Our First Galactic Ambassador

by Larry Klaes Larry Klaes is a long-time Centauri Dreams contributor, a practitioner of the Tau Zero Foundation and a serious devotee of space exploration and its history. Here he gives us a look at the Pioneer probes that first took us to the outer Solar System, journeys that foreshadowed the later exploits of the Voyagers and the more recent New Horizons mission to Pluto/Charon. It's hard to believe that it's been fully forty years since the Pioneers were launched. They came out of the era when thinking big was the order of the day, Apollo was putting astronauts on the Moon and human expansion into the cosmos seemed inevitable. When we ponder today's budget shortfalls and drifting public attention, it's heartening to recall that era even as we speculate about missions that will follow up on the findings of these two remarkable probes. The early 1970s was an exciting time for lunar and planetary exploration. On the Moon, Apollo was still placing pairs of astronauts on Earth's...

read more

Another Way of Looking at Interstellar Probes

By Michael Michaud The following post is a distinct change of pace for Centauri Dreams, a work of fiction that gets at questions at the heart of SETI. We've considered many ideas about interstellar probes that humans may one day launch toward nearby stars. But the reverse could occur: A more advanced technological civilization could send a probe in our direction, particularly after detecting signs of life or technology on a rapidly developing Earth. This idea is a challenge to the dominant scientific paradigm of contact -- our detection of radio signals from a remote society. The short story below presents one of many possible scenarios. In this case, the probe is an intelligent machine. It lacks the omniscience so often assumed in films and television programs; this form of intelligence, like ours, can misunderstand evidence and is capable of making mistakes. This story avoids the two stereotyped film and television versions of contact: being saved by altruistic aliens, or being...

read more

Titan’s Atmosphere Under Scrutiny

Of all the probe targets in the outer Solar System, Titan is in many ways the most provocative. Not long ago we looked at two concepts -- Titan Mare Explorer (TiME) and AVIATR -- that would get instruments back into Titan's atmosphere and, in the case of TiME, onto one of its northern seas. The allure of this moon is surely what goes on in that atmosphere, a nitrogen brew mixed with methane that generates complex hydrocarbons. We're learning how these fall on the surface to form patterns of dunes made up of organic material, all of this mediated by a weather cycle that involves seasonal change the Cassini spacecraft has strikingly recorded. Kathleen Mandt (Southwest Research Institute) has been studying methane in Titan's atmosphere over time using data both from Cassini and the European Space Agency's Huygens probe (digression: can it really be seven years since Huygens parachuted down through those orange skies? Good grief...) Mandt's team is looking at heavy methane -- methane...

read more

Coffee with Dr. Fermi

I cannot live without good coffee, and that means fresh beans ground right before brewing, and either manual drip or French press extraction. Every morning after publishing Centauri Dreams I make a couple of cups and go out on the deck to rest my eyes and ponder the state of things before hitting the books for background research in the afternoon. Various thoughts about what to write next always come to me, but yesterday I mused about Enrico Fermi, the legendary Italian physicist who, among so much else, left us with a great unanswered question: Where are they? If it’s so easy for the universe to make intelligent species, why is SETI coming up so short? Where are they indeed? The day was gorgeous, the air filled with birdsong, temperatures in the mid-60s and a mild breeze. What better setting to be immersed in, thinking about where life emerges and when? I imagined Fermi sitting across from me with a cup of my Costa Rica Tres Rios in his hand, wondering what he might say about the...

read more

100 Year Starship Site Launches

You'll want to bookmark the 100 Year Starship Initiative's new site, which just came online. From the mission statement: 100 Year Starship will pursue national and global initiatives, and galvanize public and private leadership and grassroots support, to assure that human travel beyond our solar system and to another star can be a reality within the next century. 100 Year Starship will unreservedly dedicate itself to identifying and pushing the radical leaps in knowledge and technology needed to achieve interstellar flight while pioneering and transforming breakthrough applications to enhance the quality of life on earth. We will actively include the broadest swath of people in understanding, shaping, and implementing our mission. And check here for news about the 2012 public symposium, which will be held in Houston from September 13-16. Quoting from that page: This year, 2012, DARPA gave its stamp of approval to and seed funded —100 Year Starship (100YSS)—a private...

read more

The Proxima Centauri Planet Hunt

Although we haven’t yet found any planets around Proxima Centauri, it would be a tremendous spur to our dreams of future exploration if one turned up in the habitable zone there. That would give us three potential targets within 4.3 light years, with Centauri A and B conceivably the home to interesting worlds of their own. And the issue we started to look at yesterday -- whether Proxima Centauri is actually part of the Alpha Centauri system or merely passing through the neighborhood -- has a bearing on the planet question, not only in terms of how it might affect the two primary stars, but also because it would tell us something about Proxima’s composition. A Gravitationally Bound System Greg Laughlin makes this case in the systemic post I referred to yesterday. It was Laughlin and Jeremy Wertheimer (UCSC) who used data from ESA’s Hipparcos mission to conclude that Proxima was indeed bound to Centauri A and B. Here I want to quote the conclusion of the duo’s paper on the matter,...

read more

Proxima Centauri: Looking at the Nearest Star

Let's start the week with a reminder about Debra Fischer's work on Alpha Centauri, which we talked about last week. There are several ongoing efforts to monitor Centauri A and B for planets and, given the scrutiny the duo have received for the past several years, we should be getting close to learning whether there are rocky worlds in this system or not. Fischer's continuing work at Cerro Tololo involves 20 nights of observing time that her grant money can't cover. Private donations are the key -- please check the Planetary Society's donation page to help if you can. While interest in the Alpha Centauri system is high, the small red dwarf component of that system has been getting relatively little press lately. But I don't want to neglect Proxima Centauri, which as far as we know is the closest star to the Earth (some 4.218 light years away, compared to Centauri A and B's 4.39 light years). From a planet around Centauri B, it would be hard to know that Proxima (also known as Alpha...

read more

Habitable Zones in Other Galaxies

We often speak of habitable zones around stars, most commonly referring to the zone in which a planet could retain liquid water on its surface. But the last ten years has also seen the growth of a much broader idea, the galactic habitable zone (GHZ). A new paper by Falguni Suthar and Christopher McKay (NASA Ames) digs into galactic habitable zones as they apply to elliptical galaxies, which are generally made up of older stars and marked by little star formation. Ellipticals have little gas and dust as compared to spirals like the Milky Way and are often found to have a large population of globular clusters. Are they also likely to have abundant planets? The answer is yes, based on the authors’ comparison of metallicity -- in nearby stars and stars with known planets -- to star clusters in two elliptical galaxies. While many factors have been considered that could affect a galactic habitable zone, Suthar and McKay focus tightly on metallicity, with planet formation dependent upon the...

read more

Closing in on Alpha Centauri

Alpha Centauri is irresistible, a bright beacon in the southern skies that captures the imagination because it is our closest interstellar target. If we learn there are no planets in the habitable zones around Centauri A and B, we then have to look further afield, where the next candidate is Barnard's Star, at 5.9 light years. Centauri A and B are far enough at 4.3 light years -- that next stretch adds a full 1.6 light years, and takes us to a red dwarf that may or may not have planets. Still further out are Tau Ceti (11.88 light years) with its problematic cometary cloud, and Epsilon Eridani (10.48 light years), a young system though one thought to have at least one planet. A warm and cozy planet around the K-class Centauri B would be just the ticket, and the planet hunt continues. One thing we've learned in the past decade is that neither Centauri A or B is orbited by a gas giant -- planets of this size should have shown up in the data by now. We've also learned that stable orbits...

read more

Neutrino Communications: An Interstellar Future?

The news that a message has been sent using a beam of neutrinos awakened a flood of memories. Back in the late 1970s I was involved with the Society for Amateur Radio Astronomers, mostly as an interested onlooker rather than as an active equipment builder. Through SARA’s journal I learned about Cosmic Search, a magazine that ran from 1979 through 1982 specializing in SETI and related issues. I acquired the entire set, and went through all 13 issues again and again. I was writing sporadically about SETI then for Glenn Hauser’s Review of International Broadcasting and later, for the SARA journal itself. Cosmic Search is a wonderful SETI resource despite its age, and the recent neutrino news out of Fermilab took me right back to a piece in its third issue by Jay Pasachoff and Marc Kutner on the question of using neutrinos for interstellar communications. Neutrinos are hard to manipulate because they hardly ever interact with other matter. On the average, neutrinos can penetrate four...

read more

How Will Humans Fly to the Stars?

by Andreas Hein The immense problems of time, distance and life support invariably mean that when we talk about an interstellar mission, we talk about robotics. But the imaginative team at Icarus Interstellar, which is now setting up projects on everything from beamed lightsails (Project Forward) to pulse propulsion engines (Project Helios), has pushed into the biggest what-if of all, the question of manned missions. And as project leader Andreas Hein reminds us in the following article, a variety of approaches have been suggested for this over the years from which a new concept study can grow. Andreas Hein received his master's degree in aerospace engineering at the Technische Universität München, and is doing his PhD at the same university in the area of space systems engineering at the Institute of Astronautics. He has participated in several mission studies: a lunar gravity measurement mission by EADS and a cubesat mission analysis. During his internship at ESA-ESTEC, he...

read more

Lightsails: Safe Passage After All?

Despite my best intentions, I still haven't put my hands on the exchange between Robert Forward and Ian Crawford on lightsails that ran back in 1986 in JBIS, nor have I managed to come up with the source of the 'lightsail on arrival' illustration I mentioned last week. This was the one showing a battered and torn sail docked in what I assume was a repair facility at the end of its long journey, and the effects of passage through the interstellar medium were all too obvious. It was a great image and I was frustrated about not being able to find the magazine it was published in, but an email from James Early quickly changed my mood. As opposed to the missing image that nagged at my memory, this was a case of having missed something perfectly obvious in the first place. I didn't know about the paper Jim did with Richard London on lightsails and the interstellar medium -- it was published in the Journal of Spacecraft and Rockets back in 2000, but somehow I didn't find it in the research...

read more

Collisions in the Interstellar Medium

Memories play tricks on us all, but trying to recall where I saw a particular image of a laser lightsail is driving me to distraction. The image showed a huge sail at the end of its journey, docked to some sort of space platform, and what defined it were the tears and holes in the giant, shredded structure. It presupposed long passage through an interstellar medium packed with hazards, and although I assumed I would have seen it on the cover of some science fiction magazine, I spent an hour yesterday scanning covers on Phil Stephensen-Payne’s wonderful Galactic Central site, but all to no avail. The image must have run inside a magazine, then, but if so, I’m at a loss to identify it other than to say it would have appeared about twenty years ago. I had hoped to reproduce it this morning because our talk about starship shielding necessarily brought up the question of whether an enormous lightsail -- some of these are conceived as being hundreds of kilometers in diameter -- wouldn’t be...

read more

Lasers: Protecting the Starship

Interesting new ideas about asteroid deflection are coming out of the University of Strathclyde (Glasgow), involving the use of lasers in coordinated satellite swarms to change an asteroid's trajectory. This is useful work in its own right, but I also want to mention it in terms of a broader topic we often return to: How to deal with the harmful effects of dust and interstellar gas on a fast-moving starship. That's a discussion that has played out many a time over the past eight years in these pages, but it's as lively a topic as ever, and one on which we're going to need a lot more information before true interstellar missions can take place. Lasers and the Asteroid But let's set the stage at Strathclyde for a moment. The idea here is to send small satellites capable of formation flying with the asteroid, all of them firing their lasers at close range. The university's Massimiliano Vasile, who is leading this work, says that the challenge of lasers in space is to combine high power,...

read more

The Largest Solar System Yet

The Kepler mission's exoplanet discoveries have been so numerous that an extension of the mission seemed all but inevitable. At the same time, bureaucracies can be unpredictable, which is why it was such a relief to have the Senior Review of Operating Missions weighing in with an extension recommendation, one followed up by NASA with extensions not just for Kepler but also for the Spitzer telescope and the US portion of ESA's Planck mission. Kepler's extension runs through fiscal 2016 (subject to review in 2014), allowing for plenty of time to home in on Earth-sized planets in the habitable zone around stars like our Sun. While Kepler's scheduled mission duration was 3.5 years, the mission was intended to be extendible to 6 years or more and this news is more than satisfying. But of course while we continue to monitor the Kepler work, we're following numerous other exoplanet stories including the European Southern Observatory's observations of the prolific star HD 10180, a Sun-like...

read more

Splashdown on Titan?

Getting to the stars may involve a sudden breakthrough -- we can't rule out disruptive technologies, nor can we predict them -- but my guess is that interstellar flight is going to be a longer, more gradual process. I can see a sort of tidal expansion into the outer system, forays to Mars, for example, followed by reassessment, retrenchment, then one day deeper study of Jupiter's moons with advanced robotics that can get under Europa's ice. The search for life may become so provocative that we have to explore Titan and Enceladus with human crews, and the imperative for planetary protection may help us further tune up our deep space technologies. The thing is, one wave of exploration inevitably begets another. Let's put no timeframe on that kind of expansion because, like the tides, it may surge at times and then fall back, hostage to budgetary problems and waves of public interest that can as easily ebb. But I could see an eventual civilization that extends throughout the Solar...

read more

Reasons for a Human Future in Space

I closed last week with two posts about the AVIATR mission, an unmanned airplane that could be sent to Titan to roam its skies for a year of aerial research. It’s a measure of Titan’s desirability as a destination that it has elicited so many mission proposals, and I want to get into the Titan Mare Explorer (TiME) as well, but let’s pause a moment to consider the nature of what we’re doing. Out of necessity, all our missions to the outer system have been unmanned, but as we learn more about long-duration life-support and better propulsion systems, that may change. The question raised this past weekend in an essay in The Atlantic is whether it should. Ian Crawford, a professor of planetary sciences at Birkbeck College (London) is the focus of the piece, which examines Crawford’s recent paper in Astronomy and Geophysics. It’s been easy to justify robotic exploration when we had no other choice, but Crawford believes not only that there is a place for humans in space, but that their...

read more

A Closer Look at the Titan Airplane

Yesterday's discussion of the AVIATR mission to Titan inevitably brought up another prominent Titan mission concept: Titan Mare Explorer (TiME). I'll have more to say about this one next week, as today I want to continue talking about AVIATR, but you can once again see how Titan enthralls us with its 'Earth-like' aspects. Need a thick atmosphere around a moon? Titan is your only play, and if, as with TiME, you want to put an instrument package into an off-planet surface lake, you'll be hard pressed to do it anywhere else, at least in this Solar System. These two mission concepts fire the imagination -- they're the kind of thing kids like me used to dream about when we plunked down our money at the newsstand for copies of Galaxy or Fantasy & Science Fiction. It's unlikely, though, that both missions will fly. If TiME, which is a Discovery-class mission finalist and thus cost-capped at $425 million, is chosen, then the odds on AVIATR probably drop. AVIATR, a New Frontiers-class...

read more

AVIATR: Roaming Titan’s Skies

Each of our highest priority targets in the outer Solar System offers something unique, from Europa’s internal ocean to the geysers of Enceladus. But Titan exerts the kind of fascination that comes from the familiar. The imagery of lakes and river channels reminds us inescapably of our home world, even if the temperature on the Saturnian moon averages a brisk 94 K, which works out to -291 degrees on the Fahrenheit scale. But because of its thick atmosphere we have options for exploring Titan that are unavailable on the other icy moons, and we’re working with a landscape that is a compelling frozen doppelgänger of Earth, a landscape we’d like to explore up close. As we saw yesterday, part of the outer system puzzle is getting supplies of plutonium-238 up to speed, and there is at least some movement on that front. If we want to get aggressive about exploring Titan, one excellent way to deploy that plutonium is aboard AVIATR (Aerial Vehicle for In-situ and Airborne Titan...

read more

Plutonium-238 and the Outer System

Powering up a spacecraft is a lot easier to manage in the Sun-rich environment inside the orbit of Mars than it is out past the orbit of Jupiter. Solar panels provide plenty of power for a satellite in near-Earth orbit, for example, but moving into the outer system invokes the need for RTGs -- radioisotope thermoelectric generators -- powered by radioactive decay. If you read through the specs on the FOCAL mission design presented here last Friday, you saw that this attempt to reach the Sun's gravitational lens would demand 20 RTGs, and thus requires resumed production of plutonium-238. What's happened is that US production of 238Pu was halted as far back as 1988, leaving us with stockpiles that should be sufficient for missions in the pipeline through the end of this decade. That's the view of Leonard Dudzinski, NASA's Radioisotope Thermoelectric Generator program executive, who was speaking at the opening session of the 43rd Lunar and Planetary Science and the Nuclear and Emerging...

read more

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

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