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Observation Settings

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Meteor shower Southern lambda-Draconids — observing times and guide

Southern lambda-Draconids visibility on 2026-11-04

Southern lambda-Draconids Visible from early morning until sunrise

Southern lambda-Draconids rise and set timetable

TimeElevation
Moonrise, 27.3% illuminated 01:50-0°
Southern lambda-Draconids radiant transit07:5222°
Southern lambda-Draconids radiant set13:51
Moonset14:12-2°
Astronomical observing session begins18:58-21°
Southern lambda-Draconids radiant rise01:49
Astronomical observing session ends04:2814°
Twilight end (−12°)04:5316°
Civil sunrise05:1817°
Sunrise05:4119°

Track Southern lambda-Draconids position throughout the night

← 4 November 2026 →

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Time
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Shift the map to change the time and observe Southern lambda-Draconids changing position in the night sky.

Moon conditions for Southern lambda-Draconids — 2026

Time

 

Meteor visibility depends strongly on the Moon’s position and brightness. This chart helps identify darker observing periods.

Blue and white show night and day; red marks when the radiant is above the horizon, the white line its transit, and grey when the Moon is above the horizon. Select a date for detailed Sun and Moon times.

MerakDubhePhecdaAliothMizarKochabSouthern lambda-Draconids

Finder Chart for Southern lambda-Draconids

Field of view 5.0°

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Observing the Southern lambda-Draconids

Radiant position:

  • Right Ascension: 10h 47m 13s"
  • Declination: 68° 00' 00s

Peak activity: Active from November 3 to November 8; with peak activity around November 4.

Southern lambda-Draconids — Observation history

Previous activity records show the reported start, peak and end dates. Exact dates may shift slightly from year to year.

Year Start date Peak date End date
2013November 1November 3November 5
2016October 31November 2November 3
2022November 3November 4November 8

Use these dates as a historical guide and check current predictions near the event.

Data Credits

Meteor data are provided by the International Astronomical Union Meteor Data Center . We thank the observers and researchers who contribute these records.