The total mass of the Sun is about 2 x 1030 kg. of which about 76 % was hydrogen when the Sun formed. However, only about 14 % of this hydrogen ever becomes available for fusion in the core. The rest remains in layers of the Sun where the temperature is too low for fusion. Part A Use the given data to calculate the total mass of hydrogen available for fusion over the lifetime of the Sun. Express your answer using two significant figures. m = kg Submit Request Answer Part B The Sun fuses about 600 billion kilograms of hydrogen each second. Based on your result from part A, calculate how long the Sun's initial supply of hydrogen can last. Give your answer in both seconds and years. Express your answer using two significant figures. t =

Astronomy
1st Edition
ISBN:9781938168284
Author:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Chapter15: The Sun: A Garden-variety Star
Section: Chapter Questions
Problem 23E: Show that the statement that 92% of the Sun’s atoms are hydrogen is consistent with the statement...
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I don't understand these concepts. Could you please explain each step for this 4 part question? 

All 4 parts are use the information in the top left of the 1st image.

The total mass of the Sun is about 2 x 1030 kg, of
which about 76 % was hydrogen when the Sun
formed. However, only about 14 % of this hydrogen
Part A
ever becomes available for fusion in the core. The
rest remains in layers of the Sun where the
temperature is too low for fusion.
Use the given data to calculate the total mass of hydrogen available for fusion over the lifetime of the Sun.
Express your answer using two significant figures.
?
m =
kg
Submit
Request Answer
Part B
The Sun fuses about 600 billion kilograms of hydrogen each second. Based on your result from part A, calculate how long the
Sun's initial supply of hydrogen can last. Give your answer in both seconds and years.
Express your answer using two significant figures.
ΑΣφ
?
t =
S
Transcribed Image Text:The total mass of the Sun is about 2 x 1030 kg, of which about 76 % was hydrogen when the Sun formed. However, only about 14 % of this hydrogen Part A ever becomes available for fusion in the core. The rest remains in layers of the Sun where the temperature is too low for fusion. Use the given data to calculate the total mass of hydrogen available for fusion over the lifetime of the Sun. Express your answer using two significant figures. ? m = kg Submit Request Answer Part B The Sun fuses about 600 billion kilograms of hydrogen each second. Based on your result from part A, calculate how long the Sun's initial supply of hydrogen can last. Give your answer in both seconds and years. Express your answer using two significant figures. ΑΣφ ? t = S
Express your answer using two significant figures.
?
t =
years
Submit
Request Answer
Part D
Given that our solar system is now about 4.5 billion years old, when will we need to worry about the Sun running out of hydrogen
for fusion?
Express your answer using two significant figures.
?
t =
billion years
Transcribed Image Text:Express your answer using two significant figures. ? t = years Submit Request Answer Part D Given that our solar system is now about 4.5 billion years old, when will we need to worry about the Sun running out of hydrogen for fusion? Express your answer using two significant figures. ? t = billion years
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