DEPOSITION
The term that refers to sediment deposited by glacier ice is "glacial till." This material is typically a mixture of various sizes of particles, ranging from clay to boulders, and is formed as glaciers advance and retreat. Glacial till is unsorted and unstratified, contrasting with sediment deposited by water, which tends to be sorted by size.
Glacial till is a type of sediment deposited by glaciers through the process of erosion and transportation. It is a mixture of different sized particles, ranging from clay to boulders, that is left behind as the glacier melts. Glacial till is an unsorted and unstratified deposit.
The boulders, sand, clay, and silt that are deposited by a glacier as it slows down and melts are called glacial till. This material is unsorted and varies in size, ranging from large boulders to fine silt. Glacial till is often found as moraines, which are accumulations of debris along the edges or at the terminus of a glacier.
The rings of Saturn consist of ice particles ranging in size from microscopic dust to large boulders. The particles are believed to be remnants of comets, asteroids, or moons that were shattered by collisions with other objects.
Conglomerate rocks can vary in size, ranging from pebble-sized particles to larger boulders. The size of the particles in a conglomerate rock depends on the transportation distance and energy of the environment in which they were deposited.
The term that refers to sediment deposited by glacier ice is "glacial till." This material is typically a mixture of various sizes of particles, ranging from clay to boulders, and is formed as glaciers advance and retreat. Glacial till is unsorted and unstratified, contrasting with sediment deposited by water, which tends to be sorted by size.
Glacial till is a type of sediment deposited by glaciers through the process of erosion and transportation. It is a mixture of different sized particles, ranging from clay to boulders, that is left behind as the glacier melts. Glacial till is an unsorted and unstratified deposit.
The boulders, sand, clay, and silt that are deposited by a glacier as it slows down and melts are called glacial till. This material is unsorted and varies in size, ranging from large boulders to fine silt. Glacial till is often found as moraines, which are accumulations of debris along the edges or at the terminus of a glacier.
Saturn is the outer planet that has rings. Its rings are composed of ice, rock, and dust particles ranging in size from small grains to boulders.
The rings of Saturn consist of ice particles ranging in size from microscopic dust to large boulders. The particles are believed to be remnants of comets, asteroids, or moons that were shattered by collisions with other objects.
Conglomerate rocks can vary in size, ranging from pebble-sized particles to larger boulders. The size of the particles in a conglomerate rock depends on the transportation distance and energy of the environment in which they were deposited.
Glacial sediment is called "glacial till." It consists of a mixture of rock debris, ranging from fine silt to large boulders, that is deposited directly by glacial ice as it melts. This sediment is typically unsorted and unstratified, reflecting the chaotic nature of glacial movement. In addition to till, glacial sediments can also include other forms like outwash, which is sorted material carried away by meltwater.
The Wentworth scale measures the grain size of sedimentary rocks, which refers to the diameter of the particles that make up the rock. The scale categorizes sediment grains into different size classes ranging from boulders to clay particles.
No. None of the inner four planets have rings.
ice, rock, and dust ranging in size from tiny grains to large boulders. These particles can vary in composition and are constantly colliding and breaking apart, creating the intricate structure of Saturn's rings that we observe.
Yes, Saturn is famous for its prominent ring system, which is composed of icy particles and debris ranging in size from dust grains to boulders. These rings are visible from Earth through a telescope and play a key role in the planet's unique appearance.
The Wentworth scale of grain size measures the average diameter of particles in sedimentary rocks, ranging from clay (less than 0.002 mm) to boulders (more than 256 mm). It helps geologists classify sedimentary rocks based on the size of the particles they are composed of.