Student Blog Entries

Bracewell’s Probes: Fiction Masquerading as Science

Bracewell, 1960 contemplates the methods to detect a signal from an advanced civilization. The paper can be considered a critique and response to Cocconi & Morrison’s seminal 1959 paper on interstellar communication. Bracewell argues that using narrow-band radio signals on Earth is a flawed approach to detect “superior communities” as these are not abundant. Bracewell posits that the inherent paucity of advanced lifeforms complicates their detection as such a society would need to search and select a correct target star potentially hundreds of light years away. Given the geological timescale for the formation of an Earth-like planet, monitoring various radio telescopes would require operating these facilities for millions of years. Furthermore, the distances would result in large time-delays for information exchange between civilizations.

Bracewell instead provides a novel solution for detection of intelligent life by considering the search from the perspective of an advanced society (arguably, much more advanced than humanity). A society with comparably primitive scientific capabilities, such as ours, would be most focused on exploring their respective planetary neighborhood for life. An advanced society could exploit this by sending durable solar-powered probes equipped with radio transmitters to candidate systems (i.e. solar-like stars) as a means to garner the attention of the primitive society. The use of probes would provide an expansive radio-relay network capable of informing the advanced society while removing the need to select the correct star to observe, as is required by Cocconi & Morrison’s proposal. Bracewell also suggests the probes would potentially house artificial intelligence and a cache of pictorial information capable of communicating with the primitive society. The probe would actively listen for signals around the system and repeat these signals to the society to make itself known.

One of the largest limitations to Bracewell’s probes are the technological requirements. To this blogger, the technological descriptions can only be relegated to the realm of science fiction. This was perhaps most apparent in Bracewell’s comment that the probe could televise an image of a constellation. The flaw in Bracewell’s arguments are the various assumptions made including that (i) life should be around sun-like stars, (ii) intelligent life can create devices capable of analyzing and using electromagnetic radiation, (iii) a primitive society will readily decipher a signal from a probe, and (iv) an advanced society has fundamentally reached a point of quasi-permanence, allowing it to persist through the millions of years of development for a primitive society. It is difficult to argue for or against the use of probes when they rely on factors outside the scope of humanity’s scientific understanding (i.e. see Figure 1). There is also the issue that Bracewell’s probe should reach out to the civilization once it detects some radio emission. As of this writing, there is no evidence of contact by such a probe.

It should be noted there have been searches for Bracewell probes (i.e. Spaewatch at KPNO; Lunan & Gatland 1973, Spaceflight, 15, 122; SETA as described in Freitas Jr. & Valdes 1985, Acta Astronautica, 12, 12, 1027). The popularity of Bracewell’s idea is also emphasized by Wikipedia, which provides examples of how these probes have permeated science fiction. The search for such probes are ongoing but, to this blogger, the search for extraterrestrial artifacts may be the wrong approach in the search for life. A probe does not necessarily need to make contact to detect life. With the growing field of astrobiology and the quest for biomarkers of life, the need for a probe to transmit and directly communicate with a primitive society appears unnecessarily complex. Logic dictates that the absence of evidence is not evidence of absence such that the search for Bracewell probes will persist until we find an advanced civilization.

Figure 1: A Bracewell ProbeOne of the many images a quick Google search provides. The configuration of such a probe is limited by one’s imagination. Above is a self-replicating Bracewell probe that could theoretically propagate and populate an entire region of the galaxy. Source: David Daring, http://www.daviddarling.info/encyclopedia/B/Bracewellprobes.html 

Project OZMA

This paper is about the searching strategy for alien civilizations and the actual experiment associated with it. In this sense, the paper addressed two questions 1) what kind of signal we should be looking for 2) how we would conduct our experiment to search for this signal. The paper suggested three ways we could look for SETI signal 1) “searching  for radiation that other civilizations are using for their own purposes” 2) searching for radiation at 1420 MHz 3) “a passive observation with a very large telescope” to search all kinds of signals.

Then the author described the effort at Green Bank Observatory to look for signals at the nearest stars such as Tau Ceti and Epsilon Eridani. Two horns and two channels were used for this experiment. One horn was used for detecting SETI signals and the other horn was for detecting background noise. The detector they were using had one narrow band channel and one broadband channel, similar to the two horns would separate the real SETI signal from the background as the signal for SETI would be stronger in the narrow band compared to the broad band. The author also mentioned the use of Dicke radiometer and superheterodyne receiver to maintain the narrow band observations with bandwidth of 100 Hz.

I think the reason this paper was assigned is because project OZMA marks one of the earliest experimental efforts to search for SETI signal. There is one obvious error in the paper such as the age of our galaxy. The author assumed it to be 25 billion years. However, we know now the age of the universe is even smaller than this number. This could be due to the fact the Hubble constant was not refined at 1960s. Although almost 60 years have passed, we still have not detected any unequivocal signal which is definitely coming from alien civilizations. That could imply maybe the advanced alien civilizations might live further than we thought before. We should also consider looking for other frequencies. In this paper, the author observed the 21cm line because it was important to us. However, whether this frequency was important for alien civilizations is not clear. This is a circular problem because we do not know what the typical frequencies advanced civilizations might emit. The type of technology developed could be significantly different.

Drake 1961 – A Recapitulation and Review of Sorts

I guess this paper is a “meta” paper, since it discusses the requirements for extraterrestrial intelligence as well as one of the first SETI experiments.

The paper directly addresses the various problems surrounding the likeliness of us discovering intelligent life, in particular the mystery (now mostly solved) behind planetary formation, the mystery (slightly explained by Miller’s experiment) behind the formation of life, the timescale of life, and the timescale of intelligent, communicative life. The majority of the paper is a sort of thought experiment, where Drake goes point by point through his equation (not mentioned) and delves into specific factors effecting each of the compounding probabilities; he plays around with numbers that seem (to someone fairly unfamiliar with SETI) sound. However, as Drake points out, there is no way for us to be sure if he is correct or not unless and until we actually find life. I personally am glad he included this, since I feel with such statements, some might misconstrue his theory to be real and supported. The media nowadays would go nuts (perhaps they did then as well).

Drake also introduces Project Ozma, the first search for intelligent communications via the National Radio Astronomy Observatory. In this search, they followed up the suggestion by Coccini and Morrison 1959 and studied two of the closest solar-like stars for radio emission. Drake agreed with both Coccini and Morrison 1959 and Bracewell 1960 that a logical (possible the most logical) frequency to study would be that of the neutral hydrogen 21cm line, since civilizations early in their astronomical technologies would start here. These two stars, Tau Ceti and Epsilon Eridani, were studied for a total of 150 hours. No evidence for intelligent communications was found, nor was it really expected apparently. As far as I know, many searches similar to this have been made over the years, and I don’t think any have led to direct evidence.