The deposition of a sequence of sedimentary rocks, the event is the first to occur to produce an angular unconformity is known as weathering.
The formation of sedimentary rocks involves the accumulation or deposition of mineral or organic particles at the Earth's surface, followed by cementation. The mechanisms that lead to the accumulation of these particles are collectively referred to as sedimentation.
In contrast to metamorphic and igneous rocks, which are generated deep beneath the Earth, sedimentary rocks are formed on or around the surface of the planet. Erosion, weathering, dissolution, precipitation, and lithification are the main geological processes that result in the formation of sedimentary rocks.
The majority of the Earth's rocky surface is composed of sedimentary rocks, although these rocks only make up a very minor portion of the planet's crust.
Therefore weathering is the first to occur to produce an angular unconformity.
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#SPJ12
Answer:
weathering
Explanation:
it first weathers then it can erode then be deposited
b. open ocean
c. coastal ocean
d. estuary
d. estuary-“regions along coastlines wherestreams or rivers flow into a bodyof salt water”. They helpprotect coastal land from floodingand erosion; nutrients and biodiversityare highFilled with soil to make land forhuman populations.
A wetlands is correct but b is a bad answer
Shang
Qing
Mughal
Answer:
Option: Meiji
Explanation:
Meiji is considered to be an important time in Japanese history because it came into power after overthrowing the Edo period (feudalism) in Japan. The Meiji period brought changes in society by establishing new political, economic and social institutions. The reforms in Japan influenced by the west. It was during the Meiji Period Japan transformed into modernity by having banks, education institution, industrial production, and military.
Answer:
I believe the answer should be B
Explanation:
This is because a globe is round just like the Earth so it is more accurate than a flat map.
B) White dwarfsC) Galaxies
D) The nebula
Answer:
A) Massive stars
Explanation:
The mass of the star determines how its end will be. The less massive will give rise to nebulas, in whose center a white dwarf will remain, which is a degenerate star that has exhausted all its fuel and is much smaller than its initial volume. And the most massive stars will become stars of neutrons, quarks, or, if they have enough mass, in black holes. For a star to end its days in the form of a neutron star it is necessary that it has a mass of at least 1.44 solar masses. This value is known as the "Chandrasekhar limit", and we owe it to the Indian astrophysicist Subrahmanyan Chandrasekhar, when we talk about neutron star we mean that it can lead to the formation of other objects
For a star to end its days in the form of a star of quarks or a black hole it is necessary that its mass be even greater. This value is set by the "Tolman-Oppenheimer-Volkoff limit", currently established by astrophysicists at approximately 2.17 solar masses. Everything we have seen so far about the life of the stars is very important because it can help us understand the phenomenon that causes the formation of a black hole.