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Science with Your Telescope Brian D. Warner Palmer Divide Observatory http://www.MinorPlanetObserver.com Space Science Institute http://www.SpaceScience.org Science is Fun! • You can use what you already have • Expands your knowledge • Professionals depend more, not less, on amateur observations • Satisfaction of collaborations and publication Asteroid Lightcurves at The Palmer Divide Observatory Why Do Asteroid Lightcurves? • Correlation between size and period. • Slow rotators - what about them is common? • Size, shape, pole orientation • Size, shape, pole orientation • Additional observations in support of radar observations • Remove observational bias towards brighter, main belt asteroids, i.e., increase statistical sampling The Palmer Divide Observatory 20” 14” The Palmer Divide Observatory 0.35m LX-200GPS North: FLI-1001E - unfiltered South: ST-9E, f/5.0 reducer, VRC 0.5m f/8.1 Ritchey-Chretien FLI-1001E (1Kx1Kx24m) FLI filter wheel - BVRC 80mm/ST-237 guiding The Palmer Divide Observatory A Typical Night • Select targets • Open observatories • Write scripts • Start runs • Download images during/after runs • Measure images and analyze data A Typical Night • Works 2 asteroids • Periodically syncs • Periodically focuses • Shuts down camera • Homes scope A Typical Night • Measure images with MPO Canopus • Plot raw data and look for obvious outliers • Do Period Search with MPO Canopus Fourier analysis Follow up • Merge multiple nights • Do Period Search on combined data set It’s Not Always Pretty! Binary Asteroids Initial Discovery at PDO (Oct. 2004 - present) 3309 5477 5905 9069 34706 76818 Brorefeld 1989 UH2 Johnson Hovland 2001 OP83 2000 RG79 Results - Hungarias From Harris Lightcurve List (August 2006) • Total Number: 70 • PDO (primary): 49 (70%) • Spin Rate Distribution: – Two peaks – Less “Spin barrier” effect versus NEO population Results - Hungarias Publishing Your Work The Minor Planet Bulletin • Published quarterly by Minor Planets Section of ALPO. • Best place for amateurs to submit. • Juried publication, in many professional libraries around the world (good PR for school programs) • Inexpensive: FREE! http://www.MinorPlanetObserver/mpb/default.htm Data Mining Asteroid Images Variable Star Search Data Mining Asteroid Images Variable Star Search Data Mining Asteroid Images Variable Star Search Data Mining Asteroid Images Data Mining Asteroid Images Binary Stars Modeling Binary Stars Binary Maker 3 http://www.binarymaker.com Modeling Binary Stars Binary Maker 3 Mass ratio input = 1.500000 Omega 1 = 4.439516 Omega inner = 4.526136 Fillout 1 = 0.150000 mass ratio < 1 = 0.666667 Omega 2 = 4.439516 Omega outer = 3.948668 Fillout 2 = 0.150000 Surface area 1 Volume 1 Mean radius 1 Temperature 1 Luminosity 1 Inclination Surface area 2 Volume 2 Mean radius 2 Temperature 2 Luminosity 2 = = = = = = 2.298928 0.321256 0.426171 5400.00 0.4662 72.000 = = = = = 1.612613 0.186599 0.355198 6000.00 0.5338 Variable Stars (Visual/CCD) American Association of Variable Star Observers (AAVSO) http://www.aavso.org Double Stars • Easy to do with CD/DSLR/Webcam equipment • Many targets in one night • Help is needed on neglected stars Double Stars Washington Double Star Catalog (WDS) http://ad.usno.navy.mil/wds/wds.html Yahoo News Group http://groups.yahoo.com/group/binary-stars-uncensored/ Double Stars aa / da RA / Dec of the primary ab / db RA / Dec of the secondary Double Stars Double Stars Publishing Your Results Journal of Double Star Observations http://www.jdso.org/ The Webb Society Double Star Circulars http://www.webbsociety.freeserve.co. uk/notes/doublest01.html Science is FUN! Society for Astronomical Sciences http://www.SocAstroSci.org Acknoweldgements Funding for this research was provided by: NASA grant NNG06GI32G NASA grant NNX06AB30G NSF grant AST-0607505