Space Flashcards

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1
Q

What is a black body?

A

A body of matter that absorbs all radiation that lands on it and it can be considered to be the perfect emitter

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2
Q

What does the narrowest peak represent on a black body diagram of emitted light?

A

Most radiation is emitted at this wavelength

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3
Q

As temperature of a black body increases, what happens to the peak wavelength of radiation emitted?

A

The peak shifts to the left ( lower wavelength )

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4
Q

What wavelength do really cold objects emit radiation at?

A

Really high wavelength like radiowaves

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5
Q

What type of light do everyday temperature black body’s emit?

A

Infrared light

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6
Q

Do stars behave like black bodies?

A

Yes because they emit a continuous spectrum of radiation

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7
Q

What’s Weins law (black bodies)

A

For each temperature, there a peak in the radiation curve called the peake wavelength

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8
Q

Define luminosity

A

Energy radiated by an object per second (in Watts)

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9
Q

What’s the relationship between luminosity and temperature or surface area?

A

Directly proportional to both

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10
Q

What is a protostar?

A

Clouds of dust and gas that clump together under gravity

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11
Q

Describe the Hertzsprung-Russell diagram.

A

Y-axis is luminosity
X-axis is temperature (goes from high to low)
Dwarfs bottom, main sequence middle diagonal, giants high right, super giant very top

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12
Q

Whats a problem with trigonometric parallax?

A

It’s only applicable to close stars, as when the distance increases the angle become too small to measure.

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13
Q

What is 1° in minutes of arc?

A

60’

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14
Q

What is a parsec?

A

The distance the star needs to be for the angle to be 1 second of arc

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15
Q

What are standard candles

A

Objects which have a known luminosity

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16
Q

How old is the universe roughly

A

13.8 billion years

17
Q

What does a high pitch of sound mean

A

The sound has a higher frequency

18
Q

What does a louder noise mean?

A

Large amplitude

19
Q

How do we know the universe is expanding.

A

By measuring the redshift of galaxies, astronomers can determine the speed at which they are moving away from us.

20
Q

Describe the characteristics of a main sequence star.

A

Constantly converting hydrogen to ugh fusion and maintaining a constant luminosity

21
Q

Describe how to find the distance of nearby stars.

A

Use trigonometric parallax go find the angle against the background that a star moves by in 6 months. Use this to find the distance .

22
Q

Why do large stars have greater luminosity

A

Surface temperature and area is the greatest. Most massive stars experience high gravitational force. Therefore, high temperature and density in the core. So rate of fusion is greatest.

23
Q

Explain the conditions required to bring about and maintain nuclear fusion in stars.

A
  • High temperature needed
  • nuclei all have positive charge leading to a large repulsive force between nuclei
  • at high temps nuclei have KE sufficient to overcome repulsion
  • nuclei must get close enough to fuse
  • required high density
  • collision rate must be high enough to sustain fusion
24
Q

Why do astronomers have difficulty in making accurate measurements to galaxies or measuring the critical density of the universe?

A

There’s a large uncertainty in bubbles constant because dark matter creates uncertainty of the values of mass and density.

25
Q

What is dark matter roughly?

A

Matter that doesn’t interact with electromagnetic force

26
Q

What is critical density?

A

The density of mass of the universe that means gravity is just strong enough to stop the expansion.

27
Q

Explain why radiation received from the earliest stars formed in the universe is in the radio wavelength region of the electromagnetic spectrum.

A
  • The radiation has to travel many light years to reach us
  • Light gets red shifted to the radio wavelength
  • The Universe is expanding so wavelength has been stretched
28
Q

What can be said about a star that is very bright, easily visible and has a orange-red colour?

A
  • It is a red giant
  • Very high luminosity (bright)
  • Large mass and volume as it is visible
  • Not a very hot star because of the orange red colour
  • Heavier elements undergo fusion on the staf