290 likes | 539 Views
TURNING THE NVO INTO AN “EVO” An Educational Virtual Observatory. Larry Marschall Project CLEA Gettysburg College. NVO EPO Workshop, JHU/STScI, July 11, 2002. THE TWO PRIME DIRECTIVES IN DEVELOPING EDUCATIONAL MATERIALS. Consider your Audience Consider your educational objectives.
E N D
TURNING THE NVO INTO AN “EVO”An Educational Virtual Observatory Larry Marschall Project CLEA Gettysburg College NVO EPO Workshop, JHU/STScI, July 11, 2002
THE TWO PRIME DIRECTIVES IN DEVELOPING EDUCATIONAL MATERIALS • Consider your Audience • Consider your educational objectives
AUDIENCES FOR CLASSROOM MATERIALS • Students :Science Majors or Non-Science Majors? • Faculty: Trained Astronomers or Not? • Institutions: HS, 2 yr, 4 yr, Univ?
Example: Introductory College Level Astronomy • Who takes introductory astronomy in the US? • 200 – 250 K students/year; mostly non-science majors. • Who teaches introductory astronomy in the US? • Most classes are taught by instructors whose Ph.D. is NOT in astronomy.
EDUCATIONAL CONSIDERATIONS FOR LABORATORY EXERCISES DIRECTED AT NON-SCIENCE MAJORS • Keep it simple • Highlight fundamental astrophysical research techniques • Avoid “black boxiness” --- methods should be transparent to user.
EDUCATIONAL CONSIDERATIONS FOR LABORATORY EXERCISES DIRECTED AT PHYSICS AND ASTRONOMY MAJORS • Complexities and tricks can be included • Clever variations on basic techniques or exotic applications are acceptable • Avoid “black boxiness” --- methods should be transparent to user. • What about teaching data mining itself? Is “Data Mining” a black box?
An Example:PROJECT CLEAContemporary Laboratory Experiences in Astronomy • Laboratory exercises illustrating modern astronomical techniques • Designed for non-science majors, but adaptable. • Simulation of measurement process. • Modern digital data and analysis techniques, using, wherever possible, real data. • Modular: each module includes software, student workbook(s) technical guide. • Funded by Gettysburg College and the NSF
PROJECT CLEAContemporary Laboratory Experiences in Astronomy Project Staff • Larry Marschall: P.I.; Graphic Design and Manuals • Glenn Snyder: Software • P.Richard Cooper: Manager and Outreach Coordinator • Also Mike Hayden, Rhonda Good, Mia Luehrmann, Helenmarie Hofmann, Marcus Lieberman, • Students: Shawn Baker, Erin Walsh, Brin Finnigan, Julia Lynch, Lauren Jones, Michell Vojtush
PROJECT CLEAContemporary Laboratory Experiences in AstronomyDISSEMINATION • Freeware (to educational users). • Software and manuals downloadable from website: • http://www.gettysburg.edu/academics/physics/clea/CLEAhome.html • Users in all states and > 60 countries • Manuals available in Spanish, Italian, Dutch, Polish, Hebrew, Kiwi, ???
PROJECT CLEAContemporary Laboratory Experiences in AstronomyTRAINING • Workshops at AAPT Sectional meetings • Workshops at AAPT national meetings • For Physics faculty who are teaching Astronomy courses: 9-day workshops on Research Techniques in Astronomy, at Gettysburg and Green Bank: June 2000, 2001, and coming up: 2003 and 2004.
PROJECT CLEAContemporary Laboratory Experiences in AstronomyASSESSMENT • Pre and post concept tests available for downloading. • Satisfaction survey available on line. • Site visits by external evaluator. • Study of lab and non-lab classes by Gina Brissenden, University of Wisconsin.
EXERCISES FROM PROJECT CLEA (3) Collaboration over the LAN
THE SEARCH FOR OBJECT XA “Capstone” Exercise • Students are given the coordinates of an unknown object and a summary of identification criteria • Access to Optical, Radio, IR and X-ray telescopes & instruments: VIREO: The Virtual Educational Observatory • Carry out an observing program of their own design, identify type of object. • Measure its physical characteristics • Write report in specified format (Journal article, lab report, etc). • Note: The Object X database currently contains 20 million stars, 50,000 galaxies, 6000 qso’s, 20,000 asteroids, 1000 pulsars, 50 million IR sources. Under development: X-ray
THE SEARCH FOR OBJECT X and the Virtual Educational Observatory
GENERAL CONSIDERATIONSin making EVO’s from the NVO • SELECTED DATA SETS, not access to the entire database, is what is required • THE USER INTERFACE is of prime importance, and should be designed, if not created, by teachers. The advice and collaboration of the research community is essential, however. • BOTH DATA and PROCESSING can be distributed, but servers may have to handle the onslaught of classes rather than sporadic users.
WHAT’S NEXT FOR PROJECT CLEA? • X-Ray Astronomy: Integrating CHANDRA data via the web and DS-9 • OLEO: The On-Line Educational Observatory on the web • “I Can’t believe it’s not a real telescope” • Teacher’s guides and more alternative student manuals.
THENATIONAL VIRTUAL OBSERVATORYis the line between observation and simulation blurring?
Modern Astronomy uses digital spectra displayed graphically.
The CLEA WEBSITE: http://www.gettysburg.edu/academics/physics/CLEAhome.html