This morning I want to circle around to a story I had planned to write about a couple of weeks ago. One thing writing Centauri Dreams has taught me is that there is never a shortage of material, and I occasionally find myself trying to catch up with stories long planned. In this case, the imaging of an exoplanet around the star Beta Pictoris demands our attention because of the methods used, which involve charge-coupled devices and wavelengths close to visible light. The detection marks real progress in visible light imaging of exoplanets. The work, which is slated to appear in The Astrophysical Journal, was conducted by researchers from the University of Arizona led by Laird Close. Charge-coupled devices (CCD) are the same kind of technology we find in digital camera imaging sensors, used here in a setting where we’d normally expect an infrared detector. But using infrared means viewing massive young planets hot enough to put out considerable heat. As the exoplanet hunt develops and...
A Glassy Sea on Titan
The second largest sea on Titan is Ligeia Mare, made up of methane and ethane in a body of liquid that is larger than Lake Superior. Now we have word that the surface of Ligeia Mare is so utterly still that it would appear like glass. The news comes from Stanford University, where geophysicist Howard Zebker had led a new study based on Cassini measurements made in 2013. "If you could look out on this sea," said Zebker, "it would be really still. It would just be a totally glassy surface." Titan seizes the imagination not only because it is planet-like, with seas and a thick atmosphere, but because we know of no other body in the Solar System besides Earth that has a complex cycle involving solid, liquid and gas. Because the thickness of Titan's atmosphere compromises optical observations, Cassini bounced radio waves off the surface and analyzed the resulting echo. Wave action could be measured by the strength of the returning echo. Zebker explains in this Stanford news release that...
What Kardashev Really Said
Whenever we're audacious enough to categorize far future civilizations, we turn to the work of Nikolai Kardashev. Nick Nielsen today looks at the well known Kardashev scale in the light of a curious fact: While many use Kardashev's rankings in their own speculations, few have gone back and dug into his original paper. In Kardashev's terms, our planet is close to attaining Type I status, which would surprise many commentators. And doesn't the ambiguity over what constitutes the energy of a star -- red dwarf? red giant? -- play havoc with cut and dried 'type' definitions? How subsequent writers have adapted and modified the Kardashev scale makes for a cautionary tale about mastering our sources before using them for further extrapolation. For that matter, are there better gauges of a civilization than its use of particular energy resources? Answering the question deepens the debate that Kardashev so fruitfully began. by J. N. Nielsen The name of Nikolai S. Kardashev is synonymous with...
Solar Probe Plus: Prelude to ‘Sundiver’?
'Sundiver' maneuvers are surely the most extreme events to which we could subject a solar sail. To my knowledge, it was Gregory Benford who first came up with the term -- he mentions in Fantasy & Science Fiction that he passed the coinage on to David Brin when Brin was working on the book that would bear its name (Sundiver, published in 1985, would be the first volume in Brin's Uplift Saga). But Benford credits Brin with the actual concept, which he needed to make his plot work, so it seems best to give credit to both writers for an idea both went on to explore, Benford not only in fiction but in scientific papers as well. The maneuver is straightforward if breathtaking. Benford explains it in terms of a carbon sail being deployed in low Earth orbit and then launched into deep space by microwave beam: Consider the sundiving sail. Approaching the Sun turned edge-on (to prevent the increasing flux of sunlight from pushing against its fall), the carbon sail heats up. At closest...
From Cosmism to the Znamya Experiments
What got me thinking about French influences on early solar sail work in Russia yesterday was the realization that science fiction was much stronger in Europe, and particularly France, in the latter part of the 19th Century than we Americans might realize. Hugo Gernsback to the contrary, the genre did not emerge in 1926 with the appearance of Amazing Stories, nor did key early texts like Mary Shelley's Frankenstein launch the genre in England. Brian Aldiss would probably argue with this (see his Trillion Year Spree, 1973), but I agree with Brian Stableford in seeing a true genre emerging first on French soil. Whether you agree or not, have a look at Stableford's essay The French Origin of the Science Fiction Genre, where I find this in reference not only to Verne but writers like George Sand (Laura: voyages et impressions, 1865) and Camille Flammarion (Récits de l'infini, 1872): These works were sometimes referred to by contemporary commentators as examples of roman...
SF Influences: A Solar Sail Theory
Last week I looked at three figures who put solar sails on the map in the 1950s -- Carl Wiley, who wrote the concept up in Astounding, Ted Cotter, who analyzed it for colleagues at Los Alamos, and Richard Garwin, who brought solar sailing into the academic journals. It was not long after Garwin's work that science fiction pounced on solar sails through a cluster of memorable stories beginning with Cordwainer Smith (Paul Linebarger) and "The Lady Who Sailed the Soul." More about that story and its era soon, including work by Poul Anderson, Jack Vance, and perhaps the best known of all from that era, Arthur C. Clarke's "Sunjammer." But today let's go way back to what is I think the first story that ever dealt with raw light as a propulsive mechanism. Georges Le Faure and Henri de Graffigny published Aventures extraordinaires d'un savant russe (The Extraordinary Adventures of a Russian Scientist) in three volumes beginning in 1889, with a fourth volume coming out under the promising...
Creative Constraints and Starflight
I discovered Karl Schroeder's work when I was researching brown dwarfs some years ago. Who knew that somebody was writing novels about civilizations around these dim objects? Permanence (Tor, 2003) was a real eye-opener, as were the deep-space cultures it described. Schroeder hooked me again with his latest book -- he's dealing with a preoccupation of mine, a human presence in the deep space regions between ourselves and the nearest stars, where resources are abundant and dark worlds move far from any sun. How to maintain such a society and allow it to grow into something like an empire? Karl explains the mechanism below. Science fiction fans, of which there are many on Centauri Dreams, will know Karl as the author of many other novels, including Ventus (2000), Lady of Mazes (2005) and Sun of Suns (2006). by Karl Schroeder My newest science fiction novel, Lockstep, has just finished its serialization in Analog magazine, and Tor Books will have it on the bookshelves March 24....
Solar Sailing Moves into the Journals
I'm just getting started with Chris Impey and Holly Henry's Dreams of Other Worlds (Princeton University Press, 2013), but glancing through it yesterday reminded me how long it has taken sail hardware to get into space. While Ted Cotter and Carl Wiley hoped for early experiments with sail ideas, we never got them until much later. Interesting mission concepts like JPL's 'gyro' sail to Halley's Comet did develop (although it never flew), and the Soviet Znamya deployments gave us some experience with thin membranes in space (I'll talk about those soon), but by and large we left interplanetary exploration for the rockets. The deep space probes and near-Earth observatories Impey and Henry cover -- Viking, Voyager, Stardust, Chandra, Hubble and their ilk -- gave us outstanding results but were not, until IKAROS, joined in space by alternative sail technologies. I'll review this book in some detail as soon as I finish it, but for today let's go back to the late 1950s, a time when Carl...
A Sail Mission Emerges
Carl Wiley, the prescient engineer who offered an early description of solar sails in "Clipper Ships of Space" (Astounding Science Fiction (May, 1951), was not the first to look into sail propulsion, but he was one of the more visible. Konstantin Tsiolkovsky's thinking on the matter in the 1920s was not widely circulated, and it may be that John Desmond Bernal, a political activist and professor at Cambridge and, later, the University of London, was Wiley's primary forerunner as far as public awareness of sail ideas is concerned. In The World, the Flesh & the Devil (1929), Bernal looked at the propulsive possibilities in light: However it is effected, the first leaving of the earth will have provided its with the means of traveling through space with considerable acceleration and, therefore, the possibility of obtaining great velocities - even if the acceleration can only be maintained for a short time. If the problem of the utilization of solar energy has by that time been solved,...
Solar Sails: Remembering Carl Wiley
If you're interested in solar sails and find yourself in California, a stop by UC Riverside's Tomás Rivera Library should be worth your time. There you will find the Carl A. Wiley collection on solar sails, containing books, manuscripts and various other materials related to sail technologies. Wiley was an aeronautical engineer who wrote the first detailed article on solar sails to reach a wide audience. Evidently concerned about the venue -- Wiley's article had been accepted by John Campbell's Astounding Science Fiction, which some of his colleagues might not have taken seriously -- he chose to write under the pseudonym 'Russell Saunders.' Finding Wiley's papers at Riverside is perhaps no surprise, given that this is the home of the Eaton Collection of Science Fiction & Fantasy, 'the largest publicly-accessible collection of science fiction, fantasy, horror and utopian literature in the world.' Pulp magazine enthusiasts like myself will note that the archive houses full runs of many...
WISE: New Stars and Brown Dwarfs
Just how early we are in our thinking about traveling beyond the Solar System is revealed in a comment made by Ned Wright, principal investigator of the WISE mission. "We don't know our own sun's backyard as well as you might think," said Wright. And he goes on to say, "We think there are even more stars out there left to find with WISE." That's a wake-up call indeed given how much WISE has already told us, and what two new studies have brought to light. Davy Kirkpatrick (Caltech) led one of these, examining data from the Wide-field Infrared Survey Explorer mission that performed two full scans of the sky in 2010 and 2011, capturing images of almost three-quarters of a billion galaxies, stars and asteroids. Analyzing data using NASA's AllWISE program, which makes it possible to compare the datasets more effectively, Kirkpatrick's team found 3,525 new stars and brown dwarfs within 500 light years of the Sun. These objects, says Kirkpatrick, were totally overlooked before now. In any...
Woven Light: Augmented Dreamstate
Heath Rezabek, an Austin, TX-based librarian, futurist and long-term thinker, continues the chronicle of his evolving work on the Vessel project and its ramifications. Developed as a strategy for preserving our cultural and biological heritage, Vessel is inevitably a way to re-examine ourselves in new and startling ways. Science fiction offers a supple way to visualize what generations in the near and far future may draw from such archives, leading perhaps to created intelligences that grow by sampling our imagery, our artifacts, our mythologies. In the passage that follows, we meet an SF writer named Thea Ramer, and learn more about Dr. Kaasura, whose early work with Vessel points to synthetic minds, re-woven patterns of quantum reality and the development of Saudade-class starships. But let Heath explain... by Heath Rezabek This is the third installment in a continuing series of speculative fiction here on Centauri Dreams. Feedback from prior installments helps shape the themes and...
Measuring Atmospheric Pressure on Exoplanets
We haven't talked much in these pages about atmospheric pressure when it comes to characterizing exoplanets, but recent discussions of 'super-Earths' and thick, hydrogen/helium atmospheres have raised the issue. All but simultaneously came the news of a paper from Amit Misra (a University of Washington graduate student) and co-authors describing a new way of detecting atmospheric pressure on exoplanets. Misra's simulations of Earth's own atmospheric chemistry involved teasing out the signature of dimer molecules from light at various wavelengths. While a monomer is a molecule that may bind chemically to other molecules, a dimer is a chemical compound made up of two similar monomers bonded together. Misra's work is intriguing because the stability of water on a planet's surface depends not just on temperature but pressure -- the latter affects water's boiling point and sublimation. Estimating surface pressure thus becomes an indicator for potential habitability. The problem is that...
Red Dwarfs: Planets in Abundance
Whether or not they’re suitable for life, habitable zone ‘super-Earths’ are seeing increased scrutiny around M-class dwarf stars because the mass ratio of planet to star makes detection easier than around more massive stars. We need radial velocity surveys to help us here because planets on orbits longer than 200-300 days will definitely be out of Kepler’s reach. Moreover, while Kepler targets many K, G and F-class stars, M-dwarfs aren’t bright enough to show up in large numbers in its field of view, making occurrence rates around such stars problematic. A 2013 paper by Courtney Dressing and David Charbonneau (Harvard-Smithsonian Center for Astrophysics) found that the Kepler sample contains 3897 stars with estimated effective temperatures below 4000K. Out of these, 64 are planet candidate host stars, with 95 candidate planets orbiting them. The researchers deduced from their analysis that about 15 percent of all red dwarfs have an Earth-sized planet in the habitable zone. Ravi...
An Interstellar Mission Statement
Yesterday I wrote about what Michael Michaud calls 'the new cosmic humanism,' looking back at an essay the writer and diplomat wrote for Interdisciplinary Science Reviews in 1979. Intelligence, Michaud believes, creates the opportunity to reverse entropy at least on the local scale, and to impose choice on a universe whose purpose we do not otherwise understand. Continuing growth into space, expansion and discovery are the kind of long-term goals humans can share, highlighting the extension of knowledge and the rediversification of our species. What Michaud is talking about is nothing less than a mission statement for extraterrestrial man, one that trades off a key uncertainty: In the face of an indifferent universe, intelligence itself may prove to be an evolutionary quirk that is of little consequence. Whether or not this is the case could depend on the decisions and purposeful choices of intelligent beings, assuming they choose to expand into the cosmos. Let me quote Michaud on...
Toward an Extraterrestrial Paradigm
Growing up in the Sputnik era, I followed the fortunes of space exploration with huge enthusiasm. In those days, the model was primarily planetary in nature, the progression from the Moon to the nearest planets and then beyond seemingly inevitable. At the same time, a second model was developing around the idea of space stations and self-contained worlds built by man, one that would reach high visibility in the works of Gerard O'Neill, but one that ultimately reached back as far as the 1920's (Oberth and Noordung) and further back to the science fiction of Jules Verne. In fact, E. E. Hale's "The Brick Moon" explored a space station as early as 1869. But even as our Mariners and Veneras explored other planets, an interstellar thread was also emerging. Robert Goddard wrote about interstellar journeys in 1918, science fiction was full of such travel as the field matured in the 1940s and '50s, and serious scientific study of interstellar flight became established by mid-century. Writing...
‘Super-Earths’ Problematic for Life
The Kepler announcements yesterday were greatly cheering to those of us fascinated with the sheer process of doing exoplanetology. The ‘verification by multiplicity’ technique propelled the statistical analysis that resulted in 715 newly verified worlds, and we have yet to turn it loose on two more years of Kepler data (check Hugh Osborn's excellent Lost in Transits site for more on the method). For those who focus primarily on habitable worlds, the results seemed a bit more sparse, with just four planets found in the habitable zone. And even where we find such, there are reasons to wonder whether a ‘super-Earth’ could actually sustain life. Apropos of this question, a team of researchers led by Helmut Lammer (Austrian Academy of Sciences) has just published the results of its modeling of planetary cores, looking at the rate of hydrogen capture and removal for cores between 0.1 and 5 times the mass of the Earth found in the habitable zone of a G-class star. Cores like these...
Kepler: Opening the Planet Verification Bottleneck
A planet like Kepler-296f is bound to get a lot of publicity. Orbiting a star half the Sun's size and only five percent as bright, this world, twice the size of the Earth, appears to orbit in the habitable zone, where liquid water could exist on its surface. We focus so much on the potential of life that the four planets announced yesterday (out of 715 newly verified worlds) inevitably get special treatment. And we learn that Kepler-296f exists in a system with four other planets, orbiting the star every thirty days. What we don't know is whether we're dealing with a small Neptune-class world surrounded by a thick hydrogen/helium atmosphere or a water world with a deep ocean. An interesting world, to be sure, but the real story in yesterday's announcements from the Kepler team has to do with the 'verification by multiplicity' technique used to validate the existence of so many planets in 305 star systems. One of the findings papers titled "Almost All of Kepler's Multiple Planet...
Science Fiction in Extreme Environments
I've had pulsars on the mind the last couple of days after our discussion of PSR 1257+12 and its contribution to exoplanetology. A bit more about pulsars today and the way we look at extreme objects through science fiction. PSR 1257+12 was discovered in 1990 by Aleksander Wolszczan using data from the Arecibo dish, and it was in 1992 that Wolszczan and Dale Frail published a paper outlining their discovery of the first planets ever found outside our Solar System. The two planets were joined by a third in 1994, but evidence for a fourth was later shown to be mistaken. In any case, the three planets confounded many astronomers, who hardly expected the first extrasolar planets to be found orbiting a radiation-spewing neutron star. Centauri Dreams regular Al Jackson was co-author of a 1992 study of PSR1257+12 that examined orbital resonance in the planets around the pulsar. In a note last night, Al mused "Just think of a K2 civilization setting up a research station on one of those to...
Tau Boötis b: A ‘3-D’ Look at Star and Planet
Strong evidence for water in the atmosphere of the hot Jupiter Tau Boötis b has turned up, thanks to work by Geoffrey Blake (Caltech) and graduate student Alexandra Lockwood. But what's intriguing about the find isn't the water -- we've found water vapor on other planets -- but the method of detection. Lockwood and Blake used a modified radial velocity technique that has previously been deployed to detect low mass ratio binary stars. A top-flight instrument like the Near Infrared Echelle Spectrograph (NIRSPEC) at the W. M. Keck Observatory in Hawaii can separate the planetary and stellar components spectroscopically to produce this result. Image: Simulated data showing the method used for detecting water vapor features around the hot Jupiter tau Boötis b. In this example, the planetary signal has been increased in strength by several orders of magnitude relative to the actual signal. The dotted lines show the blue- and red-shifts of the planetary and stellar lines in the data,...