How to photograph the Moon with any camera

The Moon is the most photographed astronomical object on Earth, and also one of the most consistently overexposed. Most beginner Moon photos come out as a featureless white circle in a black sky — because the camera, seeing a mostly dark frame, assumes it needs to expose for the darkness and blows the Moon out. But the Moon is lit by the same Sun that lights the daytime Earth. It is, quite literally, a daytime subject. Treat it as one and your Moon shots suddenly show craters, mare, and the delicate ray systems of Tycho and Copernicus.

This guide covers the exposure basics, the equipment trade-offs, why phase matters more than magnification, and how to compose a Moon shot that isn't just another close-up of a rock.

The rule is called Looney 11: ISO 100, f/11, and shutter speed 1/100 s. Or equivalently ISO 200, f/11, 1/200 s. Or ISO 100, f/8, 1/200 s. Start there and adjust half a stop either way based on your camera's histogram — you want the Moon's bright limb close to but not touching the right edge of the histogram, with plenty of contrast in the mid-tones.

The main reason to shoot manual: the camera's meter will always try to average out the black sky. Any auto or aperture-priority setting will overexpose the Moon by three to five stops. Switch to full manual, dial in Looney 11, take one frame, check the histogram, adjust.

If you're shooting near full Moon, the Moon is even brighter — reduce exposure by one stop. If you're shooting a thin crescent, the Earthshine on the unlit side is far dimmer than the sunlit crescent, and you can't capture both in a single exposure without HDR blending. Choose one.

The Moon's apparent size in your image is a direct function of your focal length (in 35mm equivalent):

At 24mm the Moon is a pinpoint in a landscape — good for compositions with a horizon.

At 100mm the Moon is a small but recognisable disc — good for including a foreground.

At 300mm the Moon fills a meaningful chunk of the frame — the standard telephoto Moon shot.

At 600mm and beyond, the Moon starts filling more than a third of the frame vertically — you get real crater detail.

Modern phones with 5× or 10× optical zoom (typically 120mm–240mm equivalent) can produce respectable Moon shots. Any DSLR or mirrorless camera with a 200–300mm lens will do well. To really see Copernicus and Tycho's ray systems, you want a 500–800mm lens or a small telescope with a T-adapter. Anything longer than 300mm should be on a tripod — Moon photography is often ruined by camera shake at long focal lengths.

What you want is the Moon a couple of days either side of first or last quarter, when the Sun is grazing the lunar surface at a low angle and every feature casts a long, dramatic shadow. The line between light and shadow — the terminator — is where all the interesting texture lives. Craters look like real craters; mountain ranges throw shadows across the plains; the whole surface looks three-dimensional.

If you have to pick one phase to shoot, pick two days after first quarter (evening sky, sets around midnight) or two days after last quarter (morning sky, rises around midnight). At those phases the terminator crosses the most photogenic features on the Moon: the Apollo landing sites, the mare Serenitatis and Tranquillitatis, and the crater fields around the lunar south pole.

For serious detail work, astrophotographers use "lucky imaging": shoot 100+ frames as a video, throw away the ones blurred by atmospheric turbulence, and stack the sharpest 10% in software like Autostakkert. Free tools like PIPP and RegiStax will process the stack. The improvement is dramatic — a stacked image from a modest telescope can rival a single-frame image from a much larger one.

The trick with this kind of shot is compression. Use a long lens (200–400mm) from far away, and align yourself so the Moon appears directly behind your foreground subject at the moment it rises or sets. The Moon will appear enormous relative to the foreground because of telephoto compression — the same effect that makes distant mountains look like they're right on top of each other from a far-away vantage point.

Planning matters. Apps like PhotoPills or The Photographer's Ephemeris will tell you where the Moon will rise or set on any date. For a "Moon behind the mountain" shot, you often have a five-minute window on the right date at the right vantage point. It's worth scouting.

The Moon rises 50 minutes later each day on average, so the same rise position moves through the day-night cycle over the month. If you want the Moon rising at sunset (the classic "big orange Moon behind the horizon" shot), that's the full Moon. If you want a crescent Moon rising in daylight, that's the last quarter. Match the phase to the composition you want.

Rapidly changing conditions matter too. Even on "clear" nights, thin cirrus cloud can dramatically soften Moon detail. Take multiple frames over the course of an hour and pick the sharpest — atmospheric seeing changes minute to minute, and one frame in ten will often be noticeably better than the rest.

The Moon is the easiest astrophoto to attempt and one of the most rewarding to master. You don't need a dark site, a telescope, or a tracking mount. You need a lens, a tripod, manual mode, and the discipline to expose for daylight instead of night.