How do scientists know the structure of other planets in the solar system?
We can also use things like radar (radio waves) to 'see' beneath clouds.
The majority of gases exhibit radio wave transparency, which enables us to identify structures that are typically hidden beneath clouds. This also holds true to some extent for other wavelengths, such as ultraviolet and infrared.
In essence, we get a reflection from a sudden change in density (e.g., gas to solid), and this can be detected by an orbiting spacecraft or a powerful telescope. The specifics vary depending on the material of the clouds.
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Scientists determine the structure of other planets in the solar system through a combination of methods, including remote sensing from orbiters and probes, seismic data analysis, gravitational measurements, and mathematical modeling based on observations and theoretical principles.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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