What is the Semi Major Axis of a Binary Star System?

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To calculate the semi-major axis (SMA) of a binary star system, one must consider the distances of both stars from the center of mass. In the example given, with star A at 50 AU and star B at 100 AU, the SMA is not simply the halfway point but rather the average distance weighted by their masses. A circular orbit does have a semi-major axis, which is equivalent to the radius in this case. If the stars maintain constant speeds, the distance between them remains constant, and this distance can be considered the SMA. The discussion highlights the importance of understanding orbital mechanics in binary systems.
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need help please in calculating semi major axis(SMA) of a binary star..
if for example
the orbital distance of star A is 50AU and star B is 100 AU from the centre of mass what would the SMA be?

is it as simple as the half way point ? ie 75AU?

thanks in advance
 
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thanks for the link, i have had good rethink re. this..
can a binary system that has a circular orbit have a SMA?
or is that called a radii when it is not elliptical?
so for the question concerned would the SMA simply be 100AU?
cheers
 
if the speeds of the 2 stars are constant, would r ( distance between M and m fig. b ) remain the same .

if so would r be the SMA? and not the distance between the centre of mass and the orbit of m (fig. a)?

oh i am getting confused!
 

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From the article I linked above :

For the special case of a circle, the semi-major axis is the radius.

If this is a simple two body problem with no other objects then the distance between M and m would stay the same.
 
many thanks for your guidence!
 
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