Topic 10 Flashcards

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1
Q

What is the Astronomical Unit

A

The astronomical unit is the mean distance between the Earth and the Sun.

1AU = 1.5 x 10^11 m

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2
Q

What is the unit of a light year a measure of

A

Distance

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3
Q

What is a light year

A

The distance through space that a light photon travels in the space of a year

1ly = 9,46 x 10^15 m

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4
Q

What can parallax be used for

A

Parallax can be used to calculate distances in space, using observations and trigonometry

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5
Q

What is a parsec

A

A parsec is an astronomical unit of distance. A star is one parsec (pc) away from the Earth if the parallax angle is 1 arcsecond

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6
Q

What is a Hertzsprung-Russell diagram

A

A Hertzsprung-Russel diagram is a plot of a star’s stellar luminosity against its surface temperature

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7
Q

What category of star is represented by the main diagonal on a HR diagram

A

The main sequence stars

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8
Q

What category of stars lie below the main sequence diagonal on a HR diagram

A

White dwarfs

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9
Q

What categories of stars lie above the main sequence diagonal on a HR diagram

A

Red giants and red supergiants

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10
Q

State the equation linking the intensity, luminosity and distance of a star

A

I = L / (4πd^2)

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11
Q

What is the doppler effect

A

The doppler effect is the apparent change of wavelength as result of relative movement between a receiver and source

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12
Q

What happens to the observed wavelength of a wave source moving away from the observer

A

The observed wavelength will increase

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13
Q

What happens to the observed wavelength of a wave source moving towards an observer

A

The observed wavelength will decrease

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14
Q

What happens to the observed frequency of a wave source moving towards an observer

A

The observed frequency will increase

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15
Q

What is red-shift

A

Red-shift is the apparent shift of the wavelength of light emitted by a star towards the red end of the light spectrum, as a result of it receding

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16
Q

What equations are used to calculate red-shift

A

z = Δλ/λ = Δf/f = v/c

17
Q

Describe how the relative speed value inputted into the equation differs depending on whether the source and receiver are nearing or receding

A

If the source and receiver are approaching each other, the value should be negative, otherwise the value is positive

18
Q

What is the difference between a positive and negative ‘z’ value

A

A positive ‘z’ value represents red shift, whereas a negative value represents blue shift

19
Q

What are the two main conclusions that can be drawn from observations of red shift from distant galaxies

A
  1. All galaxies show red shift and so all galaxies are moving away
  2. The more distant a galaxy is, the greater its red shift and so the faster it is receding
20
Q

What does the red-shift of distant galaxies provide evidence for

A

Red-shift of distant galaxies suggests that they are moving away from us. This supports the concept that the universe is expaning, which supports the Big Bang theory

21
Q

What does CMBR stand for

A

Cosmic Mircowave Background Radiation

22
Q

What is cosmic microwave background radiation

A

Radiation in the microwave region of the EM spectrum that is present in very small quantities all around us

23
Q

How does the existance of CMBR support the Big Bang theory

A

In the big bang, lots of high energy radiation was produced. As the universe has expanded over time, the wavelength of this radiation has been ‘stretched’ so that it is now in the microwave region. Other theories of the universe can’t account for the existance of CMBR

24
Q

What is the Big Bang theory

A

The Big Bang thery is a theory for the formation of the universe. It proposes that the universe began from a very small, hot and dense region, and expanded from this point

25
Q

What two quantities does Hubble’s law relate

A

The distance of a galaxy to the speed at which it is moving away

26
Q

Express Hubble’s law in words

A

The speed at which a galaxy is moving away, is directly proportional to the distance it is at

27
Q

State the defining equation for Hubble’s law

A

v = Hod

Where Ho is Hubble’s constant

28
Q

Describe what was observed when observations of galaxies’ brightnesses were compared to the predictions made by Hubble’s law

A
  • THe actual and predicted brightnesses of distant galaxies don’t always agree with each other
  • Distant galaxies aren’t as bright as predicted by Hubble’s law, suggesting that they are more distant that predicted
29
Q

State the conculsion that can be made from Hubble’s law and observations

A

The rate of expansion of the universe is accelerating, since galaxies are further away than predicted

30
Q

Give one possible explanation for the acceleration of the universe’s expansion

A

The existence of dark energy. This would explain where the energy required for the expansion rate to cnstantly accelerate comes from

31
Q

Why is the existence of dark energy still only a hypothesis

A

Dark matter and energy can’t easily be observed