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If ever there was an issue affecting the whole world, it is the threat from Near Earth Objects. To understand and try to cope with the threat requires an international response. This response should cover not only understanding the science, so that dangerous Near Earth Objects may be predicted and methods of mitigation assessed; but, equally important, how all aspects of this response should be organised. The organisation must cover the identification and coordination of the science, communication with the public, and work on measures to react to a possible impact, or deflect or destroy an incoming object. At present no international institution exists for the purpose. Spaceguard is a collective term for a variety of activities which have grown up in a number of countries over recent years, and which have done much to alert public opinion. But none has official recognition except for the US Spaceguard Survey (the name given to NASA’s survey), and so far there are no specific coordinating mechanisms in any state or government, even the United States. The need for an international approach was at the heart of our terms of reference and is central to our proposals for action developed in this chapter. Our terms of reference also asked us to confirm the nature of the hazard and potential levels of risk, which we have done in Chapters 2, 3 and 4; to identify the current British contribution to international efforts, covered in Chapter 7; and to suggest how these issues should be communicated to the public, which we cover in Recommendations 13 and 14 below and the preceding two paragraphs. Science needs The Task Force has concluded that the overall needs, worldwide, are as follows: • for survey and discovery: at least one dedicated 3 metre-class telescope in the southern hemisphere and one in the northern; the survey of smaller Near Earth Objects; the use of data from surveys being made for other purposes; the use of sky survey archives; and the use of space telescope missions where appropriate; • for accurate orbit determinations: one large telescope in each hemisphere, preferably dedicated; some time by right on various existing instruments; • for composition and gross properties: access to large telescopes and space rendezvous missions; • for academic studies: in particular of Near Earth Objects’ interactions with the atmosphere, oceans, solid earth, climate and living things, including historical evidence; and the effects on people and society. What fair contribution should Britain make to fulfilling these needs? We have taken account of existing telescopes or those under construction in which the United Kingdom is a partner; the skills of British scientists and engineers, and industry; and our view that partnership in Europe in this task is desirable. Survey and discovery Recommendation 1 Much valuable data has been gathered cheaply from observations made for purposes unrelated to Near Earth Objects. An excellent example is the photographic archive, at the Royal Observatory Edinburgh, of the United Kingdom Schmidt Telescope in Australia.These records contain invaluable historical detections of Near Earth Objects which greatly enhance the use of current observations. The records are being converted to digital form and posted on the internet for use by astronomers worldwide, with funding from the Particle Physics and Astronomy Research Council. We hope that this will continue. Plates taken with United States Schmidt telescopes are also being digitised, widening this important database. Furthermore, we wish to encourage Near Earth Object discovery by efficient use of suitable current and future wide-angle survey telescopes dedicated to other aims. Recommendation 2 No current space telescope is dedicated to the discovery of Near Earth Objects. However, a number of existing and planned missions are, and will be, able to detect objects incidentally when making observations for quite different purposes.We strongly suggest that consideration be given by space agencies to consider the use of space missions for incidental observations of Near Earth Objects. Apart from existing telescopes (see Annex D), the European Space Agency’s proposed GAIA mission and NASA’s SIRTF project could each be used in this way without substantially modifying the mission or curtailing its main purpose. Recommendation 3 Accurate orbit determination Recommendation 4 Composition and gross properties On the ground-based side, the scientific requirements could be fulfilled immediately by a number of existing telescopes to which the United Kingdom has access. For the southern hemisphere there is the 3.9 metre Anglo-Australian Telescope; in the north there are the 4.2 metre William Herschel and the 2.5 metre Isaac Newton Telescopes on La Palma in the Canary Islands, and in Hawaii the 3.8 metre United Kingdom Infra-Red Telescope. All are heavily over-subscribed; hence we believe that an arrangement should be made for small amounts of time to be provided under appropriate financial terms for spectroscopic follow-up. Several of the European Southern Observatory’s telescopes in Chile would also be excellent for this work.We have considered the great value of radar observations for determining an object’s gross structure and accurate orbit and noted that no such facility exists in the southern hemisphere. However, we do not propose any major British involvement in radar at this stage. Recommendation 5 Space rendezvous missions to asteroids or comets give a unique insight into the characteristics of the asteroid or comet being visited (Annex D). A systematic assessment of different types needs many missions, perhaps 20, to enable each type subsequently to be recognised by ground-based techniques, of great importance should countermeasures be needed. For this limited purpose it might be possible to use a series of essentially identical micro satellites, each launched economically piggy-back with other spacecraft; in this way the unit cost should be much below that of current rendezvous missions.We note that the United Kingdom is a leader in micro satellite technology. We suggest that a beginning could be made with a single demonstration mission. Recommendation 6 Coordination of astronomical observations Recommendation 7
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Studies of impacts and environmental and social effects The prediction of the consequences of an impact requires, in addition to work by astronomers, interdisciplinary research by geophysicists, oceanographers, climatologists, social scientists and others. In the United Kingdom such activities are supported by the universities and by the Research Councils (including Natural Environment Research Council, and the Economic and Social Research Council).The European Science Foundation is currently supporting a limited programme in this area. Such research is not only of great practical importance, but also excellent science. The British Government should encourage high quality research in these areas. Recommendation 8 Mitigation possibilities Recommendation 9 Organisational needs There is a hierarchy of possibilities which we now examine: first is the international structure; next European arrangements; then a British national structure; finally division of responsibilities within the national structure. No United Nations body or agency, can at present be held to represent the global interest in protection from Near Earth Objects.The UN Committee on the Peaceful Uses of Outer Space is too narrowly focused, and UNESCO with its brief on science in general is too wide. Although the Task Force is reluctant to suggest new institutions, something on the lines of the Intergovernmental Panel on Climate Change seems most nearly to meet the requirement. This Intergovernmental Panel has three main working groups: one on science; one on the impacts of change; and one on how change might be mitigated.The Panel, which brings together experts from all over the world, produces Assessments every few years, and has been an outstanding success. An Intergovernmental Panel on Threats from Space, financed by participating governments, would provide a light and unbureaucratic mechanism for coordination and consultation, issuing periodical Assessments as the situation required.Whether more formal arrangements were desirable, on the analogy of the Framework Convention on Climate Change with its successive meetings of the Parties, could be determined in the light of events. Recommendation 10 We recognise that interim measures may be needed before the integrated international structure we prefer could be fully established. In this, the International Astronomical Union, which is already doing much on the science side, should play an important role. Indeed, we expect that a final organisation based on the structure of the Inter-Governmental Panel on Climate Change would wish to continue to involve the International Astronomical Union. Regarding inter-governmental aspects, the Inter-Agency Debris Coordination group (covering the space agencies of United States, Russia, China, India, Japan, Ukraine and Europe) might be able to contribute; and for certain aspects, the UN Committee on the Peaceful Uses of Outer Space. At European level (see Chapter 6), the European Space Agency among other European institutions has already taken up the subject and could develop its interest further on behalf of its member states. The European Southern Observatory, of which most European countries are members, though not Britain, could play a major role in the study of Near Earth Objects with its facilities on excellent sites in the Southern hemisphere. The European Science Foundation, which brings together the research councils and science academies of most European countries, could help to provide and coordinate across Europe a broad base for research on all aspects of the impact problem, physical, biological and social. It already has a programme in the area and funds the European Space Science Committee with strong links to scientists in the United States. Because the threat covers all aspects of life, we believe that the European Union should also be fully engaged. We believe that the Government should discuss with other governments how Europe could best co-ordinate actions regarding Near Earth Objects, and how best to work closely with the United States, with complementary roles in specific areas, and with other interested countries. As a first step we suggest that the European Space Agency and the European Southern Observatory, with the European Union and the European Science Foundation, be asked to propose a strategy for this purpose. It could be discussed at the ministerial meeting of the European Space Agency in 2001. Recommendation 11 At national level no central coordinating body for Near Earth Objects has yet been formally identified within the government. In the event of any emergency, possible or real, virtually all parts of government would be involved, and the Cabinet itself would have to determine policy. This suggests that some Cabinet committee or ad hoc group, bringing in the Department of Trade and Industry, the Home Office, the Ministry of Defence, the Department for the Environment,Transport and the Regions, the Ministry of Agriculture, the Foreign and Commonwealth Office and other interested departments should be envisaged. The interim responsibility rests with the Minister for Science within the Department of Trade and Industry, covering the British National Space Centre and the Office of Science and Technology. The Task Force believes that a lead department should be formally designated, and lines of responsibility established against all eventualities. Recommendation 12 The lead department in Whitehall should act as the channel for recommendations to the Government,The Task Force would not expect this department to undertake all coordination and management itself. Instead the Task Force believes that a British Centre for Near Earth Objects should be set up whose mission would be to promote and co-ordinate work on the subject in Britain; to provide an advisory service to the Government, other relevant authorities, the public and the media; and to facilitate British involvement in international activities, whether through the means suggested above or through the International Astronomical Union and such other bodies as the Minor Planet Center in Boston. In doing so it would call on the Research Councils involved, in particular the Particle Physics and Astronomy Research Council and the Natural Environment Research Council, and on universities, observatories and other bodies concerned. The role of such a Centre would obviously evolve with experience. The closest analogy would be with the recently created Climate Change Centre to be established at the University of East Anglia. It should, like this, be unbureaucratic, and become the centre of a network in Britain but reaching elsewhere, with special responsibility for relations with the public. In this respect its objective would be to communicate in clear, direct and comprehensible language, avoiding excessive alarm or excessive complacency, with some very different audiences: on one hand Parliament, the general public and the media, and on the other the scientific, academic and environmental communities.The Task Force suggests that as a first step there should be a feasibility study to determine the terms of reference for such a Centre and how it might be financed. Recommendation 13 Recommendation 14 In suggesting arrangements of this kind – international, European and national – the Task Force has not attempted more than a sketch of the possibilities.The threat from Near Earth Objects may be a very old problem, going back to the origins of life, but recognition of the threat is new in human experience. Greater understanding of the problem is now coupled with the possibilities of mitigation.The creation of the structure proposed above would form a base for action, if it ever became necessary, and in the meantime give some measure of reassurance. There is no question more often asked of the Task Force:What is the point of worrying about the threat when we can do nothing about it? The answer is that we need to know far more about it than we do, and that with such knowledge something might indeed be done about it.
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| Contents Annex A, Annex B, Annex C, Annex D, Annex E, Annex F |
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