Now we can determine how much mass is converted over the Sun's lifetime (TSun-yr = 1010 years). Mkg = TSun-yr · Δmper-yr Mkg = ?
Now we can determine how much mass is converted over the Sun's lifetime (TSun-yr = 1010 years). Mkg = TSun-yr · Δmper-yr Mkg = ?
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
Problem 1LR
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Now we can determine how much mass is converted over the Sun's lifetime (TSun-yr = 1010 years).
Mkg | = | TSun-yr · Δmper-yr |
Mkg | = | ? |

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How much mass does the Sun convert into energy each second (in kg/s) if its luminosity is 3.84 x 1026 J/s?
How many kilograms of material will it burn during its lifetime (1010 years)?
What percentage of the Sun's total mass is this (M.
= 1.99 x 1030 kg)?
sun
Part 1 of 3
28
Energy is related to mass by:
E =
mc2
If we want to know the mass converted to energy per second, we can express this relation as
Amc²,
and solve for Am, where Am represents the change in mass per second.
Δm
(3 × 108 m/s)?
Am =
4.27e+9
4.27e+09| kg/s
Part 2 of 3
To determine how much mass is converted to energy over the Sun's lifetime, we should convert the amount of
mass converted per second to the amount converted per year.
1 year = 3.154e+7
seconds
Δ ,
per-yr
1.35e+17
kg/year
%D
Now we can determine how much mass is converted over the Sun's lifetime (T.
1010 years).
4)
Sun-yr
Ts
Mkg
Sun-yr · Am,
per-yr
Mkg
kg
8:29 AM
2/21/2021
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