The Formation of the Universe and the Solar System Flashcards
Introduction L1
Most widely accepted theory on how the Universe came to existence
Big Bang Theory
Who first suggested the Big Bang Theory?
Georges Lemaitre
What year did Georges Lemaitre suggest his theory?
1927
Who said, “The universe is a singularity that explodes which creates matter, space, and time, as it cools off”
Georges Lemaitre
The Universe is believed to be around ___ years
13.8 billion
The ___ is described as an extremely hot and dense point that is smaller than a single atom.
singularity
Which two other discoveries support the Big Bang Theory?
Celestial bodies are moving away from each other at a proportional distance (Edwin Hubble, 1924) & Cosmic Microwave Background (n.a., 1960s)
Edwin Hubble used the ___ ___ to calculate the speed at which celestial bodies are moving away from each other, subsequently the speed at which Universe expands
Cosmological Redshift
Planck Era
10^-43 seconds
Timeline of the Univserse (Complete, 10)
Big Bang -> Cosmic Inflation -> Particles Form -> Recombination -> Dark Ages -> First Stars & Galaxies -> Galaxy Evolution -> Clusters of Galaxies -> Galaxy -> Solar System
BB>CI>PF>R>DA>FSG>GE>COG>G>SS
Grand Unification Era
10^-35 seconds
Closest era that current physics can get to the absolute beginning of time. Universe is incredibly hot, dense, turbulent, with very fabric of space and time.
Planck Era / 10^-43 seconds
Superforce begins to break apart into the constituent forces we see. Around this time so-called inflationary energy triggers a dramatic burst of expansion, expanding the universe from far smaller than a subatomic particle to far larger than the cosmic volume we can see today.
Grand Unification Era / 10^-35 seconds
“___ ___” triggers a dynamic burst of expansion, expanding the universe from far smaller than a subatomic particle to a far larger than the cosmic volume we can see today.
inflationary energy
Energy dumped into the universe by the end of inflation leads to the appearance of particples of matter via Einstein’s celebrated equation, E=mc^2
10^-32 seconds
Last two fundamental forces still unified with one another, electromagnetism and the weak nuclear force, finally split, leaving the universe with the four separate forces we observe today.
10^-11 seconds / Electroweak Era
In 10^-6 seconds, as the universe continues to expand, it becomes cool enough to allow the familiar particples of today’s matter, protons and neutrons, to form from their constituents, known as ____
quarks
At a temperature of ___ celsius, protons and neutrons start to combine together to form nuclei, the charged cores of atoms. (200 seconds)
one billion degrees celsius
Within 20 minutes, the temperature of the universe has become too cold to drive the process, which ceases with the formation of the nuclei of hydrogen and helium, the simplest and most common chemical elements in the universe. The formation of all the other elements - including the carbon, oxygen and nitrogen needed for life - will emerge with the first massive stars millions of years later.
200 seconds
The universe has cooled to about 1,000C - cool enough for electrons to pair up with nuclei to form the first atoms.
300,000 years / Recombination Era