Observations versus Model-Based Statements about the Sun

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Homework Help Overview

The discussion revolves around understanding the internal fusion rate of the Sun and how various observations can validate the solar model that predicts temperature and density at different depths. Participants are exploring the relationship between observed phenomena and theoretical predictions regarding solar fusion.

Discussion Character

  • Conceptual clarification, Assumption checking, Exploratory

Approaches and Questions Raised

  • Participants discuss which observations can be used to verify the solar model's predictions, including total energy output, neutrino measurements, and other factors. There is a debate about the relevance of the Sun's mass and surface phenomena to the fusion rate.

Discussion Status

Some participants have provided insights into the relationship between energy output and fusion reactions, while others question the applicability of certain observations, such as the Sun's mass and solar wind effects. The conversation is ongoing, with various interpretations being explored.

Contextual Notes

There is mention of the original poster's confusion regarding the correct observations to select, indicating a potential gap in understanding the connections between the solar model and observable data.

lbtocth
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A solar model is used to calculate the expected temperature and density at all depths within the Sun. These results are then used to calculate the expected fusion rate within the Sun. We have confidence that the model is correct because it agrees with the observed characteristics of the Sun. Which of the following observations can be used to check that we really do know the Sun’s internal fusion rate?
Select all that apply.

-Measurements of the Sun’s total energy output into space
-Measurement of the Sun’s mass
-Observations of neutrinos coming from the Sun
-Observations of the total X-ray emission from the Sun’s corona
-Measurements of the varying number of sunspots on the Sun over time

Note: I keep getting the wrong answer. I need help.
 
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The total energy output matches the energy released in fusion reactions, so that's working for sure.
We also know the relative importance of fusion reactions, so measuring the neutrinos we can calculate the fusion rate.

The Sun's mass doesn't tell us the fusion rate (or just indirectly via the model that we want to test), and other surface/corona effects are not linked to the fusion rate.
 
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mfb said:
The Sun's mass doesn't tell us the fusion rate
Well I am no good in fusion/fission but aren't the nuclear reactions of Sun converting mass to energy so if we know the rate of decrease of mass, we know the rate of energy radiated?
 
You would have to subtract the mass loss from solar wind, and it's a difficult measurement - in principle yes, but that's not what the question is about.
 
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