The carbonaceous meteorites represent the mantle of the Earth. Pallesite meteorites are composed of iron and olivine which represents the transition between the core and the mantle.
yes hypothesize is a real word and yes hypothesize is like hypothesis.
Scientists use the difference in density between the inner and outer core as evidence that the inner core is solid. This was proven using seismic waves traveling through the earth.
Regions on Mars that show evidence of past water flow, organic molecules, and potential sources of energy, such as methane, lead scientists to hypothesize that life could have existed on the planet. These conditions resemble those necessary for life on Earth, suggesting that Mars may have once been habitable.
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.
Meteorites that originate from the asteroid belt can collide with Earth, carrying evidence of Earth's inner composition. By analyzing these meteorites, scientists can study the interior structure and composition of our planet.
The carbonaceous meteorites represent the mantle of the Earth. Pallesite meteorites are composed of iron and olivine which represents the transition between the core and the mantle.
Scientists used detectors which determined the mantle existed. As well, scientists must hypothesize and theorize what cannot be readily seen, and make determinations based on the evidence that does exist.
The evidence includes seismic waves, which travel at different speeds and paths through Earth's interior. By analyzing how these waves behave, scientists have determined that Earth has distinct layers such as the crust, mantle, outer core, and inner core. Other evidence comes from the study of meteorites, which provide insight into the composition of Earth's layers.
yes hypothesize is a real word and yes hypothesize is like hypothesis.
Scientists were convinced that some meteorites came from the moon because they contained mineral compositions and isotopic ratios consistent with lunar samples collected during the Apollo missions. The unique characteristics of these meteorites, such as the presence of volcanic glass beads and impact melt breccias, further supported the idea of their lunar origin.
Scientists hypothesize that plants evolved from ancient aquatic green algae that adapted to living on land. This transition is thought to have occurred around 450 million years ago, with plants developing structures like roots, leaves, and vascular tissues to help them thrive in terrestrial environments. Genetic and fossil evidence support the theory of plant evolution from algae.
WikiAnswers doesn't do "fill in the blank" statements very well. Please rephrase this, as Alex Trebeck says, in the FORM of a question.
Scientists use the difference in density between the inner and outer core as evidence that the inner core is solid. This was proven using seismic waves traveling through the earth.
Regions on Mars that show evidence of past water flow, organic molecules, and potential sources of energy, such as methane, lead scientists to hypothesize that life could have existed on the planet. These conditions resemble those necessary for life on Earth, suggesting that Mars may have once been habitable.
i know that this is stupid but how do scientists get empirical evidence.
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.