The Sun is a star in a stable part of its life cycle.
Using ideas about forces, explain how the Sun remains stable in this part of its life cycle.
The Sun is a star in a stable part of its life cycle.
Using ideas about forces, explain how the Sun remains stable in this part of its life cycle.
Describe what happens to stars of similar mass to the Sun at the end of the stable part of their life cycle.
The orbital speed of Earth around the Sun is 30 km / s. Use this value to calculate the distance of Earth from the Sun.
Show your working. State the unit of your answer.
distance = ...................................... unit = ..........
The light emitted by distant galaxies show various amounts of redshift.
State the name of the galaxy that contains our Sun.
State what is meant by redshift and describe how it is caused.
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Fig. 10.1 shows corresponding spectral lines from the Sun and from two distant galaxies P and Q. State what can be deduced about P and Q from these spectra. Explain your answer.
An astronomer compares the spectrum of light emitted by the Sun with the spectrum of light emitted by distant galaxies P and Q.
Fig. 10.1 shows the same four lines as observed in all three spectrums.
State what Fig. 10.1 enables the astronomer to deduce about galaxy P and galaxy Q.
Explain the astronomer’s reasons in your answer.
5054/02/SP/23Cambridge O Level Physics 5054 · Specimen 2023 · Paper 2 · Question 10