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
- 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.