The Moon may appear to change shape, but in fact the bright surface you see and the ‘moonlight’ that reaches Earth is actually sunlight reflecting off the lunar surface. As the Moon orbits our planet, its varying position means that the Sun lights up different regions, creating the illusion that the Moon is changing shape over time.
The best way of getting to understand the lunar phases is to regularly go out on a clear night when the Moon is in the sky and observe it.
On average 384,400km from Earth, it’s stunning to the naked eye and through binoculars or a small telescope, spectacular. It’s also a great target to photograph. For more on this, read our guide on how to photograph the Moon.
The Moon seems serene but it is hurtling eastward travelling at 3,682 km/h and, since its almost circular orbit is tipped a mere 5° relative to Earth’s, it more or less follows the ecliptic (the Sun’s apparent path) across the sky.
You may have noticed that the Moon always keeps the same face turned towards us. This is because it rotates once on its axis in exactly the same time it takes to orbit Earth – 27 days and seven hours.
This synchronisation is called tidal locking and is a result of Earth’s gravitational effect on the young Moon when it was forming.
During its elliptical journey around Earth, the Moon moves through ‘phases’, the term we use to describe how much of the lunar disc appears illuminated as seen from Earth.
In fact, the Moon is always half lit, we just don’t see it that way. Whatever phase we’re seeing, the opposite phase is happening on the far side.
And while we only ever see one terminator (the name given to the dividing line between the light and dark parts of the lunar surface) sweeping right to left across the lunar disc at any time, there are actually two of them circumnavigating the Moon exactly 180° apart; the morning terminator (which ushers in the lunar day) and the evening terminator (which brings the night behind it).
So sorry, Pink Floyd, there is no permanently dark side of the Moon.
The phases of the Moon
What many people don’t realise (even though it’s completely logical), is that there’s also a relationship between the Moon’s phases and moonrise times.
In this phase, our satellite is invisible. With the Sun and Moon on the same side of Earth, they rise together but we cannot see the Moon as it’s hidden in the Sun’s glare. There’s not much to see anyway, as its face towards us is totally in shadow.
Continuing its journey, the Moon’s western (right) edge becomes sunlit to create a sliver-thin crescent. The morning terminator starts its creep of 15.5km/h from west to east.
This one confuses non-astronomers, because it clearly looks like half a Moon, yet it’s called a quarter Moon. That’s because the terminator has completed a quarter (90°) of its 360° journey around the Moon.
By this logic a full Moon should be called a half Moon, but that’s just silly, right? In this phase, the Moon rises at noon and sets at midnight. Along the terminator, low-angled sunlight creates long shadows, throwing nearby crater and mountains into sharp relief – perfect for lunar observations.
In this phase the Moon is almost fully illuminated. The daylight area appears egg-shaped (gibbous) and is increasing in size (waxing) daily.
Halfway through the morning terminator’s journey, the Moon is on the opposite side of Earth from the Sun, with its near side fully illuminated and dazzling. Shadow-less, bleached and flat-looking, it’s not good for observation – that’s a shame because in this phase it rises as the Sun sets, sets as the Sun rises and is visible all night long!
The Moon’s western edge is being consumed by darkness as the evening terminator comes into view. The sunlit, egg-shaped area is diminishing (waning).
It’s seven days and nine hours since full Moon and, now 90° west of the Sun, just the Moon’s eastern (left) half is illuminated. At this phase it rises at midnight and sets at noon and, like the first quarter phase, offers staggering views.
With just the eastern edge sunlit you’ll admire a beautiful ‘C-shaped’ crescent. Diminishing daily (waning) it will soon disappear as the lunar cycle concludes and the Moon returns to ‘new’. While the Moon may keep the same face turned to us, it remains a daily changing delight to observe.
Over the course of a lunar cycle, the Moon simultaneously wobbles both latitudinally and longitudinally. These oscillations are known as librations.
Libration in latitude – nodding – occurs because the Moon’s axis is slightly inclined relative to Earth’s, enabling us to peer just a little over its north and, later in the month, south poles.
Libration of longitude – shaking – occurs because the Moon travels fastest when closest to Earth and slowest when farthest away.
Daily (diurnal) libration occurs because of our planet’s rotation.
We see the Moon from slightly different perspectives when it rises and when it sets, and this difference in perspective manifests as a slight apparent rotation in the satellite, first to the west and then to the east.
The combined effect of all the above means that instead of seeing just 50 per cent of the Moon, over time we actually get to see about 59 per cent.
Jane Green is a fellow of the Royal Astronomical Society and author of the Haynes Astronomy Manual