0% to 100% in five steps
What phase is it tonight?
You can name tonight's phase with two observations: how much of the disk is lit, and which side carries the light. A half-lit moon high at sunset is a first quarter; the same half-lit disk high at sunrise is a last quarter. Everything else — the day of the cycle, the percentage, the rise time — follows from one number: the 29.53-day synodic month.
0% to 100% in five steps
7.38 days between phases
50 minutes later, daily
90° east, 90° west
5.1° off the Earth's orbit
19 years, 235 lunations
Two observations — the lit fraction and the hour you see the Moon — name any phase without an instrument.
Start with the disk. Fully lit means full; exactly half lit means a quarter; a thin sliver is a crescent; anything between half and full is a gibbous. In a normal waxing run the lit fraction climbs through five steps — 0%, about 25%, 50%, about 75%, 100% — and the waning half repeats them in mirror image.
Then read the geometry. A first quarter moon stands about 90° east of the Sun and is visible from about noon to midnight; a last quarter stands 90° west, shows the opposite half of the surface — the limb with the large craters such as Tycho — and belongs to the hours after midnight. Same 50%, different phase.
For a number rather than a name, the lit fraction is approximately (1 − cos elongation) / 2, where elongation is the Sun–Moon angle in the sky. That one formula converts any estimate of the angle into a percentage illumination.
The eight named phases divide the 29.53-day synodic month into steps of about 7.38 days.
Count from new moon: day 0 is new, day 7.38 is first quarter, day 14.77 is full, day 22.15 is last quarter, and day 29.53 is the next new. The four intermediate names — waxing crescent, waxing gibbous, waning gibbous, waning crescent — sit near the midpoints, around days 3.7, 11.1, 18.5 and 25.8.
The prefixes do real work: waxing means the lit fraction is growing toward full, waning that it is shrinking back toward new. A waxing and a waning crescent show the same roughly 25% of the disk — only the lit limb and the time of night tell them apart.
The phase-by-phase table with rise times and viewing windows lives on the companion page The Eight Moon Phases Explained (/moon-phases-explained); the condensed version appears in the table below.
Work the steps in order; each one names the mistake that most often breaks it.
The check works because the cycle is strict arithmetic wearing a visual costume: light, shape and schedule all derive from the same count of days since new moon, so any two of the three predict the third.
Run the steps on three consecutive evenings and the pattern shows itself — the lit fraction grows, the terminator creeps across the disk, and moonrise slips by roughly 50 minutes a day, all at the same pace.
If two steps disagree, trust the day-count in step five: it is the only one that cannot be fooled by haze, a low horizon or a rough guess at the lit fraction.
Every figure is drawn to the cycle's own numbers — 7.38-day spacing, 50-minute drift, cosine illumination — none is decorative.
The Moon rises about 50 minutes later each day because it moves eastward around the Earth while the Earth turns.
The Moon advances about 13.2° per day along its orbit. The Earth rotates 360° in roughly 23 hours 56 minutes, so each day it must turn about 13.2° further — close to 50 minutes of rotation — before the Moon returns to the same meridian.
The drift ties each phase to a characteristic schedule: a full moon rises near sunset and is up all night; a first quarter rises near noon and sets near midnight; a last quarter rises near midnight and stands high at dawn; a new moon keeps the Sun's hours and is effectively unobservable.
Phase-by-phase rise, transit and set times — and what the 5.1° orbital tilt does to them far from the equator — are set out on the companion page Moonrise and Moonset (/moonrise-and-moonset).
| Phase | Days after new moon | Disk lit | Moonrise (approx.) | Best time to look |
|---|---|---|---|---|
| New | 0 d | 0% | Near sunrise | Not observable — the Moon keeps the Sun's hours |
| Waxing crescent | ≈3.7 d | ≈25% | Mid-morning | Evening twilight, low after sunset |
| First quarter | 7.38 d | 50% | Near noon | About noon to midnight |
| Waxing gibbous | ≈11.1 d | ≈75% | Mid-afternoon | Evening into the early hours |
| Full | 14.77 d | 100% | Near sunset | All night |
| Waning gibbous | ≈18.5 d | ≈75% | Mid-evening | Late evening to morning |
| Last quarter | 22.15 d | 50% | Near midnight | Midnight to dawn |
| Waning crescent | ≈25.8 d | ≈25% | Before dawn | Pre-dawn and morning twilight |
Rather than cite publishers, this almanac cites quantities: each claim on the page can be re-derived from the synodic month, the sidereal period, the orbital tilt and the distance range listed in the definitions.