The Moon Tonight
Nothing here is downloaded — the phase is worked out from the length of the lunar cycle. Pick any date, forwards or backwards, and you'll see the shape the Moon had on that night.
This month
Every night of the month at a glance. Click any day to jump to it.
Phases are calculated from a synodic month of 29.530589 days. Accurate to within a few hours — good enough for the naked eye, not for a spacecraft.
Things worth knowing about it
You've never seen its back
The Moon rotates exactly once per orbit, so the same face always points at us. This is called tidal locking, and Earth's gravity caused it. The far side was first photographed by the Soviet Luna 3 probe in 1959.
It pulls the oceans
The Moon's gravity drags water toward it, creating a bulge — and another on the opposite side of Earth. As the planet rotates through those bulges, coastlines get roughly two high tides a day.
It's drifting away
About 3.8 cm further from Earth every year — measured by bouncing lasers off mirrors the Apollo astronauts left behind. In the age of the dinosaurs, the Moon looked noticeably bigger.
It was probably a collision
The leading theory says a Mars-sized body called Theia struck the young Earth about 4.5 billion years ago. The debris thrown into orbit clumped together and became the Moon.
No air, huge extremes
With almost no atmosphere to hold heat, the surface swings from about 127 °C in sunlight to −173 °C in shadow. And the sky there is black even at noon.
It fits the Sun exactly
The Sun is about 400 times wider than the Moon — and about 400 times further away. That coincidence is why total solar eclipses work at all. No other planet in the solar system gets this.