At first there was a rival interpretation. It was thought that the
lines were produced in a cloud attached to the star--forming a kind
of aureole round it. The two components travel in orbits round each
other, but their orbital motion need not disturb a diffuse medium
filling and surrounding the combined system. This was a very reasonable
suggestion, but it could be put to the test. The test was again
_velocity_. Although either component can move periodically to
and fro within the surrounding cloud of calcium and sodium, it is
clear that its average approach to us or recession from us taken over
a long time must agree with that of the calcium and sodium if the star
is not to leave its halo behind. Professor Plaskett with the 72-inch
reflector at the Dominion Observatory in British Columbia carried out
this test. He found that the secular or average rate of approach of
the star[20] was in general quite different from the rate shown by the
fixed calcium or sodium lines. Clearly the material responsible for
the fixed lines could not be an appendage of the star since it was not
keeping pace with it. Plaskett went farther and showed that whereas
the stars themselves had all sorts of individual velocities, the
material of the fixed lines had the same or nearly the same velocity
in all parts of the sky, as though it were one continuous medium
throughout interstellar space. I think there can be no doubt that this
research demonstrates the existence of a cosmic cloud pervading the
stellar system. The fullness of interstellar space becomes a fact of
observation and no longer a theoretical conjecture.
The system of the stars is floating in an ocean--not merely an ocean
of space, not merely an ocean of ether, but an ocean that is so far
material that one atom or thereabouts occurs in each cubic inch. It is
a placid ocean without much relative motion; currents probably exist,
but they are of a minor character and do not attain the high speeds
commonly possessed by the stars.
Public-domain text, read in full here on John Shaqi.
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