Reconsidering the Options for Bracewell Probes
April 9, 2026 – 7:00 pmIn 1960, Ronald Bracewell proposed[1] 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.[2] The technological sophistication expected in such probes has only increased since then.)
Several strategies are commonly proposed for such machines.
1. In-system Messenger
The general form of Bracewell’s 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’s builder’s desired to be made known to any intelligent inhabitants of the star system.
2. Fly-by Messenger
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.
3. Sentinel[3]
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 – or to whoever might have succeeded them.
4. Von Neumann Sentinel
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.
Assessing Possible Probe Locations
I think we can accept that we have not yet observed any messenger probes – notwithstanding claims concerning the interstellar object ‘Oumuamua that Avi Loeb hypothesized might be a Fly-by probe[4], or the Long Delayed Echoes[5] 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.
- 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.
- 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.
- 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.
- 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.
- 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[6] 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 – surely, the latter.)
- A probe intended for long-duration observation will require a location that is stable or predictable in character or whose dynamics are easily managed.
- A very long duration probe will require access to energy resources – presumably solar, since it could hardly count on finding other energy sources at destination.
- A self-repairing or self-replicating probe – as a long duration probe ought to be – will require access to material resources.
Bearing these criteria in mind we can assess the options[7]
- Solar Orbit
- 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.
- Unless embedded in a natural object (see the Asteroid options) it would be difficult to remain undetected by reasonably competent observers on Earth.
- The orbits could be very stable
- Solar power is easily available – of course, depending on the distance from the Sun.
- Unless associated with an asteroid (again, see the Asteroid options) there would be no material resources to exploit.
- Earth
- An observation site on Earth’s surface limits the range of coverage so it’s unlikely to be selected for that reason anyway.
- Moreover, it would be too easily discoverable by inhabitants of Earth.
- The environment of the Earth is extremely active, geologically and otherwise, so any very old probes would probably not have survived.
- Energy is easily available.
- Material resources are plentiful.
- Earth Orbit
- Has excellent close observational potential
- But any body in orbit is going to be highly observable to even a modestly technically competent observer on Earth.
- Low orbits are unstable because of atmospheric drag.
- Solar energy is easily available, but
- Material resources in Earth orbit are lacking.
- Earth Co-orbit[8]
- Objects in co-orbits intermittently approach Earth to respectable distances for close observation,
- and since we’ve really only just noticed them, their detection is not that easy
- The orbits may be stable (though it’s still an open question how stable.)
- There is adequate solar power available, but
- it is not clear that co-orbits have sufficient material resources to be useful to self-repairing or self-replicating devices.
- Lagrange Point (Earth-Moon or Earth-Sun)
- The Earth Moon L4 and L5 points are within easy range of Earth for observation, but close observation of Earth would be difficult from the Earth-Sun points.
- 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 L4 and L5 points though there are many in the Earth-Sun points.
- The L4 and L5 points are stable but orbits within a ‘Lagrange Point’ require constant adjustment and thus would be likely to invite detection.
- There is adequate solar energy available in both sets of Lagrange points mentioned above
- 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.
- Planetary Moons
- Moons at too great a distance from Earth could not make close observations.
- Moons – especially the Moon of Earth – 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.
- Moons with too active environments would be unsafe, though many moons are quite inert.
- Moons at too great a distance from Earth would also suffer from a lack of solar radiation for power.
- Moons lacking the appropriate materials (like ice moons) would be useless for Von Neumann machines
- Near-Earth Asteroids
- 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.
- It would, however, be quite difficult to detect a probe if it were located on one.
- Their orbits are adequately stable, and they can be selected to have stable physical environments – avoiding out-gassers or sites with moving rubble.
- NEA are close enough to the Sun to make use of its light for power
- and they are of a wide enough variety that one with appropriate material resources would certainly be available.
- Outer Asteroids
- Close observation of the Earth is difficult at all times.
- Discovery would be near impossible if the probe’s own power emissions could be disguised or hidden.
- Their conditions of stability would be as with the NEA.
- Solar power is difficult to source at these distances,
- though material resources are plentiful.
- Outer Solar System Small Body Zones
- Close observation of Earth would be very difficult.
- Discovery would be near impossible if the probe’s own power emissions could be disguised or hidden.
- Their conditions of stability would be as with the NEA.
- Energy from the Sun would be difficult to access,
- but material resources are plentiful
Revising the Search Strategy
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’s mission, by familiarity with the sort of ‘long-duration’ 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.
Amongst the capabilities of such machines would be:
- Self-repair and self-replication of course (creating resilience and a margin of error in a system intended for long-term operations)
- Resource identification, extraction, processing, and utilisation (which are the necessary prerequisites for repair or replication, but also for any form of construction at all.)
- Refuelling
- Energy access and replenishment
- Relocation
- Environmental modification (burial, rehabilitation, etc.)
- The construction of subordinate probes
Such a probe would consequently be able to adopt a variety of strategies over the course of its mission – strategies not available to the sorts of passive monitors that have generally been imagined – 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.
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.
We might then conclude that the most likely strategy for the probe in the current situation is
- 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.)
- 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.
We might further conclude that the best way to detect these operations – assuming that asteroid interception is not yet possible for us at short notice – would be to
- 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.)
- Scan for evidence of transmissions of data from the KB site to interstellar space, and from the asteroidal probes to the KB site.
- Map the trajectories of small close-passing asteroids to determine whether there is a common point of origin to some significant number of them.
[1] Bracewell, R. N. (1960) “Communications from Superior Galactic Communities,” Nature 186:670-671. Reprinted in Cameron, A. G. (ed.) (1963) Interstellar Communication, NY: W. A. Benjamin, 243-248
[2] Gatland, K. (1972) Robot Explorers, London: Blandford Press, 239 – 244
[3] The name is in reference to the device in Arthur C. Clarke’s 1951 short story ‘The Sentinel’ (reprinted in his 1953 Expedition to Earth.)
[4] Loeb, A. ‘On the Possibility of an Artificial Origin for ‘Oumuamua’
[5] Lunan, D. (1974) ‘Space Probe from Epsilon Boötis?’, Analog XCII, 5, 66-84, January, and (1998/2013) Epsilon Boötis Revisited
[6] Freitas, R. A. jr. (1985) The Search for Extraterrestrial Artifacts (SETA) Acta Astronautica 12:1027-1034
[7] See also Gertz, J. (2016) ET: Looking Here as Well as There JBIS 69:88-92
[8] Objects are known to co-orbit with Earth in various ways, occupying Earth’s orbit and occasionally/regularly approaching relatively closely to Earth. Jim Benford in Looking for Lurkers v.2 investigated the possibility of Bracewell probes locating themselves in these co-orbits.
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