goddard Space Flight Center (GSFC), working on optical instrumentation to observe dust cyclones on Mars with optical physicist Brent Bos. She later joined the GSFC Planetary Magnetospheres Lab, conducting observing campaigns at Kitt Peak National Observatory on Jupiter's moon Io. Walker began the Ph.D. program in Space Physics at Florida Institute of Technology before transferring to the Ph.D. program in Atmospheric, Oceanic and Space Sciences at the University of Michigan.
Walker was advised by glaciologist Jeremy Bassis and her Ph.D. research focused on the geophysics of floating ice, including Ocean World ice shells and terrestrial ice shelves, in particular on the remote sensing of fracture mechanics. Significant contributions from her Ph.D. work included the first circum-Antarctic catalog of ice shelf rifts, [19] [20] ice shell thickness estimates for the South Polar region of Enceladus, [21] and theoretical work spearheaded by Bassis now referred to as the Marine Ice Cliff Instability (MICI). [22] While at Michigan, she also completed coursework towards a Masters' of Engineering in Space Systems Engineering [3] with former NASA Administrator Thomas Zurbuchen.
Walker was a postdoc at Georgia Tech working with planetary scientist Britney Schmidt on terrestrial analogs for Ocean Worlds ice-ocean interactions, and deployed with Schmidt's team to Antarctica to test the Icefin underwater vehicle. Next she was NASA Postdoc Program Fellow at the Jet Propulsion Laboratory working in the Sea Level and Ice Group on marine-terminating glacier change in Antarctica. [23] She moved to NASA Goddard Space Flight Center as a visiting assistant scientist in the Cryospheric Sciences Lab, working with Project Scientist Tom Neumann in the Project Science Office for NASA's ICESat-2 mission. She was awarded a NASA Senior Management Fellowship at NASA Headquarters, working in the Office of the Chief Scientist with James L. Green. Contemporaneously, she served as the Program Officer for the Planetary Instrument Concepts for the Advancement of Solar System Observations (PICASSO) technology development program for in the Planetary Science Division. [24] She is now on the scientific staff at Woods Hole Oceanographic Institution [25] led by Peter DeMenocal, where she works on ice-ocean interactions on Earth and in space. She uses remote sensing (including as part of the ICESat-2 Science Team) and field work, [5] and works on developing technology to explore extreme environments, including diving in HOV Alvin. [26] Most of her work is supported by NASA, [1] in addition to the National Science Foundation (NSF).
An iceberg is a piece of freshwater ice more than 15 meters long that has broken off a glacier or an ice shelf and is floating freely in open water. Smaller chunks of floating glacially derived ice are called "growlers" or "bergy bits". Much of an iceberg is below the water's surface, which led to the expression "tip of the iceberg" to illustrate a small part of a larger unseen issue. Icebergs are considered a serious maritime hazard.
The climate of Antarctica is the coldest on Earth. The continent is also extremely dry, averaging 166 mm (6.5 in) of precipitation per year. Snow rarely melts on most parts of the continent, and, after being compressed, becomes the glacier ice that makes up the ice sheet. Weather fronts rarely penetrate far into the continent, because of the katabatic winds. Most of Antarctica has an ice-cap climate with extremely cold and dry weather.
The Ross Ice Shelf is the largest ice shelf of Antarctica. It is several hundred metres thick. The nearly vertical ice front to the open sea is more than 600 kilometres (370 mi) long, and between 15 and 50 metres high above the water surface. Ninety percent of the floating ice, however, is below the water surface.
An ice shelf is a large platform of glacial ice floating on the ocean, fed by one or multiple tributary glaciers. Ice shelves form along coastlines where the ice thickness is insufficient to displace the more dense surrounding ocean water. The boundary between the ice shelf (floating) and grounded ice is referred to as the grounding line; the boundary between the ice shelf and the open ocean is the ice front or calving front.
In glaciology, an ice sheet, also known as a continental glacier, is a mass of glacial ice that covers surrounding terrain and is greater than 50,000 km2 (19,000 sq mi). The only current ice sheets are the Antarctic ice sheet and the Greenland ice sheet. Ice sheets are bigger than ice shelves or alpine glaciers. Masses of ice covering less than 50,000 km2 are termed an ice cap. An ice cap will typically feed a series of glaciers around its periphery.
The Filchner–Ronne Ice Shelf or Ronne–Filchner Ice Shelf is an Antarctic ice shelf bordering the Weddell Sea.
The Larsen Ice Shelf is a long ice shelf in the northwest part of the Weddell Sea, extending along the east coast of the Antarctic Peninsula from Cape Longing to Smith Peninsula. It is named after Captain Carl Anton Larsen, the master of the Norwegian whaling vessel Jason, who sailed along the ice front as far as 68°10' South during December 1893. In finer detail, the Larsen Ice Shelf is a series of shelves that occupy distinct embayments along the coast. From north to south, the segments are called Larsen A, Larsen B, and Larsen C by researchers who work in the area. Further south, Larsen D and the much smaller Larsen E, F and G are also named.
Iceberg B-15 was the largest recorded iceberg by area. It measured around 295 by 37 kilometres, with a surface area of 11,000 square kilometres, about the size of the island of Jamaica. Calved from the Ross Ice Shelf of Antarctica in March 2000, Iceberg B-15 broke up into smaller icebergs, the largest of which was named Iceberg B-15-A. In 2003, B-15A drifted away from Ross Island into the Ross Sea and headed north, eventually breaking up into several smaller icebergs in October 2005. In 2018, a large piece of the original iceberg was steadily moving northward, located between the Falkland Islands and South Georgia Island. As of August 2023, the U.S. National Ice Center (USNIC) still lists one extant piece of B-15 that meets the minimum threshold for tracking. This iceberg, B-15AB, measures 20 km × 7 km ; it is currently grounded off the coast of Antarctica in the western sector of the Amery region.
Smith Glacier (75°05′S112°00′W is a low-gradient Antarctic glacier, over 160 km long, draining from Toney Mountain in an ENE direction to Amundsen Sea. A northern distributary, Kohler Glacier, drains to Dotson Ice Shelf but the main flow passes to the sea between Bear Peninsula and Mount Murphy, terminating at Crosson Ice Shelf.
Mertz Glacier is a heavily crevassed glacier in George V Coast of East Antarctica. It is the source of a glacial prominence that historically has extended northward into the Southern Ocean, the Mertz Glacial Tongue. It is named in honor of the Swiss explorer Xavier Mertz.
Pine Island Glacier (PIG) is a large ice stream, and the fastest melting glacier in Antarctica, responsible for about 25% of Antarctica's ice loss. The glacier ice streams flow west-northwest along the south side of the Hudson Mountains into Pine Island Bay, Amundsen Sea, Antarctica. It was mapped by the United States Geological Survey (USGS) from surveys and United States Navy (USN) air photos, 1960–66, and named by the Advisory Committee on Antarctic Names (US-ACAN) in association with Pine Island Bay.
Thwaites Glacier is an unusually broad and vast Antarctic glacier located east of Mount Murphy, on the Walgreen Coast of Marie Byrd Land. It was initially sighted by polar researchers in 1940, mapped in 1959–1966 and officially named in 1967, after the late American glaciologist Fredrik T. Thwaites. The glacier flows into Pine Island Bay, part of the Amundsen Sea, at surface speeds which exceed 2 kilometres (1.2 mi) per year near its grounding line. Its fastest-flowing grounded ice is centered between 50 and 100 kilometres east of Mount Murphy. Like many other parts of the cryosphere, it has been adversely affected by climate change, and provides one of the more notable examples of the retreat of glaciers since 1850.
Totten Glacier is a large glacier draining a major portion of the East Antarctic Ice Sheet, through the Budd Coast of Wilkes Land in the Australian Antarctic Territory. The catchment drained by the glacier is estimated at 538,000 km2 (208,000 sq mi), extending approximately 1,100 km (680 mi) into the interior and holds the potential to raise sea level by at least 3.5 m (11 ft). Totten drains northeastward from the continental ice but turns northwestward at the coast where it terminates in a prominent tongue close east of Cape Waldron. It was first delineated from aerial photographs taken by USN Operation Highjump (1946–47), and named by Advisory Committee on Antarctic Names (US-ACAN) for George M. Totten, midshipman on USS Vincennes of the United States Exploring Expedition (1838–42), who assisted Lieutenant Charles Wilkes with correction of the survey data obtained by the expedition.
Ice calving, also known as glacier calving or iceberg calving, is the breaking of ice chunks from the edge of a glacier. It is a form of ice ablation or ice disruption. It is the sudden release and breaking away of a mass of ice from a glacier, iceberg, ice front, ice shelf, or crevasse. The ice that breaks away can be classified as an iceberg, but may also be a growler, bergy bit, or a crevasse wall breakaway.
Glacial earthquakes refer to a type of seismic event, with a magnitude of about 5, resulting from glacial calving events. The majority of glacial earthquake activity can be seen in the late summer and are found in Antarctica, Alaska, and Greenland. About 90% of these occur in Greenland. Glacial earthquakes occur most frequently in July, August, and September in Greenland. Seismographs are analyzed by scientists to identify and locate glacial earthquakes.
Ice mélange refers to a mixture of sea ice types, icebergs, and snow without a clearly defined floe that forms from shearing and fracture at the ice front. Ice mélange is commonly the result of an ice calving event where ice breaks off the edge of a glacier. Ice mélange affects many of the Earth's processes including glacier calving, ocean wave generation and frequency, generation of seismic waves, atmosphere and ocean interactions, and tidewater glacier systems. Ice mélange is possibly the largest granular material on Earth, and is quasi-2-dimensional.
Helen Amanda Fricker is a glaciologist and professor at Scripps Institution of Oceanography at the University of California, San Diego where she is a director of the Scripps Polar Center. She won the 2010 Martha T. Muse Prize for Science and Policy in Antarctica.
Liu Yan is a Chinese Antarctic researcher best known for her work on iceberg calving. She is an associate professor of geography in the College of Global Change and Earth System Science (GCESS) and Polar Research Institute, Beijing Normal University.
Britney Schmidt is an American earth scientist and astrobiologist at Cornell University. She has conducted research on the melting of ice shelves in Antarctica and studied Jupiter's moon Europa.
An ice shelf basal channel is a type of subglacial meltwater channel that forms on the underside of floating ice shelves connected to ice sheets. Basal channels are generally rounded cavities which form parallel to ice sheet flow. These channels are found mainly around the Greenland and Antarctic ice sheets in places with relatively warm ocean water. West Antarctica in particular has the highest density of basal channels in the world. Basal channels can be tens of kilometers long, kilometers wide, and incise hundreds of meters up into an ice shelf. These channels can evolve and grow just as rapidly as ice shelves can, with some channels having incision rates approaching 22 meters per year. Basal channels are categorized based on what mechanisms created them and where they formed.