25.1 A2 Level

Standard candles

7 flashcards to master this topic

Definition Flip

Define luminosity in the context of stars.

Answer Flip

Luminosity (L) is the total power of electromagnetic radiation emitted by a star. It is measured in Watts (W) and is an intrinsic property of the star.

Definition Flip

State the inverse square law for radiant flux intensity (F) in terms of luminosity (L) and distance (d).

Answer Flip

The radiant flux intensity (F) is given by F = L / (4πd²), where L is the luminosity of the source and d is the distance from the source.

Definition Flip

What is a 'standard candle' in astronomy?

Answer Flip

A standard candle is an astronomical object with a known luminosity. By comparing its known luminosity to its observed flux intensity, astronomers can determine its distance.

Key Concept Flip

Explain how standard candles are used to determine distances to galaxies.

Answer Flip

By measuring the radiant flux intensity (F) of a standard candle in a distant galaxy and knowing its luminosity (L), we can use the inverse square law (F = L / (4πd²)) to calculate the distance (d) to the galaxy.

Key Concept Flip

Give an example of a standard candle and why it is useful.

Answer Flip

Type Ia supernovae are excellent standard candles. They have a consistent peak luminosity due to their consistent formation process (white dwarf exceeding the Chandrasekhar limit), allowing accurate distance measurements to very distant galaxies.

Calculation Flip

If a star has a luminosity of 4 x 10^26 W and its radiant flux intensity measured on Earth is 8 x 10^-16 W/m², calculate its distance from Earth.

Answer Flip

Using F = L / (4πd²), we can rearrange to find d = √(L / (4πF)). Substituting the values gives d = √((4 x 10^26) / (4π * 8 x 10^-16)) ≈ 1.99 x 10^20 m.

Key Concept Flip

Describe a limitation of using standard candles for measuring extremely large distances.

Answer Flip

At extremely large distances, the observed flux intensity of standard candles becomes very faint and difficult to measure accurately. Furthermore, the effects of interstellar dust and gas absorption can affect the measurement, leading to uncertainties in distance calculations.

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