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Chapter 4: Astronomy, A Physical Perspective

Wilhelm André Astrophysics University Englisch 6 Karten

Chapter 4: Astronomy, A Physical Perspective

Karten in diesem Stapel (6)

  1. 1Light GatheringDetermined by the diameter of the lense.
    We use the formula below to determine how many magnitudes fainter stars a diameter d_2>d_1 can see.
    Light Gathering
  2. 2Angular resolutionAngular resolution
  3. 3Focal lengthThe distance from the lens at which a bundle of rays are gatheredFocal length
  4. 4Focal ratiof = aperture on a camera.
    Each f-stop on a camera changes the brightness by a factor 2. Therefor each f-stop is a factor √2.
    Focal ratio
  5. 5Linear seperation, xThe linear distance between two objects that form an angle theta with the lens/film-axis.Linear seperation, x
  6. 6Angular magnificationThis is how much the angular size of an object will increase. On binoculars or telescopes it can be 10x or 25x etc.Angular magnification

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University Astrophysics Karteikarten am Chapter 4: Astronomy, A Physical Perspective, erstellt von Wilhelm André am 03/05/2016.
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Wilhelm André
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