[net.astro] StarDate: November 9 Rotation

dipper@utastro.UUCP (Debbie Byrd) (11/09/84)

In our universe, everything is always moving.  We talk about the
movement of rotation -- right after this.

November 9  Rotation

In our universe, everything moves -- or rotates -- spins on its axis
usually slowly and ponderously -- but sometimes in a twinkling of an
eye.

A few tiny, ultra-compact stars whirl around once in only a matter of
seconds -- or less.  Other stars -- like our own sun -- take days,
weeks or months to rotate once.

And not just stars -- whole galaxies also rotate.  When you consider
the rotation of one of these vast systems of stars -- you can think of
each individual star as a molecule in a single body.  As the
body-galaxy rotates, each star is in motion around the galactic
center.  The whole gigantic assembly spins on a timescale of hundreds
of millions of years.

So things rotate -- but why?  To answer, think back to a time many
billions of years ago, when the universe was in its infancy.  All
matter was an expanded gas.  The galaxies coalesced from this gas --
and later also the stars.  In each case, separate clouds pulled apart
from the rest -- and the matter in these clouds was in motion.  As
gravity made the cloud collapse, each particle of matter moved faster
-- just as a spinning skater moves faster when she draws in her arms.

Eventually the clouds had collapsed to their current states.  Each
particle is still in motion -- only now much of that motion shows up as
the rotation of galaxies and stars.  If you could stand back from the
universe, you would see everything engaged in its own particular cosmic
dance.


Script by Deborah Byrd.



(c) Copyright 1983, 1984 McDonald Observatory, University of Texas at Austin