Open main menu
Home
Random
Log in
Settings
About Nordan Symposia
Disclaimers
Search
Changes
← Older edit
Newer edit →
See Illustration 11
(view source)
Revision as of 01:52, 29 December 2007
323 bytes added
,
01:52, 29 December 2007
no edit summary
Line 3:
Line 3:
[[Image:Bang11.gif]]
[[Image:Bang11.gif]]
+
+
BIG BANG EXPANSION SCENARIOS
+
+
The Universe is (1) open, (2) closed, or (3), flat, depending on whether the ratio of its
+
actual density to the "critical density", called omega, is <1, >1, or precisely equal
+
to 1. The "critical density" of the Universe is the density above which the Universe
+
would go on expanding forever.
[[Category: Wisenbaker Images]]
[[Category: Wisenbaker Images]]
Rdavis
Bureaucrats
,
Administrators
103,025
edits