Modeling Ice and Water Formations
Introduction:
If one thing bugs me about fantasy, action, and naval movies, it is that icy conditions portrayed always seem to be the same. So here are some tips for bigger and better ice movements and how they should look based on where your shots are taking place across the globe or even extraterrestrial ones.
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Salt vs Fresh Water Ice: What’s The Difference?
It’s all about the salt content.
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Freshwater freezes at 0°C, while seawater's freezing point is below 0°C and varies according to its salinity: the saltier the water, the lower the freezing point. Seawater loses a lot of salt when it freezes, meaning that sea ice has low salinity. Freshwater ice forms more quickly than sea ice. It forms when falling snow accumulates on the bedrock and compresses into ice. This is known as the accumulation zone. Land ice, also called continental ice, is composed of freshwater.
Salt plays a vital role in ocean circulation. In cold, polar regions, changes in salinity affect ocean density more than temperature changes. When salt enters the ocean as sea ice forms, the water's salinity increases. Because salt water is heavier, the density of the water increases, and the water sinks. The salt exchange between sea ice and ocean ice influences ocean circulation globally.
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Ice Formations:
Primary Ice: https://seagrant.umn.edu/news-info/featured-stories/lake-river-ice-formation-classification
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This first layer of ice that forms on any body of water. Depending on water turbulence, it can appear as a clear skim of ice that will thicken over time or a congealed layer of frazil or snow slush. The ice grain size varies from very large when the formation is calm to small when surfaces are turbulent. When the surface is calm, and the temperature gradient is large, crystals can be formed that will be flat or needle-shaped, with crystals as large as a few to several inches.
Secondary Ice: https://seagrant.umn.edu/news-info/featured-stories/lake-river-ice-formation-classification
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This ice formation forms below the primary ice. If the primary ice is precise and uniform, the secondary ice will be crystalline, formed of columns of crystals. If the primary ice is formed under turbulence, the secondary ice will be made up of frazil or snow-slush deposited beneath it. The secondary ice integrates with the primary ice and adds to the overall ice cover.
New Ice: https://seagrant.umn.edu/news-info/featured-stories/lake-river-ice-formation-classification
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This is the first layer of ice formed when bodies of water freeze, similar to primary ice. New ice is a technical term for a thickness of less than 10 centimeters (3.9 inches).
Young Ice: https://ice-glaces.ec.gc.ca/content_contenu/ice_codes/pop_ups_youngice_eng.html
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As the ice thickens, it enters the young ice stage, defined as ice 10 to 30 centimeters (3.9 to 11.8 inches) thick. Young ice is sometimes split into two subcategories based on color:
Gray ice (10 to 15 centimeters, or 3.9 to 5.9 inches thick)
Grey-White Ice: https://ice-glaces.ec.gc.ca/content_contenu/ice_codes/pop_ups_greywhiteice_eng.html
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Gray-white ice is 15 to 30 centimeters or 5.9 to 11.8 inches thick.
MultiYear Ice: https://nsidc.org/learn/cryosphere-glossary/multiyear-ice
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Multiyear ice has survived a summer melt season and is much thicker than younger ice, typically ranging from 2 to 4 meters thick.
Snow Slush: https://wxguys.ssec.wisc.edu/2016/01/11/whats-really-going-on-in-that-slush-puddle/
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This is surface slush from ice crystals formed in icy water by snow particles.
Sludge: https://www.netsolwater.com/what-is-sludge.php?blog=1366
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This dense layer of frazil forms at the water's surface. Like frazil, sludge gives the water a dull appearance because it scatters light. Slush sometimes takes on a spherical form when clumps of viscous slush or frazil are processed by wave action rolling them. The slush in these balls then sticks together.
Snow Ice: https://nsidc.org/learn/parts-cryosphere/snow/science-snow
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It was formed over the top of the primary ice by freezing snow wetted by external water inflow or melting from warm weather or intense sun. If it is thick enough, the freezing of the top of the snow slush may leave a layer of snow slush between it and the primary ice.
Superimposed Ice: https://www.britannica.com/science/superimposed-ice-zone
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This Ice forms on top of the primary ice layer through flooding of the ice surface by water from sources such as stream inflow, meltwater, and groundwater discharge above the water surface. Superimposed ice will freeze at the surface, sometimes leaving a slush layer.
Frazil Ice: https://en.wikipedia.org/wiki/Frazil_ice
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Frazil is small needle-ice particles that form at the water surface when the temperature above the water is below freezing. These particles are smaller than about one inch. They stick to each other in icy water and form slush, which then freezes into primary ice. Frazil scatters light and gives the water a dull appearance.
Anchor Ice: https://en.wikipedia.org/wiki/Anchor_ice
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Anchor ice usually forms undercurrents or stream flow when cooled pieces of frazil(soft or amorphous ice) stick together, forming a bottom layer of ice. This is usually formed in streams and rivers when water is supercooled, but can also form in lakes. Anchor ice transports sediment, which can destroy power generation, human-made structures, and habitat.
Ice Balls: https://www.geographyrealm.com/how-ice-balls-form/
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Ice balls form on beaches. These can be up to the diameter of a soccer ball and can be made of ice or ice covered in sand and sediment. They are formed as slush balls by wave action and arrive on the beach by waves.
Brash ice: https://www.antarctica.gov.au/about-antarctica/ice-and-atmosphere/sea-ice/pack-ice/brash-ice/
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These are floating pieces of broken ice, usually less than about 6 feet across.
Candle Ice: http://lakeice.squarespace.com/candled-ice/;jsessionid=4E62CB159AE1949B54802BB4CC6EF8E0.v5-web010
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Candle ice is rotten ice that leaves long, thin crystals as it melts. It is usually found when primary ice melts and is formed under icy conditions. Based on wind patterns, candle crystals can be vertical or horizontal. If the candle crystals are vertical, the ice surface appears white; if they are horizontal, the ice appears darker. Vertical candle crystals are stronger than horizontal ones.
Frost Smoke: https://www.sciencephoto.com/media/164911/view/-frost-smoke-rising-from-the-sea-off-ross-ice
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Sometimes called “lake smoke,” it is caused by cold air coming into contact with warm water in gaps in ice. If the temperature is freezing, the moisture may be composed of tiny ice crystals. Frost smoke can create clouds and is associated with lake-effect snow in the Great Lakes.
Ice Rind: https://seagrant.umn.edu/news-info/featured-stories/lake-river-ice-formation-classification
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This crust of ice forms from freezing sludge on calm water surfaces. It is usually less than a few inches thick.
Pancake Ice or Ice Pans: https://weather.com/science/weather-explainers/news/pancake-ice-science-behind
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These are rounded pieces of ice frozen from snow or frazil balls that have repeatedly collided with other pieces of ice. These are usually less than 2 feet in diameter.
Plate Ice: https://seagrant.umn.edu/news-info/featured-stories/lake-river-ice-formation-classification
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These are Thin ice pieces formed under calm weather conditions. These are small and look like thick, broken plate glass.
Rotten Ice: https://en.wikipedia.org/wiki/Rotten_ice
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This is melting ice that has lost its integrity. It can have a honeycomb appearance.
Floe Formation: https://www.britannica.com/science/ice-floe
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Pancake ice forms into sheet ice, fusing to form sea ice.
Fast Ice and Drift Ice: https://www.antarctica.gov.au/about-antarctica/ice-and-atmosphere/sea-ice/fast-ice/fast-ice-types/
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https://en.wikipedia.org/wiki/Drift_ice
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Fast ice is fixed and remains where it forms, often along coastlines. Drift ice, meanwhile, is carried by the currents.
Ice Free Areas: https://www.bas.ac.uk/media-post/climate-change-may-cause-expansion-to-ice-free-areas-across-antarctica/
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Ice-free areas called polynyas can form within sea ice near coastlines.
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River, Lake, Sea, and Ocean Ice:
River Ice
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Ice formation in rivers is a complex process. It is more complex than lake ice in its development. Mainly because of the way the water velocity and turbulence of the water flow. In lakes, the surface temperature drops in response to cooling by the air above. The turbulent mixing in rivers causes the water depth to cool uniformly even after its temperature has fallen below the temperature of maximum density (4° C, or 39° F). This is where all known substances undergo thermal expansion in response to heat.
Once the water temperature drops to the freezing point and further cooling occurs, it will fall below freezing in a process known as supercooling. Ice particles from the air cause further ice nucleation in the flow. This initial process forms a crystal from a solution, a liquid, or a vapor. Then, the water temperature returns to the freezing point. Ice production then matches the cooling rate occurring at the surface.
The supercooling of river water allows ice particles to stick to one another since ice particles are unstable and actively grow in supercooled water. They stick to each other by freezing when they touch surfaces and other particles cooled below the freezing point. In rivers and streams, frazil particles can stick to the bottom of the water and build up a loose, porous layer known as anchor ice. The particles will not stick to one another if the water temperature rises above freezing. Anchor ice usually forms on the bottom of shallow streams at night, when cooling occurs, and is only released under the influence of air temperature and solar radiation.
Temperature and turbulence are the two most essential factors determining how ice forms. Temperature is controlled by climate, and turbulence is affected by the size of the water body and the materials that make up that water body. Turbulence in streams is driven by the speed of water and the kinds of materials forming the stream’s channel. Bumpy materials result in more turbulence. Turbulence can also be high in large lakes when the wind can blow over the water surface for large distances and create waves and currents.
The first particles of ice in the water flow are called frazil ice. Or P3 (Primary 3). P3 ice forms in rivers with enough turbulence to mix the supercooled water to much deeper depths, often to the bottom. The turbulence is effective at removing heat from growing crystals. These particles are typically about 1 millimeter (0.04 inch) or smaller in size and usually in the shape of thin disks. Frazil appears in several types of initial ice formation in several different forms. This can include thin, sheetlike formations, ice particles that appear in larger masses, and ice particles that exhibit a slush-like appearance on the water surface.
Frazil Ice forms into pans on the surface of rivers. It is also a prevalent ice type found throughout all ice formations. These pans merge and freeze to form larger floes(a sheet of floating ice) or gather at the leading edge of an ice cover, forming an ice layer that progresses upstream. The thickness of the ice depends on the velocity of the river flow. The forces exerted by the water flow and its weight acting in the downstream direction will thicken the ice by shoving it.
As the ice cover accumulates and progresses upstream, it adds resistance to the flow and displaces water. These effects cause the river's depth to be greater upstream, reducing the velocity and enabling further upstream progression of the ice. This phenomenon is called staging by its effect of increasing the water level or “stage.”
Example of Staging: https://www.britannica.com/science/staging-ice-formation
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Once the first ice cover has formed, columnar crystals grow into the water below, forming a smooth bottom surface. An exception to this arises when above-freezing water flows beneath the ice cover. When this occurs, the moving water either causes the undersurface to melt or reshape. In some rivers, fixed ice formation occurs along the shorelines. The shore ice then gradually widens from the shoreline.
In deeper rivers, frazil produced upstream can be carried downstream and transported beneath fixed ice covers, where it may be deposited and form accumulations of ice called hanging dams. These deposits may block portions of the river’s flow. Ice formations in smaller, shallower streams may be combinations of shore ice, anchor ice deposits, small hanging dam-like accumulations, and sheet ice.
Ice in smaller streams shows more variation through the winter since most of the water comes from groundwater inflows during periods of rain. Groundwater is warm and, over time, melts the ice formed during freezing periods. At other times, it forms large ice buildups. These are called icings, Aufeis, or naleds.
As winter progresses and air temperatures rise above the freezing point, river ice melts from the heat from above and the action of the warm water flowing beneath. The turbulent water on the undersurface causes a melting pattern as the waves become oriented crosswise to the current direction. This is a standard process for both deep and shallow rivers.
During the spring periods of midwinter, thaw causes additional runoff from snowmelt and rain and increases the flow in the river. The increased flow raises the water level and breaks the ice loose from the banks. It also increases the forces exerted on the ice cover. If these forces exceed the strength of the ice, the cover will move, break up, and be transported downstream. In some places, the quantity of ice will exceed the river's capacity, and an ice jam will form. The jam may then raise the water level and cause flooding. Rivers also break up in response to runoff from snowmelt or rain.
Sea Ice
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Sea ice is where things get tricky, as salt becomes an additive factor. Sea ice and ocean ice go hand in hand, as each body of water contains salt and flows in and out of the other.
Sea ice grows and melts in salty ocean water, which sets it apart from icebergs, glaciers, lakes, and river ice. Icebergs and glaciers form from snow falling on land, while lake and river ice form from fresh water. Lake ice tends to freeze as a smooth layer, while sea ice develops into various shapes because of the turbulence of ocean water. Sea ice is vital for several reasons: it is an essential habitat for many species, protects coasts from erosion by acting as a barrier against storms and waves, and sustains Arctic Inuit populations, who depend on it for hunting, livestock farming, and fishing.
As sea ice crystals form, the salt is excluded. Sea ice contains much less salt than seawater. The older the sea ice, the lower its salt concentration. Sea ice loses its salt content over time. About 20% of the salt remains trapped in pockets of water between the ice crystals. As ice forms and the salt is excluded, the salinity of the remaining water increases. These unfrozen pockets of salty water make sea ice softer and slushy than freshwater ice, which is rigid. Sea ice is not uniformly smooth but is a surface that varies dramatically across short distances. Most sea ice features occur when sea ice either converges or spreads out.
Sea ice does not generally grow and melts in a single place. Instead, it is constantly moving and changing location. Only in places near the coast, where ice can attach to the coast or shallow shelf region, is it pinned in place and does not move.
Seawater begins to freeze at about –1.8 C, a lower temperature than fresh water. Ice formation begins at the surface with tiny needle-like ice crystals called frazil, which accumulate and make the water appear slushy and cloudy.
When frazil forms, highly saline water accumulates into brine droplets, typically expelled back into the ocean. The salinity of the surface water then rises. Some brine droplets become trapped in pockets between the ice crystals. The brine remains liquid because much cooler temperatures would require it to freeze. At this stage, the sea ice has a high salt content.
However, Over time, the brine drains out, leaving air pockets, and the salinity of the sea ice decreases. This stage is called grease ice. In calmer water, these tiny crystals can freeze together into a thin surface layer called nilas, reaching a thickness of up to 10 cm.
Wave action can break up the nilas into small pieces. These bump into each other and form rounded shapes with raised edges, called pancake ice. If temperatures remain cold, the pancake ice freezes into solid ice floes, hard surfaces covering the ocean. Ice floes then freeze together into ice fields.
Wind, ocean currents, and other forces push sea ice around, ice floes collide, and ice piles into ridges and keels. Ridges are small “mountain ranges” that form on top of the ice; keels are the corresponding features on the underside of the ice. The total thickness of the ridges and keels can be several meters, and the surface ridges can easily be 2 meters or higher.
Ridges: https://en.wikipedia.org/wiki/Pressure_ridge_(ice)
Sea Ice Keel: https://www.researchgate.net/figure/Sea-ice-keel-left-and-iceberg-keel-right_fig63_334458575
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Ridges are blocky with very sharp edges. Over time, during the summer melt, the ridges erode into smaller, smoother “hills” of ice called hummocks. This process is similar to the erosion of mountain peaks into smooth, rolling hills but at an accelerated pace. When keels erode into smooth features, they are called bummocks.
Once ice floes form, the water underneath becomes insulated, and heat loss to the atmosphere declines, so the water no longer cools, and no more ice formation occurs. Young sea ice is usually relatively thin, not more than 3-4 m thick. The ice can get thicker through precipitation, but due to the low temperatures, whatever does occur tends to accumulate. The accumulated ice and snow add to the overall thickness of the sea ice.
During the ice formation, Brine moves out of sea ice in various ways. Brine (or salted water) is water with a high-concentration salt solution. The brine migrates downward through holes and channels in the ice and empties back into the ocean. The other way is that the ice will compress surrounding the brine and break the brine pockets, allowing the brine to escape to the ocean.
The sea ice melts throughout the seasons, especially during the summer, forming small freshwater ponds called melt ponds. This freshwater travels through the cracks and holes in the ice, washing away the remaining brine. When the sea ice surface cools, brine increases in salinity to the point where it can melt the undersides of the existing ice. This leads to a downward brine migration, allowing the substance to escape into the ocean below the ice sheet.
When large sheets of sea ice are formed, they exist in two forms: fast or land-fast ice. Land-fast ice refers to the large, solid ice sheets attached to land. Pack ice consists of smaller, free-floating pieces of sea ice. They either formed independently or broke off from fast ice.
Pack ice is also subject to the currents flowing underneath, and the ice sheets are constantly moving, breaking up, or being pushed together. When pieces of ice converge, they buckle and crack or override one another as convergent lithospheric plate boundaries. These collisions can create tall, jagged pressure ridges that extend for several kilometers.
Pack Ice: https://www.britannica.com/science/pack-ice
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Snow also plays a massive role in regulating sea ice formations. Snow covers sea ice and insulates it. The insulation slows ice growth in the winter and delays melting in the summer. The snow is usually dry and hard-packed. If snow cover is thick, over-thin sea ice, the weight of the snow can push the ice down into the water below. The salty ocean water will flood the snow, creating a slushy layer. This flooded sea ice is more common in the Antarctic than in the Arctic because Antarctica has thinner ice and more snowfall.
During summer, as the snow on top of sea ice melts, the meltwater accumulates in depressions on the sea ice surface called melt ponds. These ponds absorb more heat from sunlight than the surrounding sea ice and grow in area and depth. The fresh water in melt ponds appears blue because light reflects and scatters off the sea ice surface from the bottoms and sides of the melt pond. If a pond melts through the entire thickness of the ice, the pond's color turns dark, like the ocean. Melt ponds are more common in the Arctic than in the Antarctic because Arctic ice lasts longer and Arctic sea ice has an uneven surface, giving melt ponds places to form.
Features on sea ice's surface include frost flowers and ice crystals deposited when water vapor bypasses the liquid phase and becomes a solid. Frost flowers roughen the surface and alter its electromagnetic signal.
Frost Flowers: https://en.wikipedia.org/wiki/Frost_flower_(sea_ice)
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Sea ice has an albedo than many other Earth surfaces. Albedo is a quantity that indicates how well a surface reflects solar energy. Albedo is measured in values between 0 and 1. Albedo commonly refers to the “whiteness” of a surface, with 0 meaning black and 1 meaning white. A value of 0 means the surface is a “perfect absorber” that absorbs all incoming energy. A value of 1 means the surface is a “perfect reflector” that reflects all incoming energy. An ocean albedo is approximately 0.06, while bare sea ice varies from 0.5 to 0.7. This means the ocean reflects only 6 percent of the incoming solar radiation and absorbs the rest, while sea ice reflects 50 to 70 percent of the incoming energy.
The sea ice absorbs less solar energy and keeps the surface cooler. Snow has a higher albedo than sea ice. Thick snow-covered sea ice reflects as much as 90 percent of the incoming solar radiation. This insulates the sea ice, maintaining cold temperatures and delaying ice melt in the summer. After the snow starts to melt, melt ponds may form. As the melt ponds grow and deepen, the albedo decreases, leading to higher absorption of solar radiation and an increased melting rate.
Sea ice growth mainly starts in autumn when incoming solar energy decreases, and air temperatures fall below freezing. Ice growth continues through the winter, and the ice becomes thicker as heat transfers from warm oceans to the cold atmosphere. Sea ice is continually in motion, except in coastal regions where ice grows out from and stays attached to the shore like fast ice. The motion of ice results from a balance of forces defined by Newton's Second Law, which states that force equals mass times acceleration.
Sea ice is classified by stages of development related to thickness and age. The classification process categorizes sea ice into two primary age groups: first-year and multiyear. The seawater ice process starts in an icey, dense, salty water stage that leaks from the ice and sinks. This brine is “supercooled”; it is cooled below the usual freezing point of seawater but remains liquid due to the salt content. Sheets of sea ice form when frazil crystals float to the surface, accumulate, and bond together. This process often expels salty water in “brine pockets.” When supercooled brine comes into contact with the surrounding water, it causes the water around it to freeze, creating ice stalactites, or “brinicles,” that can be several meters long, and the brinicle grows downwards.
First-year sea ice forms in winter, when temperatures are at their lowest. When temperatures rise, the seasonal sea ice melts in a process known as the breakup. First-year sea ice is about 1 to 2 meters thick. There is also multiyear sea ice that does not melt yearly and can be several meters thick.
Multiyear ice has distinct properties that distinguish it from first-year ice. It contains much less brine and more air pockets than first-year ice, which means “stiffer” ice. Less brine also means that multiyear ice is much fresher, containing minimal salt. Multiyear ice often supplies the freshwater needed for polar expeditions.
Multiyear ice is more common in the Arctic than in the Antarctic. Ocean currents and atmospheric circulation move sea ice around Antarctica, causing most ice to melt in the summer. Most of the multiyear ice that does occur in the Antarctic persists because of a circulating current in the Weddell Sea on the eastern side of the Antarctic Peninsula.
Multiyear ice has declined significantly in the Arctic in recent times. The first major complete recording of ice flow began in 1984. The first substantial drop in multiyear ice occurred from the late 1980s through about 1995. The leading cause was a positive Arctic Oscillation, which set up a wind circulation pattern that pushed multiyear ice out of the Arctic from the Beaufort Sea region through Fram Strait, east of Greenland. From 2007 to 2023, multiyear ice has remained lower than pre-2005 levels, and the overall trend is downward due to global warming.
Five principal forces act on sea ice. The first one is the most important: wind. Wind is the primary force responsible for ice motion, particularly on the timescale of days or weeks. Wind blowing on the top surface of the sea ice results in a drag force on the ice surface, which causes the ice to drift. The amount of the force depends on the speed of the wind and the characteristics of the sea ice surface. The wind affects rough ice surfaces more than smooth surfaces.
The next is ocean currents. An ocean current force acts opposite to the wind force and drags on wind-driven sea ice motion. Currents are essential in longer-term ice motion.
The Coriolis force causes objects to accelerate because of Earth's rotation. The Coriolis force is small at scales of tens to hundreds of kilometers, but it does affect processes that occur at the global scale, such as ocean currents, winds, and ice motion. In the Northern Hemisphere, the Coriolis force causes objects to deflect to the right, and in the Southern Hemisphere, objects deflect to the left. The Coriolis force barely exists at the equator, and because the force increases toward the poles, it plays a vital role in determining sea ice motion.
Internal ice stress measures the strength of the ice. Like the ocean current force, internal ice stress usually acts as a resistance to the motion caused by the wind force. Under circumstances when the sea ice pack is loosely compacted and can flow freely, the internal ice stress is minimal. When the ice is compact and cannot flow, the internal ice stress can be high. For example, ice motion is significant with a strong onshore wind. If the strong wind pushes thick, compact ice toward a shore, there may be little or no motion because the ice has nowhere to go.
Internal ice stress is also vital in deformation and features, such as ridges and leads. Sea ice is susceptible to tension forces. When the ice is “pulled apart” by winds or currents from opposite directions, the ice easily fractures and forms lead. Sea ice is also much stronger under compression forces. When the ice is pushed together by converging winds or currents, the internal ice stress keeps the ice from moving together, but if the ice is pushed together hard enough, the ice will “fail,” or break apart, and pile up into ridges.
The strength of ice depends primarily on its thickness. Thin ice breaks apart easily under compression, while thick ice is much stronger. The formation of ridges can create piles of sea ice many meters thick. Internal ice stress also depends on brine content, temperature, density, and other factors.
The relationship between thermodynamics and sea ice thickness is related to freezing degree days (FDD), which measure how cold it has been for how long. The cumulative FDD is simply the daily degrees below freezing summed over the days the temperature was below freezing.
Ice thickness increases at a rate roughly proportional to the square root of the cumulative FDD. Snow cover dramatically alters sea ice thickness. Snow is an effective insulator, slowing heat transfer from the ocean through the ice and to the atmosphere. Because of this, snow essentially slows the growth of ice.
Sea-surface tilt can also have a noticeable effect on sea-ice motion. The ocean surface is not perfectly flat. Even if the ocean were completely still, it would consist of high and low regions caused by slight differences in gravity. This undulating surface is called a geoid. Because the ocean is never at rest, the surface is higher than the geoid in some regions and lower in others.
Several factors contribute to ocean surface-level differences, including uneven heating, salinity variations, and currents. Differences in surface level result in sea-surface tilt, a force that influences ice motion.
Another thing to note is that Antarctic large-scale sea ice circulation is generally clockwise around Antarctica. There is also an average northward component, so sea ice gradually moves towards the northern ice edge after it forms. Compared to the Arctic, the Antarctic has no surrounding land boundary for the northward-flowing sea ice to run into, so the ice flows northward until it melts in warmer oceans and air temperatures.
Ocean Ice
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Similar to Sea Ice, As ocean water freezes, it forms frazil. Because salt does not freeze, the crystals expel salt into the water, and frazil crystals consist of fresh water. In calm waters, frazil crystals form smooth, thin ice, called grease ice, for its resemblance to oil slicks. This is the same process that occurs in sea ice.
In rough ocean waters, ocean frazil crystals also accumulate into pancake ice; if the motion is strong enough, thin sheets of ice slide over one another in a process known as rafting. If the ice is thick enough, ridging occurs, where the sea ice bends or fractures and piles on top of itself. Each ridge consists of above-the-surface ice, called a sail, and keels. Because of the difference in density between the ice and the water, most of the ice in a ridge is below the surface. Keels are about nine times thicker than sails. In the Arctic, ridges up to 20 meters (66 feet) thick can form when thick ice deforms.
Like sea ice, the salinity of the water is essential to the freezing process. Salinity is a measurement of the concentration of dissolved salts in water. A common way to define salinity values is now c described in practical salinity units (PSU). The average salinity of the ocean typically varies from 32 to 37 PSU, but in polar regions, it is less than 30 PSU. Sodium chloride (table salt) is the most abundant of the many salts found in the ocean.
Fresh water freezes at 0°C (32°F), but the freezing point of seawater varies. The Arctic Ocean is generally fresher than other oceans, somewhere between 30 and 34 PSU, but salinity levels vary by region, and areas with solid river inflow have even lower salinity.
Now, for some ocean ice characteristics, we will start with leads.
Leads are narrow, linear cracks in the ice that form when ice floes diverge or shear as they move parallel in oceans. The formation of leads is similar to mid-ocean ridges or shear zones that form from Earth's moving tectonic plates. The width of leads varies from a couple of meters to over a kilometer. Leads can often intersect, creating a complex network of linear ice features extending over hundreds of kilometers.
Leads are much darker than surrounding ice, which, during the summer, results in a lower ability to reflect light. Lower reflectivity leads it to absorb more solar energy than the surrounding ocean, which heats the water in the leads and speeds up the melting of surrounding ice. In summer, leads remain open and expand or close if winds and ocean currents push the surrounding ice together. Leads forming in winter will generally start to refreeze very quickly, and this refreezing process adds salt to the open ocean layer. While the lead remains open in winter, it releases heat and moisture into the atmosphere. Leads are also crucial for wildlife. Seals, whales, penguins, and other animals rely on leads for access to oxygen. Polar bears in the Arctic often hunt near leads because they know their prey will likely come to the surface to breathe in such areas.
Lead Ice: https://en.wikipedia.org/wiki/Lead_(sea_ice)
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Another characteristic of ocean ice is that of Polynyas. Polynyas exist both in oceans and in seas. They are persistent open-water areas, oval or circular holes where the water remains open because of processes that prevent sea ice from forming or quickly moving out of the region. There are two types of polynyas, open and coastal polynyas, which are classified by their various mechanisms of ice reduction.
Sensible-heat (open-ocean) polynyas happen when heat transfer occurs between two bodies at different temperatures that are in contact with each other. The body with the higher temperature transports sensible heat to the body with the lower temperature. A sensible-heat polynya forms when water above freezing upwells or moves from the ocean's lower depths to the surface. Heat transfers from the warmer water to the ice, melting it and preventing new ice from forming. The topography of the ocean bottom or overturning of water causes the warm water to rise to the surface. Sensible-heat polynyas usually form in mid-ocean areas.
Polynyas: https://mallemaroking.org/amundsen-sea-polynya/
Latent-heat (coastal) polynyas have heat transfer that occurs when their matter changes state. Latent heat is absorbed when ice melts and released into the surroundings when liquid water freezes. The process is called “latent” because it is not associated with a temperature change but a state change.
A latent-heat polynya is characterized by ocean water when it reaches its freezing point. It forms due to persistent winds pushing the ice away from a barrier, such as a coast, fast ice, a grounded iceberg, or an ice shelf. As new ice grows within polynyas, the wind blows it to the leeward side while the windward side remains ice-free. Latent heat is released as water freezes and evaporates into the air.
Polynyas are essential for the ecosystem. Like leads, they are a source of heat and moisture to the atmosphere, so they modify the weather in surrounding areas. Polynyas are also essential resources for wildlife. They provide various animals with access to the ocean and the atmosphere. Because polynyas persist for extended periods than leads and overturning ocean water brings nutrients to the surface, phytoplankton thrive in polynyas. Phytoplankton are microscopic plant-like organisms that form the basis of the marine food chain. During the summer, Antarctic polynyas are one of the most biologically productive regions in the world's oceans.
Lake Ice
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Now, let’s be less salty and move back to freshwater processes.
Lake water contains many small particles, including suspended sediment and bacteria. Ice mainly forms when the water gets supercooled from a few hundredths of a degree to a couple of degrees. Once the ice is in still water, it propagates through the supercooled water at the surface as blade-like crystals. The growth rate is controlled by the water's supercooling and the rate at which it can be conducted and radiated into the air from the top surface of the ice crystals.
The initial ice sheet or Primary Ice formation in lakes happens in quiet water with moderate temperatures. Under calm conditions, ice freezes on lakes very similarly to how it freezes in an ice-cube tray. Lake ice freezes first at the surface, starting at the edges or shoreline. Water near the shore is typically shallower and contains less heat than deeper water, so it can reach the freezing point faster than deeper water. The blades grow across the water until they run into each other. After that, dendrites (ice branches on branches) grow off the blades to fill the remaining water surface between the needles. The blades stay on the surface because they float where the supercooled water is. In good conditions, the layer is thin, and supercooling is low. The resulting ice will range from a few inches to several feet.
Warm water gets denser as it gets colder and sinks. Water Colder than 4° Celsius begins expanding and becomes less dense as it gets colder. As a result, when it becomes close to freezing, colder water floats to the top, and warmer water sinks to the bottom. The coldest water, which floats to the top of the lake in wintry conditions, freezes to form a layer of ice. When the water freezes to ice, the ice becomes significantly less dense than the water and continues to float on the lake's surface. Because the crystal lattice allows much light to pass, aquatic algae and plants can grow under lake ice.
Once the primary ice sheet has formed, supercooled water can form under it, except when it is very close to the ice. Ice sheet thickening is limited mainly by how fast heat can be conducted away from the bottom of the sheet. S1 (Secondary) ice is often called 'large-grain ice.' P2 (Primary 2) Ice forms on still water if the air is cold.
P4 (Primary 4) ice is formed when snow falls into the water, ready to freeze, creating closely spaced formation sites and having a small grain size. This is different from frozen shush, formed when snow falls on top of an ice sheet and then gets saturated with water through cracks and holes in the ice sheet. This is called 'snow-ice,' a common form of superimposed ice (T1).
Ice formation on lakes and ponds that are not affected by snow falling; rather, wind and waves, needles, and flakes form on the surface. Collisions and wave action break them up, and they can become tangled up with each other and form small rafts of several flakes. This creates many nucleation sites and allows the primary needles and branches to grow into each other a short distance away, keeping the crystal size small. This ice can evolve in different ways depending on the lake's size, the proximity to the downwind shore, the amount of wind, and other factors.
Grain size is established in the thin primary ice layer; the general texture is preserved as the secondary ice grows on the bottom of the ice sheet. The formation process is called 'slow growth.' The growth rate is controlled by the rate at which latent heat can be conducted through the ice and into the air. This results in a relatively smooth bottom on the ice sheet and a uniform ice growth rate, assuming there is no snow on the ice. Grain size increases toward the bottom of the ice sheet.
Water pressure also plays a role in deep lakes. The gravitational weight of all the water higher up in the lake presses down on the water located deeper. The pressure allows the water near the bottom of the lake to get cold without expanding and rising. Because of the pressure, the water at the bottom of deep lakes can become cold without freezing to ice.
Another characteristic of lake ice is drifting ice; drifting ice is called “pack ice” and comprises sheets of floating ice called floes separated by water. When floes are pushed together, when one floe moves on top of another, this is called “rafting.” When sheets of regular, flat lake ice are broken and pile up, this is called “hummocked ice.” Hummocked ice occurs along shores exposed to wind, pushing soils and material inland. This ice push is called ice ride-up, surge, or ramping.
Glaciers and Icebergs
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Glaciers
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Glaciers form on land and are classified by size. In Antarctica, glaciers can sometimes expand into ice platforms, part of which rests on the bedrock while parts float into the sea. The floating part is called an ice shelf. Ice shelves can cover several thousand square kilometers and reach heights of several dozen meters, creating vertical cliffs several dozen meters high.
Glaciers worldwide are shrinking in size. The worldwide shrinkage of mountain glaciers is thought to be caused by a temperature increase since the Little Ice Age, which ended in the latter half of the 19th century, and increased greenhouse gas emissions.
Water in ice caps and glaciers affects other aspects of the water cycle, such as the weather and the climate. Their Ice is very white, and since white reflects sunlight and heat, large ice fields can determine weather patterns. Air temperatures can be higher a mile above ice caps than at the surface, and wind patterns affecting weather systems can be dramatic around ice-covered landscapes.
The amount of water locked up in glaciers and ice caps is a small percentage of all water on Earth, but it represents a large percentage of the world's total freshwater. The amount of water locked up in ice and snow is only about 1.7 percent of all water on Earth, but the majority of total freshwater on Earth, about 68.7 percent, is held in ice caps and glaciers.
A glacier cave is a cave formed within the ice of a glacier. Although glacier caves are often called ice caves, the term is properly used to describe bedrock caves that contain year-round ice.
Most glacier caves are formed by water running through or under the glacier. This water often originates on the glacier's surface through melting, enters the ice at a moulin, and exits at the glacier's snout at base level. A moulin is a vertical well-like shaft formed where a surface melt stream exploits a weakness in the ice. Heat transfer from the water can cause sufficient melting to create an air-filled cavity.
Some glacier caves are formed by geothermal heat from volcanic vents or hot springs beneath the ice. One of these is the Kverkfjöll glacier cave in the Vatnajökull glacier in Iceland, measured in the 1980s at 2.8 kilometers long and with a vertical range of 525 meters. Some glacier caves are unstable due to melting and glacial motion and are subject to collapse and elimination by global warming. The study of glacier caves itself is sometimes called "glaciospeleology."
Mount Rainier (Washington, US): https://www.mountainguides.com/pop_news_npca-rainier-ice-caves.shtml
Perito Moreno Glacier (Argentina): https://www.manvsglobe.com/perito-moreno-glacier-patagonia-argentina-calafate/
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Titlis (Switzerland): https://www.titlis.ch/en/activities/glacier-cave
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Icebergs
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Icebergs form the edge of glaciers. They are blocks of ice that break away from glaciers and drift out to sea. The process of an ice chunk breaking away from a glacier to form an iceberg is called calving. The visible ‘tip of the iceberg’ typically only represents 20% of the total surface area of the ice block. Icebergs drifting in the ocean can take years to disintegrate before disappearing completely.
Tabular icebergs result from ice breaking off an ice platform and floating in the ocean. They have flat tops and are several hundred kilometers long.
Icebergs: https://www.newfoundlandlabrador.com/trip-ideas/travel-stories/famous-icebergs-of-newfoundland-and-labrador
Tabular icebergs: https://www.nationalgeographic.com/environment/article/this-iceberg-is-perfectly-rectangular-explained
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Frost Weathering:
Frost weathering is a collective term for several weathering processes induced by freezing water into ice. These include various processes, such as frost shattering, frost wedging, and cryo-fracturing. Frost weathering is noticeable in high-altitude and high-latitude areas. It is significantly associated with alpine, periglacial, subpolar maritime, and polar climates but may occur anywhere at sub-freezing temperatures.
Frost-susceptible soils expand upon freezing due to water migrating. This also happens within the pore spaces of rocks. When ice accumulations grow larger as they attract liquid water from the surrounding pores, the ice crystal growth weakens the rocks, which break over time. This is common in humid, temperate areas with exposed rock, such as sandstone. Sand can often be found just under the faces of exposed sandstone where individual grains have been eroded. This process is termed frost spalling. The traditional explanation for frost weathering is When water freezes to ice, its volume increases, and Under specific circumstances, this expansion displaces or fractures the rock. For frost weathering to occur by volumetric expansion, the rock must have almost no air that is then compressed to compensate for ice expansion.
Not all volumetric expansion is caused by the pressure of the freezing water. When ice growth induces stress in the pores of rocks, the result is called a hydrofracture, which is large interconnected pores in the rock causing hydrofracturing. If there are tiny pores, rapid freezing of water in parts of the rock may expel water, and if the water is expelled faster than it can migrate, pressure rises, fracturing the rock.
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Freeze-Thaw Weathering and Frost Wedging:
Frost Wedging
Frost wedging is a form of weathering that breaks down rocks through freezing and thawing. Water enters the rock through cracks and pores, traveling deep within it. Rocks have cracks that are not always visible, which allows them to retain moisture. As the water freezes, it expands into the rock, causing the cracks and pores to grow. The ice then thaws, and the water travels deeper within the rock. The freeze-thaw cycle continues until the rock breaks down completely. This takes time and involves many freezing and thawing cycles. Frost wedging happens in frigid climates with significant rainfall.
Examples of frost wedging include boulders and mountains with large cracks in cold climates. Rock formations caused by frost wedging happen where tectonic plate movement does not occur. Frost wedging can also happen in highways, roads, and bridges, as heavy vehicles often cause cracks where water can seep through and freeze.
Frost Wedging: https://study.com/academy/lesson/video/frost-wedging-definition-example.html
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Chemical Weathering
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Chemical weathering changes the composition of rocks' materials into another substance. Chemical weathering processes can include oxidization, rusting, dissolution, hydrolysis, or dehydration. In all these chemical weathering processes, the chemistry of the rock or minerals found in the rocks is changed.
Chemical Weathering: https://www.americangeosciences.org/education/k5geosource/content/rocks/what-is-chemical-weathering
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Frost Action Weathering
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Frost action weathering is the repeated cycle of ice formation and ice melt within the porous areas of rocks. It is a weathering process that causes disintegration. The amount of rock breakdown depends on the frequency of the freezing and thawing and the duration and intensity of the cycles. Frost action weathering happens as the spaces within the rock expand out of the frozen water, and wedging occurs between the parts of the rock, causing them to split and break down into more pieces. This process causes landslides in areas where there are rocky formations. Frost action weathering is an umbrella term for mechanical weathering processes that break down rock from freezing and thawing action. It includes frost wedging, frost shattering, and cryo-fracturing.
Other environmental factors contribute to frost action weathering. These include the area's lack of permafrost, the amount of tree cover, the type of soil or bedrock, the variability of the climate, and whether the terrain is mountainous or flat. In freeze-thaw weathering, porous and permeable rocks break down when water freezes and thaws.
Frost Action Weathering: https://study.com/academy/lesson/video/frost-wedging-definition-example.html
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Salt Weathering
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Salt weathering is physical weathering when groundwater is soaked into rocks during the freeze-thaw cycles. Groundwater contains calcium, which water evaporates, causing salt crystals to grow on and inside the rocks. These crystals grow and accumulate as more water seeps in and evaporates, putting pressure on the rocks and causing them to break down. This type of physical weathering happens in drier climates.
Salt Weathering: https://oaklandgeology.com/2014/05/11/salt-weathering-tafoni/
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Ice Formations in Caves:
An ice cave is a cavity in ice or an underground cave with permanent ice deposits. The first type of ice cave is formed by meltwater streams carving labyrinths in the bases of glaciers or by streams and wind-hollowing out tunnels in snowfields. These caves have scalloped, translucent walls that transmit a blue light. The second type of ice cave occurs when frigid winter air settles into downward-leading caverns where it cannot be forced out or when moisture freezes in cold air currents. Frozen lakes, icicles, and ice draperies are common formations. Helictite-like icicles also form where air currents deflect the freezing water.
An ice cave is any type of natural cave that contains significant amounts of perennial (year-round) ice. The cave must have a temperature below 0 °C (32 °F) all year round.
Ice can take various forms in caves, such as stalactites, stalagmites, flowstones, and curtains. These typically form from water flowing or dripping into the cave. However, the ice can also form into hairline strands and hexagonal crystals, and this may occur when ice freezes from water vapor or ice flowers when it enters through seeps. Ice can also form in lava tubes or solutional alpine caves. In lava tubes, they tend to form in lower levels of caves with a single entrance, allowing cold winter air to sink and be trapped.
In any cave in regions that reach below-freezing temperatures in winter, ice formations may be seen in entrance zones regardless of the ambient temperatures. As warmer air outside air progresses through the cave, it can melt the ice into rounded shapes with bulbous tops known as schmos.
Schmos: http://www.goodearthgraphics.com/virtcave/ice_formations/iceforms.html
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In seasonal zones outside the caves, there are two zones of ice formation: moist firn (partially compacted névé, a type of snow that has been left over from past seasons and has been recrystallized into a substance denser than névé.) and an ice-feeding zone.
Various freezing mechanisms result in distinct types of perennial cave ice, which are then categorized by how they acclimate and form.
Ponded water: Surface water that collects and ponds in a cave before freezing will form a clear ice mass. This ice can be tens of meters thick and extremely old. Large ice masses can slowly flow apart due to gravity or pressure from further accumulations. Airflow and sublimation can cause accumulation bands within the ice.
Accumulated snow: This snow is compressed under the weight of ongoing accumulations.
Ice formations: Water that freezes before ponding may form icicles, ice-stalagmites, ice columns, or frozen waterfalls.
Airborne moisture (water vapor): Freezing vapor can form frost crystals, feathers, and two-dimensional ice plates on cave walls and ceilings.
Needle ice: This is Infiltrating water that freezes within the bedrock and can sometimes be forced into the cave passage.
Intrusions: The weight of a surface glacier perched atop a cave entrance can force glacial ice a short distance into the cave.
Cave Examples:
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Bandera Volcano Ice Cave (New Mexico, United States): https://www.icecaves.com/gallery/6kt04f8562b7zdohtp8kckd44ncmc8
Bixby State Preserve (Iowa, United States): https://en.wikipedia.org/wiki/Bixby_State_Preserve
Booming Ice Chasm (Alberta, Canada): https://en.wikipedia.org/wiki/Booming_Ice_Chasm
Bortig Pit Cave (Apuseni Mountains, Romania): https://travelguideromania.com/bortig-pit-cave-underground-ice-world/#google_vignette
Canyon Creek Ice Cave (Alberta, Canada): https://hikebiketravel.com/canyon-creek-ice-cave/
Castleguard Cave (Alberta, Canada): https://en.wikipedia.org/wiki/Castleguard_Cave
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Extraterrestrial Ice:
Ice doesn’t just exist on Earth; it has been observed on other worlds, such as extraterrestrial planets and moons, most famously on one of Jupiter’s moons, Europa. This is currently one of the hottest topics in the search for alien life in the universe.
Scientists describe Europa as an "ocean world" because decades of evidence from spacecraft observations strongly suggest that an ocean of liquid water is hidden beneath the moon’s surface ice. Europa is not the only ocean world in the solar system and universe. Two of Saturn’s moons also have water characteristics as well. Enceladus has a global saltwater ocean that sprays out into space as a plume of icy particles, and the moon Titan is thought to have a subsurface ocean as well.
Europa: https://science.nasa.gov/jupiter/moons/europa/
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Enceladus: https://science.nasa.gov/saturn/moons/enceladus/
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Titan: https://science.nasa.gov/saturn/moons/titan/
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The red streaks crisscrossing Europa's surface were mysterious and unknown in substance until recently. Scientists now suspect they are a frozen mixture of water and salts. This phenomenon was most recently studied and observed on February 21, 2023.
An international team led by the University of Washington discovered a new type of solid crystal that forms when water and table salt combine in cold and high-pressure conditions. Researchers believe the new substance created in a lab on Earth could be a substance forming at the surface and bottom of Europa’s deep oceans.
The study, published in the Proceedings of the National Academy of Sciences the week of February 20th, 2023, announced the discovery of a new combination for two of Earth’s most common substances: water and sodium chloride, or table salt. Water and salts combine at cold temperatures to form a salted icy lattice, a hydrate held in place by hydrogen bonds. The only previously known hydrate for sodium chloride was a simple structure with one salt molecule for every two water molecules.
The two new hydrates, made from water and table salt at temperatures below about minus 50 C, differed. One had two sodium chlorides for every 17 water molecules, and the other had one sodium chloride for every 13 water molecules.
The experiment involved compressing a tiny amount of salty water at synchrotron facilities in France, Germany, and the U.S. between two diamonds about the size of a grain of sand, squeezing the liquid up to 25,000 times the standard atmospheric pressure. The transparent diamonds allowed the team to watch the process through a microscope. One of the two structures remained stable even after the pressure was released.
In theory, Cold, high-pressure conditions created in the lab would be common on Jupiter’s moons, where scientists think 5 to 10 kilometers of ice cover oceans up to several hundred kilometers thick, with denser forms of ice possible at the bottom.
Two upcoming space missions—the European Space Agency’s Jupiter Icy Moons Explorer mission and NASA’s Europa Clipper mission, which launches in October 2024—will hopefully confirm this theory shortly. NASA’s Dragonfly mission will launch on Saturn’s moon Titan in 2026.
Ice is on planetary bodies and is critical in how life and organisms develop throughout the universe. According to published studies from August 21, 2024, researchers have started looking at the possibility that the role of low-energy electrons created as cosmic radiation traverses through ice particles can help develop prebiotic molecules, which are the seeds of life on Earth and elsewhere in the universe. Former undergraduate Kennedy Barnes, who, with fellow undergraduate Rong Wu, led this study at Wellesley College, mentored by chemistry professor Christopher Arumainayagam and physics professor James Battat.
A few studies previously researched this suggested that electrons and photons can catalyze the same reactions. However, studies by Barnes and colleagues hinted that the prebiotic molecule yield from low-energy electrons and photons could be significantly different in space. "Our calculations suggest that the number of cosmic-ray-induced electrons within cosmic ice could be much greater than the number of photons striking the ice," Barnes explains. "Therefore, electrons likely play a more significant role than photons in the extraterrestrial synthesis of prebiotic molecules."
To understand prebiotic molecule synthesis better, the researchers tested their hypothesis by mimicking space conditions in the lab. They used an ultrahigh-vacuum chamber containing a copper substrate that could cool to ultralow temperatures, an electron gun that produced low-energy electrons, and a laser-driven plasma lamp that produced low-energy photons. The scientists then bombard nanoscale ice films with electrons or photons to see what molecules were produced.
Another type of “space ice” that exists elsewhere is exotic ice. One type of exotic ice is Ordered ice, whose hydrogen atoms are neatly organized. It most likely exists elsewhere, such as within the high-pressure gas giants and icy moons. Studying these exotic ices in the laboratory is tricky because they form slowly.
On July 12th, 2017, Stanford researchers captured the freezing water form of ice VII (“ice seven”). This substance is found naturally in otherworldly environments, such as when icy planetary bodies collide. This discovery was part of a global research effort to further understand how materials undergo phase changes between gas, liquid, and solid states.
Previous research struggled to capture the action of phase transitions and instead worked backward from stable solids in the molecular steps taken by liquids.
These timescales were achievable using the Linac Coherent Light Source, the world’s most powerful X-ray laser at the SLAC National Accelerator Laboratory, which beamed a green-colored laser at a small sample of liquid water. The laser instantly vaporized layers of diamond on one side of the target, generating a force that compressed the water to pressures exceeding 50,000 times that of Earth’s atmosphere at sea level.
As the water compacted, a separate beam from an instrument called the X-ray Free Electron Laser streamed a series of bright pulses only for a femtosecond, or a quadrillionth of a second long. The X-ray laser snapped images showing the progression of molecular changes, flip book–style, of ice VII. The phase change took six billionths of a second, or nanoseconds, to occur.
These findings furthered researchers' studies on how water freezes depending on pressure and temperature. On Earth’s surface, water crystallizes in only one way, and this process is called ice Ih (“ice one-H”) or “hexagonal ice.” The discovery of Ice VII helps scientists model remote environments such as comet impacts, the internal structures of water-filled moons like Jupiter’s Europa, and the dynamics of exoplanets called super-Earths.
In experiments with ice called Ice XIV, scientists publishing in PNAS Nexus created ordered ice up to 100 times faster than previously tried methods. Published on March 19, 2024, scientists released their observations on Ice XIV, a type of “ordered ice.” Ice XIV forms at low temperatures and extreme pressures. About ten times the pressure at the bottom of the Pacific Ocean’s Mariana Trench. Its molecules form DNA-like double helices. Glaciers made of ice XIV wouldn’t flow normally like regular ice; instead, it would shatter. Study lead author Christina Tonauer, a physical chemist who performed the experiments as a graduate student at the University of Innsbruck in Austria, said there was also a substantial textural difference.
The researchers “doped” ice with small amounts of chemicals to create gaps in the crystal lattice. These defects gave hydrogen atoms more wiggle room to rearrange into ordered structures. The team showed that introducing a tiny bit of ordinary water for heavy ice boosted the ordering. This new strategy allowed Tonauer’s team to create heavy ice XIV three times faster than previous methods. Producing such samples from heavy water could make it easier to discover new kinds of ice and recognize them in the universe.
Upcoming discoveries about ice formations in the universe will most likely come from locations closer to Earth, such as the ice bodies on the further reaches of the solar system, such as Saturn.
Saturn has 146 confirmed moons, but one, Enceladus, appears to have the ingredients for life. From 2004 to 2017, Cassini, a joint mission between NASA, the European Space Agency, and the Italian Space Agency, investigated Saturn, its rings, and its moons. Cassini studied Enceladus, which is around 313 miles (504 kilometers) in diameter, and found it harbored a liquid ocean that spanned the entire moon. The Cassini engineers didn’t anticipate analyzing any icey substances in space, so unfortunately, they could only use the dust analyzer on the spacecraft. This instrument measured the emitted ice grains and told researchers about the composition of the subsurface ocean.
Like Earth’s oceans, Enceladus’ oceans contain salt, mostly sodium chloride. The ocean also contains various carbon-based compounds and tidal heating. Liquid water, carbon-based chemistry, and energy are all critical ingredients for life. In 2023, phosphate, another life-supporting compound, was found in ice grains from Enceladus’ ocean. Phosphate is vital for all life on Earth. It is part of DNA, cell membranes, and bones. This was the first time scientists detected this compound in an extraterrestrial ocean. It is hypothesized that Enceladus’ core likely interacts with the water ocean through hydrothermal vents. These geyser-like structures then protrude from the ocean floor.
Enceladus is one of the main targets for future missions from NASA and the European Space Agency. In 2022, NASA announced that a mission to Enceladus was their second-highest priority. The European agency also announced that Enceladus was their next target for its next big mission.
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CG ICE:
Ice has been extensively studied in CGI through many computer graphics studies. Reflective and translucent materials are always the most challenging to recreate in CGI, and ice meets that criteria.
One of the more recent studies, Snow and Ice Animation Methods in Computer Graphics, was published on 30 April 2024. It was written by Prashant Goswami and released from the Blekinge Institute of Technology in Sweden.
Snow and ice animations are popular in computer graphics, and the applications and methods of creating snow and ice in CG are varied. This can include landscapes, avalanches, and physical interaction with objects in movies and games. This report aimed to identify existing animation methods in the field, provide an up-to-date summary of the research in CG, and identify gaps for promising future work. It also attempts to identify the primarily related work done on snow and ice in other disciplines, such as civil or mechanical engineering, and draw parallels with the similarities and differences in CG. This is a brief transcription of it. It’s a valuable study for understanding the various methods of creating ice-like structures in CGI.
Snow and ice bring mood and atmosphere to the scene while providing a sense of time and place.
A significant challenge when creating snow is capturing its varied visual appearance and behavior under diverse conditions, such as dry or wet, chunky or powdered snow. A similar challenge is faced with ice simulations. They require various computer resources, and creating them has only recently become easier with computer programs such as Sidefx’s Houdini. Various algorithms are needed to simulate materials in CG, and disciplines like mechanical and civil engineering, agricultural science, and physics often inspire these algorithms.
In the movie and video game industry, real physics is often not accurately incorporated into the simulations you see on TV, Film, or video games. Instead, visual accuracy is up to the client's demands and vision.
Various disciplines in the scientific community have studied mechanical properties and determined the micro-level structure of snow or ice. Some of these methods have been useful in shaping the state of the art in CG. The motivation in these fields is to model ice phenomena accurately to capture the physical accuracy of its behavior.
Snow is a visco-elastic material that exhibits properties under different conditions. The reason for the varying properties lies in its internal crystal structure at the micro level. Snow crystals form an interlocking structure as they precipitate. These crystals transform their shapes and consistency after they arrive on the ground. This leads to the formation of ice bonds when coming into close contact with each other by transporting the water molecules. Natural snow cover solidifies with time, creating a denser mixture containing ice particles.
Temperature is an important parameter to consider in ice formations. Most mathematical models require one or several parameters like stress, strain, and cohesive strength to capture snow's plasticity and deformation. In some models, for simulating granular materials, the angle of repose (AOR), the steepest angle relative to the horizontal plane on which the snow can be piled without slumping, is required to solve equations dealing with snow dynamics.
Lagrangian functions are often used to calculate snow models and simulations. Lagrangian function is a quantity that characterizes the state of a physical system. In mechanics, the Lagrangian function is just the kinetic energy (energy of motion) minus the potential energy (energy of position).
The Lagrangian approach deals with a discrete quantity of fluid as particles and computes particle trajectories. Two main Lagrangian methods are more prevalent in simulating snow and ice.
One of these methods is Smoothed particle hydrodynamics (SPH). Smoothed particle hydrodynamics (SPH) is a Lagrangian method that operates on particle-based discretization of the fluid. In contrast to static grid points, the particles carry physical quantities with them. This is an example of how the function works:
A, at a point in 3D space, r is interpolated based on the weighted contributions of particles in its neighborhood (represented by rj). Here, j represents summation over neighboring particles falling within the core radiating kernel with finite support (represented by h). Different smoothing kernels are often applied as h, mj is particle j's mass, Aj is the scalar quantity, ρj the density, and function W(r,h) is a smoother different force, such as pressure force and viscosity. The force equation in SPH is derived using the Navier-Stokes equations. An advantage of the SPH method is that mass conservation comes automatically with it.
Additionally, Lagrangian or hybrid approaches have an advantage since they can counteract solver inaccuracies and have less volume loss than Eulerian approaches.
Another method is the discrete element method (DEM). DEM is a family of Lagrangian numerical methods for computing the motion of particles interacting to predict bulk solids' behavior. It is closely related to molecular dynamics and offers the advantage of simulating millions of particles in increased resolution. DEM allows for the insertion of different forces of nature into different materials. This includes friction, gravity, plasticity, normal and tangential attractive or repulsive potentials. DEM models are effective in simulating granular materials.
Eulerian methods are grid-based, the Lagrangian methods are particle-based, and the semi-Lagrangian methods are hybrid-based.
In addition to developing snow mechanics models, focus has also been placed on understanding the basics of avalanches. Snow avalanches pose a significant hazard to people. Several factors also come into play while dealing with avalanches, such as wind, air mass, fronts, terrain topology, temperature, precipitation, snow profile, grain structure, fracture mechanics, and snow quality.
Two categories of avalanches are slab and powder avalanches. Slab avalanches occur when the snow is solidified, but powder avalanches occur in the accumulated snow due to piling layers. Certain avalanches also can have a hybrid composition. The dry or wet Avalanches can vary in their water composition. A weak layer in the structure is required for most avalanches to occur. Parameters such as fracture toughness are determined by applying a range of pressure to snow masses of different densities. Avalanches have also been studied for erosion and entertainment processes. CGI graphics are used in several applications for avalanche forecasting as well.
Dry snow avalanches initiate from a failure in a weak snow layer below a snow slab. The formation conditions of dry snow slab avalanches involve several essential factors, such as terrain, snow quality, wind, and temperature. Mechanical properties like snow microstructure, failure conditions, and fracture propagation are also studied.
The formation of wet (snow) avalanches is the introduction of liquid water, which decreases snow strength. Computer models and simulations use numerical models to account for saltation, suspension, and preferential deposition processes while simulating snow transport in steep terrains. If implemented into SPH, snow can also be a Bingham fluid. In the Bingham fluid model, two essential snow parameters, the cohesion and friction angle, are required to estimate the viscosity.
Game engines have also been used to simulate avalanche animations. Physical parameters include the initial height, bounce friction, stickiness, and damping force. Genetic algorithms determine all of these forces in the model.
The Material Point Method is also used to simulate the phenomenon. The material point method is a hybrid grid-based method that enables a wide range of snow behaviors. MPM is used at the end of modeling avalanches and landslides. 3D MPM is used to explore snow avalanches on complex real-world terrain models. The idea is to account for factors such as densification and granulation, which are hard to capture in numerical approaches for modeling avalanches. MPM is also used to model sea-ice dynamics with an elastic-de-cohesion equation for modeling material failure and an algorithm to track thickness distributions and ice compactness.
There are other mathematical equations for simulating snow and ice. Some work involving snow dynamics has been dedicated to simulating the impact of forests on flowing avalanches. The study showed that mass detrainment due to tree-avalanche interaction led to deceleration of the avalanches. Another example implemented a depth-averaged flow model for avalanche simulations, which combines simple entrainment and friction relation. In this approach for 3D simulations, two friction parameters, Coulomb friction and turbulent drag, are used. Rapid Mass Movements (RAAMS) is another popular avalanche dynamics program that simulates avalanches. RAAMS solves the depth-averaged equations, explaining avalanche flow and allowing for the colliding of snow with other objects.
When modeling, simulating, and rendering ice in CGI, it is fairly common for it to look like glass rather than ice when you first approach it. Ice has specific visual characteristics, such as being visually wet-looking, transparent in some places, less opaque in others, and visible large and small cracks. You must factor these visual cues into your render for a great result. Ice also has a slightly lower IOR than water, so that also needs to be factored in.
The opaque-looking parts of ice, such as ice cubes, are caused by clusters of microscopic bubbles that form during freezing. One method you can try to replicate this is by modeling these using geometry. Ice cubes usually have air bubbles trapped inside. These bubbles appear as a white volumetric haze in the cube's center.
Non-submerged ice will form a thin layer of liquid water interfacing it with the air, which can significantly alter its appearance. So consider adding something that can represent this in the scene as well. Ice also has Angle-dependent reflection. If this is handled incorrectly, your ice will appear glass-like.
Because ice is a semi-translucent material object, you must also play with subsurface scattering values. You can also consider using volumes to create the opaque inside of ice. You can do this by modeling the outside of the ice with geometry and then using a volume to create a sense of murkiness within the ice. You can also play with procedural noises to get details inside the ice for glacier-like and static structures.
Techniques for modeling ice depend on what rendering method you're using.
Bump mapping, when calculating lighting and refraction rays, can significantly enhance the appearance of ice. It makes the ice look textured and imperfect, like a melting ice cube.
Ice can also be rendered in video game or other real time engines. Published on 31 January 2007, Real-Time Rendering of Ice is the creation of authors Stefan Seipel and Anders Nivfor, presented at CGIM '07: Proceedings of the Ninth IASTED International Conference on Computer Graphics and Imaging.
These methods were presented as a method implementing the visual appearance of ice and its essential characteristics in real time. The proposed method could fill a given convex geometry with air particles and bubbles and add arbitrary cracks. Techniques were also presented for creating bumpy and irregular surfaces that repeatedly reflect and refract the environment. An improved image space technique for clipping a geometry using the Boolean difference of two geometries was also presented. This technique was used on the cracks to clip them against the ice's geometry. The reflection and refraction effects on the ice were implemented using environment mapping. Two-sided refraction was also accomplished by combining the normal vectors of the front and back sides of the ice object.
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Houdini Tutorial | Setup and make ICICLE in 1 HOUR!: https://www.youtube.com/watch?v=vHAew3gmJnk
SESI-Snacks V2 | 12 Ice Ice Baby: https://www.youtube.com/watch?v=C2myNvLbr3w
Creating Procedural Drift Ice in Houdini using SOPs and Solaris: https://www.andreaskj.com/coming-soon/
How to Make a Procedural Iceberg in Houdini / Redshift in 4 minutes: https://www.youtube.com/watch?v=Nv67FlTQxkc
Houdini Broken Ice Cubes Tutorial Coca-Cola Promo (Part02): https://www.youtube.com/watch?v=yzRF_jLxHC8
Tutorial 02 - Melting Ice In Houdini: https://www.youtube.com/watch?v=J0NtJNmSvDE
Breakdown: Simulating Ice Growth in Houdini: https://80.lv/articles/006sdf-breakdown-simulating-ice-growth-in-houdini/
Houdini Tutorial - Dry Ice make in Houdini 19.5: https://www.reddit.com/r/Houdini/comments/132w7yp/houdini_tutorial_dry_ice_make_in_houdini_195/?rdt=35856&onetap_auto=true&one_tap=true
Star Destroyer Ice Destruction | Advanced Star Wars Houdini Tutorial: https://www.youtube.com/watch?v=MnrWNeVd39s
Ice Growth Houdini Tutorial_Part_4_render_composition_ice_growth: https://www.youtube.com/watch?v=FG_ktOmfnI8
Houdini Frozen Geometry Tutorial: https://www.youtube.com/watch?v=EtMlUxvLbTE
Making a Glacier Ice Material in Redshift: https://www.youtube.com/watch?v=nqXvU4bHiOE
Houdini Snow and Ice 1: https://www.youtube.com/watch?v=yELy9PkO5uI
Houdini - Ice pyramid structure: https://www.youtube.com/watch?v=u0X7tn3uKPE
SESI-Snacks V2 | 06 Ice Smash: https://www.youtube.com/watch?v=5p0fwp96wI8
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