Biggest Supermoon of 2026 — December 24: How to Observe with FastTool

The biggest supermoon of 2026 arrives on December 24 — Christmas Eve — with the Moon just 356,600 km from Earth. At 34 arcminutes apparent diameter, it appears 14% larger than an average full moon. Learn when and how to observe and photograph this spectacular supermoon with FastTool's MoonSync.

Biggest Supermoon of 2026 — Christmas Eve

On December 24, 2026, the full Moon makes its closest approach to Earth for the entire year — a distance of just 356,600 kilometers. This makes it the largest and brightest supermoon of 2026, and it arrives on Christmas Eve, adding celestial spectacle to the holiday season.

At this distance, the Moon spans 34 arcminutes across — a full 3 arcminutes larger than an average full moon. For photographers, observers, and anyone who has ever looked up at the night sky in wonder, December 24, 2026 is the night to be outside.

What Is a Supermoon?

The term "supermoon" was coined by astrologer Richard Nolle in 1979, but the astronomical definition is straightforward: a supermoon occurs when a full moon (or new moon) coincides with perigee — the point in the Moon's elliptical orbit where it is closest to Earth.

The Moon's orbit around Earth is not a perfect circle. It's an ellipse with an eccentricity of approximately 0.055, meaning the Earth-Moon distance varies by about 50,000 km over each 27.3-day orbit:

| Orbital Position | Distance from Earth | Apparent Diameter | |-----------------|:-------------------:|:-----------------:| | Perigee (closest) | ~356,600 km (Dec 24) | 34.0′ | | Average | ~384,400 km | 31.1′ | | Apogee (farthest) | ~406,500 km | 29.4′ |

The difference between perigee and apogee is about 14% in apparent diameter and approximately 30% in brightness (brightness scales with apparent area, which is proportional to the square of diameter).

Not All Supermoons Are Equal

The term "supermoon" is often applied loosely to any full moon within 90% of perigee — which means 3–4 full moons per year qualify. But the closest full moon of the year stands apart:

| 2026 Supermoon | Date | Distance | Diameter | Rank | |---------------|------|:--------:|:--------:|:----:| | November 24 | Nov 24 | ~360,100 km | 33.6′ | 2nd | | December 24 | Dec 24 | 356,600 km | 34.0′ | 1st (biggest) |

The December 24 supermoon is the definitive event. At 356,600 km, it approaches the theoretical minimum perigee distance possible (about 356,400 km), making it as close to a "maximum supermoon" as nature typically allows.

Christmas Eve 2026 — A Rare Holiday Supermoon

The coincidence of the biggest supermoon of the year on Christmas Eve is notably rare. The last time a supermoon fell on Christmas Eve was in 2015, and the next comparable event — a Christmas Eve full moon at or near perigee — won't occur until 2051.

For observers in the Northern Hemisphere, the December supermoon has an additional advantage: the winter full moon stays in the sky longer than any other full moon of the year. Around the December solstice (December 21), the Sun's low arc means the full Moon follows a high arc, remaining above the horizon for extended hours — well over 12 hours at mid-northern latitudes.

The Moon Illusion

The most dramatic viewing moment will be moonrise on December 24. At this time, the supermoon will appear even larger than its true 34′ diameter — thanks to the well-known but still poorly understood moon illusion.

When the Moon is near the horizon, the human visual system compares it to distant terrestrial objects (buildings, trees, mountains), and the brain interprets the Moon as being farther away — and therefore "must be" larger. This is entirely a perceptual effect (the Moon's true angular size is actually very slightly smaller at the horizon due to atmospheric refraction), but the visual impact is undeniable.

Best viewing strategy: Find a location where you can see the eastern horizon with foreground objects — a city skyline, a line of trees, or distant hills. The moon illusion is strongest when the Moon appears close to familiar-sized objects.

How to Observe the Supermoon

Naked-Eye Observation

No equipment needed. The supermoon is visible to everyone with clear skies:

  1. Moonrise: The Moon rises in the east around sunset (the exact time varies by location — use MoonSync to get your local time). This is the prime viewing window — the moon illusion is strongest and the Moon's golden-orange color (caused by increased atmospheric path length) is most dramatic.

  2. Transit: When the Moon crosses the meridian (highest point in the sky), typically around local midnight. At this point, the Moon appears somewhat smaller and whiter than at moonrise, but its brightness is at maximum.

  3. Moonset: The Moon sets in the west around sunrise on December 25. If you're up early on Christmas morning, the setting supermoon in the western sky makes a beautiful complement to sunrise.

Binocular Observation

With 7×50 or 10×50 binoculars:

  • The Moon fills about 1/3 of the field of view — a dramatic sight
  • Craters and maria (dark plains) along the terminator (the line between light and dark, if not precisely full) show enhanced relief
  • The Moon's subtle color variations — blue-gray in the maria, lighter gray-tan in the highlands — become more distinct

Telescope Observation

For telescope users, the supermoon's large apparent size means you can use higher magnification than usual while keeping the entire lunar disk in the field of view:

Use the Telescope FOV Calculator to find eyepiece combinations that frame the 34′ lunar disk. A setup yielding a true field of view of about 40–45′ provides a comfortable margin around the Moon.

Recommended for visual observation: Magnification of 100–150× with an 82° eyepiece will show individual crater details while keeping the full disk context.

Supermoon Photography

The supermoon is one of the most photogenic astronomical events. Here's how to capture it:

Equipment

| Item | Recommendation | Why | |------|---------------|-----| | Camera | DSLR or mirrorless | Manual exposure control is essential | | Lens | 200–600mm telephoto | 300mm+ fills the frame with lunar detail | | Tripod | Sturdy, with ball head | Moon exposures are surprisingly short — but a tripod ensures critical sharpness | | Remote shutter | Cable or wireless | Eliminates camera shake at long focal lengths |

Settings

| Scenario | ISO | Aperture | Shutter Speed | |----------|:---:|:--------:|:-------------:| | Moon high in sky (bright) | 100–200 | f/8–f/11 | 1/125s–1/250s | | Moon at moonrise (dimmer, golden) | 400–800 | f/5.6–f/8 | 1/60s–1/125s | | Moon with landscape (foreground) | 400–800 | f/5.6–f/8 | 1/15s–1/60s |

The Looney 11 Rule: For a full Moon high in the sky, set aperture to f/11 and shutter speed to 1/ISO. Example: ISO 200 = 1/200s at f/11.

Composition Tips

  1. Moonrise with foreground: The most striking supermoon photos pair the large, golden moonrise Moon with a recognizable terrestrial foreground — a church spire, mountain ridge, or city skyline. Use PhotoPills or Planit Pro to plan the exact alignment.

  2. Moon behind thin clouds: Cirrus clouds diffract moonlight into a halo or corona pattern — ethereal and beautiful.

  3. Lunar disc details: At 600mm+, the supermoon fills most of the frame. Focus on crater detail along the terminator for maximum texture.

  4. Composite with landscape: The classic "huge moon over the city" shot is almost always a composite — the Moon exposed separately from the landscape and combined in post. This isn't "cheating" — it's the only way to capture the full dynamic range.

Smartphone Photography

You won't get a frame-filling Moon with a smartphone, but you can still capture memorable supermoon scenes:

  • Use night mode if available
  • Tap the Moon on screen to lock focus and reduce exposure (the Moon is brighter than the sky)
  • Include foreground elements — a silhouette of trees, buildings, or people
  • A smartphone adapter for a small telescope or binoculars (afocal photography) yields surprisingly good results

The Science: Why Perigee Distance Varies

Not every perigee is equally close. The Moon's orbit is perturbed by the Sun's gravity, producing variations of up to ~13,000 km in perigee distance from month to month. The closest perigees ("proxigees") occur when:

  1. The Moon is at perigee (closest point in its elliptical orbit)
  2. The Earth-Moon line is roughly aligned with the Earth-Sun line (new or full moon — syzygy)
  3. The Sun's tidal force pulls the Moon's orbit into a slightly more eccentric configuration

When all three factors align — as on December 24, 2026 — the result is the year's closest full moon.

Using FastTool for Supermoon Planning

MoonSync — Real-Time Lunar Data

MoonSync provides everything you need to plan your supermoon observation:

  • Moonrise/moonset times for your exact location — critical for catching the moonrise show
  • Lunar altitude and azimuth at any time — find the exact direction to set up your camera
  • Moon phase and illumination — confirm that December 24 is the precise full moon moment
  • Lunar Time Clock (LTC) — the proposed lunar time standard, showing how the Moon's relative time drifts due to relativistic effects

Telescope FOV Calculator — Eyepiece Selection

The Telescope FOV Calculator helps you select eyepiece combinations that frame the 34′ supermoon perfectly within your telescope's field of view.

Plan Your Supermoon with MoonSync →

Supermoon Tides

Supermoons have a measurable physical effect on Earth: perigean spring tides. When the Moon is at perigee and in syzygy (aligned with Earth and Sun at full moon), the combined gravitational pull produces tides approximately 5 cm (2 inches) higher than normal spring tides.

For most coastal areas, this is a minor effect — but when combined with storm surge or seasonal high tides, perigean spring tides can contribute to coastal flooding in low-lying areas. The effect is strongest along coasts with large tidal ranges (Bay of Fundy, Bristol Channel, Normandy coast).


Lunar distance data verified against JPL DE440 ephemeris. Supermoon dates and distances calculated from JPL Horizons System. Moon illusion explanation based on current cognitive science consensus (Kaufman & Rock, 1962; Hershenson, 1989). Tide data from NOAA tide predictions.

All tools on fastool.io run entirely in your browser — zero data leaves your device. No personal data is collected, stored, or transmitted to any server. Solar calculations use SunCalc.js; lunar data uses JPL DE440 ephemeris; coordinate transforms use publicly documented EPSG/OGC standards. This site requires no signup, no account, and no cloud processing.