Are we going to detect 500,000 near-Earth objects in the next fifteen years as technologies improve? The Association of Space Explorers thinks so, and lays out its view of the danger we face from asteroids and other near-Earth objects in a new report. I'm looking through an executive summary of Asteroid Threats: A Call for Global Response right now, not long after the release of the report's results late last week. The ASE hopes to involve the United Nations in a global information network that would improve our existing capabilities at finding and tracking dangerous objects. It would also set up an oversight group to advise the Security Council about the risks and the best ways to deflect potential impactors. Why the UN? Because it's a global problem. The report points out that trying to deflect an incoming asteroid would create questions of authorization, liability and financial action that inevitably involve the international community. Citing its belief that existing technology...
Musings on the Ages of Man
Centauri Dreams takes an optimistic view of the human future, one in which interstellar flight becomes a reality at some point in this millennium. My impression is that we'd all better be optimists. Think about the Drake Equation. Perhaps its most significant variable is the lifetime of a technological civilization, a figure that has implications for any creatures who have developed the tools to go into space. If the lifetime of such a civilization averages a million years, then the 'where are they' question Fermi asked becomes more charged. Shouldn't we be detecting them? But if the average lifetime of a technological culture is, say, five hundred years, then we may be confronted with a galaxy filled with wreckage, planets where life persists in evolving and forming intelligent beings who bring about their own destruction. Like I say, I'd rather be an optimist, but none of us knows the real answer. I note that Jan Zalasiewicz (University of Leicester) has offered up a new book that...
Latest Carnival: Electric Sails and More
The latest Carnival of Space is stuffed with good things, among them Dave Mosher's manipulations of an asteroid impact calculator run by Cardiff University's Ed Gomez. Dave works through a worst-case scenario -- a 1300-foot wide asteroid striking the East River, turning most of New York City into a crater. Fascinatingly, the impact calculator lets users adjust the parameters on such strikes, so that turning the impactor into a 400-meter piece of ice produces a crater 3.5 miles wide, two miles less than the first scenario. The calculator looks to be a great educational tool. NextBigFuture continues to study the electric sail concept, developed at the Finnish Meteorological Institute and under active examination. Electric sails ride the solar wind, but unlike magsails, they use a mesh of tethers kept at high positive voltage, held in place by centrifugal acceleration from the spinning spacecraft. Solar wind protons, repelled by the positive voltage of the mesh, create the needed...
Rough Sailing on the Solar Wind
All of nature is a kind of laboratory, which is why good propulsion ideas can flow from astronomical observations that show us how things work. Recent news about the solar wind is a case in point. An analysis of data from the Ulysses spacecraft shows that the solar wind is now lower than at any time previously measured. That has implications for the heliopause, that region where the solar wind encounters true interstellar space, for this region plays a role in shielding the Solar System from the effects of galactic cosmic rays. "Galactic cosmic rays carry with them radiation from other parts of our galaxy," says Ed Smith, NASA's Ulysses project scientist at the Jet Propulsion Laboratory in Pasadena, Calif. "With the solar wind at an all-time low, there is an excellent chance the heliosphere will diminish in size and strength. If that occurs, more galactic cosmic rays will make it into the inner part of our solar system." Image: The Ulysses spacecraft. Credit: Jet Propulsion...
Colliding Worlds: The Ultimate Extinction Event
When Worlds Collide, the 1932 novel of planetary catastrophe, presented the most extreme extinction event imaginable. A pair of wandering planets enters the Solar System, one on collision course with the Earth, the other destined to be captured into orbit around the Sun. The doughty crew of an escaping rocket, on their way to a new life on the captured world, can only watch in horror as the Earth is destroyed. Now we learn about a 'when worlds collide' scenario that seems to have involved two mature, Earth-sized planets in a distant Solar System. The system in question is BD+20 307, originally thought to be a single star with a massive, warm dust disk, but now known to be a close binary orbiting the common center of mass every 3.42 days. Both stars are similar to the Sun in mass, temperature and size. Moreover, the system seems to have an age comparable to our own Sun, and the sheer amount of dust at roughly Venus to Earth distance is quite interesting. We would expect the dust...
A Dark Flow in the Cosmos
Seeing things that are otherwise invisible means looking for their effect on the things we can see. Examples abound: The presence of dark matter was originally inferred from the shape of galaxies, and the fact that the mass of what we could see couldn't explain how these cities of stars held together. Dark energy turned up through minute examination of supernovae, shaping the idea that the acceleration of the universe is an ongoing phenomenon. And now we have another unusual effect suggesting the presence of matter beyond the observable universe. The work grows out of the study of some 700 galactic clusters whose X-rays, emitted by hot gases, cause measurable effects on photons from the cosmic microwave background. This is the Sunyaev-Zel'dovich effect, in which high energy electrons impart some of their energy to the CMB. A variant of the SZ effect helps us study galactic clusters in ways that now suggest the presence of inflation in the early universe. Thus Alexander Kashlinsky...
Interstellar Flight in Context: A Bet Already Won?
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.