Motion in the Universe Notes
Edexcel IGCSE Physics: Revision notes
Key facts
- The universe contains billions of galaxies; a galaxy holds billions of stars; our Sun is in the Milky Way.
- Gravitational field strength depends on the mass of the body and the distance from its centre.
- Gravity provides the force that keeps moons, planets, satellites and comets in orbit.
- Planet and moon orbits are nearly circular; comet orbits are highly elliptical.
- Orbital speed .
The universe and galaxies
The universe is billions of galaxies. Each galaxy is billions of stars held together by gravity, and our Sun is in the Milky Way.
A galaxy is a huge collection of billions of stars held together by gravity.
Our Sun and Solar System are in the Milky Way galaxy, which is one of billions of galaxies in the universe.
- 1
Universe
billions of galaxies
- 2
Galaxy
billions of stars, held together by gravity
- 3
Milky Way
our galaxy, containing the Sun and Solar System
What holds the stars of a galaxy together?
Gravitational field strength
Gravitational field strength is the force of gravity per unit mass. It is bigger for a more massive body and smaller at greater distance from its centre.
Gravitational field strength differs from place to place. The Moon has much less mass than Earth, so its is smaller.
Weight changes with , but mass stays the same everywhere.
Worked example
Find the weight of a 60 kg astronaut on the Moon ( N/kg).
- 1
.
- 2
.
Why is g smaller on the Moon?
What keeps things in orbit
Gravity pulls an orbiting body towards the central mass. Without it, the body would travel in a straight line.
Gravitational force provides the centripetal force that keeps an object on a curved path. It makes moons orbit planets, planets orbit the Sun, satellites orbit Earth and comets orbit the Sun.
Its velocity is along the tangent, while the force points to the centre.
Moons orbit
- Planets
Planets orbit
- The Sun
Satellites orbit
- Earth
Comets orbit
- The Sun
If gravity suddenly switched off, a planet would
Shapes of orbits
Planets and moons follow nearly circular orbits. Comets follow highly elliptical orbits, so their distance and speed change a lot.
A comet comes very close to the Sun at one point and travels far away at another.
Its distance from the Sun, and so its orbital speed, varies hugely in one orbit. A planet's speed is roughly steady.
Planets
- Nearly circular
- Roughly constant distance
Moons
- Nearly circular
- Orbit their planet
Comets
- Highly elliptical
- Very close, then very far
Which body has a highly elliptical orbit?
Orbital speed
In a circular orbit, speed is the circumference divided by the time for one orbit.
In one orbit, a body travels the circumference, , in one time period . Average speed is distance divided by time.
is the orbital radius and is the orbital speed.
- Orbital speed
Worked example
A satellite orbits at a radius of m with a time period of 6000 s. Find its orbital speed.
- 1
.
- 2
.
The orbital radius doubles but the period stays the same. The speed
Try an exam question
A satellite is in a circular orbit around the Earth. The orbital radius is m and the time period is 6000 s. State what provides the force that keeps the satellite in orbit and calculate its orbital speed.
[4 marks]
- [1]The force of gravity (gravitational attraction to the Earth) keeps it in orbit.
- [1].
- [1].
- [1] m/s.
That's the notes covered.
Carry on to the next subtopic.