Hello!
Kepler's Third law helps us here. It states, in the general form, that for two bodies orbiting each other
where is the period,
is the (mean) distance,
and
are the masses and
is the gravitational constant.
We'll use this law twice, for the given system of two stars and for the system Earth+the Sun. For the latter we can neglect the mass of Earth. So we have
...
Hello!
Kepler's Third law helps us here. It states, in the general form, that for two bodies orbiting each other
where is the period,
is the (mean) distance,
and
are the masses and
is the gravitational constant.
We'll use this law twice, for the given system of two stars and for the system Earth+the Sun. For the latter we can neglect the mass of Earth. So we have
where is the given stars' period,
is the distance between stars,
is their combined mass which we have to find,
is the Earth's period (1 year),
is the distance between Earth and the Sun, and
is the mass of the Sun.
Actually we are asked to find which is equal to
(times, dimensionless).
So the answer is: the combined mass of the 2 stars is 22.5 solar masses.
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