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 layers they are studying

To identify the layers of the Sun based on temperature data, the astronomers can compare the recorded temperatures to the established temperature profiles of the Sun's layers. The Sun has distinct layers, namely the core, radiative zone, convective zone, photosphere, chromosphere, and corona, each characterized by specific temperature ranges.

For example:

1. **Core**: Approximately 15 million degrees Celsius
2. **Radiative Zone**: Ranges from about 7 million to 2 million degrees Celsius as you move outward
3. **Convective Zone**: Approximately 1.5 million degrees Celsius at the outer boundary
4. **Photosphere**: Around 5,500 degrees Celsius
5. **Chromosphere**: Roughly 4,500 to 25,000 degrees Celsius
6. **Corona**: About 1 to 3 million degrees Celsius, but it can spike to several million degrees Celsius during solar events.

By analyzing their temperature data and determining the specific temperature readings, the astronomers can correlate these values to the known temperature ranges of the Sun's layers. This process allows them to identify which layers they are studying based on the recorded temperatures. For instance, if they measure temperatures around 5,500 degrees Celsius, they can conclude that they are likely observing the photosphere.

In summary, utilizing established temperature profiles of the Sun's layers is a practical method for the scientists to identify which specific layers of the Sun they are studying.