Centauri Dreams has little use for pessimism. The operative assumption in these precincts is that humanity will muddle through somehow and eventually get to the stars, whether in a matter of centuries or millennia. But it's always good to have a backup plan in the event of catastrophe, which is what the Norwegian government has been working on. Who knows when some rogue asteroid like 99942 Apophis may beat the odds and fall, with shattering results, to Earth? The Svalbard International Seed Vault has the aim of protecting the world's agriculture in a vast seed bank, one that would house three million seed samples. Collecting and maintaining the seeds is the Global Crop Diversity Trust, whose executive director, Cary Fowler, likened the vault to a safety net in a recent BBC story, saying "Can you imagine an effective, efficient, sustainable response to climate change, water shortages, food security issues without what is going to go in the vault - it is the raw material of...
Celestial Postage
It's hard to believe that Sir Patrick Moore started his astronomy program The Sky at Night fifty years ago. Since then, BBC viewers have known where to turn for a view of things celestial, one with that particular Moore mix of savvy and amiable, eccentric enthusiasm that comes across so well in his many books. So what a pleasure to see that a set of stamps has now gone on sale honoring his work. How else would you see interstellar scenery on an postal envelope? A news account in the Telegraph quotes Sir Patrick thus: "I feel deeply honoured. I would like to think that we have played a part in introducing astronomy to people who would otherwise have paid no real attention to the heavens. Many years hence, philatelists will still be admiring these stamps paying tribute, not to me, but to The Sky At Night." Can you imagine a show running for fifty years with the same host? I hate to disagree with the gentleman, having grown up reading his books, but the tribute future stamp admirers pay...
Debris Disk Around a Dead Star
Our Solar System in the distant future may look something like the Helix nebula today. That's because in about five billion years, the Sun will have become a white dwarf, its inner planets swallowed up by its earlier expansion, its outer planets, asteroids and comets surviving in distant orbits and colliding with each other to form a ring of dusty debris. The Sun will undergo, in other words, a kind of rejuvenation, experiencing what scientists call 'late bombardment' in a system that has become dynamically young again. Such a disk has now been found in the Helix nebula, some 700 light years away in Aquarius. It took the infrared tools of the Spitzer Space Telescope to sort out the glow of the dusty disk that circles the remnant white dwarf between 35 and 150 AU out. The assumption is that the disk is the result of smashups in the outer system, presumably involving objects like those in our Kuiper Belt or comets from an Oort-like cloud. Image: Spitzer's infrared view of the Helix...
Minkowski and His Legacy
Centennaries are worth celebrating, especially when they involve people whose work advanced our understanding of reality. A big one comes up in 2008, about which this clue: "The views of space and time which I wish to lay before you have sprung from the soil of experimental physics, and therein lies their strength. They are radical. Henceforth space by itself, and time by itself, are doomed to fade away into mere shadows, and only a kind of union of the two will preserve an independent reality." The speaker is Hermann Minkowski (1864-1909), the German scientist and mathematician who didn't survive the 1908 presentation he began with these words by more than a few months (he died of appendicitis the following January). The talk, entitled Raum und Zeit, contains Minkowski's view that time and space must be understood together as a four dimensional concept called spacetime. That idea played a material role in furthering Einstein's later development of General Relativity. Indeed,...
Planet Hunting in the News
It's good to see that Greg Laughlin's systemic project is getting some public attention. This article in the Santa Cruz Sentinel goes through the basics, explaining how amateurs can use the systemic console to identify possible planets around other stars. "We want to demonstrate that it's not just public outreach, it's a way of carrying out research," Laughlin adds, and that fusion is what the Net is bringing to exoplanetary studies.
A Cold, Bright Universe
To see heat, you'd better be cold. In space, at least, because when you're looking in infrared wavelengths, the heat of your instrumentation can overwhelm the image you're trying to get. Infrared light is hugely useful, especially when it lets us see through clouds of dust to what lies beyond. Take a look at the image below, which penetrates the dust to show stars in the center of the Milky Way. I ran into it thanks to a post on QUASAR9 and have been musing about spacecraft cooling ever since. Image: A mosaic of many smaller snapshots, the detailed, false-color image shows older, cool stars in bluish hues. Reddish glowing dust clouds are associated with young, hot stars in stellar nurseries. The galactic center lies some 26,000 light-years away, toward the constellation Sagittarius. Credit: Susan Stolovy (SSC/Caltech) et al., JPL-Caltech, NASA. The Spitzer Space Telescope, which caught this image with its infrared cameras, has to be cooled to near absolute zero (-459 degrees...
A Map of Dark Matter
Looking at the beautiful swirl of a spiral galaxy, it's hard to imagine how much we're not seeing. But current studies indicate that dark matter in a typical galaxy outweighs the stars in it by ten to one. That's the conclusion of astronomer Michael Strauss (Princeton), who has been working on how the dark matter halos of such galaxies cluster. Combine those calculations with the visible information provided by quasars and you can say something about the mass of the halos. This is fascinating work indeed, using Sloan Digital Sky Survey data that reveal quasar superclusters divided by vast regions of empty space. The quasars themselves are bright concentrations of gas falling into supermassive black holes at the center of galaxies. And it's clear they're embedded in massive concentrations of dark matter. Says Strauss: "We can't observe the dark halos directly, but we know from theoretical calculations how they should cluster with one another. By measuring the clustering of the...
Warming Up the Ancient Earth
The early Earth presents us with a conundrum. 3.75 billion years ago, the Sun is thought to have been 25 percent fainter than it is today. Yet liquid water existed on Earth's surface instead of the ice we would expect. How? The answer may be carbon dioxide in the atmosphere, a conclusion drawn from work on ancient rocks in northern Quebec. Says Stephen Mojzsis (University of Colorado at Boulder), "We now have direct evidence that Earth's atmosphere was loaded with CO2 early in its history, which probably kept the planet from freezing and going the way of Mars." The rocks studied by Mojzsis and team show the presence of iron carbonates that are thought to have precipitated from oceans of that distant era. And they could only have formed in an atmosphere that contained CO2 levels far higher than we see today. Thus we witness carbon dioxide's role as a climatic thermostat, raising Earth's temperatures by holding in the weaker heat provided by the Sun. The area of Hudson's Bay under...
Sir Arthur and the Imagination
Centauri Dreams has no idea how you quantify something as elusive as imagination, but if anyone should have a go at it, that man is Arthur C. Clarke. Thus the interesting news of the center being established in his name in Las Vegas. Its goal: "...to investigate the reach and impact of human imagination." The Clarke Foundation hopes to raise $70 million for the project, which Clarke says aims to "...accord imagination as much regard as high academic grades in the classroom - anywhere in the world." Exactly how this is done will be fascinating to see. It's good to learn that Sir Arthur's health is on the mend, and to hear him in this recent message on KurzweilAI.net talking about a rejuvenated space program: Notwithstanding the remarkable accomplishments during the past 50 years, I believe that the Golden Age of space travel is still ahead of us. Before the current decade is out, fee-paying passengers will be experiencing sub-orbital flights aboard privately funded passenger vehicles,...
Magsails on the Solar Wind?
When we talk about solar sails for space missions, we normally think of physical objects, vast but incredibly thin sheets of high-tech material pushed by the momentum imparted by solar photons. Someday we may use such sails to ply routes between the planets, but as researchers ponder such technologies, they're also looking at the possibilities of magnetic sails using a different kind of propulsion. Rather than being pushed by photons, a magsail interacts with the plasma of the solar wind. And that makes for some interesting possibilities. The solar wind is a stream of charged particles moving at high speeds -- 500 kilometers per second and more -- and if you can harness it through technologies like Robert Winglee's Mini-Magnetospheric Plasma Propulsion (M2P2), you can ride that wind on a magnetic bubble hundreds of kilometers in diameter. Someday magsails may even provide deceleration capability for interstellar probes as they arrive in distant solar systems. All that puts the...
Looking at Exoplanet Atmospheres
Actually seeing something is so much more rewarding than just inferring its presence. But in the case of exoplanets, looking at the actual light bouncing off a distant planet does more than just satisfying our curiosity. Starshade concepts and other methods of terrestrial planet detection point to an ultimate payoff: We want to analyze the light of a distant world to learn what elements are found in its atmosphere. These become clues to conditions there, and even markers of possible life. Centauri Dreams readers know I'm a great admirer of the starshade concept, not only as developed by Webster Cash in his New Worlds Imager designs but also as widely studied for other possible missions (for more on starshades, see the UMBRAS site). Starshades are all about direct observation -- images, spectroscopy, photometry -- rather than methods like radial velocity studies that find planets through the motions of their parent stars. And I like starshade technologies because they seem to offer...
A Starshade Overview
Want to build a starshade to spot Earth-like worlds around other stars? Start with a Hubble-like telescope a few million miles from Earth. Add a 30-meter wide disk with petal-like extensions, separated by 10,000 miles from the telescope. Watch what happens next. Using lasers, the two parts would line up, with the star shade just blocking out the light from a nearby star from the center of the telescope's view. Calculated mathematically to throw away the light from the star but keep the light from any planets it held (this is the "occulting" part of the occulted), the device would be able to detect planets smaller than Earth orbiting stars within 35 light years of Earth, Cash and his colleagues calculate. The key is the petal shape of the shade, which scatters starlight from the telescope's view. From an overview of planet-finder technologies by Dan Vergano in USA Today. Webster Cash, whose name is frequently found in the Centauri Dreams archives, is a major part of the...
Tuning Darwin’s Target List
Barrie Jones (The Open University, UK) will have an interesting job in ESA's planned Darwin mission. Darwin's goal is to find Earth-like worlds around other stars. Jones will prioritize planetary systems so the mission's telescopes -- three instruments mounted on separate spacecraft -- can concentrate on those most likely to have Earth-like planets in their habitable zones. He's already done computer modeling on many currently known planets, finding that half of them occur in systems where a stable orbit for a terrestrial world exists in the habitable zone. But much depends on how you deal with planetary migration, says Jones, discussing his computer modeling in a recent interview. A gas giant moving through the inner system to become a 'hot Jupiter' may or may not preclude the presence of an Earth-like planet -- recent work gives us hope that it will not, but the issue is still undecided. Says Jones: If Earths can form after the giants migrate toward the star and become "Hot...
GEMSS: Hunting for Red Dwarf Exoplanets
If I were a betting man, I would put some money on this proposition: The first detection of a potentially habitable planet will be made before the end of this decade, and the planet will be found around an M-class red dwarf. The method will doubtless be photometry, picking up the slight drop in light caused by such a planet transiting its star. A planet the size of our Earth will block about one percent of the stellar flux, as a recent paper points out, and a one percent photometric dip is quite detectible. Image: An animation of a stellar transit around HD 209458. Credit: Transits of Extrasolar Planets Network. Although TEP concluded its work in 2001, you can still read about it online. So the key is to find the right M-dwarf, with its planetary system lined up so that the hypothetical terrestrial world passes between its star and us. That's no small challenge, but Paul Shankland (U.S. Naval Observatory), who is lead author on the paper mentioned above, is working with colleagues...
Into the Wormhole
Can we find and actually traverse a wormhole? Crowlspace looks at the possibilities and links to a paper by Nikolai Kardashev that we'll be examining here in the next week or so. A snippet: Relativity gives no clear indication of where wormholes end. They might link to other places (and times) in our Universe or in other Universes. When the worm-ways of the Universe are finally explored there will be a whole new breed of adventurers required to travel to their far-ends, risking being lost in a wholly other Universe and time. After hardy explorers have mapped the wormhole network of the Universe what will happen then? A provocative scenario indeed! Read the whole thing here.
The Approach of Gliese 710
The Astroprof's Page takes a look at the interesting star Gliese 710, a K7 dwarf with a particular claim to distinction: it's headed in the direction of our Sun at about 24 kilometers per second. Give it 1.4 million years and the star will have closed to within a light year of Sol, shining at a magnitude of 1.2 and disturbing the icy debris out in the Oort Cloud. A rain of comets moving into the inner system is the probable result. Barnard's Star is moving towards us too, closing to within four light years around 10000 AD, but we needn't wait for a close stellar pass to start worrying about catastrophic collisions. As the battered surface of the Moon suggests, the Solar System can be a hostile place, making a space-based infrastructure to prevent future disaster an imperative.
Davies and the ‘Goldilocks Enigma’
A recent mention of Paul Davies reminds me (belatedly, to be sure) to point you to "We Were Meant to Be Here," an interview Phillip Adams conducted with the physicist on ABC Radio National. The occasion was Davies 60th birthday last June, the conversation's title reflective of the usual Davies range across the deepest issues of life in the cosmos. Davies, formerly at Macquarie University, has left Australia and is now active at Arizona State, where he is establishing the Institute for Fundamental Concepts in Science. Other good audio is available at Davies' site. Also, a review of his The Goldilocks Enigma: Why is the Universe Just Right for Life? (Allen Lane, 2006) is available here.
Darwin and Luna
Some years back, the fine space writer William E. Burrows helped to establish ARC, the Alliance to Rescue Civilization. ARC's purpose was to create an imperishable archive that would contain a record of our civilization in the event of catastrophe. Now a part of the Lifeboat Foundation, ARC envisioned making a 'backup' of the human experience, with the Moon as just one venue. In today's Wall Street Journal, Burrows looks at the dangers of returning to the Moon vs. staying home: It is therefore reasonable to ask whether such an incredibly expensive and dangerous undertaking is worth it. The answer is an unequivocal yes. But the truly compelling reason to build a lunar base is not for adventure, though there will be plenty of that. Nor is it to mine resources to gain riches, though that will eventually happen. The overriding reason to establish a colony on the moon is humanity's survival: Darwin achieves liftoff. Do we really need the current space station? Burrows says no -- we...
An Oscillating Universe After All?
Expansion, turnaround, contraction and bounce. Those are the four components of a new model of the universe created by researchers at the University of North Carolina at Chapel Hill. Their work offers an alternative to the Big Bang theories in the marketplace and sets up a cyclical progression in which an infinite number of independent universes emerge from what's left of matter just before the end of time. Tough going, this. But think of the universe's vast expansion pushing everything progressively further out until all matter disintegrates. This is the turnaround point, and it is here that each fragmented 'patch' of what had been matter collapses and contracts. "We discuss contraction which occurs with a very much smaller universe than in expansion," write the researchers, "and with almost vanishing entropy because it is assumed empty of dust, matter and black holes." The key is that this collapse occurs individually, so that rather than causing the Big Bang to run in reverse,...
Philosophia Naturalis #6 Now Online
The sixth edition of Philosophia Naturalis is out, published by Charles Daney on his Science and Reason blog. It's a 'carnival' of interesting writing in the weblog format, pointing to writing by diverse and sundry authors on the physical sciences and technology. Carnivals like this one seem to be gaining popularity, a welcome thing because they offer pointers to sites I hadn't known about, and the topics are always interesting. Good coverage of the American Astronomical Society meeting shows up here, along with work on dark matter, the Antikythera Mechanism, and a wonderful explanation of light cones and Einsteinian relativity. I'm pleased that Philosophia Naturalis includes two recent posts on the James Webb Space Telescope from these pages.