(meteorobs) Meteor Activity Outlook for September 19-25, 2009

[Robert Lunsford]

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 progresses from its new phase (Sep. 18) to
nearly half illuminated. This weekend the very thin waxing crescent moon
sets early in the evening and will not interfere with observing. As the week
progresses the moon sets later each night but will still set before the
active morning hours arrive. The estimated total hourly rates for evening
observers this week is near four as seen from the northern hemisphere and
two from the southern hemisphere. For morning observers the estimated total
hourly rates should be near seventeen 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.

The radiant positions and rates listed below are exact for Saturday
night/Sunday morning September 19/20. 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 00:56 (014) +05. This area of the sky lies in southern Pisces, three
degrees southeast 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 05:00
(075) +07. This position is located in western Orion, two degrees east of
the fourth magnitude star known as Pi 3 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 fourteen 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 four per hour as seen from
rural observing sites and one per hour during the evening hours. Locations
between these two extremes would see activity between the listed figures.

The table below presents a summary of the expected activity this week. Rates
and positions are exact for Saturday night/Sunday morning September 19/20,
but may be used all week.

Southern Taurids (STA)  - 00:56 (014) +05   Velocity - 29km/sec.
Northern Hemisphere - 3 per hr. Southern Hemisphere - 3 per hr.

Nu Eridanids (NUE) - 05:00 (075) +07   Velocity - 68km/sec.
Northern Hemisphere - <1 per hr. Southern Hemisphere - <1 per hr.

*For a detailed explanation on the different classes of meteor showers and
other astronomical terms, please visit:
http://www.amsmeteors.org/showers.html#X2009

Clear Skies!
Robert Lunsford
American Meteor Society