September Epsilon Perseids Meteor Shower
September Epsilon Perseids activity peaks with a listed zenithal hourly rate of 8. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Your guide to the sky
A quiet night. A wide-open sky. Then a streak of light. Find annual showers and possible outbursts, with a clear distinction between predicted activity and what you may actually see.
Plan ahead
The next 400 days in the available catalog. Event pages explain local visibility and prediction uncertainty.
September Epsilon Perseids activity peaks with a listed zenithal hourly rate of 8. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
September Lyncids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
A daytime shower included for radio observation; it is not a normal naked-eye event.
October Camelopardalids activity peaks with a listed zenithal hourly rate of 5. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Draconids activity peaks with a listed zenithal hourly rate of 5. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Epsilon Geminids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Orionids activity peaks with a listed zenithal hourly rate of 20. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Leonis Minorids activity peaks with a listed zenithal hourly rate of 2. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Southern Taurids activity peaks with a listed zenithal hourly rate of 7. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Northern Taurids activity peaks with a listed zenithal hourly rate of 5. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Leonids activity peaks with a listed zenithal hourly rate of 15. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Alpha Monocerotids activity peaks with a listed zenithal hourly rate of Var. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
November Orionids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Phoenicids activity peaks with a listed zenithal hourly rate of Var. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
IMO lists this as a radiant reference date rather than a confirmed true maximum.
Sigma Hydrids activity peaks with a listed zenithal hourly rate of 7. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Monocerotids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Geminids activity peaks with a listed zenithal hourly rate of 150. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Ursids activity peaks with a listed zenithal hourly rate of 10. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Comae Berenicids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Quadrantids activity peaks with a listed zenithal hourly rate of 80+. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Gamma Ursae Minorids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Alpha Centaurids activity peaks with a listed zenithal hourly rate of 6. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
April Lyrids activity peaks with a listed zenithal hourly rate of 18. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Pi Puppids activity peaks with a listed zenithal hourly rate of Var. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Eta Aquariids activity peaks with a listed zenithal hourly rate of 50. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Eta Lyrids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
A daytime shower included for radio observation; it is not a normal naked-eye event.
June Bootids activity peaks with a listed zenithal hourly rate of Var. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
July Pegasids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
July Gamma Draconids activity peaks with a listed zenithal hourly rate of 5. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Alpha Capricornids activity peaks with a listed zenithal hourly rate of 5. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Southern Delta Aquariids activity peaks with a listed zenithal hourly rate of 25. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Eta Eridanids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
A probably weak Perseid dust-trail encounter is predicted.
A potentially strong Perseid dust-trail encounter is predicted, with a modeled ZHR of 280.
Rarified fragments of the 1479 Perseid trail may add to background activity.
A modeled concentration of many old Perseid trails may produce activity unlike the usual shower.
A Perseid filament encounter is predicted with a modeled ZHR of about 50.
Perseids activity peaks with a listed zenithal hourly rate of 110+. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Kappa Cygnids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Aurigids activity peaks with a listed zenithal hourly rate of 6. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
September Epsilon Perseids activity peaks with a listed zenithal hourly rate of 8. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
September Lyncids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
A daytime shower included for radio observation; it is not a normal naked-eye event.
October Camelopardalids activity peaks with a listed zenithal hourly rate of 5. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Draconids activity peaks with a listed zenithal hourly rate of 5. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Orionids activity peaks with a listed zenithal hourly rate of 20. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Southern Taurids activity peaks with a listed zenithal hourly rate of 7. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Catalog refreshed . Dates and predictions come from the catalog used by Forecast Bar, with a source on every event.
Calendar day groupings use UTC. Event times adapt to your device’s time zone when JavaScript is available. Exact local visibility and weather can differ from the global catalog timing.
A little context. A better view.
Showers are active over a range of dates. The catalog peak is a global prediction; a useful local viewing window also depends on darkness and how high the radiant is above your horizon.
A zenithal hourly rate (ZHR) describes ideal conditions with the radiant overhead and a dark sky. Clouds, light pollution, moonlight and a low radiant can greatly reduce visible counts. A listed rate is not a promise.
Find a dark location with an open view, allow about 20–30 minutes for your eyes to adjust, and look across a wide area of sky. A telescope is not necessary for visual meteor watching.
Daytime radio showers and provisional radiant reference dates are retained in the catalog for completeness. Their event pages explain when they are not ordinary naked-eye observing opportunities.
Learn more: NASA’s meteor-watching advice
Past events, preserved for reference.
Aurigids activity peaks with a listed zenithal hourly rate of 6. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Kappa Cygnids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
Perseids activity peaks with a listed zenithal hourly rate of 100. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
A weak Perseid filament encounter is predicted near the traditional maximum, with timing uncertainty of about five hours.
A predicted encounter with one branch of the old 1079 Perseid dust trail; no reliable activity-rate estimate is available.
Eta Eridanids activity peaks with a listed zenithal hourly rate of 3. Actual visible rates depend on sky darkness, radiant altitude, and local weather.
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