A maria
When the outer surface of the Moon cooled, it solidified to form a crust over the molten interior, leading to the formation of the Moon's solid landscape. This cooling process caused the surface to contract, creating features like cracks and ridges. Additionally, volcanic activity occurred in some regions, resulting in the formation of lunar maria—dark basaltic plains. Over time, impacts from asteroids and comets further shaped the Moon's surface, creating craters and other geological features.
after collisions subsided, the earth's surface was able to cool, but the interior remained hot
Hot molten rocks from the interior of the earth are called magma when they are beneath the earth's surface and lava when they reach the surface through volcanic eruptions.
The surface of a mineral can appear a different color than its interior due to a variety of reasons such as weathering, surface impurities, or oxidation. These factors can alter the mineral's chemical composition or structure, leading to a change in color at the surface compared to the interior.
A large body of air that has relatively uniform temperature and humidity characteristics is known as an air mass. Air masses form over regions where the air remains relatively stationary for an extended period, acquiring the properties of the underlying surface, such as deserts or oceans. They can be classified into different types, such as tropical, polar, maritime, and continental, depending on their source regions. When air masses move, they can interact with one another and lead to various weather phenomena.
Maria, also known as lunar seas, are the dark relatively flat regions of the moon's surface that were formed when interior lava filled large basins.
The dark-colored, relatively flat regions of the Moon's surface are called lunar maria. These maria were formed when basins on the Moon were filled with basaltic lava following impact events in the past.
The dark-colored, relatively flat regions of the moon's surface that were formed when interior lava filled large basins are called lunar maria. These areas appear darker than the surrounding highlands due to their lower reflectivity and lack of craters. The lunar maria are thought to have formed from ancient volcanic activity on the moon.
craters
the regions are, in order from surface to center: the surface, which is 10,000 degrees F. then there is the convection zone, then the radiation zone. Finally, we reach the core which is 27,000,000 degrees F.
A plateau is a large, flat area commonly found in the interior of continents. Plateaus are typically elevated landforms with a relatively flat, level surface that rise above the surrounding terrain. They are formed by geological processes such as faulting, volcanic activity, or erosion.
The lunar maria (singular: mare) are large, dark, basaltic plains on Earth's Moon, formed by ancient volcanic eruptions.no that won't fit in my crossword _ _ _ _ amaria
The Sun's interior is composed of the core, radiative zone, and convective zone. The core is where nuclear fusion occurs, generating the Sun's energy. The surface of the Sun is known as the photosphere, which emits light and heat into space.
The Mercator map projection does not represent area correctly. the equatorial regions are relatively small and the polar regions relatively large (if Greenland looks larger than Australia then the area proportions are wrong Australia has more than three times the surface area of Greenland).
The sun's radiation heat to the surface of the entire Earth is approximately 2,500 times greater than the heat coming from the Earth's interior. This is due to the immense energy output of the sun compared to the relatively smaller amount of heat generated within the Earth.
Earth's surface is free to radiate heat into space. The interior is not. The interior does transfer heat the the surface, but rather slowly. It is hot due to residual heat from Earth's formation and from the heat generated by the decay of radioactive elements.
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