We haven't found any technosignatures among the stars, but the field is young and our observational tools are improving steadily. It's worth asking how likely an advanced civilization will be to produce the kind of technosignature we usually discuss. A Dyson swarm should produce evidence for its existence in the infrared, but not all advanced technologies involve megastructures. Even today we can see the movement of human attention into cyberspace. Would a civilization living primarily within virtual worlds produce a detectable signature, or would it more or less wink out of observability? In 2020, Valentin Ivanov (ESO Paranal) and colleagues proposed a modification to the Kardashev scale based on how a civilization integrates with its environment (citation below). The authors offered a set of classes. Class 0 is a civilization that uses the environment without substantially changing it. Class 1 modifies its environment to fit its needs, while Class 2 modifies itself to fit its...
Attack of the Carbon Units
"The timescales for technological advance are but an instant compared to the timescales of the Darwinian natural selection that led to humanity's emergence -- and (more relevantly) they are less than a millionth of the vast expanses of cosmic time lying ahead." -- Martin Rees, On the Future: Prospects for Humanity (2018). by Henry Cordova This bulletin is meant to alert mobile units operating in or near Sector 2921 of a potential danger, namely intelligently directed, deliberately hostile, activity that has been detected there. The reports from the area have been incomplete and contradictory, fragmentary and garbled. This notice is not meant to fully describe this danger, its origins or possible countermeasures, but to alert units transiting near the area to exercise caution and to report on any unusual activity encountered. As more information is developed, a response to this threat will be devised. It is speculated that the nature of this hazard may be due to unusual manifestations...
Toward Kardashev Type I
It seems a good time to re-examine the venerable Kardashev scale marking how technological civilizations develop. After all, I drop Nikolai Kardashev's name into articles on a regular basis, and we routinely discuss whether a SETI detection might be of a particular Kardashev type. The Russian astronomer first proposed the scale in 1964 at the storied Byurakan conference on radio astronomy, and it has been discussed and extended as a way of gauging the energy use of technological cultures ever since. The Jet Propulsion Laboratory's Jonathan Jiang, working with an international team of collaborators, spurs this article through a new paper that analyzes when our culture could reach Kardashev Type I, so let's remind ourselves of just what Type I means. Kardashev wanted to consider how a civilization consumes energy, and defined Type I as being at the planetary level, with a power consumption of 1016 watts. This approximates a civilization using all the energy available from its home...
Interstellar Implications of the Electric Sail
Not long ago we looked at Greg Matloff’s paper on von Neumann probes, which made the case that even if self-reproducing probes were sent out only once every half million years (when a close stellar encounter occurs), there would be close to 70 billion systems occupied by such probes within a scant 18 million years. Matloff now considers interstellar migration in a different direction in a new paper addressing how M-dwarf civilizations might expand, and why electric sails could be their method. It’s an intriguing notion because M-dwarfs are by far the most numerous stars in the galaxy, and if we learn that they can support life, they might house vast numbers of civilizations with the capability of sending out interstellar craft. They’re also crippled in terms of electromagnetic flux when it comes to conventional solar sails, which is why the electric sail comes into play as a possible alternative, here analyzed in terms of feasibility and performance and its prospects for enabling...
Europa’s Double Ridges: Implications for a Habitable Ocean
I’m always interested in studies that cut across conventional boundaries, capturing new insights by applying data from what had appeared, at first glance, to be unrelated disciplines. Thus the news that the ice shell of Europa may turn out to be far more dynamic than we have previously considered is interesting in itself, given the implications for life in the Jovian moon’s ocean, but also compelling because it draws on a study that focused on Greenland and originally sought to measure climate change. The background here is that the Galileo mission that gave us our best views of Europa’s surface so far showed us that there are ‘double ridges’ on the moon. In fact, these ridge pairs flanked by a trough running between them are among the most common landforms on a surface packed with troughs, bands and chaos terrain. The researchers, led by Stanford PhD student Riley Culberg, found them oddly familiar. Culberg, whose field is electrical engineering (that multidisciplinary effect again)...
Good News for a Gravitational Focus Mission
We’ve talked about the ongoing work at the Jet Propulsion Society on the Sun’s gravitational focus at some length, most recently in JPL Work on a Gravitational Lensing Mission, where I looked at Slava Turyshev and team’s Phase II report to the NASA Innovative Advanced Concepts office. The team is now deep into the work on their Phase III NIAC study, with a new paper available in preprint form. Dr. Turyshev tells me it can be considered a summary as well as an extension of previous results, and today I want to look at the significance of one aspect of this extension. There are numerous reasons for getting a spacecraft to the distance needed to exploit the Sun’s gravitational lens – where the mass of our star bends the light of objects behind it to produce a lens with extraordinary properties. The paper, titled “Resolved Imaging of Exoplanets with the Solar Gravitational Lens,” notes that at optical or near-optical wavelengths, the amplification of light is on the order of ~ 2 X 1011,...
NASA Interstellar Probe: Overview and Prospects
A recent paper in Acta Astronautica reminds me that the Mission Concept Report on the Interstellar Probe mission has been available on the team's website since December. Titled Interstellar Probe: Humanity's Journey to Interstellar Space, this is the result of lengthy research out of Johns Hopkins Applied Physics Laboratory under the aegis of Ralph McNutt, who has served as principal investigator. I bring the mission concept up now because the new paper draws directly on the report and is essentially an overview to the community about the findings of this team. We've looked extensively at Interstellar Probe in these pages (see, for example, Interstellar Probe: Pushing Beyond Voyager and Assessing the Oberth Maneuver for Interstellar Probe, both from 2021). The work on this mission anticipates the Solar and Space Physics 2023-2032 Decadal Survey, and presents an analysis of what would be the first mission designed from the top down as an interstellar craft. In that sense, it could be...
Toward a Multilayer Interstellar Sail
Centauri Dreams tracks ongoing work on beamed sails out of the conviction that sail designs offer us the best hope of reaching another star system within this century, or at least, the next. No one knows how this will play out, of course, and a fusion breakthrough of spectacular nature could shift our thinking entirely – so, too, could advances in antimatter production, as Gerald Jackson’s work reminds us. But while we continue the effort on all alternative fronts, beamed sails currently have the edge. On that score, take note of a soon to be available two-volume set from Philip Lubin (UC-Santa Barbara), which covers the work he and his team have been doing under the name Project Starlight and DEEP-IN for some years now. This is laser-beamed propulsion to a lightsail, an idea picked up by Breakthrough Starshot and central to its planning. The Path to Transformational Space Exploration pulls together Lubin and team’s work for NASA’s Innovative Advanced Concepts office, as well as work...
AB Aurigae b: The Case for Disk Instability
What to make of a Jupiter-class planet that orbits its host star at a distance of 13.8 billion kilometers? This is well over twice the distance of Pluto from the Sun, out past the boundaries of what in our system is known as the Kuiper Belt. Moreover, this is a young world still in the process of formation. At nine Jupiter masses, it's hard to explain through conventional modeling, which sees gas giants growing through core accretion, steadily adding mass through progressive accumulation of circumstellar materials. Core accretion makes sense and seems to explain typical planet formation, with the primordial cloud around an infant star dense in dust grains that can accumulate into larger and larger objects, eventually growing into planetesimals and emerging as worlds. But the new planet - AB Aurigae b - shouldn't be there if core accretion were the only way to produce a planet. At these distances from the star, core accretion would take far longer than the age of the system to produce...
Ramping Up the Technosignature Search
In the ever growing realm of acronyms, you can't do much better than COSMIC - the Commensal Open-Source Multimode Interferometer Cluster Search for Extraterrestrial Intelligence. This is a collaboration between the SETI Institute and the National Radio Astronomy Observatory (NRAO), which operates the Very Large Array in New Mexico. The news out of COSMIC could not be better for technosignature hunters: Fiber optic amplifiers and splitters are now installed at each of the 27 VLA antennas. What that means is that COSMIC will have access to the complete datastream from the entire VLA, in effect an independent copy of everything the VLA observes. Now able to acquire VLA data, the researchers are proceeding with the development of high-performance Graphical Processing Unit (GPU) code for data analysis. Thus the search for signs of technology among the stars gains momentum at the VLA. Image: SETI Institute post-doctoral researchers, Dr Savin Varghese and Dr Chenoa Tremblay, in front of one...
Microlensing: K2’s Intriguing Find
Exoplanet science can look forward to a rash of discoveries involving gravitational microlensing. Consider: In 2023, the European Space Agency will launch Euclid, which although not designed as an exoplanet mission per se, will carry a wide-field infrared array capable of high resolution. ESA is considering an exoplanet microlensing survey for Euclid, which will be able to study the galactic bulge for up to 30 days twice per year, perhaps timed for the end of the craft’s cosmology program. Look toward crowded galactic center long enough and you just may see a star in the galaxy's disk move in front of a background star located much further away in that dense bulge. The result: The lensing phenomenon predicted by Einstein, with the light of the background star magnified by the intervening star. If that star has a planet, it's one we can detect even if it's relatively small, and even if it's widely spaced from its star. For its part, NASA plans to launch the Roman space telescope by...
Methane as Biosignature: A Conceptual Framework
A living world around another star will not be an easy catch, no matter how sophisticated the coming generation of space- and ground-based telescopes turns out to be. It’s one thing to develop the tools to begin probing an exoplanet atmosphere, but quite another to be able to say with any degree of confidence that the result we see is the result of biology. When we do begin picking up an interesting gas like methane, we’ll need to evaluate the finding against other atmospheric constituents, and the arguments will fly about non-biological sources for what might be a biosignature. This is going to begin playing out as the James Webb Space Telescope turns its eye on exoplanets, and methane is the one potential sign of life that should be within its range. We know that oxygen, ozone, methane and carbon dioxide are produced through biological activity on Earth, and we also know that each can be produced in the absence of life. The simultaneous presence of such gases is what would intrigue...
SETI as Exploration
Early exoplanet detections always startled my friends outside the astronomical community. Anxious for a planet something like the Earth, they found themselves looking at a 'hot Jupiter' like 51 Pegasi b, which at the time seemed like little more than a weird curiosity. A Jupiter-like planet hugging a star? More hot Jupiters followed, which led to the need to explain how exoplanet detection worked with radial velocity methods, and why big planets close to their star should turn up early in the hunt. Earlier, there were the pulsar planets, as found by Aleksander Wolszczan and Dale Frail around the pulsar PSR B1 257+12 in the constellation Virgo. These were interestingly small, but obviously accumulating a sleet of radiation from their primary. Detected a year later, PSR B1620-26 b was found to orbit a white dwarf/pulsar binary system. But these odd detections some 30 years ago actually made the case for the age of exoplanet discovery that was about to open, a truly golden era of deep...
A Hybrid Interstellar Mission Using Antimatter
Epsilon Eridani has always intrigued me because in astronomical terms, it's not all that far from the Sun. I can remember as a kid noting which stars were closest to us - the Centauri trio, Tau Ceti and Barnard's Star - wondering which of these would be the first to be visited by a probe from Earth. Later, I thought we would have quick confirmation of planets around Epsilon Eridani, since it's a scant (!) 10.5 light years out, but despite decades of radial velocity data, astronomers have only found one gas giant, and even that confirmation was slowed by noise-filled datasets. Even so, Epsilon Eridani b is confirmed. Also known as Ægir (named for a figure in Old Norse mythology), it's in a 3.5 AU orbit, circling the star every 7.4 years, with a mass somewhere between 0.6 and 1.5 times that of Jupiter. But there is more: We also get two asteroid belts in this system, as Gerald Jackson points out in his new paper on using antimatter for deceleration into nearby star systems, as well as...
Antimatter-driven Deceleration at Proxima Centauri
Although I've often seen Arthur Conan Doyle's Sherlock Holmes cited in various ways, I hadn't chased down the source of this famous quote: "When you have eliminated all which is impossible, then whatever remains, however improbable, must be the truth." Gerald Jackson's new paper identifies the story as Doyle's "The Adventure of the Blanched Soldier," which somehow escaped my attention when I read through the Sherlock Holmes corpus a couple of years back. I'm a great admirer of Doyle and love both Holmes and much of his other work, so it's good to get this citation straight. As I recall, Spock quotes Holmes to this effect in one of the Star Trek movies; this site's resident movie buffs will know which one, but I've forgotten. In any case, a Star Trek reference comes into useful play here because what Jackson (Hbar Technologies, LLC) is writing about is antimatter, a futuristic thing indeed, but also in Jackson's thinking a real candidate for a propulsion system that involves using...
An Abundance of Technosignatures?
What expectations do we bring to the hunt for life elsewhere in the universe? Opinions vary depending on who has the podium, but we can neatly divide the effort into two camps. The first looks for biosignatures, spurred by our remarkably growing and provocative catalog of exoplanets. The other explicitly looks for signs of technology, as exemplified by SETI, which from the start hunted for signals produced by intelligence. My guess is that a broad survey of those looking for biosignatures would find that they are excited by the emerging tools available to them, such as new generations of ground- and space-based telescopes, and the kind of modeling we saw in the last post applied to a hypothetical Alpha Centauri planet. We use our growing datasets to examine the nature of exoplanets and move beyond observation to model benchmarks for habitable worlds, including their atmospheric chemistry and even geology. Technosignatures are a different matter, and it's fascinating to read through a...
A New Title on Extraterrestrial Intelligence
Just a quick note for today as I finish up tomorrow's long post. But I did want you to be aware of this new title, Extraterrestrial Intelligence: Academic and Societal Implications, which has connections with recent topics and will again tomorrow, when we discuss a new paper from Jason Wright and SETI colleagues on technosignatures. As with the recent biography of John von Neumann, I haven't had the chance to read this yet, but it's certainly going on the list. The book is out of Cambridge Scholars Publishing. Here's the publisher's description: What are the implications for human society, and for our institutions of higher learning, of the discovery of a sophisticated extraterrestrial intelligence (ETI) operating on and around Earth? This book explores this timely question from a multidisciplinary perspective. It considers scientific, philosophical, theological, and interdisciplinary ways of thinking about the question, and it represents all viewpoints on how likely it is that an...
Modeling a Habitable Planet at Centauri A/B
Why is it so difficult to detect planets around Alpha Centauri? Proxima Centauri is one thing; we’ve found interesting worlds there, though this small, dim star has been a tough target, examined through decades of steadily improving equipment. But Centauri A and B, the G-class and K-class central binary here, have proven impenetrable. Given that we’ve found over 4500 planets around other stars, why the problem here? Proximity turns out to be a challenge in itself. Centauri A and B are in an orbit around a common barycenter, angled such that the light from one will contaminate the search around the other. It’s a 79-year orbit, with the distance between A and B varying from 35.6 AU to 11.2. You can think of them as, at their furthest, separated by the Sun’s distance from Pluto (roughly), and at their closest, by about the distance to Saturn. The good news is that we have a window from 2022 to 2035 in which, even as our observing tools continue to improve, the parameters of that orbit...
Why Fill a Galaxy with Self-Reproducing Probes?
We can’t know whether there is a probe from another civilization – a von Neumann probe of the sort we discussed in the previous post – in our own Solar System unless we look for it. Even then, though, we have no guarantee that such a probe can be found. The Solar System is a vast place, and even if we home in on the more obvious targets, such as the Moon, and near-Earth objects in stable orbits, a well hidden artifact a billion or so years old, likely designed not to draw attention to itself, is a tricky catch. As with any discussion of extraterrestrial civilizations, we’re left to ponder the possibilities and the likelihoods, acknowledging how little we know about whether life itself is widely found. One question opens up another. Abiogenesis may be spectacularly rare, or it may be commonplace. What we eventually find in the ice moons of the outer system should offer us some clues, but widespread life doesn’t itself translate into intelligent, tool-making life. But for today, let’s...
Probing von Neumann Expansion
Before getting into the paper I want to discuss today, I want to mention the new biography of John von Neumann by Ananyo Bhattacharya. I make no comment on The Man from the Future (W. W. Norton & Company, 2022) yet because while I have a copy, I haven't had time to read it. But be aware that it’s out there – it’s getting good reviews, and given the impact of this remarkable figure on everything from programmable computers to game theory and the interstellar dispersion of civilizations, it’s a book you’ll at least want to stick on your reference list. I figure anyone who masters calculus by the age of eight, as von Neumann is reputed to have done, is going to turn out to make a substantial contribution somewhere. I’m also interested in how polymaths function, moving with what seems effortless ease through diverse fields of study and somehow leaving their mark on each. What a contrast to our age of micro-specialization, where relentless drilling down into a single topic – and this...