AstroNube · Subject Guides

Imaging the Moon
with the Dwarf 3

The Moon is the most rewarding first target for any smart telescope — bright, detailed, and visible from suburban gardens. This guide covers every phase, the best features to target, optimal Dwarf 3 settings, and how to get the most from your data.

Why start with the Moon

Any sky conditions
Light pollution, suburban skies, and thin cloud all have negligible impact. If you can see the Moon, you can image it.
Instant results
No EQ Mode, no dark frames, no waiting for a dark sky. Point, lock, and you have a detailed image within minutes.
🔬
Surface detail
Craters, mountain ranges, rilles, and ancient lava plains — the Moon offers more fine detail per session than any other target accessible to the Dwarf 3.
📱
Learns the app
Lunar mode in the DWARFLAB app is the most forgiving mode to learn tracking, filter selection, and basic parameter control before moving to deep sky work.

Imaging quality by phase

🌑
New Moon
0–5% illumination
Not visible
The Moon is not visible — it rises and sets with the Sun. The new moon window is actually the best time to image deep sky objects as the sky is at its darkest.
🌒
Waxing Crescent
5–49% illumination · Sets early evening
Excellent
Outstanding for detail work. The terminator runs through the most dramatic terrain — Clavius, Tycho, and the southern highlands are fully in shadow relief. Ideal window: 3–7 days after new moon.
🌓
First Quarter
~50% illumination · Sets around midnight
Excellent
The terminator bisects the disc through Mare Imbrium and the Apennine mountains. Copernicus crater is at its most dramatic with long shadow relief. One of the best nights of the lunar month.
🌔
Waxing Gibbous
50–99% illumination · Visible most of night
Good
Large illuminated area offers wide coverage. Terminator detail on the eastern maria. The great ray systems around Tycho and Copernicus begin to extend across the disc.
🌕
Full Moon
100% illumination · Up all night
Different character
No terminator shadows — craters lose their relief and look flat. However: ray systems are at maximum visibility, albedo features (bright/dark regions) are clearest, and the full disc mosaic is most striking. A different kind of imaging, not worse.
🌖
Waning Gibbous
50–99% illumination · Rises late evening
Good
Mirror of waxing gibbous but now on the western limb. Mare Orientale region and the western highlands. The Moon rises later — late night / early morning sessions.
🌗
Last Quarter
~50% illumination · Rises around midnight
Excellent
The terminator now illuminates the western side — Oceanus Procellarum, Mare Humorum, and the Grimaldi basin are in dramatic relief. Mirror image of the first quarter but a different set of features highlighted.
🌘
Waning Crescent
5–49% illumination · Rises before dawn
Excellent
Thin crescent in the pre-dawn sky — challenging to catch but rewarding. Earthshine (light reflected from Earth illuminating the dark limb) is most visible and most photogenic in this phase.

Dwarf 3 settings by scenario

Scenario Exposure Gain Filter Mode EQ Mode Notes
Full disc — quick look Auto Auto VIS Lunar No Auto Parameters work reliably here
Crescent — terminator detail 1/250–1/100s 10–30 VIS Lunar No Bright limb will be overexposed — expose for terminator
First / Last Quarter 1/400–1/200s 0–20 VIS Lunar No Keep gain low — the disc is bright
Full Moon disc 1/800–1/400s 0–10 VIS Lunar No Full Moon is very bright — shortest practical exposure
Full disc mosaic 1/400–1/200s 0–15 VIS Lunar / Mosaic Yes (Mosaic) Use Mosaic Mode for full disc at telephoto scale. EQ Mode required.
Earthshine (dark limb) 1–5s 40–60 VIS Astro / Manual Yes Expose for the dark limb — bright limb will saturate. Crescent phases only.
Time lapse Auto Auto VIS Time Lapse No 5–30 second intervals. Great for showing Moon moving across a fixed star field.

Features worth targeting

Tycho Crater
Southern highlands · 85km diameter
One of the youngest large craters on the Moon, with a prominent central peak and a dramatic ray system extending across the entire disc. Best near first quarter when in shadow relief.
★ The ray system is most visible at full moon
Copernicus Crater
Mare Imbrium border · 93km diameter
A beautifully preserved impact crater with terraced walls, a complex central peak group, and a hummocky ejecta blanket. Considered one of the most photogenic craters on the Moon.
★ Best 8–10 days after new moon
Clavius Crater
Southern highlands · 225km diameter
One of the largest impact craters visible, containing a notable curved chain of progressively smaller craters across its floor. The scale is striking — fits within the Dwarf 3 telephoto field of view.
★ Best 7–9 days after new moon
🏔Apennine Mountains
Mare Imbrium border · 600km range
The most dramatic mountain range on the Moon, with peaks rising to 5km. They form the southeastern border of Mare Imbrium and are spectacularly lit at first quarter. Contains Mons Hadley — the landing area of Apollo 15.
★ Best at first quarter
🌊Mare Imbrium
Northern hemisphere · 1,100km basin
A vast ancient lava plain — the "Sea of Rains". At first quarter the mountainous border is in dramatic shadow relief while the dark basaltic plain is fully lit. Contains several ghost craters barely visible as circular ridges.
★ Best at first quarter and waxing gibbous
Vallis Alpes (Alpine Valley)
Northern highlands · 180km long
A remarkable straight valley cutting through the lunar Alps, formed by a fault system. A thin central rille runs along its floor — challenging to resolve but rewarding in good seeing conditions.
★ Best at first quarter
🌊Mare Crisium
Eastern limb · 740 × 560km basin
An isolated circular mare basin near the eastern limb — striking because it appears isolated from the connected mare system. Particularly dramatic at crescent phase when it sits right on the lit side of the terminator.
★ Best 4–6 days after new moon
Earthshine
Dark limb · Crescent phases only
The faint glow on the dark portion of a crescent Moon, caused by sunlight reflected from Earth illuminating the lunar night side. Photographically beautiful — requires longer exposure than the bright crescent, causing the bright limb to saturate.
★ Best 2–4 days after new moon

Imaging tips

01

Expose for the terminator, not the limb

The terminator (day/night boundary) is where all the shadow detail lives. Expose to retain detail there — the bright limb will often saturate slightly and that's acceptable. The app's histogram helps judge this.

02

Wait for the Moon to gain altitude

At low altitude the Moon passes through more atmosphere, causing shimmer and colour fringing. Wait until it's above 25–30° for noticeably sharper results. At 53°N the full Moon in winter stays low — late spring and summer are better for altitude.

03

Single best frame vs stacking

Unlike deep sky imaging where stacking is essential, the Moon is bright enough that a single well-exposed frame can be excellent. Stacking helps in poor seeing — the app's lucky imaging approach picks the sharpest frames. Use Video mode for best-frame selection on planetary and lunar detail work.

04

Let the scope thermally stabilise

Bring the Dwarf 3 outside 15–20 minutes before imaging. A warm scope in cold air creates tube currents that blur the image — the same applies to lunar as to deep sky. Especially important in Ireland where the temperature difference between indoors and outside can be significant.

05

Use Mosaic Mode for the full disc

At the telephoto focal length (150mm), the Moon doesn't quite fit in one frame. Mosaic Mode stitches multiple adjacent frames for a full disc image. EQ Mode must be active. This gives a significantly more detailed full disc image than a single frame at the wide-angle lens setting.

06

Seeing matters more for the Moon than for DSOs

Deep sky stacking can overcome moderate turbulence. Lunar detail work cannot — atmospheric shimmer directly limits resolution. The best lunar seeing at 53°N typically occurs in late spring and early autumn when temperature gradients are minimal. Check seeing forecasts on Meteoblue or Clear Outside before a detail session.

07

The same crater looks different every lunation

The terminator crosses each feature at a slightly different illumination angle each month due to lunar libration. Tycho at day 7 after new moon in January looks different from Tycho at day 7 in July. Revisiting targets is always worthwhile.

Processing approach

In-app (Infinity Lab)

No external software needed

The DWARFLAB app's Infinity Lab tools handle basic lunar enhancement. Stellar Studio applies sharpening, contrast, and colour adjustments to your stacked result. Sufficient for sharing quality output without any additional software.

  • Open your session in Infinity Lab
  • Apply Stellar Studio auto enhancement
  • Adjust sharpness slider — lunar detail responds well to modest sharpening
  • Export at full resolution

External processing

Siril / Photoshop / GIMP

For maximum detail, process the raw FITS files from the Dwarf 3 in dedicated software. Lunar images benefit from sharpening techniques like unsharp mask or wavelets which the in-app tools apply in a simplified form.

  • Export FITS from the app to your device or via WiFi transfer
  • Open in Siril — apply any remaining calibration
  • Convert to 16-bit TIFF for further processing
  • Apply wavelets or unsharp mask in GIMP/Photoshop
  • Subtle contrast curve to lift shadow detail

Tools & next steps