The Big Bang theory (spec 8.13P)
Hot dense start; expansion ever since.
The Big Bang theory is the currently accepted scientific model of the universe's evolution. Its main statements:
- The universe began in an extremely HOT, DENSE state about 13.8 billion years ago.
- Space, time, energy and matter all began at this point — there is no meaningful 'before'.
- Since then, the universe has been EXPANDING and COOLING.
- As it cooled, the fundamental particles formed, then atoms (hydrogen and helium), then stars and galaxies under gravity.
Main arguments in favour (spec 8.13P).
-
Red-shift of distant galaxies (spec 8.17P, 8.18P) — almost every distant galaxy is moving away, with the speed increasing with distance. This is exactly what an expanding universe should look like.
-
Cosmic microwave background (spec 8.14P) — a uniform 2.7 K microwave radiation from all directions, exactly matching the predicted relic of the hot early universe.
-
Element abundances (not on the spec but useful context) — the observed proportions of hydrogen (~75%) and helium (~25%) in the universe match the predictions of Big Bang nucleosynthesis.
-
Galaxy evolution — looking at very distant (and therefore older) galaxies shows them in earlier stages of development than nearby ones.
The Big Bang is not a 'theory' in the casual sense of 'guess' — it is a fully developed scientific model with multiple independent lines of evidence.
- Universe started hot + dense ~13.8 Gyr ago.
- Has been expanding and cooling ever since.
- Evidence: red-shift, CMB, element abundances, galaxy evolution.