During this period the moon wanes from nearly half illuminated down to only a few percent by the end of the week. This weekend the waning crescent moon will rise during the early morning hours and will cause interference with viewing meteor activity. This can be overcome by observing areas of the sky free of lunar glare. By the end of the week the moon will not be a factor as it becomes slender and rises just before dawn. The estimated total hourly meteor rates for evening observers this week is near 4 as seen from mid-northern latitudes (45N) and 3 as seen from tropical southern locations (25S). For morning observers the estimated total hourly rates should be near 12 as seen from mid-northern latitudes (45N) and 10 as seen from tropical southern locations (25S). Rates during this period are slightly reduced during the morning hours due to moonlight. The actual rates will also depend on factors such as personal light and motion perception, local weather conditions, alertness and experience in watching meteor activity. Note that the hourly rates listed below are estimates as viewed from dark sky sites away from urban light sources. Observers viewing from urban areas will see less activity as only the brightest meteors will be visible from such locations.

The radiant (the area of the sky where meteors appear to shoot from) positions and rates listed below are exact for Saturday night/Sunday morning September 24/25 These positions do not change greatly day to day so the listed coordinates may be used during this entire period. Most star atlases (available at science stores and planetariums) will provide maps with grid lines of the celestial coordinates so that you may find out exactly where these positions are located in the sky. A planisphere or computer planetarium program is also useful in showing the sky at any time of night on any date of the year. Activity from each radiant is best seen when it is positioned highest in the sky, either due north or south along the meridian, depending on your latitude. It must be remembered that meteor activity is rarely seen at the radiant position. Rather they shoot outwards from the radiant so it is best to center your field of view so that the radiant lies at the edge and not the center. Viewing there will allow you to easily trace the path of each meteor back to the radiant (if it is a shower member) or in another direction if it is a sporadic. Meteor activity is not seen from radiants that are located below the horizon. The positions below are listed in a west to east manner in order of right ascension (celestial longitude). The positions listed first are located further west therefore are accessible earlier in the night while those listed further down the list rise later in the night.

Radiant Positions at 9pm LDT

Radiant Positions at 2100 Local Summer Time

Radiant Positions at 1am Local Daylight Saving Time

Radiant Positions at 0100 Local Summer Time

Radiant Positions at 5am LDT

Radiant Positions at 0500 Local Summer Time

These sources of meteoric activity are expected to be active this week.

Experienced observers are urged to be on the lookout for any activity from the October Capricornids (OCC). These meteors are possibly related to lost comet D/1978 R1 (Haneda-Campos). If the comet still exists it would reach perihelion in November 2016. A moderate display of bright meteors was seen from Australia on October 3, 1972. Other attempts at observing these meteors were less successful. With a favorable lack of moonlight in the evening sky during this period, observers are urged to monitor for any very slow meteors radiating from the border of Capricornus and Aquila near the position 20:06 (302) -09. This position is roughly 5 degrees northwest of the naked eye double star known as Algedi (alpha2 Capricorni). While the possible maximum is a week away, members of this stream may be visible this week from a position slightly west at 19:44 (296) -10. This position is best placed near 20:00 when the radiant lies highest above the horizon. While this area of the sky is fairly well placed for northern observers, it is much more favorably placed for those south of the equator where it lies much higher in the sky. Like the Daytime Sextantids mentioned below, any observations of these stream (either positive or negative) would be important to our understanding of these streams.

The Southern Taurids (STA) are active from a large radiant centered near 01:20 (020) +06. This position lies in southeastern Pisces, 4 degrees southeast of the 4th magnitude star known as epsilon Piscium. These meteors may be seen all night long but the radiant is best placed near 0200 local summer time (LST) when it lies on the meridian and is located highest in the sky. Rates at this time should be near 2 per hour regardless of your location. With an entry velocity of 29 km/sec., the average Southern Taurid meteor would be of slow velocity.

The September Epsilon Perseids (SPE) are active from the 5th through the 28th with the peak occurring on the night of September 8/9. The radiant is currently located at 04:32 (068) +42. This position lies in eastern Perseus, between the bright stars Capella (alpha Aurigae) and epsilon Persei. The radiant is best placed near 0500 LST, when it lies highest above the horizon. Rates are expected to be less than 1 per hour no matter your location. With an entry velocity of 65 km/sec., most activity from this radiant would be swift.

The Orionids (ORI) are active from a radiant located at 05:16 (079) +09, which places it in northwestern Orion, 4 degrees northwest of the 2nd magnitude star known as Bellatrix (gamma Orionis). This area of the sky is best placed in the sky during the last hour before dawn, when it lies highest above the horizon in a dark sky. Current rates would be near 2 per hour no matter your location. With an entry velocity of 67 km/sec., most activity from this radiant would be of swift speed.

The Daytime Sextantids (DSX) are not well known due to the fact that the radiant lies close to the sun and these meteors are only visible during the last couple of hours before dawn. The radiant is located at 10:00 (150) 00. This position lies in western Sextans, just west of the 4th magnitude star known as alpha Sextantis. This position is also 12 degrees south of the 1st magnitude star known as Regulus (alpha Leonis). This area of the sky is best placed in the sky during the last hour before dawn, when it lies highest above the horizon in a dark sky. Current rates would be most likely less than 1 per hour no matter your location. Spotting any of this activity would be a notable accomplishment. With an entry velocity of 33km/sec., most activity from this radiant would be of medium-slow speed.

As seen from the mid-northern hemisphere (45N) one would expect to see approximately 8 sporadic meteors per hour during the last hour before dawn as seen from rural observing sites. Evening rates would be near 3 per hour. As seen from the tropical southern latitudes (25S), morning rates would be near 6 per hour as seen from rural observing sites and 2 per hour during the evening hours. Locations between these two extremes would see activity between the listed figures. Morning rates are slightly reduced during this period due to moonlight.

The table below presents a list of radiants that are expected to be active this week. Rates and positions are exact for Saturday night/Sunday morning except where noted in the shower descriptions.

SHOWERDATE OF MAXIMUM ACTIVITYCELESTIAL POSITIONENTRY VELOCITYCULMINATIONHOURLY RATECLASS
RA (RA in Deg.) DECKm/SecLocal Summer TimeNorth-South
October Capricornids (OCC)Oct 0219:44 (296) -101520:00<1 – <1III
Southern Taurids (STA)Oct 1001:20 (020) +062902:002 – 2II
September Epsilon Perseids (SPE)Sep 904:32 (068) +426505:00<1 – <1II
Orionids (ORI)Oct 2205:16 (079) +096707:002 – 2I
Daytime Sextantids (DSX)Sep 2710:00 (150) 003312:00<1 – <1IV