Meteor Activity Outlook for August 2-8, 2008

Meteor activity kicks into high gear in August as
seen from the northern hemisphere. The main reason for all this activity is the
Perseid shower that peaks on August 12. The shower is active most of the month
and remains above the level of the sporadic background for a week centered on
August 12. The sporadic activity is also increasing as seen from the northern
hemisphere and is now nearly double the rates from just three months ago. As seen
from south of the equator, meteor rates are still decent but falling rapidly. The
sporadic rates seen at the beginning of the month will be twice as much as those
seen during the last days of the month. The Perseid radiant does not rise high
into the sky as seen in the southern hemisphere so rates from this shower are
greatly reduced when compared to the northern hemisphere.

During this period the moon reaches its first
quarter phase on Friday August 8th. At that time the moon will be located ninety
degrees east of the sun and will set near 0100 local daylight time (LDT). This
weekend the waxing crescent moon will set soon after the end of evening twilight
and will not interfere with observing. As seen from the mid-northern hemisphere
(45 N) the estimated total hourly rates during the evening observers would be near
three. For morning observers the estimated total hourly rates should be near twenty
four. For those located in the mid-southern hemisphere (45 S) morning rates would
also be near twenty four and evening rates near three. Locations between these two
extremes would see activity between the listed figures. These rates assume that you
are watching from rural areas away from all sources of light pollution. 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 August 2/3. 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:

The Kappa Cygnids (KCG) are active from a wide radiant located at 18:52
(283) +58. This position is located in southern Draco, four degrees
northwest of the fourth magnitude star Kappa Cygni. Current rates would be
near one shower member per hour. With an entry velocity of 25 km/sec. most
of these meteors will appear to travel slower than average. The radiant is
best placed near 2300 Local Daylight Time (11pm LDT) when it lies nearly
overhead for much of the Northern Hemisphere. Due to its high northern
declination this activity is not well seen from the Southern Hemisphere.

The Alpha Capricornids (CAP) are active from a wide radiant
located at 20:44 (311) -8. This position lies in western Aquarius, two degrees
northwest of the fourth magnitude star Epsilon Aquarii. The radiant is best placed
near 0100 local daylight time (LDT), when it lies on the meridian and is highest
in the sky. Current rates would be near one per hour for those in the northern
hemisphere and two as seen from the southern hemisphere. Don’t confuse these meteors
with the nearby antihelion meteors, which have a radiant just to the east. Both
radiants need to be in your field of view to properly sort these meteors. With an
entry velocity of 23 km/sec., most activity from this radiant would be slow, a bit
slower than the antihelions. This radiant is well seen except for far northern
latitudes where it remains twilight all night long and the radiant does not rise
as high into their sky.

The large Antihelion (ANT) radiant is now centered at 21:32 (323) -13.
This area of the sky lies in northeastern Capricornus, four degrees northwest of the
third magnitude star Delta Capricornii. Actually any meteor from eastern Capricornus
as well as western Aquarius, could be a candidate for this shower. This radiant
is best placed near 0200 LDT when it lies on the meridian and is highest in the
sky. Rates at this time should be near two for northern observers and three for
observers south of the equator. With an entry velocity of 30 km/sec., the average
Antihelion meteor would be of medium-slow speed.

The Delta Aquariids (SDA) are still active from a radiant at 22:52 (343)
-15. This position lies in southwestern Aquarius, very close to the third magnitude
star Delta Aquarii. The radiant is best placed near 0300 LDT, when it lies highest
in the sky. Current rates would range from two to five shower members per hour,
depending on your latitude. With an entry velocity of 41 km/sec., most activity from
this radiant would be of average velocities. These meteors tend to be faint so the
darkest skies are necessary in order to see this shower well.

The Pisces Austrinids (PAU) is a weak shower with a radiant is located at
23:04 (346) -28. This area of the sky lies in western Piscis Austrinus, just
northeast of the bright star Fomalhaut (Alpha Piscis Austrini). These meteors
are best seen near 0300 LDT, when the radiant lies highest above the horizon. One
can expect rates near one per hour from the southern hemisphere and less than one
from the north. At 35/km per second, these meteors are of average velocity, slower
than the Aquariids but faster than the Alpha Caps and the antihelion meteors.

Perseid (PER) activity is now near five per hour as seen from the northern
hemisphere. These rates will increase gradually as we approach the peak on the
morning of August 12. The current radiant position lies at 02:16 (034) +55,
which is located in extreme northwestern Perseus, just two degrees south of the
famous “Double Cluster”. The nearest easily seen star is Eta Persei which lies
six degrees to the northeast. The radiant is well placed for those in the
northern hemisphere during the last few hours before dawn. Due to the high northern
declination (celestial latitude) of the radiant, rates seen from the Southern
Hemisphere are very low when compared to those seen north of the equator. At 59
km/sec., Perseid meteors are swift, often exhibiting persistent trains. More
details on viewing the Perseid meteor shower are available at:
http://www.amsmeteors.org/showers.html#PER

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 eleven per hour as seen from rural observing sites and three
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 but may be used all week.