The night sky is about to put on a show – but whether you see just a handful of meteors or a dazzling stream of streaks could come down to timing, moonlight, and where you’re watching from. And this is the part most people miss: even on an active week, small details like your location and light pollution can make or break your meteor-watching experience.
Meteor Activity Outlook for 29 November – 5 December 2025
During this week, the Moon reaches its full phase on Friday, December 5, which has a huge impact on how many meteors you will actually see. On that date, the Moon sits opposite the Sun in the sky, meaning it stays above the horizon all night and floods the sky with bright light, washing out fainter meteors. Earlier in the week, especially this weekend, the Moon is in its waxing gibbous phase and will set in the early morning hours, creating a short but valuable dark window between moonset and dawn when meteor activity becomes easier to spot.
Expected Meteor Rates
For evening observers this weekend, the overall expected hourly meteor rate is quite modest. From mid-northern latitudes around 45°N, you can expect roughly 3 meteors per hour, while observers near tropical southern latitudes around 25°S may see about 2 per hour. These low evening numbers are mainly due to interference from the bright Moon, which drowns out many of the fainter meteors that would otherwise be visible.
If you are watching in the early morning hours before dawn, the outlook is significantly better. From mid-northern latitudes (around 45°N), observers can expect hourly rates near 18 meteors, while those in tropical southern regions (about 25°S) may see around 12 meteors per hour under good conditions. This difference between evening and morning rates is normal because the Earth’s rotation brings the observer into the direction of the meteoroid stream in the early morning, but the strong moonlight still reduces what could otherwise be even higher counts.
Factors Affecting What You Actually See
The real number of meteors you personally observe can differ a lot from these estimates. Your individual sensitivity to light and motion, how dark-adapted your eyes are, your level of alertness, and your previous experience watching meteors all play important roles. Local weather conditions are also critical; even thin haze or patchy clouds can hide many faint meteors and create the impression that the “shower is weak” when the sky is actually just not cooperating.
It is important to remember that the quoted hourly rates assume you are observing from a truly dark location with minimal light pollution, such as a rural area far from city lights. In urban or suburban environments, skyglow from artificial lighting significantly reduces the number of visible meteors, limiting you mostly to the brightest streaks. This is one of those points that often sparks debate: is it worth going out in a city? It can be, but expectations must be adjusted because city observers will inevitably see fewer meteors than those under dark, rural skies.
Radiant Positions and How to Use Them
The radiant is the point in the sky from which meteors from a particular shower seem to originate, much like the vanishing point of parallel lines in perspective drawing. For this forecast, the radiant positions and expected rates are calculated specifically for Saturday night and Sunday morning, November 29–30, but they change only slowly from night to night. Because of this, these same coordinates are accurate enough to use throughout the entire period of November 29 to December 5.
Most star atlases, whether printed books, online sky charts, or maps included in planetarium software, display celestial coordinates using right ascension and declination. You can use these coordinate grids to locate each shower’s radiant in the sky with decent accuracy. If you are new to stargazing, this can feel a bit technical at first, but with a simple atlas or sky app, matching the listed coordinates to the sky becomes much easier and helps you know roughly where the meteors are radiating from.
Charts and Tools for Orientation
Accompanying this outlook are sky charts that show radiant positions for three key times: evening, midnight, and morning. The center of each chart corresponds to the point directly overhead (the zenith) for that specific hour, helping you quickly orient yourself to what is above you at that time. These charts are drawn for an observer facing south, but you can mentally rotate them—or physically rotate a printed version—to match any direction you are facing.
A simple star wheel (planisphere) or a planetarium app on a phone or tablet is also extremely helpful, especially for beginners. These tools let you set the date and time to see a realistic depiction of the sky from your location at any hour of the night, all year round. With them, you can confirm which constellation you are looking at and cross-check the radiant positions listed in the forecast more easily, making your observing session smoother and more enjoyable.
Best Time to Watch Each Radiant
Meteor activity from a given radiant is strongest when that radiant is highest above the horizon, a position known as culmination. Depending on your latitude, this happens either due south or due north along the imaginary line called the meridian, which runs from north to south through the point overhead. When a radiant is low in the sky, more meteors occur below your horizon, so fewer are visible; when it is high, you can see more of the total activity.
Some radiants rise only after midnight and do not reach their peak height until after sunrise, when the sky is already bright. For these radiants, the best practical time to observe is during the final hours before dawn, when they are high enough to be productive but the sky is still dark. This is why serious meteor observers often set alarms for the early morning rather than staying out all night.
Where to Look in the Sky
A common misconception is that you should stare directly at the radiant to see the most meteors, but this is rarely the best approach. In practice, meteors from a shower appear to streak outward from the radiant and travel across the sky, so you usually see them some distance away from the radiant itself. If you look too close to the radiant, many meteor trails will appear too short to be impressive.
For best results, center your view so that the radiant sits near the edge of your field of vision rather than directly in the middle. This gives each meteor more room to draw a visible trail and makes it easier to mentally trace the meteor’s path back toward the radiant to decide whether it belongs to that shower or is just a random (sporadic) meteor. Also remember that if a radiant is far below the horizon for your location, its meteors will not be visible at all because the meteoroids are entering the atmosphere on the other side of the Earth.
Order of Radiants by Right Ascension
The list of meteor sources for this week is arranged from west to east by right ascension, which is the sky’s version of longitude. Radiants listed first have smaller right ascension values, meaning they appear in the sky earlier in the night for most observers. As the night progresses, radiants with larger right ascension values rise and become observable later.
This west-to-east ordering helps you plan when to observe each shower. For example, if you know a radiant with a small right ascension is already up in the evening, you can start watching for its meteors early. Radiants farther east will require more patience, only becoming high enough for productive viewing as the night moves toward midnight and the early morning hours.
Showers Expected to Be Active This Week
Several distinct sources of meteoric activity are expected to be active during this period. Some are well-known showers that return every year with fairly predictable rates, while others are more subtle or only occasionally produce strong outbursts. Here is where it gets interesting—and sometimes controversial—because some showers have a reputation based on one dramatic past event but are usually very quiet in typical years.
December Phoenicids (PHO)
The December Phoenicids form a periodic meteor shower that only rarely produces noticeable activity. Historically, the only truly impressive display occurred in 1956, when reported Zenithal Hourly Rates (ZHR) reached around 100 meteors per hour, a remarkable burst that has never been matched since. Most years, this shower is weak enough that many casual observers see little or nothing from it.
The usual activity period for the Phoenicids runs from December 1 to December 5, with a maximum expected on December 1. At the time of peak, the radiant is located at right ascension 00:28 (7 degrees in RA) and declination -27 degrees. This spot lies in the northern part of the constellation Sculptor, about 8 degrees southwest of the bright second-magnitude star Diphda (beta Ceti) in Cetus. Because of the radiant’s southerly position, the shower is best placed in the southern sky shortly after evening twilight ends, especially for observers in the southern hemisphere.
Observers south of the equator are at a clear advantage for this shower, as the radiant climbs higher in their sky, bringing more meteors into view. By contrast, northern observers see the radiant much lower, reducing the number of visible meteors. With a relatively slow entry velocity of about 15 kilometers per second, Phoenicid meteors appear as extremely slow-moving streaks, which can actually be quite striking and easy to follow with the naked eye when they do occur. But here’s where it gets controversial: some enthusiasts still go out hopeful for a repeat of 1956, even though most years have been quiet.
Northern Taurids (NTA)
The Northern Taurids originate from a broad radiant region located in the constellation Taurus. The radiant lies in central Taurus, about 3 degrees east of the fourth-magnitude star tau Tauri, making it relatively easy to pinpoint with a star chart or planetarium app. This shower is known more for occasional bright fireballs than for high numbers of meteors.
To get the best view of the Northern Taurids, observers should face generally southward around local midnight (LST), when the radiant is well positioned above the horizon. Under typical conditions, this shower produces about 1 meteor per hour from the northern hemisphere, and less than 1 per hour from locations south of the equator. With an entry speed around 25 kilometers per second, Northern Taurid meteors show a medium-slow apparent velocity, often giving observers a bit more time to catch the streak.
November Orionids (NOO)
The November Orionids are active from November 13 through December 12, with their peak activity occurring around November 30. During this week, the radiant is located at right ascension 06:08 (92 degrees) and declination +16 degrees. This position places it in the northeastern part of the constellation Orion, roughly 1 degree north of the fourth-magnitude star nu Orionis.
The radiant of the November Orionids is best positioned in the northern sky at roughly 01:00 local standard time, when it stands highest above the southern horizon. At that time, expected hourly rates are around 3 meteors as seen from the northern hemisphere and about 2 meteors per hour from south of the equator, assuming dark skies and favorable conditions. The entry velocity is approximately 42 kilometers per second, so most meteors from this shower appear of medium speed—fast enough to be exciting but not so rapid that they vanish instantly.
Sigma Hydrids (HYD)
The sigma Hydrids are a lesser-known shower active from November 22 through December 31, with their maximum activity forecast for December 7. During the current period, the radiant is located at right ascension 07:52 (118 degrees) and declination +04 degrees. Interestingly, this puts it in central Canis Minor, about 3 degrees southeast of Procyon (alpha Canis Minoris A), a prominent zero-magnitude star that serves as an excellent landmark.
Around 03:00 local standard time, the sigma Hydrids radiant reaches its highest point above the southern horizon, making that the ideal time to observe them. The expected hourly rate is low—around 1 meteor per hour—regardless of whether you are in the northern or southern hemisphere. However, they have a high entry velocity of about 59 kilometers per second, so the meteors that do appear often look swift and striking, leaving quick, sharp trails across the sky.
Puppid–Velid Complex (PUP)
The Puppid–Velid Complex is not a single sharp radiant but a broad region containing many weak radiants in the constellations Puppis and Vela. Visual observations and photographic studies have identified numerous individual radiants in this area during November and December, which together form a complex pattern of overlapping meteor sources. When their combined activity is near maximum, this complex can reach a ZHR of about 10, though actual observed rates are typically lower for most observers.
Activity from the Puppid–Velid Complex begins around December 1 and continues until approximately December 15. The exact date of maximum is not firmly established, so December 7 is often used as a practical midpoint of the activity period. During this outlook, the center of activity is near right ascension 08:40 (130 degrees) and declination -44 degrees, a location in western Vela close to the fourth-magnitude star e Velorum. The shower is best observed around 04:00 local standard time, when the radiant stands highest in the southern sky.
Observers in the southern hemisphere are again favored for this complex, as the radiant climbs high above their horizon, making more of the meteors visible. For most northern hemisphere observers, the radiant stays low in the southern sky, so meteors that do appear tend to have long, low tracks and can persist noticeably as they move across the field of view. With an entry speed near 44 kilometers per second, Puppid–Velid meteors display an average apparent velocity, neither extremely fast nor especially slow.
Leonids (LEO)
The Leonids are one of the most famous meteor showers, active each year from October 27 to December 7, with a sharp maximum typically around November 17. During this part of the cycle, the radiant is located at right ascension 10:44 (161 degrees) and declination +17 degrees. This puts it in central Leo, about 2 degrees south of the faint star 51 Leonis, making the constellation a useful guide when hunting for Leonid meteors.
The Leonid radiant is best placed in the eastern sky during the last hour before morning twilight, when it is highest in a dark sky and conditions are best for catching any remaining activity. While Leonids are visible from the southern hemisphere, observing conditions are generally more favorable north of the equator, where the radiant climbs higher. At this stage in the shower, expected hourly rates are less than 1 meteor per hour from any location, but the meteors that do appear are typically very fast because of a high entry velocity of about 71 kilometers per second.
Sporadic Meteors
Sporadic meteors are those that cannot be clearly linked to any known or active meteor shower. Over long timescales, meteor streams spread out and weaken until they can no longer be recognized as organized showers, and many sporadics are remnants of this evolutionary process. Away from the peaks of major annual showers, these sporadic meteors make up most of the meteors seen on any random night, creating a steady background of activity.
From mid-northern latitudes around 45°N, a rural observer during the last hour before dawn can expect to see about 12 sporadic meteors per hour under good conditions. In the evening from the same locations, the rate is lower, around 2 sporadics per hour. From tropical southern latitudes near 25°S, the morning rate is typically around 8 sporadics per hour, dropping to about 1 per hour in the evening. Observers at latitudes between these examples can anticipate sporadic activity that falls between these ranges, with evening rates further diminished by moonlight when the Moon is bright.
Summary of Active Showers (Table Overview)
The following information is presented in tabular form in the original outlook to help visual observers quickly compare active showers that are within reach of the naked eye. For each shower, the table lists the date of maximum activity, the celestial coordinates of the radiant (right ascension and declination, with RA given both in hours/minutes and degrees), the approximate entry velocity in kilometers per second, the local standard time of culmination, the expected hourly rate for observers in the northern and southern hemispheres, and a class ranking indicating the overall intensity of the shower.
For Saturday night and Sunday morning, November 29–30, the table includes these showers:
- Phoenicids (PHO): Maximum around December 1, radiant at RA 00:28 (7°), Dec -27°, entry speed about 15 km/s, culminating near 01:00 LST, with hourly rates under 1 meteor for both north and south, rated Class III.
- Northern Taurids (NTA): Maximum around November 12, radiant near RA 04:56 (74°), Dec +24°, entry speed near 29 km/s, culminating around 01:00 LST, with about 1 meteor per hour from the north and fewer than 1 from the south, classified as Class II.
- November Orionids (NOO): Maximum around November 28, radiant at RA 06:08 (92°), Dec +16°, entry velocity about 44 km/s, culminating near 02:00 LST, with hourly rates of roughly 3 from the north and 2 from the south, also Class II.
- Sigma Hydrids (HYD): Maximum around December 9, radiant at RA 07:52 (118°), Dec +04°, entry speed near 59 km/s, culminating around 03:00 LST, with less than 1 meteor per hour from either hemisphere, classified as Class II.
- Puppid–Velids (PUP): Maximum around December 7, radiant near RA 08:40 (130°), Dec -44°, entry velocity about 44 km/s, culminating at roughly 04:00 LST, with rates under 1 meteor per hour north and south, assigned to Class II.
- Leonids (LEO): Maximum around November 17, radiant at RA 10:36 (159°), Dec +19°, high entry velocity near 70 km/s, culminating about 06:00 LST, with less than 1 meteor per hour expected from both hemispheres at this time, categorized as Class I.
Meteor Shower Class Scale
The class system is used to group meteor showers by their typical strength and reliability, especially in terms of their Zenithal Hourly Rate under ideal observing conditions. Class I showers represent the strongest annual events, with ZHRs typically around ten or more meteors per hour, making them the headline showers most observers plan for each year. Class II showers are solid, minor showers that consistently produce noticeable activity, with ZHRs usually ranging from about two to ten.
Class III showers are more irregular and do not show significant activity every year. They are often weak or absent in many seasons but retain the potential to generate major outbursts under special conditions, as has been hinted at for some historic events. Class IV showers are very weak minor sources, with ZHRs rarely exceeding about two meteors per hour; studying these faint showers is usually best left to experienced observers who employ careful plotting, timing, and angular velocity measurements to determine whether an individual meteor belongs to a particular shower.
Because Class IV showers produce so few visible meteors, they are also attractive targets for video and photographic work, where long exposures and sensitive sensors can collect more data than the human eye. Beginners are generally encouraged to focus on showers rated Class I to III, where the activity is stronger and the connection between what is seen and the shower predictions is easier to recognize. But here’s where opinions can differ: some dedicated meteor fans argue that chasing faint Class IV showers is where the real scientific fun begins, while others feel beginners should stick to brighter, more dramatic events.
Now it’s your turn: given these conditions—bright Moon, modest shower activity, and the contrast between northern and southern hemisphere views—would you still head out to watch this week’s meteors, or do you prefer to wait for stronger, darker-sky events? Do you agree that even a weak shower can be worth it for the experience, or do you think forecasts like this tend to overhype modest activity? Share your thoughts and let the debate begin.
