Every sub-topic AQA can examine in this topic, with its reference number from the official specification. The Y12 and Y13 tags show when each sub-topic is usually taught.
3.9.1 Telescopes
3.9.1.1Astronomical telescope consisting of two converging lensesY13
3.9.1.2Reflecting telescopesY13
3.9.1.3Single dish radio telescopes, I-R, U-V and X-ray telescopesY13
3.9.1.4Advantages of large diameter telescopesY13
3.9.2 Classification of stars
3.9.2.1Classification by luminosityY13
3.9.2.2Absolute magnitude, MY13
3.9.2.3Classification by temperature, black-body radiationY13
3.9.2.4Principles of the use of stellar spectral classesY13
3.9.2.5The Hertzsprung-Russell (HR) diagramY13
3.9.2.6Supernovae, neutron stars and black holesY13
3.9.3 Cosmology
3.9.3.1Doppler effectY13
3.9.3.2Hubble's lawY13
3.9.3.3QuasarsY13
3.9.3.4Detection of exoplanetsY13
Try 3 questions
Easy, medium and hard questions from this topic, each with a worked solutions and the mark for every step. All 95 questions in this topic, free, no account needed.
Thermodynamics
Not needed for Year 12Easy
Black body radiation · Year 13 · 3 marks
A black body is heated from 3000 K to 6000 K.
(a)
Define a black body.
(1)
(b)
Describe two changes to its emission spectrum.
(2)
Show worked solutionHide worked solution
Working, step by stepMarks
Part (a)1 mark
A body that absorbs all the radiation that falls on it.
B1
Part (b)2 marks
The peak moves to a shorter wavelength.
B1
The intensity at every wavelength (and the total power) increases.
B1
Total3
MMethodMethod mark: for a correct method, even with a slip.
AAccuracyAccuracy mark: for a correct answer from a correct method.
BIndependentIndependent mark: for a correct fact or result on its own, with no method needed.
With your permission, SUVAT counts which pages are visited: anonymously, with no tracking cookies. (One essential cookie keeps you signed in; that needs no permission.)May SUVAT count page visits, anonymously and without tracking cookies?How your data is used