Comments submitted to the Microgravity Review Panel
Interested parties were invited through the web site to submit comments to the Microrogravity Review Panel during October and November 2002.
There were 45 responses, all of which were presented to the Panel for consideration.
Each respondent was asked if their submission could be published, and 39 replied that they were content (no reply was taken to mean consent was withheld). These responses are given below:
Prof J E Allen, Oxford University
Prof O Alpar, School of Pharmacy, University of London
Dr LG Briarty, ex University of Nottingham
Dr Rob Buckle, Medical Research Council
Dr Anthony MJ Bull, Imperial College London
Prof Naomi Chayen, Imperial College London
Prof WT Coakley, Cardiff University
Dr Charles Cockell, British Antarctic Survey
Prof JL Culhane, FRS, University College London/Mullard
Space Science Laboratory
Dr Nick Davey, Imperial College London
Prof Howell G.M Edwards, Bradford University
Dr Kevin Fong BSc MBBS MRCP, University College London
Dr Peter J. Fraser, Aberdeen University
Prof Allen Goodship, Royal Veterinary College and University
College London
Dr Monica M. Grady, Natural History Museum
Dr Mike Grocott MBBS MRCP FRCA, University College London
Prof LD Hall, University of Cambridge
Dr M H Harrison, QinetiQ Ltd
Prof. JD Hunt FRS, University of Oxford
Dr DBR Kenning, University of Oxford
Dr Peter D. Lee, Imperial College London
Dr Denny Levett MA BM BCh MRCP, University College London
Dr Nicholas Lockerbie, University of Strathclyde
Roger Longstaff, Guest Associates (Europe) Ltd.
Prof. Matthew J. Dring & Dr. Thomas Wiedemann, Queen's
University Belfast
Dr Patrick Magee, University of Bath
Dr M. A. Mendes-Tatsis, Imperial College London
Dr Hugh Montgomery, University College London
Prof Marco Narici, Manchester Metropolitan University
Prof Terence Partridge, Medical Research Council
Dr Peter Quested, NPL & Prof Ken Mills, Imperial College
London
Dr Jonathan Reeve, Addenbrooke's Hospital
Professor Michael J Rennie PhD FRSE, University of Dundee
(now Nottingham)
Dr TJ Stevenson, University of Leicester
Dr J R R Stott, QinetiQ Ltd
Prof Ian A. Sutherland, Brunel Institute for Bioengineering
Prof Pankaj Vadgama, Queen Mary, University of London
Dr T L Whateley, University of Strathclyde
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Department of Engineering Science |
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01865 273000 |
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Fax |
01865 273010 |
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E-mail |
john.allen.eng.ox.ac.uk |
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Brief summary of
main points |
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I wish to make a firm proposal that the I have been a
member of the Advisory Board for the International Microgravity Plasma
Facility (IMPF) since its inception. All the recommendations of this board
are readily available on the web at <http:/www.microgravity.net>. I am
also a member of an active European Network on Complex (Dusty) Plasmas; seven
laboratories are engaged in this activity, in |
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Further details and
background |
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.Scientific and Technological Relevance The basic science in this project is that of the study of the behaviour of dust particles in a plasma. Such particles are somewhat like floating Langmuir probes in that no net current flows to them. In the steady state case the electron current and the ion current must therefore be equal, if secondary emission is negligible. The dust particle then acquires a negative charge, of the order of 10,000 electrons and a corresponding negative potential. The particles then interact with each other and can form "crystal-like" structures, or behave more like liquids or gases. The mixture of dust particles, ions and electrons is sometimes referred to as a "colloidal plasma". However the analogy cannot be carried too far, because the system is not in thermal equilibrium. The interaction between particles is not completely understood. Clearly there is a repulsive force, since they are all negatively charged (in the vast majority of cases). Some experimental reports in
the literature describe a screened Coulomb potential, but agreement has not
yet been reached on the factors that determine the screening length. One of
the difficulties here is that laboratory experiments have been carried out on
the behaviour of dust particles in a space charge sheath. This is because the
weight of the dust pulls the dust particles out from the plasma and into the
adjacent sheath. These experiments are of considerable interest but
experiments in the central plasma region are essential, which is the reason
for devising experiments to be performed on the International Space Station,
where gravitational effects are practically eliminated. The technological
relevance relates largely, but not exclusively, to nanotechnology. As an
example, microcrystals can be grown in plasma
discharges in Silane or Methane and very
interesting results have been obtained on the growth of microcrystalline
silicon films at the Ecole Polytechnique
in In general the research is of interest to
three different communities: those working in space science, those working in
technological plasmas and those working in basic plasma physics. In space
science dust is important in interstellar clouds, comets, interplanetary dust,
the magnetosphere, the ionosphere and planetary rings. Needless to say,
plasma is ubiquitous, so the dust particles will become charged. Much of this
dust is in regions where gravity is unimportant. The technological relevance
has already been referred to. One can add that nowadays particles are grown
in gas discharge plasmas for use as chemical catalysts and for compression
into new materials with improved mechanical properties; such research has
been carried out for some years at the Ecole Polytechnique de Lausanne, |
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Affiliation |
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Address |
Centre for Drug Delivery Research 29 – |
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Telephone |
020 7753 5928 |
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Fax |
020 7753 5942 |
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E-mail |
Oya.alpar@ams1.ulsop.ac.uk |
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Brief summary of main points |
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As a member of the ESA Topical Team, I would like to impress the
importance of an active |
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Further details and background |
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Microsphere and microencapsulation technologies have
found application in a range of industries, from pharmaceutical and
biomedical to agrochemical and electronics. There are however, fundamental
processes involved in the microencapsulation process for which a more
detailed and mechanistic understanding is required. For example the
interfacial phenomena occurring during solvent exchange at the solid/liquid
and liquid/liquid interfaces, and the increased crystallinity
of large polymer molecules. The microgravity environment of the ISS provides
the ideal environment to isolate the different aspect of the
microencapsulation process for a more comprehensive approach to the work. Using a requisite
multidisciplinary approach, elucidation of these mechanisms will provide a
strong platform for further development of microsphere
delivery systems for gene, vaccine and drug delivery, as well as biomedical
diagnostic technologies. In addition to the
contribution to the advancement of science, and its implication on
terrestrial health, there is also considerable commercial benefit to be
gained by improving on microencapsulation technology. |
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Dr LG Briarty |
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Affiliation |
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Address |
9 The Cloisters Beeston NG9 2FR |
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Telephone |
(44) (0) 115 9250 964 |
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Fax |
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E-mail |
lgbriarty@waitrose.com |
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Brief summary of
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The microgravity research, but the current
research organisation and funding climate mitigates against their taking up this
interest. Goodwill towards the significant in the past as I can testify
from my own experience as a PI on various missions (Shuttle IML-1, two parabolic
flights, Foton 12 mission). This can't last much longer unless we make some real investment in the programme; the result of the off and even antagonism towards Throughout nearing retirement. In most other countries a further generation
is being brought on and it is these who will
understand and make use of the ISS as a research facility.
This isn't the case in the left out. As well as being a research facility the
ISS is a major stimulus to international scientific collaboration. It will result in new and expanded research programmes from which the Hope this helps Greg Briarty |
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Further details and
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Dr Rob Buckle |
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Affiliation |
Medical Research Council |
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Address |
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Telephone |
020 7636 5422 |
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Fax |
020 7670 5124 |
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E-mail |
robin.buckle@headoffice.mrc.ac.uk |
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Brief summary of
main points |
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MRC has recently been examining its research strategy in relation to space-based biomedical research programmes, and to this end the MRC and BNSC recently hosted an international workshop to discuss this issue, and the benefits that such programmes might provide for terrestrial health needs. More specifically: · While biomedical research in space is clearly needed to support the programmes of manned space flight, the main benefit of such research is to the health of astronauts, rather than to the health of the terrestrial population. ·
The · Any decision to commit funding towards space research programmes should only be taken once a rigorous cost / benefit analysis has been undertaken. |
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Further details and
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The MRC and BNSC recently hosted a one-day workshop
entitled ‘Space for health, or health for space?’ at the Royal Society in
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Anthony MJ Bull |
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Affiliation |
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Address |
Department of Bioengineering |
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Telephone |
+44 20 7594 5186 |
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Fax |
+44 870 125 4985 |
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E-mail |
a.bull@imperial.ac.uk |
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Brief summary of
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To quickly summarise my relevant research
interest, it is chiefly in the field of movement analysis and the mechanics
of joints in microgravity. I have some experience of microgravity research,
undertaking flights with both ESA and with the Russians. I and my colleagues would wish to be able
to maintain and obtain extended access to parabolic flight programmes in the
future. This work simply cannot be attempted without these experimental
conditions. If you wish to know a little more about the
work, then do contact me. |
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Further details and
background |
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Joint loading in
microgravity: muscle optimisation of movement. Different muscular control
strategies for movement. Applications of the work: devising different control
strategies of bone loading - redistributing load on the joint, bone
re-modelling (osteoporosis applications). |
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Naomi
Chayen |
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Affiliation |
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Address |
Biological
Structure and Function Section, Division
of Biomedical Sciences, Faculty
of Medicine, Technology
and Medicine, |
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Telephone |
020-75943240 |
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Fax |
020-75943169 |
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E-mail |
n.chayen@ic.ac.uk |
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Brief summary of
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Why crystallise proteins? Protein
crystallisation has gained a strategic and commercial relevance in the
post-Genomic era in which X-ray crystallography will play a major role.
Current genome projects are expected to reveal numerous new targets for
therapy of human disease. However, it
is usually not the genes themselves which are the targets, but the proteins
encoded by them. The function of these proteins is determined by their three-dimensional
structure and drugs can influence the function by precise atomic interactions
with the protein. The most powerful technique for determining protein
structure is X-ray crystallography, which is totally dependent on highly
ordered crystals. Obtaining such crystals is the major bottleneck to
structure determination. With the advent of Structural Genomics this problem
is becoming increasingly acute giving rise to an urgent need for designing
new and improved methods for producing high quality crystals. The demand for
structures is not only in the medical sector but also in industries that
utilise protein engineering for making a variety of products (agricultural, washing
powders, sugars and many other products).
It is often the case that crystals are produced, but they are not of
good enough quality to undergo X-ray analysis. It is still not understood why
some proteins (as well as other biological macromolecules) do crystallise
with ease, while most refuse to produce suitable crystals. Better
understanding of the fundamental principles of the crystallisation process
will enable the design of new and improved methods for producing the desired
crystals. Current
problems regarding crystallization in Space The
issue of crystallisation in Space is a controversial one due to conflicting
results reported in the scientific literature. A large number of scientific publications
report that crystallisation of macromolecules in microgravity does indeed
improve the quality of the crystals obtained. On the other hand, there are
other reports opposing this claim, this is mailnly
due to the fact that the success rate of protein crystallisation in Space has
to date, only been 20%. The reasons
for this are only now beginning to emerge.
In recent years, experiments in micogravity
are being conducted in a far more systematic way compared to previous
experiments which were heavily reliant on luck. This is due to improved
apparatus and awareness of the subject. With the aid of CCD video and other
diagnostic tools it is now possible to monitor crystal growth in Space. As a
result, researchers are beginning to realise the crucial factors on which to
focus when conducting experiments in Space. (e.g.
the importance of finding the optimal conditions in Space which may be totally different from the optimal conditions
on Earth as well as the consequence of choosing the right method of
crystallization). A variety of
apparatus made by NASA and The European Space Agency (ESA) for conducting
both screening and diagnostic experiments in microgravity is now available
using all methods of crystallization. British Experiments British
scientists have set some bench marks and have influenced the way of
conducting protein experiments in microG which
others are following (e.g. highlighting of the work done by Helliwell in Science (1995) 270, 1921;
discontinuation of the vapour diffusion method by ESA based on the results of
Chayen and Helliwell
(1999) Nature 398, 20). Dr Skinner who was in During
the period of flying via ESA, We UK Scientists did the microG
work without any support, really in our spare time, while the other Europeans
received handsom funding form their National
Agencies. But, at least we had the flight opportunities which are now at
threat. Because the Protein
crystallisation in MicroG lost credibility in its
early days due to over stating of its merits by some American Scientists. In
recent years the experiments are being done more thoroughly and
critically. It is apparent that we are
only now grasping how best to utilise the microgravity environment. Hence it
would be a great shame if we would have to stop now when we have better
understanding combined with possibilities of continuous access to the
International Space station. Moreover for the British scientists, it would be
a pity if others will reap the benefits of the effort that we have invested,
while we will become bystanders. Imperial Experiments in microgravity: · Crystallisation of Reverse transcriptase on the Russian Photon 7 ('Kashtan Mission') · Crystallisation of lysozyme on Spacehab 1 · Crystallisation of crustacyanin on the IML-2 mission · Crystallisation of crustacyanin on the UMSL-2 mission · Crystallisation of crustacyanin on the LMS mission PUBLICATIONS · Chayen, N.E., "Microgravity Protein Crystallisation Aboard the Photon Satellite" J. Cryst. Growth 153 (1995), 175-179. ·
Chayen, N.E.,
Gordon, E.J. and Zagalsky, P.F., "The
Crystallisation of Apocrustacyanin C1 on the
International Microgravity Laboratory (IML-2) · Chayen, N.E., Snell, E.H., Helliwell, J.R. and Zagalsky, P.F., "CCD video Observation of Microgravity Crystallisation: Apocrustacyanin C1" J. Cryst.Growth 171 (1997), 219-225. · Snell, E.H., Cassetta, A., Helliwell, J.R., Boggon, T.J., Chayen, N.E., Weckert, E., Holzer, K., Schroer, K. Gordon, E.J. and Zagalsky, P.F., "Partial Improvement of Crystal Quality for Microgrvity Grown Apocrustacyanin C1" Acta Cryst. D 53 (1997), 231-239. · Ries Kautt, M., Broutin, I., Ducruix, A., Shepard, W., Kahn, R., Chayen, N., Blow, D., Paal, K., Littke, W., Lorber, B., Theobald-Dietrich, A. and Giege, R., "Crystallogenesis Studies in Microgravity with the Advanced Protein Crystallisation Facility on SpaceHab-01" J. Cryst. Growth 181 (1997), 79-96. · Boggon, T.J., Chayen, N.E., Snell, E.H., Dong J., Lautenschlager, P., Potthast, L., Siddons, P. Stojanoff, V., Gordon, E., Thompson, A., Zagalsky, P.F., Bi, R.C.and Helliwell, J.R., "Protein Crystal Movements and Fluid Flows During Growth" Phil. Trans. R. Soc. Lond. A. 356 (1998), 1045-1061. · Dong, J., Boggon, T.J., Chayen, N.E., Rafetry, J., Bi R-C and Helliwell, J.R., "Bound Solvent Structures for Microgravity, Ground Control, Gel and Microbatch Grown HEW Lysozyme Crystals at 1.8Å Resolution" Acta Cryst. D 55(1999) 745-752. · Snell, E.H., Chayen, N.E. and Helliwell, J.R., "Crystallisation of Biological Macromolecules in Microgravity" (1999). The Biochemist December issue 19-24. · Chayen, N.E. and Helliwell, J.R., "Space-grown Crystals May Prove their Worth" Nature 398, (1999) 20. · Helliwell, J.R., Snell, E.H., Chayen, N.E., Judge, R.A., Boggon, T.J. and Pusey, M.L. "Fluid Physics and Macromolecular Crystal Growth in Microgravity" in "Physics of Fluids in Microgravity" Monti R. ed (2002) · Chayen, N.E. and Helliwell, J.R. (2002) "Protein Crystallization in Microgravity: Are We Reaping the Full Benefit of Outer Space?" New York Academy of Sciences in press. What I have written above is a short summary of the
situation. I can of course supply much more detail if necessary as well as
references for all the statements made |
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