Meteor Activity Outlook for July 6-12, 2007

For observers in the northern hemisphere meteor activity finally picks up in July after months of low rates. Several showers become active this month and peak toward the end of the month. Sporadic activity increases with each passing week throughout the northern summer. Activity seen in the southern hemisphere is peaking and will remain strong throughout the month. Later in the month strong minor shower activity will offset the falling sporadic rates in the south. Sporadic rates as seen from the southern hemisphere are highest early in the month, then fall quite steeply as the southern winter progresses.

During this period the moon reaches its last quarter phase on Saturday July 7. At this time the moon rises near 0100 local daylight time (LDT) and will remain in the sky the remainder of the morning. The moon becomes less of a factor with each passing night as it wanes toward its new phase. The estimated total hourly rates for evening observers this week is near two for those located north of the equator and four for observers south of the equator. For morning observers the estimated total hourly rates should be near nine for those located in the northern hemisphere and sixteen for those viewing from south of the equator. 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 due to moonlight.

The radiant positions listed below are exact for Saturday night/Sunday morning July 7/8. 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. Doing this 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 Alpha Capricornids (CAP) are active from a wide radiant located at 19:12 (288) -15. This position lies in eastern Sagittarius, four degrees east of the second magnitude star Nunki (Sigma Sagittarii). The radiant is best placed near 0100 local daylight time, when it lies highest in the sky. Current rates would be near one per hour, no matter your location. Don't mix these meteors with the more numerous 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. 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 Antihelion (ANT) radiant is now centered at 19:52 (298) -19. This area of the sky is located in a remote area of eastern Sagittarius, seven degrees southwest of the third third magnitude star Dabih (Beta Capricorni). 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 one per hour as seen in the northern hemisphere and two per hour for those located south of the equator. With an entry velocity of 30 km/sec., the average antihelion meteor would be of medium-slow speed.

Sirko Molau's study of video radiants has revealed activity during the period July 8-15, from an area in northwestern Aquarius. Maximum occurs on July 10 with the radiant located at 21:00 (315) -04. This position lies five degrees northwest of the third magnitude star Sadalsuud (Beta Aquarii). This radiant is best placed near 0300 LDT when it lies highest in the sky. It appears that nine percent of the total sporadic activity for the night is related to this radiant. This would equate to only 1-2 shower members per hour at best. With a bright moon in the sky, seeing any activity from this radiant would be difficult. At 40km/sec., the average meteor from this radiant would be of medium velocity.

The Delta Aquarids (SDA) are active from a radiant located at 21:32 (323) -20. This position lies in eastern Capricornus, close to the variable star Epsilon Capricornii. The radiant is best placed near 0300 local daylight time, when it lies highest in the sky. Current rates would be very low, especially with the moon still in the morning sky. 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. This shower peaks on July 28 with expected ZHR's near twenty.

Sporadic rates are now rising for observers in the northern hemisphere and are peaking for those located south of the equator. One would expect to see perhaps six random meteors during the last hour before dawn from rural observing sites located in the northern hemisphere. During the first dark hour after the end of evening twilight, perhaps two random meteors can be seen per hour. Sporadic rates increase as the night progresses so rates seen near midnight would be near four per hour. Late morning sporadic rates seen from the southern hemisphere are now near twelve per hour from rural observing sites. During the first dark hour after the end of evening twilight, perhaps four random meteors can be seen per hour, increasing to eight by midnight. Morning rates are reduced due to moonlight.