Topic 11 telescopes Flashcards

(32 cards)

1
Q

simply, how do telescopes work

A

have a lens, mirror or both to enlarge images by collecting light

lens/mirror place at end of tube, light is magnified/reflected to an eyepiece which shows an enlarged image of what is being viewed

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2
Q

what are the 2 types of telescope

A

refractor, reflector

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3
Q

describe refractor telescope

A

convex lens used at end of a tube to bring an image into focus at a point
-another lens called an eyepiece is used at the opposite end of the tube to magnify the image

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4
Q

what is convex lens made of

A

glass coated in a film to allow less light to be reflected and more to pass through the lens

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5
Q

give 2 examples of refracting telescopes

A

GALILEAN
KEPLERIAN

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6
Q

give features of galilean telescope

A

-uses concave lens aa eyepiece
-typically fixed focus
-has limited field of view

REFRACTING

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7
Q

give features of keplerian telescope

A

-uses convex lens
-larger and heavier than galilean
-focusable
-images are inverted

REFRACTING

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8
Q

what are the 2 reflector telescopes

A

newtonian
cassegrain

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9
Q

give features of newtonian reflector

A

-concave mirror reflects light
-focuses by secondary mirror further up tube @ 45 degree angle
-magnified using eyepiece

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10
Q

give features of a cassegrain reflector

A

reflects loght from concave lens to seco dary mirror
-this mirror is facing primary mirror, reflectes light back down toward sprimary but focuses through a small hole behind primary

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11
Q

what is a reflector’s mirror usually made of

A

glass with an aluminium coating

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12
Q

give 3 reasons why reflectors have gained popularity over refractors

A

-higher resolution can be achieved with a smaller tube
-refractors suffer from chromatic abberation (colour can be warped)
-refractors suffer from lens sagging

-refractors have a maximum size of 1 metre wide

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13
Q

define aperture

A

amount of light the telescope receuves (larger lens/mirror=higher aperture)

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14
Q

what does aperture determine

A

how well we are able to see fainter objects

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15
Q

what is light grasp

A

kight-gathering power
-measure of telescope’s ability to capture light and is directly related to size of instruments main lens/mirror

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16
Q

what is light grasp directly proportional to

A

area of objective element and thus the square diameter of ovjective element

17
Q

true fov=?

A

apparent fov/magnification

18
Q

define resolution

A

how a telewcope will shwo the detail of an object being observed

19
Q

how can you increase resolution

A

increase aperture size

20
Q

what else determines the resolution

A

-diffraction of light caused by atmosphere
-wavelenght
-quality of telescope
-contrast
-brightness
-observer’s quality of eyesight

21
Q

what is another phrase for a telescope’s resolution

A

angular resolution
or
resolving power

22
Q

formula for resolution

A

wavelength/diameter

23
Q

what did galileo discover

A

jupiter’s four large satellites
moon’s uneven surface
venus’ phases
sunspots

24
Q

what was galileo the first to do

A

he was the first telescopic observer to make published astronomical observations

25
name 4 advantages of using reflecting telescopes over refracting telescopes
1. chromatic abberation 2. very long focal lengths 3. using large aperture objectives 4. use of multiple mirrors
26
why are mirrors better than lenses
cheaper to manufacture
27
which telescope uses a counterweight why doesnt the other telescope type
reflector as refractors need a sizeable mount to manage its latge weight
28
why are mirrors an advantage over lenses
-lenses absorb more wavelengths than mirros -all parts of lens need to be manufactured and maintained to keep free of impurities but only one side needs to be kept pristine in a mirror -focal lengths can be increased while retaining short tube by adding more mirrors
29
30
when does chromatic abberation occur
when a lens fails to focus light rays colours to the same focal point
31
who invented reflecting telescopes
isaac newton
32
whats a barlow lens
allows eyepieces to be slotted into it, can increase magnification by factor of 2 or 3