The Moon is bright enough to fool a camera meter and distant enough to expose every weakness in your technique. The top moon photography settings are not a single preset: they are a controlled starting point built around the Moon’s phase, your focal length, and the amount of atmosphere between you and the lunar surface. Start here, then adjust from your histogram rather than trusting the preview alone.
| Moon phase / scene | Starting exposure | ISO | Aperture | Best use |
|---|---|---|---|---|
| Full Moon | 1/250 to 1/500 second | ISO 100 | f/8 to f/11 | Bright lunar disk, minimal clipping |
| First or last quarter | 1/125 to 1/250 second | ISO 100 to 200 | f/8 to f/11 | Craters and mountain shadows |
| Thin crescent | 1/30 to 1/125 second | ISO 200 to 800 | f/5.6 to f/8 | Slim lit arc and earthshine |
| Moon plus landscape | Bracket 1/250 second to 4 seconds | ISO 100 to 400 | f/5.6 to f/8 | Composite or blended exposure |
Why the Moon needs daylight-style exposure
A full Moon looks like a night-sky object, but its sunlit surface is roughly as bright as a sunlit landscape. That is why an automatic mode often gives you a white, featureless circle. Your camera sees a mostly black frame and tries to brighten it. The Moon does not need that help.
Use Manual mode, spot-meter the Moon if your camera offers it, and begin at ISO 100, f/11, and 1/250 second. This is a practical variation of the classic lunar exposure rule. Check the histogram after every short test burst. Keep the brightest data close to the right side without piling hard against it. Highlight warnings are useful here: flashing regions on the Moon usually mean crater detail has already been lost.
The Moon travels eastward against the background stars by about 13 degrees per day, or roughly 0.5 degrees per hour. Its apparent disk is only about 0.5 degrees wide. At long focal lengths, that motion and Earth’s rotation become visible quickly, so a fast shutter is insurance against softness even on a tripod.
Top moon photography settings by camera and lens
Your lens determines how large the Moon appears in the frame. A 200 mm lens on a full-frame camera makes a satisfying small disk in a wider scene. Around 400 mm begins to reveal major maria and stronger crater structure. At 600 mm or more, atmospheric turbulence can become the limiting factor, not the resolution of the camera.
DSLR and mirrorless cameras
Shoot RAW, use single-point autofocus on the lunar edge or a high-contrast crater boundary, then inspect at 100 percent magnification. If autofocus hunts, switch to manual focus with magnified live view. Focus on the sharp transition between the bright lunar surface and black sky, not on the soft glow around it.
For a full or nearly full Moon, use ISO 100, f/8, and 1/320 second as a mission-ready baseline. Open to f/5.6 only when your lens is visibly sharper there or when haze forces a faster capture sequence. Avoid very small apertures such as f/16 unless you need them for a landscape, because diffraction can soften fine detail.
Turn off image stabilization when the camera is firmly mounted on a tripod if your lens manual recommends it. Use a 2-second self-timer, remote release, or phone app to prevent vibration. Electronic first-curtain shutter or a fully electronic shutter can also help, though some cameras may show rolling-shutter artifacts with fast movement or flickering artificial light in a foreground scene.
Phones and compact cameras
A phone’s telephoto camera can record a clean Moon, especially at 3x to 5x optical zoom. The weakness is digital zoom. It enlarges pixels rather than adding lunar information, so stop near the camera’s true optical focal length whenever possible.
In a manual or Pro mode, set ISO 25 to 100, exposure compensation between -1 and -2 EV, and the fastest available shutter speed. Tap and hold to lock focus and exposure on the Moon. If the image still looks like a glowing dot, reduce exposure further. A small tripod and a 3-second timer matter more than most phone accessories.
Pick the phase that matches the photo
A full Moon is dramatic near the horizon and ideal for recognizable lunar silhouettes, but it is not usually the best phase for surface texture. With sunlight coming almost straight down, many craters look flatter. The first-quarter and last-quarter phases produce stronger shadows along the terminator, the moving line between lunar day and night. That is where ridges, crater rims, and mountain chains gain depth.
Plan your target by altitude as well as phase. The Moon is typically sharper at 45 degrees altitude than at 10 degrees because you are shooting through much less turbulent, moisture-heavy atmosphere. The popular oversized Moon at the horizon is an optical illusion. It is not physically larger there, and it is often distorted by haze.
For a foreground composition, low altitude can still be the right creative decision. Use a planning tool to identify when the Moon will be between 5 and 15 degrees above your chosen skyline, then arrive 20 to 30 minutes early. The exact rise time varies by location and shifts by roughly 50 minutes later each day, so use location-specific data rather than a national time listing.
Beat the atmosphere before chasing more magnification
The Earth-Moon distance changes throughout the month from about 356,500 km at perigee to about 406,700 km at apogee. That changes the apparent lunar diameter by roughly 14 percent. It is real, but it is less decisive than stable air, accurate focus, and avoiding excessive digital zoom.
Look for nights after a cold front, when the air is often drier and steadier. Avoid shooting across rooftops, parking lots, or sun-warmed pavement. Those surfaces release heat that ripples the image. If the Moon looks like it is shimmering in live view at 600 mm, take many frames rather than endlessly refocusing. Atmospheric seeing changes from second to second.
For detailed lunar work, capture 20 to 100 images with identical settings, then select the sharpest frame or stack them in dedicated software. This is especially valuable when the Moon is below 30 degrees altitude. Do not mistake stacking for a cure-all: blown highlights and missed focus cannot be repaired afterward.
Build a reliable lunar shooting sequence
Start with a clear objective. If you want crater detail, prioritize a quarter Moon, a focal length of 300 mm or longer, and an altitude above 30 degrees. If you want a Moonrise behind a landmark, prioritize position, foreground distance, and the narrow time window near the horizon.
Take three test exposures one stop apart. For example, from a 1/250-second base exposure, record 1/125, 1/250, and 1/500 second. Review sharpness, not just brightness. At 400 mm and beyond, a slightly darker but sharper file is usually the better source image because lunar highlights are easy to lift only up to a point.
Then keep tracking the conditions. The Moon’s brightness changes with phase, cloud thickness, and altitude. A thin veil of cloud may require one or two stops more exposure, while a clear full Moon can handle 1/500 second at ISO 100. Treat every session as a live observation, not a copied camera recipe.
The payoff arrives when you stop photographing a bright circle and start recording a world 384,400 km away. Set the baseline, watch the histogram, and let the phase, altitude, and local sky conditions call the final command.