This Hour's Moon
NASA SVS · loading…- Phase
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- Illuminated
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- Distance
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- Apparent size
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- Moonrise
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- Moonset
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Rise and set for your location — set it on the dashboard.
Every render on this page is built from laser-altimeter maps made by the Lunar Reconnaissance Orbiter — the real terrain, the real tilt, the real shadows for the real hour.
Rise and set for your location — set it on the dashboard.
Thirty days of moon in a few seconds. Watch two things: the phase sweeping through its cycle, and the whole disk slowly rocking side to side. That wobble is libration — the Moon's orbit is tilted and not quite circular, so over a month we peek slightly around its edges. We see about 59% of the Moon from Earth, not 50%.
Computed in your browser for every day this month. The percentage is how much of the visible disk is lit at midday.
Eclipse maps tell you where the shadow goes. This tells you what you'll see — computed for your location (set it on the dashboard).
What the Moon does next — quarters, closest and farthest approach, and the next time it slides into Earth's shadow.
Quarters, apsides, and eclipses are computed in your browser with Astronomy Engine, which is accurate to about a minute over centuries. The moon renders come from NASA's Scientific Visualization Studio, generated for every hour of the year from Lunar Reconnaissance Orbiter terrain and imagery. A perigee full moon — a "supermoon" — looks about 14% bigger and 30% brighter than one at apogee.