Astronomy Flashcards

1
Q

What factor determines the type of lifecycle a star undergoes?

A

The size of the star

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2
Q

What two phases do all stars of the same or greater size than the sun undergo?

A

Protostar and main sequence phase

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3
Q

What do stars like the sun become at the end of their life-cycle?

A

A black dwarf

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4
Q

What two things can starts much bigger than the sun become at the end of their lifecycle?

A

Neutron star and black hole

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5
Q

What two phases do stars of similar size to the sun go through between being a main sequence star and a black dwarf?

A

Red giant and white dwarf

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6
Q

What two phases do stars of greater size to the sun go through between being a main sequence star and a neutron star/black hole?

A

Red supergiant and supernova

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7
Q

What is the transition of the star from the nebula stage to the main sequence?

A

The nebula increases in size until it’s pulled in due to its gravity, causing GPE to turn into KE, the collision between particles cause this KE to turn into thermal energy and eventually the nebula will become dense and hot enough to begin fusion

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8
Q

What occurs in the stage when a star is a main sequence star?

A

The fusion in the star release energy, this energy balance out with the gravitational potential energy leaving the star and the star is in equilibrium so will not collapse due to gravity or expand due to radioactive behaviour, it’s stable

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9
Q

What happens when a star transitions to the red giant stage?

A

Once all of the hydrogen fuel has been used up, the star begins to fuse helium and other larger nuclei and this cause the star to expand and become a red giant

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10
Q

When does a red giant become a white dwarf?

A

Once all reactions have taken place, the star’s gravity pulls in all of its mass, making a small dense white dwarf and this will cool down to form a black dwarf

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11
Q

Why are telescopes located outside the earths atmosphere?

A

The earths atmosphere absorbs many EM waves making it difficult to detect certain waves, light pollution can make some images less clear and telescope in scale can operate both night and day

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12
Q

What is the disadvantage of telescopes located outside the atmosphere?

A

They’re difficult to maintain as they have to be repaired in space

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13
Q

What are the disadvantages of optical telescopes?

A

They can only be used at night when the sky is clear and they can’t be used when the weather is cloudy

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14
Q

What is the use of radio telescopes?

A

They are not weather dependent and they are usually large and expensive

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15
Q

What is the steady state theory?

A

it says that the universe has always existed but is expanding and creating matter to counteract the loss in density

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16
Q

What is the Big Bang theory ?

A

It states that the universe expanded from a very small dense point about 14 billion years ago

17
Q

What is red-shift?

A

A perceived increase in the wavelength of light due to the source moving away from the observer

18
Q

What does red-shift provide evidence for?

A

The universe expanding and this supports the big bang theory

19
Q

What does the Big Bang theory suggest?

A

The entire universe started from a very small, hot and dense region in space

20
Q

Compare the observed red-shift of two galaxies, one further away than the other

A

The galaxy that is further away is travelling faster and the observed red-shift is greater the further away it is

21
Q

What did scientists observe to provide evidence that the universe is expanding at an ever faster rate?

A

They observed supernova which suggested that galaxies are moving away at an ever so fast rate

22
Q

Prior to observations of supernova, what was believed about the rate of expansion of the universe and why?

A

The rate expansion was expected to occur more slowly and it was thought that gravitational forces would cause this slowing down

23
Q

What does CMBR stand for?

A

Cosmic microwave background radiation

24
Q

What does CMBR provide further evidence for?

A

The big bang theory and it’s believed the CMBR originates from radiation produced in the Big Bang

25
Q

How does the existence of CMBR support the expansion of the universe?

A

It’s thought that gamma radiation was released in the Big Bang and the expansion of the universe has stretched this radiation, resulting in the microwave radiation present today

26
Q

Why does your weight vary across planets?

A

The gravitational field strength of a planet varies depending on the size of the planet and this means that your weight will also vary

27
Q

What is gravitational field strength on earth?

A

10N/kg

28
Q

What does our solar system consist of?

A

The sun (our star), mercury, Venus, earth, mars, Jupiter, Saturn, Uranus and Neptune, the planets natural satellites, dwarf planets and comets and asteroids

29
Q

What are the names of plants in order (starting with the closest to the sun)?

A

Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune

30
Q

What did Ptolemy suggest about the universe?

A

That the earth was at the centre

31
Q

What did Copernicus suggest about the universe?

A

That the sun is at the centre and the planets orbit it

32
Q

What did Galileo contribute to theories about the universe?

A

He used telescopes to support Copernicus’ suggestion about the sun, and suggested that moons orbit planets

33
Q

What are the orbits of moons, planets comets and artificial satellites?

A

They orbit in an elliptical shape

34
Q

Why for a stable orbit, the radius of orbit must change if the speed changes?

A

At higher speeds, the object requires a greater centripetal force, for a greater centripetal force, the gravitational force must increase and this is achieved by the radius of the orbit being reduced

35
Q

How does the force of gravity acting on a satellite affects its speed and velocity?

A

The force can alter its velocity since the direction is continually changing and it can’t cause a change of speed since there is no force component in the direction of motion