Topic 7 - Astronomy Flashcards

1
Q

Weight of any object depends on

A

Gravitational field strength(g)

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2
Q

Gravitational field strength depends on

A

The mass of the body creating the field
The distance from the body

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3
Q

The stronger the gravitational field strength

A

the larger the velocity needed to balance it and stay in orbit

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4
Q

Our solar system consists of

A

The sun
8 planets and their satellites
Dwarf planets
Asteroids and comets

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5
Q

The names of the 8 planets in order from least distance to the sun

A

Mercury, venus, earth, mars, jupiter, saturn, uranus, neptune

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6
Q

The geocentric model stated

A

The earth was the centre of the solar system. The sun, moon and planets orbited earth in perfect circles.

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7
Q

The heliocentric model

A

The sun is the centre. The planets orbited the sun in perfect circles. Moons orbited planets.

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8
Q

The current soalr system model

A

The sun is the centre. Planets orbit in elliptical orbits ratehr than circles.

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9
Q

Moon orbits

A

Almost circular orbits

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10
Q

Planet orbits

A

Orbit a star in an elliptical shape

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11
Q

Comet orbits

A

Highly elliptical orbits

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12
Q

Artificial satellites are

A

Human built objects that orbit the earth

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13
Q

Artificial satellite orbits

A

Fairly circular orbits

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14
Q

For planet and moon orbits, they move at

A

A constant speed but a changing velocity, so they are constantly accelerating

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15
Q

The force that makes the planet or moon change direction is called

A

The centripetal force

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16
Q

How does centripetal force work

A

The planet is constantly trying to move straight rather than in an orbit. The centripetal force is always towards the centre of the orbit, so it causes the planet to keep moving but change direction.

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17
Q

If orbital speed changes then

A

The radius of the orbit must also change

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18
Q

orbital speed increases or decreases effect

A

Increases - Orbital radius decreases
Decreases - Orbital radius increases

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19
Q

The two theories for the creation of the universe

A

The steady state theory
The big bang

20
Q

Steady stae theory states that

A

The universe has always been how it is now, and always will.
As the universe expands, new matter is constantly created
The density of the universe stays the same
No beginning or end to the unvierse

21
Q

The big bang theory

A

All the matter in the universe was in a very small space
Ver ydense and very hot
It exploded, and the expansion started
A finite age for the universe(13.8bn yrs)

22
Q

Evidence of the big bang theory

A

Red-shift
Cosmic microwave background radiation

23
Q

Why is the big bang the accepted theory

A

It has more evidence than the steady state theory

24
Q

Red shift full process

A

Different elements absorb different frequencies and wavelengths of light
When we look at light from distant galaxies compared to erath, it is lower frequency
Theis means it is shifted to the red side of the spectrum

25
Q

Red shift proves

A

That all distant galaxies are moving away from us fast
More distant galaxies have greater red-shifts, so the further away, the faster ther moving

26
Q

CMB radiation is

A

Cosmic microwave background radiation. Low frequency EM raqdiation(moslty microwaves) detected form all parts of the Universe.

27
Q

CMB proves big bang because

A

There has to have been an original source of the radiation, which is the explosion

28
Q

Red shift can prove both

A

Big bang and steady state because they both state the universe is expanding

29
Q

The stages of a star life-cycle

A

Nebula
Protostar
main sequence star
Red giant/supergiant
Supernova/white dwarf
Neutron star/black hole

30
Q

Nebula is

A

A cloud of dust and gas

31
Q

Protostar process

A

The force of gravity pulls nebula together. The temperature rises with density. Nuclear fusion starts to occur, which makes the core hot

32
Q

Main sequence star process

A

A long stable period
The gravity and nuclear fusion trying to expand the star balance out
The heavier the shorter it spends as this

33
Q

Red supergiant process

A

Stars much bigger than the sun become this.
Hydrogen in core runs out, so the nuclear fusion stops and it gets compressed by gravity
The hydrogen and helium outside go through nuclear fusion, so it get even bigger
It turns red because the surface cools

34
Q

Red giant process

A

Stars the size of the sun
Hydrogen in core runs out, so the nuclear fusion stops and it gets compressed by gravity
The hydrogen and helium outside go through nuclear fusion, so it get even bigger
It turns red because the surface cools

35
Q

White dwarf process

A

A red giant becomes unstable and ejects its outer layers. Only a hot, dense solid core is left

36
Q

Supernova process

A

Red supergiants undergo mroe fusion and get brighter again
Heavier elements are made
The balance constantly shifts betwenn graivty and thermal expansion
Eventually it explodes into a supernova

37
Q

Neutron star/balck hole process

A

Supernova throws outer layers of dust and gas into space
Leaves a very dense core called a neutron star.
If the star is massive enough, it will collapse and become a black hole
Balck holes are very dense points in space that absorbs everything around it, including light

38
Q

Telescopes are used to

A

Observe the universe

39
Q

Telescopes use

A

Refraction and reflection to see distant objects

40
Q

Optical telescopes

A

Detect visible light

41
Q

Ways to increase resolution of optical telescopes

A

Increase aperture of the objective lens
Higher quality objective lens

42
Q

Aperture is

A

The diameter of the objective lens(big lens at end of telescope)

43
Q

Space telescopes

A

Telescopes located outside the atmosphere

44
Q

Space telescopes are in space to

A

Capture light absorbed by the atmosphere
Avoid light pollution and air pollution

45
Q

Different telescoeps can see

A

Different types of EM radiation

46
Q

Different types of telescopes eg

A

X-ray telescopes
Radio telescopes