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Astronomy

How ideas about the Solar System and ways of observing it have changed

  • 3 things to know
  • Paper 1

Overview

The geocentric and heliocentric models, telescope evidence from Jupiter's moons and the phases of Venus, elliptical orbits, why models change, and observing by naked eye, telescope, photography and digital detectors, including radio, X-ray and orbiting telescopes.

What you need to know

Answer each one before you reveal it.

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Key term

Which model of the Solar System is accepted today?

Key term

Give one early telescope observation that supported the Sun-centred model of the Solar System.

Key term

State a telescope observation of Venus that supported the Sun-centred model of the Solar System.

Questions from this subtopic

Each one with the model answer underneath.

  1. 1

    Describe the geocentric model of the Solar System.

    Model answer

    In the geocentric model the Earth sits at the centre and the Sun, Moon, planets and stars all move around the Earth in circles.

  2. 2

    Describe the heliocentric model of the Solar System.

    Model answer

    In the heliocentric model the Sun sits at the centre and the Earth and the other planets orbit around it.

  3. 3

    Which model of the Solar System is accepted today?

    Model answer

    The heliocentric model, with the Sun at the centre and the planets orbiting it.

  4. 4

    Give one early telescope observation that supported the Sun-centred model of the Solar System.

    Model answer

    Four moons were seen orbiting Jupiter, which showed that not everything in the sky moves around the Earth.

  5. 5

    State a telescope observation of Venus that supported the Sun-centred model of the Solar System.

    Model answer

    Venus was seen to go through a full set of phases, which can only happen if Venus orbits the Sun.

  6. 6

    How were the shapes of the planets' paths corrected after the first Sun-centred model was proposed?

    Model answer

    Perfectly circular paths were replaced by slightly elliptical orbits, which matched the observed positions of the planets far better.

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