Phoenicid Meteor Shower
- Active
- December 1 – December 5
- Peak
- Around December 1–2
- Peak rate (ZHR)
- Variable (about 100 in 1956)
- Radiant
- Sculptor (0h 32m, −27°)
- Speed
- 15 km/s (slow)
- Parent comet
- 289P/Blanpain
- Best seen from
- Southern Hemisphere
- Best time
- Evening, from dusk until around midnight
Next peaks
| Expected peak (UTC) | Moon at peak | Moonlight |
|---|---|---|
| December 2, 2026, around 1h | Waning crescent, 41% lit | Some |
| December 2, 2027, around 7h | Waxing crescent, 16% lit | Little or none |
The timing and radiant have shifted between returns, so the IMO suggests checking for meteors from about ten days before the peak date.
Computed from the shower's peak solar longitude (λ☉ 249.5°). Real peaks can come a few hours early or late, and you will see meteors on the nights either side. The peak hour may be in daylight where you are; watch the darkest hours of the nearest night.
The Phoenicids are a shower you watch for the chance, not the numbers: most years bring no clear activity, but they have surprised observers before. If anything appears, the meteors are among the slowest you will ever see.
Where the meteors come from
The parent is Comet 289P/Blanpain. Discovered by J.-J. Blanpain in 1819, it was soon lost for nearly two centuries. In 2003 the Catalina Sky Survey found a faint near-Earth object, 2003 WY25, which is probably the same comet. It orbits the Sun in about 5.3 years, and Jupiter's pull keeps shifting its orbit and dust trails, so encounters are hard to predict. The grains arrive at only about 15 km/s.
When to watch
Activity is listed for December 1 to 5, peaking around December 2 (see the table above). Calculated encounter dates have varied, so the IMO suggests watching from about ten days earlier. The radiant is highest in the early evening.
How to find the radiant
The current radiant lies in faint Sculptor, about 9° (roughly a fist at arm's length) south-southwest of Diphda (Beta Ceti), a lone bright star. From the Southern Hemisphere it passes high overhead in the evening. From about 40°N it climbs only about 23° above the southern horizon and sets around midnight. The original radiant was much farther south, in Phoenix, which gave the shower its name.
What to expect
In a normal year, expect nothing you can be sure of. If Earth meets a dust trail, the meteors will drift slowly across the sky. A population index of about 2.8 (still uncertain) suggests more faint meteors than bright ones. From the north, the low radiant cuts any display to a fraction.
Viewing tips
- Watch from dusk, when the radiant is highest.
- Northern observers need a low, open southern horizon.
- Look for very slow meteors: a Phoenicid crawls.
- Note where any Phoenicids come from, not just how many.
History and notable displays
The shower was discovered on December 5, 1956, when a sudden outburst was seen in the Southern Hemisphere. By the IMO's estimate the ZHR probably reached about 100, and the strongest activity was seen from the Japanese expedition ship Soya in the Indian Ocean. No clear activity followed until December 1, 2014, when meteors arrived at the time predicted by Sato and Watanabe. Encounters calculated for 2024 produced no significant activity.
About the numbers. The ZHR (zenithal hourly rate) is how many meteors one observer would see in an hour under a perfectly dark sky with the radiant straight overhead. Real counts are almost always lower: under suburban skies, or with the radiant low, expect a half to a quarter of it, or less.
Sources
- International Meteor Organization, Meteor Shower Calendar 2026
- International Meteor Organization, Meteor Shower Calendar 2027
- IAU Meteor Data Center, shower 254 (PHO)
- Kasuga (2024), Comet 289P/Blanpain: Near-Perihelion Activity and the Phoenicids, The Astronomical Journal
- Jewitt (2006), Comet D/1819 W1 (Blanpain): Not Dead Yet, The Astronomical Journal 131
- NASA/JPL Small-Body Database, 289P/Blanpain
Checked November 8, 2026.