Meteor showers occur when Earth passes through a stream of debris left behind by a comet (or, in rare cases, an asteroid) as it orbits the Sun. Comets are essentially dirty snowballs — mixtures of ice, dust, and rocky material. As a comet approaches the Sun, solar heat vaporizes its ices, releasing dust and small particles that spread along the comet's orbital path over thousands of years.
When Earth intersects this debris stream, the particles — called meteoroids — enter the atmosphere at high speed (typically 11 to 72 km/s) and burn up due to friction with air molecules, producing the streaks of light we call meteors. Because all the particles in a stream travel in parallel paths, they appear to radiate from a single point in the sky called the radiant.
Select a month from the dropdown to filter meteor showers active during that period. The tool displays all showers with their active date range, peak date, ZHR (Zenithal Hourly Rate), radiant constellation, entry speed, and parent body. Showers currently active are highlighted in green; upcoming showers are highlighted in blue.
To see all showers for the year, select "All Months." This gives you a complete annual calendar of meteor activity.
ZHR stands for Zenithal Hourly Rate — the theoretical number of meteors a single observer would see per hour under ideal conditions: a perfectly dark sky, the radiant directly overhead (at the zenith), and no obstructions. In practice, actual observed rates are almost always lower than ZHR because:
A realistic estimate for a typical dark-sky observer is about 50–60% of the ZHR. For the Perseids (ZHR ~100), expect to see 50–70 meteors per hour under good conditions.
The radiant is the point in the sky from which shower meteors appear to originate. It is named after the constellation where it is located — hence "Perseids" from Perseus, "Leonids" from Leo, and so on. The higher the radiant is above the horizon, the more meteors you will see, because more of the sky is exposed to the incoming stream.
For most northern hemisphere showers, the radiant rises during the evening and reaches its highest point in the pre-dawn hours. This is why meteor shower rates are typically highest between midnight and dawn — the radiant is highest, and the observer is on the leading side of Earth as it moves through the debris stream.
The speed at which meteoroids enter the atmosphere affects their appearance. Slow meteors (around 11–25 km/s, like the Taurids) tend to be bright, long-lasting, and sometimes orange or red. Fast meteors (60–72 km/s, like the Leonids) are typically white or blue-white, brief, and may leave persistent glowing trains. The Geminids, despite being relatively slow at 35 km/s, are known for producing many bright meteors and occasional fireballs.
The most important factors for a successful meteor shower observation are:
| Shower | Peak | ZHR | Speed |
|---|---|---|---|
| Quadrantids | Jan 3 | 120 | 41 km/s |
| Perseids | Aug 12 | 100 | 59 km/s |
| Geminids | Dec 14 | 150 | 35 km/s |
| Leonids | Nov 17 | 15 | 71 km/s |
| Eta Aquariids | May 6 | 50 | 66 km/s |