Astrophysics Flashcards

(49 cards)

1
Q

What are disadvantages of refracting telescopes?

A

Chromatic and spherical aberration.
Distortion due to warping of glass.
Expensive.

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2
Q

What is chromatic aberration?

A

Different wavelengths focus at different points causing blurred image.

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3
Q

What is spherical aberration?

A

Spherical lens means rays focus at different points.
Closer to centre of lens = focuses further away.

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4
Q

Which colour of light focuses furthest from lens due to chromatic aberration?

A

Red.

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5
Q

What is resolving power / Rayleigh criterion?

A

Minimum angle at which two objects are able to be differentiated between.
Central maximum of one sits over the first minimum of the other.

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6
Q

What is quantum efficiency?

A

Number of photons detected / Number of photons incident x 100

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6
Q

What is a CCD and how does it work?

A

Silicon chip divided into pixels.
Incident light liberates electrons which are trapped in potential wells.
Number of electrons liberated is proportional to intensity of light.
Pattern built up by electrons forms image.

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7
Q

What is the quantum efficiency of a CCD?

A

Around 70%

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8
Q

What is the gathering power?

A

Energy / photons collected per second.

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9
Q

What is brightness of a telescope proportional to?

A

d^2

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10
Q

What is luminosity

A

Total energy emitted per second (power).

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11
Q

What number is used to compare the brightness of stars?

A

2.512

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12
Q

What is a parsec?

A

Distance an object must be to have a parallax of one arcsecond when observed from Earth.

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13
Q

What is a light year?

A

Distance an EM wave travels in a year.

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14
Q

What is apparent magnitude?

A

Magnitude of a star as seen from Earth.

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15
Q

What is spacial resolution?

A

How far apart objects need to be to be distinguishable.

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16
Q

What is a blackbody?

A

Absorbs and can emit all wavelengths of EM radiation.

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17
Q

What is the area under a black body curve?

A

Intensity.

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18
Q

Which telescopes cannot be grounded on Earth?

A

Infrared
UV
X-Ray
Gamma

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19
Q

What do lines on absorption spectrum refer to?

A

Photons absorbed by gases.

20
Q

What do lines on an emission spectrum refer to?

A

Photons emitted from energy levels.

21
Q

Where do electrons with a high temp reside in for Balmer series?

A

n=2 level, so strong lines.

22
Q

Where do electrons with a low temp reside in for Balmer series?

A

n=1 level, so weak lines.

22
Q

Where do electrons with a very high temp reside in for Balmer series?

A

n=3 level, so less strong lines.

23
What is the lifetime of a star similar in mass to our Sun?
- Gas cloud - Main sequence (H burning) - Red giant (He burning) - Dwarf
24
What is Hydrogen burning?
Fusion of Hydrogen into Helium.
24
What is radiation pressure?
Pressure exerted upon any surface with EM radiation.
25
What will a star < 1.4 solar masses turn into?
White dwarf
26
What will a star > 3 solar masses turn into?
Black hole
26
What will a star > 1.4 solar masses turn into?
Neutron star
27
What is the neutron degeneracy force?
Repulsive strong nuclear force, counteracts inwards gravity.
28
What is the Schwarzschild radius?
Radius at which light cannot escape a black hole.
28
How does a type 1a supernova occur?
- White dwarf steals energy from a close star. - Gains mass and collapses at 1.4 solar masses. - High temp means carbon can be fused. - Undergoes nuclear fusion and explodes in supernova.
29
What is a standard candle?
An object of known luminosity.
30
If the apparent frequency of a star is less than the true frequency of a star what happens?
Red shifted.
30
If the apparent frequency of a star is greater than the true frequency of a star what happens?
Blue shifted.
31
What are the units for velocity and distance in Hubble's law?
km/s and Mpc
32
What are 3 pieces of evidence of the big bang?
- Expansion of the universe. - Cosmic microwave background radiation. - Relative abundance of H and He.
33
What is CMB?
High frequency radiation released after big bang when matter and radiation 'decoupled' (universe cooled). Variations are thought to be seeds of galaxies.
34
How does red shift support the big bang theory?
Galaxies further away are accelerating away from us. Reverse time back puts all matter and universe into one place, universe started from one infinitely dense and hot point.
35
How does the relative abundance of H and He support the big bang theory?
H to He is 3:1. Early universe was hot enough to fuse He but cooled too quickly to fuse anything heavier.
36
What is a quasar?
Active galactic nuclei, supermassive black hole at the centre of the galaxy.
37
How is a quasar formed?
Gravitational pull of material is so strong that the collisions of these in the accretion disk produce extremely high amounts of radio (high energy) waves.
38
How were quasars discovered?
High levels of high frequency radiation. Brightest celestial objects in universe, jets of radiation shoot out either side.
39
What is an exoplanet?
A planet that orbits a star outside of our solar system.
40
What are the two methods of detecting exoplanets?
Transit and radial velocity / doppler.
41
Describe the radial velocity / doppler method of detecting an exoplanet.
Orbits centre of mass which makes star wobble. If wobble is aligned to our line of sight, red and blue shifts will be seen.
42
Describe the transit method of detecting an exoplanet.
As planet moves between the observer and the star, apparent magnitude will change (dip in light curve).
43
What is absolute magnitude?
Magnitude of a star if it was 10 parsecs from Earth.