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Gravity in the solar systemIB MYP Physics: Revision notes

Section 1

Gravitational force depends on mass and distance

Every object attracts every other object with a gravitational force. The force is:

  • larger when the masses are larger
  • smaller when the objects are further apart

The force falls off quickly with distance. If the distance is doubled, the force becomes one quarter of its original size. This is the inverse-square idea. The Sun's pull on Neptune is therefore far weaker than its pull on Earth.

Key termsgravitational forceinverse-square idea

Section 2

Gravity keeps things in orbit

An orbit is the curved path of one object around another. Gravity holds:

  • planets in orbit around the Sun
  • moons in orbit around planets
  • satellites in orbit around the Earth

Gravity acts towards the centre of the orbit, at right angles to the object's direction of motion. It does not change the speed, but it keeps changing the direction, so the object follows a curve instead of a straight line.

Key termsorbitsatellite
Common mistake

Satellites stay up because of gravity and their sideways speed, not because there is no gravity. Their engines are not needed to keep them moving.

Section 3

Orbital speed and orbital period

The orbital period is the time for one complete orbit. For objects orbiting the same body:

  • the closer the orbit, the faster the object moves and the shorter the period
  • the further away, the slower it moves and the longer the period, because the gravitational pull is weaker and the path is longer

Mercury orbits the Sun in 88 days, Earth in 365 days and Neptune in about 165 years. Satellites in low orbit, such as the ISS, take about 90 minutes.

Key termsorbital periodorbital speed
Exam tip

For average orbital speed use speed = distance ÷ time, with the distance as the length of the orbit (circumference).

Section 4

Free fall

An object is in free fall when gravity is the only force acting on it. It accelerates towards the centre of the planet.

An orbiting object is in free fall. It falls towards the Earth, but because it moves sideways at high speed, the Earth's surface curves away beneath it, so it keeps falling around the Earth without hitting it.

Key termsfree fall

Section 5

Weightlessness in orbit

Astronauts on the International Space Station seem to float, but gravity there is still about 90% of its value at the surface. They are not far enough away to escape it.

The astronauts and the station are in free fall together, so the floor does not push on the astronauts. They feel weightless, but their mass is unchanged and gravity still acts on them.

Key termsweightlessness

Must Know

  • Gravitational force increases with mass and decreases with distance (double the distance, one quarter the force)
  • Gravity keeps planets, moons and satellites in orbit
  • Closer orbits mean higher speed and shorter periods
  • Objects in orbit are in free fall
  • Astronauts feel weightless because they are in free fall, not because gravity has gone

That's the notes covered.

Carry on to the next subtopic.

Exam questions on Gravity in the solar system

  1. Astronomers in Chile compare the planets orbiting the Sun. Mercury is the closest planet to the Sun and Neptune is the furthest.
    Explain why Neptune takes much longer than Mercury to orbit the Sun.2 marks
  2. A communications satellite orbits the Earth in a circular path at a constant height. Its engines are switched off.
    Explain why the satellite does not move off in a straight line.2 marks
  3. A student collects data about four planets. Mercury is 58 million km from the Sun and has an orbital period of 88 days. Earth is 150 million km away with a period of 365 days. Mars is 228 million km away with a period of 687 days. Jupiter is 778 million km away with a period of 4333 days.
    Describe the trend in the data and calculate how many times longer Jupiter's orbital period is than Earth's.3 marks
See the full worksheet

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).