The Universe -- Year 10 Flashcards

1
Q

1 pc = ___ ly = ___ km
___ ly = ___ km

A

1 pc = 3.26 ly
3.26 ly = 9.461 km

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2
Q

A singularity is…

A

an infinitely dense point of matter that existed before the Big Bang.

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3
Q

Define anti-matter.

A

Particles that have properties opposite to that of normal matter.

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4
Q

How much time after the Big Bang did the particles of matter and anti-matter annihilate each other?

A

0.001 second.

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5
Q

What does the “Big Bang” refer to?

A

The rapid expansion of the initial singularity.

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6
Q

Define antimatter.

A

Particles that have properties opposite to that of normal matter.

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7
Q

What happened 3 minutes after the Big Bang?

A

Protons and neutrons combined to form atomic nuclei, about 75% hydrogen, 25% helium and a small fraction of lithium.

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8
Q

When was all the matter and energy to ever exist formed?

A

3 minutes after the Big Bang.

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9
Q

What happened 5,000 years after the Big Bang?

A

Atoms formed!

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10
Q

3 minutes - 5,000 years after the Big Bang, the universe was…

A

A plasma of hydrogen, helium, and lithium nuclei and free electrons.

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11
Q

The universe formed ___ years after the Big Bang.

A

1 billion (1,000,000,000)

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12
Q

What is redshift?

A

A change in light’s wavelength towards the red end of the visible spectrum.

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13
Q

Explain the cosmological red shift of stars.

A

Cosmological red shift, or red shift, is the shift of light coming from stars towards the red end of the spectrum. It is similar to the doppler effect, which describes the lengthening of shortening of waves emanating from a moving object. For example, an ambulance moving towards a person will have a higher pitch than an ambulance moving away from a person, because the sound waves are being shortened by the ambulances forward motion. The doppler effect can’t be applied to cosmological red shift because light does not travel through a medium like sound does. However the principle of the doppler effect can explain red-shift. When the fabric of space between stars expands, the stars begin to move away from each other. Hence, the light observed from one star coming from the other will be red-shifted, because the wavelengths are lengthening– similar to how the sound waves were longer when the ambulance was moving away from the person in the given example. Cosmological red-shift can be used as evidence for the Big Bang theory, as it suggests that the universe is expanding (stars are moving away from each other due to the expansion of space between them).

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14
Q

What is the CMBR?

A

The left-over heat radiation from the Big Bang, which has redshifted due to the expansion of the universe. Was originally released 100,000 years after the Big Bang as UV and visible light when the universe cooled enough to allow radiation to pass through it.

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15
Q

Why do images of the CMBR show clumps of matter?

A

Because the universe was not of uniform density when the CMBR was released.

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16
Q

Which element are stars mostly made up of?

A

Hydrogen.

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17
Q

In the centre of stars, ____ atoms fuse together to form ___ atoms. This reaction releases a lot of energy, including ____.

A

In the centre of stars, hydrogen atoms fuse together to form helium atoms. This reaction releases a lot of energy, including visible light.

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18
Q

The release of energy pushing outwards from the core of stars is caused by ____.

A

Nuclear fusion (i.e. hydrogen to helium).

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19
Q

What forces balance each other out when a star is fusing hydrogen in its core?

A

The inward force of gravity and outward force of nuclear fusion.

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20
Q

Stars are essentially hot balls of gas consisting of different elements. Depending on their initial mass, they evolve in different ways. However, they all start off as (1)____ originating from (2)_____.

A

(1) Protostars
(2) Nebulae

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21
Q

Explain why the size of a star impacts its life-cycle.

A

A large star fuses hydrogen more quickly and has more gravity. This means it has a shorter life-span and more intense events, like a super-nova rather than a planetary nebula, or the formation of a black hole, occur.

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22
Q

What main factor determines the stages a star goes through?

A

Its mass.

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23
Q

Compare and contrast the size of a sun-like star and a massive star.

A

A Sun-like star, or a small star, and a massive star both originate from nebulae, which are interstellar regions of gas and dust. The force of gravity causes the nebula to contract into a protostar. A Sun-like star will form into an average-sized star. The Sun is only 1 solar mass, whereas stars bigger than 7 solar masses are considered large. The Sun will turn into a red giant, whereas a large star will turn into a red supergiant. This transformation, in both cases, is caused by the force of nuclear fusion releasing energy that causes the star to expand outwards (as it is greater than the force of gravity). However, as the rate of nuclear fusion slows, the stars transform again. This process happens more quickly and intensely in large stars, because gravity acts more strongly on them, and also because hydrogen fuses more quickly in their cores. In large stars, therefore, when the forces of energy become imbalanced, gravity causes the star to rapidly contract and then explode, resulting in a supernova. This is known as a supernova, and leaves the core of the star as an extremely dense neutron star. In supermassive stars, a black hole is formed due to the total collapse of the core. On the other hand, in small stars, the energy released by nuclear fusion exceeds the inward force of gravity, and one last burst of energy is released. This forms a planetary nebula as the outer layers puff outwards. When these are lost into space, the core remains as an extremely hot, dense and small white dwarf.

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24
Q

As gravity pulls matter towards other matter, a sphere forms. Why?

A

Only a sphere allows every point on its surface to have the same distance from the centre, so that no part of the object can further ‘fall’ toward its centre. Gravity just keeps on pulling.

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25
Q

What’s a nebula?

A

An interstellar region of gas and dust.

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26
Q

What’s a neutron star?

A

An extremely dense star left over after a supernova.

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27
Q

What’s a red giant?

A

A star that has stopped fusing hydrogen in its core.

28
Q

What’s a supernova?

A

An explosion of a massive star at the end of its life.

29
Q

What’s a white dwarf?

A

A small, very dense and hot star formed at the end of a small star’s lifetime.

30
Q

The luminosity of stars is a measure of…

A

The intrinsic brightness of a celestial object.

31
Q

A red giant is?

A

A star that has stopped fusing hydrogen in its core.

32
Q

The formula for conversion of kelvins to degrees celsius is…

A

amount of kelvins - 273.15 = degrees celsius.

33
Q

Formula for conversion of degrees celsius into kelvins is…

A

amount of degrees celsius + 273.15 = kelvins

34
Q

List the stages of a small star’s life-cycle.

A

Protostar (from nebula), main-sequence star, red giant, planetary nebula, white dwarf.

35
Q

List the stages of a large star’s life-cycle.

A

Protostar (from nebula), main-sequence star, red supergiant, supernova, neutron star (or if it’s supermassive, black hole).

36
Q

Galaxies can be classified into three main groups. They are:

A

Spiral, elliptical and irregular.

37
Q

How do we know what kind of galaxy the Milky Way is?

A

Because we can observe images of out night sky and compare it with pics of other galaxies.

38
Q

The Local Group includes:

A

The Andromeda and Triangulum galaxies, the Milky Way, and the Small and Large Magellanic Clouds.

39
Q

One popular theory on how galaxies form is that:

A

Irregular and elliptical galaxies form when galaxies collide with each other and spiral galaxies form on their own, with their spiral shape resulting from the spinning motion of the galaxy.

40
Q

Supermassive black holes are the centres of most galaxies. Okay?

A

Okay!

41
Q

An astronomical unit is…

A

The average distance between Earth and the Sun. This is about 150 million km.

42
Q

Galaxies further away appear different from closer galaxies because

A

we are observing them at a much younger stage in their lives.

43
Q

The nebula from which our solar system formed was made up of mostly ____ elements.

A

Lighter.

44
Q

Why are inner, rocky planets like Venus and Earth small?

A

Because they are made of heavy elements which were rarer in the nebula from which our solar system formed than light elements.

45
Q

Why do the rocky planets exist in the inner solar system? (and not the outer solar system, for example).

A

Because the inner solar system was too warm for light elements to exist as liquids (they melted into gases) so only compounds with high melting points (meaning they did not melt easily) were able to form.

46
Q

Do short period comets orbit the sun frequently or occasionally?

A

Frequently.

47
Q

Short period comets originate in the…

A

Kuiper Belt.

48
Q

The Kuiper belt is part of the outer solar system and extends from the orbit of (1) ____ to around (2) ___ AU from the Sun.

A

(1) Neptune
(2) 55

49
Q

The Kuiper Belt is a region of icy bodies left over from….

A

The formation of our solar system.

50
Q

The Oort Cloud lies in the ____ parts of the solar system.

A

Outermost.

51
Q

The Oort Cloud is around 5000- (1) _____ AU from the (2) _____.

A

(1) 100,000
(2) Sun

52
Q

Exoplanets are…

A

Planets that orbit stars other than the Sun.

53
Q

What is the boundary just inside Jupiter’s orbit called?

A

The frostline.

54
Q

What is accretion?

A

The process of matter collecting together into a bigger mass.

55
Q

The gas giants are mostly made of…

A

Hydrogen and helium.

56
Q

Gas giants have cores made up of…

A

Rock and ice.

57
Q

Why are gas giants like Jupiter and Saturn made of so much hydrogen and helium?

A

Because their large cores allowed them to attract lots of hydrogen and helium before the solar wind cleared the solar system.

58
Q

Why is the frost line significant?

A

Outside the frost line boundary, temperatures are so low that hydrogen, helium and other compounds that are gases on Earth are able to condense and exist as liquids.

59
Q

Optical telescopes collect and amplify light. What do we use to make them?

A

The first optical telescope made my Galileo used lenses to collect light and magnify the image. Today, we use mirrors, because large mirrors are easier to make than large lenses. It needs to be large, because the larger the mirror or lens is, the more fine detail can be observed, and the higher the resolution.

60
Q

When hydrogen elements are excited by energy, they emit radio waves– like they are squealing in excitement. Why is this significant to radio telescopes?

A

Radio telescopes detect these radio waves from space.

61
Q

Radio waves can travel through dust clouds. Why is this significant to radio telescopes? Does this make them better than other telescopes?

A

Since radio waves can travel through dust clouds, astronomers can discover and map out objects that cannot be seen with an optical telescope using a radio telescope. This makes them better for some activities than other telescopes, like optical telescopes, which do not have this property.

62
Q

How have radio telescopes advanced scientific understanding of the universe?

A

They have enabled the discovery of pulsars (rapidly spinning neutron stars), quasars (primordial galaxies with supermassive black holes), supernova remnants and black holes.

63
Q

List two limitations of radio telescopes.

A

1) they must be situated away from large populations where there are few radio signals (such as from radios, TVs and mobile phones).
2) The resolution of radio telescopes is extremely poor.

64
Q

List two limitations of optical telescopes.

A

1) They must be located away from populated areas that cause light pollution. Otherwise, the image will be unclear, making it difficult to see faint celestial objects, due to the interference.
2) They must be located at high altitudes. This is to minimize the impact of atmospheric turbulence, which distorts the quality of observations. This turbulence, caused by variations in Earth’s atmosphere, results in blurry images.

65
Q

Do space telescopes allow astronomers to gather clearer images than they would using optical telescopes? Why?

A

Yes, because space telescopes don’t experience interference by the atmosphere or light pollution.

For example, the Hubble Telescope was able to produce images 50% sharper than an optical telescope on Earth.

66
Q

What are some discoveries made with space telescopes?

A

Hubble telescope: astronomers have traced the evolution and formation of galaxies,
discovered that most galaxies contain supermassive black holes, and
mapped the presence of the mysterious dark matter that makes up most of the universe’s mass and structure.

67
Q

List the steps in the formation of a solar system.

A

1) Cloud of gas and dust clumps together due to the force of gravity… accretion of matter occurs due to the force of gravity.
2) The cloud of gas and dust begins to rotate and becomes a disk. This pulls nearby material and creates the core of a protostar.
3) The core gains in heat and energy, until it becomes hot enough to facilitate the temperature of nuclear fusion.