{"id":716,"date":"2026-04-09T19:00:18","date_gmt":"2026-04-09T09:00:18","guid":{"rendered":"https:\/\/stevewatson.info\/blog\/?p=716"},"modified":"2026-04-09T19:04:20","modified_gmt":"2026-04-09T09:04:20","slug":"reconsidering-the-options-for-bracewell-probes","status":"publish","type":"post","link":"https:\/\/stevewatson.info\/blog\/2026\/04\/09\/reconsidering-the-options-for-bracewell-probes\/","title":{"rendered":"Reconsidering the Options for Bracewell Probes"},"content":{"rendered":"<p><span style=\"color: #000000;\">In 1960, Ronald Bracewell proposed<\/span><a href=\"#_ftn1\" name=\"_ftnref1\">[1]<\/a>\u00a0<span style=\"color: #000000;\">that technologically advanced extraterrestrial civilisations might send automated probes to other star systems capable of detecting and communicating with any appropriately advanced civilizations that they might exist. Such probes are called Bracewell probes. Bracewell included the condition that the probes would require at least a degree of intelligence, and it is now common to assume that they will in fact contain an advanced AI of high intelligence. Similarly, though not part of the original hypothesis, it is now also commonly assumed that they would be capable of self-repair or self-replication (Von Neumann machines.) (The need for self-reparability and for at least moderate intelligence in interstellar probes of any kind was argued as far back as 1972.<\/span><a href=\"#_ftn2\" name=\"_ftnref2\">[2]<\/a> <span style=\"color: #000000;\">The technological sophistication expected in such probes has only increased since then.)<\/span><\/p>\n<p><span style=\"color: #000000;\">Several strategies are commonly proposed for such machines.<\/span><\/p>\n<p style=\"padding-left: 40px;\"><span style=\"color: #000000;\">1.\u00a0 \u00a0 In-system Messenger<\/span><\/p>\n<p style=\"padding-left: 40px;\"><span style=\"color: #000000;\">The general form of Bracewell\u2019s original proposal was for a probe that upon arrival in a star system would put itself into orbit about the star and search for signs of intelligent life in the star system. If any were detected it would attempt to make itself known. Should contact be made it would then enter into communication. It would carry with it a database of information that the probe\u2019s builder\u2019s desired to be made known to any intelligent inhabitants of the star system.<\/span><\/p>\n<p style=\"padding-left: 40px;\"><span style=\"color: #000000;\">2.\u00a0 \u00a0 \u00a0Fly-by Messenger<\/span><\/p>\n<p style=\"padding-left: 40px;\"><span style=\"color: #000000;\">Bracewell later accepted that a probe that did not enter orbit about the star but merely passed through the system at a reasonable pace would be able to achieve almost everything that an In-system messenger probe could.<\/span><\/p>\n<p style=\"padding-left: 40px;\"><span style=\"color: #000000;\">3.\u00a0 \u00a0 \u00a0Sentinel<\/span><a href=\"#_ftn3\" name=\"_ftnref3\">[3]<\/a><\/p>\n<p style=\"padding-left: 40px;\"><span style=\"color: #000000;\">Bracewell further proposed the idea of a sentinel probe that arrives in a system and establishes itself in some location from which it can discreetly monitor the system for the development of intelligent life or for the development of technological competence in existing intelligent life. The probe could then choose to initiate contact or not according to the designs of its builder, but it would certainly communicate its observations and the occurrence of some threshold event (such as radio communication) to its builders \u2013 or to whoever might have succeeded them. <\/span><\/p>\n<p style=\"padding-left: 40px;\"><span style=\"color: #000000;\">4.\u00a0 \u00a0 \u00a0Von Neumann Sentinel<\/span><\/p>\n<p style=\"padding-left: 40px;\"><span style=\"color: #000000;\">As mentioned, for various obvious reasons, it is now commonly supposed that Sentinel probes are likely to be Von Neumann machines: that upon arrival in a star system with adequate material and energy resources they would be capable of replicating themselves and sending those new machines on to further star systems, while the original remains in the system as a sentinel.<\/span><\/p>\n<p><span style=\"color: #000000;\"><strong>Assessing Possible Probe Locations<\/strong><\/span><\/p>\n<p><span style=\"color: #000000;\">I think we can accept that we have not yet observed any messenger probes \u2013 notwithstanding claims concerning the interstellar object \u2018Oumuamua that Avi Loeb hypothesized might be a Fly-by probe<\/span><a href=\"#_ftn4\" name=\"_ftnref4\">[4]<\/a><span style=\"color: #000000;\">, or the Long Delayed Echoes<\/span><a href=\"#_ftn5\" name=\"_ftnref5\">[5]<\/a> <span style=\"color: #000000;\">of radio signals that have been observed since 1927 and that Bracewell himself thought were the sort of thing that an In-system Messenger probe might create to attract attention to itself. This is in line with the plausible idea that, with the fate of humanity at stake, such indiscriminate METI would be quite inadvisable. If we accept the possibility of sentinel probes as they have been described, on the other hand, it is natural to wonder whether they might be already present in our own Solar System, and where they might be if they were. There are several criteria that can guide the search.<\/span><\/p>\n<ol>\n<li><span style=\"color: #000000;\">Assuming that the probes will be primarily interested in Earth, which is of obvious biological interest, and which now hosts an intelligent space-faring life-form, the location should allow close observational access to Earth.<\/span><\/li>\n<li><span style=\"color: #000000;\">On the other hand, since we would expect the probes and their mission profiles to be designed so that contact with intelligent species is at the discretion of the probe itself (to the greatest degree possible,) the location should allow the probe to remain undetected as it operates.<\/span>\n<ul>\n<li><span style=\"color: #000000;\">In any case, the fact that we have not observed such a probe is evidence enough that if it does exist it does not want to be discovered just yet.<\/span><\/li>\n<li><span style=\"color: #000000;\">Note that no location or strategy is going to be undetectable for all levels of technology. Eventually, we will be able to detect any probe if it remains active in the Solar System.<\/span><\/li>\n<li><span style=\"color: #000000;\">Note further in this context that there is probably a minimum size for a probe that wishes to observe from a distance, transmit its findings home, and survive the space environment. R Freitas<\/span><a href=\"#_ftn6\" name=\"_ftnref6\">[6]<\/a> <span style=\"color: #000000;\">has given a rough estimate of the size we can expect as about 1-10m across (though this is based on assumptions concerning the survivability of meteoroid impacts and the likely observation distance and resolution that may not be universally relevant or reliable. It also assumes that the interstellar drive system is either of insignificant size or has separated from the active probe \u2013 surely, the latter.)<\/span><\/li>\n<\/ul>\n<\/li>\n<li><span style=\"color: #000000;\">A probe intended for long-duration observation will require a location that is stable or predictable in character or whose dynamics are easily managed.<\/span><\/li>\n<li><span style=\"color: #000000;\">A very long duration probe will require access to energy resources \u2013 presumably solar, since it could hardly count on finding other energy sources at destination.<\/span><\/li>\n<li><span style=\"color: #000000;\">A self-repairing or self-replicating probe \u2013 as a long duration probe ought to be \u2013 will require access to material resources.<\/span><\/li>\n<\/ol>\n<p><span style=\"color: #000000;\">Bearing these criteria in mind we can assess the options<\/span><a href=\"#_ftn7\" name=\"_ftnref7\">[7]<\/a><\/p>\n<ol>\n<li><span style=\"color: #000000;\">Solar Orbit<\/span>\n<ol>\n<li><span style=\"color: #000000;\">The ability to closely observe Earth would be dependent upon the particular orbit: but unless it were actually co-orbital with Earth (see that option below,) the opportunities would be very intermittent.<\/span><\/li>\n<li><span style=\"color: #000000;\">Unless embedded in a natural object (see the Asteroid options) it would be difficult to remain undetected by reasonably competent observers on Earth.<\/span><\/li>\n<li><span style=\"color: #000000;\">The orbits could be very stable<\/span><\/li>\n<li><span style=\"color: #000000;\">Solar power is easily available \u2013 of course, depending on the distance from the Sun.<\/span><\/li>\n<li><span style=\"color: #000000;\">Unless associated with an asteroid (again, see the Asteroid options) there would be no material resources to exploit.<\/span><\/li>\n<\/ol>\n<\/li>\n<li><span style=\"color: #000000;\">Earth<\/span>\n<ol>\n<li><span style=\"color: #000000;\">An observation site on Earth\u2019s surface limits the range of coverage so it\u2019s unlikely to be selected for that reason anyway.<\/span><\/li>\n<li><span style=\"color: #000000;\">Moreover, it would be too easily discoverable by inhabitants of Earth.<\/span><\/li>\n<li><span style=\"color: #000000;\">The environment of the Earth is extremely active, geologically and otherwise, so any very old probes would probably not have survived.<\/span><\/li>\n<li><span style=\"color: #000000;\">Energy is easily available.<\/span><\/li>\n<li><span style=\"color: #000000;\">Material resources are plentiful.<\/span><\/li>\n<\/ol>\n<\/li>\n<li><span style=\"color: #000000;\">Earth Orbit<\/span>\n<ol>\n<li><span style=\"color: #000000;\">Has excellent close observational potential<\/span><\/li>\n<li><span style=\"color: #000000;\">But any body in orbit is going to be highly observable to even a modestly technically competent observer on Earth.<\/span><\/li>\n<li><span style=\"color: #000000;\">Low orbits are unstable because of atmospheric drag.<\/span><\/li>\n<li><span style=\"color: #000000;\">Solar energy is easily available, but<\/span><\/li>\n<li><span style=\"color: #000000;\">Material resources in Earth orbit are lacking.<\/span><\/li>\n<\/ol>\n<\/li>\n<li><span style=\"color: #000000;\">Earth Co-orbit<\/span><a href=\"#_ftn8\" name=\"_ftnref8\">[8]<\/a>\n<ol>\n<li><span style=\"color: #000000;\">Objects in co-orbits intermittently approach Earth to respectable distances for close observation,<\/span><\/li>\n<li><span style=\"color: #000000;\">and since we\u2019ve really only just noticed them, their detection is not that easy<\/span><\/li>\n<li><span style=\"color: #000000;\">The orbits may be stable (though it\u2019s still an open question how stable.)<\/span><\/li>\n<li><span style=\"color: #000000;\">There is adequate solar power available, but<\/span><\/li>\n<li><span style=\"color: #000000;\">it is not clear that co-orbits have sufficient material resources to be useful to self-repairing or self-replicating devices.<\/span><\/li>\n<\/ol>\n<\/li>\n<li><span style=\"color: #000000;\">Lagrange Point (Earth-Moon or Earth-Sun)<\/span>\n<ol>\n<li><span style=\"color: #000000;\">The Earth Moon L<sub>4<\/sub> and L<sub>5<\/sub> points are within easy range of Earth for observation, but close observation of Earth would be difficult from the Earth-Sun points.<\/span><\/li>\n<li><span style=\"color: #000000;\">Lagrange points are inherently interesting and would be expected to draw the attention of any intelligent observers on Earth. It would be hard for any sizeable object to remain undetected there unless hidden within a natural body. There are no such bodies in the Earth Moon L<sub>4<\/sub> and L<sub>5<\/sub> points though there are many in the Earth-Sun points.<\/span><\/li>\n<li><span style=\"color: #000000;\">The L<sub>4<\/sub> and L<sub>5<\/sub> points are stable but orbits within a \u2018Lagrange Point\u2019 require constant adjustment and thus would be likely to invite detection.<\/span><\/li>\n<li><span style=\"color: #000000;\">There is adequate solar energy available in both sets of Lagrange points mentioned above<\/span><\/li>\n<li><span style=\"color: #000000;\">The Earth-Moon points are empty, as noted, and It is not clear that even the Earth-Sun points have sufficient material resources to be useful to self-repairing or self-replicating devices.<\/span><\/li>\n<\/ol>\n<\/li>\n<li><span style=\"color: #000000;\">Planetary Moons<\/span>\n<ol>\n<li><span style=\"color: #000000;\">Moons at too great a distance from Earth could not make close observations.<\/span><\/li>\n<li><span style=\"color: #000000;\">Moons \u2013 especially the Moon of Earth \u2013 would be obvious targets for intelligent observers on Earth, and an object on one would be detectable unless buried; but if it were buried it is unlikely that it could observe.<\/span><\/li>\n<li><span style=\"color: #000000;\">Moons with too active environments would be unsafe, though many moons are quite inert.<\/span><\/li>\n<li><span style=\"color: #000000;\">Moons at too great a distance from Earth would also suffer from a lack of solar radiation for power.<\/span><\/li>\n<li><span style=\"color: #000000;\">Moons lacking the appropriate materials (like ice moons) would be useless for Von Neumann machines<\/span><\/li>\n<\/ol>\n<\/li>\n<li><span style=\"color: #000000;\">Near-Earth Asteroids<\/span>\n<ol>\n<li><span style=\"color: #000000;\">These spend a lot of time at a great distance from Earth so that the opportunities for close observation from them would only be intermittent.<\/span><\/li>\n<li><span style=\"color: #000000;\">It would, however, be quite difficult to detect a probe if it were located on one.<\/span><\/li>\n<li><span style=\"color: #000000;\">Their orbits are adequately stable, and they can be selected to have stable physical environments \u2013 avoiding out-gassers or sites with moving rubble.<\/span><\/li>\n<li><span style=\"color: #000000;\">NEA are close enough to the Sun to make use of its light for power<\/span><\/li>\n<li><span style=\"color: #000000;\">and they are of a wide enough variety that one with appropriate material resources would certainly be available.<\/span><\/li>\n<\/ol>\n<\/li>\n<li><span style=\"color: #000000;\">Outer Asteroids<\/span>\n<ol>\n<li><span style=\"color: #000000;\">Close observation of the Earth is difficult at all times.<\/span><\/li>\n<li><span style=\"color: #000000;\">Discovery would be near impossible if the probe\u2019s own power emissions could be disguised or hidden.<\/span><\/li>\n<li><span style=\"color: #000000;\">Their conditions of stability would be as with the NEA.<\/span><\/li>\n<li><span style=\"color: #000000;\">Solar power is difficult to source at these distances,<\/span><\/li>\n<li><span style=\"color: #000000;\">though material resources are plentiful.<\/span><\/li>\n<\/ol>\n<\/li>\n<li><span style=\"color: #000000;\">Outer Solar System Small Body Zones<\/span>\n<ol>\n<li><span style=\"color: #000000;\">Close observation of Earth would be very difficult.<\/span><\/li>\n<li><span style=\"color: #000000;\">Discovery would be near impossible if the probe\u2019s own power emissions could be disguised or hidden.<\/span><\/li>\n<li><span style=\"color: #000000;\">Their conditions of stability would be as with the NEA.<\/span><\/li>\n<li><span style=\"color: #000000;\">Energy from the Sun would be difficult to access,<\/span><\/li>\n<li><span style=\"color: #000000;\">but material resources are plentiful<\/span><\/li>\n<\/ol>\n<\/li>\n<\/ol>\n<p><span style=\"color: #000000;\"><strong>Revising the Search Strategy<\/strong><\/span><\/p>\n<p><span style=\"color: #000000;\">Such are the usual assessments of the options, but it should be noted that these assessments assume that the probes are only minimally active after they have settled down to wait in the solar system and to monitor and observe. This is an assumption possibly driven by considerations of resource and energy conservation over the long term of a probe\u2019s mission, by familiarity with the sort of \u2018long-duration\u2019 space probes that we have constructed, and even by the natural association of the ideas of waiting and monitoring and observing (as a sentinel does) with passivity. This may, however, mislead as to the possible strategies that are within the capacity of intelligent machines sophisticated enough to be actually self-repairing or self-replicating. We should assume that any such machine is effectively a universal constructor.<\/span><\/p>\n<p><span style=\"color: #000000;\">Amongst the capabilities of such machines would be:<\/span><\/p>\n<ol>\n<li><span style=\"color: #000000;\">Self-repair and self-replication of course (creating resilience and a margin of error in a system intended for long-term operations)<\/span><\/li>\n<li><span style=\"color: #000000;\">Resource identification, extraction, processing, and utilisation (which are the necessary prerequisites for repair or replication, but also for any form of construction at all.)<\/span><\/li>\n<li><span style=\"color: #000000;\">Refuelling<\/span><\/li>\n<li><span style=\"color: #000000;\">Energy access and replenishment<\/span><\/li>\n<li><span style=\"color: #000000;\">Relocation<\/span><\/li>\n<li><span style=\"color: #000000;\">Environmental modification (burial, rehabilitation, etc.)<\/span><\/li>\n<li><span style=\"color: #000000;\">The construction of subordinate probes<\/span><\/li>\n<\/ol>\n<p><span style=\"color: #000000;\">Such a probe would consequently be able to adopt a variety of strategies over the course of its mission \u2013 strategies not available to the sorts of passive monitors that have generally been imagined \u2013 adapting to changing circumstances. Such a probe might set up orbital monitoring stations about a world of interest if that world had no intelligent observers on it, or it might relocate to a moon if observers arose. It might create a series of probes to embed in asteroids to pass close by the target planet if that planet had developed intelligent observes. It might relocate all its probes to the outer system if the intelligence on that planet became observationally competent or capable of inter planetary travel.<\/span><\/p>\n<p><span style=\"color: #000000;\">Given such capabilities, the assessment of the various locations at which we might hope to discover evidence of a Von Neumann\/Bracewell probe in the Solar System should begin with an assessment of our present or immediately foreseeable observational and technological competence on the grounds that any possible VN\/B probe would have made a similar assessment and adapted its operations to continue being undetected by us while observing as best it still could.<\/span><\/p>\n<p><span style=\"color: #000000;\">We might then conclude that the most likely strategy for the probe in the current situation is<\/span><\/p>\n<ul>\n<li><span style=\"color: #000000;\">Maintain a site in the Kuiper Belt on a large resource-rich body consisting of the VN\/B probe itself and including whatever further infrastructure is required to continue operations (construction, replication, fuel extraction, etc.)<\/span><\/li>\n<li><span style=\"color: #000000;\">Dispatch probes hidden within small (1m-10m) bodies passing close by the Earth and returning to deep space. These could be sent in a constant stream so that Earth would remain under continuous close observation.<\/span><\/li>\n<\/ul>\n<p><span style=\"color: #000000;\">We might further conclude that the best way to detect these operations \u2013 assuming that asteroid interception is not yet possible for us at short notice \u2013 would be to<\/span><\/p>\n<ul>\n<li><span style=\"color: #000000;\">Search for Infra-Red or other techno-signatures in the KB and on close-passing rocks as they return to deep space (those probes are likely to want to move from their cover or alter their trajectories and all such velocity changes will require energy use whose effects cannot be hidden.)<\/span><\/li>\n<li><span style=\"color: #000000;\">Scan for evidence of transmissions of data from the KB site to interstellar space, and from the asteroidal probes to the KB site.<\/span><\/li>\n<li><span style=\"color: #000000;\">Map the trajectories of small close-passing asteroids to determine whether there is a common point of origin to some significant number of them.<\/span><\/li>\n<\/ul>\n<p><a href=\"#_ftnref1\" name=\"_ftn1\">[1]<\/a> <span style=\"color: #000000;\">Bracewell, R. N. (1960)<\/span> &#8220;<a href=\"https:\/\/lweb.cfa.harvard.edu\/~loeb\/Bracewell1960.pdf\">Communications from Superior Galactic Communities<\/a>,<span style=\"color: #000000;\">&#8221;\u00a0<em>Nature<\/em>\u00a0<strong>186<\/strong>:670-671. Reprinted in Cameron, A. G. (ed.) (1963)\u00a0<em>Interstellar Communication<\/em>, NY: W. A. Benjamin, 243-248<\/span><\/p>\n<p><a href=\"#_ftnref2\" name=\"_ftn2\">[2]<\/a> <span style=\"color: #000000;\">Gatland, K. (1972)<em> Robot Explorers<\/em>, London: Blandford Press, 239 \u2013 244<\/span><\/p>\n<p><a href=\"#_ftnref3\" name=\"_ftn3\">[3]<\/a> <span style=\"color: #000000;\">The name is in reference to the device in Arthur C. Clarke\u2019s 1951 short story \u2018The Sentinel\u2019 (reprinted in his 1953 <em>Expedition to Earth.<\/em>)<\/span><\/p>\n<p><a href=\"#_ftnref4\" name=\"_ftn4\">[4]<\/a> <span style=\"color: #000000;\">Loeb, A.<\/span> <a href=\"https:\/\/lweb.cfa.harvard.edu\/~loeb\/Loeb_Astrobiology.pdf\">\u2018On the Possibility of an Artificial Origin for \u2018Oumuamua\u2019<\/a><\/p>\n<p><a href=\"#_ftnref5\" name=\"_ftn5\">[5]<\/a> <span style=\"color: #000000;\">Lunan, D. (1974) &#8216;Space Probe from Epsilon Bo\u00f6tis?&#8217;,\u00a0<em>Analog<\/em>\u00a0XCII, 5, 66-84, January, and (1998\/2013)<\/span> <a href=\"https:\/\/www.duncanlunan.com\/epsilonbootis.asp\">Epsilon Bo\u00f6tis Revisited<\/a><\/p>\n<p><a href=\"#_ftnref6\" name=\"_ftn6\">[6]<\/a> <span style=\"color: #000000;\">Freitas, R. A. jr. (1985)<\/span> <a href=\"https:\/\/www.rfreitas.com\/Astro\/SETAActa1985.htm\">The Search for Extraterrestrial Artifacts (SETA)<\/a> <span style=\"color: #000000;\"><em>Acta Astronautica<\/em>\u00a0<strong>12<\/strong>:1027-1034<\/span><\/p>\n<p><a href=\"#_ftnref7\" name=\"_ftn7\">[7]<\/a> <span style=\"color: #000000;\">See also Gertz, J. (2016)<\/span> <a href=\"https:\/\/arxiv.org\/pdf\/1609.04635\">ET: Looking Here as Well as There<\/a> <span style=\"color: #000000;\"><em>JBIS<\/em> <strong>69<\/strong>:88-92<\/span><\/p>\n<p><a href=\"#_ftnref8\" name=\"_ftn8\">[8]<\/a> <span style=\"color: #000000;\">Objects are known to co-orbit with Earth in various ways, occupying Earth\u2019s orbit and occasionally\/regularly approaching relatively closely to Earth. Jim Benford in<\/span> <a href=\"https:\/\/arxiv.org\/pdf\/1903.09582\">Looking for Lurkers v.2<\/a> <span style=\"color: #000000;\">investigated the possibility of Bracewell probes locating themselves in these co-orbits.<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>In 1960, Ronald Bracewell proposed[1]\u00a0that technologically advanced extraterrestrial civilisations might send automated probes to other star systems capable of detecting and communicating with any appropriately advanced civilizations that they might exist. Such probes are called Bracewell probes. Bracewell included the condition that the probes would require at least a degree of intelligence, and it is [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[54],"tags":[],"class_list":["post-716","post","type-post","status-publish","format-standard","hentry","category-space"],"_links":{"self":[{"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/posts\/716","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/comments?post=716"}],"version-history":[{"count":3,"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/posts\/716\/revisions"}],"predecessor-version":[{"id":719,"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/posts\/716\/revisions\/719"}],"wp:attachment":[{"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/media?parent=716"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/categories?post=716"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/stevewatson.info\/blog\/wp-json\/wp\/v2\/tags?post=716"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}