Settings first: f/11, ISO 100, 1/125s. That is the classic Looney 11 rule for a full moon, and it works because the moon’s surface is sunlit — it is reflecting direct sunlight back at you. Once you internalize this counterintuitive fact, moon photography stops being mysterious. The moon is a sunlit subject that happens to be 238,900 miles away, and you expose it accordingly.
The real challenge is not the exposure. It is making the moon look large, detailed, and connected to the landscape below it. A 50mm lens renders the moon as a tiny bright dot — technically accurate to your field of view but emotionally underwhelming. A 400mm telephoto transforms that dot into a textured sphere where you can see individual craters, maria, and the terminator line between light and shadow. And when you position that telephoto moon behind a building, tree, or mountain on the horizon, the compression effect makes the moon appear enormous relative to the foreground — the same effect that makes those breathtaking moonrise-over-the-city images possible.
This guide covers planning, focal length selection, exposure, and the critical technique of balancing the bright moon against a darker landscape.
What You Need
Camera body: Any camera with manual exposure control. A crop-sensor body actually helps here — it multiplies your effective focal length by 1.5x or 1.6x, so a 300mm lens becomes a 450-480mm equivalent, producing a larger moon in the frame.
Telephoto lens: This is the defining piece of gear for moon photography. Here is how focal length translates to moon size in the frame (full-frame sensor):
- 200mm: Moon fills roughly 1.8% of the frame width. Small but usable with a compelling foreground.
- 300mm: Moon fills roughly 2.8%. A good minimum for moon-and-landscape compositions.
- 400mm: Moon fills roughly 3.7%. Craters become visible. Strong compression with foreground subjects.
- 500mm: Moon fills roughly 4.6%. Rich surface detail.
- 600mm: Moon fills roughly 5.5%. Individual craters and maria are clearly defined.
A 2x teleconverter doubles your focal length (200mm becomes 400mm) at the cost of 2 stops of light and some sharpness. For moon photography, where you are shooting at f/8 to f/11 anyway, the light loss is rarely an issue.
Sturdy tripod: At 400mm and above, even microscopic vibrations show as blur. Use a heavy tripod, disable image stabilization, and trigger the shutter with a remote release or the camera’s 2-second timer.
Remote shutter release or intervalometer: Eliminates vibration from pressing the shutter button. A wireless remote or cable release works well. The camera’s built-in 2-second delay timer is a free alternative.
Moon-tracking app: Apps like PhotoPills, The Photographer’s Ephemeris, or Planit Pro show you the exact time, compass bearing, and elevation angle of moonrise for any date and location. These are essential for planning compositions where the moon appears behind a specific landmark.
Camera Settings Breakdown
The Looney 11 Rule: For a full moon in a clear sky, set f/11, ISO 100, and a shutter speed of 1/ISO (1/100s at ISO 100). This rule works because the moon’s surface receives the same intensity of sunlight as a sunlit landscape on Earth. Think of it this way: if you were standing on the moon’s surface, you would use the same sunny-16 rule as on Earth.
Adjustments by moon phase:
- Full moon: f/11, ISO 100, 1/125s
- Gibbous (75% illuminated): f/8, ISO 100, 1/125s
- Quarter moon (50%): f/5.6, ISO 100, 1/125s
- Crescent (25%): f/4, ISO 200, 1/125s
These are starting points. Atmospheric haze, thin clouds, and the moon’s elevation angle all affect brightness. A moon near the horizon passes through more atmosphere and appears dimmer and warmer than a moon high overhead.
Aperture for moon-only shots: f/8 to f/11 hits the sweet spot of your lens’s optical performance. Avoid f/16 and smaller on telephoto lenses — diffraction softens fine crater detail.
Aperture for moon-and-landscape: This is where it gets challenging. At f/11 with the moon properly exposed, the landscape below is likely several stops darker and will appear nearly black. Solutions include shooting during twilight, bracketing, or using a graduated ND filter (which rarely works well because the moon sits at a variable position in the frame).
Shutter speed: Keep it at 1/125s or faster for focal lengths above 300mm. The moon moves across the sky at roughly 15 degrees per hour — which sounds slow, but at 600mm, that motion becomes visible as blur in exposures longer than 1/2 second. At 400mm, stay at or above 1/100s. At 200mm, 1/50s is workable.
ISO: Start at your base (100 or 200). Only raise ISO if atmospheric dimming requires it or if you need to freeze motion at a faster shutter speed. For the moon surface alone, ISO 100-200 is almost always sufficient.
Focus: Manual focus is required. Autofocus systems struggle with the moon — it is a small, bright object against a dark sky, and AF often locks onto nothing or hunts endlessly. Use live view zoom to focus manually on the lunar surface detail.
Step-by-Step Guide
1. Plan the Moonrise Time and Position
The difference between a forgettable moon photo and a stunning one often comes down to planning. You need to know three things: when the moon rises, where on the horizon it rises, and what foreground subject you can align with it.
Open a moon-tracking app and enter your date and location. The app will show you the moonrise time (which varies by roughly 50 minutes each day — the moon rises about 50 minutes later each successive evening), the compass bearing of the moonrise point, and the moon’s trajectory across the sky.
For the most dramatic moonrise images, you want the moon low on the horizon behind a recognizable foreground subject. This means you need to be positioned so that your shooting angle aligns the moon with the subject. Most planning apps include an augmented reality view that lets you hold up your phone at your shooting location and see exactly where the moon will appear relative to the buildings, hills, or trees in front of you.
The best moonrise images happen when the moon is within 5 to 10 degrees of the horizon. At this low angle, atmospheric haze gives the moon a warm amber or orange color, the moon appears at its largest due to the well-known moon illusion (an optical phenomenon, not actual size change), and the moon is close enough to the horizon to appear alongside foreground subjects.
Plan to arrive 15 to 20 minutes before the predicted moonrise time to set up your gear, compose your shot, and test your settings.
2. Choose Your Focal Length
Your focal length determines both the moon’s size and the compression effect with your foreground.
For a moon-and-landmark composition: Longer is better. At 400mm and beyond, you must stand far from your foreground subject — a building, a tree, a statue. This distance compresses the perspective, making the moon appear large behind the subject. A church steeple with a full moon appearing to sit on top of it is achieved not by being close to the church, but by being half a mile to a mile away with a 400-600mm lens.
Calculate the distance you need: if the moon should appear roughly the same visual size as your foreground subject, and the subject is 50 feet tall, you will need to be approximately 1,500 to 3,000 feet away at 400-600mm. The planning apps mentioned above can calculate this precisely.
For a moon-only surface detail shot: Use your longest focal length. At 600mm on a crop sensor (900mm equivalent), the moon fills a substantial portion of the frame and individual craters are clearly visible. The Copernicus crater (58 miles in diameter), the rays extending from Tycho crater, and the dark maria plains all resolve as distinct features.
For a wide moonrise landscape: At 70-200mm, you capture the moon as part of a larger scene — a mountain range, a coastline, a city skyline. The moon will be smaller but contextualized within the landscape. These shots rely on strong foreground composition because the moon alone cannot carry the image at moderate focal lengths.
3. Expose for the Moon’s Surface
Set your camera to manual mode. Input the Looney 11 settings for the current moon phase (see the settings breakdown above). Take a test shot and zoom in on the LCD.
You should see surface detail — the contrast between bright highlands and dark maria, the shadow-casting rims of major craters, the bright rays radiating from Tycho or Copernicus. If the moon is a featureless white circle, you are overexposed. Stop down the aperture or increase the shutter speed.
The crescent and gibbous phases produce the most visually interesting surface detail because the terminator (the line between the lit and unlit portions) casts long shadows across the lunar surface, revealing topography. A full moon, while bright and dramatic in the sky, is lit face-on and appears relatively flat in photographs.
For the earthshine effect on a thin crescent — where the dark portion of the moon is faintly visible — you need a much longer exposure that overexposes the bright crescent. Bracket several exposures: one for the bright crescent, one for the earthshine, and blend them in post-processing.
4. Balance Moon and Landscape Exposure
This is the core technical challenge of moonrise photography. The moon’s surface brightness at full phase is approximately EV 15 (equivalent to a sunlit landscape), while the twilight landscape below might be EV 6 to EV 10 — a difference of 5 to 9 stops. You cannot expose for both in a single frame without one being too bright or too dark.
Solution 1: Shoot during twilight (the golden window). For roughly 10 to 25 minutes around moonrise (when the moon is near the horizon), the ambient light from the fading twilight can be within 2 to 3 stops of the moon’s brightness. This is the magical window when a single exposure can render both the moon and the landscape acceptably. The exact timing depends on the moon phase and the time of year. A full moon rises at approximately sunset, making the twilight alignment nearly automatic. A gibbous moon rises later, so the twilight balance shifts.
During this window, set your exposure to split the difference: slightly overexpose the moon (accepting some lost surface detail) and slightly underexpose the landscape (accepting deeper shadows). An exposure around f/8, ISO 400, 1/60s often works for the twilight balance. Fine-tune from there.
Solution 2: Bracket and blend. Take two exposures from the same tripod position without moving the camera. First, expose for the moon: f/11, ISO 100, 1/125s. Second, expose for the landscape: f/11, ISO 800 to 1600, 1 to 4 seconds. Blend the two in post-processing, using the well-exposed moon from the first frame and the landscape from the second.
This technique requires that the moon not move significantly between frames. At 400mm, shoot both frames within 5 seconds of each other to minimize the moon’s positional shift.
Solution 3: Accept the silhouette. Expose for the moon and let the landscape go dark. A silhouetted skyline, tree, or mountain ridge against a properly exposed moon is a legitimate and compelling compositional choice. The dark foreground becomes a graphic shape that frames and grounds the celestial subject.
5. Focus Precisely on the Lunar Surface
Autofocus rarely locks reliably on the moon. Switch to manual focus and use your camera’s live view at maximum magnification (10x or higher on most cameras).
Point the camera at the moon and zoom the live view display to fill the screen with the lunar disc. Slowly rotate the focus ring until the edge of the moon is razor-sharp — look for a clean, crisp boundary between the bright surface and the dark sky. If the moon is past first quarter, focus on the terminator where the shadow detail is most visible.
Once focus is set, do not touch the focus ring. If your lens has a focus lock switch, engage it. Some photographers tape the focus ring with a small piece of gaffer tape as insurance against accidental bumps.
If you are including a foreground landmark, you face a depth of field decision. At f/8 and 400mm, depth of field is very shallow at close distances but nearly infinite past a few hundred meters. If your foreground subject is at least 200 to 300 meters away, both the subject and the moon (at optical infinity) will be within the depth of field at f/8. If the subject is closer, you may need to focus stack or accept a slightly soft foreground.
Common Mistakes
Using too short a focal length. A 50mm moon photo is almost always disappointing. The moon is tiny in the frame and shows no surface detail. Invest in focal length — rent a 150-600mm zoom if you do not own one. The difference between 100mm and 400mm in moon photography is the difference between a dot and a textured world.
Overexposing the moon. The most common settings error. A bright, featureless white disc is an overexposed moon. Use the Looney 11 rule as your starting point and verify surface detail in every test shot.
Shooting the moon high in the sky. A moon at 45 degrees elevation against empty sky lacks context, atmospheric color, and foreground interest. The most compelling moon images happen within 10 degrees of the horizon, during or immediately after moonrise (or before moonset).
Not planning the alignment. Showing up at a scenic overlook and hoping the moon rises behind the landmark rarely works. The moon’s rise point shifts along the horizon throughout the month. Planning apps eliminate guesswork and ensure you are in the right spot.
Handholding at extreme focal lengths. At 400mm, even the steadiest hands produce some blur. A tripod is not optional for sharp moon detail. If you must handhold, push ISO to 800-1600 and use the fastest shutter speed possible (1/500s or above), accepting increased noise as the tradeoff.
Ignoring atmospheric conditions. Haze, humidity, and air pollution dim the moon and reduce contrast. The moon photographs best in dry, clear air. Winter often provides the cleanest atmospheric conditions for moon photography in temperate climates. If the moon looks hazy to your naked eye, it will look hazy in your photos.
Taking It Further
Moonrise timelapses. Set your intervalometer to fire every 3 to 5 seconds as the moon rises. The resulting time-lapse shows the moon lifting off the horizon, changing color from amber to white as it climbs through the atmospheric layers. Over 30 to 45 minutes, the moon’s trajectory across the sky becomes a dramatic visual arc.
Lunar phase project. Photograph the moon at the same focal length every 3 to 4 days through an entire 29.5-day lunar cycle. This series shows the progression from new moon through crescent, quarter, gibbous, and full phases, then back again. The terminator’s shadow reveals different surface features at each phase.
Moonrise behind multiple landmarks. Using your planning app, identify 5 to 10 local landmarks and calculate the dates when the full (or gibbous) moon will rise directly behind each one. Over several months, build a portfolio of the same moon in dramatically different compositional contexts.
Lunar eclipses. A total lunar eclipse turns the moon a deep red-orange (the “blood moon” effect) as Earth’s shadow covers the surface. During totality, the moon is dramatically dimmer — expect settings around f/4, ISO 1600, 1 to 4 seconds. The red color and unusual dimness create images unlike any other moon photography.
International Space Station transits. With precise planning (websites like transit-finder.com calculate these), you can photograph the ISS silhouetted as it crosses the moon’s face. The transit lasts only 0.5 to 1.5 seconds and requires a fast burst rate (10 fps or higher) at the exact predicted moment. These are among the most rewarding captures in astronomical photography.
ShutterCoach Connection
Upload your moon photos to ShutterCoach for feedback on exposure accuracy, sharpness, and composition. The AI mentor can help you evaluate whether you captured sufficient surface detail, whether your foreground-to-moon balance works, and how to refine your planning for the next moonrise. Tracking your lunar photography in ShutterCoach over multiple sessions creates a visible record of your growth as you progress from basic moon snapshots to planned, precisely executed compositions that showcase both technical skill and creative vision.