September offers longer nights and cooler
temperatures in the northern hemisphere. In the sky, no major showers are visible
from either hemisphere but the northern hemisphere enjoys the advantage of higher
sporadic rates. The two recognized minor showers active in early September have
high northern declinations (celestial latitude) therefore are much better suited
to be viewed from locations north of the equator. During the second half of the
month the antihelion radiant becomes entangled with the two Taurid radiants and
it is impossible to separate them. Therefore the antihelion radiant will be excluded
from the list from the second half of September until the end of the Taurid activity
period late in November. Observers in the southern hemisphere suffer from some of
their lowest rates of the year this month. The Taurid radiants are not too badly
placed so observers south of the equator can expect to see a little of this activity
toward the end of the month.

During this period the moon reaches its last
quarter phase on Saturday the 12th. At this time the moon will rise near 0100 LDT
(Local Daylight Time) and will remain in the sky the rest of the night. This will
create some lunar interference which can be easily overcome by observing with the
moon at your back. As the week progresses the moon wanes and rises later each
morning. Thus conditions improve with each passing night. The estimated
total hourly rates for evening observers this week is near four as seen from the
northern hemisphere and three from the southern hemisphere. For morning observers the
estimated total hourly rates should be near sixteen from the northern hemisphere and
seven as seen from the southern hemisphere. 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. Morning rates are reduced
by moonlight this week.

The radiant positions and rates listed below are exact
for Saturday night/Sunday morning September 12/13. 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.

The following showers are expected to be active this week:


Recent video studies by Sirko Molau have revealed that activity from the Southern
Taurids (STA)
is actually detectable beginning on September 7th. So for now until
December 10th, the Taurid radiants will replace the Antihelion source since they
overlap. The large Southern Taurid radiant is now centered at 00:38 (010) +04. This
area of the sky lies on the Pisces/Cetus border, five degrees southwest of the fourth
magnitude Delta Piscium. The radiant is large so that any meteor from Pisces, northern
Cetus, northeastern Aquarius, or southwestern Pegasus could be a candidate for this
shower. This radiant is best placed near 0200 LDT when it lies on the meridian and
is located highest in the sky. Maximum activity is not until October 10th so current
rates should be near three no matter your location. With an entry velocity of 29 km/sec.,
the average Southern Taurid meteor would be of medium-slow speed.


The same study of video radiants by Molau has revealed a radiant in Eridanus active
from September 3rd through the 23rd. Maximum activity occurred on September 6th.
The Nu Eridanid (NUE) radiant is currently located at 04:44 (071) +03. This
position is located on the Orion/Eridanus border, two degrees west of the fourth
magnitude star known as Pi 5 Orionis. The radiant is best placed near 06:00 LDT
when it lies highest in the sky. Hourly rates are expected to be near one, no matter
your location. At 68 km/sec., these meteors are swift with the brightest members
often exhibiting persistent trains.


As seen from the mid-northern hemisphere (45N) the Sporadic rates are
becoming more active. One would expect to see approximately twelve random meteors
during the last hour before dawn from rural observing sites and three per hour
during the evening hours. As seen from the mid-southern hemisphere (45S) morning
rates would be near three per hour as seen from rural observing sites and two
per hour during the evening hours. Locations between these two extremes would see
activity between the listed figures. Morning rates are reduced by moonlight.

The table below presents a summary of the expected activity this week. Rates and
positions are exact for Saturday night/Sunday morning September 12/13, but may be
used all week.

SHOWER DATE OF MAXIMUM ACTIVITY CELESTIAL POSITION ENTRY VELOCITY CULMINATION HOURLY RATE CLASS*     RA (RA in Deg.) DEC Km/Sec Local Daylight Time North-South  
             
Southern Taurids (STA) Oct 10 00:38 (010) +04 29 02:00 3 – 3 II
Nu Eridanids (NUE) Sep 06 04:44 (071) +03 68 06:00 1 – 1 IV

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