Paul Gilster | Centauri Dreams

Interstellar Space: Uses of the Medium

by Paul Gilster | Mar 20, 2012 | Missions | 3 Comments

One of the first things we need to do in terms of interstellar exploration is to get a spacecraft built for the purpose to travel outside the heliosphere and give us solid measurements on the interstellar medium. The Voyagers are doing their best but they were never designed for what has become their interstellar mission, and while we can marvel at their longevity, it's with the knowledge that their resources are few and their years of useful data gradually drawing to an end. Something along the lines of Ralph McNutt's Innovative Interstellar Explorer would do the job nicely, allowing us to sample the environment that much longer missions will have to work in. Lorentz Force Turning The interstellar medium (ISM) is important not just because we have to learn about things like shielding a fast-moving spacecraft and cosmic ray flux but also because we may be able to use some aspects of the medium for deceleration. Yesterday's discussion of magsails reminded me of a 1969 paper by P. C....

Braking Against a Stellar Wind

by Paul Gilster | Mar 19, 2012 | Interstellar Medium | 12 Comments

This morning I want to pick up on the 'problem of arrival' theme I began writing about on Friday, and we'll look at interstellar deceleration issues a good bit this week. But I can't let Monday start without reference to the Icarus results from Gran Sasso that finds neutrinos traveling at precisely the speed of light. All of this adds credence to the growing belief that the earlier Opera experiment was compromised by equipment problems. The news is all over the place (you might begin with this BBC account) and while we'll keep an eye on it, I don't plan to spend much time this week on neutrinos. We still have much to get done on the subject of slowing down. Magsails and Local Resources When you begin to unlock the deceleration issue, the options quickly multiply, and you find yourself looking into areas that weren't remotely the subject of your earlier research. As we saw on Friday, the concept of magnetic sails grew organically out of Robert Bussard's idea of an interstellar ramjet....

Starships: The Problem of Arrival

by Paul Gilster | Mar 16, 2012 | Sail Concepts | 30 Comments

You wouldn't think that slowing down a starship would be the subject of a totally engrossing novel, but that's the plot device in Poul Anderson's Tau Zero (1970, though based on a 1967 short story called "To Outlive Eternity"). Anderson's ramscoop starship, the Leonora Christine, can't slow down because of damage suffered in mid-cruise. Edging ever closer to the speed of light, the crew experiences all sorts of time dilation wonders as they wrestle to regain control, and the ending, while scientifically dubious, is also in every way unforgettable. Anderson could be guilty of over-writing but few writers are gifted with his sheer imaginative sweep. I'm thinking that coupling a ramscoop with a problem in deceleration is just the ticket for getting into the whole issue of starship arrivals. We can start with Robert Bussard's 1960 paper "Galactic Matter and Interstellar Spaceflight," which unwittingly paved the way for the whole magsail concept. Bussard came up with what for a time...

WISE: Into the Infrared Sky

by Paul Gilster | Mar 15, 2012 | Deep Sky Astronomy & Telescopes | 13 Comments

As promised, we now have the infrared sky at a new level of detail thanks to the labors of the Wide-Field Infrared Survey Explorer (WISE) mission, which has now mapped (with a few slight glitches) more than half a billion objects, from galaxies to stars to asteroids and comets. We can now expect a new wave of papers from the more than 2.7 million images WISE has delivered at four infrared wavelengths and can explore the WISE atlas of some 18,000 images ourselves. The Big Picture But first, I want to step back and look at astronomical discovery in context, a thought spurred by Larry Klaes, who sent me a note originally posted on the HASTRO-L mailing list (by Rich Sanderson, of the Springfield Science Museum in Massachusetts). Every now and then I read something that wraps back into the past and yet implies future things, generating a sense of connection with what the enterprise is all about. Such is the case in this passage Sanderson quotes from an 1875 book by Richard Proctor that...

Thoughts on Antihydrogen and Propulsion

by Paul Gilster | Mar 14, 2012 | Antimatter | 22 Comments

Normally when we talk about interstellar sail concepts, we're looking at some kind of microwave or laser beaming technologies of the kind Robert Forward wrote about, in which the sail is driven by a beam produced by an installation in the Solar System. Greg and Jim Benford have carried out sail experiments in the laboratory showing that microwave beaming could indeed drive such a sail. But Steven Howe's concept, developed in reports for NASA's Institute for Advanced Concepts, involved antimatter released from within the spacecraft. The latter would encounter a sail enriched with uranium-235 to reach velocities of well over 100 kilometers per second. That's fast enough to make missions to the nearby interstellar medium feasible, and it points the way to longer journeys once the technology has proven itself. But everything depends upon storing antihydrogen, which is an antimatter atom -- an antiproton orbited by a positron. Howe thinks the antihydrogen could be stored in the form of...

Looking Into Kepler’s Latest

by Paul Gilster | Mar 13, 2012 | Astrobiology and SETI, Exoplanetary Science | 37 Comments

I've held off a bit on the latest Kepler data release because I wanted some time to ponder what we're looking at. The list of candidate planets here is based on data from the first sixteen months of the mission, and at first blush it seems encouraging in terms of our search for Earth-class planets. But dig deeper and you realize how much we still have to learn. Not all the trends point to the near ubiquity of rocky worlds in the habitable zone that some have hoped for. You might remember, for example, Carl Sagan famously saying (on 'Cosmos') that one out of every four stars may have planets, with two in each such system likely to be in the habitable zone. Kepler's Candidates and Some Qualifications I remember being suitably agog at that statement, but we've learned more since. John Rehling, writing an essay for SpaceDaily, didn't miss the Sagan quote and uses it to contrast with his own analysis of the new Kepler material showing that Earth-like planets may be considerably harder to...

Upcoming Interstellar Sessions

by Paul Gilster | Mar 12, 2012 | Culture and Society | 3 Comments

It's shaping up to be an interesting week. I want to get to the recent Kepler data release, and also to the antimatter news from CERN, and I also want to talk about everything from decelerating an interstellar craft to models of expansion into the galaxy a la Frank Tipler. [And thanks to Centauri Dreams reader Eric Goldstein for reminding me of the upcoming WISE data release on the 14th!]. For today, though, let's look at two upcoming conferences, especially since I'm running behind in getting to the first of them, the CONTACT 2012 gathering, which is coming up right away. The full title of this one is CONTACT: Cultures of the Imagination, and it's a meeting with a rich history. Back in 1979, Jim Funaro was teaching a course in anthropology at Cabrillo College (Aptos, CA) that used science fiction as a vector into the scientific issues his course raised. The course allowed students to go to work creating cultures and, in a game-like simulation, to explore how the fictional societies...

Science Fiction and the Probe

by Paul Gilster | Mar 9, 2012 | Culture and Society | 30 Comments

Physicist Al Jackson, who is the world's greatest dinner companion, holds that title because amongst his scientific accomplishments, he is also a fountainhead of information about science fiction. No matter which writer you bring up, he knows something you never heard of that illuminates that writer's work. So it was no surprise that when the subject of self-replicating probes came up in these pages, Al would take note in the comments of Philip K. Dick's story "Autofac," which ran in the November, 1955 issue of H. L. Gold's Galaxy. A copy of that issue sits, I am happy to say, not six feet away from me on my shelves. This is actually the first time I ever anticipated Al -- like him, I had noticed "Autofac" as one of the earliest science fiction treatments of the ideas of self-replication and nanotechnology, and had written about it in my Centauri Dreams book back in 2004. If any readers know of earlier SF stories on the topic, please let me know in the comments. In the story, the two...

Intelligent Probes: The Spread-Spectrum Challenge

by Paul Gilster | Mar 8, 2012 | Astrobiology and SETI | 21 Comments

Let's imagine for a moment that John Mathews (Pennsylvania State University) is right in theorizing that space-faring civilizations will use self-reproducing probes to expand into the galaxy. We've been kicking the issues around most of this week, but the SETI question continues to hang in the background. For if there really are extraterrestrial civilizations in the nearby galaxy, how would we track down their signals if they used the kind of communications network Mathews envisions, one in which individual probes talked to each other through tight-beam laser communications designed only for reception by the network itself? One problem is that the evidence we're looking for would most likely come in the form of spread-spectrum signals, a fact Jim Benford pointed out in a comment to my original post on Mathews, and one that also pointed to recent work by David Messerschmitt (UC-Berkeley). The latter makes a compelling case for spread-spectrum methods as the basis for interstellar...

SETI and Self-Reproducing Probes

by Paul Gilster | Mar 7, 2012 | Astrobiology and SETI | 14 Comments

It was back in the 1980s when Robert Freitas came up with a self-reproducing probe concept based on the British Interplanetary Society's Project Daedalus, but extending it in completely new directions. Like Daedalus, Freitas' REPRO probe would be fusion-based and would mine the atmosphere of Jupiter to acquire the necessary helium-3. Unlike Daedalus, REPRO would devote half its payload to what Freitas called its SEED package, which would use resources in a target solar system to produce a new REPRO probe every 500 years. Probes like this could spread through the galaxy over the course of a million years without further human intervention. A Vision of Technological Propagation I leave to wiser heads than mine the question of whether self-reproducing technologies like these will ever be feasible, or when. My thought is that I wouldn't want to rule out the possibility for cultures significantly more advanced than ours, but the question is a lively one, as is the issue of whether...

Robotic Networks Among the Stars

by Paul Gilster | Mar 6, 2012 | Missions | 62 Comments

Imagine a future in which we manage to reach average speeds in the area of one percent of the speed of light. That would make for a 437-year one-way trip to the Alpha Centauri system, too long for anything manned other than generation ships or missions with crews in some kind of suspended animation. Although 0.01c is well beyond our current capabilities, there is absolutely nothing in the laws of physics that would prevent our attaining such velocities, assuming we can find the energy source to drive the vehicle. And because it seems an achievable goal, it's worth looking at what we might do with space probes and advanced robotics that can move at such velocities. How, in other words, would a spacefaring culture use artificial intelligence and fast probes to move beyond its parent solar system? John Mathews ( Pennyslvania State) looks at the issue in a new paper, with a nod to the work of John von Neumann on self-reproducing automata and the subsequent thoughts of Ronald Bracewell...

Oxygen Detected at Saturn’s Moon Dione

by Paul Gilster | Mar 5, 2012 | Uncategorized | 7 Comments

We recently looked at biosignatures as part of a discussion about using polarized light to examine exoplanet atmospheres. As if on cue, we now get a reminder of how carefully the biosignature hunt must proceed. It's not enough, for example, to find one or two interesting gases in a distant atmosphere, for natural processes can account for potential biomarkers, which is why we need to find gases like ozone and methane, oxygen and carbon dioxide existing simultaneously. The most recent discovery from Cassini data puts an exclamation point on the matter with the discovery of molecular oxygen ions in the thin atmosphere of Dione, one of Saturn's 62 moons. With a radius of no more than 560 kilometers, Dione is evidently composed of a layer of water ice surrounding a rocky core. We are not, obviously, talking about a thick atmosphere around a world this small. Cassini and its CAPS instrument (Cassini Plasma Spectrometer) closed to within 503 kilometers of the surface in April of 2010,...

A New Take on Planet Formation

by Paul Gilster | Mar 2, 2012 | Exoplanetary Science | 10 Comments

Figuring out how planets form is an old occupation, with the basic ideas of planetary accretion going back several centuries, though tuned up, to be sure, in the 1970s and tweaked ever since. In a disk of gas and dust orbiting a young central star, dust grains begin to clump together, eventually forming planetesimals. Accretion models assume that these small planetesimals bang into each other and gradually grow. The assumption is that in the inner system at least temperatures are hot and the era of planet formation occurs well after the central star has formed. Image: Artist's conception of a protoplanetary disk. Credit: NASA/JPL-Caltech/T. Pyle. Adjust for distance from the star and subsequent planetary migration in the gas/dust disk and you can come up with a system more or less like ours, with rocky inner worlds and gas giants out beyond the snow line, the latter being the distance from the star where it is cool enough for volatile icy compounds to remain solid. But Anne...

Finding Life Through Polarized Light

by Paul Gilster | Mar 1, 2012 | Exoplanetary Science | 16 Comments

One of these days we're going to have a new generation of telescopes, some in space and some on the Earth, that can analyze the atmosphere of a terrestrial world around another star. It's not enough to find individual gases like oxygen and ozone, carbon dioxide or methane. Any of these can occur naturally without ramifications for life. But finding all of these gases in the same atmosphere is telling, because without life to replenish them, some would disappear. Getting the data is going to be hard, which is why new work using the European Southern Observatory's Very Large Telescope is so interesting. The work involves 'Earthshine,' the reflection of sunlight off the Earth that is in turn reflected off the surface of the Moon. It's faint, to be sure, but Earthshine is visible in a crescent Moon when the light of the entire lunar disc is visible although only the crescent is brightly lit. Michael Sterzik (ESO) and team have used Earthshine to analyze our own planet's biosignature, and...

Remembering an Astronautical Pioneer

by Paul Gilster | Feb 29, 2012 | Culture and Society | 6 Comments

by Claudio Maccone Physicist Les Shepherd, whose funeral is today, left friends throughout the astronautical community. Claudio Maccone, who worked with Shepherd on many occasions, was quick to offer his recollections of this remarkable man whose standards of excellence and unflagging support helped many young scientists as they embarked on careers in space science. A young guy (44 years old, i.e. "young" by IAA standards) joins the IAA Interstellar Space Exploration Committee (ISEC) headed by Les Shepherd and Giovanni Vulpetti: that happened at the World Space Congress in Washington, D.C., USA, also known as the 43rd IAC, August 28 - September 5, 1992). I was then working at Alenia Spazio SpA in Torino (Turin), Italy, and I had this secret love for future interstellar space missions ("secret" since at my space company nobody was interested, of course). So, I consulted with my good old friend and "teacher" (he is senior than I) Giovanni Vulpetti, who was in a similar position at...

Les Shepherd, RIP

by Paul Gilster | Feb 28, 2012 | Culture and Society | 5 Comments

There are so many things to say about Les Shepherd, who died on Saturday, February 18, that I scarcely know where to begin. Born in 1918, Leslie Robert Shepherd was a key player in the creation of the International Astronautical Federation (IAF), becoming its third president in 1957 -- this was at the 8th Congress in Barcelona just a week after the launch of Sputnik -- and in 1962 he would be called upon to serve as its president for a second time. A specialist in nuclear fission who became deeply involved in nuclear reactor technology, Shepherd was one of the founding members of the International Academy of Astronautics (IAA), and served as chairman of the Interstellar Space Exploration Committee, which met for the first time at the 1984 IAF Congress in Lausanne, Switzerland. The IAF Congress in Stockholm the following year was the scene of the first ISEC symposium on interstellar flight, one whose papers were subsequently collected in one of the famous 'red cover' issues of the...

Project Icarus: Contemplating Starship Design

by Paul Gilster | Feb 27, 2012 | Missions | 68 Comments

Andreas Tziolas, current leader of Project Icarus, gave a lengthy interview recently to The Atlantic's Ross Andersen, who writes about starship design in Project Icarus: Laying the Plans for Interstellar Travel. Icarus encounters continuing controversy over its name, despite the fact that the Icarus team has gone to some lengths to explain the choice. Tziolas notes the nod to Project Daedalus leader Alan Bond, who once referred to "the sons of Daedalus, perhaps an Icarus, that will have to come through and make this a much more feasible design." I like that sense of continuity -- after all, Icarus is the follow-on to the British Interplanetary Society's Project Daedalus of the 1970s, the first serious attempt to engineer a starship. I also appreciate the Icarus' team's imaginative re-casting of the Icarus myth, which imagines a chastened Icarus washed up on a desert island planning to forge wings out of new materials so he can make the attempt again. But what I always fall back on is...

FTL Neutrinos: Closing In on a Solution

by Paul Gilster | Feb 24, 2012 | Exotic Physics | 56 Comments

The news that the faster-than-light neutrino results announced to such widespread interest by the OPERA collaboration have now been explained has been spreading irresistibly around the Internet. But the brief piece in ScienceInsider that broke the news was stretching a point with a lead reading "Error Undoes Faster-Then-Light Neutrino Results." For when you read the story, you see that a fiber optic cable connection is a possible culprit, though as yet an unconfirmed one. Sean Carroll (Caltech) blogged on Cosmic Variance that while he wanted to pass the news along, he was reserving judgment until a better-sourced statement came to hand. I've thought since the beginning that a systematic error would explain the 'FTL neutrino' story, but I still was waiting for something with more meat on it than the ScienceInsider news. It came later in the day with an official CERN news release, and this certainly bears quoting: The OPERA collaboration has informed its funding agencies and host...

M-Dwarfs: A New and Wider Habitable Zone

by Paul Gilster | Feb 23, 2012 | Exoplanetary Science | 18 Comments

I want to work a new paper on red dwarf habitability in here because it fits in so well with yesterday's discussion of the super-Earth GJ1214b. The latter orbits an M-dwarf in Ophiuchus that yields a hefty 1.4 percent transit depth, meaning scientists have a strong lightcurve to work with as they examine this potential 'waterworld.' In transit terms, red dwarfs, much smaller and cooler than the Sun, are compelling exoplanet hosts because any habitable worlds around them would orbit close to their star, making transits frequent. When I first wrote about red dwarfs and habitability in my Centauri Dreams book, it was in connection with the possibilities around Proxima Centauri, but of course we can extend the discussion to M-dwarfs anywhere, this being the most common type of star in the galaxy (leaving brown dwarfs out of the equation until we have a better idea of their prevalence). Manoj Joshi and Robert Haberle had published a paper in 1997 that described their simulations for...

A Waterworld Around GJ1214

by Paul Gilster | Feb 22, 2012 | Exoplanetary Science | 42 Comments

I love the way Zachory Berta (Harvard-Smithsonian Center for Astrophysics) describes his studies of the transiting super-Earth GJ1214b. Referring to his team's analysis of the planet's atmosphere, Berta says "We're using Hubble to measure the infrared color of sunset on this world." And indeed they have done just this, discovering a spectrum that is featureless over a wide range of wavelengths, allowing them to deduce that the planet's atmosphere is thick and steamy. The conclusion most consistent with the data is a dense atmosphere of water vapor. Discovered in 2009 by the MEarth project, GJ1214b has a radius 2.7 times Earth's and a mass 6.5 times that of our planet. It's proven to be a great catch, because its host star, an M-dwarf in the constellation Ophiuchus, offers up a large 1.4 percent transit depth -- this refers to the fractional change in brightness as the planet transits its star. Transiting gas giants, for example, usually have transit depths somewhere around 1 percent,...

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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).

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