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Ice ages are recurring periods in the Earth’s history, usually thousands or tens of thousands of years in length, when the entire Earth experiences colder climatic conditions. During these periods, enormous continental glaciers called ice sheets cover large areas of the Earth’s surface. Ice ages are separated by warmer periods called interglacial periods. Several ice ages have occurred throughout our planet’s history. The last ice age peaked about 18,000 years ago, after which the Earth again began to warm.
Ice age intervals seem to correspond with long periods of worldwide climatic cooling. It should be noted that there are numerous factors that affect the Earth’s climate. There are two main natural factors, however, that are thought to influence long-term changes in the Earth’s climate.
Plate Tectonics
- Changes in the positions of the continents are linked to periods of multiple glaciations. The presence of large landmasses at the poles seems to trigger the development of extensive ice sheets. For example, throughout the Ice age that occurred during the Pennsylvanian and Permian geologic eras (250 –350 million years ago), the southern portion of the super-continent Pangaea was at the South Pole. Scientists believe this may have caused extensive glaciation over what are now Africa, South America, India, Antarctica, and Australia.
- Major uplift at continental plate boundaries can cause profound changes in oceanic and atmospheric circulation patterns. Changing circulation patterns cause climate change. Some scientists hypothesize that climatic changes caused by uplift are critical to the development of ice ages.
- Large or numerous volcanic eruptions, also the result of plate tectonics, release huge amounts of gases (carbon dioxide and water vapor) that act to trap heat within the atmosphere, causing global warming (sometimes referred to as the greenhouse effect). In contrast, particles of ash can impact the global climate by reducing the amount of solar radiation reaching Earth’s surface, causing global cooling.
Milankovitch Cycles
Named after the Serbian mathematician Milutin Milankovich, the Milankovitch cycles describe variations in Earth’s position as it orbits the Sun that affect the amount of sunlight it receives. One cycle involves the shape of Earth’s orbit, which varies from being more elliptical to more circular. Another cycle involves Earth’s “tilt” on its axis, which is not perpendicular to the plane of its orbit around the Sun. Presently, Earth tilts 23.5¾ from the perpendicular, but there is evidence that in the past this angle varied from 22¾ to 24¾. A third variation involves Earth’s “wobble.” Like a top wobbling on its axis, Earth wobbles as it orbits. The results are that sometimes the North Pole points to the North Star, and sometimes it points to the star Vega. These cycles vary from tens of thousands to hundreds of thousands of years and can be traced back through the Earth’s geologic record.
Several ice ages have occurred throughout our planet’s history. Major periods of glaciations occurred during the late Proterozoic Era (between 600 and 800 million years ago), during the Pennsylvanian and Permian Eras (between about 250 and 350 million years ago), and the late Neocene to Quaternary Eras (the last 4 million years). Somewhat less extensive glaciations occurred during parts of the Ordovician and Silurian Eras (between about 430 and 460 million years ago). The most recent ice age began about 1.8 million years ago during the Pleistocene Era. During this time, giant ice sheets advanced and retreated many times in North America and Europe.
Recent cycles of advancing and retreating ice sheets have occurred approximately every 100,000 years. Each cycle consists of a long, generally cold period during which the ice sheets slowly reach their maximum size, and a relatively short, warm period during which the ice sheets rapidly retreat.
We are now in a warm period that has lasted more than 10,000 years, which is longer than many of the previous warm intervals. If the pattern of glacial cycles holds true, scientists believe the Earth is soon due for another cold period. In the 1800s, global temperatures began decreasing during a period known as the Little Ice Age. Currently, patterns indicate that the Earth is nearing the end of an interglacial period, meaning that another ice age is predicted in a few thousand years.
Glaciers are huge sheets of moving ice that erode the land as they move. Due to their sheer mass, glaciers flow like very slow rivers. Glaciers store about 75% of the world’s freshwater. Some glaciers are as small as football fields, while others grow to be over one hundred kilometers long (about 100,000 football fields, or 62.2 miles).
Glaciers begin to form when snow accumulates and remains in an area year-round. If temperatures do not rise enough to completely melt the snow, snow continues to accumulate. Each year, new layers of snow bury and compress the previous layers. The weight of the overlying snow puts enough pressure on the bottommost snow layers to compress them into large, thickened ice masses. This compression forces the snow to re-crystallize. During recrystallization, the crystals interlock to create ice that essentially behaves like rock. Once a mass of compressed ice reaches a critical thickness, it becomes so heavy that it begins to move.
The glacier terminus is the leading edge of a glacier. The accumulation zone is the area where snowfall is added (usually near the top of the glacier). The ablation zone is the area of the glacier where glacial ice is being lost through evaporation, melting, or calving (see below). When a glacier flows rapidly over uneven land, the top of the glacier bends and breaks, creating huge cracks called crevasses. Internal stresses build up in the ice that cannot be relieved by internal deformation alone, and crevasses form at the surface of the glacier. Glaciers leave grooves, gouges, and scratches on the landscape called glacial striations that record their passage.
As a glacier moves, it picks up rock pieces from the landscape. Debris of all sizes that is stuck in the glacial ice can scour and erode the land. From this action, valleys can become wider and deeper, forming u-shaped (or trough) valleys. Glaciers can carve bowl-shaped depressions, called cirques, into a mountainside. A tarn is a lake that forms by ice melting in a cirque. An arête is the steep ridge that forms between two adjacent cirques. A col is a low spot on an arête. A horn is a peak formed when three or more adjacent cirque glaciers carve away the side of a mountain.
Continental glaciers scour linear finger lakes out of pre-existing stream channels. Paternoster lakes are a series of lakes that form in the low spots of a u-shaped valley; a stream that flows through the valley links them.
Drumlins are elongated hills formed of till (an unsorted mixture of mud, sand, pebbles and rock deposited by a glacier) with a distinctive streamline shape that results from having been overridden by a glacier or modified by meltwater. The long axis of a drumlin indicates the direction of glacier flow. Eskers are the deposits of rivers and streams that flowed on, in, or under a glacier. They form mounds or hills that meander across a landscape roughly parallel to the path of the original glacial river. Kettle holes are formed by blocks of ice that separate from the main glacier. Under the right conditions the ice blocks will melt and leave behind holes or depressions that fill with water to become kettle ponds or kettle lakes.