The Universe: How the Solar System was Made
2011 · 45 MIN · IMDB 7.2 · 71 VOTES
Overview
At 4.6 billion years old, the Solar System is our solid, secure home in the Universe. But how did it come to be? In this episode we trace the system's birth from a thin cloud of dust and gas. Shocked by a nearby supernova, the pull of gravity and natural rotation spun it into a flat disc from which the Sun and planets coalesced. It all happened in the space of 700 million years, during which the planets jockeyed for position, dodging the brutal bombardment of deadly asteroids and setting into the neat, stable system that we now realize might be a rarity in the universe.
Dialogue Timeline — 667 lines
A SAMPLE ACROSS THE RUNTIME — EVERY LINE IS SEARCHABLE
00:00:00 In the beginning, there was darkness, and then-- Bang! Giving birth to
00:01:57 it can send a shockwave through this molecular cloud...
00:03:41 The collapsing cloud destined to become our
00:05:22 The most basic of these motions is circular, like
00:06:58 Mm-hmm.
00:08:14 nebula.
00:10:07 First we take the sugar crystals, and we pour that into
00:11:22 microscopic at this point, far smaller than the melting sugar
00:13:34 The thick rotating disc made mostly of hydrogen gas, is embedded with solids.
00:15:32 were able to attract ices of water, amonium, methane and carbon dioxide
00:17:57 We see this process happening in other solar systems being formed as well.
00:19:49 the rest of the universe.
00:21:42 In some systems, the cores of contracting clouds never glow
00:24:01 the planets in the inner part of the Solar System
00:25:21 hard, this stuff breaks really easy, and it crumbles.
00:27:02 isn't that the same process that actually forms a planet?
00:28:24 objects in them than they do today.
00:30:30 Solar System must have been a spectacular event.
00:32:23 Early on, the outer planets tended to move around quite a bit.
00:34:23 What if we were to add Jupiter to the system?
00:36:11 The resonance is a cataclysm whose effects sweep
00:38:30 Some have speculated that much of the water we have on Earth is
00:40:48 One of the exciting things about the Dawn Mission
00:42:35 Some systems have Jupiter-sized planets close to their suns
Cast & Characters
Erik Thompson
Narrator
Alex Filippenko
Self - Univ. of California, Berkeley
Michael Mischna
Self - NASA
Michael Mischna
JPL
Edward Young
Self - Univ. of California, Los Angeles
Clifford V. Johnson
Self - Univ. of Southern California
Laura Danly
Self - Griffith Observatory
Mike Brown
Self - Caltech
Charles Beichman
Self - NASA Exoplanet Science Institute
Ryan Johnson
Self - Special effects artist
Ryan C. Johnson
Special Effects artist
Dialogue Record
Lines indexed667
Dialogue density14.8 lines / min
First line00:00:00
Final line00:42:35
Production Record
LanguageEnglish
IMDb votes71