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9702 · 25.1

Standard candles

Cambridge 9702 Paper 4 — Standard candles (25.1). Senpai Corner diagram-backed pilot with premium structure and live visuals.

Need to know

What you need to know

  • 25.1 Standard candles.
  • Luminosity L is defined as the total power output of radiation emitted by a star .
  • It is measured in Watts.
  • The observed amount of intensity F is the observed amount of intensity, or the radiant power transmitted normally through a surface per unit of area, of radiation measured on defined as Earth.
  • Light leaving a star can be assumed to be a uniformly spread out like a spherical shell.
  • Hence, the inverse square law of flux can therefore be calculated using 𝐹 = 𝐿 4𝜋𝑑 2 Here L is the luminosity of the source (watts), d is the distance between the star and Earth (m).

Explanation

Standard candles

  1. 25.1 Standard candles.
  2. Luminosity L is defined as the total power output of radiation emitted by a star .
  3. It is measured in Watts.
  4. The observed amount of intensity F is the observed amount of intensity, or the radiant power transmitted normally through a surface per unit of area, of radiation measured on defined as Earth.