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
Typical Type 1a Supernova Light Curve
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.
Answer:
Step 1: Write down the magnitude equation
- Where
- Apparent magnitude, = 11
- Absolute magnitude, = −19
Step 2: Substitute in the values of m and M and rearrange
Step 3: Take logs of both sides to determine the distance d