Meteor Activity Outlook for March 14-20, 2008

March is the slowest month for meteor activity.
No major annual showers are active and only two very weak minor showers produce
activity this month. The sporadic rates continue a slow decline as seen from the
mid-northern latitudes and mid-southern rates reach a fist half minimum. There
is not much to look forward to this month expect for the evening fireballs that
seem to peak this time of year from the northern hemisphere. This could be due to
the fact the antapex lies highest this time of year during the evening hours.

During this period the moon reaches its first
quarter phase on Friday March 14th. At this time the moon will be located 90 degrees
east of the sun and will set near 0100 Local Daylight Time or midnight Local Standard
Time. Toward the end of this period the moon will be in the sky most of the night
limiting dark skies to a short period just before dawn. As seen from the mid-northern hemisphere (45 N) the estimated
total hourly rates during the evening observers would be two. For morning observers
the estimated total hourly rates should be near eight. For those located in the
mid-southern hemisphere (45 S) morning rates would be near fifteen and evening
rates near two. 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. Evening rates are reduced due to moonlight.

The radiant positions and rates listed below are exact
for Saturday night/Sunday morning March 15/16. 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 wide Antihelion (ANT) radiant is now centered at 12:32 (188) -04. This
area of the sky lies in western Virgo, three degrees southwest of the third magnitude
star Porrima (Gamma Virginis). This radiant is best placed near 0200 LDT time
(0100 LST) when it lies on the meridian and is highest in the sky. Actually
any meteor from western Virgo, northern Corvus, or northeastern Crater could be a
candidate for this shower. Rates at this time should be near two per
hour no matter your location. With an entry velocity of 30 km/sec., the average
Antihelion meteor would be of medium-slow speed.

The Gamma Normids (GNO) are active from a radiant located at 16:04 (241)
-50. This area of the sky is located in central Norma, five degrees west of the
fourth magnitude star Gamma Normae. This shower peaked on the 13th so rates
are now slowly falling to near 1-2 per hour as seen from deep southern latitudes.
These meteors are best seen between 0500 and 0600 LDT (0400 and 0500 LST), when
the radiant lies highest above the horizon. This
shower is best seen from the southern hemisphere, where the radiant lies high in
the sky at dawn. Meteors from this shower are not visible north of 40 degrees
north latitude and also poorly seen in the most of the northern hemisphere. An
occasional member may be seen from the northern tropics. At 56 km/sec. the Gamma
Normids will usually produce meteors of swift velocity.

As seen from the mid-northern hemisphere (45N) the Sporadic rates are
still slowly falling. One would expect to see approximately eight random meteors
during the last hour before dawn from rural observing sites and two per hour
during the evening hours. As seen from the mid-southern hemisphere (45S) morning
rates would be near 12 per hour as seen from rural observing sites and two per
hour during the evening hours. Evening rates are reduced due to moonlight.

The table below presents a condensed version of the expected activity this week.
Rates and positions are exact for Saturday night/Sunday morning.