Global reference time: October 1, 2026 at 12:58 UTC. Your local calendar date may differ.
Catalog activity begins
Catalog activity ends
The peak is not necessarily the best time to look from your location. Horizon, darkness, Moon position and weather determine the useful observing window.
What to expect
Visibility & observing notes
A daytime shower for radio observation; not an ordinary naked-eye event.
Any listed zenithal hourly rate assumes ideal observing conditions. Your visible count can be much lower; it is not a local forecast.
IMO shower code
221-DSX
Ideal zenithal hourly rate
5
Observation method
Radio
Make it local
Can I see it near me?
See the best time to look and whether clouds might get in the way. Local weather is usually available up to 16 days ahead.
Approximate area
City names: GeoNames (CC BY 4.0). Try a nearby city if your town is not listed.
Your network can suggest an approximate area; it may be wrong if you use a VPN. A city you choose is remembered in this tab until you close it. Precise location needs your browser’s permission and is never saved here. Your location stays out of share links and calendar downloads.
Choose a place for your local sky outlook.
Understand the moment
Earth crosses a trail of debris
The geometry behind Daytime Sextantids Meteor Shower
Meteor showers happen as Earth encounters debris left along a comet’s or asteroid’s orbit. Small particles entering the atmosphere create the streaks we see; they are separate from the large planetary bodies in the explorer.
Follow Earth’s position through the year. This entry is for radio observation, so darkness and the Moon’s phase do not determine whether a radio receiver can detect activity.
Opens . Each scene is an exact daily sample, without interpolation; it is separate from the catalog peak of 12:58 UTC.
How to read the scene: The lab does not model a debris stream, radiant, outburst or meteor count. Use the event’s source and local outlook for activity predictions and observing conditions.
A little context. A better view.
Meteor Showers: a field guide
01
The peak is a reference point
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.
02
Read meteor rates carefully
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.
03
Give the sky your attention
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.
04
Some entries need specialist equipment
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.
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.
October Camelopardalids activity peaks with a listed zenithal hourly rate of 5. Actual visible rates depend on sky darkness, radiant altitude, and local weather.