
Icebergs breaking off glaciers at Cape
York, Greenland
A
glacier is a perennial mass of ice which moves
over land. A glacier forms in locations where the mass accumulation
of snow and ice exceeds
ablation over many
years. The word
glacier comes from
French via the
Vulgar Latin glacia, and ultimately
from
Latin glacies meaning
ice. The corresponding area of study is called
glaciology.
Glacier ice is the largest reservoir of
fresh water on
Earth, and
is second only to
oceans as the largest
reservoir of total water. Glaciers cover vast areas of the
polar regions and are found in
mountain ranges of every continent including
Australasia (there are glaciers in New Zealand which forms part of
the continent of Australasia). In the tropics glaciers are
restricted to the highest mountains. The processes and landforms
caused by glaciers and related to them are referred to as
glacial. The process of glacier growth and
establishment is called
glaciation. Glaciers are
indicators of climate and are important to world water resources
and sea level variation. They are an important component of the
more encompassing
cryosphere.
Types of glaciers
Glaciers are categorized in many ways including by their
morphology, thermal characteristics, or their behavior. Two common
types of glaciers are Alpine glaciers, which originate in
mountains, and Continental ice sheets, which cover larger
areas.
Alpine glaciers form on mountain slopes and are
also known as mountain, niche, or
cirque
glaciers. An alpine glacier that fills a valley is referred to as a
valley glacier.
Larger glaciers that cover an entire
mountain, mountain chain, or volcano are
known as an ice cap or ice field, such as the Juneau Icefield
. Ice caps feed
outlet
glaciers, tongues of ice that extend into valleys below,
far from the margins of the larger ice masses.
Ice sheets are the largest glaciers. These
enormous masses of ice are not visibly affected by the landscape as
they cover the entire surface beneath them, with possible exception
near the glacier margins where they are thinnest.
Antarctica
and Greenland
are the only places where continental ice sheets currently exist. These regions
contain vast quantities of fresh water. The volume of ice is so
large that if the
Greenland ice
sheet melted, it would cause sea levels to rise six meters
(20 ft) all around the world. If the
Antarctic ice sheet melted, sea levels
would rise up to 65 meters (210 ft).
Ice
shelves are areas of floating ice, commonly located at the
margin of an ice sheet. As a result they are thinner and have
limited slopes and reduced velocities.
Ice streams
are fast moving sections of an ice sheet.. They can be several
hundred kilometers long.
Ice streams have
narrow margins and either side ice flow is usually an order of
magnitude less. In Antarctica, many ice streams drain into large
ice shelves.
However, some drain
directly into the sea, often with an ice
tongue, like Mertz
Glacier
. In Greenland and Antarctica, ice streams
ending at the sea are often referred to as tidewater glaciers or
outlet glaciers, such as Jakobshavn Isbræ
( ).
Tidewater glaciers are glaciers that terminate in
the sea. As the ice reaches the sea pieces break off, or
calve, forming
icebergs. Most
tidewater glaciers calve above sea level, which often results in a
tremendous splash as the iceberg strikes the water. If the water is
deep, glaciers can calve underwater, causing the iceberg to
suddenly explode up out of the water.
The Hubbard Glacier
is the longest tidewater glacier in Alaska and has
a calving face over ten kilometers long. Yakutat Bay
and Glacier Bay
are both popular with cruise ship passengers
because of the huge glaciers descending hundreds of feet to the
water. This glacier type undergoes centuries-long
cycles of advance and retreat that
are much less affected by the climate changes currently causing the
retreat of most other glaciers. Most tidewater glaciers are outlet
glaciers of ice caps and ice fields.
In terms of thermal characteristics, a
temperate glacier
is at melting point throughout the year, from its surface to its
base. The ice of a
polar glacier is always below freezing
point from the surface to its base, although the surface snowpack
may experience seasonal melting. A
sub-polar glacier has
both temperate and polar ice, depending on the depth beneath the
surface and position along the length of the glacier.
Formation

Formation of glacial ice
Glaciers form where the accumulation of snow and ice exceeds
ablation. As the snow and ice thicken, they reach a point where
they begin to move, due to a combination of the surface slope and
the pressure of the overlying snow and ice. On steeper slopes this
can occur with as little as 50 feet of snow-ice. The snow which
forms temperate glaciers is subject to repeated freezing and
thawing, which changes it into a form of granular ice called
firn. Under the pressure of the layers of ice
and snow above it, this granular ice fuses into denser and denser
firn. Over a period of years, layers of firn
undergo further compaction and become glacial ice. Glacier ice has
a slightly reduced density from ice formed from the direct freezing
of water. The air between snowflakes becomes trapped and creates
air bubbles between the ice crystals.
The distinctive blue tint of glacial ice is often wrongly
attributed to
Rayleigh
scattering due to bubbles in the ice. The blue color is
actually created for the same reason that
water is blue, that is, its slight absorption of red
light due to an
overtone of the infrared
OH stretching mode of the
water molecule.
Anatomy
The location where a glacier originates is referred to as the
glacier head. A glacier terminates at the glacier foot, or
terminus. Glaciers are broken into zones
based on surface snowpack and melt conditions. The ablation zone is
the region where there is a net loss in glacier mass. The
equilibrium line separates the ablation zone and the accumulation
zone. At this altitude, the amount of new snow gained by
accumulation is equal to the amount of ice lost through ablation.
The accumulation zone is the region where snowpack or superimposed
ice accumulation persists. A further zonation of the accumulation
zone distinguishes the melt conditions that exist. The dry snow
zone is a region where no melt occurs, even in the summer, and the
snowpack remains dry. The percolation zone is an area with some
surface melt, causing
meltwater to
percolate into the
snowpack. This zone
is often marked by refrozen
ice lenses,
glands, and layers. The snowpack also never reaches melting point.
Near the equilibrium line on some glaciers, a superimposed ice zone
develops. This zone is where meltwater refreezes as a cold layer in
the glacier, forming a continuous mass of ice. The wet snow zone is
the region where all of the snow deposited since the end of the
previous summer has been raised to 0°C. The upper part of a glacier
that receives most of the snowfall is called the
accumulation
zone. In general, the
glacier accumulation zone accounts
for 60-70% of the glacier's surface area, more if the glacier
calves icebergs. The depth of ice in the accumulation zone exerts a
downward force sufficient to cause deep
erosion of the rock in this area. After the glacier
is gone, this often leaves a bowl or amphitheater-shaped
isostatic depression ranging from large
lake basins such as the Great Lakes or Finger Lakes to smaller
mountain basins, known as
cirques.
The "health" of a glacier is usually assessed by determining the
glacier mass balance or
observing terminus behavior. Healthy glaciers have large
accumulation zones, more than 60% of their area snowcovered at the
end of the melt season, and a terminus with vigorous flow.
Following the
Little Ice Age, around
1850, the glaciers of the Earth have retreated substantially
through the 1940s (see
Retreat of glaciers since
1850). A slight cooling led to the advance of many alpine
glaciers from 1950-1985. However, since 1985 glacier retreat and
mass balance loss has become increasingly ubiquitous and
large.
Motion

Nadelhorn Glacier above Saas-Fee,
Valais, Switzerland
Glaciers move, or flow, downhill due to the internal deformation of
ice and
gravity. Ice behaves like an easily
breaking solid until its thickness exceeds about 50 meters
(160 ft). The pressure on ice deeper than that depth causes
plastic flow. At the molecular
level, ice consists of stacked layers of molecules with relatively
weak bonds between the layers. When the stress of the layer above
exceeds the inter-layer binding strength, it moves faster than the
layer below.
Another type of movement is through
basal
sliding. In this process, the glacier slides over the terrain
on which it sits,
lubricated by the
presence of liquid water. As the pressure increases toward the base
of the glacier, the melting point of water decreases, and the ice
melts. Friction between ice and rock and
geothermal heat from the Earth's
interior also contribute to melting. This type of movement is
dominant in temperate, or warm-based glaciers. The geothermal heat
flux becomes more important the thicker a glacier becomes.
The rate of movement is dependent on the underlying slope, amongst
many other factors.
Fracture zone and cracks
The top 50 meters of the glacier, being under less pressure, are
more rigid; this section is known as the
fracture zone,
and mostly moves as a single unit, over the plastic-like flow of
the lower section. When the glacier moves through irregular
terrain, cracks up to 50 meters deep form in the fracture zone. The
lower layers of glacial ice flow and deform plastically under the
pressure, allowing the glacier as a whole to move slowly like a
viscous fluid. Glaciers flow downslope, usually this reflects the
slope of their base, but it may reflect the surface slope instead.
Thus, a glacier can flow rises in terrain at their base. The upper
layers of glaciers are more brittle, and often form deep cracks
known as
crevasses. the presence of
crevasses is a sure sign of a glacier. Moving ice-snow of a glacier
is often separated from a mountain side or snow-ice that is
stationary and clinging to that mountain side by a
bergshrund. This looks like a crevasse but is at
the margin of the glacier and is a singular feature.
Crevasses form due to differences in glacier velocity. As the parts
move at different speeds and directions,
shear forces cause the two sections to break
apart opening the crack of a crevasse all along the disconnecting
faces. Hence, the distance between the two separated parts while
touching and rubbing deep down, frequently widens significantly
towards the surface layers, many times creating a wide chasm.
Crevasses seldom are more than 150 feet deep. Beneath this point
the plastic deformation of the ice under pressure is too great for
the differential motion to generate cracks. Transverse crevasses
are transverse to flow, as a glacier accelerates where the slope
steepens. Longitudinal crevasses form semi-parallel to flow where a
glacier expands laterally. Marginal crevasses form from the edge of
the glacier, due to the reduction in speed caused by friction of
the valley walls. Marginal crevasses are usually largely transverse
to flow.
Crevasses make travel over glaciers hazardous. Subsequent heavy
snow may form fragile
snow bridges,
increasing the danger by hiding their presence at the surface.
Below the equilibrium line glacier meltwater is concentrated in
stream channels. The meltwater can pool in a proglacial lake, a
lake on top of the glacier, or can descend into the depths of the
glacier via
moulins.
Within or beneath the glacier the stream will flow in an englacial
or sub-glacial tunnel. Sometimes these tunnels reemerge at the
surface of the glacier.
Speed
The speed of glacial displacement is partly determined by
friction. Friction makes the ice at the bottom of
the glacier move more slowly than the upper portion. In alpine
glaciers, friction is also generated at the valley's side walls,
which slows the edges relative to the center. This was confirmed by
experiments in the 19th century, in which stakes were planted in a
line across an alpine glacier, and as time passed, those in the
center moved farther.
Mean speeds vary greatly. There may be no motion in stagnant areas,
where trees can establish themselves on surface sediment deposits
such as in Alaska.
In other cases they can move as fast as 20-30
meters per day, as in the case of Greenlands's Jakobshavn
Isbræ
( ), or 2–3 m per day on Byrd Glacier
the largest glacier in the world in
Antarctica. Velocity increases with increasing slope,
increasing thickness, increasing snowfall, increasing longitudinal
confinement, increasing basal temperature, increasing meltwater
production and reduced bed hardness.
A few glaciers have periods of very rapid advancement called
surges. These glaciers exhibit
normal movement until suddenly they accelerate, then return to
their previous state. During these surges, the glacier may reach
velocities far greater than normal speed. These surges may be
caused by failure of the underlying bedrock, the ponding of
meltwater at the base of the glacier — perhaps delivered from
a
supraglacial lake — or the
simple accumulation of mass beyond a critical "tipping
point".
In glaciated areas where the glacier moves faster than one
kilometer per year,
glacial
earthquakes occur. These are large scale
tremblors that have seismic magnitudes as high as
6.1.
The number
of glacial earthquakes in Greenland
show a peak every year in July, August and
September, and the number is increasing over time. In a
study using data from January 1993 through October 2005, more
events were detected every year since 2002, and twice as many
events were recorded in 2005 as there were in any other year. This
increase in the numbers of glacial earthquakes in Greenland may be
a response to
global warming.
Seismic waves are also generated by the
Whillans Ice Stream, a large,
fast-moving river of ice pouring from the West Antarctic Ice Sheet into the
Ross Ice
Shelf
. Two bursts of seismic waves are released
every day, each one equivalent to a magnitude 7 earthquake, and are
seemingly related to the
tidal action of the
Ross Sea. During each event a 96 by 193 kilometer (60 by 120 mile)
region of the glacier moves as much as .67 meters (2.2 feet)
over about 25 minutes, remains still for 12 hours, then moves
another half-meter.
The seismic waves are recorded at seismographs around Antarctica
, and even as far away as Australia, a distance of more than 6,400
kilometers. Because the motion takes place of such along
period of time 10 to 25 minutes, it cannot be felt by scientists
standing on the moving glacier. It is not known if these events are
related to global warming
Ogives
Ogives are alternating dark and
light bands of ice occurring as narrow wave crests and wave valleys
on glacier surfaces. They only occur below
icefalls but not all icefalls have ogives below
them. Once formed, they bend progressively downglacier due to the
increased velocity toward the glacier's centerline. Ogives are
linked to seasonal motion of the glacier as the width of one dark
and one light band generally equals the annual movement of the
glacier. The ridges and valleys are formed because ice from an
icefall is severely broken up thereby increasing ablation surface
area during the summertime creating a swale and creating space for
snow accumulation in the winter creating a ridge. Sometimes ogives
are described as either wave ogives or band ogives in which they
are solely undulations or varying color bands respectively.
Geography

Black ice glacier in Aconcagua
vicinity, Argentina
Glaciers occur on every continent, except Australia and
approximately 47 countries.
Extensive glaciers are found in Antarctica
, Chilean Patagonia,
Canada
, Alaska
, Greenland
and Iceland
. Mountain glaciers are widespread, e.g., in
the Andes, the Himalaya
, the Rocky
Mountains, the Caucasus, and the
Alps. On mainland Australia no glaciers exist
today, although a small glacier on Mount Kosciuszko
was present in the last glacial period, and Tasmania
was extensively glaciated. The South Island
of New
Zealand
has many glaciers including Tasman
, Fox
and Franz Josef Glaciers
. In New Guinea
, small, rapidly diminishing, glaciers are located
on its highest summit massif of Puncak Jaya
. Africa has glaciers on Mount
Kilimanjaro
in Tanzania, on Mount Kenya
and in the Ruwenzori Range
.
Permanent snow cover is affected by factors such as the degree of
slope on the land, amount of snowfall and the
winds. As
temperature decreases with
altitude, high
mountains —
even those near the
Equator — have permanent
snow cover on their upper portions, above the
snow line.
Examples include Mount Kilimanjaro and the
Tropical Andes in South America; however, the only snow to occur
exactly on the Equator is at on the southern slope of Volcán
Cayambe
in Ecuador
.
Conversely, areas of the Arctic such as Banks Island
and the Dry Valleys in Antarctica
are considered polar
deserts and receive little snowfall despite the bitter
cold. Cold air, unlike warm air, is unable to transport much
water vapor.
Even during glacial periods of the Quaternary, Manchuria,
lowland Siberia
, and central
and northern Alaska,
though extraordianarily cold with winter temperatures believed to
reach in parts, had such light snowfall that glaciers could not
form.
In
addition to the dry, unglaciated polar regions, there are some
mountains and volcanoes in Bolivia
, Chile
and Argentina
that are high ( - ) and cold, but the relative lack
of precipitation prevents snow from accumulating into
glaciers. This is because these peaks are located near
or in the hyperarid Atacama
desert
.
Glacial geology

Diagram of glacial plucking and
abrasion
Rocks and sediments are added to glaciers through various
processes. Glaciers erode the terrain principally through two
methods:
abrasion and
plucking.
As the glacier flows over the bedrock's fractured surface, it
softens and lifts blocks of rock that are brought into the ice.
This process is known as plucking, and it is produced when
subglacial water penetrates the fractures and the subsequent
freezing expansion separates them from the bedrock. When the ice
expands, it acts as a lever that loosens the rock by lifting it.
This way, sediments of all sizes become part of the glacier's load.
The rocks frozen into the bottom of the ice then act like grit in
sandpaper.
Abrasion occurs when the ice and the load of rock fragments slide
over the bedrock and function as sandpaper that smooths and
polishes the surface situated below. This pulverized rock is called
rock flour. This flour is formed by rock
grains of a size between 0.002 and 0.00625 mm. Sometimes the
amount of rock flour produced is so high that currents of
meltwaters acquire a grayish color. These processes of erosion lead
to steeper valley walls and mountains slopes in alpine settings,
which then can cause avalanches and rock slides which further add
material to the glacier.
A visible characteristics of glacial abrasion are
glacial striations. These are produced
when the bottom's ice contains large chunks of rock that mark
scratches in the bedrock. By
mapping the
direction of the flutes the direction of the glacier's movement can
be determined.
Chatter marks are seen
as lines of roughly crescent shape depressions in the rock
underlying a glacier caused by the abrasion where a boulder in the
ice catches and is then released repetitively as the glacier drags
it over the underlying basal rock.
The rate of glacier erosion is variable. The differential erosion
undertaken by the ice is controlled by six important factors:
- Velocity of glacial movement
- Thickness of the ice
- Shape, abundance and hardness of rock fragments contained in
the ice at the bottom of the glacier
- Relative ease of erosion of the surface under the glacier.
- Thermal conditions at the glacier base.
- Permeability and water pressure at the glacier base.
Material that becomes incorporated in a glacier are typically
carried as far as the zone of ablation before being deposited.
Glacial deposits are of two distinct types:
- Glacial till: material directly deposited from glacial ice.
Till includes a mixture of undifferentiated material ranging from
clay size to boulders, the usual composition of a moraine.
- Fluvial and outwash: sediments deposited by water. These
deposits are stratified through various processes, such as boulders
being separated from finer particles.
The larger pieces of rock which are encrusted in till or deposited
on the surface are called
glacial
erratics. They may range in size from pebbles to boulders,
but as they may be moved great distances they may be of drastically
different type than the material upon which they are found.
Patterns of glacial erratics provide clues of past glacial
motions.
Moraines
Glacial
moraines are formed by the
deposition of material from a glacier and are exposed after the
glacier has retreated. These features usually appear as linear
mounds of
till, a non-sorted mixture of rock,
gravel and boulders within a matrix of a fine powdery material.
Terminal or end moraines are formed at the foot or terminal end of
a glacier. Lateral moraines are formed on the sides of the glacier.
Medial moraines are formed when two different glaciers, flowing in
the same direction, coalesce and the lateral moraines of each
combine to form a moraine in the middle of the merged glacier. Less
apparent is the ground moraine, also called
glacial drift,
which often blankets the surface underneath much of the glacier
downslope from the equilibrium line. Glacial meltwaters contain
rock flour, an extremely fine powder
ground from the underlying rock by the glacier's movement. Other
features formed by glacial deposition include long snake-like
ridges formed by streambeds under glaciers, known as
eskers, and distinctive streamlined hills, known
as
drumlins.
Stoss-and-lee erosional features are formed by glaciers
and show the direction of their movement. Long linear rock
scratches (that follow the glacier's direction of movement) are
called
glacial
striations, and divots in the rock are called
chatter marks. Both of these features are
left on the surfaces of stationary rock that were once under a
glacier and were formed when loose rocks and boulders in the ice
were transported over the rock surface. Transport of fine-grained
material within a glacier can smooth or polish the surface of
rocks, leading to
glacial polish.
Glacial erratics are rounded
boulders that were left by a melting glacier
and are often seen perched precariously on exposed rock faces after
glacial retreat.
The term
moraine is of
French origin, and it was coined by peasants
to describe alluvial embankments and rims found near the margins of
glaciers in the French
Alps. In modern geology,
the term is used more broadly, and is applied to a series of
formations, all of which are composed of till.
Drumlins

A drumlin field forms after a glacier
has modified the landscape.
The teardrop-shaped formations denote the direction of the ice
flow.
Drumlins are asymmetrical, canoe shaped
hills with aerodynamic profiles made mainly of till. Their heights
vary from 15 to 50 meters and they can reach a kilometer in length.
The tilted side of the hill looks toward the direction from which
the ice advanced (
stoss), while the longer slope follows
the ice's direction of movement (
lee).
Drumlins are found in groups called
drumlin fields or
drumlin camps.
An
example of these fields is found east of Rochester,
New York
, and it is estimated that it contains about 10,000
drumlins.
Although the process that forms drumlins is not fully understood,
it can be inferred from their shape that they are products of the
plastic deformation zone of ancient glaciers. It is believed that
many drumlins were formed when glaciers advanced over and altered
the deposits of earlier glaciers.
Glacial valleys
Before glaciation, mountain valleys have a characteristic
"V" shape, produced by downward erosion by
water. However, during glaciation, these valleys widen and deepen,
forming a
"U"-shaped glacial valley.
Besides the deepening and widening of the valley, the glacier also
smooths the valley due to erosion. In this way, it eliminates the
spurs of earth that extend across the valley. Because of this
interaction, triangular cliffs called
truncated spurs are formed.
Many glaciers deepen their valleys more than their smaller
tributaries. Therefore, when the glaciers recede
from the region, the valleys of the tributary glaciers remain above
the main glacier's depression, and these are called
hanging valleys.
In parts of the soil that were affected by abrasion and plucking,
the depressions left can be filled by lakes, called
paternoster lakes.
At the 'start' of a classic valley glacier is the
cirque, which has a bowl shape with escarped walls on
three sides, but open on the side that descends into the valley. In
the cirque, an accumulation of ice is formed. These begin as
irregularities on the side of the mountain, which are later
augmented in size by the coining of the ice. Once the glacier
melts, these corries are usually occupied by small mountain lakes
called
tarns.
There may be two glacial cirques 'back to back' which erode deep
into their backwalls until only a narrow ridge, called an
arête is left. This structure may result in a
mountain pass.
Glaciers are also responsible for the creation of
fjords (deep coves or inlets) and
escarpments that are found at high
latitudes.
Features of a glacial landscape
Arêtes and horns (pyramid peak)
An
arête is a narrow crest with a
sharp edge. The meeting of three or more arêtes creates pointed
pyramidal peaks and in extremely
steep-sided forms these are called
horn.
Both features may have the same process behind their formation: the
enlargement of cirques from glacial plucking and the action of the
ice. Horns are formed by cirques that encircle a single
mountain.
Arêtes emerge in a similar manner; the only difference is that the
cirques are not located in a circle, but rather on opposite sides
along a divide. Arêtes can also be produced by the collision of two
parallel glaciers. In this case, the glacial tongues cut the
divides down to size through erosion, and polish the adjacent
valleys.
Roche moutonnée
Some rock formations in the path of a glacier are sculpted into
small hills with a shape known as
roche moutonnée or
sheepback
rock. An elongated, rounded, asymmetrical, bedrock knob can be
produced by glacier erosion. It has a gentle slope on its
up-glacier side and a steep to vertical face on the down-glacier
side. The glacier abrades the smooth slope that it flows along,
while rock is torn loose from the downstream side and carried away
in ice, a process known as 'plucking'. Rock on this side is
fractured by a combination of various forces, such as water, ice in
rock cracks, and structural stresses.
Alluvial stratification
The water that rises from the
ablation
zone moves away from the glacier and carries with it fine
eroded sediments. As the speed of the water decreases, so does its
capacity to carry objects in suspension. The water then gradually
deposits the sediment as it runs, creating an
alluvial plain. When this phenomenon occurs
in a valley, it is called a
valley train. When the
deposition is to an
estuary, the sediments
are known as "
bay mud".

Landscape produced by a receding
glacier
Outwash plains and valley trains are usually accompanied by basins
known as
kettles. These are glacial
depressions which are produced when large ice blocks are stuck in
the glacial alluvium and after melting, they leave holes in the
sediment. The diameter of these depressions ranges from 5 m to
13 km, with depths of up to 45 meters. Most are circular in
shape due to the melting blocks of ice becoming rounded. Lakes
often form in these depressions and these are known as kettle
lakes.
Deposits in contact with ice
When a glacier reduces in size to a critical point, its flow stops,
and the ice becomes stationary. Meanwhile, meltwater flows over,
within, and beneath the ice leave
stratified alluvial deposits. Because of
this, as the ice melts, it leaves stratified deposits in the form
of
columns,
terraces and
cluster. These types of deposits are
known as
deposits in contact with ice.
When those deposits take the form of columns of tipped sides or
mounds, they are called
kames. Some
kames form when meltwater deposits sediments through
openings in the interior of the ice. In other cases, they are just
the result of fans or
deltas towards the
exterior of the ice produced by meltwater.
When the glacial ice occupies a valley it can form terraces or
kame along the sides of the valley.
A third type of deposit formed in contact with the ice is
characterized by long, narrow sinuous crests composed fundamentally
of
sand and
gravel
deposited by streams of meltwater flowing within, or beneath the
glacier. After the ice has melted these linear ridges or
eskers remain as landscape features. Some of these
crest have heights exceeding 100
meters and their lengths surpass 100 km.
Loess deposits
Very fine glacial sediments or
rock flour
is often picked up by wind blowing over the bare surface and may be
deposited great distances from the original fluvial deposition
site. These
eolian loess deposits may be very deep, even hundreds of
meters, as in areas of China and the Midwestern United States.
Katabatic winds can be important in
this process.
Transportation and erosion
- Entrainment is the picking up of loose
material by the glacier from along the bed and valley sides.
Entrainment can happen by regelation or
by the ice simply picking up the debris.
- Basal Ice Freezing is thought to be to be made
by glaciohydraulic
supercooling, though some studies show that even where physical
conditions allow it to occur, the process may not be responsible
for observed sequences of basal ice.
- Plucking is the process involves the glacier
freezing onto the valley sides and subsequent ice movement pulling
away masses of rock. As the bedrock is
greater in strength than the glacier, only previously loosened
material can be removed. It can be loosened by local pressure and
temperature, water and pressure release of the rock itself.
- Supraglacial debris is carried on the surface
of the glacier as lateral and medial moraines. In summer ablation,
surface melt water carries a small load and this often disappears
down crevasses.
- Englacial debris is moraine carried within the body of the glacier.
- Subglacial debris is moved along the floor of
the valley either by the ice as ground
moraine or by meltwater streams formed by pressure
melting.
Deposition
- Lodgement till is identical to ground moraine. It is material that is
smeared on to the valley floor when its weight becomes too great to
be moved by the glacier.
- Ablation till is a combination of englacial
and supraglacial moraine. It is released as a stationary glacier
begins to melt and material is dropped in
situ.
- Dumping is when a glacier moves material to
its outermost or lowermost end and dumps it.
- Deformation flow is the change of shape of the
rock and land due to the glacier.
Isostatic rebound
Isostatic pressure by a glacier on the Earth's crust
This rise of a part of the
crust is
due to an
isostatic adjustment. A large
mass, such as an ice sheet/glacier, depresses the crust of the
Earth and displaces the
mantle
below. The depression is about a third the thickness of the ice
sheet. After the glacier melts the mantle begins to flow back to
its original position pushing the crust back to its original
position.
This post-glacial rebound, which lags
melting of the ice sheet/glacier, is currently occurring in
measurable amounts in Scandinavia and
the Great
Lakes
region of North America.
An interesting geomorphological feature created by the same
process, but on a smaller scale, is known as dilation-faulting. It
occurs within rock where previously compressed rock is allowed to
return to its original shape, but more rapidly than can be
maintained without faulting, leading to an effect similar to that
which would be seen if the rock were hit by a large hammer. This
can be observed in recently de-glaciated parts of Iceland.
Glaciers on Mars

Northern polar icecap on Mars
Elsewhere in the
solar system, the vast
polar
ice caps of
Mars
rival those of the Earth and show glacial features. Especially the
south polar cap is compared to glaciers on Earth.
Other glacial
features on Mars are glacial debris aprons and the lineated valley
fills of the fretted terrain in northern Arabia Terra
. Topographical features and computer models
indicate the existence of more glaciers in Mars' past.
Martian glaciers are affected by the thin atmosphere of Mars.
Because of the low atmospheric pressure, ablation near the surface
is solely due to
sublimation, not
melting. As on Earth, many glaciers are covered with
a layer of rocks which insulates the ice. A radar instrument
onboard the
Mars
Reconnaisance Orbiter found ice under a thin layer of rocks in
formations called
Lobate Debris
Aprons (LDA's).
Image:Gullies and tongue-shaped glacier.jpg|Gullies in a crater in
Eridania, north of the large crater Kepler. Also, features that may
be remains of old
glaciers are present.
One, to the right, has the shape of a tongue.
Image:Lobate Debris Apron in Phlegra Montes.JPG|
Lobate Debris Apron in
Phlegra Montes,
Cebrenia quadrangle. The debris apron is
probably mostly ice with a thin covering of rock debris, so it
could be a source of water for future Martian colonists. Scale bar
is 500 meters long.
Image:Moreux Crater moraines.JPG|
Moreux
Crater moraines and kettle holes, as seen by HIRISE.
Image:Tributary Glacier.JPG|Tributary Glacier, as seen by
HiRISE.
See also
Cited references
- *
- Bindschadler, R.A. and T.A. Scambos. Satellite-image-derived
velocity field of an Antarctic ice stream. Science, 252(5003),
242-246, 1991
- What causes the blue color that sometimes appears in snow
and ice ?
- [Benson, C.S., 1961, Stratigraphic studies in the snow and firn
of the Greenland Ice Sheet, Res. Rep. 70, U.S. Army Snow, Ice and
Permafrost Res Establ., Corps of Eng., 120 pp]
- http://folk.uio.no/kaeaeb/publications/grl04_paul.pdf Frank
Paul, et al., 2004, Rapid disintegration of Alpine glaciers
observed with satellite data, GEOPHYSICAL RESEARCH LETTERS,
VOL. 31, L21402, doi:10.1029/2004GL020816, 2004
- Recent Global Glacier Retreat
Overview
- W.S.B. Paterson, Physics of ice
- Hughes, T. West Antarctic ice streams. Reviews of Geophysics
and Space Physics, 15(1), 1-46, 1977
- T. Strozzi et al.: The Evolution of a Glacier Surge
Observed with the ERS Satellites (pdf, 1.3 Mb)
- The Brúarjökull Project: Sedimentary environments of a
surging glacier. The Brúarjökull Project research
idea.
- Meier & Post (1969)
-
http://people.deas.harvard.edu/~vtsai/files/EkstromNettlesTsai_Science2006.pdf
Ekström, G., M. Nettles, and V. C. Tsai (2006)"Seasonality and
Increasing Frequency of Greenland Glacial Earthquakes",Science,
311, 5768, 1756-1758, doi:10.1126/science.1122112
-
http://people.deas.harvard.edu/~vtsai/files/TsaiEkstrom_JGR2007.pdf
Tsai, V. C. and G. Ekström (2007). "Analysis of Glacial
Earthquakes", J. Geophys. Res., 112, F03S22,
doi:10.1029/2006JF000596
-
http://people.deas.harvard.edu/~vtsai/files/TsaiEkstrom_JGR2007.pdf
Tsai, V. C. and G. Ekström (2007). "Analysis of Glacial
Earthquakes", J. Geophys. Res., 112, F03S22,
doi:10.1029/2006JF000596
- Glossary of Glacier Terminology
- C.D. Ollier: Australian Landforms and their
History, National Mapping Fab, Geoscience Australia
- Collins, Henry Hill; Europe and the USSR; p.
263. ISBN 1256350003
- Yukon Beringia Interpretive Center
- Huntington, Ellsworth; The Character of Races;
p. 55. ISBN 040509955X
- Earth History 2001 (page 15)
- On the Zoogeography of the Holarctic
Region
- Kargel, J.S. et al.:Martian Polar Ice Sheets and
Mid-Latitude Debris-Rich Glaciers, and Terrestrial Analogs,
Third International Conference on Mars Polar Science and
Exploration, Alberta, Canada, October 13-17, 2003 (pdf 970
Kb)
- Fretted Terrain: Lineated Valley Fill,
Mars Global Surveyor Mars Orbiter Camera, Malin Space Science
Systems/NASA
- Martian glaciers: did they originate from the
atmosphere?, ESA Mars Express, 20 January 2006
- Head, J. et al. 2005. Tropical to mid-latitude snow and ice
accumulation, flow and glaciation on Mars. Nature: 434.
346-350
- http://www.marstoday.com/news/viewpr.html?pid=18050
-
http://news.brown.edu/pressreleases/2008/04/martian-glaciers
- Plaut, J. et al. 2008. Radar Evidence for Ice in Lobate Debris
Aprons in the Mid-Northern Latitudes of Mars. Lunar and Planetary
Science XXXIX. 2290.pdf
- Holt, J. et al. 2008. Radar Sounding Evidence for Ice within
Lobate Debris Aprons near Hellas Basin, Mid-Southern Latitudes of
Mars. Lunar and Planetary Science XXXIX. 2441.pdf
Uncited references
- An excellent less-technical treatment of all aspects, with
superb photographs and firsthand accounts of glaciologists'
experiences. All images of this book can be found online (see
Weblinks: Glaciers-online)
- An undergraduate-level textbook.
- A textbook for undergraduates avoiding mathematical
complexities
- A textbook devoted to explaining the geography of our
planet.
- A comprehensive reference on the physical principles underlying
formation and behavior.
External links