Carbonaceous chondrites are very low in iron, which is different than meteorites which have a high iron content. Stone meteorites also have high levels of iron in them.
wieners
Meteorites are valuable to geologists because they provide insights into the early stages of the solar system and the formation of planets. They can help determine the age of the Earth and other celestial bodies, as well as provide evidence of past geological processes, such as impacts and volcanic activity. Meteorites also contain unique mineral compositions and isotopic ratios that can be studied to understand the chemical evolution of the solar system.
There could be sedimentary rocks on the Moon, the processes forming them would be different from those on the earth but it is possible that there are processes moving and layering Moon dust which could be regarded as a sediment. However, in general there is no erosion or deposition happening on the Moon as it does on Earth and therefore no rocks formed as a result of these processes.
asteroids, comets, planets, stars, galaxies, black holes, red dwarfs, moons, meteors, unidentified space objects, and much more that scientists have not even discovered. Everything that ever existed. Well, it all started with 98% Hydrogen and Helium, and through various processes (e.g. stellar nucleosynthesis), formed the other elements. so I guess that could be one answer...
A chromosome controls cell processes by biological processes such as mitosis and meiosis. These cell processes are what direct cell processes such as cell growth and division.
meteorites water flow and death
wieners
Asteroids and gravity create the surface features on the moon.
Asteroids and gravity create the surface features on the moon.
Petroleum coke (Pet coke or petcoke) is a carbonaceous solid that is derived from oil refinery coker units or other cracking processes. It is over 90% carbon.
Meteorites are valuable to geologists because they provide insights into the early stages of the solar system and the formation of planets. They can help determine the age of the Earth and other celestial bodies, as well as provide evidence of past geological processes, such as impacts and volcanic activity. Meteorites also contain unique mineral compositions and isotopic ratios that can be studied to understand the chemical evolution of the solar system.
There could be sedimentary rocks on the Moon, the processes forming them would be different from those on the earth but it is possible that there are processes moving and layering Moon dust which could be regarded as a sediment. However, in general there is no erosion or deposition happening on the Moon as it does on Earth and therefore no rocks formed as a result of these processes.
The material that forms rocks ultimately does come from asteroids. But the rocks on earth have been destroyed, re-formed, and altered numerous times by geologic processes, so it would be erroneous to say they are "made of asteroids." As to how: The planets originated from a disk of gas and dust orbiting the young sun. The dust coalesced into larger particles, which eventually grew into asteroids. These asteroids collided with one another, forming larger and larger bodies. Some of these became planet-like objects called planetesimals, which collided to form proto-planets. Eight of these proto-planets eventually became the planets we know today, including Earth.
Uniformitarianism is a principle that geologic processes that occurred in the past can be explained by current geologic processes. So, it is the idea that the same geologic processes that same Earth today have been at work during all of Earth's history. Catastrophism is a principle that states that geologic change occurs suddenly. Catastrophies include floods, asteroids, earthquakes, etc. Today, modern geology is based on the idea that gradual geologic change is interrupted by catastrophies.
processes in observing processes in identifying processes in desribing processes in comparing processes in classyfying processes in inferring processes in guessing processes in preducting processes in hypothesizing processes in measuring processes in experamenting
Olivine is one of the most abundant minerals in the Earth's upper mantle, comprising up to 50% of some mantle rocks. It is also common in meteorites and on the Moon and Mars. However, it is less common on the Earth's surface due to weathering processes that break it down into other minerals.
The largest moons in our solar system are subjected to various processes. For example, tidal forces from their parent planet can lead to tidal heating, causing geological activity and volcanism. Impact cratering from collisions with asteroids or other objects can also occur. Additionally, some moons may experience geological processes such as tectonic activity, cryovolcanism (volcanic activity with water or ice instead of molten rock), and erosion caused by the moon's own atmosphere or external factors.