Meteor Activity Outlook for February 28-March 6, 2009

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 first 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 Wednesday March 4th. At this time the moon lies ninety degrees
east of the sun in the and sets near midnight. During this entire period the more
active morning hours are free from lunar interference. The estimated total hourly
rates for evening observers this week is near two as seen from the northern
hemisphere and three for those situated south of the equator. For morning observers
the estimated total hourly rates should be near ten for those located in the
mid-northern hemisphere (45 N) and fourteen for those viewing from the mid-southern
hemisphere (45 S). 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. Evening rates are slightly reduced
due to lunar interference.

The radiant positions and rates listed below are exact
for Saturday night/Sunday morning February 28/March 1. 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 weak Delta Leonids (DLE) reached maximum on Wednesday February 25th.
Visual rates are currently less than one per hour, no matter your location. The
radiant is now located at 11:28 (172) +15. This area of the sky lies in eastern
Leo between two fairly bright stars, Denebola (Beta Leonis) and Theta Leonis.
This radiant is best placed near 0100 local standard time when it lies on the
meridian and is highest in the sky. With an entry velocity of 23 km/sec., the
average Delta Leonid meteor would be of slow speed. Do not confuse these meteors
with the overlapping Antihelion radiant, whose center lies thirteen degrees to
the south. To separate these meteors, the observer must be facing in a direction
that allows both radiants to be included within your field of view.

The wide Antihelion (ANT) radiant is now centered at 11:32 (173) +02. This
area of the sky lies in southeastern Leo, five degrees west of the fourth magnitude
star Beta Virginis. This radiant is also best placed near 0100 LST. Due to the
large size of this radiant, any meteor radiating from southeastern Leo, western
Virgo, or eastern Sextans 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 15:00 (225)
-51. This area of the sky is located in southern Lupus, two degrees northwest of
the third magnitude star Zeta Lupi. with the maximum not occurring until March 13th,
current visual rates would still be less than one shower member per hour, no matter
your location. These meteors are best seen between 0400 and 0500 local
standard time, 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 throughout most of the northern hemisphere. An occasional
shower member may be seen from the northern tropics, shooting upwards from the
southern horizon. At 56 km/sec. the Gamma Normids will usually produce meteors of
swift velocity.

As seen from the mid-northern hemisphere (45N) one would expect to see approximately
nine Sporadic meteors per hour during the last hour before dawn as seen
from rural observing sites. Evening rates would be near two per hour. As seen from
the mid-southern hemisphere (45S), morning rates would be near twelve 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. Evening
rates are slightly reduced due to lunar interference.

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.