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books
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words
š§
Mass-Luminosity Relation
The more massive
star
s are generally the more luminous
Luminosity
varies as the fourth power of the
mass
Can be used to find the distance to
binary star
systems
Formula
L
L
s
u
n
=
(
M
M
s
u
n
)
a
\frac{L}{L_{sun}} = (\frac{M}{M_{sun}})^a
L
s
u
n
ā
L
ā
=
(
M
s
u
n
ā
M
ā
)
a
L
s
u
n
L_{sun}
L
s
u
n
ā
and
M
s
u
n
M_{sun}
M
s
u
n
ā
are the
luminosity
and
mass
of the
Sun
1
<
a
<
6
1 < a < 6
1
<
a
<
6
Star
Astronomy