The Universe - Unit 2 Flashcards

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1
Q

Major features in the universe

A

Galaxies, stars, solar systems, nebulae

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2
Q

outline what a nebula is

A

a large cloud made of interstellar gas and dust that mark the beginning of a new star or are the remnants of supernovas.

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2
Q

outline what a star is

A

stars are giant balls of hot gas and plasma held together by gravity. stars are composed primarily of hydrogen, helium and small amounts of other elements.

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2
Q

ouline what a galaxy is

A

giant collections of stars, gas and dust, held together by the attractive force of gravity. The majority of galaxies feature a central bulge and a flattened disc. The different types of galaxy include ellipitical, spiral and irregular.

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3
Q

outline what a solar system is

A

a solar system consists of a star and one or more planets which orbit the star

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4
Q

1 AU

A

150 million km

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5
Q

proportions

A

-> galaxies are typically 100,000 light years in diameter
-> 100 billion stars in each galaxy
-> stars are generally a million kilometers in diameter or so
-> distance between earth and sun is around 150 million km

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5
Q

light year

A

the distance that light travels (going at 300,000km/s) in a year

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6
Q

star birth

A

Stars form from vast clouds of gas and dust called nebulae. A small disturbance can cause the cloud to collapse, until the star becomes hot enough for nuclear fusion to begin. The newborn star is called a protostar

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7
Q

small star life

A

nebula -> main sequence star -> red giant -> planetary nebula -> white dwarf -> white dwarf cooling -> black dwarf

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8
Q

large star life

A

nebula -> main sequence star -> supergiant -> supernova -> neutron star or black hole

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9
Q

telescopes

A

Instruments that collect and focus light and other forms of electromagnetic radiation using lenses, mirrors and reflecting dishes.

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10
Q

Optical telescopes

A

Can only see the very narrow band of visible light
Two types: Reflectors + refractors
Reflectors use a series of curved and angled mirrors to focus light whereas refractors use a series of lenses to magnify the images.
Advantage - Available to general public
Disadvantage - Chromatic abberation, lens distortion

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10
Q

Radio telescopes

A

Gather radiation and focus it to a point where it can be observed
Advantage - Unaffected by clouds, can be used in day and night
Disadvantage - More complicated to obtain good quality images that show all the details of celestial objects

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10
Q

Different types of telescopes

A

Optical
radio
Infrared and x-ray telescopes
Space telescopes

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11
Q

Infrared and x-ray telescopes

A

Tend to be space-based
Infrared light emitted from very hot space objects can be seen using infrared and x-ray telescopes
Advantage - Able to see objects within dusty clouds
Disadvantage - Ground based infrared telescopes need to be kept at very high altitudes which is a cumbersome process

12
Q

Space telescopes

A

Get around the Earth’s atmosphere so that we can get a clearer view of planets stars and galaxies.
Advantage - Are not obstructed by the Earth’s atmosphere
Disadvantage - Very expensive to build and to maintain

13
Q

Discoveries made with telescopes

A

Galileo used his optical telescope to discover that Venus had phases, proving that it orbits around the Sun and not the Earth.
Radio telescopes have discovered several powerful radio galaxies and qasars.
Space telescopes such as the NEOWISE probe have been used to detect comets, asteroids and other space objects.
Radio telescopes found CMB radiation
Hubble used his telescope to find that galaxies were moving away from us (red shift)

13
Q

Describe the Big Bang Theory

A

The Big Bang theory states that the universe expanded from a very small dense point about 14 billion years ago and has been continuing to do so.

14
Q

Different models of describing the origin of the universe

A

-> Earth-centred universe
-> Sun-centred universe
-> Steady state theory
-> Big bang theory

14
Q

Identify and outline the evidence for the expanding universe (big bang) theory

A

Red shift - wavelengths emitted from objects had shifted towards the red end of the electromagnetic spectum, proving that they were moving away from earth
Cosmic Microwave Background Radiation - The CMB is incredibly uniform in all directions, with only tiny fluctuations in temperature suggesting that the universe was once in a very hot, dense, and uniform state, as expected from the Big Bang. The fact that we see the same temperature everywhere, even in the farthest reaches of the universe, indicates that the early universe was once in a nearly uniform, thermal equilibrium state before it began expanding and cooling.
Abundance of elements - The relative amounts of hydrogen and helium are consistent with the amounts that are predicted to have been producing after the big bang.

15
Q

Errors in theories

A

Geocentric universe -> The planets orbit the Sun and the Earth is not at the centre of the universe
Heliocentric universe -> The universe has more in it than just stars and a few planets, the sun is not at the centre of our universe. Copernicus assumed there were circular orbits, but this lead to many inaccurate calculations.
Steady state theory -> Observations of distant galaxies show that they are very different from nearby galaxies — more irregular, with less structure and more star formation. This suggests that the universe has evolved over time. The Steady State theory couldn’t explain this evolving nature of galaxies because it assumed that the universe was in a steady, unchanging state.

16
Q

Reliability, accuracy, validity

A

How consistent the results are, how close the results are to other findings and known information, whether the controlled variables were kept the same and the experiment was fair

17
Q

dependent variable and independent variable

A

y axis, x axis : right column, left colum