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(meteorobs) Meteor Activity Outlook for August 23-29, 2002



Meteor Activity Outlook for 
 August 23-29, 2002

By Robert Lunsford 
AMS Visual Program Coordinator

  The moon reaches its last quarter phase on Thursday August 31. With the moon's bright glare in the sky most of the night this week, meteor observing will be difficult and most likely unrewarding. The showers listed below are active during this period but will be difficult to observe. If your sky is transparent and the limiting magnitude exceeds +5.0 then you may be able to achieve some success at observing during this period. The estimated total hourly rates for evening observers this week should be near 3 for those viewing from the Northern Hemisphere and 2 for those located in the Southern Hemisphere. For morning observers the estimated total hourly rates should be near 5 for those located in the Northern Hemisphere and 3 for those in the Southern Hemisphere. 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. Morning rates are reduced by moonlight during this period.

The positions listed below are exact for Saturday night/Sunday morning August 24/25. The positions do not change greatly day to day so these positions may be used during this entire period. Most star atlases (available at science stores and libraries) 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 location. Meteor activity is not seen from radiants that are located below the horizon. The radiants below are listed in a west to east manner in order of right ascension (celestial longitude). The radiants listed first are located further west therefore are accessible earlier in the night while those listed last rise later in the night. This list also provides the order of ascending velocity for each radiant with those listed first usually being much slower than those last on the list. Velocity should not be the prime factor for shower association as all showers can produce slow meteors. Slow meteors can be produced from normally swift showers, such as the Leonids, when meteors appear near the radiant or close to the horizon. The true velocity is only revealed in shower members seen far from the radiant and high in the sky.

The detailed descriptions of each shower will return next week when moonlight becomes less of a factor.

Kappa Cygnids                   19:12 (288)  +60
North Iota Aquarids           22:08 (332)  -05
Antihelion                             23:04 (346)  -05
North Delta Aquarids        23:08 (347)  -02
Pi Eridanids                         03:20 (050)  -16
Gamma Doradids               03:52 (058)  -51

Northern Apex                    04:04 (061)  +36
Southern Apex                   04:04 (061)  +06
Perseids                               04:20 (065)  +60
Alpha Aurigids                    05:04 (076)  +42

Clear Skies!
Robert Lunsford
AMS Visual Program Coordinator