Worldships: A Interview with Greg Matloff

The first conference devoted solely to worldships takes place today in London at the headquarters of the British Interplanetary Society. It seemed a good time to check in with Gregory Matloff, a man I described when writing Centauri Dreams (the book) as the ‘renaissance man of interstellar studies.’ Perhaps best known for his continuing work on solar sails, Matloff’s interests have nonetheless ranged widely. He brought deep space propulsion to a wide audience in his book The Starflight Handbook (1989), which covers the full spectrum of interstellar options, but for over three decades has continued to produce scientific papers investigating issues ranging from laser ramjets to beamed microwave missions. A recent interest has been the expansion of the human biosphere into space, as discussed in books like Paradise Regained: The Regreening of Earth (Springer, 2009) and the soon to be published Biosphere Extension: Solar System Resources for the Earth, written with C Bangs. These last titles indicate that the interest in worldships Matloff first cultivated in papers for JBIS in the early 1980s continues to burn bright, as the following will confirm.

PG: Greg, I know you have a paper slated for the worldship conference that the British Interplanetary Society is holding today in London even though you couldn’t be there in person. And I know you’ve also been drafted by the Benfords to give a talk at the 100 Year Starship conference coming up in Orlando in October. When I first surveyed the field for my Centauri Dreams book back in 2004, I learned you were one of the early voices on this intriguing concept, the idea that a spacecraft might become a vast habitat capable of carrying thousands, even hundreds of thousands, of people between the stars.

GM: I was one of the early scientific writers who addressed the idea. The concept itself goes back to the 1930s and even earlier. Worldships are mentioned in a philosophical essay by J. D. Bernal, The World the Flesh and the Devil (1929). There is also an absolutely wonderful science fiction novel by Olaf Stapledon called Starmaker (1937). He not only talks about world ships but also implies that stars themselves are conscious.

PG: The 1930s were an extraordinarily productive period both for science and science fiction.

GM: Extremely productive.There was a literary group at Oxford University that has become justly famous. C.S. Lewis and J.R.R. Tolkien took part in this, and Stapledon was often discussed. I would have loved to have been there to have heard these guys kicking their ideas around in the era before World War II, a time when they all knew what was coming. It must have been fabulous. The worldship idea then disappears, although Tsiolkovsky mentions it when talking about space greenhouses and things like that. He doesn’t really develop it, and nobody touches it to my knowledge until the 1970s.

Then came Dandridge Cole, before Gerard O’Neill comes onto the scene, talking about ‘macrolife’ and the possibility of hollowing out asteroids to create workable habitats. Gerard O’Neill himself is important because he takes the idea and makes it concrete. O’Neill had major people working for him, such as Brian O’Leary, who was an astronaut, and Thomas Heppenheimer, who becomes a well known space writer. Eric Drexler would became the co-founder of the field of nanotechnology. So these are very bright folks, and they worked with O’Neill on the space colonies. O’Neill somewhere in there quotes Stapledon, and Arthur Clarke refers to him as a true science fiction visionary. He’s referring to Starmaker.

Image: Dandridge Cole, who coined the term ‘macrolife’ to refer to human colonies in space and their evolution. Credit: Wikimedia Commons.

PG: Are worldships a theme in science fiction today?

GM: I found in the last 30 years maybe a couple of pieces, including Greg Benford and David Brin with Heart of the Comet (1986). People are hollowing out Halley’s comet and making it livable. The book also speculates about uploading of the human essence into a computer and things like that. What seems to have happened in science fiction in the last 20 or 30 years is to me many steps back. We’ve gone in the direction of military science fiction on the one hand and fantasy on the other. I go in looking for science fiction and would like to buy something but it’s very hard for me to find something in a Barnes & Noble that I’d like to buy. That to me is sort of depressing.

Looking Inward: Prospects and Consequences

PG: This seems to be a long way from the intense vision of the 1930s.

GM: Exactly. Now it is possible that we might be doing inward exploration rather than outward exploration. A recent book we purchased is How the Hippies Saved Physics, by David Kaiser (2011). The book talks about folks who started to apply quantum mechanics to human consciousness. It turns out C and I knew one of them fairly well, Evan Harris Walker, who died a few years ago. He was very much involved in this approach. I think what happened is that inward exploration, probably because of the 70s, had replaced outward exploration in many peoples’ minds. There may be some sense to it because people in the 70s thought they could do exploration by taking a pill or something similar. Later on learning how to do it by meditation and yoga comes to seem easier than funding a trillion dollar project to launch a few people into deep space.

PG: Just as setting up computerized VR is easier. Maybe we’re still going in the same direction.

GM: Yes, I think so. In fact, about two years ago, in October of 2009, C and I went to a meeting of singularity people. We were guests of Greg Benford. It was very interesting to hear these brilliant mathematicians talking about a virtual reality and folding human consciousness into it. Its a seductive thought. Now, is it more seductive than SETI? Is it more seductive than actually going out and colonizing new worlds or spreading the biosphere beyond the Earth — I don’t know!

I run into this with students all the time. Some of them are much more interested in inner exploration than outer exploration, and I don’t have any answers for this, except that I do hope that we also extend the biosphere, because I think it should be a goal of technological consciousness. It’s something we can do and it’s something we should do rather than having everybody just living in a little box. You and I may turn out to be in the minority on this.

Image: Olaf Stapledon, whose vision became a focal point for C.S. Lewis and J.R.R. Tolkien, and influenced Lewis’ subsequent science fiction, which was partly written in response to Stapledon’s ideas.

Near-Term Drivers for a Worldship

PG: Could be, but I suppose the worldship concept is sort of the ultimate extension of the expansion of the biosphere. Because these are gigantic vessels. Just how big are they?

GM: There are various estimates of the size of a worldship. If we’re talking about an interstellar ark, something that is like living in a submarine, it’s something that may be the size of a submarine. This is Edward Gilfillan in the 1970s

. The Outsiders are doing exactly that, traveling in worldships, and they consider it nearly low class to travel at a speed greater than one or two percent of the speed of light.

PG: I love that because it’s such a reversal of conventional thinking. Everyone is trying to go as fast as possible, and at the same time we all have the sense of short-term horizons. Here we’re saying, what’s your rush? And if we don’t get there in this generation, maybe we can in the next, or maybe in a hundred generations.

GM: Exactly. And that’s what they do. As I recall, the reason that terrestrials developed hyperdrive in these stories is that it’s a trade item for the Outsiders. They don’t care about things like that, but they’re trading for the things they want. Sure, hyperdrive is an interesting technique; it allows you to go fast if you want, but to us the voyage is the more important thing.

PG: I love the Niven stories of that era. Now you remind me I must go back and do some re-reading of those tales.

GM: Sure! They’re fabulous. And the more I think about it, the more significant science fiction is to science. Visionary science fiction is very, very important. People like Clarke, Asimov, Stapledon. Asimov does speculate that the early migrations from Earth are by worldships. He calls them interstellar arks.

PG: In which books?

GM: In the Foundation series, he does mention that the ruins of some of these arks are discovered around planets orbiting various stars, including one or two planets in the Alpha Centauri system, and they’re not sure where they come from. One of the speculations is that they come from Sol originally, 50,000 years ago. But the records have been lost.

The Worldship and the Sail

PG: Greg, although you are not going to London for the worldship conference, I know a paper of yours will be presented there on the question of using a sail for propusion. Tell us more about that.

GM: What has happened with the sail is that we know that solar sails are the only propulsion system for interstellar travel that people have suggested to date that can be used for acceleration, deceleration and cosmic ray shielding enroute. Because you simply wind it around the habitat. So it’s a tri-use device, which none of the others methods have. And what I do is I review a lot of the literature including acceleration and deceleration and I talk about the fact that right now the most investigated sail material is beryllium. People at NASA hate that.

Image: John Desmond Bernal, a British physicist and crystallographer whose The World, The Flesh & The Devil (1929) investigated a human presence in worldships and discussed the possibilities of solar sailing long before it became fodder for scientific papers.

Les Johnson [NASA MSFC] was at a conference in Aosta, I forget if that’s the one you were at, and when I described the work of a beryllium sail, he did a wonderful imitation of Indiana Jones and said, “Oh no, why did it have to be beryllium?” Because he’s making a very good point. If NASA wishes to build an Oort Cloud explorer which is going to be a small scale 2000 year ark — and in fifty or sixty years they could build this to demonstrate a prototype interstellar spacecraft and also to do exploration of the Oort Cloud — right now beryllium is their only candidate for the sail, but beryllium is also very toxic. Les was saying if we do this, we’re going to have to deal with huge losses and tremendous safety issues. I understood his point, but technology is changing very rapidly.

There are things like carbon nanotubes and more recently graphene. These are interesting because they could have thickness measured in nanometers. Maybe a couple of molecules thick. They would have a finite either reflectivity or absorptivity, which means even though they are extremely low in mass, they are very strong. They’re going to be pushed by photons. So you could certainly imagine lowering the interstellar transit time with the sail to something like a millennium, maybe even lower than that. I don’t know. I would hesitate to say that we’ve discovered everything.

PG: I actually remember Les saying that about beryllium two years ago in Aosta. But you’re saying that these possibilities are going to be significantly thinner than anything we might do with beryllium?

GM: I think they’ll be both thinner and stronger than what we’re doing with beryllium, and they may not be toxic to work with. Right now they are amazingly expensive. If you were going to come up with enough graphene to cover a postage stamp, it would cost something like a hundred million dollars. So to build a real starship would bankrupt the planet. Even if we paid it out over a century. So the graphene price has to come down by many orders of magnitude.

One person at the Aosta congress did suggest that this isn’t impossible because this is what happened with aluminum. Aluminum when it first became recognized as a possibly significant commercial metal, probably a century and a half ago, was remarkably expensive. But a number of commercial processes were developed and the price began to drop dramatically. And as it dropped, people found more and more applications, driving the price down still further.

PG: What sort of mission configuration would you foresee? We can talk about a close solar pass, but our colonists are not in any great rush anyway, are they?

GM: They’re not. If you are using graphene, you might even be able to start with something like Earth orbit to get there in a thousand years. Because it’s very, very thin. A lot depends upon how its reflectivity or absorptivity varies with temperature. We really don’t know much about this material at this point to any great depth. I’m going to be talking about this also in Orlando, and presenting some of the numbers one of the guys presented at Aosta. But it’s not something you can get your hand around at this point. It’s still a brand new material that’s extremely difficult to work with. It’s very expensive, and there are only a handful of labs on the planet that can fabricate the stuff. So right now it’s a scientific material but not yet an engineering material.

Life Within the Colossus

But I do think if you’re going to extrapolate how to engineer a worldship, you would think about something that is a small version of an O’Neill colony. It maybe has the dimensions of a small skyscraper, maybe a hundred meters high, twenty meters across. That’s the payload. The payload might mass something like 107 kilograms if it’s using a 2000 year beryllium sail, an inflatable sail, maybe the sail size is 600-700 kilometers.

PG: Huge sociological issues come into play when we’re talking about millennial voyages.

GM: Our crew would have to deal with interesting sociological matters. How do we become a society that stays intact for that long? And it was interesting that Arthur C. Clarke was not an optimist about the sociology. He was an optimist about the technology. In one of the Rama novels [in the series that began with Rendezvous with Rama, 1972], Rama was an alien worldship that comes to the solar system and aliens invite the terrestrials to fly a ship out and colonize it and live there with some of the aliens. Ultimately a few thousand terrestrials take advantage of this, and they have to decide how to live on this worldship. They decide to have a society with a lot of sports events, so they build stadiums for these. What happens is one of the major team players says I can take this place over. And he develops a cadre of fellows to work with him who enslave or massacre the other males and the various women become sex slaves.

He develops a fascist state with him on top. And what happens is one of the women revolts and she is able to get in contact with the worldship intelligence, which is the supreme intelligence of the universe, so she has a good deal of help, and because of this there is a very successful revolution. But OK. In any event, what Clarke is presenting there is pessimism about sociology and so was Heinlein in ‘Universe’/’Common Sense’ in the early 1940s. He has a worldship going between Earth and Centauri and the society falls apart. So basically all the people assume this is their universe. These two stories became the novel Orphans of the Sky, published as such in 1963.

It’s a brilliant story and of course the protagonists break in somehow to the holy of holies, the control room, they see what the stars are, they learn about the universe and they just happen to be passing through a solar system which is probably the Centauri system and there happens to be a livable planet. Somehow the shuttlecraft is operable by non-experts and they are able to elicit a landing. OK, Heinlein was playing the odds to have a happy ending to the thing, but the sociology is going to be a major factor because we haven’t had small human communities isolated for that long. There have been a couple of experiments and their results aren’t that good.

One of the experiments is the Vikings in Vinland. And when you look at that, the Vikings come and settle a small colony in Vinland [the account is told in the Saga of the Greenlanders]. One of the women is Freydis, the daughter of Erik the Red, who decides it’s too cold in the winter. She wants to be warmer, and why must she have only one male to snuggle up with? So she slaughters all her sisters and she has all the men now. This is in a small colony and they have nothing to do with the surrounding people, who they call Skraelings, the native Americans. So that’s an example maybe of a space colony gone wrong and becoming a tragedy.

Image: Robert Heinlein was one of a number of science fiction writers of his time who investigated the potential — and the problems — of worldships. Credit: The Heinlein Trust.

PG: On the other hand, I suppose one potential cause for optimism would be that a large enough worldship is going to have quite a large population, so perhaps that kind of diversity might play to survival. But I think the larger point you make is exactly in tune with the upcoming starship conference, mainly that while we usually think of interstellar ideas in terms of the propulsion that would get a probe there, the field actually demands a multidisciplinary approach.

GM: Very true. You make a good point about having a large population and I think O’Neill speculates that for a space habitat to be self-sufficient, it needs a population of something approaching a hundred thousand. Certainly tens of thousands of people. Then you have to say, what are they all going to do? If you have a large population like this, what will they do between stars? You have to design a ship in such a way that maybe the ship is never completely finished. Maybe the ecology always needs adjustment for it to work. Or maybe you have a second ship launched with materials to be mined as needed. Going out to the second ship and mining that becomes one of the periodical heroic episodes for this enclosed culture. Because look at the fact that we do seem to need heroes, in war or hopefully more frequently in sports. Look at the number of sports the industrialized and developed world practices today, and that’s to keep sane. That is largely to take the people who would be actual warriors and give them a role in society so they don’t have to go around other countries hacking off peoples’ heads.

A Multidisciplinary Study

PG: So all these things point us in the direction of the need to assess sociology, philosophy, history, to look at how humans have done in other settings when they’re in remote places.

GM: Yes. I would love to know the early history of the Minoan colonies in places like what is now Gaza. Or when the Minoan/Mycenaean peoples colonized Miletus in Asia Minor. Miletus becomes the parent for Russia, for many of the eastern European countries, because many of the people from there starting in about 1000 BC begin to build colony cities around the Black Sea area. I would love to know how many of these succeeded, how many failed, what the interaction was. Did they war with each other, did they war with the indigenous populations? I’m likewise fascinated with the early story of the Etruscans. They were obviously strongly influenced by the Minoan/Mycenaean civilization, but how did they do this? Were they a direct colony? We’ll probably never know. Or were they indigenous people who traded to try to build their own cities?

PG: You mentioned the possibility of having a second ship that might have resources the first could exploit. Is there an argument to be made that human nature says in any case a second ship is a good idea because you need to have a neighbor, a potential other, out there with you?

GM: It’s a possibility, that you might send instead of one ship a small fleet, particularly if you’re using something like a solar sail or a photon sail or maybe even an electric sail — you don’t have to pay for the propulsion. And in either case like this, conceivably, you could send as many colonies or habitats as wanted to go. That may offer something like this, because they could trade with each other, maybe they could have political or athletic contests with each other, maybe even there could be some form of highly ritualized warfare. I know that warfare among some of the native American population was initially very ritualized in just such a fashion. So we might be able to find all types of possible models in history and pre-history to go with.

PG: This discussion harkens back to that wonderful 1983 conference Interstellar Migration and the Human Experience, where you did have a very multidisciplinary group coming together to look at this kind of question, relating the topic to events like the settlement of the Pacific islands.

GM: Yes, that’s exactly what Ben Finney did. Unfortunately, I was not at that conference [held at Los Alamos in 1983], and always wish I had been. I’ve never met Ben Finney and would like to. I’m hoping he’s at the 100 Year Starship conference.

PG: Same here. I’m looking forward to seeing you at that conference, Greg, and want to thank you for your time this evening. As always, it has been a pleasure to talk to you.

Addendum: Kelvin Long sends via his smartphone this shot of the lunching worldship conference crew at the BIS headquarters where, as I post this (1600 UTC), the event should be just wrapping up.

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Report on the 2011 Mars Society Annual Convention

by Richard Obousy

After a stint as project leader for the Project Icarus starship design study, Richard Obousy now serves as Module Lead Primary Propulsion for the effort. Dr. Obousy’s doctoral work at Baylor University focused on the possibility that dark energy could be an artifact of Casimir energy in extra dimensions. For Icarus, he has pivoted to the study of fusion propulsion systems for this ongoing reworking of the original Project Daedalus concept. He’s also fascinated with the possibilities of getting off our planet more easily and establishing a human presence on Mars, all ideas he was able to explore at the Mars Society’s latest meeting, from which this report.

As a native of Texas, living only a couple of hours drive from Dallas, I was thrilled to discover that that was where the Mars Society planned to hold its 14th International Mars Society Convention. This was a perfect opportunity for me to meet space enthusiasts, to present to this community some of the ideas coming out of Project Icarus, and to learn from a successful non-profit foundation how to engage with its members, while delivering something valuable to the field of Mars research.

For those not familiar with the Mars Society, it is a non-profit charity founded in 1998 by Mars exploration luminary Bob Zubrin. The society is devoted to the cause of exploring and, ultimately settling, the red planet. The society has over 4,000 members and is active in over 50 countries worldwide. A large number of volunteers engage in public outreach programs in an effort to foster support for Mars research and exploration, and a notable feature of the society is its commitment to ongoing technical projects – the most exciting of which are arguably the research stations that the society has set up in hostile environments. The purpose of these research stations is to simulate the conditions and environment that early Mars explorers might face. Currently there are research stations in both an arctic environment and a desert environment, representing evidence for what can be accomplished by a devoted collection of volunteers.

The conference itself spanned four days, as numerous presentations relating to Mars exploration were delivered by a selection of scientists, engineers, and private hobbyists. An entire afternoon session was devoted to the topic of nuclear rockets and several of the original engineers involved in the NERVA (Nuclear Engine for Rocket Vehicle Exploration) program presented. NERVA was a fascinating facet of the US space research program, leading to nuclear rocket engines actually being certified as flight worthy in the late 60s, after extensive testing. The untimely cancellation of NERVA was largely a result of the Nixon administration’s lack of interest in the manned exploration of Mars, which it saw as both costly and strategically irrelevant, with the space race already ‘won’ after the successful Apollo moon landings.

One talk that still resonates with me was given by Dr. John Hunter, an ex-theoretical physicist turned space engineer. Hunter is the director of Quicklaunch, a company planning to use a light gas gun to launch payloads into space. The basic idea behind the gas gun is to use a large piston which imparts force to a gaseous working fluid through a smaller diameter barrel which contains the projectile to be accelerated. The gun that Hunter is working on gives the projectile, a single stage rocket engine plus payload, an initial speed of 6 km/s which launches it to approximately 100 km altitude.

Image: Quicklaunch’s larger QL-1000 systems will be built after the smaller QL-100 versions have proven high reliability. Each QL-1000 is a $500M system delivering up to 5 launches/day. After servicing one customer they can switch azimuth and launch angle to accommodate a different customer. At T=0 the vehicle leaves the muzzle and the four sabot petals are stripped away. Meanwhile the muffler closes behind the vehicle, capturing 99% of the hydrogen to be recycled. Credit: Quicklaunch.

At this point, the rocket engine fires and gives the projectile the final kick it needs to circularize its orbit. Using this technique, Hunter believes that he will be able to attain launch costs of $500/lb. Contrast this with the Space Shuttle costs of around $10,000/lb and the economics quickly makes sense. Even Elon Musk’s heavy Falcon launcher will be around the $1000/lb mark, so Hunter’s gas gun looks like an attractive option! One obvious limitation is that the high gee forces (~100 g’s) experienced during the initial launch exclude the possibility of human passengers, and so the gas gun will likely focus on launching propellant payloads. The resulting fuel ‘depots’ could enable future manned lunar and Mars exploration, if Quicklaunch were used in tandem with traditional launch systems. I encourage anyone interested in this fascinating technology to take a look at the Quicklaunch website which contains more details on their plans and accomplishments to date.

Image: Quicklaunch in Earth orbit. At T=9 minutes final maneuvering is performed until the vehicle docks with the depot. At that point a line is opened allowing the propellant to communicate with the rest of the depot. Propellant types will include both storable and cryogenics. Standard propellants are RP-1, LH2 and LOX. In addition xenon, argon and water can be delivered. Credit: Quicklaunch.

Zubrin himself gave a fascinating talk titled “VASIMR: Hoax or Silver Bullet,” arguing hotly that Chang-Diaz’s VASIMR is unlikely to produce any better efficiency than current ion engines, and that the promises being made regarding the utility of the engine are exaggerated. Zubrin believes that research into VASIMR is nothing more than a distraction, since NASA is adopting the mindset that the VASIMR is a necessary technological precursor for a manned mission to Mars. Zubrin argues that a manned Mars landing can be accomplished using off-the-shelf technology available today, for a small fraction of the $450 billion price tag that NASA initially suggested in the “90-day Study” in 1989.

Another of Zubrin’s talks, titled the “Transorbital Railroad,” urges NASA to devote a budget of $1.2 billion per year to pay for launches, possibly using SpaceX technology, to deliver payloads into orbit. The payload mass would be sold to paying customers at $50/kg, and if there were unused payload space, this could be filled with tanks containing water, kerosene and liquid oxygen. These tanks would then be left in orbit and made available to anyone who could reach them. Using the Falcon Heavy launch vehicle, Zubrin estimates that 765 metric tonnes could be launched annually. The main thrust behind this heavily government subsidized plan would be to create a space-based economic sector welcoming to entrepreneurs. His belief is that the tax revenues that would be generated from this endeavor would pay for the Transorbital Railroad many times over. The name Transorbital Railroad is adopted from the history of the settlement of the American West, where the building of the Transcontinental Railroad opened up a plethora of economic opportunities for Americans of the era.

Image: Mars Society founder Robert Zubrin. Credit: The Mars Society.

There were many more talks at the conference, equally worthy of discussion, but the ones reviewed here probably had the biggest impact on me for one reason or another. I was happy to meet with Bob Zubrin at the speakers party one night, and share with him some of the exciting work being conducted by Project Icarus, which was met with enthusiasm by Bob – a former nuclear engineer. Being involved in the area of interstellar research, I was reaching, somewhat, into a community whose goals vary from my own field. However, I felt that there was a common theme and a collective unity that binds the Mars Society with those of non-profits like the Tau Zero Foundation and Icarus Interstellar – namely a core of dedicated volunteers pushing a vision forward, while being supported by a network of collaborators spread across the globe. The success of the Mars Society is a testament to what can be accomplished by such volunteers and I was genuinely happy to be a part of that last weekend.

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Heinlein and the 100 Year Starship Study

Anyone who looks back on Robert Heinlein’s ‘juvenile’ novels, twelve books written for young adults between 1947 and 1958, as inspiration for his current work gets my attention. I loved every one of those novels, particularly Citizen of the Galaxy (1957) and Starman Jones (1953), but David Neyland says it was Time for the Stars (1956) that got him thinking about the 100 Year Starship Study. If you’ve been keeping up with Centauri Dreams, you know that the Defense Advanced Research Projects Agency (DARPA), which handles cutting-edge research and development for the US military, is putting on a starship symposium this fall in Orlando, FL.

This follows up on the earlier DARPA Request for Information and will lead to the award of $500,000 or so in seed money to an organization that can best pursue the study’s goals. Neyland, who is director of DARPA’s Tactical Technology Office, has been explaining what the study is all about to newspapers like the Los Angeles Times, which ran a story on it on August 6. Heinlein’s books came up naturally in the interview, for it turns out that Neyland was quite a science fiction reader in his youth and found Time for the Stars a natural fit with his mission to inspire a new generation of scientists and engineers with the dream of starflight. The key to the linkage is Heinlein’s use of a foundation that would facilitate long-term thinking and planning.

Thus the Long Range Foundation, which in the novel creates technologies that take generations to deliver, but eventually benefit not a single government or corporation but the entire species. In the book, twins Tom and Pat Bartlett turn out to have telepathic talents that allow them to communicate with each other instantaneously, and other twins display the same gift. It’s a useful trait because it appears that using such twins is the only way to stay in touch with a far-ranging starship. Thus a representative of the Long Range Foundation comes to visit the twins and their father, where we learn about the background of the organization, as told by Tom Bartlett:

Its coat of arms reads: “Bread Cast Upon the Waters,” and its charter is headed: “Dedicated to the Welfare of Our Descendants.” The charter goes on with a lot of lawyers’ fog but the way the directors have interpreted it has been to spend money only on things that no government and no other corporation would touch. It wasn’t enough for a proposed project to be interesting to science or socially desirable; it also had to be so horribly expensive that no one else would touch it and the prospective results had to lie so far in the future that it could not be justified to taxpayers or shareholders. To make the LRF directors light up with enthusiasm you had to suggest something that cost a billion or more and probably wouldn’t show results for ten generations, if ever … something like how to control the weather (they’re working on that) or where does your lap go when you stand up.

It turns out, of course, that a foundation like this pays off in a big way, having developed a number of exploratory starships called ‘torchships’ that can reach a substantial percentage of the speed of light, more than enough for time dilation to kick in. And as the young Bartlett reflects upon a school paper he has written on it, he realizes that the Long Range Foundation (LRF) has been having the desired effect for some time:

Mr. McKeefe had told us to estimate the influence, if any, of LRF on the technology “yeast-form” growth curve; either I should have flunked the course or LRF had kept the curve from leveling off early in the 21st century – I mean to say, the “cultural inheritance,” the accumulation of knowledge and wealth that keeps us from being savages, had increased greatly as a result of the tax-free status of such non-profit research corporations. I didn’t dream up that opinion; there are figures to prove it. What would have happened if the tribal elders had forced Ugh to hunt with the rest of the tribe instead of staying home and whittling out the first wheel while the idea was bright in his mind?

Neyland credits Heinlein, then, with the notion that inspired the 100 Year Starship Study, but he also points to Jules Verne, whose From the Earth to the Moon appeared in 1865. The point of such books isn’t that they were accurate in terms of the actual technologies involved — Verne shot his crew off to the Moon from a giant cannon in ways that would have mashed them to a pulp — but that they inspired people to think about the larger topic of traveling on such a momentous journey. And Neyland noticed that it was just over 100 years later that Apollo 11 set down at the Sea of Tranquility. Like Verne, then, we may not have all the answers about starflight (to say the least) but a starship study may inspire people to ask the right questions and think big.

At a press conference in June, Neyland spoke to journalists about the study (see this Centauri Dreams story on the event), noting that in the Request for Information period that produced over 150 responses, some people had misconstrued the study’s intent. DARPA has no plans to build a starship, in other words, but to develop understanding about how research into such long range matters can be conducted, and to encourage the inevitable spinoffs as such studies are pursued. Hence the planned award to a single group that can become the locus of interstellar studies over a long time period (and if none is deemed suitable, DARPA won’t disburse the money). Here’s how he describes the study’s true goals, as told to the Times:

A lot of folks think that we’re asking for somebody to come in with a plan on how to build a starship. That’s actually the wrong answer. What we’re looking for is an intuitive understanding of the process of inspiring research and development that comes up with tangible products.

“Products” doesn’t mean physical products, but might be a new computer algorithm, a new kind of physics, a new set of mathematics, a new philosophical or religious construct, a new way of growing grain hydroponically. The organization needs to have the gestalt of how to inspire that kind of research.

Will we, in the same hundred year stretch that separated Verne from Apollo, develop the technologies we need for an actual trip between the stars? It’s an energizing thought, but from our perspective today we have no way of knowing. Nonetheless, the idea of creating an organization that can shepherd various approaches to a starship — and this is a multi-disciplinary undertaking that ranges from physics to biology to sociology and more — is one that surely captures the imagination. What spinoffs it might generate along the way are open to conjecture. Unlike so much in today’s world, the project is inherently long-term, looks out well beyond current lifetimes, and asks what will produce results not just for us but for future generations as well.

The agenda for the 100 Year Starship Study symposium is now available online [but see Jim Benford’s comment below]. And if Heinlein’s Time for the Stars is what led David Neyland to this, maybe it’s time for me to re-read it. “We know the questions to ask, but we don’t know all the questions to ask,” Neyland told the Times. “We can hypothesize where we want to get to, but it’s a pretty broad target that we’re aiming for.” A broad target indeed, and it’s high time we began gathering the resources that, if interstellar flight one day proves not just possible but practical, will eventually lead us to a mission.

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Studying the Darkest World

A planet orbiting the star GSC 03549-02811, about 750 light years away in direction of the constellation Draco, is showing us a new way of extracting information about a distant system. The planet is a gas giant called TrES-2b, discovered by the Trans-Atlantic Exoplanet Survey in 2006. Studying the star using data from Kepler observations over a span of 50 orbits, David Kipping (Harvard-Smithsonian Center for Astrophysics) and David Spiegel (Princeton University) have detected the faint brightness variations caused by planetary phase changes during its orbits. The light from the planet dims and brightens as it moves through its phases around the star.

“In other words, Kepler was able to directly detect visible light coming from the planet itself,” says Kipping, and what we’ve learned is that TrES-2b is remarkably dark, reflecting less than one percent of the sunlight falling on it. The planet is blacker than any moon or planet in our solar system, as black as coal, or in Kipping’s analogy, “less reflective than black acrylic paint.” That’s quite a contrast with Jupiter, whose ammonia clouds reflect more than a third of incoming sunlight, creating a notably bright object, as anyone who enjoys taking walks at night and looking at the sky can attest.

But TrES-2b is similar to Jupiter only in its mass. This is a world that reaches temperatures of more than 1000 degrees Celsius, making ammonia clouds impossible. It’s no surprise that ‘hot Jupiters’ like this should be dark because of light-absorbing chemicals like vaporized sodium and potassium or gaseous titanium oxide in the atmosphere, all of which would lead to low albedos of a few percent. But a puzzle remains. The team went on to combine the Kepler measurements with Spitzer and ground-based data, all of which suggest, as the paper on this work reports, that there is an extra ‘absorber’ that contributes to the blackness of TrES-2b:

… models with no extra absorber are completely inconsistent with observations, even on the basis of the Kepler data alone. The upshot is that some extra opacity source appears to be required to explain the emergent radiation from this extremely dark world. Owing to this optical opacity, our models that are consistent with the data have thermal inversions in their upper atmosphere…

It’s remarkable to me that using just four months of Kepler photometry, Kipping and Spiegel have been able to detect light from the darkest exoplanet yet found. But the high-precision photometry allowed by a Kepler or CoRoT is now coming into its own, with detections already reported of phase variations for planets like CoRoT-1b, HAT-P-7b, CoRoT-3b and Kepler-7b. Thus a technique that has already been tested and refined through long use in studying eclipsing binary stars is emerging thanks to space-based instruments as a factor in understanding exoplanets, even when, like TrES-2b, they are at the very lowest limits of detectability.

The paper is Kipping and Spiegel, “Detection of visible light from the darkest world,” accepted by Monthly Notices of the Royal Astronomical Society Letters (preprint).

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New Evidence for Life’s Precursors in Space

Is there a ‘goldilocks’ class of meteorite, one in which we can say that conditions were just right for producing the stuff of life? That’s one of the conclusions scientists at NASA’s Goddard Space Flight Center are reaching by studying samples taken from twelve carbon-rich meteorites, nine of them recovered from Antarctica. Their evidence shows that some of the building blocks of DNA, which carries the genetic blueprint for life, were most likely created in space before falling to Earth through meteorite and comet impacts. Thus we move closer to answering a key question:

“People have been discovering components of DNA in meteorites since the 1960’s, but researchers were unsure whether they were really created in space or if instead they came from contamination by terrestrial life,” said Dr. Michael Callahan of NASA’s Goddard Space Flight Center, Greenbelt, Md. “For the first time, we have three lines of evidence that together give us confidence these DNA building blocks actually were created in space.”

Grinding up samples of the meteorites, the Goddard team went to work with a liquid chromatograph and a mass spectrometer to separate and study the chemical structure of the compounds inside. What they found were adenine and guanine, nucleobases that connect with two other nucelobases to form the rungs of the DNA ladder. Nucleobases are essential to life. Appearing with them were hypoxanthine and xanthine, which are not found in DNA but do appear in other biological processes.

So far so good, but the question of separating these materials from possible terrestrial contamination remains. The next part of the story is thus significant. In two of the meteorites, traces of three molecules structurally similar to nucleobases showed up: purine, 2,6-diaminopurine, and 6,8-diaminopurine. This news release from GSFC points out that the latter two are almost never used in biology. Callahan says these ‘nucleobase analogs’ point to an origin in space:

“You would not expect to see these nucleobase analogs if contamination from terrestrial life was the source, because they’re not used in biology, aside from one report of 2,6-diaminopurine occurring in a virus (cyanophage S-2L). However, if asteroids are behaving like chemical ‘factories’ cranking out prebiotic material, you would expect them to produce many variants of nucleobases, not just the biological ones, due to the wide variety of ingredients and conditions in each asteroid.”

Image: Meteorites contain a large variety of nucleobases, an essential building block of DNA. (Artist concept credit: NASA’s Goddard Space Flight Center/Chris Smith).

So that’s one line of evidence pointing to a non-terrestrial origin, but usefully, it’s not the last. The next step was to analyze an eight-kilogram sample of Antarctic ice using the same methods as were used with the meteorites. The amounts of the two nucleobases, plus hypoxanthine and xanthine, in the ice were much lower than in the meteorites, and none of the nucleobase analogs were found in the ice sample. As an additional check, the team analyzed Australian soil near the fall site of one of the meteorites — the Murchison meteorite — with nucleobase analog molecules, and found none of the nucleobase analog molecules that were detected in the meteorite.

A final and compelling bit of evidence is that the GSFC team was able to produce both the biological and non-biological nucleobases in a non-biological reaction using hydrogen cyanide, ammonia and water. “This provides a plausible mechanism for their synthesis in the asteroid parent bodies, and supports the notion that they are extraterrestrial,” adds Callahan, who points to the type of meteorites known as CM2 as the ‘goldilocks’ class of meteorite, optimized to make more of these molecules. Thus the notion that the building blocks of life arrived on our planet through impacts is given a boost, one that strongly points to their non-terrestrial origin.

After all, hydrogen cyanide is common in the interstellar medium, and thus likely to produce chemical reactions on space debris. Amino acids have turned up in samples of comet Wild 2 and in various carbon-rich meteorites. The new work tells us that nucelobases, the building blocks of genetic material like DNA and RNA, can have an extraterrestrial origin in meteorites rather than being the result of contamination. The idea that the early Earth could have been seeded with these important molecules seems less speculative all the time. Says Jim Cleaves (Carnegie Institution for Science), who worked on the meteorite samples: “This shows us that meteorites may have been molecular tool kits, which provided the essential building blocks for life on Earth.”

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