When engineer Carl Wiley brought solar sails to a wide audience in 1951, he envisioned a particular kind of sail. Wiley, who wrote under the byline Russell Saunders, published "Clipper Ships of Space" in the May issue of Astounding Science Fiction that year, seven years before the first technical paper on sails, Richard Garwin's "Solar Sailing: A Practical Method of Propulsion within the Solar System," appeared in the journal Jet Propulsion. As you can see in the illustration, which ran with the original essay in Astounding, Wiley envisioned the sail as taking a parachute shape, with the payload attached to the sail circumference. Varieties of Sail Design But there are many ways of doing sails. Square or rectangular sail designs (think of those images of IKAROS shot by its detached cameras) have been the focus of recent work, with the result that many alternatives have not reached the same level of technological readiness. But along with parachute sails, spinning disk sails,...
The Perseid Project: Crowd-sourcing the Meteor Stream
An individual meteorite can tell us much about the composition of ancient Solar System material, but today I want to mention a project that is taking the aggregate view. Chris Crawford has set up the Perseid Laptop Meteor Observation Project as a way to use 'crowd-sourcing' to build up a three-dimensional map of the Perseid meteor stream. Here's what Chris said about it in a recent email: This will be one of the better years for Perseids; the Moon, which often interferes with the Perseids, will not be a problem this year. So I'm putting together something that's never been done before: a spatial analysis of the Perseid meteor stream. We've had plenty of temporal analyses, but nobody has ever been able to get data over a wide area -- because observations have always been localized to single observers. But what if we had hundreds or thousands of people all over North America and Europe observing Perseids and somebody collected and collated all their observations? This is crowd-sourcing...
Adaptive Optics and the Giant Magellan Telescope
Anything we can do to advance the cause of adaptive optics is all to the good. It's obvious that a space-based observatory is preferable if we want to get the sharpest look at a distant object, but launch costs are still high and the kind of intricate interferometry missions that will one day let us take a close look at a distant exoplanet are still on the drawing boards. In the interim, learning how to get around the distortion caused by a planetary atmosphere allows us to do things with Earth-based telescopes that earlier astronomers wouldn't have thought possible. The kind of laser adaptive optics in use at the University of Arizona represents a useful advance in the state of the art. Make a telescope mirror pliable enough to respond to hundreds of actuators positioned on its back side and you can create a series of tiny adjustments as you look at the sky. The adjustments are necessary because atmospheric turbulence blurs the image, the result of rising heat disturbing the air a...
Project Argus: Finding a ‘Benford Beacon’
It's heartening to see James and Gregory Benford's work on extraterrestrial beacons receiving broader coverage. We've looked at the relevant papers in these pages [run a search on 'Benford' in our database and you'll pull up articles by and about them], but news features like this one in TIME Magazine are pushing the Benford brothers' work out to a much larger audience. That's an important step, because right now the view of SETI most likely held by the average person relates to movies like Contact, in which huge dishes pointed at particular stars seem to be the way to proceed. The Benfords want to re-write that scenario in a big way. We'll have to leave as debatable the question about how far away our own television transmissions can be received. James Benford commented here not long ago that a civilization of approximately our technological level would not be able to receive broadcast signals as weak as those we've sent out carrying the likes of Milton Berle and I Love Lucy....
Pegging the Movements of a Potential Impactor
NASA's workshop on identifying objectives for missions to near-Earth objects will be held next week, August 10-11 at the Renaissance Mayflower Hotel in Washington, DC. We can hope that this gathering of NASA leaders, academics, and space experts from across the international community will help keep the public's attention on the need for such missions. Part of the reason for having the workshop is to communicate NASA's preliminary plans for a human mission to an NEO, a useful step as we build expertise about these objects and ponder strategies to handle any future impact scenarios. You can follow the video stream at the appropriate time here. Meanwhile, the continuing survey of near-Earth objects has produced another one, asteroid 101955 1999 RQ36, with a slight impact possibility in 2182. We can call this object a Potentially Hazardous Asteroid (PHA) based on the results from the two mathematical models -- Monte Carlo Method and line of variations sampling -- being used to study it....
Solar Sails: Charting an Operational Future
Japan's IKAROS sail has thus far conducted a triumphant mission, demonstrating the principles of sail deployment, solar photon propulsion and attitude control in a functioning space sail. While the solar sail community has never received the press attention I believe this innovative propulsion technology deserves, it's heartening to realize that a long and sustained effort, even one operating under the radar, so to speak, can produce such striking results. The 2nd International Symposium on Solar Sailing (ISSS 2010) has just wrapped up in Brooklyn, but if you go back to the first of these conferences, conducted in June of 2007 in Ammersee, Germany, you'll find that the program was laced with representatives of ESA, NASA and JAXA (presentations from that meeting are available online), attacking the issue of getting a solar sail operational from every angle even as the budgets of the representative agencies were being cut back. The needed theoretical work proceeds absent the necessary...
Oxygen & Wildfires: Clues to Early Life
How big can an insect get? One night a few years back, I opened the door onto our patio to let the dogs out and an enormous flying, buzzing thing came through the door. When I say 'enormous,' I simply mean it was big enough to startle both dogs enough that they ran upstairs, causing me to grab for a flyswatter as it flitted and hummed around the room. I lost sight of it and suddenly all was silent. Our cat had sprung, and the bug was quickly dispatched. We dubbed it 'Mothra' and added it to our dog lore. After all, where were our Border Collie and Sheltie when we needed them? Peering down at us from the upstairs landing, while the cat did the dirty work. 'Mothra' was probably no more than an inch long -- he was noisier than he was big. But there was a time when 'enormous' really meant something. Meganeura is a genus of insects dating to the Carboniferous period when creatures related to our own familiar dragonfly boasted wingspans of two feet or more. Meganeura monyi is considered...
Imaging Giants and Dwarfs
Was it really three years ago that New Horizons moved past Jupiter, returning images of its stunning systems of storms and cloud? The mission continues to go well, and the photo below, taken by the spacecraft's Long Range Reconnaissance Imager (LORRI) paints an unusual portrait of Jupiter and two of its largest moons from a distance of more than 16 AU, looking back toward the inner system. Note how faint the moons are, the consequence of the fast shutter speed used, with an exposure time of 0.009 seconds. I like what mission principal investigator Alan Stern says: "This haunting image of Jupiter - far in the distance back in the Sun's warmer clines from whence New Horizons came - reminds us of Voyager's family postcard of the planets taken from beyond Neptune's orbit about 20 years ago. Perhaps after we flyby Pluto in 2015, we'll try something similar from our perch aboard New Horizons." Image: The New Horizons team looked back at Jupiter during Annual Checkout (ACO) 4 to test the...
Can the Pioneer Anomaly Be Explained by Inertia Modification?
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...