Natural satellites
A satellite is anything that orbits around a larger object. A natural satellite is any celestial body in space that orbits around a larger body. Moons are called natural satellites because they orbit planets.
What are satellites?
Dr Allan McInnes tells us what a satellite is, how they vary in size and, depending on their function, the type of orbit they are placed into.
Point of interest: The small, university satellites Allan mentions are known as CubeSats – small 10 cm cubes.
Nature of science
In this video, Allan talks about small satellites – or CubeSats – he say's, "they tend to be university satellites". Science and technology are always advancing and while this was true when we interviewed Allan in 2013, small satellites are now also being employed by a number of organisations. NASA has an article where you can learn more about small satellites .
Satellites that are made by people and launched into orbit using rockets are called artificial satellites. There are thousands of artificial satellites orbiting the Earth.
The Moon
Any large object that orbits around a planet is called a moon (small ‘m’). The Earth has one moon called the Moon (capital ‘M’). The Moon takes 27.3 days to orbit the Earth once, moving at an orbital speed of 1 km/s.
Find out more about our Moon here.
Moons around other planets
Galileo was the first person to discover that other planets can have moons. He saw that Jupiter had four moons with his newly invented telescope in 1610 AD. At first, he thought they were stars, but he noticed that, each night, the four points of light appeared to change positions slightly. He realised they were actually moons orbiting around Jupiter. Another astronomer of the time, Simon Marius, named them Io, Europa, Ganymede and Callisto after the lovers of Zeus, the ancient Greek mythological King of the Gods and Men. We now know that Jupiter has at least 64 moons.
Jupiter’s largest moons
Galileo discovered Jupiter’s largest moons in 1610. Another astronomer of the time, Simon Marius, named them Io, Europa, Ganymede and Callisto after the lovers of Zeus, the ancient Greek mythological King of the Gods and Men. Currently Jupiter has 53 named moons and another 26 awaiting official names. Combined, scientists now think Jupiter has 79 moons.
Image courtesy of NASA.
All except two of the planets (Venus and Mercury) in our Solar System have natural satellites called moons.
Other natural satellites in our Solar System
Planets, asteroids and comets orbit around stars such as our Sun and so can also be thought of as natural satellites. Our Solar System has eight official planets as well as millions of minor planets, asteroids, comets and other objects orbiting around the Sun. All of these can be thought of as natural satellites.
All of these natural satellites are held in orbit by the attraction of gravity between the satellite and the object it is orbiting.
Natural satellite satellite
Satellite of
Orbital speed (average)
Time for one orbit orbit
Orbital radius (average)
The Moon
Earth
1.0 km/s
27.3 days
384,000 km
Io
Jupiter
17.33 km/s
1.77 days
421,700 km
Europa
Jupiter
13.74 km/s
3.55 days
670,900 km
Ganymede
(Solar System’s largest moon)
Jupiter
10.88 km/s
7.16 days
1.07 million km
Callisto
Jupiter
8.20 km/s
16.69 days
1.88 million km
Phobos
Mars
2.14 km/s
0.32 days
9,400 km
Ceres
(largest asteroid
Sun
17.88 km/s
4.6 years
4.14 million km
Halley’s Comet
Sun
Aphelion ~1 km/s
Perihelion ~71 km/s
75–76 years
(next seen in 2061)
At perihelion – 90,000 km
At aphelion – 5.25 million km
Earth
Sun
29.8 km/s
365.26 days
149.6 million km
Jupiter
Sun
13.0 km/s
11.9 years
778.55 million km
Venus
Sun
35.0 km/s
224.7 days
108.21 million km
For elliptical orbits, perihelion means closest orbital approach to the Sun, and aphelion means furthest orbital distance from the Sun.
Earth’s natural satellite: the Moon
The Moon orbits the Earth once every 27.3 days. This time period is called the orbital period or sidereal period. However, the time from one full moon to the next is 29.5 days (called the synodic period). This extra time is because of the change in angle as the Earth revolves around the Sun.
Moon months
The diagram is an explanation of the moon’s sidereal and synodic months. One full orbit of the Earth takes 27.32 days – the sidereal month. From one full moon to the next takes 29.53 days – the synodic month.
The Moon appears to move across the sky from east to west, in the same direction as the Sun moves. However, this motion is apparent and not true. The Moon is in fact orbiting the Earth in a west to east direction. The reason that it appears to rise in the east and set in the west is because of the Earth’s very fast axial rotation. The Earth rotates once each day, and the Moon orbits the Earth once every 27.3 days. This means that the Moon’s true orbital motion around the Earth can be seen only indirectly. The distance moved by the Moon in 1 day can be observed by comparing its position in the sky at one time with its new position exactly 24 hours later.
Apparent motion of the Moon
The apparent motion of the Moon from night to night. Each night, it moves around 13° to the east, which is approximately 26 Moon diameters.
Nature of science
Galileo was able to view only four of Jupiter’s 64 moons. He was limited by the quality and power of the telescopes available to him at the time. Nowadays with far more powerful and high-quality telescopes, we can see further and with more detail. Gains in scientific knowledge and understanding are often connected to technological advances in the equipment used to aid our powers of observation.
Related content
Since the earliest times, humans have made observations of the night sky. These observations led to the development of models to explain the movement of these natural satellites. Explore this further in Our solar system – revolutionary ideas.
Comets are natural satellites and scientists want to discover more about them. Find out about some of this work in To catch a comet – the Rosetta Mission.
Activity ideas
These student activities include a mix of hands-on and literacy-based investigations.
Gravity and satellites: true or false? – this is a useful pretest to establish student understanding
Observing natural satellites – get your students to turn their eyes to the night sky and practice their observation skills
Spotting satellites – can your students spot artificial satellites – like the ISS – as they pass overhead?
Useful links
Learn more about the Moon from NASA.
Explore these natural satellites further on NASA's SpacePlace website: Moon and Comets.