Precisely similar effects must be produced by the loss of weight in the
two components of a binary star. Here both components are radiating
away energy, and so are simultaneously losing weight. Detailed
calculation shews that they must continually recede from one another,
but that the shape of their orbit will undergo no change.
Neither separately nor in combination do the two effects just described
explain either the shapes or the sizes of the observed orbits of binary
stars as a whole. To interpret these we must call on yet a third
agency, the gravitational forces from passing stars. We have already
seen how these account for the statistical distribution of orbits which
is actually observed.
The combination of all three agencies, tidal friction, extending over
millions of years, loss of weight, extending over millions of millions
of years, and disturbance from passing stars, extending over a similar
period, is responsible for the evolution of binary star systems. Their
aggregate effect is to widen the distance between the two stars, while
at the same time knocking the orbit out of shape.
SUBDIVISION. While these changes are going on in the orbital
arrangement of a binary system, the two components are themselves
changing their physical condition on account of their continual loss
of weight, and, as with the parent stars, this loss of weight will
generally result in a shrinkage in the size of the star. The shrinkage
of either component of the system causes its shape to run through the
sequence of configurations we have already enumerated, and if the
shrinkage continues for long enough, the component may end by further
dividing into two separate masses. Either or both of the constituents
of a binary system may subdivide into binary sub-systems in this way,
resulting in a system of either three or four stars. H. N. Russell
has shewn mathematically that when a binary system _P_, _Q_ divides
into a triple system, _P_, _q_, _qʹ_, through _Q_ breaking up into two
constituents _q_, _qʹ_, the distance between _q_ and _qʹ_ cannot be
more than about a fifth of the original distance _PQ_. This theoretical
law is well confirmed by observation. Fig. 13 shews a typical multiple
system, and we notice that the separations in each of the various
sub-systems are all quite small in comparison with those of the main
systems.
[Illustration: Fig. 13. A typical multiple star.]
The development of the hypothetical primitive chaos has now been traced
through five generations of astronomical bodies,
_chaos—nebulae—stars—binary systems—sub-systems_,
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