Robert Forward used to talk about antimatter factories in space, installations that would draw their power from the Sun. He would point out that at a distance of 1 AU, our star delivers a gigawatt of energy for each square kilometer of collector. And being Robert Forward, he thought big: Build a collector array one hundred kilometers on a side to produce a power input of ten terawatts, enough to drive several antimatter factories at full power and produce a gram of antimatter each day. Forward saw the antimatter problem as a matter of scaling and cost (and he often talked about 'small problems of engineering'). As we've seen in the last few days, James Bickford (Draper Laboratory) is more than aware of both these issues, but unlike Forward, he's keen on mining naturally occurring sources of antimatter right here in the Solar System. Forward's huge factories may some day be built, but for now, let's talk about how to get our early antimatter missions into the realm of possibility by...
Finding Antimatter in the Solar System
James Bickford's antimatter work for NASA's Institute for Advanced Concepts, a Phase II study completed just as NIAC was announcing its closure, prompted a number of comments from readers when I opened discussion of it on Monday. And I can see why. We're used to thinking of antimatter production as an extraordinarily expensive process happening only in particle accelerators. And even when we commit the resources to make it, we get only the tiniest amounts, and at costs so high that they make propulsion concepts for antimatter seem chimerical. But Bickford wants us to consider a naturally occurring source of antimatter, one that might offer the potential of being collected in space for a variety of missions. Key to the idea is the fact that high-energy galactic cosmic rays (GCR) continually bombard the upper atmosphere of the planets in our Solar System, as well as interacting with material in the interstellar medium. The result is 'pair production,' the creation of an elementary...
New Discovery Around 55 Cancri
I want to get back to James Bickford's antimatter study tomorrow, at which time I'll set up the full report for download here. This work has already elicited plenty of response, both in comments and backchannel, so tomorrow we'll talk about the mechanisms that create antimatter in our Solar System naturally (as opposed to what we do with particle accelerators), and also ponder how realistic missions to harvest such antimatter could be built around technologies currently in the pipeline. Right now, though, the news conference on 55 Cancri is ongoing, the news from this system more and more interesting now that another planet, the fifth, has been discovered. This is the first system found with this many planets, although the assumption is there will be many, many others. But 55 Cancri, some 41 light years away in the constellation Cancer, bears some resemblances to our own Solar System. The farthest planet from the star is a gas giant about four times Jupiter's mass orbiting every 14...
Antimatter For Deep Space Propulsion
Great ideas fan out in unexpected directions, which is why James Bickford now looks at antimatter in a new light. Bickford (Draper Laboratory, Cambridge MA) realized that an adaptation of Robert Bussard's interstellar ramscoop might have its uses in collecting antimatter. The concept grew out of the realization that antimatter sources were available not only near the Earth but farther out in the Solar System, where antiparticles could be collected and used to boost spacecraft initially to speeds of 100 kilometers per second. That's sufficient for interstellar precursor missions outside the heliosphere, including the possibility of getting a payload to the Sun's gravitational focus, where a new kind of space-based astronomy waits to be exploited. Refine the process enough and you start talking about even greater speeds through more efficient antimatter collection, one great benefit being that instead of producing the stuff in Earth-bound particle accelerators, you're actually mining...
‘Missing Mass’ Theory Revised
Has ten percent of the mass of the universe disappeared? Not really, but it's true to say that our assessment of that mass has to be reconsidered, given recent findings on the nature of x-rays emitted from the vast spaces at the heart of galaxy clusters. How we interpret the x-ray data has a great bearing on how we calculate the mass of gases in the galactic clusters, and the mass of the clusters themselves. The story begins in 2002, when a University of Alabama in Huntsville team studying warm, x-ray emitting gas in galactic clusters reported that it had found large amounts of comparatively low-energy x-rays in addition to higher energy 'hard' x-rays. The so-called 'soft' x-ray emitting atoms were assumed to exist at a density of one atom per cubic meter, but their cumulative mass was thought to amount to as much as ten percent of that needed to hold galactic clusters together. But a closer look at data provided by the Chandra X-Ray Observatory, among other instruments, found no...
White Dwarf Merger (and the Implications)
The recent news about an unusual supernova in Hercules some 300 million light years away has a wider significance than might first appear. Supernovae are important for more than their role in seeding the cosmos with heavy metals forged in their stellar furnaces. They're also widely used cosmological markers. Type Ia supernovae, thought to be well understood, typically occur in a band of brightness that makes them 'standard candles,' useful in calculating cosmic distances. It was work on Type Ia supernovae, in fact, that led to the discovery of the universe's accelerating expansion. And what the latest find implies is that, contrary to earlier thinking, this kind of supernova may be more varied than previously thought. The new find -- supernova 2006gz -- appears to result from the collision of two white dwarfs that had been in orbit around each other. The evidence: a strong spectral signature of unburned carbon and clear signs of compressed layers of silicon. Both spectral signatures...
A Tunguska Reminder
Universe Today offers up the latest edition of the Carnival of Space while announcing it will become the new venue for this gathering of Web links on space-related subjects. Among the posts garnered this time, it's Universe Today's own take on the Tunguska event that should most resonate with Centauri Dreams readers. Tadeusz J. Jopek (Astronomical Observatory UAM in Poland) and team have run simulations of the 1908 explosion to estimate the velocity and impact angle of the Tunguska meteorite. "We believe that TCB originated as the result of a breakup of a single body: a comet or an asteroid. In our study we concluded that it is more probable that it was an asteroid. We cannot point to which one; instead we have found several candidates for the Tunguska parent, and the asteroid 2000 WK63 is an example of it," Dr. Tadeusz said. Interesting! The relevant question, of course, is just how often we can expect such impacts to occur. Tunguska was, happily, a largely unsettled place at the...
A Volcanic Cause of Dinosaur Extinctions?
The Chicxulub crater in the Yucatan gets plenty of press whenever the subject of asteroid deflection comes up, it being the supposed evidence of the 'dinosaur killer' that changed life on Earth forever some 65 million years ago. But other factors may have played a role in the dinosaur extinctions, among them geological events in India, now studied in the form of the so-called 'Deccan Traps,' immense lava beds that show the ancient flow of lava from the same era over an area of hundreds of miles. If current work is correct, the main phase of these eruptions released ten times the amount of climate-altering gases into the atmosphere as Chicxulub itself, which would have occurred more or less at the same point in geological history. And if iridium deposits were an early clue to what happened in the Yucatan, marine sediments and microscopic marine fossils point to the power of the volcanoes. The life forms that created these fossils are known to have evolved just after the extinction...