Centauri Dreams

Imagining and Planning Interstellar Exploration

Views of Proxima Centauri

alpha_centauri_A_B_Poxima

I haven’t yet read Stephen Baxter’s new novel Proxima, but because of my admiration for his previous books, it’s at the top of my reading list. Judging from the Amazon description, Proxima gets into issues that for me make red dwarfs utterly compelling. What would a habitable planet look like around such a star, tidally locked so that its sun never moved in the sky? What would it be like to move around this world, going from a warm substellar point toward twilight and then a frigid night on the dark side?

Given that this M-class red dwarf is 18,000 times fainter than the Sun, you wouldn’t expect it to make much of an impression in photographs. The one above (credit: European Southern Observatory) is instructive because it puts the entire Alpha Centauri system in context. At top left we have Centauri A and B, which are bright enough to merge together and appear as a single bright object. At the lower right is the arrow indicating Proxima Centauri, so faint as to be barely visible. Proxima is 4.218 light years from Earth and roughly 15,000 AU from Centauri A and B.

The image below gives us a brighter look. Taken by the Hubble Space Telescope, it isolates Proxima from the other two stars, but even here the red dwarf is a point-like object whose image is distorted by diffraction spikes produced within the telescope itself.

proxima

Image: The closest known star, Proxima Centauri is here imaged by the Hubble instrument. Credit: ESA/Hubble & NASA.

Proxima should remain a main sequence star for another four trillion years, about 300 times the current age of the universe. The planet search here is inconclusive, but here’s what we’ve got so far: Work by Michael Endl (UT-Austin) and Martin Kürster (Max-Planck-Institut für Astronomie), using seven years of high precision radial velocity data from the UVES spectrograph at the European Southern Observatory, can identify no planet of Neptune mass or above out to about 1 AU from the star. No super-Earths larger than 8.5 Earth masses have been detected in orbits of less than 100 days.

As for the habitable zone where liquid water could exist on the surface of a planet, it is thought to be between 0.022 and 0.054 AU, which would produce orbits between 3.6 and 13.8 days. The Proxima investigations have yet to find anything here, but the most we can say is that super-Earths of 2-3 times the mass of the Earth in circular orbits have been ruled out. That still leaves a lot of possibilities to be investigated as we refine our techniques and apply them to this intriguing star. Radial velocity capability down to one Earth mass is getting closer here.

Alpha_Centauri_relative_sizes

Image: Comparative sizes of the Alpha Centauri stars, with the Sun thrown in for comparison. Credit: Wikimedia Commons.

Because Proxima is a flare star that can experience sudden changes in brightness, any life evolving on a planet around it would have to have found a way to protect itself from such radiation. Even so, the star’s nearness to the Sun has made it a staple in science fiction, from Murrray Leinster’s 1935 story “Proxima Centauri”, published in Astounding Stories through Heinlein’s Orphans of the Sky (1963), where it was the logical destination for a starship, to the new Stephen Baxter novel. I’ll have more to say about the latter in upcoming posts. A search through the archives here will pull numerous articles on Proxima, including The Proxima Centauri Planet Hunt and Proxima Centauri: Looking at the Nearest Star.

tzf_img_post

Les Johnson: Big Projects and Deep Time

Not long ago I pulled a wonderful 1950 film out of my collection for a long-overdue viewing. I remember 711 Ocean Drive from late night television airings, and when it popped up a few years back on a local cable channel, I made a recording. Edmund O’Brien and Joanne Dru are the key players in this gritty tale about an electronics expert who gets drawn into big-time crime, and the ending, which takes place at the Hoover Dam straddling the Nevada/Arizona border, is simply terrific, with O’Brien taking the fall after his shady dealings have been exposed.

711 ocean drive - 1950

Image: On the run at the Hoover Dam in Joseph Newman’s 711 Ocean Drive.

Titanic forces, vast engineering, gunplay in the desert, all artfully directed by Joseph M. Newman — what more could you want? And now, thanks to Les Johnson, I connect Hoover Dam not only with a film noir classic but with long-term thinking and starflight. Johnson, speaking in his role as a science writer with deep connections to science fiction, told the recent Eve Online conference in Las Vegas that we as a species need to think big and think long if we are to realize our interstellar dreams. Hoover Dam was the example he used to remind us what it will take to reach the stars.

Deep Time and Future Engineering

I’m always looking for examples of long-term thinking in our history, because as a species, we actually do this pretty well. The Egyptian pyramids are an obvious example, and so are many European cathedrals, some of which were generational in their construction. Some cathedrals went up relatively quickly, to be sure — the main structure at Chartres took a mere 25 years. Others, like Lincoln or Notre-Dame in Paris, were a century or more in the making. The foundation stone at Cologne was laid in 1248 and by the time of the Reformation, the structure remained unfinished, to be completed only in 1880, having become a national project.

Johnson’s invocation of the Hoover Dam is a reminder that not all the great projects were undertaken by civilizations long gone. As a culture, we often seem to think in short time-frames, but we do have the engineering skills to do much better. This Discovery News story quotes Johnson as saying “this dam was built in the 1930s, but the design life of the dam itself (not the power systems) is 2,000 years … that’s foresight! That’s engineering planning. That’s something we shouldn’t be afraid of today when planning for our (species’) future.”

Johnson is well known in these pages not only because of his work at NASA’s Marshall Space Flight Center, but also for his non-NASA activities, which include writing and editing as well as frequent public appearances. Going Interstellar (Baen, 2012), which he edited with science fiction author Jack McDevitt, is a collection of fiction and non-fiction that belongs on your shelf if you share my passion for interstellar flight. And Solar Sails: A Novel Approach to Interplanetary Travel (Copernicus, 2007), which he wrote with Greg Matloff and Giovanni Vulpetti, is a wise introduction to the possibilities and the problems of building sails in space.

Methods like nuclear pulse (think Orion) and antimatter have their advantages, but all require us to carry fuel onboard, and in the case of antimatter, creating enough of that fuel — not to mention storing it — is a major problem. But Johnson can point to sail successes that tell us we’re moving into the era of space applications. The IKAROS sail put Japan into space first with a functioning sail, and NASA’s NanoSail-D deployed a smaller sail in 2011, a year after IKAROS. We now look forward to NASA’s 1200 square meter Sunjammer mission in 2015, even as the Planetary Society continues to develop its Lightsail 1. They’re a long way from interstellar applications, but these missions show us that sails are swiftly climbing the ladder of technological readiness.

Thinking long and thinking big work together. Building the kind of sail that could be laser-boosted into interstellar speeds would mean creating a sail as big as Nevada itself, and Johnson pointed out that the energy output needed for it would equal the energy output of the entire human race today. The point is that the much smaller sail experiments we run today can build toward a future where such structures become possible because of the technologies we’ll create in coming centuries. And if we continue our work with that long-term perspective in mind, we can speak of starflight in ways that do not violate known physics even if they demand huge engineering.

An Icelandic Perspective

The world of gaming seems a good place to stretch our concepts, and in the case of Eve Online, the setting is itself enormous. We’re talking about an MMORPG, which stands for Massively Multiplayer Online Role-Playing Game, and this one has a community of half a million, with a canvas that stretches across the galaxy and is stuffed with star systems ready to be explored.

Eve Online comes out of one of my favorite places, Iceland, and reminds me of travel experiences there over the past thirty years. Back in the 1970s, working on medieval linguistics in grad school, I went to Iceland under the urging of a wonderful professor named George Lane, who was himself fluent in Icelandic and had inspired my own interest in the language. Strolling through the numerous bookshops of Reykjavik, I found that modern editions of the great medieval works, from the sagas to the poetic Eddas, were readily available. The language itself retained much of the medieval structure in ways that most modern tongues do not.

thingvellir-61

And maybe it was walking around at the site called Thingvellir (Þingvellir) on a foggy late afternoon in August that started teaching me about perspective. It was here that Iceland’s general assembly, the Alþing, first met in about 930 AD, on land that is situated at the boundaries of tectonic plates, a fissure zone that runs through Iceland itself. I walked about a mile from the small hotel and looked back across the valley as a bit of Sun emerged and a rainbow arced across the landscape. It was as if a Viking past reached all the way into the present day, and that day was itself the outgrowth of physical processes that came up out of the Earth’s deep core.

We carry the past with us wherever we walk but the sense of ‘deep time’ that overcame me that day is sometimes lost in the rush to complete day-to-day tasks. I think Les is right that we need to recover it as we look toward a human destiny among the stars. “Thingvellir is a place of echoes,” said a friend when I got back to Reykjavik. She was an English writer who had travelled often there and she knew what she was talking about. We must look back, far back, and then forward into a deep future, building our bridges as if our ancestors were crossing them.

tzf_img_post

Kepler-78b: Rocky World in Unusual Orbit

When I was first learning about astronomy by reading every book I could find on the subject — I spent a lot of time at the library in my youth — I was fascinated to hear stories of a planet closer to the Sun than Mercury. The French scientist Urbain Le Verrier pondered the existence of such a world in the 19th Century, wondering if it wouldn’t explain peculiarities in Mercury’s orbit. When an amateur astronomer named Edmond Modeste Lescarbault claimed he had observed a transit of such a planet in 1859, Le Verrier’s investigation satisfied him that the detection was legitimate. He went on to announce the discovery of the planet he dubbed Vulcan in Paris in 1860.

Despite a string of other observing claims later in the century, the existence of Vulcan is now discounted, although the possibility of asteroids in tight solar orbits hasn’t been ruled out. As for Mercury, it fell to Einstein to demonstrate that apparent anomalies in its orbit could be explained by his theory of General Relativity. Vulcan was an intriguing story in those days of my early astronomy reading, as I asked myself how anything could survive closer to the Sun than Mercury, and conjured up hellish landscapes dominated by a sky-swallowing star above.

But if we don’t have Vulcan in our own Solar System, it’s clear that many other systems do have planets in extraordinarily close orbits. Yesterday I listened in on the news conference describing Kepler-78b, one of the new class of ‘ultrashort period’ planets that Kepler has put into our databases. To qualify as an ultrashort period planet, the world has to orbit with a period of less than twelve hours. Defying the imagination, Kepler-78b bests even that figure, orbiting a star somewhat smaller and less massive than the Sun in a mere 8.5 hours.

78b

Image: Kepler-78b is a planet that shouldn’t exist. This scorching lava world, shown here in an artist’s conception, circles its star every eight and a half hours at a distance of less than 1.6 million kilometers. According to current theories of planet formation, it couldn’t have formed so close to its star, nor could it have moved there. Credit: David A. Aguilar (CfA).

Dimitar Sasselov (Harvard-Smithsonian Center for Astrophysics) told the audience that we had now found about a dozen objects orbiting various stars with periods of between three and ten hours, creating serious questions about how such planets form and survive. It’s even conceivable, said Sasselov, that Kepler-78b is the core of a former gas giant. Amidst the questions, what we do know is that its radius is about 1.2 times that of Earth and its mass 1.7 times Earth’s. With both size and mass measured, it’s possible to calculate the density, and that figure works out to 5 grams per cubic centimeter, which is a density much like our planet’s.

Kepler-78b, then, is most likely made of rock and iron. The work to demonstrate this points to the synergy between two kinds of observation and also relies on a dual investigation that produced confirming results. The planet was first observed by Kepler using the transit method, in which a planet moves in front of its star as seen from Earth and thus creates a dip in its lightcurve. Andrew Howard and team at the University of Hawaii at Manoa then used the Keck ten-meter instrument with the HIRES spectrograph to measure the star’s radial velocity, thus allowing the determination of the planet’s mass. The density reading follows from the size and mass.

Howard told the news conference that thirty hours of observations over eight nights went into the Keck work, which was a difficult measurement because the star is young and has many starspots. With an orbital period this short, the team was able to observe an entire orbit in a single night, however, and the starspot ‘noise’ could be filtered out. At the same time, Francesco Pepe (University of Geneva), using data from the HARPS-North spectrograph in the Canary Islands, was leading a companion study that verified the Keck team’s radial velocity observations. “The gold standard in science is having your findings reproduced by other researchers,” said Howard. “In this case, we did not have to wait for this to happen.”

78b_2

Image: This illustration compares our Earth with the newly confirmed lava planet Kepler-78b. Kepler-78b is about 20 percent larger than Earth, with a diameter of 9,200 miles, and weighs roughly 1.8 times as much as Earth. Credit: David A. Aguilar (CfA).

So we have an Earth-sized planet with Earth-like density in an orbit that remains a mystery. The star Kepler-78b orbits was larger than it is now when the planetary system was forming. “[The planet] couldn’t have formed in place because you can’t form a planet inside a star,” said Sasselov. “It couldn’t have formed further out and migrated inward, because it would have migrated all the way into the star. This planet is an enigma.” It is also a world that will eventually be torn apart by gravitational forces as it is drawn inexorably closer to the star, although according to this CfA news release, that won’t happen for another three billion years.

With temperatures as high as 3100 K on the surface, Kepler-78b is some 40 times closer to its star than Mercury is to the Sun, making my musings about Vulcan’s sky seem relatively tame. The papers are Howard et al., “A rocky composition for an Earth-sized exoplanet,” published online in Nature 30 October 2013 (abstract), and Pepe et al., “An Earth-sized planet with an Earth-like density,” published online in Nature 30 October 2013 (abstract).

tzf_img_post

HD 21997: Challenge to Planet Formation Theories

HD 21997 is a star in the southern constellation Fornax (the Furnace) that is yielding some surprising data about how planetary systems form. About 235 light years from Earth, the star is 1.8 times the mass of the Sun and is thought to be about thirty million years old. Observations by an international team using ESA’s Herschel Space Observatory and the Atacama Large Millimeter/sub-millimeter Array (ALMA) in Chile show a ring of material around the star that contains not only a good deal of gas but also the dust produced by the collision of planetesimals.

PR_2013_11_1gr

Image: ALMA images of the disk around HD 21997. The left image shows the emission of cold dust grains, situated in a ring around the central star. The middle image displays the emission from carbon monoxide, and shows that gas can also be found closer to the star than dust. The right image depicts the velocity of the gas. The red-colored parts of the disk move away from us, while the blue-colored parts move towards us, indicating that the gas is rotating/orbiting around the central star. Credit: Á. Kóspál (ESA) and A. Moór (Konkoly Observatory).

This is an unusual finding because our models of planet formation predict that the primordial gas should be completely out of a young system after no more than ten million years, pulled into the star itself, or aiding in the formation of gas giant planets, with the balance simply dissipating because of intense radiation from the young star. But the disk around HD 21997 is obviously a hybrid, one that links the early and late phases of disk evolution. Moreover, the dust ring and the gas ring do not coincide. Ágnes Kóspál (ESA) sees this as a clue to how the two disks formed:

“The gas ring starts closer to the central star than the dust. If the dust and the gas had been produced by the same physical mechanism, namely by the erosion of planetesimals, we would have expected them to be at the same location. This is clearly not the case in the inner disk.”

The amount of gas is striking. The team’s data show that the total gas mass is somewhere between thirty and sixty times the mass of the Earth, an indication that the gas disk really is primordial material, as the amount of gas freed by collisions between planetesimals would be insufficient to explain this quantity. What’s ahead is a search for more systems like HD 21997 for further information about how our models of planet formation may need to be revised.

This is not the first time we’ve found indications of hybrid disks. In fact, disks around ? Pictoris, HD 32297, 49 Ceti, HD 172555, and HD 32297 are also known to contain small amounts of gas, a finding that has energized debate about whether the gas was produced by planetesimal collisions or was leftover material from the primordial disk. HD 21997 takes the debate to another level, because the amount of gas and the displacement of the two disks are strong indicators that the gas here is primordial, with all that implies about the need to adjust our models.

atacama

Image: Antennas of the Atacama Large Millimeter/submillimeter Array (ALMA), a compound telescope on the Chajnantor Plateau in the Chilean Andes. The final ALMA configuration has 66 antennas acting like a single telescope. Signals from this array made it possible to spatially resolve the emission of both the dust grains and the gas molecules. Credit: ESO/C. Malin.

The two papers on this work are Kóspál et al., “ALMA observations of the molecular gas in the debris disk of the 30 Myr old star HD 21997,” Astrophysical Journal Volume 776, Issue 2 (2013 – abstract) and Moór et al., “ALMA continuum observations of a 30 Myr old gaseous debris disk around HD 21997,” Astrophysical Journal Letters Volume 777, Issue 2 (2013 – abstract). See also this MPIA news release.

tzf_img_post

Desert Planets Around Carbon-Rich Stars?

Habitable zones are always controversial. Bring up the classic definition of a zone where liquid water can exist on the surface and you run into queries about places like Europa, far outside the HZ in those terms but perhaps capable of supporting life beneath the ice. For that matter, exotic forms of life cannot be ruled out in settings like Titan, though they would be nothing like what we’re familiar with on Earth. Nonetheless, refining our methods to look for life on planets with liquid water is a rational way to proceed and we’re developing the needed tools.

As we wait for those tools to be funded and built — projects like Terrestrial Planet Finder are on indefinite hold — we can continue to develop our theoretical models for living planets. On that score, Torrence Johnson (JPL) and colleagues have had interesting things to say lately. Johnson spoke at the American Astronomical Society Division of Planetary Sciences meeting in Denver earlier this month, addressing the question of planets rich in carbon. You would think that plentiful carbon, given its importance in living systems, would be a plus, but it turns out that having too much carbon is a serious problem even for planets in clement orbits like the Earth’s.

Here life has yet another ‘filter’ to get through. For the Earth is made up largely of silicates rather than carbon because the Sun is relatively carbon-poor. We assume that stars with much higher carbon content than the Sun will spawn planets so infused with carbon that they may have layers of diamond. What they apparently won’t have, according to Johnson’s models, is water. Much of the available oxygen in such a system would go into making carbon monoxide, with little oxygen left for making water ice. That means no icy asteroids delivering water to planetary surfaces.

Comets and asteroids are thought to have delivered the bulk of Earth’s water billions of years ago, moving into the inner system from beyond the ‘snow line’ where ice was plentiful. Carbon-rich planetary systems will simply lack this resource. Says Johnson: “There’s no snow beyond the snow line… The building blocks that went into making our oceans are the icy asteroids and comets. If we keep track of these building blocks, we find that planets around carbon-rich stars come up dry.”

PIA17550_ip

Image: This artist’s concept illustrates the fate of two different planets: the one on the left is similar to Earth, made up largely of silicate-based rocks with oceans coating its surface. The one on the right is rich in carbon — and dry. Chances are low that life as we know it, which requires liquid water, would thrive under such barren conditions. Credit: NASA/JPL.

This NASA news release has more, and the paper on this work fully develops the importance of the carbon-to-oxygen ratio, a result not only of elements from the Big Bang but also the hydrogen, helium, nitrogen, silicon, carbon and oxygen inherited from earlier generations of stars. The paper notes:

Planetary systems around stars with compositions that di?er from the Sun’s will have planetesimals – formed beyond the snow line – which have a wide range of silicate and metal, carbon and ice proportions. The fraction of silicate plus metal in extrasolar planetesimals should depend strongly on the C/O ratio in a given circumstellar nebula, which controls the abundance of water ice, clathrate hydrates, and stochiometric hydrates in the condensed solids. Other volatile ices are less strongly a?ected by the host star compositions in our study, although C-bearing ices such as CO (ice and clathrate), CO2 and CH3OH will be more abundant with increasing C/O. The planetesimal population of our own outer solar system, as incompletely known as it is, represents only one trajectory through the planetesimal composition space de?ned by the possible range of C/O and metallicities seen in other stars.

One day, then, we may find an Earth-mass planet in a star’s habitable zone that, because of its star’s composition, is highly unlikely to have anything alive on it. We’re not yet able to make the kind of spectroscopic observations that would flag life’s presence in a planetary atmosphere, but the paper adds that we can follow up these studies in the near-term by using instruments like the James Webb Space Telescope to study the planet-forming zones of young solar systems and the effect of primordial elements through heavy element enrichment in extrasolar giant planets.

The paper is Johnson et al., “Planetesimal Compositions in Exoplanet Systems,” The Astrophysical Journal Volume 757, No. 2 (2012), p. 192 ff (abstract)

tzf_img_post

Starship Century Symposium, London

Oxford-based Stephen Ashworth, who attended the recent Starship Century event in London, obviously took copious notes, as reflected in the piece that follows. Ashworth is a Centauri Dreams regular, a writer and musician who, like so many of us on this site, ponders the big questions of our engagement with — and exploration of — the universe. Here he reflects on the immense challenge of starflight and lets us know how a number of key players now see it. For more of Stephen’s perceptive work, check in regularly at his Astronautical Evolution site.

by Stephen Ashworth

Stephen Ashworth

The new book Starship Century, edited by physicists James and Gregory Benford and with contributions from many active in the interstellar field, takes a broad view of questions of interstellar exploration, the editors told this meeting at the Royal Astronomical Society in London on 21 October 2013. In the first place, why has there been such a surge of interest over the past decade or so, with several new organisations devoted to interstellar travel appearing on the scene? Is the 21st the century humanity will build starships, and if so, why and how?

With Voyager 1 now having crossed the heliopause and New Horizons due to make its flyby of Pluto in less than two years time, finishing the initial reconnaissance of the Solar System, together with a flood of exoplanet discoveries, including the first indications of a planet in the Alpha Centauri system, the time appears right for interstellar exploration to inspire growing interest, James Benford said in his introductory talk.

Yet the task is immense. Before our ancestors learned to ride horses, they were only able to move at a walking speed, on the order of a metre per second. The Apollo astronauts departed from and returned to Earth at speeds around 104 times faster. A cruising speed of a significant fraction of the speed of light, necessary to reach the stars in a reasonable period of time, would require another 104 times jump.

Moreover, in order to make that jump one is running up against the limits of known energy sources. An object flying at 3.75% of light speed possesses the same kinetic energy per kilogram of mass as that released in a thermonuclear explosion.

Benfords

Image: James (left) and Gregory Benford at the Starship Century symposium, along with a bust of Sir Isaac Newton.

In an article in Physics Today back in 1968, Freeman Dyson predicted that the first interstellar voyages would be possible in 200 years time. However, he recently reiterated that they would still be possible in 200 years time – the familiar tale of an ever-receding goal. Harnessing the immense energies of nuclear fusion reactions, whether for commercial power generation or for rocket propulsion, is not turning out to be easy.

What about the attitude of the public? Benford displayed a cartoon: an ascending sequence of technological achievements in chronological order – a horse-drawn wagon, a car, a locomotive, an aircraft, a space rocket – as rough drawings on a wall. Then you notice that the artist is a caveman. Then zoom out, and you see a cavewoman watching him skeptically, and asking him when he’s going to get the meat in for their dinner. The triumphalist belief in inevitable progress is a nerdish pursuit, and the majority of the public can see no further than the desire to solve their day to day problems.

(However, in The Demon-Haunted World Carl Sagan wrote of the critical importance of those denigrated as “nerds” in making progress possible – his example was James Clerk Maxwell. – Comments in parentheses such as this are my personal reflections after the event.)

For the present, interstellar progress is in the hands of six private groups, all with very small budgets: the British Interplanetary Society (the oldest, founded in 1933), the Tau Zero Foundation, Icarus Interstellar, the 100 Year Starship Organization, the Institute for Interstellar Studies, and most recently the New Horizons Message Initiative. (Given its website and organisation of meetings such as this one, surely Starship Century itself counts as the seventh group?)

Cascading opportunities among a galaxy of planets

James Benford’s brother Gregory presented a quotation about the prospect for development of North America from Thomas Jefferson back in 1812: “It will take a thousand years for the frontier to reach the Pacific.” Jefferson was assuming that colonists would be limited to the capabilities of horse-drawn wagons, yet the steam engine was already a reality, and communications across the continent were vastly accelerated when the trans-continental railroad was completed in 1869.

Martin Rees & Greg Benford

Image: Lord Martin Rees and Gregory Benford.

So Jefferson’s estimate was out by more than an order of magnitude. It didn’t occur to him that opportunities in technology and the economy would cascade to drive settlement of the interior. In a similar way, during the coming century we could be seeing a combination of nuclear rockets, robotics and 3D printing working together to accelerate the economic opening up of the Solar System, which will be essential to exploring beyond it.

Ian Crawford, professor of astronomy at Birkbeck College, London, displayed a plot of exoplanet discoveries made by the Kepler mission (see below), the conclusion of which had to be that virtually all main-sequence stars do in fact have planets of one sort or another. But because it is easier to find them by the transit method, only four are currently known (with varying levels of reliability) within 15 light-years of the Sun, orbiting Alpha Centauri B, Tau Ceti, Epsilon Eridani, and the red dwarf GJ 674.

planets-580x429

Image: A new analysis examined the frequencies of planets of different sizes based on findings from NASA’s Kepler spacecraft, correcting for both incompleteness and false positives. The results show that one in six stars has an Earth-sized planet in a tight orbit. Credit: F. Fressin (CfA)

More nearby planets will surely be discovered as techniques improve, with the James Webb Space Telescope, the Transiting Exoplanet Survey Satellite (TESS, the planned successor to Kepler) and Europe’s Exoplanet Characterisation Observatory (EChO) in prospect, as well as continuing improvements in adaptive optics applied to large ground-based telescopes.

The ideal tool would be something like Europe’s Darwin space interferometer, which would be capable of obtaining the spectra of Earthlike exoplanets. But Darwin is not currently under development. And, as Charles Cockell has pointed out, even if the spectra of gases associated on Earth with life (H2O, CO2, O3) are obtained, they would not definitively prove that life had to be present, nor would they tell us anything about the nature of that life if it existed. The spectrum of Earth must have appeared much the same over the past two billion years, through dramatically different epochs of its biological history.

The only way to be sure would be to send an interstellar probe that could make in-situ measurements. Crawford presented his shopping list for the instruments he would like to carry on that probe, with a whole array of orbiters, landers and atmospheric entry probes, arriving at a mass decelerated into the target system in the range of 150 to 200 tonnes.

Ian Crawford

Image: Ian Crawford discussing instrumentation for an interstellar probe.

But his reasons for interstellar exploration extend beyond science. He presented arguments from the seventeenth-century philosopher John Locke, who reasoned that the human imagination cannot produce anything genuinely new. In order to refresh both science and our broader culture, therefore, it is necessary to go out and physically discover genuinely new things. Interstellar exploration more than any other pursuit puts us on track to discover things that have never been thought of before.

Stephen Baxter, the well-known science fiction author and, like Crawford, an Icarus team member, discussed what might happen if one of our interstellar probes were to encounter intelligence at its destination. On the assumption that we had not known of the existence of intelligent life there when the probe was despatched, contact would take place when the vehicle was remote from any direct human control. How would it detect and recognise alien intelligence, and how might it be programmed to respond?

Stephen Baxter

Image: Stephen Baxter on probes and the potential for contact.

Of course, the extraterrestrials might see our vehicle arriving, and Baxter discussed ways in which this might come about. (Implausible, I thought: if they were that technically advanced, they would surely have visited us long before. The time window in which they are developed enough to detect, say, the exhaust from the fusion engine of a decelerating vehicle, and to recognise it for what it is, but not developed enough to be launching their own interstellar vehicles, would be only a few centuries at most in the history of a species whose origin is not coordinated with that of H. sapiens and might well be millions to billions of years earlier or later.)

These issues are presented in more detail in Baxter’s article in the Jan./Feb. 2013 issue of JBIS. He also noted that his own latest novel, Proxima, is, appropriately enough, an interstellar yarn.

The word from the A.R.

(I don’t know if people still call the Astronomer Royal “A.R.”, but I did re-read Fred Hoyle’s classic The Black Cloud not so long ago, and they certainly did then.)

Lord Martin Rees, the Astronomer Royal, has written extensively on the cosmos and the outlook for human civilisation. He brought an astronomer’s perspective on time to the Symposium, particularly future time: assuming we do not become extinct, post-human evolution will be much longer than that which led up to us, and will moreover be accelerated and directed in new ways by genetic and computer technologies. So far as our evolution is concerned, we have not yet reached even the halfway point.

What role, he asked, will humans play in space? In contrast with Ian Crawford’s well-known view, he did not see any case for astronauts as scientific explorers in an age of increasingly capable robots. But the human adventure of space travel in person was undeniable. He gave two pointers to the human future in space: China might leapfrog the US and send astronauts to Mars, and meanwhile the private sector was also on the verge of sending passengers into space. NASA had become risk-averse, creating an opportunity for privately funded adventurers who were willing to accept greater levels of risk – not as “space tourists”, for that phrase gives a misleading impression of safety and regularity, but as participants in a dangerous sport akin to deep ocean diving or making the ascent of Everest.

Rees at Podium

Image: The Astronomer Royal analyzes current space efforts.

(I would disagree with the A.R. on two points here. Having already experienced the disappointment of seeing Soviet cosmonauts fail to reach the Moon, I do not share the enthusiasm for Chinese manned spaceflight. They are currently about where the two traditional superpowers were before the Salyut 6 breakthrough in the late 1970s. I have heard no reason why a Chinese Apollo, Shuttle or continuously occupied Station programme, were such to appear, would be any more sustainable than their American and Russian originals, and they are nowhere near even beginning the major structural reorganisation currently underway across the Atlantic, essential for meaningful progress at this point. Meanwhile, although we do not yet have space tourism as such, the creation of a mass market for space travel at a level of at least 5,000 passengers/year worldwide (say, one planeload of 20 every weekday of the year) at near-airline standards of service seems to me to be vital for consolidating our hold on low Earth orbit, bringing the costs down and reliability up to levels that allow for sustained exploration beyond near-Earth space.)

Lord Rees stated, reasonably enough, that there would never be mass emigration from Earth, and so Earth’s problems would have to be solved on their own terms. But by the end of the current century there could well be small groups of pioneers living away from the mother planet. Interstellar travel, however, is for post-humans, whether genetically modified but still biological humans, or entirely manufactured beings.

He pointed out that explorers of our own planet were in some ways going into the unknown to a far greater extent than astronauts ever will. They were crossing oceans and continents about which nothing was known but much was imagined, completely out of touch with their port of origin, unlike any astronaut, whose journey takes them to lands already surveyed by telescope and probed by robot precursors, and in direct line of sight radio communication (if delayed by light travel time) with Earth. But what terrestrial explorers did have was a high expectation of profitable discoveries leading them ever onward.

As an astronomer, Lord Rees was naturally no stranger to the longest possible future perspectives, when the apparently accelerating cosmological expansion has carried almost all the universe beyond our horizon, leaving only the matter in the Local Group of galaxies accessible to our remote descendants. Maybe they would find that they were living in only one universe in a multiverse, or in someone else’s simulated universe.

General discussion

The presentations were followed by general discussion. There was some debate about the key factors in our intelligence, and in that of any intelligent alien species which we might meet elsewhere in the Galaxy. Biologist and science fiction author Paul McAuley pointed out that species other than ourselves use and make tools, and suggested that the key to our success had been our ability to archive knowledge for future generations to use.

Paul McAuley (2)

(My own view is that an archive, such as a library containing books, is itself a kind of tool, so that does not answer the question. My answer would be that we are unique in that we not only use and make tools, but that critically we use tools to make better tools. It is this recursive use of technology back onto itself in order to make better technology that is what drives progress.)

I should like to draw particular attention to what was said about the near-term future, before an interstellar mission is even launched. For it is what happens on Earth and in space over the next few years which will determine whether or not our civilisation even has an interstellar future.

Image: Science fiction writer Paul McAuley.

Ian Crawford made the point that the single most important factor was to reduce the cost of access from Earth’s surface to orbit, whether this was done with single-stage-to-orbit spaceplanes, or by construction of a space elevator. (Here let me link to the latest news on Britain’s Skylon spaceplane programme, managed by interstellar pioneer Alan Bond of Daedalus and worldships fame.)

James Benford argued for nuclear rockets, firstly fission engines of the type developed by NASA in the late 1960s, later fusion engines, which would open up the Solar System. SpaceX, he agreed, would surely succeed in lowering costs, but in his view there was also a case for beamed power for access to space. His brother cautioned that the laser-ignition fusion work in which he had been involved forty years previously had still not achieved a useful result, but that there were good prospects for fusion based on the proton-boron reaction. Stephen Baxter proposed that large-scale geoengineering projects, such as building a solar parasol to keep Earth cool, or the large-scale development of solar power satellites, might be an important driver of progress.

The debate over whether space agencies or the private sector are in the better position to lead produced a number of points. Governments are broke, James Benford said, hence the private sector must lead. Governments are risk-averse, Lord Rees added, leading to the same conclusion – new moves will be spearheaded by crazy billionaires, leading small groups of eccentric but highly motivated people. In his view, this would be no bad thing: we should encourage everyone to explore the limits of what humans can do.

But Gregory Benford (whose novel The Martian Race features the Chinese government competing, with European collaboration, in a race to Mars) allowed a possible leading role for government in the case of China.

Ashworth and McAuley 2

Image: The discussion continues. Stephen Ashworth (left) and Martyn Fogg.

Ian Crawford cautioned that space could not be allowed to become a free-for-all because of the dangers involved when, for example, asteroidal material impacts Earth. One could imagine a private group holding Earth to ransom in this way. It would therefore be necessary for us to evolve appropriate political institutions to ensure that space development is beneficial for all.

James Benford picked up this theme, stating that what governments can do is to make developments possible, or impossible. In the case of railways and canals they set up rights of way, for example by the purchase of land for the trans-continental railroad across the United States. Clearly, governments are also the guarantors of private property, and of the whole system of law and order on which economic prosperity depends. A creative synergy between government and private enterprise is therefore surely the way forward.

Next step: read the book!

In summary, then, this was a stimulating meeting with several of the key thinkers in the interstellar field. It was an excellent opportunity for people in Britain like myself who cannot hop across the Atlantic to attend interstellar conferences in the US, and it deserved to have been more fully attended (as it was, there were seats to spare in the smallish auditorium where the meeting took place).

The breadth and confidence of the vision of humanity’s and post-humanity’s interstellar future, presented in this and many other conferences, contrasts oddly with the current confusion and controversy about the direction of the public space programme in the United States, and with the apathy and stagnation in Europe. Clearly a major reorganisation of the space industry is under way, leading towards a more economically based industry in which government is one customer among many, as is already the case for Earth satellites but not yet the case for manned spaceflight, or for robotic ventures beyond geostationary orbit.

More details and discussion, from the speakers at this meeting and many others, may be found in the Starship Century book.

My thanks to the Benfords and to our hosts at the Royal Astronomical Society for organising this event.

tzf_img_post

Charter

In Centauri Dreams, Paul Gilster looks at peer-reviewed research on deep space exploration, with an eye toward interstellar possibilities. For many years this site coordinated its efforts with the Tau Zero Foundation. It now serves as an independent forum for deep space news and ideas. In the logo above, the leftmost star is Alpha Centauri, a triple system closer than any other star, and a primary target for early interstellar probes. To its right is Beta Centauri (not a part of the Alpha Centauri system), with Beta, Gamma, Delta and Epsilon Crucis, stars in the Southern Cross, visible at the far right (image courtesy of Marco Lorenzi).

Now Reading

Version 1.0.0

Recent Posts

On Comments

If you'd like to submit a comment for possible publication on Centauri Dreams, I will be glad to consider it. The primary criterion is that comments contribute meaningfully to the debate. Among other criteria for selection: Comments must be on topic, directly related to the post in question, must use appropriate language, and must not be abusive to others. Civility counts. In addition, a valid email address is required for a comment to be considered. Centauri Dreams is emphatically not a soapbox for political or religious views submitted by individuals or organizations. A long form of the policy can be viewed on the Administrative page. The short form is this: If your comment is not on topic and respectful to others, I'm probably not going to run it.

Follow with RSS or E-Mail

RSS
Follow by Email

Follow by E-Mail

Get new posts by email:

Advanced Propulsion Research

Beginning and End

Archives