May is a fairly slow month for meteor activity.
The Eta Aquariids are very active the first two weeks of the month then fade as
the month progresses. The only other showers active this month are the Eta Lyrids
and the Antihelion radiant. These will add only 1-2 meteors per hour to the total
count. Sporadic rates are low but steady as seen from the mid-northern hemisphere
(45 N). Sporadic rates seen from the mid-southern hemisphere (45 S) continue
to rise this month toward a maximum in July.

During this period the moon waxes from a half
illuminated state to nearly full by the end. This weekend the waxing gibbous
moon sets during the early morning hours allowing a few hours of dark sky observing
between moonset and the start of morning twilight. Later in the period the nearly
full moon is above the horizon nearly the entire night making meteor observations
difficult. The estimated total hourly rates for evening observers this week is near
one as seen from the northern hemisphere and two for those situated south of the
equator. For morning observers the estimated total hourly rates should be near
twelve for those located in the mid-northern hemisphere (45 N) and twenty 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 reduced due to moonlight.

The radiant positions and rates listed below are exact
for Saturday night/Sunday morning May 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 wide Antihelion (ANT) radiant is now centered at 15:40 (235) -20. This
area of the sky lies in eastern Libra, five degrees northwest of the second
magnitude star Dschubba (Delta Scorpii). This radiant is best placed near 0200
LDT when it is located on the meridian and lies highest in the sky above the
horizon. Due to the large size of this radiant, any meteor radiating from
southeastern Libra, extreme eastern Hydra, southwestern Ophiuchus, or northwestern
Scorpius could be a candidate for this shower. Rates at this time should be near
two per hour as seen from the southern hemisphere and only one as seen from north
of the equator. With an entry velocity of 30km/sec., the average Antihelion meteor
would be of medium-slow speed.


The Eta Lyrids (ELY) are produced by comet IRAS-Araki-Alcock, which passed
very close to the Earth twenty six years ago this May. Weak activity from this
radiant has been seen in most years from May 6 through May 14, with maximum activity
occurring on May 10. Activity from this source will not be noticed until late in
this period when the radiant position will be located at 19:12 (288) +45. This
area of the sky is located in northeastern Lyra, five degrees west of the third
magnitude star Delta Cygni. The best time to view this activity is just before the
start of morning twilight, when the radiant lies highest in a dark sky. With an
entry velocity of 43 kilometers per second, a majority of these meteors will appear
to move at moderate speeds.


The video studies of Sirko Molau have revealed a weak radiant active in Cygnus
this time of year. The Xi Cygnid (XCG) radiant is currently located at
21:44 (326) +45. This area of the sky is located in eastern Cygnus, very
close to the fourth magnitude star Rho Cygni. Maximum activity occurred on
April 27 so current rates are expected to now be less than one per hour. These
meteors are best seen during the last dark hour before dawn, when the radiant
lies highest above the horizon in a dark sky. This shower is best seen from the
northern hemisphere, where the radiant lies high in the sky at dawn. At 44 km/sec.
the Xi Cygnids will usually produce meteors of medium velocity.


The Eta Aquariids (ETA) are particles from Halley’s Comet, produced in
Earth-crossing orbits many centuries ago. We pass closest to these orbits
from May 5 through the 9th. During this period the Eta Aquariids are at
their best, capable of producing ZHR’s of sixty. The actual visible rates
are most often less than half this figure due to the low altitude of the
radiant at dawn. Observed hourly rates at maximum normally vary from zero at
60 degrees north latitude to 25 near the equator and back down to near zero
again in Antarctica, where the radiant elevation is very low. Hourly rates this
weekend are anywhere from zero to five per hour depending on your latitude and
observing conditions. Rates will increase significantly as the week progresses
as we approach the May 7 maximum. The radiant is currently located at 22:20 (335) -02.
This area of the sky is located in northern Aquarius, just south of the fourth
magnitude star Gamma Aquarii. The best time to view this activity is just
before the start of morning twilight, when the radiant lies highest in a
dark sky. No matter your location these meteors will appear from the eastern
sky and shoot in all directions. If the radiant has sufficient altitude Eta
Aquariid meteors can also be seen shooting down toward the eastern horizon.
With an entry velocity of 68 kilometers per second, a majority of these
meteors will appear to move swiftly with a high percentage of the bright
meteors leaving persistent trains. More tips on viewing the 2009 Eta Aquariids are
available at: http://www.amsmeteors.org/showers.html#ETA


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

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.

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  
             
Antihelion (ANT) 15:40 (235) -20 30 02:00 1 – 2 II
Eta Lyrids (ELY) May 10 19:12 (288) +45 43 05:00 <1 - <1 II
Xi Cygnids (XCG) Apr 27 21:44 (326) +45 44 07:00 <1 - <1 IV
Eta Aquariids (ETA) May 7 22:20 (335) -02 68 08:00 5 – 5 I

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