Stellar Evolution (Edexcel IGCSE Physics)

Exam Questions

2 hours17 questions
1a3 marks

The sentence gives information about the life cycle of a star. 

Use the words in the box to complete the sentence. Some words may be used more than once, or not at all.

electron             supernova             giant             dwarf          momentum  neutron

A very dense .................................. star is left behind when a large red .................................. star blows up in an explosion called a ..................................

1b1 mark

Which of the following statements is a property used to classify stars?

  • Radius

  • Distance from the Earth

  • The times when it is visible to observers on Earth

  • Colour

1c3 marks

Draw lines between the colour and the temperature to show the correct colour and temperature of the stars. 

star-temp-colour-match-sq-edexcel-igcse

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2a2 marks

This paragraph is from a website. 

A star forms when enough dust and gas are pulled together. Masses smaller than a star may also be formed when dust and gas are pulled together.

 (i) State the name of the force that pulls the dust and gas together.

(ii) State the name of the object described as mass smaller than a star that may form when the gas and dust are pulled together.

2b3 marks

The diagram shows part of the life cycle of a star with a similar mass to the Sun.  

black dwarf          nebula          fusion          white dwarf          main sequence star

Use words from the box to label the stages in the life cycle. 

8-2-2b-e-life-cycle-solar-mass-stars-label-sq-edexcel-igcse

 

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3a1 mark

What is the absolute magnitude of a star a measure of?

  • The brightness of stars if they were the same distance away from the Earth

  • The temperature of stars

  • The density of star clusters

  • The distance the star is away from the Earth

3b3 marks

The table gives some statements about the absolute magnitude scale. 

Put ticks (✓) in the boxes to show which three statements are correct.

Statement

Correct (✓)

The brighter the star the larger the magnitude

 

The brighter the star the smaller the magnitude

 

The dimmer the star the larger the magnitude

 

The brightness of the star depends upon how much light the star emits

 

The brightness of the star depends upon the radius of the star

 

The brightness of the star depends upon how far away the star is

 

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4a3 marks

Describe how stars are formed.

4b3 marks

Add words from the box in the gaps to make the sentences correct. 

decay          balanced          fission          resultant forces          fusion          forces

(i) Nuclear ...................................... releases energy inside stars. 

(ii) A star is stable during the 'main sequence' period in its life because the ...................................... within it are ......................................

4c4 marks

The life cycle of a star after the 'main sequence' period depends on the size of the star.  A particular star is much larger in size than the Sun. 

Complete the stages of the life cycle of this star.

8-2-4c-e-life-cycle-larger-stars-box-fill-sq-edexcel-igcse

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5a2 marks

The Hertzsprung-Russell (HR) diagram is used to classify stars. 

Label the horizontal and vertical axes of the diagram by writing in the boxes.

8-2-5a-e-hr-fill-in-axis-sq-edexcel-igcse
5b4 marks

The words in the box detail the different classifications of stars. 

supergiants            white dwarfs          main sequence stars          giants

Complete the table by matching the star classification with the area it is found on the HR diagram.

Area

Classification

A

 

B

 

C

 

D

 

5c2 marks

The Sun is labelled on the HR diagram.  

Use the HR diagram to identify the luminosity and temperature of the Sun.

luminosity of the Sun = ................... LSun

 temperature of the Sun = ................... K

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1a1 mark

The diagram shows some incomplete notes about a stellar process. An astronomer left the notes to a colleague for them to decipher. 

Flowchart depicting stages of star formation, with stage 4 missing. Stages involve dust and gas cloud collapse, nuclear fusion, and final star instability.

Name the process described in the diagram.

1b1 mark

The colleague wants to include some extra detail in stage 3.

Which of the following correctly describes the physical process outlined in stage 3 and the 'smaller nuclei' and 'bigger nuclei' that are mentioned?

 

physical process

smaller nucleus

larger nucleus

A

nuclear fission

hydrogen 

helium

B

nuclear fusion 

helium

hydrogen

C

nuclear fission

helium

hydrogen

D

nuclear fusion

hydrogen

helium

    1c1 mark

    The longest stage in this process is

    • stage 2

    • stage 3

    • stage 4

    • stage 5

    1d4 marks

    (i) State the name given to the star in stage 4.

    (ii) Explain what happens in stage 4.

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    2a4 marks

    The colour of visible light a star emits tells us how hot or cold it is.

    The table contains the colour classifications of the visible light emitted from stars. 

    Complete the table by placing a number from 1 − 7 in each box in order of decreasing temperature.

    Colour

    Number

    Yellow-white

     

    Blue

     

    Red

     

    Yellow

     

    Yellow-orange

     

    White

     

    Blue-white

     

    2b5 marks

    (i) State and explain which stage in a star's life cycle is the coolest.

    (ii) State the final stage in the life cycle of a star similar in size to the Sun and explain its colour.

    2c2 marks

    Explain how stars similar to the Sun are formed.

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    3a1 mark

    What are the properties of luminosity and temperature for a main sequence star? 

     

    Luminosity

    Temperature

    A

    low

    low

    B

    low

    high

    C

    high

    low

    D

    high

    high

      3b1 mark

      A Hertzsprung-Russell (H-R) diagram is a plot of luminosity against temperature for a range of stars.

      8-2-3b-m-hr-diag-q-edexcel-igcse

      One group on the H-R diagram is the main sequence.

      Once hydrogen fusion has ceased in its core, the Sun (labelled S) will move to a new position on the H-R diagram above.

      What is the new position of the Sun?

        3c3 marks

        State the letter for the position of a white dwarf on the H-R diagram and describe its temperature and luminosity in relation to the Sun. 

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        4a2 marks

        Most of the stars in the universe are main sequence stars, including the sun. 

        Describe the similarities between main sequence stars.

        4b2 marks

        The table gives some statements about the relationship between a star's colour and its surface temperature. 

        Add ticks (✔) to the table to show which two statements are correct.

        Statement

        Correct (✔)

        red stars have a relatively high temperature

         

        blue stars have a relatively high temperature 

         

        yellow stars have a relatively low temperature

         

        blue-white stars have a relatively low temperature

         

        4c4 marks

        The table shows the colour and surface temperature of several known stars.

        Colour

        Surface Temperature (K)

        Example

        red

        < 3500

        Betelgeuse

        orange

        3500 - 5000

        Aldebaran

        yellow

        5000 - 6000

        Sun

        yellow-white

        6000 - 7500

        Canopus

        white

        7500 - 10 000

        Vega

        blue-white

        10 000 - 25 000

        Rigel

        blue

        > 25 000

        10 Lacertae

        (i) Identify a star with a temperature of 7000 K.

        (ii) Identify a star with a temperature of 2000 K.

        (iii) State and explain which of the stars you identified is likely to be the largest.

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        5a2 marks

        Explain what is meant by the absolute magnitude scale.

        5b1 mark

        Describe the relationship between the absolute magnitude of a star and its brightness.

        5c3 marks

        A selection of celestial objects and some information about their apparent brightness is detailed below. 

        Object

        Information

        Venus

         Venus has a higher absolute magnitude than the Moon

        Moon

        The Moon is the closest object to Earth

        Sirius

        Sirius has an apparent brightness of nearly zero

        Faintest star

        The faintest star that can be seen by the naked eye

        Sun

        The Sun is the brightest star as viewed from Earth

        Faintest object

        The faintest object that can be seen by the naked eye

        Put each object into the correct place on the apparent brightness scale. 

        8-2-5c-m-apparent-magnitude-scale-edexcel-igcse

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        6a4 marks

        A Hertzsprung-Russell (H-R) diagram is shown below. 

        8-2-6a-m-hr-diagram-labelling-sq-igcse

         Label the axis and complete the missing numbers on the scale.

        6b4 marks

        State and describe the type of star found in each region labelled A, B, C and D on the H-R diagram.

        6c2 marks

        On the H-R diagram:

        (i) Add a cross (X) to show the position of the Sun.

        (ii) Draw an arrow to show the direction the star labelled (*) would move as it cools down and emits less energy.

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        1a8 marks

        The table shows the 5 stages of the life cycle of a star that has a similar mass to the Sun. 

        Stage 1

        Initially, there is a massive cloud of dust and gas in space.

        Stage 2

         

        Stage 3

        Hydrogen nuclei join together to make helium nuclei

        Stage 4

         

        Stage 5

        The star eventually becomes unstable. An outer layer of dust and gas is ejected leaving behind a core. The core collapses due to gravity.

         (i) State and explain what happens in stage 2 of the diagram.

        Include specific references to the relationships between

        • the masses of the bodies involved and the forces acting between them

          • the separation of the bodies involved and the forces acting between them

        (ii) State and explain what happens in stage 4 of the diagram.

        1b1 mark

        The timescale of stage 3 is in the order of

        • 105 to 106 years

        • 106 to 107 years

        • 109 to 1011 years

        • 1012 to 1015 years

        1c2 marks

        Explain why the star remains stable during stage 3 for the length of time you selected in part (b).

        1d5 marks

        For stars with much larger masses than our Sun, stages 1 to 3 are almost exactly the same as lower mass stars. For the later stages, 4 and 5, the processes begin to differ. 

        Compare and contrast the final two stages in stars with much larger masses than our Sun and stars with similar masses to our Sun.

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        2a4 marks

        The table contains information on the mass of different stars.

        Star Name

        Star Mass / kg

        Earth's Sun

        1.989 × 1030

        Proxima Centauri

        2.446 × 1029

        VY Canis Majoris

        3.381 × 1031

         (i) Compare the masses of Proxima Centauri and VY Canis Majoris to the Sun.

        (ii) Explain how these differences will affect the time these stars can remain stable.

        2b5 marks

        Describe what will happen to each of the stars after they leave the main sequence stage.

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        3a2 marks

        A Hertzsprung‑Russell diagram shows how different astronomical objects may be classified according to their colour and absolute magnitude.

        8-2-3a-h-hr-diagram-colour-abs-maganitude-sq-igcse

        The diagram shows three stages of evolution for stars of similar mass to the Sun.

        (i) Add an S to the Hertzsprung-Russell diagram to show the position of the Sun.

        (ii) Star X has the same surface temperature as the Sun but would be brighter than the Sun if it were the same distance away from Earth as the Sun.

        Add an X to the Hertzsprung-Russell diagram to show the position of star X. 

        (iii) Star Y has a hotter surface temperature than the Sun but would be dimmer than the Sun if it were the same distance away from Earth as the Sun.

        Add a Y to the Hertzsprung-Russell diagram to show the position of star Y.

        3b6 marks

        Describe the evolution of stars of similar mass to the Sun.

        You should refer to the temperature and brightness of the stars in your answer.

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        4a6 marks

        An amateur astronomer is compiling a list of stars he can see through his telescope along with their temperature, colour, absolute magnitude and brightness relative to our Sun. 

        His observations so far are detailed in the table.

        Star

        Surface Temperature (K)

        Colour

        Absolute Magnitude

        Brightness relative to the Sun

        Betelgeuse

        3500

        red

        −5.9

        100 000

        Aldebaran

        3900

        orange

        −0.6

        400

        Sun

        5800

        yellow

        4.6

        1

        Canopus

        7400

        yellow-white

        −2.5

        14 000

        Vega

        9600

        white

        0.6

        40

        Rigel

        11 000

        blue-white

        −8.1

        120 000

        10 Lacertae

        36 000

        blue

        −4.4

        25 000

        Plot the data on a suitable graph using the grid below.

        8-2-4a-h-temp-abs-magnitude-gridlines-blank-sq-igcse
        4b5 marks

        Canopus has already passed through the red giant branch after exhausting all of the hydrogen in its core. The rest of the stars listed are either in their main sequence or red giant stages.

        (i) On your graph, identify the following regions:

        • Main sequence

        • Red giants

        • Red supergiants

        • Blue supergiants

        (ii) Draw an arrow on your graph to show the path Canopus is likely to take in its next evolutionary stage.

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        5a1 mark

        The editor of a science magazine is writing an article on the Hertzsprung-Russell diagram.

        All objects on a Hertzsprung-Russell diagram emit electromagnetic radiation. The editor is particularly interested in objects R and S, as shown in the diagram.

        8-2-5a-h-hr-diagram-temperature-luminosity-mcq-igcse

        Which of the following statements about object R and object S is correct?

        • R emits radiation with a higher mean frequency than S

        • R emits radiation with a longer mean wavelength than S

        • S and R both emit radiation with the same intensity

        • S emits radiation with a shorter mean wavelength than R

        5b2 marks

        Describe the relationship between the colours and values of temperature on the Hertzsprung-Russel diagram.

        5c2 marks

        The editor requires more information to complete the article. 

        (i) The Moon is the brightest object in the night sky.

        Suggest why the Moon cannot be shown on the Hertzsprung-Russell diagram.

        (ii) Suggest why black holes are not plotted on the Hertzsprung-Russell diagram..

        5d8 marks

        The editor plots the location of the Sun on the Hertzsprung-Russell diagram.

        8-2-5d-h-hr-diagram-temperature-luminosity-with-sun-sq-igcse

        He states that object R will eventually move to the same position as object S someday.

        (i) Comment on the validity of the editor's statement. 

        (ii) The editor wants to compare the evolutionary path of the Sun with the path of object R.

        Draw the evolutionary paths of the Sun and object R on the Hertzprung-Russell diagram.

        (iii) Explain the paths you have drawn in (ii).

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        6a2 marks

        An astronomer is collecting data for stars with a range of spectral classes and wants to plot a graph of spectral class against absolute magnitude to see if any patterns can be identified.

        The data the astronomer has collected is shown in the table below.

        Star

        Spectral Class

        Decimal Class

        Absolute Magnitude

        Sun

        G2

        5.2

        4.8

        Sirius B

        A2

        3.2

        11.2

        Proxima Centauri

        M6

         

        15.6

        61 Cygni

        K5

         

        7.5

        Betelgeuse

        M1

         

        −5.9

        Rigel

        B8

         

        −7.8

        Bellatrix

        B2

         

        −2.8

        Vega

        A0

         

        0.6

        Barnard's Star

        M4

         

        13.2

        Procyon B

        F5

         

        13

        Complete the data from the table using the conversion table below.

        Spectral Class

        Decimal Class

        O

        1 (e.g. 1.1 = O1)

        B

        2

        A

        3

        F

        4

        G

        5

        K

        6

        M

        7

        6b6 marks

        (i) On the grid below, plot a graph of absolute magnitude against star class using the data from the table in (a).

        (ii) On your graph, identify the following regions:

        • Main sequence

        • Red supergiants

        • Blue supergiants

        • White dwarfs 

        8-2-6b-h-hr-diagram-gridlines-blank-sq-igcse

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