The Formation of the Universe and the Solar System Flashcards

Introduction L1

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1
Q

Most widely accepted theory on how the Universe came to existence

A

Big Bang Theory

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2
Q

Who first suggested the Big Bang Theory?

A

Georges Lemaitre

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3
Q

What year did Georges Lemaitre suggest his theory?

A

1927

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4
Q

Who said, “The universe is a singularity that explodes which creates matter, space, and time, as it cools off”

A

Georges Lemaitre

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5
Q

The Universe is believed to be around ___ years

A

13.8 billion

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6
Q

The ___ is described as an extremely hot and dense point that is smaller than a single atom.

A

singularity

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7
Q

Which two other discoveries support the Big Bang Theory?

A

Celestial bodies are moving away from each other at a proportional distance (Edwin Hubble, 1924) & Cosmic Microwave Background (n.a., 1960s)

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8
Q

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

A

Cosmological Redshift

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9
Q

Planck Era

A

10^-43 seconds

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10
Q

Timeline of the Univserse (Complete, 10)

A

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

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11
Q

Grand Unification Era

A

10^-35 seconds

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12
Q

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.

A

Planck Era / 10^-43 seconds

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13
Q

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.

A

Grand Unification Era / 10^-35 seconds

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14
Q

“___ ___” 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.

A

inflationary energy

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15
Q

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

A

10^-32 seconds

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16
Q

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.

A

10^-11 seconds / Electroweak Era

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17
Q

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 ____

A

quarks

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18
Q

At a temperature of ___ celsius, protons and neutrons start to combine together to form nuclei, the charged cores of atoms. (200 seconds)

A

one billion degrees celsius

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19
Q

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.

A

200 seconds

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20
Q

The universe has cooled to about 1,000C - cool enough for electrons to pair up with nuclei to form the first atoms.

A

300,000 years / Recombination Era

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21
Q

the universe consists of about 75% hydrogen and 25% helium. With the electrons now bound to atoms, the universe finally becomes transparent to light - making this the earliest epoch observable today.

A

300,000 years / Recombination Era

22
Q

proton + neutron = nuclei

collab w very first stars (light)

A

200m years

23
Q

The force of gravity starts to pull together huge regions of relatively dense cosmic gas, forming the vast, swirling collections of stars we call galaxies. These in turn start to form clusters, of which one - the so-called Local Group - contains our own Milky Way galaxy

A

0.5bn - 1bn years

24
Q

The force of gravity trying to slow the cosmic expansion begins to lose out to the anti-gravitational effect of “dark energy”, a mysterious force which has been accelerating the cosmic expansion ever since.

A

9bn years

25
Q

A region of gas and dust from exploding stars in the Milky Way galaxy starts to collapse under its own gravity, forming a small star surrounded by a disk of rocky material and gas. Swarms of giant chunks of debris form within the disc, collide and merge - forming the Earth, moon and other planets.

A

9.1bn years (4.6 bn years ago)

26
Q

Local Group

A

Galaxies (with Milky Way)

27
Q

A model describing the formation, evolution of Solar System.

A

The Nebular Hypothesis

28
Q

In Nebular Hypothesis, a group of protostars, one of which will become the Sun, form from a cloud of debris left by prior star explosions in the Milky Way.

A

4.6 b years ago

29
Q

In Nebular Hypothesis, the giant planets Jupiter, Saturn, Uranus, and Neptune form around the protosun. At least Uranus and Neptune form closer to the Sun than where they are today. One or more ice giants may have also formed that were later ejected from the solar system.

A

4.59 b years ago

30
Q

In Nebular Hypothesis, Let there be light: The Sun begins fusing hydrogen into helium

A

4.55 years ago

31
Q

In Nebular Hypothesis, the sun gravitationally separates from its protostar siblings

A

4.5 - 4.1 b years ago

32
Q

In Nebular Hypothesis, Life begins on Earth

A

3.8-3.5 b years ago

33
Q

In Nebular Hypothesis, Mars loses most of its atmosphere and water

A

3 b years

34
Q

In Nebular Hypothesis, volcanism on the moon stops

A

1 b years

35
Q

In Nebular Hypothesis, an impact on the moon forms tycho crater; saturn gets its rings.

A

100 m years

36
Q

In Nebular Hypothesis, a giant asteroid hits Earth, triggering global climate change. Three quarters of life, including dinosaurs, go extinct.

A

66 m years

37
Q

Space Expands, ___ Stretches

A

Light

38
Q

origin of fluctuations

A

Cosmic Inflation

39
Q

coupled to light and dark matter particles start building structures

A

ordinary matter particles

40
Q

ordinary matter particles decouple from light & the cosmic microwave background is released

A

recombination

41
Q

ordinary matter particles fall into the structures created by dark matter

A

dark ages

42
Q

clusters of galaxies & superclusters form

A

Galaxy evolution

43
Q

One unified force combined instead of multiple forces in the universe

A

superforce

44
Q

who proposed the Nebular Hypothesis? (2)

A

Immanuel Kant, Pierre Laplace

45
Q

Why is an electron negatively charged but does not come together with a proton?

A

It is because electrons has so much KE that it wanders rather than staying

46
Q

When electrons are excited, they go ____ the nucleus

A

away from

47
Q

When the KE of the e- is low, they ___ to the nucleus

A

go back

48
Q

kaya pa ba

A

k lang

49
Q

e- energy is low = it will ___ itself to the proton

A

not attach

50
Q

you will never know the exact position of an e- due to erratic movements

A

Heisenberd Uncertainty Principle