Luminosity and intensity of starsEdexcel A-Level Physics: Flashcards
Card 1 of 120 of 12 known
Question
Define the luminosity of a star.
Tap or press Space to reveal
Tap card or press Space to flip
See all 12 cards
- Define the luminosity of a star.
- The total power it radiates in all directions across all wavelengths, in watts.
- Define intensity.
- Power received per unit area, perpendicular to the radiation, in W m⁻².
- State the equation linking intensity, luminosity and distance.
- Where does the 4πd² come from?
- It is the surface area of a sphere of radius d, over which the star's power is spread.
- What happens to the intensity if the distance from a star doubles?
- It falls to one quarter.
- What happens to the intensity if the distance from a star triples?
- It falls to one ninth.
- State two assumptions in using I = L/4πd².
- The star radiates equally in all directions; no light is absorbed or scattered between the star and the observer.
- Rearrange I = L/4πd² to find the distance.
- Rearrange I = L/4πd² to find the luminosity.
- What is the luminosity of the Sun?
- W
- Two stars give the same intensity at the Earth, and one has four times the luminosity of the other. Compare their distances.
- The more luminous star is twice as far away.
- Why is luminosity not the same as how bright a star looks?
- Apparent brightness (intensity) also depends on the distance from the star.
Exam questions on Luminosity and intensity of stars
- An astronomer measures the intensity of the light received from distant stars using a telescope fitted with a sensitive detector.Explain why the intensity of the light received from a star decreases as the distance from the star increases.2 marks
- The Sun has a luminosity of 3.85 × 10²⁶ W. The mean distance from the Sun to the Earth is 1.5 × 10¹¹ m. Assume that the Sun radiates equally in all directions and that no radiation is absorbed on its way to the planets.The planet Mars is 2.3 × 10¹¹ m from the Sun. Calculate the intensity of sunlight at Mars.2 marks
- Astronomers measure the intensity of light from a bright star, S, as 1.2 × 10⁻⁷ W m⁻² at the Earth. Star S is 8.1 × 10¹⁶ m from the Earth.Calculate the luminosity of star S.3 marks
Written by the Exaim team, led by Shaun Daswani (Head of Upper Secondary, Improve ME Institute; MSc Financial Mathematics, Imperial College London; BSc, UCL) and Jason Daswani (operational lead, Improve ME Institute; LSE).