Lobate pattern of glaciation

He continued: The superficial aspect of the formation is that of an irregular, intricate series of drift ridges and hills of rapidly, but often very graceful, undulating contour, consisting of rounded domes, conical peaks, winding and occasionally geniculated ridges, short, sharp spurs, mounds, knolls, and hummocks, promiscuously arranged, accompanied by corresponding depressions, that are sometimes even more striking in character.

On moraine loops: It is disposed in a series of great loops which give to the whole a peculiar arcuate expression. A remarkable peculiarity is the extraordinary fact that the lateral portions of these great loops do not simply join, forming re-entrant angles, but coalesce and are prolonged sometimes a hundred miles (160 km) or more between the lobate areas embraced by the loops, forming a peculiar morainic type, to which the term intermediate or interlobate moraines will be applied. (p. 313) Chamberlin recognized twelve such great loops (lobes) encompassing broad valleys in the northern United States--see Table 8-1.

	Hudson River, New York: NASA space-shuttle photo, STS58-81-038, 70 mm format. Low-oblique view toward northwest over Long Island, New York City, Hudson River, and Catskill Mts. Reddish-brown color shows autumn foliage of forest in Catskills, October 1993. During the late Wisconsin glaciation, an ice lobe extended southward along the Hudson valley and reached a maximum position marked by end moraines on Long Island and Staten Island. NASA Johnson Space Center, Imagery Services.
	Finger Lakes, New York: NASA space-shuttle photo, STS51B-33-028, 70 mm format, 4/85. Near-vertical view of Lake Ontario and New York Finger Lakes. Finger Lakes occupy deep, ice-carved valleys that diverge southward from the Ontario basin. South of the Finger Lakes, a network of river valleys marks the path of ice-marginal melt-water drainage related to the Ontario ice lobe. NASA Johnson Space Center, Imagery Services.
	Lake Michigan and Green Bay, WI/MI: NASA space-shuttle photo, STS28-153-22, 5-inch format, 8/89. High-oblique view toward southwest over Lake Michigan and Green Bay (right of lake). Large ice lobes followed both basins toward the south; ice flow was split by bedrock high that forms Green Bay peninsula and islands to the north. NASA Johnson Space Center, Imagery Services.
	Prairie Coteau, MN/SD: NASA space-shuttle photo, STS36-152-110, 5-inch format, 3/90. Near-vertical view of Coteau des Prairies, eastern South Dakota and western Minnesota. Lakes are frozen, but ground is snow free in this late winter scene. The prominent light-colored zone along the eastern edge is the Bemis Moraine, which formed along the western side of the Des Moines lobe during late Wisconsin glaciation. Small elongated lakes in the moraine occupy tunnel valleys that were eroded by melt water flowing out from beneath the ice lobe. NASA Johnson Space Center, Imagery Services.

1. A broad depression, reaching well backward along the line of glacial movement, was effective in producing prolongations of the ice (p. 183). Horberg and Anderson (1956) reached a similar conclusion, noting that bedrock topography was most important for controlling the form of ice lobes. Broad, bedrock troughs of the Great Lakes are prime examples of this phenomenon--a major ice lobe was active in each.

   Great Lakes, United States and Canada: NASA space-shuttle photograph, STS064-54-022, 9/94, 5-inch format. High-oblique view toward southwest with sunglint from lake surfaces; Lake Ontario to left, Lake Michigan to far right. Great Lakes basins were eroded by large ice lobes that spread southward from the Laurentide Ice Sheet. NASA Johnson Space Center, Imagery Services.

2. In glacial flow as applied to the marginal portions of the ice ... the movement was essentially at right angles to the border (p. 184). Thus, ice movement ascended from basins toward highlands; a radial or divergent flow pattern developed in the ice lobes.

3. Ice overriding in a deep current covering all topographic features will be less affected by these topographic features, which produce deflections only in the basal ice flow.

   Memorial plaque to T.C. Chamberlin on a large erratic boulder, University of Wisconsin, Madison. Chamberlin's service to Wisconsin and geology are commemorated on this monument. Photo © by J.S. Aber.

The shape, thickness, and rate of movement of a glacier lobe are controlled by many variables--substratum topography, ice supply from interior of ice sheet, basal melt-water conditions, nature of substratum sediment, permafrost, etc. Two general forms of ice lobes were developed along the southern margin of the Laurentide ice sheet (Clark 1992).

• Relatively thick lobes with steep margins, such as the Green Bay lobe. These lobes presumably advanced over permafrost by a combination of plastic flow and limited basal sliding. Such lobes were able to maintain continued movement for an extended period of time, which resulted in well-developed drumlin fields, lacking eskers and tunnel valleys, behind end moraines.

• Relatively thin lobes with gentle margins, such as the Lake Michigan lobe. These lobes advanced rapidly over thawed ground by surging on water-lubricated beds or deforming beds. Repeated advances alternated with ice stagnation; hummocky moraine, eskers, tunnel valleys and other geomorphic features of stagnant ice are common. Some ice lobes, that were thick and slow during early phases of ice advance, changed to thin and fast lobes during later stages of glaciation (Patterson 1993).

1. Outer zone: Thick and nearly continuous glacial sediment of various kinds, large end moraines, much ice-push deformation of soft substratum. Plains and lowlands located beyond shield/mountain areas and underlain by sedimentary bedrock; may also be found in interior positions. Lobate style of glaciation is the rule with multiple tills and interglacial deposits commonly preserved.

   	Thick sequence of glacial strata exposed in Golden Valley bluffs, near Medicine Hat, Alberta. The bluffs reveal >80 m of glacial sediments that form a blanket, which buries the preglacial landscape of southern Alberta. Photos © by J.S. Aber.
   	Streeter Moraine in Logan County, southeastern North Dakota. This moraine is located on the Missouri Coteau; it was formed along the western margin of the James ice lobe. The moraine contains many large ice-shoved hills, like the example seen on the horizon.
   	Glacial sequence exposed in quarry near Freienwalde, northeastern Germany. The light-colored mass at top is a bedrock raft (megablock) of Oligocene glimmersand (micaeous sandstone) that was thrust over the brown-colored glacial sediment underneath.
   	Cape Cod, Massachusetts: NASA space-shuttle photograph, STS071-708-040, 07/06/95, 70 mm format. Low-oblique view toward northwest. Cape Cod, Nantucket, Martha's Vineyard, and other offshore islands consist of moraines and ice-shoved hills built along the margins of ice lobes during the late Wisconsin glaciation, around 18,000 to 20,000 years ago. NASA Johnson Space Center, Imagery Services.

2. Intermediate zone: Thin and discontinuous glacial sediment with large areas of exposed basement rocks. Located in shield/mountain areas of crystalline bedrock. Long eskers and glacial lineaments, but few end moraines and little ice-push deformation. Deposits date mainly from final phases of the last glaciation.

   	View over crystalline shield terrain, Stockholm, eastern Sweden. The hill top is exposed bedrock without any sediment or soil cover. Lower on the hill sides, thin moraine cover is present--see next photo. This bedrock landscape is typical of the intermediate zone of glaciation.
   	Closeup view of thin moraine cover on lower portion of bedrock hill. The sediment is only one boulder-layer in thickness.

3. Inner zone: Moderately thick and continuous glacial sediment with ribbed and Rogen moraine, drumlins, and common ice-push deformation (Aber and Lundqvist 1988). Central shield/mountain areas and/or sedimentary substratum. Crust was depressed 100s of m; multiple tills and deposits predating last glaciation are commonly preserved.

   	Andersön, a small drumlin (background) within Storsjön lake, central Sweden. Glacial sediment forms a near-continuous cover in foreground. The drumlin and sediment cover are typical of the inner zone of glaciation--see next photo.
   	Closeup view of exposure on side of Andersön drumlin. Fine sand/silt is folded around a core of coarse gravel. Overriding ice molded the ice-pushed hill into a small drumlin. Ice movement from right to left; scale pole is 2 m long.

Glacial landscape patterns on Mars

The infamous canals of Mars are really giant valleys eroded by immense water floods. These floods were triggered when episodic volcanism melted large volumes of permafrost in the Tharsis Bulge region. The floods scoured channel networks leading to a large basin in the northern hemisphere, in which Oceanus Borealis was formed. Oceanus Borealis covered up to 40 million km² with an average water depth of about 1700 m (1 mile). Such oceans may have formed repeatedly following major volcanic outbursts.

During each oceanic phase, a mild climate with moderate greenhouse effect came into being. Water vapor was circulated in the atmosphere around the planet. Snowfall and glacier formation occurred in the southern hemisphere resulting in a vast Austral Ice Sheet. The array of glacial landforms present on Mars bears a striking similarity to glacial features of the Earth. The mild climatic episodes on Mars evidently were short-lived, however, because volcanism was not continuous. The climatic history of Mars apparently consisted of long, cold intervals of permafrost punctuated by short, mild, oceanic/glacial episodes. The final glacial epoch took place late in martian history, not less than about 100,000 years nor greater than 20 million years ago (Kargel and Strom 1992).

The ultimate failure of Mars' episodic greenhouse climate can be attributed to the planet's small size. The planet's interior cooled early in its history, and volcanic emission of CO₂ became intermittent. Weak gravity allowed much of the atmosphere to escape, so that a permanent greenhouse effect and mild climate could not become established.

This volcanic-climatic scenario along with the chance of martian life remain highly controversial subjects among planetary scientists and the public. The possibility of past life on Mars has major theological as well as scientific implications. A series of NASA missions are designed to collect data from martian atmospheric and surficial environments. These unmanned missions may culminate ultimately in manned expeditions by the mid-21st century. Only then could we firmly establish the evidence for past glaciation and the possibility of ancient life on Mars.