Supernovae as Standard Candles (AQA A Level Physics): Revision Note

Exam code: 7408

Katie M

Written by: Katie M

Reviewed by: Tim

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Type 1a supernovae as standard candles

  • A standard candle is defined as:

An astronomical object of known brightness that can be used to calculate galactic distances

  • The most common examples of standard candles are:

    • cepheid variable stars

    • type 1a supernovae

  • Type 1a supernovae can be used as standard candles because they reach the same peak value of absolute magnitude each time

    • This type of supernova involves an exploding white dwarf in a binary star system

    • The white dwarf increases in mass as it attracts material from its binary pair

    • Eventually the white dwarf reaches a critical mass, known as the Chandrasekhar limit 

    • This critical mass means the explosion is the same each time, hence it produces a very consistent light curve

Light curve of a Type 1a supernova, where absolute magnitude rises to a peak of −19 near day 0 before steadily fading. Time is shown in days, from about −30 to 250, and absolute magnitude from −12 to −21.
The light curve of a type 1a supernova always has the same characteristic shape and reaches the same peak absolute magnitude
  • Another advantage of using type 1a supernovae as standard candles is that they are extremely bright

    • This means they can be used to measure the distance to the furthest galaxies

Worked Example

An astronomer observes a type 1a supernova in a distant galaxy with an apparent magnitude of +11 at its peak of brightness.

At its peak, it is known that a type 1a supernova has an absolute magnitude of about −19.

Show that the galaxy is about 10 Mpc away.

[2]

Answer:

Step 1: Write down the magnitude equation

m − M = 5 log (d10)

  • Where:

    • Apparent magnitude, m = 11

    • Absolute magnitude, M = −19

Step 2: Substitute in the values of m and M and rearrange

5 log (d10) = 11 − (−19) = 30

log (d10) = 305 = 6 [1 mark]

Step 3: Take logs of both sides to determine the distance d

d10 = 106

d = 10 × 106 pc = 10 Mpc [1 mark]

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Katie M

Author: Katie M

Expertise: Curriculum Expert

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.

Tim

Reviewer: Tim

Expertise: Content Creator

Timothy graduated with a first class degree in Mathematics and Physics from the University of Warwick. After working as a postgraduate researcher, Timothy has worked as a content creator for various online revision platforms, creating physics resources for a range of levels and exam boards.