Lesson 10.2.1
10.2.1 Hertzsprung-Russell diagram and the life cycle of stars Quiz: Pearson Edexcel Physics, Unit 10
20 questions
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Lesson 10.2.1, Hertzsprung-Russell diagram and the life cycle of stars: 20 multiple choice questions for the Pearson Edexcel Physics (9PH0), Unit 10: Space, written with Revision Ninja.
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The 20 questions
-
How is surface temperature represented on the horizontal axis of an HR diagram?
- Increasing to right
- Constant throughout
- Decreasing upwards
- Decreasing to right
-
What process provides the primary energy source for a main sequence star?
- Helium core fusion
- Gravitational collapse
- Carbon core fusion
- Hydrogen core fusion
-
What happens to a star's outer layers as it transitions into a red giant?
- They expand and cool
- They contract and heat
- They contract and cool
- They expand and heat
-
What describes the fusion activity inside a white dwarf star?
- Hydrogen fusion
- Carbon fusion
- No fusion occurs
- Helium fusion
-
Where on a Hertzsprung-Russell diagram is a star with high temperature and high luminosity located?
- Bottom left
- Bottom right
- Top left
- Top right
-
Where on a Hertzsprung-Russell diagram are red dwarfs located?
- Bottom left
- Bottom right
- Top right
- Top left
-
Why can a star with a low surface temperature have a very high luminosity?
- Very small radius
- Very large radius
- High density
- Rapid rotation
-
A star has the same surface temperature as the Sun but 100 times the Sun's luminosity. What is the ratio of its radius to the Sun's radius?
- 100
- 10
- 1/10
- 50
-
A star has the same radius as the Sun but twice its surface temperature. How many times its luminosity?
- 16 times
- 8 times
- 2 times
- 4 times
-
A star has radius 10 times the Sun's radius and surface temperature 3000 K, compared with the Sun at 5800 K. Approximately how does its luminosity compare with the Sun's?
- about 1400 times
- about 7 times
- about 100 times
- about 0.07 times
-
How do luminosity and surface temperature change when a star becomes a red giant?
- Luminosity rises, temperature rises
- Luminosity falls, temperature falls
- Luminosity falls, temperature rises
- Luminosity rises, temperature falls
-
Why do high-mass main sequence stars have shorter lifetimes than low-mass stars?
- Lower core density
- Lower core temperature
- Higher fusion rate
- Less hydrogen fuel
-
Why are most observed stars located on the main sequence of the HR diagram?
- Final evolutionary stage
- Briefest stellar phase
- Highest temperature phase
- Longest evolutionary stage
-
Why does a white dwarf have a low luminosity despite its high surface temperature?
- High hydrogen fuel
- Large surface area
- Small surface area
- Low core mass
-
A star of radius 1.0 x 10^9 m has surface temperature 10000 K. What is its luminosity? Use σ = 5.67 x 10^-8 W m^-2 K^-4.
- 7.1 x 10^27 W
- 1.4 x 10^28 W
- 7.1 x 10^25 W
- 5.7 x 10^27 W
-
Which properties place red giants in the top right of an HR diagram?
- Low luminosity, high temperature
- High luminosity, high temperature
- Low luminosity, low temperature
- High luminosity, low temperature
-
What changes a star's position on a Hertzsprung-Russell diagram as it evolves?
- Mass and velocity
- Charge and radius
- Pressure and density
- Luminosity and temperature
-
Which change moves a star vertically upwards on an HR diagram at constant temperature?
- Increasing its temperature
- Increasing its radius
- Decreasing its radius
- Decreasing its luminosity
-
What remnant can be left behind after a massive star undergoes a supernova?
- Protostar
- White dwarf
- Neutron star
- Red giant
-
Why is a main sequence star more luminous than a red dwarf of equal radius?
- Smaller surface area
- Higher surface temperature
- Lower surface temperature
- Greater core mass
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