Worlds in the making: The evolution of the universeArrhenius, Svante
Science
Worlds in the making: The evolution of the universe
Arrhenius, Svante
Cosmogony
We have already mentioned (page 116) the peculiar clouds of light which
were observed around Nova Persei. Two annular clouds moved away from
this star with velocities of 1.4 and 2.8 seconds of arc per day between
March 29, 1901, and February, 1902. If we calculate backward from
these dates the time which must have elapsed since those gases left the
star, we arrive at the date of the week—February 8 to 16, 1901—in
satisfactory agreement with the period of greatest luminosity of the
star of February 23d. It would, therefore, appear that these emanations
came from the star and were ejected by the radiation pressure. Their
light did not mark any noticeable polarization, and could not be
reflected light for this reason. We may suppose that the dust particles
discharged their electric charges, and that the gases became thereby
luminous.
In this case we were evidently witnesses of the grand _finale_ of
the independent existence of a celestial body by collision with some
other body of equal kind. The two colliding bodies were both dark, or
they emitted so little light that their combined light intensities
did not equal that of a star of the twelfth magnitude. As, now, their
splendor after the collision was greater than that of a star of the
first magnitude, although their distance has been estimated to be at
least 120 light years,[14] their radiation intensity must have exceeded
that of the sun several thousand times. Under these circumstances the
mechanical radiation pressure must also have been many times more
powerful than on the surface of the sun, and the masses of dust which
were ejected by the new star must have possessed a velocity very much
greater than that of solar dust. Yet this velocity must have been
smaller than that of light, which, indeed, the effect of the radiation
pressure can never equal.
[Footnote 14: One light year corresponds to 9.5 billion
kilometres, and it is the distance which the light traverses in
the course of a year.]
[Illustration: Fig. 46.—Diagram indicating the consequences
of a collision between two extinct suns, A and B ‘moving’ in
the direction of the straight arrows. A rapid rotation in
the direction of the curved arrows results, and two powerful
streamers are ejected by A B, the explosive substances from the
deeper strata of A and B being brought up to the surface by the
collision]
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