The staggering difficulty posed by interstellar flight pushes us to imagine alternatives to today's technologies. Using conventional rocketry we're forced to amass so much propellant that the craft we want to send seem impossible to build, even if we could afford the vast fuel bill. A jacked up rocket engine is, of course, nothing but an old technology pushed to its extreme imaginative limits. And you could sense the constraints in that vision at the recent Joint Propulsion Conference in Hartford (CT), discussed not only in these pages but also here by Ray Villard. I mention Villard's comments because while I focused on Robert Frisbee's antimatter rocket concepts in my Centauri Dreams post, Ray tackles the much broader question of how we place technologies within the context of scientific progress. The news director for the Hubble Space Telescope, Villard is well versed in the rewards and challenges of spaceflight, but he's nonplussed with some of the reaction to the Hartford...
Notes & Queries 22 September 2008
Hugh Everett's 'many worlds' interpretation of quantum mechanics spawned not just the idea of a multiverse, but apparently quite a few interpretations on what a multiverse implies. If you're intrigued by the notion that our cosmos is one of what may be an infinite number of universes, you'll want to read Dan Falk's report in Sky & Telescope on the recent multiverse conference held at the Perimeter Institute for Theoretical Physics (Waterloo, ONT). Particularly interesting is the growth of multiverse thinking as string theory has come to the fore, with all the controversy that implies. And then there's the notion of 'eternal inflation,' which conceives of endless big bangs, each creating a separate cosmos. Laura Mersini-Houghton (University of North Carolina) is concerned about how multiverses spawned by quantum theory, string theory and inflation can be reconciled, as Falk notes: ...it's not at all clear how these different kinds of multiverses - grounded in quite different physical...
Exoplanets on the Fringe
Most Centauri Dreams readers will be familiar with the concept of interferometry by now. The idea is to combine light from multiple telescopes, allowing the combined array to act like a single telescope with a diameter equivalent to the distance between the telescopes. Thus we have the European Southern Observatory's VLTI (Very Large Telescope Interferometer), which uses two telescope elements some 200 meters apart. The VLTI has now put a new instrument called PRIMA into operation, with useful exoplanetary implications. PRIMA (Phase Referenced Imaging and Microarcsecond Astrometry) is designed to pick out the tiny motions a star makes as it is influenced by unseen planetary companions. We've long studied such wobbles in stars through radial velocity methods -- these analyze the light from the star, determining through Doppler shifts in the star's spectrum how a companion object may be influencing it. But PRIMA will find the wobbles through actual imaging, using incredibly precise...
Dark Matter’s Galactic Implications
Segue 1 is one of the tiny satellite galaxies orbiting the Milky Way whose dark matter component has caused great astronomical interest. As we saw in this post a couple of weeks ago, these ultra-faint objects have been turning up in Sloan Digital Sky Survey data, surprising astronomers by their mass, which indicates they're dominated by dark matter. Consider them top-heavy with the stuff: Segue 1 turns out to be a billion times fainter than the Milky Way, yet a study by members of the same team shows that it is a thousand times more massive than would be expected by its visible stars. The new regime of faint galaxies offers intriguing observational clues to galaxy formation while putting dark matter's properties on display. Thus Marla Geha (Yale University): "These dwarf galaxies tell us a great deal about galaxy formation. For example, different theories about how galaxies form predict different numbers of dwarf galaxies versus large galaxies. So just comparing numbers is...
On Stellar Migrations and Habitability
The idea of a galactic habitable zone (GHZ) has a certain inevitability. After all, we talk about habitable zones around stars, so why not galaxies? A stellar habitable zone is usually considered to refer to those areas around the star where liquid water can exist on a planetary surface. Those who believe that confining habitable zones to regions like these carries an implicit bias -- limiting them to life much like our own -- miss the point. The habitable zone concept simply tells us where it makes the most sense to search for the kind of life we can most readily recognize, and as such, it hardly rules out other, more exotic forms of life. But while liquid water takes precedence in a stellar habitable zone, a galactic HZ is still being defined. Charles Lineweaver and team have examined it, among other things, in terms of stellar metallicity (the elements heavier than hydrogen and helium found in the body of a star), concluding that there is a ring several kiloparsecs wide...
Direct Imaging and Its Exoplanetary Uses
As I taper back on my post-surgical medications (see yesterday's post), a coherent universe is gradually coalescing around me once again. Still, I think I'll take today relatively easy, looking at just one of the two stories I've been pondering during my brief convalescence. The first is intriguing not so much because of what it appears to be -- a planet around another star, as imaged by the Gemini North Telescope on Mauna Kea -- but rather because of where that planet seems to have formed. Have a look. The image at right shows the torturously named 1RXS J160929.1-210524, a star some 500 light years from Earth, along with the apparent companion of that star. The team behind this work has been surveying a group of stars in the so-called Upper Scorpius association, a group of relatively young stars that formed some five million years ago. Gemini is equipped with adaptive optics capabilities that make finding different types of companions around such stars feasible. This one seems to be...
A Brief Delay
Several interesting items in the news today but I won't be able to get to them, try as I might. I'm just coming off surgery yesterday (minor), and although I'm otherwise fine, the pain medication I'm taking makes me so groggy that I hesitate to post. So bear with me until tomorrow, when I should have a new item up some time in the afternoon.
Evidence for Planets in Protoplanetary Disks
Using a near-infrared spectrograph attached to ESO's Very Large Telescope, astronomers have been able to examine the inner protoplanetary disks around three interesting stars, with results showing the sheer diversity of the apparently emerging systems. Only a few million years old, all three stars could be considered analogs of our own Sun, going through processes like those that produced the Solar System some 4.6 billion years ago. The disks under study show regions where the dust has been cleared out, the possible signature of planetary influence. The new work, which offers higher resolution than was earlier available, demonstrates that the previously known gaps in the dust still contain molecular gas, an indication that the dust has begun to form planetary embryos or that a planet has already formed and is clearing the disk gas as it orbits. The likely planets include a massive gas giant orbiting the star SR 21 at a distance of something less than 3.5 AU, and a possible planet...
Tracing Our Interstellar Relatives
The idea that life on Earth might have originated elsewhere, on Mars, for example, has gained currency in recent times as we've learned more about the transfer of materials between planets. Mars cooled before the Earth and may well have become habitable at a time when our planet was not. There seems nothing particularly outrageous in the idea that dormant bacteria inside chunks of the Martian surface, blasted into space by comet or asteroid impacts, might have crossed the interplanetary gulf and given rise to life here. But what of an interstellar origin for life on Earth? The odds on meteoroids from a system around the average galactic field star not only striking the early Earth but delivering viable microbes are long indeed. But if we consider the Sun's probable origin in a cluster of young stars, all emerging from the same collapsing cloud, the picture changes significantly. Now we're dealing with much smaller distances between stars and slow relative motion as well, conditions...
Centauri Flyby: The Ultimate X Prize?
What should be the goals of the next generation of X Prizes? Peter Diamandis is just the man to ask the question. It was Diamandis' foundation that led to the launch of a private manned spacecraft in 2004, and since then his team has gone on to sponsor an automotive X Prize offering $10 million to anyone who can produce a marketable car that can get 100 miles per gallon. Sixty teams are at work on that one, and prizes focusing on renewable energy are also in the works. The big fish in the pond is the Google Lunar X Prize, which offers $30 million for the first privately funded robotic mission to the Moon. Nor is Diamandis alone. In fact, the landscape is awash in prizes. The Virgin Earth Challenge, brainchild of British aviation mogul Richard Branson, offers $25 million to anyone who designs a viable way to remove greenhouse gases from the Earth's atmosphere. For that matter, what about the Saltire Prize, for which Scotland has found £10 million for renewable energy breakthroughs?...
Gamma-Ray Burst Aimed Directly at Earth
A massive gamma-ray burst detected last March, believed to be the brightest ever seen, turns out to have been aimed directly at the Earth. A narrow jet that drove material toward us at 99.99995 of the speed of light is revealed in the data, itself wrapped within a somewhat slower and wider jet. The best estimates are that an alignment like this occurs only once every ten years. Says Paul O'Brien (University of Leicester, and a member of the team working on the Swift satellite): "We normally detect only the wide jet of a GRB as the inner jet is very narrow, equivalent to not much more than 1/100th the angular size of the full Moon. It seems that to see a very bright GRB the narrow jet has to be pointing precisely at the Earth. We would expect that to happen only about once per decade. On March 19th, we got lucky." It could be said that any information we get about GRBs is in a sense lucky, given how tricky are the constraints for observing them. And indeed, another GRB just degrees...
Sailing Messenger to a Mercury Encounter
Who would have thought the planet Mercury would prove so useful in explaining how solar sails work? The Messenger spacecraft's recent course adjustment maneuvers have proven unnecessary because controllers have been able to use its solar panels creatively, harnessing solar radiation pressure (SRP). And what better place to shake out such methods but on your way to a Sun-drenched planet that moves in an environment where SRP can be eleven times higher than that near Earth? It may come as a surprise that we are already using solar sailing techniques on operational missions, but Messenger is not the first. In fact, we can go back to another Mercury mission, Mariner 10, which took advantage of the effect of solar photons on its twin solar panels, each about nine feet in length and three feet in width, a highly usable 55 square feet that not only generated power but got the spacecraft out of serious trouble. Launched in 1973, Mariner 10 ran into problems with its stabilizing gyroscopes...
Cepheid Variables: A Galactic Internet?
Making contact with an extraterrestrial civilization, whether by microwave, laser or neutrino, highlights the problem of time. Suppose you are looking for a newly emerging technological culture around another star. When do you transmit? After all, even the most powerful signal sent to Earth a million years ago would have no listeners, which is why some have suggested putting actual artifacts in promising solar systems. Rather than transmitting over time-scales measured in eons, you leave an object that can be decoded and activated for communications. All kinds of interesting science and science fictional scenarios flow from that idea. But what if you want to contact not just a few highly targeted systems, but instead send a signal intended for everyone in the galaxy with the means to receive it? As John Learned (University of Hawaii) and team speculate in a new paper, one way to do that would be to select highly visible and important stars to carry your message. Cepheid variables are...
First Images from Steins Flyby
Fine work by Rosetta on the Steins flyby. Check here for more imagery of the 'diamond in the sky,' with cratering suggesting extreme age. Image: Asteroid Steins seen from a distance of 800 km, taken by the OSIRIS imaging system from two different perspectives. The effective diameter of the asteroid is 5 km, approximately as predicted. At the top of the asteroid (as shown in this image), a large crater, approximately 1.5-km in size, can be seen. Scientists were amazed that the asteroid survived the impact that was responsible for the crater. Credits: ESA ©2008 MPS for OSIRIS Team MPS/UPM/LAM/IAA/RSSD/INTA/UPM/DASP/IDA.
Open Courseware: Self-Study and Space
I'm a great believer in the open courseware concept that MIT has done so much to promote. The idea is to do away with the password-protected gatekeeper function that so many university and college Web sites impose, opening access to those course materials an instructor chooses to put online. Some 1800 courses in 33 different disciplines have made their way to the Web via MIT's gateway, their offerings ranging from audio of lectures, lecture notes and exams to PDFs and video files. It's a pleasure to see that Bruce Irving is tracking MIT's venture on his Music of the Spheres site, a post I've chosen to highlight from this week's Carnival of Space collection. Bruce notes one recent addition to the MIT catalog, a course called Space Systems Engineering that looks at design challenges in both ground and space-based telescopes, ultimately attempting to choose the top-rated architectures for a lunar telescope facility. But the MIT offerings are wide ranging. I'm seeing courses on aerospace...
Solar Sails: The Interstellar Prospect
The vast laser-driven sails envisioned by Robert Forward have always fired my imagination. Hundreds of kilometers in diameter, they would rely upon a gigantic Fresnel lens in the outer Solar System to keep the critical laser beam tightly collimated over interstellar distances. Forward conceived of mission designs to stars as far away as Epsilon Eridani, journeys that could be achieved within a human lifetime. He even provided return capability through the use of a multi-part sail. You can read a fictional treatment of this in his novel Rocheworld. But how do we get from here to there? As of today, we're close enough to having an operational space sail that if we can talk SpaceX into lofting the NanoSail-D duplicate, we could be shaking out our first space sail within months. Assuming we do go operational before too many months (or years!) pass, the question then becomes, what kind of missions are possible between the laser-beamed lightsail of science fictional imagining and the...
Cosmic Dust from the Main Belt
With the Steins encounter looming, let's keep the focus on the asteroid belt, in this case by examining a connection between that distant region and our own planet. Cosmic dust particles -- tiny bits of pulverized rock up to a tenth of a millimeter in size -- move continuously through the Solar System, a kind of micro-thin fog of micrometeorites that contributes hundreds of billions of particles to Earth's atmosphere. New research into the makeup of some 600 of these particles now reveals their chemical and mineral content, allowing an overview that points to their origin. The suspected source: A group of asteroids between Mars and Jupiter. You can see one of the Koronis asteroids in the image at left, which shows 243 Ida as photographed by the Galileo probe. What we now believe about the Koronis asteroids is that they were formed some two billion years ago by the breakup of a much larger asteroid. Within the Koronis family are the ninety or so Karin asteroids, which seem to be in a...
Rosetta Closes on Asteroid
Get out to about 2.4 AU from the Sun (2.41 AU, to be precise) and your radio signals have a long travel time. It takes 20 minutes to cross the 360 million kilometers between Earth and the Rosetta spacecraft, and that, of course, is one-way. As we've learned from all our deep space missions, spacecraft are largely on their own for the brief and critical window of an encounter, like the one with asteroid Steins that is coming up for Rosetta. Opportunities for possible trajectory correction maneuvers exist both on September 4 and 5th, but it's on the 4th that Rosetta's controllers will have their last chance to acquire optical images for navigation. Uplink commands for asteroid fly-by mode will be sent on the morning of the 5th and then we wait for results as the vehicle flips for observation and tracking. Rosetta will close to within 800 kilometers of the asteroid, passing it at a speed (relative to Steins) of 8.6 kilometers per second. Image: The approach of Rosetta's spacecraft to...
Dark Matter’s ‘Building Blocks’
Although we often talk about the Magellanic Clouds as satellites of the Milky Way, recent research seems to point to a different conclusion. The dwarf galaxies may be moving too fast to be bound to our own, cities of stars simply flowing past us in the night. Be that as it may, the Milky Way still has over twenty other dwarf galaxies in orbit around it, eighteen of which have been the subject of recent work aimed at calculating their masses. The odd results have striking implications for dark matter. For the dwarf galaxies around us vary greatly in brightness, from a thousand times the luminosity of the Sun to a billion times that amount. You would assume that the brightest dwarf galaxy would have the greatest mass, while the faintest would show the least. The surprise is that all the dwarf galaxies have roughly the same mass, some ten million times the mass of the Sun within their central 300 parsecs. Here's Manoj Kaplinghat (University of California at Irvine) with a helpful...
Preserving Future History
With our eyes on a proposed interstellar future, we don't want to neglect the real challenges of preserving the steps taken along the way. I'm thinking about this because of a post on an astronomy list (thanks to Larry Klaes for the pointer) by Richard Sanderson, who is curator of physical science at the Springfield Science Museum (MA). Sanderson is worried about the media upon which we store our information, and for good reason. Here's the issue in a nutshell: The difficulties that future historians may encounter are related to the ephemeral nature of digital information and the media used to store it. I can visit an old monastery in Europe, find a giant leather-bound astronomy book from the 17th century, blow off the dust, open it, and read the pages (provided I can read Latin). The only tools required are my eyes and hands. But imagine someone living in the 23rd or 24th century who finds an old box of computer diskettes or CDs. Even if the diskettes haven't been corrupted and the...