I had intended to start the week with a look at Charlie Stross' ideas on the 'starship' metaphor, but I'll hold the Stross essay until tomorrow because I want to finish up Marcus Chown's piece in New Scientist. On Friday we talked about the idea of using Hawking radiation from a man-made black hole to propel a starship. That's outrageous idea number one, but Chown actually began the article with a look at Jia Liu's ideas on using dark matter to propel a ship, something along the lines of a Bussard ramjet without the hydrogen. The Uses of Speculation I enjoy looking at speculative concepts, even when they're so far out on the edge that they've attained a kind of intellectual redshift, but New Scientist's squib for the story surprised me: "We could reach the stars if we built a black hole starship or a dark matter rocket - we've got the physics to do it." Er, no, we don't have the physics to build a dark matter rocket. We don't know what dark matter is. The case for its existence seems...
A Universe Optimized for Starships?
When you consider that conventional chemical rockets extract a mere 10-8 of the energy locked up in their fuel, the attraction of antimatter becomes undeniable. Could we build an engine that extracts 100 percent of the energy created by matter-antimatter annihilation? Louis Crane (Kansas State University) is dubious, pointing to problems of storage and the difficulty of making enough antimatter to get the job done. Black Holes as a Propulsion Option Working with colleague Shawn Westmoreland, Crane has been exploring a different and far more speculative option for upping the energy extraction levels. What about using black holes for propulsion? Specifically, Crane and Westmoreland ask whether Hawking radiation from black holes can power a starship, calculating that a black hole of about a million tons would be just the right size, small enough to generate the needed Hawking radiation, while large enough to survive for the duration of a century-long star crossing. Adam Crowl has...
Circumstellar Disk Around a Massive Star
The image at the right shows HD200775, a close binary that contains one star ten times the mass of the Sun. The two stars illuminate the surrounding cavity of molecular gas, the closest of which forms the reflection nebula known as NGC7023. The binary is located some 1400 light years from Earth and is the subject of recent work by an international team that has produced the first well-resolved images of a circumstellar disk around a young, massive star. You can see the disk they found in the mid-infrared in the second image below. Image: HD200775 and its nebula. The bright star at the center is HD200775, which illuminates the surrounding nebula. The upper and lower part of HD200775 is the reflection nebula NGC7023. The hourglass-shaped nebula extending in the east-west direction (east is left) encircles a cavity formed by past outflow activity. Okamoto et al. zoomed in and imaged an area around HD200775. Credit: DSS/2MASS/Subaru Telescope. What we're after is a better understanding...
How Do Brown Dwarfs Form?
Now that we are looking forward to the WISE mission (Wide-Field Infrared Survey Explorer) and its investigations into nearby brown dwarfs, it's startling to realize that we detected the first of these objects as recently as 1995. Today they're all the rage, particularly among that small band of us obsessed with missions to nearby interstellar space. A cool, dim brown dwarf could be the closest star to our Sun, an obvious target for a future probe once long-haul propulsion options begin to mature. Brown dwarfs are too cool to trigger hydrogen fusion, so it takes infrared capabilities like those of WISE or the Spitzer Space Telescope to tell us much about these dim objects. A key question has been whether they form like planets or stars. Spitzer may have found the answer in the form of two 'proto brown dwarfs' that have been located in a cloud called Barnard 213, a region of the Taurus-Auriga complex where young objects abound. The finding is significant because we've never before...
A New Shape for the Heliosphere
One problem with journeys that are beyond today's technologies is that we forget, in our zeal to get a payload to the target, how little we know about the regions we'll pass through along the way. It's amazing how little we know, for example, about the heliosphere around the Solar System, yet any probe pushing into interstellar space will have to cross from the region of space under the Sun's influence into a zone where the interstellar medium flows around this 'bubble,' disturbing the solar wind and creating a secondary bubble, the heliosheath. We don't yet have a global view of what spacecraft will encounter in the heliosheath as the solar wind is heated and slowed by these interactions. Only recently have we gotten the Voyagers into these regions, and in any case these doughty vehicles can only produce single-point measurements. But we've got the IBEX (Interstellar Boundary Explorer) spacecraft making observations from near Earth, and now we learn that Cassini, our intrepid Saturn...
Bringing the Starshade to Reality
The goal of detecting a terrestrial class exoplanet has burned bright in the imagination ever since the discovery of the first planets orbiting main sequence stars. In a recent SEED Magazine story, Lee Billings (one of the most graceful science writers now working) harkens back to then NASA administrator Daniel Goldin's 1996 speech at the American Astronomical Society meeting in San Antonio, Texas. Goldin talked about seeing Earth-like exoplanets up close, speculating that in 25 years we might be able to obtain images with a resolution to see clouds, continents and oceans. I'm going to use a different Goldin quote than Lee did, from a later speech, but the idea is clear enough in either iteration. Here Goldin is speaking about the classrooms of the mid-21st Century and what they might look like: When you look on the walls, you see a dozen maps detailing the features of Earth-like planets orbiting neighboring stars. Schoolchildren can study the geography, oceans, and continents of...
“RuBisCo Stars”: Part II
by Joe Davis Yesterday we followed Joe Davis' adventures in Puerto Rico as he arranged for the transmission of a message to the stars near the 35th anniversary of the famous message to M13, sent from the same site in 1974. Today Davis concludes the story, with a look at how the 'RuBisCo' message was put together, and thoughts on the ins and outs of getting unusual projects approved in today's scientific climate. I had a sort of showdown with Arecibo's interim Director, Dr. Michael C. Nolan at the last minute and Danielle Hofmans' detailed notes have made it possible for me to recount that conversation here. Nolan's main problem was about politics. Arecibo once received a "Golden Fleece" award from Senator Proxmire for its involvement with the search for extraterrestrial intelligence, including its role in the Sagan-Drake transmission of 1974. That recollection has special resonance now since there are very serious ongoing concerns about future funding for the observatory. Nolan...
“RuBisCo Stars” and the Riddle of Life
by Joe Davis We've looked before at the work of MIT biology research affiliate Joe Davis, whose passion is the melding of science and art. Among his many ideas are the creation of an 'infogene,' engineering a sign of human intelligence into the genome of bacteria that could be flung into the heavens by the trillion, and a three-masted Gulf Coast tower that would discharge laser beams into the sky. In 1986, Davis used MIT's Millstone radar to beam a signal to Epsilon Eridani, Tau Ceti and two other stars. His most recent adventure takes him to the great telescope at Arecibo. It involves the 35th anniversary of the Drake/Sagan transmission to M13, a messaging strategy based on molecular biology, and the emergence of the coolest iPhone in the world. What follows is a narrative describing events that took place just over one week ago: I traveled from Boston to Puerto Rico on 03 November to deliver a lecture for the University of Puerto Rico's Biology Colloquium (Rio Piedras campus) in...
Notes & Queries 11/17/09
Focus on FOCAL I'm just back from a weekend in Texas, meeting with Hal Puthoff and Eric Davis at the Institute for Advanced Studies in Austin and spending a great deal of time with Claudio Maccone, who flew in from Italy and goes on from Texas to a presentation at the SETI Institute. Our subject was largely FOCAL, the ambitious mission Maccone has championed to develop a spacecraft that can be sent to the Sun's gravitational lens at 550 AU and beyond. Because gravity-focused radiation remains along the focal axis beyond 550 AU, such a spacecraft would continue making high-quality observations in various wavelengths long beyond this distance. We live in an era of tight budgets and, to put it bluntly, lack of vision. Although FOCAL requires only near-term advances in technology and would represent the most ambitious undertaking ever attempted in space, the problem will be to find the funding to make it happen. A second issue is to develop a critical mass of scholarship in support of...
Targeting Planetary Migration
When the stars are properly aligned, expect remarkable things. How useful, for example, to find that a planet we would like to know much more about -- HAT-P-7b, about 1000 light years from Earth -- is not only providing intriguing transit information right now, but is also in Kepler's field of view. We'd like to know whether there are massive outer planets in this system, or possibly a binary companion. These are questions that the Kepler observatory may be able to answer. Any transiting exoplanet is obviously of high interest, but HAT-P-7b stands out a bit more following the publication of two recent papers in separate journals. Both used the Subaru Telescope to examine the planet's unusual orbit, which appears to be retrograde or polar. This is useful stuff, because it's telling us something about how planetary systems form, offering useful evidence about planetary migration models. What we would expect is that planets that form in protoplanetary disks around young stars would have...
WISE: Brown Dwarf Hunter Extraordinaire
Friday is a travel day for me, so be aware that comment moderation will be slow and sporadic. I just have time to get in word about the upcoming launch of the WISE mission, slated for December 7. NASA is planning a media briefing next Tuesday (November 17) to discuss the mission, which is designed to scan the entire sky at infrared wavelengths, spotting perhaps hundreds of thousands of asteroids and studying a wide range of stars and galaxies. The technology is fascinating in and of itself. WISE will image the entire sky in the infrared, using detectors kept below 15 Kelvins (which is only 15 degrees C above absolute zero) by a solid hydrogen cryostat. The telescope will be oriented to look out at right angles to the Sun, always pointing away from the Earth, so that its observations sweep out a circle in the sky. After six months, the instrument will have observed the entire sky, producing nearly 1.5 million images and creating, ultimately, an atlas of the entire celestial sphere....
The Lithium Clue to Exoplanets
The exoplanet watch among our readers is clearly in full operation, to judge from the number of backchannel messages I received about the latest work from HARPS (High Accuracy Radial Velocity Planet Searcher). The remarkable ESO spectrograph attached to the La Silla 3.6-meter telescope now offers evidence that Sun-like stars that host planets will show a sparser lithium signature than stars without planets. Says Garik Israelian, lead author of the paper now appearing in Nature: "For almost ten years we have tried to find out what distinguishes stars with planetary systems from their barren cousins. We have now found that the amount of lithium in Sun-like stars depends on whether or not they have planets." All of this helps us understand our own star, whose low levels of lithium (140 times less than it should have had when formed) have long been apparent. The HARPS work draws on an analysis of some 500 stars, including seventy known to host planets. Ace planet hunter Michel Mayor...
LightSail: A Near-Term Space Sail
From the fusion-powered Project Icarus, designed to handle the interstellar long-haul, to the first tentative solar sail experiments in near-Earth space seems like quite a jump. But we needed to be reminded of the need for research on both ends of the spectrum, the things that are doable today and the concepts we want to shape for tomorrow. How heartening, then, to see the Planetary Society's new commitment to the solar sail in the form of a project called LightSail, which will include several missions designed to demonstrate the potential of photons for propulsion. Make no mistake about it, solar sail technology is a practical solution for leaving the fuel at home. We know the principle works. Photons carry no mass but they do carry momentum. Missions designed to operate close to the Sun already have to factor in the pressure exerted by the photon stream, and in a famous case, controllers used the solar panels aboard the Mariner 10 spacecraft (launched in 1973 to explore Mercury) to...
Project Icarus Symposium: Part Two
by Pat Galea Project Icarus will update the Project Daedalus starship designed by the British Interplanetary Society in the 1970s. As we saw yesterday, developments in technology allow new options in a number of areas, but also raise questions about the mission's scope and choice of targets. Pat Galea now concludes his discussion of the recent Project Icarus symposium in London, after which the terms of reference for the project, now frozen, are listed. Propulsion Options Richard Obousy tackled the part of the system that is the most obvious, the most important and probably the most difficult: the engine. As I've noted above, the Daedalus propulsion system uses pulsed nuclear fusion to accelerate the craft to about 12% of the speed of light. Even at such an immense speed, the mission time to Barnard's Star (5.9 light years from Sol) is about fifty years. Obousy took us through different methods of propulsion that have been proposed, such as chemical rockets, electric ion engines and...
Report on the Project Icarus Symposium
by Pat Galea The Tau Zero Foundation has been working with the British Interplanetary Society on Project Icarus, a starship study that updates the famous Project Daedalus work from the 1970s. Pat Galea, a software engineer with a lively interest in the physics of interstellar flight, attended the recent symposium that launched the project, and here provides us with a report that I will publish in two parts, concluding tomorrow. Just over thirty years ago, British Interplanetary Society (BIS) members carried out one of the most complete studies of an interstellar vehicle ever made. Even today, Project Daedalus retains its status as an outstandingly comprehensive reference design. Its final report sits on the shelf of many a starship enthusiast. In the intervening years, technology and science have advanced in many of the areas that are crucial to the Daedalus mission plan and design. The time has come to re-examine Daedalus in light of the progress that has been made, so Kelvin Long...
MiniSpaceWorld Design Contest Nears Finish
My friend Tibor Pacher reports that the MiniSpaceWorld Design Contest is getting quite interesting, with six submissions of high quality, all going in different directions. Tibor's goal is to build a scale model world that, like the famous Miniatur Wunderland in Hamburg, shows off space technology in tiny, exquisite detail. We're used to seeing this kind of thing particularly in the model railroad world, so why not extend the idea into space as a tool for educators? Now you can go to the site to see basic maps from the contestants. The contest award ceremony is to be held in Budapest on December 5 in the Congress Hall of the Research Centre for Social Studies, a Hungarian Academy of Sciences institute, and as Tibor notes, this is in the Budapest castle district, so there is much more to do in the area for those lucky enough to attend. Be aware that voting on the submissions is open until November 15, and have a look at the MSW site for more information.
The Gravitational Lens and Communications
If we can get the right kind of equipment to the Sun's gravitational focus, remarkable astronomical observations should follow. We've looked at the possibilities of using this tremendous natural lens to get close-up images of nearby exoplanets and other targets, but in a paper delivered at the International Astronautical Congress in Daejeon, South Korea in October, Claudio Maccone took the lensing mission a step further. For in addition to imaging, we can also use the lens for communications. The communications problem is thorny, and when I talked to JPL's James Lesh about it in terms of a Centauri probe, he told me that a laser-based design he had worked up would require a three-meter telescope slightly larger than Hubble to serve as the transmitting aperture. Laser communications in such a setup are workable, but getting a payload-starved probe to incorporate a system this large would only add to our propulsion frustrations. The gravitational lens, on the other hand, could serve up...
Cometary Clues to Solar System Origins
The Earth receives thousands of tons of interplanetary dust every year as it makes its way around the Sun. Can we trace any of this material to a particular source? Scientists from the Carnegie Institution think the answer is yes, at least in the case of comet Grigg-Skjellerup. The Carnegie team worked with interplanetary dust particles (IDPs) collected by a NASA aircraft in 2003, just after the Earth had passed through the comet's tail, focusing on the chemical, isotopic and micro-structural composition of the grains. Collecting Comet Dust A bit of background: NASA's Scott Messenger (JSC-Houston) predicted that Grigg-Skjellerup dust grains could be captured in the stratosphere at a specific time of the year (the comet reappears every five years). The dust collection flights that followed his prediction involved an ER-2 high-altitude aircraft flown out of Dryden Flight Research Center in 2003. Out of this work came the new mineral now called Brownleeite, a manganese silicide found in...
Dark Matter: Results and Further Planning
If you're going to snare dark matter, you'd better have incredibly accurate detectors. So the thinking goes at Case Western Reserve, where researchers are planning the most sensitive experiment yet to go after WIMPs (weakly interacting massive particles). WIMPs are almost impossible to detect because they don't give off radiation and pass through normal matter unimpeded. The CWRU group has received a three year $3.2 million National Science Foundation grant to design a new WIMP detector. The existence of dark matter is a theory that received support in 2006 when the collision of two distant galaxies was analyzed in ways that seemed to show the effects of dark matter on a cloud of galactic gas. Dark matter could provide the needed mass that keeps galaxies like the Milky Way from flying apart, but we still need a direct detection. The new experiment is a 20-ton liquid xenon detector called LZD. The Case Western group proposes LZD as an experiment for the Deep Underground Science and...
Is There a Flaw in General Relativity?
By Larry Klaes We have much to do as we scramble to explain the universe's continuing acceleration. Dark energy seems to be demanded by the data, but there are holdouts who argue for a reinterpretation of General Relativity. Tau Zero journalist Larry Klaes looks at one proponent of a revised GR who sees exceptions to the rule in a far earlier era. Albert Einstein's work created one of the biggest revolutions in the history of science and radically changed our perceptions of the Cosmos. One of his later breakthrough ideas is the Theory of General Relativity, or GR for short. Really massive objects such as the Sun literally warp space and time around them as they move through the heavens. Since Einstein first published his ideas on GR in 1915, scientists have been able to use the theory to understand the behaviors of even more massive celestial bodies and the very beginning of the Universe itself. Image: This key Einstein paper included the effect of gravitation on the shape of space...