The Moon

A picture of the Moon taken by the Galileo spacecraft

The Galileo spacecraft took these images of the Moon on 7 December 1992 on its way to explore the Jupiter system in 1995-97. The distinct bright ray crater at the bottom of the image is the Tycho impact basin. The dark areas are lava rock filled impact basins: Oceanus Procellarum (on the left), Mare Imbrium (center left), Mare Serenitatis and Mare Tranquillitatis (center), and Mare Crisium (near the right edge).
Source: Courtesy NASA/JPL-Caltech.

Average Distance from the Earth: 384 400 km (0.0026 AU)

Size (Equatorial Diameter): 3475.6 km (0.272 x that of Earth)

Mass: 7.35 x 1022 kg (0.012 x that of Earth)

Rotation Period: 27.3 days

Temperature: 117°C (sunlit side), -163°C (far side)

Gravity: 1.7 m/s2 (0.17 x that of Earth)

We see the Moon in our northern sky and though it may appear large, especially when seen close to the horizon, our view of the Moon is actually small enough to be covered by your thumb.

The mass of the Earth and the Moon are similar when compared to the other planets in the solar system, so the Earth and Moon could be said to be companion planets. The Moon is thought to have formed when a rogue Mars-sized planet collided with the Earth 4.6 billion years ago.


The Moon is a rocky object and its surface consists of rock and dust, all of a uniform grey colour. The dark areas that dominate the near side are called maria, or 'seas', and were formed by lava flows about three billion years ago. The lunar surface is also covered with craters from impacts of meteorites, mostly very small (around 1mm) but occasionally much larger. The Clementine probe found evidence of water ice at the base of a permanently shadowed crater near the Moon's south pole, known as the South Pole-Aitken Basin.
Largest sea: Mare Imbrium (The Sea of Showers),
diameter 1300 km.
Largest crater: Bailly, diameter 295 km.
Deepest crater: Newton, depth 8.85 km.


The Moon has no atmosphere, so there is no erosion or weathering of surface features. The footprints left by the Apollo astronauts will still be clearly visible thousands of years from now.

Phases of the Moon

As the Moon orbits the Earth it appears to change shape as different parts of its illuminated face are visible from Earth. The four phases of the Moon are as follows:


A New Moon cannot be seen from the Earth. It is too close to the Sun in the sky and only the far side is facing us. 


At First Quarter we see half of the Moon. It rises around midday and sets around midnight.   


A Full Moon rises at Sunset and sets at Sunrise. We see the entire sunlit side.


At Last (or Third) Quarter we see half of the Moon. It rises about midnight and sets around midday.

The Lunar Month

A month is the time taken for the Moon to make one apparent orbit of the Earth, travelling at an average speed of 3680 km/h. It can be measured in the following three ways:

  • Synodic Month: 29.5 days
    This is the time between successive New Moons and is the basis for our calendar month.
  • Sidereal Month: 27.3 days
    This is the time taken for the Moon to return to the same spot against the background stars. It so happens that this is the same as the Moon's rotation period, which means that the same side of the Moon always faces the Earth.
  • Anomalistic Month: 27.55 days
    This is the time between successive perigees or closest approaches to the Earth.

Dates in Lunar Exploration

March 1840. First photograph of the Moon.
2 January, 1959. Luna 1 is the first probe to fly by the Moon.
13 September 1959. Luna 2 is the first probe to crash land on the Moon.
31 January 1966. Luna 9, is launched and is the first to soft-land on the lunar surface.
25 December 1968. Apollo 8 makes the first manned flight around the Moon.
20 July 1969. Apollo 11 makes the first manned landing.
21 July 1969. Neil Armstrong is the first person to walk on the Moon.
December 1972. Eugene Cernan, Apollo 17, is the last person on the surface (so far).
21 February 1994. The Clementine spacecraft goes into orbit around the Moon.

The Moon's Orbit

The Moon's orbit is tilted by 5° to the ecliptic, ie it gets to 5° North and 5° South of the ecliptic. Hence it is as much as 28.5° north or south of the Celestial Equator and as little as 18.5° North or South. This means the Moon can be higher or lower than the Sun. The points where it crosses the Ecliptic are called the Nodes. These points precess (move backwards) with time.

Against the background stars the Moon moves about its own width (0.5°) every hour or a little over 13° per day. The Sun travels 1° per day, so, with respect to the Sun, the Moon travels 12° per day. Each month it moves all the way around the sky and a little more. The Moon moves around the Earth about 13 times in one year.

The Sun is the main offender in disturbances of the Moon's orbit, its gravitational influence being twice that of the Earth on the Moon. The Moon is affected by 150 direct periodic variations and 500 smaller variations in its passage.

The Moon arrives approximately 50 minutes later per day on the meridian (between 38 and 66 minutes). The variations are due to changes in orbital speed, variations in the Sun's apparent speed along the ecliptic and changes in the inclination of the Moon's orbit.

Rising times of the Moon can vary from 13 minutes to 80 minutes on latitude. Greatest delay in rise is near Full Moon close to the Spring Equinox. Least delay in Moonrise is near the Autumn Equinox.

The Moon's distance from the Earth varies by about 5.49%. The Moon is slightly larger and moves faster when it is at perigee.

Due to the constant motion of the Moon about the Earth, Full Moon is only an instant. However, when we view the Moon it does appear full a few days before and after the exact time of the phase. Moon phases are between 6 or 7 days apart due in part to the Moon's elliptical orbit and that the Earth-Moon system is in orbit around the Sun.


The Moon shines only by reflected light. The albedo of the Moon is 0.07, which means it reflects only 7% of the light falling on it. (The albedo of the Earth is 0.39).

The Moon is at magnitude -12.7. The faintest stars seen by our eyes are magnitude 6, the brightest star is -1.58. The Moon is 33,000 times brighter than Sirius. It is also 14 magnitudes dimmer than the Sun, ie sends out approximately 400,000 times less light to us.

Our eyes adapt to light changes whereas cameras don't. Therefore as the sky gets dark it appears that the Moon is dazzling. In fact, it is only a dull grey colour. If we could surround the sky with full moons then the sky would still be only 1/4 as bright as one Sun in the sky even though the sky would be filled with 105,000 full moons. A full moon is 465,000 times fainter than a sunny day. The only reason why we are able to see features outside by moonlight is that the eye is amazingly adaptable. A sheet of white paper by moonlight is 2,000 times darker than black velvet in sunlight. Yet some people are able to read a book by moon light.

The surface brightness of the Moon is not uniform and hence a quarter phase Moon is not half as bright as a Full Moon. The Moon is a sphere, so more light is reflected back when the Moon's face is directly towards us. The Moon is brighter in the middle and greyer towards the terminators. The Moon's surface is covered with valleys and mountains that don't reflect much light back. A first quarter Moon is therefore about 1/10 the brightness of a Full Moon. Approximately 2.4 days before Full Moon results in a brightness that is half of a Full Moon.

Comments (23)

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Sofia 12 July, 2009 11:24
Thankyou for your help in my project. i found this info about the moon very useful. I hope that i will get to use it again soon
Rob Henderson 4 August, 2009 19:14
I am of the opinion that the DarkSide as mention above refers to the far side of the moon, that half that we never see. I think it should be changed to the shadow side.
Discovery Centre 5 August, 2009 13:05

Hi there Rob. Thanks for sharing your feedback with us. We will forward your comments to the Museum's Curator of Astronomy for her consideration.

Discovery Centre 6 August, 2009 11:14

Dear Rob - sorted! Our astronomer agrees that "far side" makes better sense than "dark side," since both sides of the moon experience times of light, dark and shadow. Thanks again for your feedback.

macee 17 November, 2009 05:17
Is it possible that there could be more planets in the Solar System than the ones we know about? Please answer, Thanks.
Discovery Centre 17 February, 2010 11:03

Hi Macee, thanks for your enquiry. There will not be any other designated Planets in our Solar System, but there will be other Dwarf Planets possibly found and designated.  At the moment we have 5 Dwarf Planets; Ceres (which was an asteroid), Pluto (which was reclassified from a Planet), Eris, Haumea, and Makemake.  With a current potential of up to 200 new Dwarf Planets. The International Astronomical Union (IAU) will decide which will be the next Dwarf Planet to be classified.

Alisha 8 February, 2010 16:47
Hi umm i found the website ufull. But can you put a picture of the moon on the 28th of april 2010?
Discovery Centre 9 February, 2010 14:21
Hi Alisha - You can find a list of moon phases for 2010 at our Planetarium site, on this page.
cara 18 May, 2010 11:08
this came so handy for my science project due the next day THNX!!!!!!!
Kevin 4 July, 2010 11:24
Great site thanks - and also a terrific display at the Planetarium. I read recently that the light we see reflected from the moon varies by up to 30% depending on the moons distance from the earth. If this is true, on what dates will the moon appear most brilliant this year? Thanks Kevin
Val 26 July, 2010 09:22
Thank you for your great information about the Moon. I have one question. Does the same side of the Moon face the Earth as it moves around the Earth? This would mean that it rotates on its axis approx every 27 days. Or does it not rotate at all?
Discovery Centre 27 July, 2010 12:34

Hi Val,

The Moon does rotate on its axis – it takes roughly a month for the Moon to orbit the Earth and a month to rotate on its axis – that’s why the same side of the Moon always faces the Earth. If the Moon didn’t rotate, then over one orbit of Earth we would see all of the Moon.

Ian 8 November, 2010 19:06
What are the moon phases for the rest of the year?
Discovery Centre 9 November, 2010 16:14
Hi Ian, you can find the Moon Phases at top right under 'Related Resources'.
matt 7 April, 2011 14:53
hey you replied to Val that it takes a month for the moon to rotate on its axis. I thought that for us to see the same side of the moon it should be 24 h... Am I wrong?
Discovery Centre 10 April, 2011 14:56

Hi Matt,

The Moon both rotates on its axis and revolves around the Earth in the space of a month - effectively its day and its month are the same length of time - this is why we see only one side of it from Earth. I found an animation on Youtube that might help to explain this a bit better.

Alec 7 May, 2014 01:29
thank you so much this helped a lot on my essay about the solar system
jack wagstaff 16 December, 2014 02:16
this website is great
Moi 19 October, 2015 14:39
How can the Earth's and Moon's masses be similar since they are not the same size ? Please answer
Discovery Centre 19 October, 2015 14:53
Hello Moi - we think you may have misread the information above - the masses of Earth and the Moon are quite different (the Moon has the mass of 0.012 of Earth, as stated above). The section that states that the Earth and Moon have similar masses that you quoted is taken out of context, it relates the masses of Earth and the Moon having similar masses compared to the masses of other planets in the Solar System; for example Saturn (100x the mass of Earth) or Jupiter (more than 300 x the mass of Earth), etc.
Moi 20 October, 2015 02:28
Ho! Thank you for your explaination, it makes a lot more sense now !!! By the way, this website is a really good source of information and I use it all the time.
Casey 4 October, 2016 18:28
When will the 2018 Moon phase data be available?
Discovery Centre 14 March, 2017 15:26
Hi Casey, apologies for missing your comment. You can find this information via the timeanddate website; see the links in our Skynotes page.    



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