The Outer Space Treaties

1969 ◽  
Vol 73 (705) ◽  
pp. 751-758
Author(s):  
Francis Vallat

In this lecture I intend to talk about two treaties adopted under the auspices of the General Assembly of the United Nations. To give them their full titles, they are the Treaty on Principles Governing the Activities of States in the Exploration and Use of Outer Space including the Moon and other Celestial Bodies and the Agreement on the Rescue of Astronauts, the Return of Astronauts and the Return of Objects Launched into Outer Space. For convenience, I shall call them the Treaty on Outer Space and the Agreement on Rescue and Return.

1985 ◽  
Vol 79 (1) ◽  
pp. 163-168 ◽  
Author(s):  
Carl Q. Christol

On July 11, 1984, the 1979 Agreement Governing the Activities of States on the Moon and Other Celestial Bodies entered into force following the deposit with the Secretary-General of the United Nations of the fifth instrument of ratification. The Agreement, following its adoption by the General Assembly, was opened for signature on December 18, 1979. In the intervening years, it has been signed by Austria, Chile, France, Guatemala, India, Morocco, the Netherlands, Peru, the Philippines, Romania and Uruguay. The fifth state to deposit its ratification was Austria, which followed Chile, the Philippines, Uruguay and the Netherlands.


Author(s):  
W. F. Foster

On September 10, 1971, the United Nations Committee on the Peaceful Uses of Outer Space adopted and decided to submit to the General Assembly for consideration and final adoption a draft Convention on International Liability for Damage caused by Space Objects. Approval of the Convention was recommended by the First Committee of the General Assembly on November 11, 1971; and on November 29, 1971 it was endorsed by the General Assembly. The Convention on International Liability for Damage Caused by Space Objects marks the culmination of a decade of debate and negotiation of the problem of liability for damage arising from outer space activities.


Author(s):  
Mazlan Othman

The United Nations briefly considered the issue of extra-terrestrial intelligence at the 32nd session of the General Assembly in 1977. As a result, the Office of Outer Space Affairs was tasked to prepare a document on issues related to ‘messages to extra-terrestrial civilizations’, but this area has not been followed through in more recent times. This discussion paper describes the United Nations’ activities in the field of near-Earth objects in some detail, and suggests that this might be used as a model of how Member States could proceed with dealing with this issue in case the existence of extra-terrestrial life/intelligence is established.


2018 ◽  
Vol 13 (S349) ◽  
pp. 79-89
Author(s):  
Karel A. van der Hucht

AbstractThe Minor Planet Center, established in 1947 by the IAU, is the international repository and clearinghouse for the world’s minor planet observations. Since 1989, CCD surveys of Near Earth Objects at ground-based astronomical observatories are operational, mainly in the USA. As of 23 August, 2018, a total of 18,545 Near Earth Asteroids (NEAs) and 107 Near Earth Comets (NECs) have been registered and daily updates are made publicly available on the internet by the MPC, NASA-JPL-CNEOS and ESA-SSA-NEOCC.Concern about the possibility of NEO impacts has been picked up by the United Nations Committee on the Peaceful Uses of Outer Space (UN-COPUOS), where the IAU has observer status, and formally expressed since 1999. This led in 2014 to the formation of two international coordinating bodies for NEO detection and NEO impact mitigation: the International Asteroid Warning Network (IAWN) and the Space Mission Planning Advisory Group (SMPAG).In support of these developments, the IAU 28th General Assembly, Session II, held in Beijing on 30 August 2012, adopted a Resolution (3B) recommending the establishment of an International NEO EarlyWarning System, as proposed by the IAU Division III (now Division F) Working Group on Near-Earth Objects. The GA recommended “… that the IAU National Members work with the United Nations Committee on the Peaceful Uses of Outer Space (UNCOPUOS) and the International Council for Science (ICSU), to coordinate and collaborate on the establishment of an International NEO Early Warning System, relying on the scientific and technical advice of the relevant astronomical community, whose main purpose is the reliable identification of potential NEO collisions with the Earth, and the communication of the relevant parameters to suitable decision makers of the nation(s) involved. ….”The NEO hazard issue received world-wide attention on 13 February 2013 when a NEA with an estimated size of 17 to 20 meters and an estimated mass of 11,000 tons exploded over Chelyabinsk (Russia), releasing 440 kT TNT of energy at an altitude of ∼23 km.Subsequently, on 5 December 2014, the United Nations General Assembly adopted a Resolution (69/85, 9–10), noting “… the importance of information-sharing in discovering, monitoring and physically characterizing potentially hazardous near-Earth objects to ensure that all countries, in particular developing countries with limited capacity in predicting and mitigating a near-Earth object impact, are aware of potential threats, emphasizes the need for capacitybuilding for effective emergency response and disaster management in the event of a near-Earth object impact, .…”In spite of all dedicated NEO surveys operational to date, the present inventory and thus our assessment of the level of threat of NEOs is severely limited by their huge number and by the available observational capabilities. E.g., while the estimated number of all NEOs larger than 40 meters in diameter is ∼700, 000, only ∼2% have been detected to date. For NEOs with sizes between 40 and 140 meters, the detection percentage amounts to less than 1% of the estimated number. Only dedicated space-based surveys, preferably in the infrared, will be able to provide the much needed orders of magnitude improvement in the detection, tracking and characterizing of NEOs. One promising project is the NASA-JPL NEOCam mission, studied since 2005 but not yet approved: a dedicated infrared observatory aiming to detect, track and characterize NEO’s from the Sun-Earth Lagrange point L1.As Yeomans puts it: we better find them before they find us (Yeomans 2013). Traditionally, astronomers are looking back into the past, if only because of the limited speed of light. But we should realize that the clear and present danger posed by hazardous Near Earth Objects to mankind and all other life forms obliges us to look also forward, into the future. Provided with the proper means, we astronomers can do that, as a small service to society, including ourselves. The astronomical community at large should give high priority to NEO survey projects, in particular space-based surveys.


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