Gravity bends light. If gravity is too strong it bends light completely. Gravity bends (distorts) not only space, but space-time. This planetarium show is a friendly introduction to the General Theory of Relativity suitable for general audiences. You do not have to know what the local metricization of Riemanian manifolds are to appreciate the basis and the results of the General Theory of Relativity. Black Bubbles are the most extreme results of this theory; some people also call these black bubbles, black holes, but bubbles capture a better picture of the events horzion and what really goes on there. They are literally Gravity to the Max. By looking at something in its most extreme case facets that are not revealed in mundane application like normal falling motion on the earth are shown.
The infinite time dilation (time asymmetry) between an outside the
bubble
observer and an observer who decides to visit the bubble are explained.
Some
of the other weird properties of Black Bubbles including resent
observation
of the vicinity of a black bubble in the center of our galaxy will be
shared with the audience. Anyone
with an inquiring mind and imagination of a typical third grader can
enjoy
this planetarium show. Those few people who do not want to flex
(distort)
or exercise (move) their mind are advised to stay home and watch
mindless
television so called reality shows, that are doubtless on at the same
time
on
Saturday evening.
PowerPoint presentation
used on November 22, 2007.
Stars orbiting around the 2.6 million solar mass black hole in the
center of our galaxy movie.
Gravitational waves from two merging black holes movie
done at the GSFC
in 2006 by Joan Centrella, John Baker, and Dale Choi.
Hubble
Black Hole Astronomy Site shown on November 21, 2009.
Spining Black Bubbles
merging can cause the spins to flip.
Image from
http://www.spacetimetravel.org/expeditionsl/expeditionsl.html;
of
a simulated
view of a black bubble (hole) in front of the Milky Way Galaxy. The
black bubble is 10 solar masses so its Swartzshield radius, events
horizion radius, is 30 kilometers,
and is viewed from a distance of 600 kilometers which is 200
Swartzshield radi away and essentially Newtonian garvity at this far
distance of 600 kilometers from the Bubble.

Montgomery College's Planetarium home page
Web page by Dr. Harold Alden Williams.
Last changed 5:25P.M. November 22, 2009.