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				Large Alt-Az Telescope Forum
 Presentations, Panel Discussion, and Walkabout
 
				Friday, August 13, 1:00-3:30 PM, 
				Oregon Star Party 2010  
				Amateur telescope makers have broken the 1-meter telescope 
				barrier, and are now rapidly heading toward 1.5 and even 2.0 
				meter portable telescopes. OSP2010 will feature large alt-az 
				telescope forum consisting of a number of short PowerPoint 
				presentations, a panel discussion, and a special Mel Bartels 
				guided large scope walkabout.  The key to large aperture 
				portable telescopes is, of course, affordable lightweight 
				mirrors, and advances are being made in meniscus, foam glass, 
				spun epoxy and other mirror technologies.  Advances in other key 
				areas include direct drive motors and controllers (no gears, 
				belts, or friction rollers) and large telescope portability.  
				While some portable large alt-az telescopes will be used for 
				stunning visual observations—deep observing—others will be 
				non-imaging “photon funnels” used either signally or in arrays 
				for light bucket photometric or spectroscopic observations. 
				 Oregon Star Party 
				2010 Science Workshop
 The Oregon Star Party 
				(OSP) 2010 Science Workshop will feature quantitative 
				measurements of visual double stars with both equatorial and 
				Dobsonian telescopes equipped with Celestron Micro Guide 
				astrometric eyepieces, followed by analysis of the observations 
				and preparation of a paper for publication in the Journal of 
				Double Star Observations (JDSO). The star party workshop is 
				based on a one-weekend research seminar held at Pine Mountain 
				Observatory during the last two summers (Genet et al 
				2010). Russ Genet and Jo Johnson will introduce small telescope 
				science and visual double star observations in a general 
				interest one hour session on Thursday (2:00 PM). This will be 
				followed by a one-hour “how to” working session for workshop 
				participants led by Jo. Observations will be made that night, 
				the data will be analyzed on Friday, and a paper prepared for 
				publication. A general interest, one hour wrap-up/summary 
				PowerPoint presentation will be given on Saturday at 1:00 PM 
				describing how this pioneering workshop went and the scientific 
				results. To our knowledge, this will be the first ever science 
				workshop at a major star party with observational results 
				published in a scientific journal. Double stars make 
				particularly excellent targets for both students and amateur 
				astronomers. The concepts, mathematics, and observations 
				involved are straightforward. To measure the angular separation, 
				the observer needs to measure the scale constant for the linear 
				scale of the eyepiece in arc seconds per division via a drift 
				calibration, count the number of divisions between the primary 
				and secondary stars, and multiply the number of divisions by 
				this scale constant. Position angle is measured relative to the 
				north celestial pole by aligning the stars along the linear 
				scale and allowing the primary star to drift from the center of 
				the eyepiece to an outer protractor. A small correction is 
				needed to calculate the position angle when the Celestron 
				Micro-Guide eyepiece is used (Teague 2004). Most double star 
				researchers try to answer two questions: 1) is the double star 
				an optical, coincidental line-of-sight double or a 
				gravitationally bound binary system? 2) if the double star is a 
				binary, what are masses of the two components? To answer the 
				first question, astronomers look at the stars' two dimensional 
				proper motion vectors and trigonometric parallax (Arnold 2010). 
				To answer the second, astronomers use Isaac Newton's version of 
				Johannes Kepler's Third Law.  Although answering these questions 
				usually requires observations spread over many years, each 
				individual observation adds to the final solution.  The 
				individual observations, published in the in the Journal of 
				Double Star Observations, are additionally published in the
				Washington Double Star Catalog maintained by the US Naval 
				Observatory, adding to some two centuries of visual double star 
				observations.             The equipment 
				required to make scientifically useful visual double star 
				observations is affordable, as only a telescope, astrometric 
				eyepiece, and simple stop watch are needed. Quality observations 
				have been made on telescopes as small as three inches (Grisham 
				2008). There are two common laser-etched astrometric eyepieces, 
				the Meade and Celestron, each of which cost around $150.  We 
				prefer the Celestron eyepiece as its double, slightly spaced 
				apart “ruler” allows dimmer stars to be seen with precision 
				between the two rulers.             Finally, the 
				Journal of Double Star Observations offers swift, quality 
				publication which allows students and amateur astronomers to 
				experience both technical science writing and peer review. Many 
				experts in the field are willing to offer advice and collaborate 
				which helps neophytes complete their analysis and paper. The 
				research and science writing experience is directly applicable 
				to master’s theses, dissertations, and executive summaries. Agenda Thursday 12 AugustIntroduction to Small Telescope Science and Visual Double Star 
				Observations (main tent)
 Everyone is invited to get a feel for what this is all about.
 2:00-3:00   Overview:  Small Telescopes & 
				Astronomical Research, Russ Genet & Jo Johnson.3:00-4:00   Tutorial: How to Measure Visual Double Stars, Jo 
				Johnson
  Working Sessions for Visual Double Star 
				Teams (only)Thursday 12 August
 5:00-7:00   Get acquainted dinner together, 
				final formation of teams.7:00-9:00   Group tutorial observations demonstrating the 
				process by team leaders
 9:00-Late   Team observations of assigned double stars
 Friday 13 AugustWorking Sessions for Visual Double Star Teams (only)
 Late morning (to be arranged)   Data analysis
 Afternoon   Complete data analysis, draft 
				paper(s)Evening   Group dinner, polish papers, discuss exit briefing
 
 Saturday 14 August
 Morning (to be arranged)   Finalize exit PowerPoint briefings
 Saturday 14 AugustOSP2010 Science Workshop Results (main tent)
 Everyone is invited to hear the research results from the teams
 1:00-2:00   Research team reports 
				(introduced & MCed by Jo Johnson) ReferencesArnold, Dave. 2010. Considering proper motion in the 
				analysis of visual double star observations. In
 Small Telescopes and Astronomical Research, eds. R. Genet, J 
				Johnson, V. Wallen. Santa Margarita, CA:
 Collins Foundation Press.
 Genet, Russell, Berry, Richard, Johnson, 
				Jolyon, and Frey, Thomas. 2010. Pine Mountain Observatory summer 
				research workshop. In Small Telescopes and Astronomical 
				Research, eds. R. Genet, J. Johnson, V. Wallen. Santa 
				Margarita, CA: Collins Foundation Press. Grisham, Darrell, Johnson, Jolyon, Genet, 
				Russell, and Arnold, David. 2008. Double star measurements with 
				a three inch Tasco telescope. Journal of Double Star 
				Observations, 4 (1),     10-13. Teague, Tom. 2004. Simple techniques of 
				measurement. Observing and Measuring Visual Double Stars, ed. Bob Argyle. London: Springer.
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