Astro-Physics Flashcards

1
Q

Give two equations for magnification of a refracting telescope.

A

1) M = α / β
2) M = Fo / Fe (Focal Objective / Focal Eyepiece)

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2
Q

Define 1 arc minute.

A

1/60 of a degree

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3
Q

What is 1 degree in arc minutes

A

60 arc minutes

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4
Q

What’s the equation for angular size of an object

A

Diameter of object / Distance to eye or lense

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5
Q

List two “aberrations” of refracting telescopes

A

1) Chromatic Aberration
2) Spherical Aberration

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6
Q

What is meant by Chromatic Aberration

A

The refractive index of a lens is different for different wavelengths so different colours are brought to focus at different points. SHORTER WAVELENGTH => SMALLER FOCAL LENGTH

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7
Q

What is meant by Spherical Aberration

A

Due to manufacturing difficulties, imperfections in a lens cause rays further from the principle axis to be brought to focus closer to the lens.

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8
Q

What criteria must be met for a a refracting telescope to be in “normal adjustment”

A
  • Objective and eyepiece lenses share a principle focus (separation = Fo + Fe)
  • Must be focused at infinity (meaning everything in frame is in focus)
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9
Q

What is meant by the term Collecting power of a telescope

A

How much light enters the telescope hence determining the brightness of the observed image

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10
Q

What is the relationship between collecting power and telescope aperture

A

Collecting power is directly proportional to (Diameter of Aperture)^2

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11
Q

What is meant by the term Resolving Power of a telescope

A

How well the telescope can distinguish between two nearby objects

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12
Q

What is an airy disc

A

It’s a circular diffraction patter around stars caused by diffraction at the telescopes aperture.

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13
Q

What is the Rayleigh Criterion

A

The minimum angular separation for two object to be resolved

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14
Q

When will the minimum angular separation for the Rayleigh Criterion occour

A

When the central maximum of one airy disc coincides with the first minimum of the second airy disc.

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15
Q

List 4 disadvantages of refracting telescopes

A
  • Very difficult to create large lenses
  • Large lenses can deform under their own weight
  • Very difficult to manoeuvre quickly
  • Suffer from chromatic and spherical aberration
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16
Q

List 4 advantages of reflecting telescopes

A
  • Can be made of smaller composite mirrors
  • Large single mirrors can be made fairly easily
  • No chromatic or spherical aberration when using parabolic mirrors
  • Light weight allows quick response to astronomical events