| Mercury, 
              July/August 1996 Table of Contents 
              
 by 
              James C. White II, Middle Tennessee State University  (c) 
              1996 Astronomical Society of the Pacific 
               Every 
              August, Earth swings through the dusty path of Comet Swift-Tuttle. 
              The tiny grains of dust leap to their fiery deaths in our atmosphere 
              -- and we are witness to the year's finest meteor shower. 
              
               Comet 
              Hyakutake wowed us this spring [see Guest Observer, May/June, p. 
              11]. Comet Hale-Bopp teases us now for a potentially spectacular 
              show next spring. And have you forgotten the humiliation that Comet 
              Shoemaker-Levy 9 inflicted on mighty Jupiter two years ago? You 
              had better put on a helmet to protect yourself, because bits of 
              the sky are going to be falling soon. You guessed it: Another of 
              those darned comets is to blame! 
               I 
              exaggerate. Earth is indeed going to be pelted by cometary debris, 
              but don't worry. Instead, be happy. We north of the equator will 
              have a front-row seat for an annual astronomical spectacle. 
               From 
              about July 17 through Aug. 24, Earth will pass through the debris 
              spit out by Comet Swift-Tuttle. Like all comets, Swift- Tuttle is 
              a shameful litterbug, leaving a trail of dust and pebbles as it 
              orbits the Sun every 130 years. Each August, our planet crosses 
              this dust-strewn path. 
               Swift-Tuttle 
              last passed through the inner solar system in 1992, chucking a fresh 
              load of cometary cigarette butts, so a good show may be in store 
              this year. The bits of material, most smaller than a grain of sand, 
              will plunge into our atmosphere at 59 kilometers per second (130,000 
              miles per hour) [see "The Stars Are Falling," March/April, p. 6]. 
              Because of our orbit around the Sun, the shooting stars will seem 
              to streak out from the direction of the constellation Perseus -- 
              hence the name Perseids. 
               Some 
              people were disappointed at last year's performance. Blame the bright 
              Moon: It drowned out all those faint meteors. This year, the Moon 
              won't interfere. Meteor-watchers estimate we'll see 200 meteors 
              per hour from dark locations. 
               In 
              recent years, meteor-watchers have noticed two peaks in the number 
              of Perseids per hour. The first is a burst of meteors which occurs 
              as Earth sails through a tight, dense stream of centuries-old debris. 
              Half a day later comes the second, "traditional" maximum. Asia and 
              Europe, brace yourselves for prime viewing of the first maximum 
              on the evening of Aug. 12. North America has the best vantage point 
              for the traditional maximum.  
              
             Observing 
              Guidelines  A 
              meteor shower is more than a show. It's an experience. All you need 
              is a clear sky and a willingness to sacrifice sleep. Find an open 
              space with a good view of the sky. Don't fret if you live in the 
              city; your cousins in the country, away from city lights, will have 
              a better view, but you will still be able to see plenty of meteors. 
              Once you have staked out your space, unfold that lounge chair or 
              blanket and crack open that thermos of hot chocolate. 
               The 
              best time to observe a meteor shower is after midnight, as your 
              nighttime location moves head-on into the path of the cometary debris. 
              You may see some non-Perseid meteors (so- called sporadic meteors) 
              before midnight. Perseid meteors will have trails that you can trace 
              back to a point in the sky near the lovely Double Cluster in Perseus 
              [see SkyTalk, p. C-4]. 
               As 
              observers, we are interested in the number of Perseids per time 
              interval. Recruit a viewing companion, and choose an interval whose 
              length you feel comfortable with. Why not try successive 15-minute 
              intervals, with short breaks in between? You must concentrate on 
              the sky during the intervals, and short (2- to 3-minute) breaks 
              between intervals give you a chance to stretch. 
               At 
              the beginning of each interval, have your companion record the time. 
              Then, simply lie there for 15 minutes, looking straight up, and 
              count. Each time you cry, "Meteor!" your observing buddy should 
              make a mark. Don't look away during these observations or else you'll 
              miss some. At the end of the interval, record the local time and 
              switch jobs with your companion. If you can't convince someone to 
              observe with you, use a tape recorder to record your time readings 
              and observations; you can add up your meteor counts later by playing 
              back the recording. 
               Complete 
              as many of the observing intervals as you care to; the more you 
              make, the more useful your data will be. Tabulate the number of 
              meteors observed per interval, and make sure to label the table 
              with the local time and date of each interval. 
               I 
              encourage you to begin your observations about a week before the 
              night of Aug. 11-12 and continue until about a week after. On each 
              evening of your observations, you should assess how bright the sky 
              is. To do this, estimate the magnitude of the dimmest star you can 
              see. Sky charts provide you with magnitudes of easily identified 
              stars. In Nashville, say, the faintest star may have a magnitude 
              of 4.0. In rural Tennessee, it may be 6.0. The brightness of the 
              sky will determine how many meteors you can see -- and will allow 
              us to compare counts from different locations. 
               If 
              you'd like to try something different, listen for meteors 
              using an FM radio [see "Falling Stars of August," May/June 1993, 
              p. 93]. 
               Incorporate 
              your observations into a document with the following information: 
              name of the project (such as, "Observing the Perseids"), your name 
              or the name of your group, latitude and longitude of the observing 
              location, mailing address, telephone number, and email address, 
              if available. In your report, please provide accurate time and date 
              information, as well as written commentary. 
               Please 
              submit your completed report by Sept. 30, 1996 by email to 2032694@mcimail.com 
              or by regular mail to John Isles, Attn: Guest Observers, 1016 Westfield 
              Drive, Jackson, Mich. 49203-3630. The selection committee will evaluate 
              the reports and choose the Guest Observer for the January/February 
              1997 issue. 
               JAMES 
              C. WHITE II is a professor in the Department of Physics and 
              Astronomy at Middle Tennessee State University in Murfreesboro. 
              His email address is jwhite@physics.mtsu.edu. 
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