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.ppt

National 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.



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----------
Bill.St.Arnaud () Canarie ca
starnau () attglobal net
www.canarie.ca/~bstarn

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