by Richard Obousy Physicist Richard Obousy here takes a look at an intriguing new paper by Mike McCulloch, a researcher at Plymouth University. In addition to his work in theoretical physics and warp drive possibilities, Obousy is current project leader and primary propulsion design lead for Project Icarus, a joint venture between the British Interplanetary Society and the Tau Zero Foundation to re-think the original Project Daedalus starship design. In the review below, Obousy places McCulloch's work on the Pioneer anomaly in the context of current thinking on dark matter, dark energy and the nature of mass. Does the Higgs field explain inertial mass, or are there alternatives? Read on. Few areas of research have garnered as much attention from both the public and scientific communities as those of dark energy and dark matter - and for good reason. Both terms stem from observations of the physical universe that, simply put, don't belong within the well-understood framework of known...
Statites: Hovering Over the Pole
Robert Forward's Indistinguishable from Magic is a genial and absorbing read, a collection of essays and fiction illustrating some of the scientist's most memorable ideas. And while gigantic lightsails driven by laser beam to other stars always come to mind when Forward's name is mentioned, it's fascinating to page through his thoughts on antimatter, black holes and time machines. Long a Forward admirer, I was pleased to see that another of the concepts discussed in this book recently made an appearance at this month's solar sail conference in Brooklyn. 'Statites' are a Forward construct, a word he coined to describe a spacecraft that uses a solar sail to hover over a region rather than orbiting the Earth. Let Forward describe what he calls a 'technique for hanging things in the sky': ...I have the patent on it -- U.S. Patent 5,183,225 "Statite: Spacecraft That Utilizes Light Pressure and Method of Use"... The unique concept described in the patent is to attach a television broadcast...
New Planets Highlight Orbital Resonance
We're learning a lot more about how planets interact with each other gravitationally. 'Resonance' is the operative term here. When planets are locked in a 2:1 orbital resonance, the outer planet orbits the host star once for every two orbits of the inner planet. A 3:2 resonance occurs when the outer planet orbits the star twice for every three orbits of the inner planet. Resonance (technically 'mean motion resonance') prevents close encounters between planets and provides long-term orbital stability. And if the 2:1 resonance is the most common pattern, it's also true that things can change when planets migrate to different parts of their system. John Johnson (Caltech) describes the result of fast inner migration: "Planets tend to get stuck in the 2:1. It's like a really big pothole. But if a planet is moving very fast it can pass over a 2:1. As it moves in closer, the next step is a 5:3, then a 3:2, and then a 4:3." Johnson's work on resonance has born fruit in a new paper in which...
The Enduring Legacy of the Voyagers
by Larry Klaes The Faces from Earth project, run so energetically by Tibor Pacher, is planning its next 'E.T. Are You Out There?' campaign, following a successful campaign in May that introduced interstellar concepts to school children in five countries. In this piece, journalist Larry Klaes looks back at the Voyager spacecraft, which will be the subject of the new Faces from Earth campaign. The Voyagers electrified all of us with the discovery of volcanoes on Io and a possible ocean beneath Europa's ice, and the ensuing stream of images from planets and moons never before seen up close. They also carried golden discs bearing information about their builders. As of this morning (EST), Voyager 1 is 15 hours, 44 minutes, 56 seconds in light-travel time from home, at the edge of the Solar System but, as Larry makes clear, hardly forgotten. In the first decade of the Space Age, humanity succeeded in sending a handful of robotic space probes to Earth's two nearest planetary neighbors,...
Time Travel: Ways Around Paradox
Time travel holds such perennial fascination that even though its relationship with interstellar issues is slim, I can't resist reporting on new ideas about it. John Cramer's time experiments seem stuck in limbo, but now we have new work from Seth Lloyd (MIT) and colleagues about one way out of the paradoxes time travel seemingly creates. The 'grandfather paradox,' returning to the past to kill your own grandfather and thus causing your future self not to exist, seems inevitable if we grant the existence of what are called 'closed timelike curves' (CTCs), the paths through spacetime that would let a time traveler interact with his or her self in the past. Ways Around Paradox Lloyd's team gets past that problem by describing a particular version of closed timelike curves formed with what is called 'post-selection.' The idea is to describe these CTCs in terms of quantum mechanics, starting with the assumption that time travel is a communications channel from the future to the past. Is...
Solar Sailing’s ‘Gossamer Road’
With more attention now being focused on possible missions to an asteroid, we should keep in mind that DLR, the German Aerospace Center, has been looking into an asteroid mission via solar sail for some time now. One 2006 paper from DLR's Institute of Space Simulation pondered a 70-meter sail for use in a projected mission to the Near-Earth Object 1996FG3 within ten years of launch. It's an interesting notion, one that would involve the sail hovering over the NEA hemisphere opposite to the Sun, deploying a lander and return capsule. DLR has been into serious sail studies for some time now, as the photo below attests. It's a 1999 shot of the ground deployment of a square solar sail 20 meters to the side. As you can see, this is a square sail made up of four triangular sail segments, an exercise that could readily lead to a sail deployment in space if the European Space Agency opts for funding such a mission. Just what ESA has in mind for such technology was the subject of a...
Sasselov: Planets ‘Like Earth’ in Kepler Data
Dimitar Sasselov, a co-investigator on the Kepler mission, said in a TED Talk just posted that Kepler had uncovered numerous terrestrial planet candidates in its early data. Have a look at the video below (around the 8-minute mark). "Small planets dominate the picture," says Sasselov, showing a chart of planet candidates. A great deal of work has to go into confirming these results, but Sasselov goes on to say "The statistical result is loud and clear, and the statistical result is that planets like our own Earth are out there. Our Milky Way galaxy is rich in these kinds of planets." How many will be confirmed, and how many shown to be habitable? Much work ahead.
The Solar Sail in Context
The final day of the Second International Symposium on Solar Sailing (ISSS 2010) kicks off this morning with Roman Kezerashvili (City University of New York) discussing solar sail missions as a way of testing fundamental physics. Last year in Aosta I listened with fascination as Kezerashvili discussed close solar passes ('Sundiver' missions) that could approach as close as 0.05 to 0.1 AU to the Sun, depending on the development of materials technology. The remarkable feature of his talk, though, was the consideration of General Relativity's effects in such close proximity to the Sun, which could create huge navigation issues. The 'Sundiver' as an Exercise in Physics Fail to account precisely for spacetime curvature and frame dragging in this environment and such a mission could find itself with a million-kilometer deflection enroute to its target. Even more exotically, time slows in close proximity to the Sun due to relativistic effects, so that the observer on Earth measures about...
A New View of Ontario Lacus
Before I move into today's story on Titan, I want to mention that those of us who weren't able to attend the ongoing Second International Symposium on Solar Sailing (ISSS 2010) can take heart in the fact that selected papers from the proceedings have been quickly published online. Conferences vary tremendously in the resources they make available during and after the event, but the ISSS organizers are obviously intent on wide distribution of these interesting talks. Let's hope those papers not yet included will find their way online in coming days. TZF's Pat Galea has posted a number of photos from day one of the event on Flickr, including this shot of JAXA's Osamu Mori delivering an early talk on the IKAROS mission. Project leader for IKAROS, this man is a solar sail pioneer. For those of you who've asked, the focus of ISSS 2010 is indeed near-term, although several longer-range papers will be presented. With our first operational solar sail only recently launched, this is a time to...
Musings on Sails and Stars
Solar Sails in Brooklyn I should probably clean out my office, and would, if I could find the time, but things keep happening in the deep space community and I keep writing about them. I had the program for ISSS 2010 (the Second International Symposium on Solar Sailing) right beside me when I started to write yesterday's entry, and by the time I got to the part on the conference, the program had disappeared into the wilderness of printouts, notebooks and letters. Thus I missed the fact that Colin McInnes would be in attendance at the sessions, a major addition to the already stellar lineup. McInnes could be said to have written 'the' book on solar sailing, a densely packed tome that lays out the principles and speculates on future missions. Meanwhile, it's heartening to see how international the solar sail effort has been from the outset, even if all the space agencies have continued to wrestle with their own funding demons. Much good work has gone on at Germany's DLR, for example,...
Notes & Queries 7/19/10
WISE Completes First Full Survey The WISE mission completed its first survey of the entire sky on July 17, generating more than a million images, of which one of the most beautiful is surely the image of the Pleiades cluster below. We're looking in the infrared at a mosaic of several hundred image frames with the combined light of WISE's four detectors working in a range of wavelengths. The cluster of stars in seen in a dense latticework of dust in an area covering seven square degrees, equivalent to about 35 full moons. Image: In this infrared view of the Pleiades from WISE, the cluster is seen surrounded by an immense cloud of dust. When this cloud was first observed, it was thought to be leftover material from the formation of the cluster. However, studies have found the cluster to be about 100 million years old -- any dust left over from its formation would have long dissipated by this time, from radiation and winds from the most massive stars. The cluster is therefore probably...
HD 209458b: A Comet-like Tail
The exoplanet HD 209458b is the subject of such intense scrutiny that the discovery of a comet-like 'tail' is almost anti-climactic. After all, this transiting 'hot Jupiter' has given us plentiful information about its atmosphere (including the presence of a massive storm), and its tight orbit around its primary, orbiting that star in 3.5 days, would imply an atmosphere in continual turmoil. Now we learn that some of the atmosphere is indeed escaping into space, with the result that stellar winds evidently push the cast-off material into a long stream behind the planet. Jeffrey Linsky (University of Colorado in Boulder) explains the observations: "Since 2003 scientists have theorized the lost mass is being pushed back into a tail, and they have even calculated what it looks like. We think we have the best observational evidence to support that theory. We have measured gas coming off the planet at specific speeds, some coming toward Earth. The most likely interpretation is that we...
Jupiter Looms in Mission Plans
We learned in May that Jupiter's South Equatorial Belt (SEB) had disappeared, an event that still has skywatchers puzzled, though it's not without precedent. In fact, the SEB fades out every now and then, with recent fadings in 1989, 1993 and 2010, and we can expect an outburst of storms and vortices when the enigmatic belt returns, probably within the next two years, based on historical precedent. All of which puts the spotlight on Juno, a Jupiter mission intended for launch in August of 2011. Juno is all about the giant planet's core, its magnetic field, its auroras and the amount of water and ammonia in its atmosphere. Juno's Jovian Science Maybe Juno will tell us whether the disappearance of the South Equatorial Belt is the result of ammonia cirrus forming on top and hiding the belt from view. But there is much more to learn. Hydrogen gas deep in Jupiter's atmosphere is pressed into metallic hydrogen, a fluid that acts like an electrically conducting metal and is thought to be...
‘Nemesis’ and Orbital Change
The idea of 'Nemesis,' a hypothetical dark companion to the Sun, won't quite go away, and it's possible that the WISE mission may help us either identify such an object or else demonstrate that it's not there. The idea is simple enough: Sol's companion would perturb the Oort Cloud in its orbit, causing comets to enter the inner Solar System, thus increasing the likelihood of an impact with the Earth. Throw in an apparent periodicity in extinction events first described back in 1984 and you have an intriguing case. But Adrian Melott (University of Kansas) and Richard Bambach (Smithsonian Institution) have reconsidered Nemesis in terms of extinction events in a new paper, one that looks at the timing of these incidents in light of the movements of Nemesis over time. They extend the original 26 million year extinction periodicity slightly, to 27 million years, and are careful to note that there is no consensus on the matter among paleontologists. But the real question they tackle is...
SETI and Detectability
by James Benford We recently looked at a paper by Duncan Forgan and Robert Nichol on the question of detecting extraneous emissions from an extraterrestrial civilization using technology like the Square Kilometer Array. James Benford (Microwave Sciences) has some thoughts on the issue growing out of his own work with brother Gregory on interstellar beacons and SETI reception in general. No one has put the question of interstellar beacons to tighter scrutiny than the Benfords, with particular regard to bringing the SETI discussion, as Jim puts it, "onto a quantitative basis, as opposed to rampant speculation, as is typical of the playing-tennis-without-a-net approach taken previously." The Benfords' work on interstellar beacons appears this month in Astrobiology. I give full citations at the end of this post. The Forgan & Nichol paper on detection of leakage radiation does neglect our continuing use of microwave beams not only for radar, but also for likely future beaming of power for...
ESA’s Rosetta in Flawless Encounter
Centauri Dreams readers should know the name Stuart Atkinson, whose excellent Cumbrian Sky site I've linked to before. I don't have many occasions to reproduce poetry in these pages (although I did quote some lines from Coleridge's 'Kubla Khan' in honor of Huygens' landing), but when I saw what Stuart had sent in to ESA's Rosetta team, I knew I had to highlight it here. Rosetta's encounter with the asteroid 21 Lutetia should bring out a bit of the poet in all of us, but Stuart nails what I felt: For all these years you were merely A smear of light through our telescopes On the clearest, coldest night; a hint Of a glint, just a few pixels wide On even your most perfectly-framed portraits. But now, now we see you! Swimming out of the dark - a great Stone shark, your star-tanned skin pitted And pocked, scarred after aeons of drifting Silently through the endless ocean of space. Here on Earth our faces lit up as we saw You clearly for the first time; eyes wide With wonder we traced the...
WASP-3c: Implications for Finding Earthlike Planets
Learning about planets through inference is a necessary procedure, given the state of our technology. We do have a few direct images of exoplanets now, but when relying on radial velocity data or transits, we're looking at the effects planets cause upon our measurements of their stars. With CoRoT and Kepler now yielding high-quality transit data, it's encouraging to see how we can go to work on this information to learn even more about the systems they study. Thus the announcement of WASP-3c, a second planet found around a star in the constellation Lyra, whose existence was pegged by its effect on the previously known planet. WASP-3b was discovered by the Wide Angle Search for Planets project (SuperWASP), a British extrasolar planet detection program that uses robotic observatories that monitor stars for transit events. Eight wide-angle cameras monitor millions of stars, with 26 exoplanets now discovered. The new work, led by Gracjan Maciejewski (Jena University, Germany) went to...
SETI: Stiff Odds Against Eavesdropping
Take a look at the frequency range of our SETI searches and you'll see that we are probing into new territory. Project Phoenix, which ran from 1995 to 2004, used radio telescopes at Arecibo, Parkes (NSW, Australia) and Green Bank (WV, USA), working in a frequency range of 1.2 to 3 GHz. The BETA project used a 26-meter radio telescope to examine the so-called 'waterhole' frequencies between 1400 and 1720 MHz, which seemed a likely place to look for an extraterrestrial beacon because this range covers an unusually quiet band of the electromagnetic spectrum between the hydrogen spectral line and the strongest hydroxyl line. With the Allen Telescope Array coming online, we can look forward to a search of 250,000 stars in the 'waterhole' region, but new facilities like LOFAR (Low-Frequency Array) are pushing into the megahertz area in pursuit not only of SETI but also astrophysical studies of the early universe. LOFAR makes me think back to my shortwave radio days, tuning around these...
Lutetia Encounter Approaches
Asteroids are much in the news these days, with Japanese and European missions returning outstanding photos and information about them. While we await testing on what may be fragments of the asteroid Itokawa from the Hayabusa team, we now prepare for another asteroid flyby on the part of the European Space Agency's Rosetta spacecraft, which carries DLR's Philae lander, a craft destined for eventual touchdown on the comet 67P/Churyumov-Gerasimenko. But that's not until 2014, when the most detailed study of a comet ever attempted reaches its destination. Along the way, Rosetta has delivered interesting asteroid results, including a 2008 flyby of the 'diamond in the sky' asteroid called Steins. We can now look forward to a flyby of the main belt asteroid 21 Lutetia, which will occur on July 10. Three instruments on the lander -- a magnetometer and plasma monitor (ROMAP), and two gas analyzers -- will be switched on during the flyby. More in this DLR news release, which notes that...
TrES-2b: Pushing Exomoon Limits
The planet known as TrES-2b is an interesting and useful place. Just over Jupiter mass, it orbits a solar mass star some 717 light years from Earth, a 'hot Jupiter' in a tight 2.47-day orbit. It's also a transiting planet, discovered by the Trans-Atlantic Exoplanet Survey, which uses small, automated equipment and off-the-shelf technology to get the job done, feeding planet candidates to larger installations like the Keck Observatory and Palomar Observatory. But TrES-2b has a new and important distinction: It's in the field of view of the space-based Kepler telescope. Now we're really in business. Exomoon-hunter David Kipping (University of London) said in a recent email that when this planet is viewed in 'short-cadence mode' with Kepler, it's like seeing transits in High Definition. And indeed, that seems to be the case, as you can see in the diagram below. Kepler offers two measurement cadences: 1 minute cadence for up to 512 targets and a 30 minute cadence for up to 170,000 stars....