19 Flashcards

(21 cards)

1
Q

Why are telescopes better than the human eye for observing distant objects?

A

Because they gather more light using larger apertures, improving brightness and resolution.

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2
Q

What formula is used to calculate the light-gathering power (LGP) of a telescope?

A

LGP ∝ D², where D is the diameter of the mirror or lens.

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3
Q

What is the angular magnification of a telescope?

A

m = -fo/fe, where fo is the focal length of the objective and fe is the focal length of the eyepiece.

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4
Q

Why are large refracting telescopes difficult to build?

A

Large lenses sag under their own weight, are expensive to make, and cause chromatic aberration.

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5
Q

What are the advantages of reflecting telescopes over refracting ones?

A

They can be larger, avoid chromatic aberration, and are structurally supported from behind.

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6
Q

What is a Newtonian focus in a reflecting telescope?

A

It uses a flat mirror to redirect light to the side of the telescope for easier viewing.

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7
Q

What limits the resolution of any optical device like a telescope?

A

Diffraction, due to the wave nature of light.

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8
Q

What is the formula for the diffraction limit (Rayleigh’s criterion)?

A

θ = 1.22 λ / D

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9
Q

What does a smaller angular resolution mean?

A

Better resolving power—ability to distinguish closely spaced objects.

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10
Q

What are the units and conversion for angular resolution?

A

Radians or arc-seconds (1° = 3600 arc-seconds)

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11
Q

What three factors improve telescope observations?

A

More light larger telescope,longer exposure

Smaller angular resolution , larger telescope

Atmospheric effect
Adaptive optics go to space top of mountain

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12
Q

What are adaptive optics?

A

Technology that corrects for atmospheric distortion by adjusting the mirror shape in real-time.

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13
Q

Why do we place telescopes in space?

A

To avoid atmospheric distortion and absorption of non-visible radiation.

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14
Q

Which wavelengths can pass through Earth’s atmosphere?

A

Visible light and radio waves.

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15
Q

Name telescopes specialized for non-visible wavelengths.

A

HST (visible, UV, IR), Chandra (X-ray), Spitzer (IR), CGRO (Gamma-ray), LIGO (gravitational waves).

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16
Q

What does LIGO detect?

A

Gravitational waves—ripples in spacetime from cosmic events.

17
Q

What is light pollution?

A

Bright city lights that limit our ability to see stars clearly.

18
Q

What is the advantage of segmented mirrors like JWST?

A

Easier to build large-diameter telescopes by assembling smaller segments.

19
Q

How is exposure time related to light gathering?

A

LGP ∝ Area × Time; longer exposure allows more detail in images.

20
Q

What is the diffraction pattern from a circular aperture?

A

A central bright spot surrounded by concentric rings of alternating brightness.

21
Q

Chromatic Aberration

A

an optical distortion that causes a lens to focus different colors of light at slightly different points, resulting in color fringing or a “color blur” along the edges of objects in an image