THE UNIVERSE AND THE SOLAR SYSTEM Flashcards

1
Q

What are the Non-scientific Thought

A
  1. Ancient Egyptians believed that the world arose from an infinite sea at the first rising of the sun
  2. God Mbombo felt an intense stomach pain and then vomited the star, sun and moon
  3. Sacrifice of Purusha and its body parts became the earth, sky, sun, moon
  4. Monotheistic Religions believed that a supreme being created the universe
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2
Q

they believed that the world arose from an infinite sea at the first rising of the sun

A

Ancient Egyptians

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3
Q

They felt an intense stomach pain and vomited the stars, sun, and moon

A

God Mbombo

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4
Q

He was sacrificed by the gods, the primal man whose head, feet, eyes, and mind became the sky, earth, sun, and koon

A

Purusha

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5
Q

They believed that a supreme being created the universe

A

Monotheistic religion

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6
Q

3 Monotheistic religions

A
  1. Judaism
  2. Christianity
  3. Islam
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7
Q

It maintains the new matter is created as the universe expands thereby maintaining its density

A

Steady State Model

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8
Q

They created the Steady State Model

A

Bondi and Gould and by Hoyle

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9
Q

When was the Steady State Model created

A

1948

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10
Q

postulates that 13.8 billion years ago, the universe expanded from a tiny, dense and hot mass to its present size and much cooler state

A

Big Bang Theory

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11
Q

2 Theories or Ideas in the Big Bang Theory:

A
  1. General Relativity
  2. Cosmological Principle
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12
Q

gravity is thought as a distortion of space-time and no longer described by a gravitational field

A

General Theory of Relativity

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13
Q

explains the peculiarities of the orbit of Mercury and the bending of light by the Sun and has passed rigorous tests

A

General Relativity

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14
Q

assumes that the universe is homogenous and isotropic when averaged over large scales

A

Cosmological Principle

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15
Q

The Big Bang Theory has withstood the tests for expansion:

A
  1. The redshift
  2. Abundance of hydrogen, helium and lithium
  3. The uniformly pervasive cosmic microwave background radiation the remnant heat from the bang
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16
Q

Evolution of the Universe according to the Big Bang Theory

A

• Time zero until 10^-43 second later, all matter and energy in the universe existed as a hot, dense, tiny state
• Underwent extremely rapid, exponential inflation until 10^-32 second until 10 seconds
• Nucleosynthesis took place and produced protons, neutrons, atomic nuclei, then hydrogen, helium, and lithium until 20 minutes after time zero when sufficient cooling didnt allow further nucleosynthesis
• Until 380,000 years, the cooling universe entered a matter-dominated period when photons decoupled from matter and light could travel freely as still observed today in the form of cosmic microwave
• As it cools down, stars rise after 380,000 years and galaxies would form after 100 million years from time zero
• 9.8 billion years until the present, the universe became dark-energy dominated and underwent accelerating expansion
• After 9.8 billion years after the big bang theory, the solar system was found

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17
Q

is located in the milky way galaxy

A

Solar System

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18
Q

a huge disc and spiral shaped aggregation of about at least 100 billion stars and other bodies

A

Milky Way Galaxy

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19
Q

1 light year =

A

9,.4607 x 10^12km

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20
Q

revolves around the galactic center once in about 240 million years

A

solar system

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21
Q

Milky Way is part of the

A

Local Group of galaxies

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22
Q

is part of the so called Local Group of galaxies

A

Milk Way

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23
Q

How old is the Earth and Solar system

A

4.6 billion years old

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24
Q

Large Scale Features of the Solar System:

A
  1. Much of the mass of the Solar System is concentrated at the center while angular momentum is held by outer planets
  2. Orbits of the planets elliptical and are on the same. All planets revolve around the sun
  3. Periods of revolution of the planets increase with increasing distance from the Sun, innermost planet moves fastest, outermost is slowest
  4. All planets are located at regular intervals from the Sun
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25
Q

Small scale feature of the Solar System:

A
  1. Most planets rotate prograde
  2. Inner terrestrial planets are made of high melting materials and they rotate slower. They also have thin/no atmosphere, higher densities, and lower volatiles
  3. Outer planets rotate faster, have thick atmosphere, lower densities, and fluid interiors
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26
Q

rotation of counterclockwise when viewed from above the Earth’s North Pole

A

Prograde

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27
Q

What are the four outer planets or gasgiants

A
  1. Jupiter
  2. Uranus
  3. Saturn
  4. Neptune
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28
Q

Are made of high melting materials and they rotate slower due. They also have thin/no atmosphere, higher densities, and lower volatiles

A

Inner terrestrial planets

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29
Q

Rotate faster, have thick atmosphere, lower densities, and fluid interiors

A

Outer planets

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30
Q

Elements Abundance on Earth, Meteorites and Universe

A

Si
Al
Fe
Mg
Ca
Na
K
Mn

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31
Q

Hypothesis about the Origin of the Solar system:

A
  1. Nebular Hypothesis
  2. Encounter Hypothesis
  3. Protoplanet Hypothesis
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32
Q

Who created the Nebular Hypothesis

A

Emanuel Swedenborg
Immanuel Kant
Pierre Simon Laplace

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33
Q

Rotating gaseous cloud that cools and contracts in the middle to form the sun and the rest into disc that become the planets

A

Nebular Hypothesis

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34
Q

sun-star encounter that would have drawn from the sun matter that would condense to planets

A

James Jeans (1917)

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35
Q

Sun comet encounter that sent natter to form planet

A

Buffon (1749)

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36
Q

Who created the planetissimal hypothesis

A

T.C. Chamberlain and F.R Moulton (1904)

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37
Q

involves. star much bigger than the Sun passing by the Sun and draws gaseous filaments from both out which planetissimals were formed

A

Planetissimal hypothesis

38
Q

Sun’s companion star colliding with another to form a protoplanet that breaks up to form Jupiter and Saturn

A

Ray Lyttleton (1940)

39
Q

proposed that sun passed through a dense interstellar cloud and emerged with a dusty, gaseous envelope that became the planets

A

Otto Schmidt’s accretion theory

40
Q

rogue star passes close to the sun then gas is tidally removed from both rogue star and sun. The rogue star material is less dense and becomes outer Solar system planets while the inner solar system material is more dense and becomes terrestrial planets

A

Encounter Hypothesis

41
Q

a variation of James Jean’s near collision hypothesis

A

M.M. Woolfson’s capture theory

42
Q

Noble prize winner that studies on meteorites in the 1950s that led to the conclusion that meteorite constituents have changed very little since the solar system’s early history and can give clues about their formation

A

Harold Urey’s

43
Q

Is the current hypothesis in the solar system

A

Protoplanet Hypothesis

44
Q

4.6 billion years ago, in the orion arm of the milky way galaxy, slow rotating gas and dust starts to contract due to gravity. Most of the mass move to the center and becomes a proton sun while the remaining form a disc that becomes planets. Due to collisions, the fragments began to stick to each other that formed larger bodies of planets. When the proton-sun is established as a star, its solar wind blasts from the inner planets to beyond mars to form gas giants leaving behind a system we know today

A

protoplanet hypothesis

45
Q

comprises all space and time and all matter and energy in it

46
Q

how many baryonic matter

A

4.6% baryonic matter

47
Q

matter consisting of protons, electrons, neutrons

A

baryonic matter

48
Q

how many cold dark matter

A

24% cold dark matter

49
Q

how many dark energy

A

71.4% dark energy

50
Q

The universe is made up of:

A

4.6% baryonic matter
24% cold dark matter
71.4% dark energy

51
Q

matter that has gravity but does not emit light

A

cold dark matter

52
Q

source of anti gravity

A

dark energy

53
Q

can explain what may be holding galaxies together for the reason that the low total mass is insufficient for gravity alone to so so while dark energy can explain the observed accelerating expansion of the universe

A

Dark matter

54
Q

3 most abundant elements

A

Hydrogen
Helium
Lithium

55
Q

building block of galaxies born out of clouds of gas and dust

56
Q

are like furnaces where elements are synthesized or combines/fused together

A

Stellar interiors

57
Q

most stars such as the sun belong to the so-called

A

main sequence stas

58
Q

burn up their hydrogen faster than smaller stars

A

Massive main sequence stars

59
Q

minimum temperature for H fusion

60
Q

cluster of billions of stars and clusters of galaxies

61
Q

He discovered the Redshift

A

Edwin Hubble

62
Q

when was the red shift discovered

63
Q

the universe expands because galaxies are moving away from each other

64
Q

he observed that spectral lines of starlight made to pass through prism are shifter toward the red part of the electromagnetic spectrum, toward the bad of lower frequency; thus, the inference that the star or galaxy must be moving away from us

A

Edwin Hubble

65
Q

are formed in clouds of gas and dust, known as nebulae

66
Q

a cloud of gas (hydrogen) and dust in space

67
Q

glows brightly because the gas in it is energized by the stars that have already formed within it

A

Emission Nebula

68
Q

starlight reflects on the grains of dust in a nebula

A

reflection nebula

69
Q

dense clouds of molecular hydrogen which partially or completely absorb the light from stars behind them

A

Dark Nebula

70
Q

are the outer layers of a star that are lost when the star changes from a red giant to a white dwarf

A

Planetary nebula

71
Q

luminous globe of gas producing its own heat and light by nuclear reactions

72
Q

born from nebulae and consist mostly of hydrogen and helium gas

73
Q

faintest stars

74
Q

example of an emission nebula

A

orion nebula

75
Q

smallest mass possible for a star

76
Q

also called as large planet

A

brown dwarfs

77
Q

objects with less than critical mass shine

A

brown dwarfs

78
Q

large bright star with a cool surface

79
Q

they are very bright because they are very large

80
Q

very large stars (red giants) are often called

A

super giants

81
Q

have diameters between 10 and 100 times that of the sun

82
Q

these stars gave diameters up to 1000 times that of the sun and have luminosities often 1M times greater than the sun

A

super giants

83
Q

very cool, faint and small stars approximately one tenth the mass and diameter of the sun

84
Q

examples of red dwarf

A

Proxima Centauri
Barnard’s Star

85
Q

very small, hot star, the last stage in the life cycle of a star like the sun

A

white dwarf

86
Q

explosive death of a star

87
Q

2 general types of supernova

A

type 1: occur in binary star systems in which gas from one star falls on to a white dwarf, causing it to explode

type 2: occur in stars ten times or more massive as the sun, which suffer runway internal nuclear reactions at the ends of their lives leaving a neutron star or black holes

88
Q

composed mainly of neutrons and are produced when a supernova exploded, forcing the protons and electrons to combine

A

neutron stars

89
Q

form from massive stars at the end of their lifetimes

90
Q

nothing can escape from it, even light, due to its gravitational pull

A

blackholes