Two astronomers are viewing temperature data from each of the sun's layers, but the layers aren't identified. Describe one way the scientists can use temperature to identify which layer they are studying.(1 point)

Responses

The highest temperatures are from the corona.
The highest temperatures are from the corona.

The lowest temperatures are from the core.
The lowest temperatures are from the core.

The highest temperatures are from the radiative zone.
The highest temperatures are from the radiative zone.

The lowest temperatures are from the photosphere.

One way the scientists can use temperature to identify which layer they are studying is by observing that the highest temperatures are from the corona.

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Apply the Quotient Rule of Integer Exponents to simplify 23 to the power of 65÷ 23 to the power of 32

To simplify (23^65)/(23^32), we can use the quotient rule of exponents, which states that when dividing two numbers with the same base, we subtract the exponents. In this case, the base is 23, and the exponents are 65 and 32.

Using the quotient rule, we have:
(23^65)/(23^32) = 23^(65-32) = 23^33

Therefore, (23^65)/(23^32) simplifies to 23^33.

The highest temperatures are from the corona.

To identify which layer they are studying based on temperature, the astronomers can analyze the temperature data and look for certain patterns or characteristics that are specific to each layer of the Sun. Here are two possible approaches the scientists can use:

1. Comparing temperature profiles: The astronomers can examine the temperature data from different layers of the Sun and compare them. They can look for a significant increase or peak in temperature in one layer compared to the others. In this case, if they observe the highest temperatures in a particular layer, such as the corona, they can conclude that they are studying the corona.

2. Referencing known temperature ranges: Scientists have already established temperature ranges for different layers of the Sun based on previous studies and observations. For example, the core is known to have extremely high temperatures, while the photosphere has comparatively lower temperatures. The astronomers can compare the temperature data they are analyzing with these known temperature ranges. If they find that the temperatures fall within the expected range for a specific layer, they can identify that they are studying that layer.

By using one or both of these methods, the scientists can confidently identify which layer of the Sun they are studying based on the temperature data.