Rethinking Galactic Empire

How much would an extraterrestrial civilization resemble our own? The question resonates because on the one hand, the signature of our activities is what we tend to translate into the SETI search. We look, for example, for the signs of civilizations that are like us but more advanced technologically, which means we apply human thinking and motivations to cultures that are by definition not human. This is natural enough, because we're the only technological civilization we know about, but it leads to results that may mislead us and obscure the actual situation. Fermi's Great Silence bothers us because we assume that what Milan ?irkovi? calls advanced technological civilizations (ATCs) will necessarily move out into the galaxy to colonize it. Yet we see no signs of this, no presence of an expansive power, no characteristic emissions telling us of any intelligence operating around nearby stars. This observation becomes a paradox only if we think in specifically human terms, relating...

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Weekend Reading on Catastrophe

Alan Boyle uses the occasion of Neal Turok's appointment as executive director of the Perimeter Institute for Theoretical Physics to interview the scientist on topics dear to the heart of Centauri Dreams readers. The ekpyrotic universe idea championed by Turok uses the idea of multidimensional 'branes' whose occasional collisions spark events like the Big Bang. A cyclic model emerges that sees multiple 'bangs,' using today's accelerating universe as a condition for the arrival of the next cycle. It's fascinating stuff, but does it assume the eventual validation of string theory? Boyle quotes Turok: "In my opinion, string theory is the most promising avenue we have for the unification of gravity and the fundamental forces. But that doesn't mean I'm not critical of it. I think sometimes people do exaggerate its achievements thus far. We need to keep an open mind." Turok, as director of Cambridge University's Center for Theoretical Cosmology, worked with Princeton's Barry Steinhardt on...

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Laser Help for Terrestrial Planet Search

Boosting the sensitivity of our exoplanet search tools by a hundredfold is no small matter, yet that's just what optical frequency combs, when implemented with an ultrafast laser, may be able to do. A frequency comb is created by a laser that generates short, equally spaced pulses of light. 'Locking' the individual frequencies -- keeping them in phase with each other -- is essential, as is producing pulses that are no more than a few million billionths of a second long. The image below explains the name, the graph giving the impression of nothing more than a fine-toothed comb (and see this National Institute of Standards and Technology backgrounder for further details on how these combs work). We've looked at laser combs before, in particular in the work being performed at the Harvard Smithsonian Center for Astrophysics, which is involved in the deployment of such a comb at the William Herschel Observatory in the Canary Islands. The resultant instrument, called the HARPS-NEF...

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Filaments of Missing Matter?

It's hard enough to figure out what dark energy and dark matter are, a task that will occupy physicists for a long time to come. But even if we confine ourselves to 'normal' or 'baryonic' matter (accounting only for some four or five percent of the universe), we're still left with a problem. Baryons are heavy subatomic particles like protons and neutrons that experience the strong nuclear force, and the problem is that even these relatively familiar particles are only partially accounted for. So where is the missing baryonic matter? The answer may lie in a thin haze of hot, low-density gas that connects galactic clusters. Call it WHIM, for warm-hot intergalactic medium. Dutch and German scientists now think they have uncovered a filament of such gas that connects the clusters Abell 222 and Abell 223. The properties of the gas, visible primarily in the far ultraviolet and X-ray bands, fit with simulations in terms of density and temperature. The scientists used the XMM-Newton X-ray...

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Arecibo Observatory May be Safe at Last

By Larry Klaes Any good news from Arecibo is welcome, and Larry Klaes here delivers it. The observatory, threatened with closure despite its key role in the hunt for Earth-crossing asteroids, may have found at least temporary deliverance. Politics seems to have played a role, as Larry notes, but for once with results that benefit science rather than compromising it. Meanwhile, a new study of the Chixculub impact 65 million years ago tells us that a hail of carbon cenospheres -- tiny carbon beads -- may have fallen planet-wide following the strike. The more we learn about past impacts, the more we realize how important a role our planetary radars play in forestalling future catastrophe. What exists on the island of Puerto Rico that is over 1,000 feet across, could hold ten billion bowls of cereal, pick up a cell phone call from the planet Venus, once sent a message to any potential inhabitants of a distant globular star cluster, discovered the first planets around another star, has...

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A Space-Based Asteroid Telescope

One of the world's largest impact craters (see below) lies under Mexico's Yucatan peninsula, evidently a major player in the demise of the dinosaurs. Chicxulub is 180 kilometers in diameter, the subject of continuing research by the man who identified it, Alan Hildebrand (University of Calgary). So you could say Hildebrand has an idea what massive impacts from asteroids can do to the Earth's surface, having studied the environmental effects caused by this one and mapping the crater's structure to identify mineral, oil and gas resources. That interest has led Hildebrand into an ongoing asteroid hunt, and explains his current plans to build and launch a space-based observatory designed to look for near-Earth objects. The scientist currently uses use a retrofitted satellite tracking telescope in NEO work here on Earth. The instrument, based at the University of Calgary's Rothney Astrophysical Observatory (some 75 kilometers southwest of the city) is an extensive re-build, a Cold War era...

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The Odds on Interstellar Panspermia

Our recent look at panspermia concepts was largely devoted to the transmission of life via microbes or spores here in our own Solar System. The even richer question of how life might pass from star to star is far more problematic, but as a follow-up to that earlier story, I want to look at work that graduate student Jess Johnson did with Jonathan Langton and advisor Greg Laughlin at the University of California, Santa Cruz. Their work suggests that while life might readily survive an interstellar journey, it is unlikely to wander close enough to seed another system. Ponder the era here on Earth known as the Late Heavy Bombardment (LHB). After the period of planetary accretion ended some 4.4 billion years ago, life apparently began. But 3.8 to 4 billion years ago, the LHB saw the planet again pummeled, causing debris to be ejected into space. Looking specifically at the mass that is ejected at 16.7 kilometers per second in the direction of the Earth's motion (this is Solar System...

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Near-Term Concepts for a Fast Ticket Outward

From the first anniversary edition of the Carnival of Space, I'll send you this week to Brian Wang's discussion of two propulsion concepts for the near future. VASIMR (variable specific impulse magnetoplasma rocket) is under active development at Franklin Chang Diaz' Ad Astra Rocket Company, a site to monitor for developments in a technology that offers potential specific impulses from 1,000 to 30,000 seconds. That's a major upgrade compared to conventional rocket designs, and one that could conceivably get us to Mars in as little as 39 days. The Finnish solar electric sail concept, which we've also looked at here, may be well enough along for a flight test in 2010, assuming the budgetary gods are smiling. Our next step outward depends upon bumping up trip times to relatively nearby destinations like Mars and the asteroids, and these are two of the more promising concepts for making that a reality.

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Black Holes in Intergalactic Space?

Physicists have recently theorized that the merger of two black holes would create gravitational waves that could eject the resultant object from its galaxy. Now such a black hole event has been observed for the first time. Theory predicted that the gravitational waves would be emitted primarily in one direction, pushing the newly enlarged black hole in the opposite, and that is what we seem to be looking at, according to scientists at the Max Planck Institute for Extraterrestrial Physics (MPE). We can't see black holes themselves, nor have we yet directly detected gravitational waves. But we can observe the interactions around black holes, in this case the broad emission lines of gases carried with the recoiling black hole as it exits its galaxy, which contrast with the narrow emission lines of the gases the object left behind. These data allowed the object's speed -- a scorching 2650 kilometers per second -- to be measured. The recoil caused by the merger is pushing the black hole,...

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Scattering Life Through the Cosmos

Olaf Stapledon's Last and First Men (1930), amongst other wonders, pictures our descendants millions of years hence moving from world to world as they attempt to save the species. The Moon approaches the Earth, an imminent peril the 'Fifth Men' escape by terraforming Venus, unfortunately destroying indigenous life forms there. Later, the Fifth Men move on to Neptune, and when their existence there is endangered, they make an attempt to save themselves as a species by seeding their cells among the stars. Interestingly enough, Francis Crick (famed as a co-discoverer of the structure of DNA) suggested in 1973 that life could have been intentionally sent from elsewhere in the universe with the express purpose of finding a new home, an idea that made the later work of Fred Hoyle and Chandra Wickramasinghe seem positively tame. We're talking panspermia, the idea that life can survive long journeys through space to seed other planets (a notion Hoyle addressed in 1982's Evolution from...

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Ancient Galaxies Packed with Stars

Just how different were things in the early universe? One answer comes from a study of galaxies whose light has taken eleven billion years to reach us. In this early era -- the universe would have been less than three billion years old -- researchers have found galaxies so unusually compact that they compress a galaxy's worth of stars into a space only five thousand light years across. Such objects would be able to fit into the central hub of the Milky Way. What's more, these ultra-dense galaxies may account for as much as half the number of all galaxies of their mass that existed at this time. "In the Hubble Deep Field, astronomers found that star-forming galaxies are small," said Marijn Franx of Leiden University, The Netherlands. "However, these galaxies were also very low in mass. They weigh much less than our Milky Way. Our study, which surveyed a much larger area than in the Hubble Deep Field, surprisingly shows that galaxies with the same weight as our Milky Way were also very...

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The ‘Great Filter’ Tackles Fermi

Suppose for a moment that life really is rare in the universe. That when we are able to investigate the nearby stars in detail, we not only discover no civilizations but few living things of any kind. If all the elements for producing life are there, is there some kind of filter that prevents it from proceeding into advanced and intelligent stages that use artifacts, write poetry and build von Neumann probes to explore the stars? Nick Bostrom discusses the question in an article in Technology Review, with implications for our understanding of the past and future of civilization. Choke Points in the Past Maybe intelligent beings bring about their own downfall, a premise that takes in more than the collapse of a single society. Alaric's Goths took Rome in 410, hastening the decline of a once great empire, but the devastated period that followed saw Europe gradually re-build into the Renaissance. And as Bostrom notes, while a thousand years may seem like a long time to an individual,...

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Surface Oceans Around Distant Stars

Would large amounts of water on the surface provide a glint of light in both the infrared and visible spectrum if we study a distant exoplanet long enough? That's the premise of an investigation now in progress, one aiming to find Earth-like planets in the habitable zone of a star. Darren Williams (Penn State Erie) and Eric Gaidos (University of Hawaii) have something more in mind than analyzing a planetary atmosphere for signs of water. They want to spot planets with water on the surface. If the goal sounds chimerical now, bear in mind that various planet-hunting missions like Terrestrial Planet Finder (in its various incarnations) and Darwin are being designed to allow direct observation of planets as small as the Earth. Such observatories, which may be in place within two decades or less, could also examine the visible and infrared light curve of such planets over the course of an entire orbit. "We are going to look at the planets for a long time," says Williams. "They reflect one...

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Dark Matter: Flashes Beneath the Earth

Dark matter is interesting in its own right, a mysterious 'something' that according to WMAP data must account for 23 percent of the universe (the breakdown now thought to be 72 percent dark energy, 23 percent dark matter, 4.6 percent atoms and less than 1 percent neutrinos). From a propulsion standpoint, dark matter intrigues us because it may represent a reaction mass conceivably useful for future space flight. It's also Nobel Prize territory for the team that identifies it, which is why so many teams are looking, with one team's provocative results drawing criticism. The Italian and Chinese physicists on the DAMA Project have held out since 2000 for their claim that they are detecting dark matter beneath the Gran Sasso mountain in Italy. The modulation is yearly and could represent the Earth's motion through a dark matter stream as it orbits the Sun. The larger DAMA/LIBRA experiment now reaffirms the phenomenon, which appears as flashes in the team's sodium iodide detector. With...

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Down and Dirty in the Data

astroENGINE.com hosts the 51st Carnival of Space, a lengthy compilation indeed, from which I'll draw Ian Musgrave's interesting post on a possible transit at 83 Leonis as the feature of the week. If you want to find out what it's like to get your hands dirty juggling the data, trying to sift out signal from noise and working with all the imponderables that go into spotting the signature of a transiting world, have a look. Ian finds a noisy 83 Leonis but one that just might show a transit. A self-described 'mathematically challenged biologist,' this is a writer whose work is always worth watching. In this case, what he's doing reflects the broadening participation of amateurs in exoplanet projects, an idea Greg Laughlin has championed, so it's no surprise to see that Ian has drawn from Laughlin's expertise in his current work.

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Degrees of Visibility

Alexander Zaitsev's latest contribution to the debate over sending messages to the stars is a short paper that looks at how visible our planet might be thanks to transmissions from planetary radars like Arecibo, Goldstone or the Evpatoria site from which directed transmissions have already been sent. METI (Messaging to Extra-Terrestrial Intelligence) is broadly dedicated to transmitting messages to stars likely to have habitable planets, but so far the number of transmissions is relatively sparse. The debate over METI discusses the wisdom of continuing them without broader discussion. But tucked within that debate is the specific question of our civilization's visibility. For in addition to the messages that have already been sent, beginning with the Arecibo message in 1974 and continuing in the far more targeted transmissions from Evpatoria between 1999 and 2003, we are using our planetary radars to perform crucial astronomical studies. The work these dishes do in refining our...

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Electric Sails: Leave the Propellant at Home

A Finnish design making the news recently is hardly the only concept for near-term space sailing, but the possibility of testing it in space for a relatively small sum of money is attractive. This is especially true at a time when strapped budgets like NASA's are focused on ratcheting up conventional propulsion techniques to get us back to the Moon and on to Mars. Yes, let's keep pushing outward into nearby space with what we've got, but we need next-generation thinking, too, and the Finnish sail, the work of Pekka Janhunen and Arto Sandroos, points in that direction. Unlike magnetic sails that create an artificial magnetosphere around the spacecraft, the Finnish concept is to use long, thin conductive wires that are kept at a positive potential through the use of an onboard electron gun. The two researchers considered how the charged particles of the solar wind would interact with a single charged wire in a 2007 paper that we looked at in this Centauri Dreams article just over a...

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Hawking and the Long Result

Sometimes it's hard to believe that Stephen Hawking is only sixty-six. Not just because of his indomitable fight against Lou Gehrig's disease, which is a story in its own right, but because his position at the summit of modern physics has kept him in the public eye for an exceedingly long time. Now, in a speech commemorating the fiftieth anniversary of NASA, Hawking has taken aim at the question of why space matters. And it's not surprising that this Star Trek fan quoted his favorite show. "If the human race is to continue for another million years, we will have to boldly go where no one has gone before ... It will not solve any of our immediate problems on planet Earth, but it will give us a new perspective on them and... Hopefully, it will unite us to face a common challenge." But of course, that question of solving our immediate problems on Earth is what is often subject to debate. Although the space budget is usually overestimated (a recent conversation illustrated this, a friend...

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A ‘Hot Jupiter’ in Our Solar System?

Serendipity is a wondrous thing. Start writing about the early history of the Solar System, as I intended to do yesterday, and you wind up discussing 'hot Jupiters' around other stars. But there actually is a bridge between the two concepts, and it comes in the form of a question. If we find gas giants in scorchingly hot orbits around other stars, why was there no hot Jupiter in our own Solar System? Or was there? That question was what originally led me to the paper by Avi Mandell, Sean Raymond and Stein Sigurðsson that occupied yesterday's post. For in their analysis of how giant planets migrate through an early planetary system, wreaking havoc on newly forming worlds but also scattering them interestingly throughout nearby space, these researchers paused to examine the implications of these studies for our own system. Having demonstrated through their simulations that the migration of a gas giant through an inner system may be common, and that systems that experience it often form...

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Habitable Worlds and Hot Jupiters

What happens to potentially habitable planets when a gas giant swings through the neighborhood? It's a pertinent question when you consider the surprises that 'hot Jupiters' have given us. 22 percent of known extrasolar planets show an orbital radius of less than 0.1 AU, and 16 percent are located within 0.05 AU of their host star. That's a surprise given the assumption that these gas giant planets must form much further out in their systems, but it can be explained by inward migration of the giant planet, a process under much study that is generally thought to be caused by interactions with the protoplanetary disk. Such a migration would seem to spell trouble for planets already orbiting closer to the star, leading some to believe that systems with hot Jupiters are unlikely homes for living worlds. But recent simulations of the growth of such systems make it clear that a hot Jupiter isn't necessarily a deal-breaker for habitable worlds. Are we going to have to add such systems into...

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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).

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