Sentences with phrase «orangeburg scarp»

Though careless with individual lives, she seems careful with the type, but no: «From scarped cliff and quarried stone / She cries, «A thousand types are gone: / I care for nothing, all shall go.

Scarping out the flesh when you don't own a true coconut flesh scarier thingy is not the easiest task... I went back and forth between a grapefruit spoon and a zester until I had enough for this salad.

When squash is done, using a fork scarp the squash to release the strands.

Add to a blender and blend on low, scarping down the sides.

As early as 4 years old I was using watercolors, playing with my mother's fabric scarps and spending a lot of time outside looking at plants and day dreaming about creating something with all the natural color I saw.

The authors use LiDAR and field data to identify linear scarps, sags, and swales that cut across both bedrock and Quaternary deposits along the Leech River fault.

This raisin - like shrinkage occurred no more than 1 billion years ago, based on the age of pre-existing small craters that the scarps run through (Science, DOI: 10.1126 / science.1189590).

It is the longest such scarp to be discovered on Mercury.

A 1000 - kilometre - long cliff, or scarp, though to be formed as Mercury's surface contracted, was found, cutting across the rim and floor of the Rembrandt basin.

A 20 - mile (32 - kilometer) crater west of Dantu is covered in steep slopes, called scarps, and ridges.

Images from the Lunar Reconnaissance Orbiter (LRO) spacecraft, released in October, show a pattern of cliffy scarps all across the lunar surface (as shown on the map above, with white dots indicating newly discovered scarps and black dots marking previously known ones).

Lunar geologists reckon that the scarps were created as the moon's core lost heat and contracted.

Examination of some of the scarps with MRO's Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) confirmed that the bright material is frozen water.

The craft has also spied many new «scarps,» or faults, extending hundreds of kilometers.

These eight scarps, with slopes as steep as 55 degrees, reveal new information about the internal layered structure of previously detected underground ice sheets in Mars» middle latitudes.

The new ice - scarp studies confirm indications from fresh - crater and neutron - spectrometer observations that a layer rich in water ice begins within just one or two yards of the surface in some areas.

The scarps directly expose bright glimpses into vast underground ice previously detected with spectrometers on NASA's Mars Odyssey (MRO) orbiter, with ground - penetrating radar instruments on MRO and on the European Space Agency's Mars Express orbiter, and with observations of fresh impact craters that uncover subsurface ice.

Such a scarp runs vertically along the right edge of the image (bottom), which encompasses a horizontal extent of about 200 kilometers.

Dundas and co-authors say that banding and color variations apparent in some of the scarps suggest layers «possibly deposited with changes in the proportion of ice and dust under varying climate conditions.»

Scientists have not determined how these particular scarps initially form.

«If you had a mission at one of these sites, sampling the layers going down the scarp, you could get a detailed climate history of Mars,» suggested MRO Deputy Project Scientist Leslie Tamppari of NASA's Jet Propulsion Laboratory, Pasadena, California.

Researchers who located and studied the scarp sites with the High Resolution Imaging Science Experiment (HiRISE) camera on MRO reported the findings today in the journal Science.

To reproduce the vertical collapse of landslide material in the landslide scarp area and the extreme thinning and runout in the front, the model must take into account the presence of ice in the calculations.

The side of Pluto's largest moon viewed by NASA's passing New Horizons spacecraft in July 2015 is characterized by a system of «pull apart» tectonic faults, which are expressed as ridges, scarps and valleys — the latter sometimes reaching more than 4 miles (6.5 kilometers) deep.

While the erosional scar can heal rather quickly, Simms noted, initially the coast is reshaped due to newly formed channels, cuts and scarps.

At 80 million years ago, wind would have caused this scarp to migrate across the surface and the rock below the scarp would have gone from being buried — and safe from cosmic rays — to exposed,» Farley explains.

Geologists have developed a relatively well - understood model, called the scarp retreat model, to explain how this type of environment evolves.

Over time, as wind blows sand against the small cliffs, or scarps, that bound the Yellowknife outcrop, the scarps erode back, revealing new rock that previously was not exposed to cosmic rays.

Russell's team also noticed a variety of colors and minerals on the asteroid's surface, with bright spots — perhaps crystals or another reflective material — interspersed with black streaks on scarps and crater walls.

But one of these old beaches, the Pliocene - era Orangeburg Scarp, warps and bends along its course from Florida to North Carolina.

A model that doesn't consider the asthenosphere would show the Orangeburg Scarp sinking.

Geologists examine a section of the Orangeburg Scarp along the James River in Virginia.

«But clearly, the Orangeburg Scarp is going up,» Rowley says.

The shape of the lakes indicates a process called uniform scarp retreat, where the borders of the lakes are expanding by a constant amount each time.

Yeats said Gwadar is several hundred kilometers southwest of the earthquake's epicenter, making it highly unlikely that the new island is a fault scarp.

The older, more cratered surfaces of Lutetia also feature a variety of roughly parallel, curvilinear features, including scarps, troughs, fractures, faults, grooves and pit chains.

The height of the scarp surrounding the upper island is about 400 meters (1,300 feet), while the scarp surrounding the southern island is about 600 meters (2,000 feet) high.

As ice withdraws from a region, wind exposes the layers sculpting valleys and scarps.

Lobate scarps are cliffs caused by thrust faults that have broken the surface and reach up to a height of nearly two miles.

In order to determine how Mercury may have shrunk, the researchers studied tectonic features, called lobate scarps, and wrinkle ridges on the planet, which result from interior cooling and surface compression.

The new inset takes us a step closer, revealing craters, rills and scarps reminiscent of Mercury or even Earth's Moon.

The scarps are cliffs that expose and provide access to the subseafloor, without the need for drilling, making it easier to tease out what is living at depth in oceanic crust.

The sides of abyssal hills are fault escarpments (or scarps) created by vertical uplift of the seafloor during many events of fault slippage that produce frequent earthquakes.

These low - altitude images revealed small fault scarps that are orders of magnitude smaller than the larger scarps.

«These steep banks or slopes, which are known as scarps, currently only change very slowly from year to year, retreating by a few millimeters and getting a bit dustier in the summer.»

«The young age of the small scarps means that Mercury joins Earth as a tectonically active planet, with new faults likely forming today as Mercury's interior continues to cool and the planet contracts,» said lead author Tom Watters, Smithsonian senior scientist at the National Air and Space Museum in Washington, D.C.

This shrinking produced a wrinkled crust with scarps kilometers high and hundreds of kilometers long.

Mercury is marked with great curved cliffs or lobate scarps that were apparently formed as Mercury cooled and shrank a few kilometers in size.

That shape suggests that the lakes were formed by what scientists call «uniform scarp retreat,» in which whole stacks of rock are eroded away to form cliffs.

A jagged scarp, or wall of cliffs, known as Piri Rupes borders the young, nearly crater - free plains of Piri Planitia.