Stars & The Universe (Cambridge (CIE) IGCSE Physics)

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  • What two elements is the Sun mostly composed of?

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  • What two elements is the Sun mostly composed of?

    The two elements the Sun is mostly composed of are hydrogen and helium.

  • True or False?

    The Sun is a planet which makes up over 99% of the mass of the Solar System.

    False.

    The Sun is a star which makes up over 99% of the mass of the Solar System.

  • Name the main types of radiation emitted by the Sun.

    The main types of radiation emitted by the Sun are in the infrared, visible and ultraviolet regions of the electromagnetic spectrum.

  • What is nuclear fusion? (Extended Tier Only)

    Nuclear fusion is the joining of two smaller nuclei to form one larger nucleus, releasing a large amount of energy in the process.

  • Where do nuclear reactions take place in stars? (Extended Tier Only)

    Nuclear reactions take place in the centres (cores) of stars.

  • How is the Sun powered? (Extended Tier Only)

    The Sun is powered by the nuclear fusion of hydrogen into helium.

  • What is the Milky Way?

    The Milky Way is a galaxy containing billions of stars, including our Sun.

  • What is the difference between a galaxy and the Universe?

    A galaxy is a large collection of stars, whereas the Universe is made up of billions of galaxies.

  • Define a light-year.

    A light-year is the distance travelled by light in one year.

  • What is the diameter of the Milky Way in light years?

    The diameter of the Milky Way is 100 000 light years.

  • How many metres are there in one light-year? (Extended Tier Only)

    There are 9.5 × 1015 m in one light-year.

  • True or False?

    All stars form from a cloud of dust and gas which becomes a protostar and then a stable star. (Extended Tier Only)

    True.

    All stars follow the same initial stages in their life-cycle:

    1. Nebula (cloud of dust and gas)

    2. Protostar

    3. Stable star

    The stages that follow depend on the mass of the stable star that forms.

  • When does a protostar become a stable star? (Extended Tier Only)

    A protostar becomes a stable star when nuclear fusion reactions are initiated in its core and the inward force of gravity is balanced by the outward pressure from the fusion reactions.

  • What forces, including their direction, act when a star is in a stable state? (Extended Tier Only)

    The forces acting on a star in a stable state are:

    1. Inward gravitational force

    2. Outward pressure due to energy released by fusion

  • True or False?

    Nuclear fusion provides the pressure that prevents stars from collapsing under gravity. (Extended Tier Only)

    True.

    The thermal pressure provided by nuclear fusion reactions prevents stars from collapsing under gravity.

  • Name the stages, in the correct order, in the life cycle of a star similar to the Sun. (Extended Tier Only)

    The stages, in the correct order, in the life cycle of a star similar to the Sun are:

    1. Nebula (cloud of dust and gas)

    2. Protostar

    3. Stable star

    4. Red giant

    5. Planetary nebula

    6. White dwarf

    7. Black dwarf

  • When does a stable star turn into a red giant? (Extended Tier Only)

    A stable star turns into a red giant when hydrogen in the star's core begins to run out and the star begins to fuse helium into heavier elements.

  • True or False?

    A high mass star will eventually explode as a supernova and become a white dwarf. (Extended Tier Only)

    False.

    A high mass star will eventually explode as a supernova and become a neutron star or a black hole.

  • What is the Doppler effect?

    The Doppler effect is the change in wavelength or frequency of a wave due to the relative motion between the source and the observer.

  • True or False?

    The Doppler effect applies to sound waves only.

    False.

    The Doppler effect applies to both sound waves and light waves.

  • True or False?

    Waves emitted by a stationary object have a constant wavelength.

    True.

    When an object emits waves, the wavefronts spread out symmetrically.

    This means the wavelength of the waves is constant.

  • True or False?

    The frequency of a wave emitted by a moving object increases if the object is moving away from an observer.

    False.

    If an object moves away from an observer, the waves spread out, so the wavelength increases and the frequency decreases.

  • What is redshift?

    Redshift is the increase in the observed wavelength of a light source when it moves away from an observer.

  • What is blueshift?

    Blueshift is the decrease in the observed wavelength of a light source when it moves towards an observer.

  • Which end of the light spectrum has a higher frequency, red or blue?

    The blue end of the light spectrum has a higher frequency.

  • How can astronomers determine if the light from a distant galaxy is redshifted?

    Astronomers can determine if the light from a distant galaxy is redshifted by:

    • Comparing the light spectra of a distant galaxy and an object on Earth (or close to Earth, such as the Sun)

    • If the lines from the distant galaxy appear closer to the red end of the spectrum, then the light has been redshifted

  • True or False?

    The greater the distance to a galaxy, the greater the redshift observed.

    True.

    The greater the distance to a galaxy, the greater the redshift observed, indicating that the galaxy is moving away faster.

  • What is the Big Bang theory?

    The Big Bang theory states the Universe originated from a very small region that was extremely hot and dense, which has been expanding and cooling for approximately 13.8 billion years.

  • True or False?

    The Big Bang theory states that the Universe began from a single point.

    True.

    According to the Big Bang theory, the Universe began from a very small region that was extremely hot and dense.

  • True or False?

    The Universe is currently contracting.

    False.

    The Universe is currently expanding, as evidenced by the redshift of distant galaxies.

  • What does the observation of redshift from distant galaxies imply about the Universe?

    The observation of redshift from distant galaxies implies that the Universe is expanding.

  • How does galactic redshift provide evidence for the Big Bang theory?

    Galactic redshift refers to the observation that light from distant galaxies is shifted toward longer, redder wavelengths.

    This indicates that distant galaxies are moving away from Earth.

    This provides evidence that the Universe must be expanding, which means that galaxies must have been closer together in the past.

  • What are the two main pieces of evidence for the Big Bang theory? (Extended Tier Only)

    The main evidence for the Big Bang theory comes from:

    1. Galactic redshift

    2. Cosmic microwave background radiation (CMBR)

  • What is cosmic microwave background radiation (CMBR)? (Extended Tier Only)

    CMBR is a type of electromagnetic radiation with a wavelength in the microwave region. It is observed to be very uniform at all points in space.

  • What is the origin of CMBR? (Extended Tier Only)

    The CMBR was originally emitted at the time of the Big Bang when the Universe was formed.

  • How does CMBR provide evidence for the Big Bang theory? (Extended Tier Only)

    CMBR provides evidence for the Big Bang Theory because it represents remnant radiation from the Big Bang which has been redshifted to the microwave region of the electromagnetic spectrum.

  • True or False?

    CMBR is completely uniform in temperature. (Extended Tier Only)

    True.

    CMBR has minuscule temperature fluctuations on the order of 0.00001 K, implying that objects in the Universe are uniformly spread out.

  • How can the distance to a galaxy be estimated? (Extended Tier Only)

    The distance to a galaxy can be estimated from the brightness measurements of a standard candle (an object of known brightness) called a supernova in the galaxy being observed.

  • Define Hubble's Law. (Extended Tier Only)

    Hubble's Law states that the speed of recession of a galaxy is directly proportional to its distance from Earth.

  • Define the Hubble Constant. (Extended Tier Only)

    The Hubble constant (H0) is the ratio of the speed of recession of a galaxy to its distance from the Earth.

  • Express Hubble's Law as an equation. (Extended Tier Only)

    Hubble's Law can be expressed as the equation v space equals space H subscript 0 d

    Where:

    • v = the speed of recession of the galaxy, measured in km/s

    • H subscript 0 = the Hubble constant (2.2 × 10–18 per second)

    • d = the distance to the galaxy, measured in km

  • What is the currently accepted value of the Hubble constant? (Extended Tier Only)

    The currently accepted value of the Hubble constant (H0) is 2.2 × 10–18 per second.

  • True or False?

    The further away a galaxy is, the faster it is moving away from us. (Extended Tier Only)

    True.

    Hubble's Law shows that the further away a galaxy is from Earth, the faster it is moving away from us.

  • What does 1 over H subscript 0 represent? (Extended Tier Only)

    The term 1 over H subscript 0 represents the age of the Universe, or the amount of time the Universe has been expanding.

  • True or False?

    According to Hubble's Law, if Galaxy A is twice as far away as Galaxy B, then Galaxy B must be moving away from Earth at twice the speed of Galaxy A. (Extended Tier Only)

    False.

    Hubble's Law states that the distance to a galaxy open parentheses d close parentheses and the speed it moves away from Earth open parentheses v close parentheses are directly proportional to each other.

    Therefore, if Galaxy A is twice as far away as Galaxy B, Galaxy A must be moving away at twice the speed of Galaxy B.

  • What is the estimated age of the Universe based on Hubble's Law? (Extended Tier Only)

    The estimated age of the Universe based on Hubble's Law is about 13.7 billion years.

  • How can the age of the Universe be determined from a graph of recessional velocity against distance? (Extended Tier Only)

    The age of the Universe can be determined from a graph of recessional velocity against distance because it is equal to the gradient of the graph.