[net.space] The soap-bubble theory of galaxy formation

dipirro@amber.DEC (GENERIC PERSONAL_NAME STRING) (01/08/86)

>A recent 3-D map of the distribution of the galaxies in the universe
>has given evidence that the mass is distibuted roughly on the surface
>of large bubble shaped regions of space.  The interiors of these regions
>are largely devoid of galaxies.  The effect is a "Soapsuds" distribution
>of galaxies.  This all seems to indicate that some very explosive events
>and the resultant shock waves very early in the history of the universe
>had a profound effect on the evolution of the galaxies.

I also read this study. The 3D map is currently of one quarter of the
northern hemisphere of the universe (a 3D map of the universe would be
quite an accomplishment, but which way is north in the universe?). They expect
to find the same "bubble" effect in the other parts of the universe. Does this
mean we should stop talking about the big bang and start talking about the
big bangs? This seems to imply that *all* galaxies are not moving away from
each other but away from the center of their bubble. Are the bubbles themselves
moving or will some bubbles eventually collide (the bubbles do seem to be
expanding)? In the latter case, we should be able to discover some galaxies
actually moving towards the milky way. I just hope that some omnipotent being
doesn't accidently pop our bubble.

Steve DiPirro
Digital Equipment Corp.

ethan@utastro.UUCP (Ethan Vishniac) (01/09/86)

> Does this
> mean we should stop talking about the big bang and start talking about the
> big bangs? This seems to imply that *all* galaxies are not moving away from
> each other but away from the center of their bubble. Are the bubbles themselves
> moving or will some bubbles eventually collide (the bubbles do seem to be
> expanding)? In the latter case, we should be able to discover some galaxies
> actually moving towards the milky way
> 
> Steve DiPirro

The motion associated with each "bubble" is a small perturbation to the
general expansion of the universe.  If it weren't we would have noticed
this a long time ago.  This work in no way invalidates the theory of the
big bang.  It does give some clues as to the processes that made the
universe slightly inhomogeneous.  As to bubbles colliding, some may but
such collisions would not be exceptionally dramatic, a little like shooting
marbles at each other across the room.  A few spectacular collisions (which
in the case of galaxies means mergers and funny looking aggregates) and
a lot of misses.
-- 
"These are not the opinions    Ethan Vishniac
 of the administration of      {charm,ut-sally,ut-ngp,noao}!utastro!ethan
 the University of Texas,      ethan@astro.UTEXAS.EDU
 but they are the opinions     Department of Astronomy
 of your favorite deity, who   University of Texas
 is in daily communication 
 with me on this (and every 
 other) topic. 

wyatt@cfa.UUCP (Bill Wyatt) (01/10/86)

> >A recent 3-D map of the distribution of the galaxies in the universe
> >has given evidence that the mass is distibuted roughly on the surface
> >of large bubble shaped regions of space.
> > [...]
>
> I also read this study. The 3D map is currently of one quarter of the
> northern hemisphere of the universe [...]
>

Just a point of detail - the CFA Redshift survey is a magnitude-limited
sample (down to 14.5) of all galaxies in the Zwicky-Nilson catalog with
galactic latitude above +40 and declination above 0 degrees, or below
galactic latitude -30 degrees and above dec of -2.5 degrees. The funny
limits arise since the galactic plane is tilted relative to the solar
system and the earth. The original survey contains 2402 galaxies. I
suspect it is to this survey you refer as being 1/4 of the sky.

The "bubble map" is the result of an extension to fainter objects
(15.5). Since this would result in an increase by a factor of about 4 in
the number of objects (and easily a factor of 5-10 in exposure time per
object, assuming same telescopes, detectors, etc.), the map was
restricted to a swath of 120 by 6 degrees, chosen to intersect the Coma
Cluster of galaxies. The additional depth clearly shows the bubble
effect even in this much smaller pie-shaped slice of the universe.

--
Bill    UUCP:  {harvard,genrad,allegra,ihnp4}!wjh12!cfa!wyatt
Wyatt   ARPA:  wyatt%cfa.UUCP@harvard.ARPA