Interesting People mailing list archives
Grids for Kids - training the innovators of tomorrow (fwd)
From: Dave Farber <dave () farber net>
Date: Mon, 11 Aug 2003 08:11:33 -0400
Date: Mon, 11 Aug 2003 08:04:38 -0400 (EDT) From: chodge5 () utk edu To: Dave Farber <dave () farber net> This is something else you might be interested in forwarding to IP.....It's nice occasionally to hear about something that's *not* depressing. -c ---------- Forwarded message ---------- Date: Sun, 10 Aug 2003 16:24:47 -0400 (EDT) From: CAnet-NEWS () canarie ca Subject: [news] Grids for Kids - training the innovators of tomorrow For more information on this item please visit the CANARIE CA*net 4 Optical Internet program web site at http://www.canarie.ca/canet4/library/list.html -------------------------------------------[It has been long recognized that innovation is one of the prime drivers of increased productivity and economic growth. In turn, science and engineering education is one of the important contributors in the schooling and training of the innovators of tomorrow. Yet despite that well known connection, enrolment in science and engineering programs continues to decline and it still remains a challenge to entice larger representation from women and minority groups to enrol in these programs. Part of the problem is the difficulty in making science and engineering "real" and exciting for high school and university students.The following news article is a great example where researchers at universities and government labs are working with educators to build programs and programs where students can be participants in real scientific research projects. With the latest developments in networks, grids and peer to peer distributed computing, what some have come to call the Third Wave of the Internet, there is no reason why many other research programs could be expanded not only to tap into the computing resources at our schools, but also to engage and excite the bright young minds in leading edge research and discovery. Virtual astronomical observatories, remote access to electronic telescopes, protein matching, and digital transmission from telescopes like the Faulkes project are all early examples of the potential of this technology. For more examples please see http://www.canarie.ca/canet4/library/general/escience_jan2003.pptNational governments generally do not play much of a role in education which is usually a state or provincial responsibility. But national governments are usually the primary funders of most research in universities as well as government laboratories. National government could possibly play a critical role in the early stages of science and engineering education by facilitating and enabling a greater degree of involvement by researchers and students through programs like "Grids for Kids" using high speed networks and distributed peer to peer computing and many other related tools. National government labs have been the instrument of many different policy directions in the past from industrial development to solving regional disparity. Maybe now they can also have a role in addressing the critical challenge of science and engineering education from grade school through to university.The following Faulkes Telescope project is one great example of such activity. -- BSA]HE FAULKES TELESCOPE PROJECT NEWSLETTER #4 August 2003 - Introduction This is the fourth newsletter from the Faulkes Telescope Project and aims to give potential users of the telescopes up-to-date information on what is happening. The Faulkes Telescope Project is building two large astronomical telescopes, to be located in Hawaii and Australia, which will be dedicated to use by school students. Because of the position of the telescopes they will be available for direct use in real-time during the UK school day. The principal project sponsor is the Dill Faulkes Educational Trust. A .pdf version of this newsletter with images can be found at http://www.faulkes-telescope.com/newsletter4.htm - Status of the Telescopes The first Faulkes Telescope (FT North) is now nearing completion on the mountain of Haleakala in Hawaii. First light on the telescope took place on the 7th August and the first science camera images are expected later the same month. FT North will be used with initial schools later this year and more generally from January 2004. Schools registrations will be opened this autumn. The second, identical telescope (FT South) in now being packed in Birkenhead, where it was manufactured, and will be shipped to its Australian site in September. It will be operational later in 2004. Images of the FTN telescope and its enclosure can be seen on the project web site, www.faulkes-telescope.com. - UK Government Dept. for Education and Skills funds FT Project Following meetings between the FT project and senior staff at the DfES, Dill Faulkes, Richard Beare and Paul Roche gave a presentation to the then Minister for Further and Higher Education, Margaret Hodge. The Minister was clearly impressed with the project, and as a result we have secured substantial funds from the DfES to assist with the first three years of operations. The DfES was particularly keen that the Project should develop proper Continuing Professional Development (CPD) and educational programmes to support teachers in their use of the telescopes, and so Richard Beare (at Warwick Univ.) and David Bowdley (Abraham Darby School, Telford) will be working on this aspect of the FT project over the next three years. David and Richard report later in this newsletter on progress with some of the exciting "education/research" projects that are planned for the start of FT North operations. - National Schools Observatory The Faulkes Telescope project has agreed with Liverpool John Moores University that the UK Schools use of the Faulkes Telescopes and the Liverpool Telescope will be coordinated via the portal www.schoolsobservatory.org.uk. This is intended to make it easier for schools to access all three telescopes. - Asteroid Hunting with the Faulkes Telescopes The Faulkes Telescope Near Earth Object (NEO) Follow-up Education/Research Project has made excellent progress and all the major elements are now in place to launch this project when the first Faulkes Telescope is available in the Autumn of 2003. Teacher training programmes are well advanced in their development stage and the first schools will be approached about joining this project as Development Partners in the new academic year (September 2003). Agreement has been reached with the Minor Planet Center (MPC) in the USA that results from schools using the Faulkes Telescopes will be accepted by them as genuine scientific data. The software to be used is Astrometrica (http://www.astrometrica.at/) and we have negotiated a license agreement to allow us access to this free of charge. Schools will be able to use the Faulkes Telescopes to image asteroids that pose a possible collision threat with the Earth or to image other interesting NEOs. After performing image analysis Schools can then report their data to the MPC who will use them to refine the orbit for the asteroid. The MPC may also on occasion request through the FT project that a school make an urgently needed observation of an NEO that has a particularly worrying preliminary orbit that could bring it close to the Earth. Schools making any observations of NEOs and reporting them to the MPC will have their names published in the MPC electronic circulars that are published daily. What is special about schools using the FTs for their NEO observation work is that they will be using two of the largest astronomical telescope anywhere in the World that are doing this kind of work on a regular basis. Using large telescopes will mean that FT schools can image asteroids that are much fainter than those that can be accessible to amateur astronomers - this puts FT schools in an enviable position. It is also possible that in the process of making their observations schools could also discover new asteroids. In this case, sometime in the future, they would get the right to name their discovery! We are also pleased to inform you that the principal scientific advisors for these projects are as follows: NEO Follow-up: Jay Tate of The Spaceguard Centre (www.spaceguarduk.com) Asteroid Rotation and Classification: Dr Alan Fitzsimmons (Queen's University, Belfast) For further information about the asteroid projects contact david.bowdley () faulkes-telescope com. - Other Education Projects using the Faulkes Telescopes In addition to the asteroid projects work has progressed on several other projects for schools. These include imaging and measuring galaxies, finding the ages of star clusters by plotting colour-magnitude diagrams, studying variable stars, imaging interacting galaxies, and imaging planetary nebulae (the beautiful shells of glowing gas surrounding stars that have recently run out of nuclear fuel and are now losing their outer layers out into space). We have called these projects "education/research" projects because they involve students doing investigations which produce new scientific data as well as being educational. In some cases the new data consists of a high quality image. It may be surprising to learn, for example, that very few of the thousands of nearby galaxies have ever been imaged with the sort of resolution and image quality that the Faulkes Telescopes are capable of. Over time, images of galaxies obtained by schools will build up into a scientifically valuable digital catalogue for the use of professional astronomers, as well as giving individual schools and students the kudos of seeing their names associated with the best images ever taken of 'their' galaxies (or planetary nebulae, or interacting galaxies), and these will be publicly available on the Faulkes website for all the world to admire, and - who knows? - some of them may eventually find their way into a coffee table book along the lines of those containing Hubble images. For the telescopes to be used to their full educational potential, however, projects must involve more than just imaging - educationally interesting and valuable as that is. It is important that scientific conclusions should be drawn and/or measurements made using the images obtained. Take a spiral galaxy for example. There is a wealth of scientific information that students can obtain by carefully observing an image - the blue spiral arms are regions containing recently-formed, massive, hot, blue stars. The central bulge contains yellowish stars which are both cooler and older. Understanding how we can deduce this ties in with the work to be found in most syllabuses on the life cycles of stars, and just how much detail students go into can depend on their age, ability and educational stage, so that the same project can be adapted for use at a wide range of different levels. However we believe that it is important, at any level, that students do some 'real' science, in the sense that they are not just repeating set procedures with known answers as with many traditional school 'experiments'. It is important to use the telescopes to encourage students to think for themselves and to have a sense of ownership of the projects that they undertake. This is helped by the fact that in most cases the observations and/or measurements will be new (as already explained) so that students will be able to talk about 'my galaxy' or 'my asteroid'. To encapsulate this idea of doing real science, the project has adopted the catch phrase 'Real time, real science, real scientists'. The third part of this is the involvement of professional astronomers and in all projects the original ideas for useful investigations have come from them as well as ongoing involvement as needed. Returning to the topic of galaxies, three different but interrelated projects are now effectively finished (and these can be viewed on the Faulkes website, along with the asteroid projects - click the 'Education' link and then the re-direction link, followed by the link to the list of projects). The first project is essentially an imaging project in which the science consists of linking detailed observations of a galaxy with underlying scientific processes and then classifying the galaxy according to the Hubble Classification. The second project involves measuring the spiral arms of galaxies - measuring out how tightly wound they are, how large the central bulge is in relation to the overall disc, and so on, and, again, these quantitative measurements are related to the Hubble Classification. A special spiral arm measuring tool has been developed using Microsoft Excel and this makes it very easy for students to make accurate measurements quickly and easily. The third project involves plotting the surface brightnesses of galaxies along lines through their centres and correlating features in the graphs (such as peaks) with features in the images (such as spiral arms). For advanced level students the surface brightness profiles can be analysed quantitatively, again making use of specially developed and easy-to-use spreadsheet tools. - Image Processing Software Considerable time has been devoted to finding and trying out suitable software for use with the Faulkes Telescopes. Astrometrica has already been mentioned for asteroid work. For general imaging we are recommending some free software called Iris (http://www.astrosurf.com/buil/us/iris/iris.htm). This has been used successfully in Australia with children as young as primary age, but is capable of doing most of the image processing work that is needed for Faulkes projects. For those who need to study imaging in more depth (because their syllabus demands it for example) or who are simply interested in learning more, we are recommending the excellent 'The Handbook of Astronomical Image Processing' by Berry and Burnell. This costs in the region of £78 in the UK but is well worth the investment because it is accompanied by a CD-ROM containing the equally excellent software package 'Astronomical Image Processing for Windows' - AIP4WIN for short. For plotting surface brightness profiles another piece of free software is recommended, DS9. For further details of the recommended software consult the education page of the Faulkes Telescope website. - Development Partner Schools It has already been mentioned that a small number of schools will be acting as 'Development Partners' with the Faulkes Telescope Project from this autumn, trying out the educational projects and providing feedback, once the Hawaiian telescope is in its initial phase of operation. Once this telescope has been 'commissioned' and is fully operational after Christmas it is hoped that a much larger number of schools will choose to become involved in the initial pilot phase, which we envisage lasting for a year or more. If you are interested in being involved as a Development Partner, please email paul.roche () faulkes-telescope com. - Telescopes in Education Paul Roche continues the PPARC National Award programme, "Telescopes in Education", which has been extended to run until spring 2004. Recent events saw Paul visiting Durham, Glasgow, Edinburgh, Hampshire, and talking to around 80 primary school teachers and PGCE students at the Univ. of Kingston, 30 secondary science teachers in Cambridge, and an entire primary school in Cardiff, promoting robotic and real-time astronomy. He has recently developed a "whole school" project for primary schools involving the Sun, as an introduction to the more sophisticated(?!) projects envisaged by the National Schools Observatory and the FT project. This was successfully piloted (despite typically cloudy Welsh July weather) at Birchgrove Primary School in Cardiff, with children from ages 5 to 11 taking part in a range of activities covering day/night, seasons, scale and size of the Solar system, the Sun as a star, light, shadows, time, religion and observing sunspots! - Dill Faulkes revisits old school On June 26th, Dill Faulkes was the guest of honour at the prize giving evening for his old school. John Cleveland Community College in Hinckley was the Hinckley Grammar School when Dill attended, and he found that much of the old site had disappeared, although a few familiar landmarks remained. During the day, pupils at the school received talks from Paul Roche, Lucie Green (Univ. of Glamorgan) and Anastasia Pappa (National Space Centre, Leicester) on various aspects of astronomy and space science. - Join the Project If you want to become involved in the Project as a teacher or student user, or in other ways, please contact us at the e-mail address below. ------------------------------------------------------------------------ For further information contact paul.roche () faulkes-telescope com Project Web site: www.faulkes-telescope.com ------------------------------------------------------------------------ The Faulkes Telescope project partners in the UK are the Dill Faulkes Educational Trust, the Particle Physics and Astronomy Research Council, the University of Leicester and the National Space Centre, Leicester, Liverpool John Moores University and the Royal Observatory Greenwich. The Department for Education and Skills is providing funding. The overseas partners are the University of Hawaii, and in Australia, the Australian National University, Swinburne University of Technology and the Anglo-Australian Observatory. ------------------------------------- To subscribe or unsubscribe to the CANARIE-NEWS list please send e-mail to: majordomo () canarie ca In the body of the e-mail: subscribe news end -------------------------------------These news items and comments are mine alone and do not necessarily reflect those of the CANARIE board or management.---------- Bill.St.Arnaud () Canarie ca starnau () attglobal net www.canarie.ca/~bstarn
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- Grids for Kids - training the innovators of tomorrow (fwd) Dave Farber (Aug 11)