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Although moonlight reduces the number of meteors visible, it does illuminate the landscape allowing impressive scenes like this to be captured. Here we have a bright Perseid meteor captured over the outskirts of Tucson, Arizona. Thanks to veteran astrophotographer Eliot Herman for sharing this outstanding desert vista with us! ©Eliot Herman

Meteor activity increases in October when compared to September. A major shower (the Orionids) is active all month long and there are also many minor showers to be seen. Both branches of the Taurids become more active as the month progresses, providing slow, graceful meteors to the nighttime scene. The Orionids are the big story of the month reaching maximum activity on the 22nd. This display can be seen equally well from both hemispheres which definitely helps out observers located in the sporadic-poor southern hemisphere this time of year. Sporadic activity is still good as seen from the northern hemisphere. In the southern hemisphere though, the sporadic activity is near its annual nadir.

During this period the moon reaches its new phase on Saturday September 28th. At this time the moon will be located near the sun and will not be visible at night. As the week progresses the waxing crescent moon will enter the evening sky but will not interfere with viewing meteor activity as it sets long before the more active morning hours arrive. The estimated total hourly meteor rates for evening observers this week is near 4 for those viewing from the northern hemisphere and 3 for those located south of the equator. For morning observers the estimated total hourly rates should be 13 as seen from mid-northern latitudes (45N) and 8 as seen from tropical southern locations (25S). 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 28/29. 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.
These sources of meteoric activity are expected to be active this week.

We are now encountering inbound debris from comet 2P/Encke, which has a radiant superimposed upon the anthelion radiant. Since it has been shown that meteors from 2P/Encke are more numerous we will recognize this activity as the Taurids. There are two distinct radiants for the Taurids. The activity profile for the Southern Taurids is unusual in that there are several peaks and valleys throughout the activity period. The difference between the peaks and valleys is not great, but definitely noticeable in video data. These peaks occur near October 10, October 29 through November 3, and near November 15th. After this last peak activity slowly wanes and eventually disappears by Christmas. The Northern branch reaches maximum near November 3rd and remains in a plateau-like peak for about 10 days. After November 12th activity slowly wanes and disappears about a week before Christmas. See the charts and table below for positions of these radiants.

The September Epsilon Perseids (SPE) are active from September 3 through October 3 with the peak occurring on September 11th. The radiant is currently located at 04:40 (070) +41. This position lies in eastern Perseus near the spot occupied by the 4th magnitude star known as 58 Persei. The radiant is best placed near 0500 local ssummer time (LST), when it lies highest above the horizon. Rates are expected to be less than 1 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 04:49 (072) +17. This area of the sky lies in central Taurus, 3 degrees east of the 1st magnitude orange star known as Aldebaran (alpha Tauri). The radiant is best placed near 0500 LST, when it lies highest above the horizon. Current hourly rates would be near 2 per as seen from the northern hemisphere and 1 as seen from south of the equator. With an entry velocity of 67 km/sec., most activity from this radiant would be of swift speed.

The first members of the epsilon Geminids (EGE) are expected this week. This source is active from September 30 through October 25 with maximum activity occurring on October 11. The radiant is currently located at 05:23 (080) +28, which places it in northeastern Taurus near the spot occupied by the bright 2nd magnitude star known as El Nath (beta Tauri). 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 less than 1 per hour no matter your location. With an entry velocity of 70 km/sec., most activity from this radiant would be of swift speed.

The nu Eridanids (NUE) were co-discovered by Japanese observers using SonotoCo and Juergen Rendtel and Sirko Molau of the IMO. Activity from this long-period stream stretches from August 24 all the way to November 16. Maximum activity occurred on September 24th. The radiant currently lies at 05:28 (082) +07, which places it in northern Orion, 1 degree east of the 2nd magnitude star known as Bellatrix (gamma Orionis). This area of the sky is best seen during the last dark hour before dawn when the radiant lies highest in a dark sky. Current rates are expected to be near 1 per hour during this period no matter your location. With an entry velocity of 67 km/sec., the average meteor from this source would be of swift velocity.

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 currently located at 10:16 (154) -02. This position lies in central Sextans, 2 degrees southeast of the 4th magnitude star known as alpha Sextantis. 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 mid-northern hemisphere (45N) one would expect to see approximately 10 sporadic meteors per hour during the last hour before dawn as seen from rural observing sites and 3 per hour during the evening hours. As seen from the tropical southern latitudes (25S), one would expect to see 7 sporadic meteors per hour during the last hour before dawn as seen from rural observing sites. Evening rates would be near 2 per hour. Locations between these two extremes would see activity between the listed figures.

The list below offers the information from above in tabular form. Rates and positions are exact for Saturday night/Sunday morning except where noted in the shower descriptions.
SHOWER DATE OF MAXIMUM ACTIVITY CELESTIAL POSITION ENTRY VELOCITY CULMINATION HOURLY RATE CLASS
RA (RA in Deg.) DEC Km/Sec Local Summer Time North-South
Northern Taurids (NTA) Nov 03 00:56 (014) +12 28 02:00 1 - <1 II
Southern Taurids (STA) Oct 10 01:13 (018) +05 27 02:00 1 - 1 II
September Epsilon Perseids (SPE) Sep 11 04:40 (070) +41 65 05:00 <1 - <1 II
Orionids (ORI) Oct 22 04:49 (072) +17 67 05:00 2 - 1 I
epsilon Geminids(ORI) Oct 11 05:23 (080) +28 70 06:00 <1 - <1 II
nu Eridanids (NUE) Sep 24 05:28 (082) +07 67 06:00 1 - 1 IV
Daytime Sextantids (DSX) Sep 29 10:16 (154) -02 33 11:00 <1 - <1 IV
Zgodnie z:
Robert Lunsford


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