Yuri’s Night To Be Observed Worldwide

April 12 is a memorable date, the anniversary of Yuri Gagarin's 108-minute orbital flight in 1961. It's also the date, some twenty years later, when NASA launched Columbia, the first Space Shuttle (and boy do I remember the trepidation of watching that one go up). Celebrating these milestones is Yuri's Night, marked by 119 parties scheduled in 32 countries on six continents. Check the celebration site for parties near you. And for stay-at-homes, be aware that Second Life is hosting one of the venues online. Thanks to Frank Taylor for the tip on this. And note (via Larry Klaes) David S. F. Portree's fine tribute to Gagarin's accomplishment. Nice cover of an early 1930's Science Wonder Stories on the same page. Somewhere Hugo Gernsback is smiling...

read more

Water Vapor in an Exoplanet’s Atmosphere

Another discovery thanks to transits. The atmosphere of the exoplanet HD 209458b has been found to contain water vapor. And while that's not unexpected, the effectiveness of the transit method in making the find underlines how significant are the occasions when a planet passes in front of its star as seen from Earth. Studying the infrared spectrum, as Travis Barman did at Lowell Observatory, shows the apparent signature of water vapor absorption when compared to the visible spectrum. But don't expect an ocean world here. The planet involved orbits its star every three and a half days; HD 209458b is, in fact, a 'hot Jupiter,' its upper atmosphere heated to temperatures as high as 10,000 degrees K. The planet is doubtless losing thousands of tons of material every second as it vents gases into the incendiary environment so near its primary. Nonetheless, finding water vapor does provide confirmation of theories that suggest almost all extrasolar planets have water vapor in their...

read more

Red Foliage Under an Alien Sky

Years ago I wrote a story called 'Rembrandt's Eye,' using as background a planet whose foliage was predominantly red. The story, which ran in a short-lived semi-pro magazine called Just Pulp, came back to mind when the news from Caltech arrived. Researchers at the Virtual Planetary Laboratory there now believe that Earth-type worlds may have foliage that is largely yellow, orange or, as in the case of my planet, red. The green of Earth's plant life is anything but a universal standard. This interesting conclusion emerges from computer models designed to provide pointers for the future search for plant life on exoplanets. After all, astronomers will need to know what they might see in the spectra we'll one day be able to harvest from space-borne observatories. Ponder everything that's involved, from the color of the main sequence primary star to the aquatic habitats of aqueous plants. The search involves the way photosynthesis might occur under varying conditions, with the filtering...

read more

Of Time Travel and Funding

Traveling to the planets takes big money and we've been part of the squabbing over where NASA money in particular ought to be allocated. But what about projects that take small money? The term is relative, of course, but John Cramer (University of Washington) thinks $20,000 should suffice to run his experiment in time travel, and with NASA's Institute for Advanced Concepts now shutting down, he's having a hard time raising it. This Seattle Post-Intelligencer story has more. We've looked at Cramer's work before, but a brief summary is in order. It involves Einstein's 'spooky action at a distance,' the so-called Einstein-Podolsky-Rosen effect. Quantum entanglement seems to mean that two entangled particles influence each other no matter how far distant in space. That action appears to be instantaneous, which introduces the paradoxical outcome of suggesting that something can communicate faster than the speed of light. Einstein, of course, would say that's flat out impossible. Quantum...

read more

RIPL: A New Kind of Planet Hunt

Since we've recently been discussing astrometry, the discipline that measures star distances and movements, now would be a good time to look at two significant projects that go beyond optical methods to use radio astrometry in planet hunting. The Radio Interferometric Planet Search (RIPL) will draw on the Very Long Baseline Array, ten dish antennae spanning more than 5000 miles, and the 100-meter Green Bank telescope in West Virginia. The target: 29 active low-mass stars to be examined in a three-year planet hunt. The targets are significant because they're a kind of star that's currently out of reach for radial velocity techniques. All are M dwarfs that are active, meaning they display 'starspots' (analogous to sunspots), flares or other activity in their chromospheres. The more active a faint star like this, the more likely that radial velocity measurements will be distorted with a 'jitter' that disturbs the precision of the measurement. RIPL ought to be able to sort out the...

read more

Calibrating a Standard Candle

Cepheid variables are simply indispensable. It was Harvard's Henrietta Leavitt who, in 1912, discovered a relationship between the cycle of variable brightness in these stars and their luminosity. With a classic Cepheid, the longer the period of the star, the greater its intrinsic brightness. That sets up the method: Determine the period of the variable, check its apparent magnitude with the absolute magnitude corresponding to that period, and you can measure the distance. The relevant term is 'standard candle.' But put telescopes into space and you can refine these measurements, as studies of Cepheid variables with the Hubble Space Telescope have now shown. That's helpful because we'd like to know the Hubble constant -- the universe's rate of expansion -- as accurately as possible, and Cepheids are one of our best tools. To fine-tune the Cepheid method, a team from the University of Texas at Austin has directly measured the distance to ten Cepheid variables, using Hubble to trace...

read more

A New Red Dwarf Planet

A Neptune-class planet has been discovered around the nearby red dwarf GJ 674, and it's an intriguing one. Using the HARPS spectrograph on the European Southern Observatory's 3.6 meter telescope at La Silla (Chile), the discovery team determined that the new planet was 0.039 AU from its parent star, yielding a temperature of some 450 degrees K. With a minimum mass estimate of about 11 times the mass of Earth, it completes an orbit every 4.69 days. Whether GJ 674 b is largely gaseous or rocky is unknown, although further observations of its orbital eccentricity may yield clues. We're not down to Earth-mass planets yet, but this is an interesting find. This is the second-closest known planetary system (after Epsilon Eridani). GJ 674 is less than 15 light years away and it's one of the brightest M dwarfs in our field of view. That makes the transit situation interesting, as Greg Laughlin noted in this systemic post: At first glance, such an effort might appear to be hampered by the fact...

read more

Sunshades for Global Warming

Could a cloud of two-foot wide sunshades 60,000 miles long save the Earth from a global warming emergency? Roger Angel (Steward Observatory, University of Arizona) has been studying the idea of making the spacecraft out of micron-thick glass weighing one gram per sunshade. That's the weight of a butterfly for each unit, but we're talking about trillions of them out at the L1 Lagrangian point, an almost fixed zone in relation to Earth whose mild orbital instability can be overcome by onboard intelligence. Total sunshade mass: 20 million tons. This article in the Arizona Daily Wildcat has more on the improbable concept and what Angel is doing today: One of the big problems for the project is getting the total mass of all the sunshades into space...so Angel came up with using electromagnetic force to propel the spacecraft up a two-kilometer launch tube. The launch tube would have a series of electrical coils that propel the rocket until it accelerates to escape velocity, about 25,000...

read more

Amateur Radio: Where the Real DX Is

Back in the 1980's, I was active as a shortwave listener. I was, in radio jargon, an SWL and not a ham, meaning I only listened and didn't transmit. It was great fun to tune in distant stations, and the more challenging the better, which is why the Falkland Islands were always high on the list (I never received their station), and Tristan da Cunha was the ultimate catch (all but impossible here on the US east coast). It wasn't long before I drifted into utility DXing, listening for non-broadcast stations in remote places, everything from low-frequency aviation beacons to ship-to-shore communications, and I got a kick out of monitoring radiotelephone traffic from places like Little America (Antarctica) back to the States. Finally my interests converged and I started thinking about the ultimate DX -- receiving a signal from the stars. SETI efforts were in their early days then, but I began to wonder whether an amateur receiving rig could hope to snag some kind of extraterrestrial...

read more

Sizing Up the Asteroid Threat

The potential threat from near-Earth asteroids can sometimes seem purely theoretical, an academic exercise in how orbits are calculated and refined. But when we start quantifying possible damage from an asteroid strike, the issue becomes a little more vivid. Modeling potential impact points all over the planet, a University of Southampton (UK) team has worked out some stark numbers. The University's Nick Bailey presented the results at the recent Planetary Defense Conference in Washington. The researchers put a software package called NEOimpactor to work on asteroids under one kilometer in diameter and assumed an impact speed of 20 kilometers per second. Obviously, larger objects are out there and the impact velocity is arbitary, but asteroids in this size range seem to hit the Earth every 10,000 years, frequent enough that the next one that does hit will probably fit this description. Says Bailey: 'The consequences for human populations and infrastructure as a result of an impact...

read more

Electric Sail Rides the Solar Wind

A Finnish team has introduced a new wrinkle on the solar sail idea. Or more specifically, on the general principles of the magnetic sail, which would tap the propulsive power of the solar wind to push a 'sail' created as a field around the spacecraft itself. The so-called 'electric sail' would use fifty to one hundred 20-kilometer long charged tethers, their voltage maintained by a solar-powered electron gun aboard the vehicle. We're talking about tethers made of wires that are thinner than a human hair, thin enough that each can be wound into a small reel. But unwind the tethers and you get interesting results. The electric field of each wire now extends tens of meters into the solar wind flow. A single tether yields the equivalent effective area of a sail roughly a square kilometer in size. You can see the promise of deploying multiple tethers to reach high velocities. What's more, this sail allows the spacecraft to 'tack' towards the Sun as well as sailing outward from it. All...

read more

A Note on the Enzmann Starship

The always reliable Adam Crowl takes on fueling requirements for starship projects like Daedalus, with an interesting look at alternatives for mining He3. The Daedalus team, members of the British Interplanetary Society who created the first in-depth study of a starship, had hoped to tap Jupiter's atmosphere for the job, but Crowl examines Saturn, Uranus and Neptune as well, finding Saturn the best fit. Adam then tackles a fascinating article by G. Harry Stine (thereby launching me on a search for the back issue of the magazine in question, now almost irretrievably hidden in the recesses of my office). Here's how he describes it in Crowlspace: I have just received an issue of the October 1973 Analog - the one with a gorgeous Rick Sternbach cover of two Enzmann starships and the cover article by G. Harry Stine, "A Program for Star Flight". It's quite a memorable article as Stine was arguing for a star flight program to begin c.1990, and the development of a massive in-space industrial...

read more

Einstein, Updike and the Academy

John Updike reviews Walter Isaacson's new biography of Einstein in The New Yorker, from which this excerpt on why a job in the Swiss patent office was actually a good thing for the young genius: "Had he been consigned instead to the job of an assistant to a professor," Isaacson points out, "he might have felt compelled to churn out safe publications and be overly cautious in challenging accepted notions." Special relativity has a flavor of the patent office; one of the theory's charms for the fascinated public was the practical apparatus of its exposition, involving down-to-earth images like passing trains equipped with reflecting mirrors on their ceilings, and measuring rods that magically shrink with speed from the standpoint of a stationary observer, and clocks that slow as they accelerate — counterintuitive effects graspable with little more math than plane geometry. Einstein would later say, upon taking his first professorship (at Zurich), that in doing so he had become...

read more

Freeman Dyson: Reasons for Optimism

Centauri Dreams believes profoundly in what I might call 'realistic optimism.' While an aggressive belief in the human future can be overstated, it's important to remember that intellectual fashions come and go, leaving many a futurist trying to explain another failed prediction. The view here is that the vast problems that face our species are solvable through common sense and technology, and that somehow we will engage our tools to get us off-planet before we annihilate ourselves. Playing into this notion is the work of David Haussler, cited recently by Freeman Dyson as one reason for his own deeply optimistic view of the future. Studying the human genome, Haussler and team at UC Santa Cruz discovered a section of DNA called Human Accelerated Region 1. HAR1 evidently shows up in the genomes of a wide range of species, from mouse to chicken to chimpanzee. It was apparently unchanged for about three hundred million years, as Dyson told Benny Peiser in a recent interview (see this New...

read more

Double Stars May Be Aswarm with Planets

The number of stars with possible planets keeps going up. The astronomy books I read as a kid operated under the assumption that we needed to look at Sun-like stars to find planets, and that meant single rather than double or triple systems. The tantalizingly close Alpha Centauri stars were all but ruled out because of their assumed disruptive effects on planetary orbits. No, find a nice G-class star all by itself and there you might have a solar system something like our own and, who knows, a second Earth. Today we're fitting binary stars into the planetary picture with ease. Astronomers see little reason to rule them out. Consider what David Trilling (University of Arizona) has to say about the matter in an upcoming paper: "There appears to be no bias against having planetary system formation in binary systems. There could be countless planets out there with two or more suns." Just imagine the possible sunsets. Image: Our solitary sunsets here on Earth might not be all that common...

read more

Red Dwarf Planets: Too Dry for Life?

Sometimes I imagine an ancient place where a dim sun hangs unmoving at zenith, and a race of philosophers and poets works out life's verities under an unchanging sky. Could a place like this, on a terrestrial world orbiting an M-class red dwarf, really exist? A new paper by Jack Lissauer (NASA Ames) casts doubt on the idea. Lissauer argues that planets inside an M dwarf's habitable zone are probably lacking in water and other volatiles, and are thus unable to produce life as we know it. The question is important because M dwarfs make up as much as 75 percent of the stars in our part of the galaxy. If we include them as candidates for life, we add a hundred billion or more potential habitats in the Milky Way alone. We've known for some time that although the proximity of such a terrestrial M dwarf planet to its star would cause it to be tidally locked -- one side in constant light, the other in darkness -- habitable regions might still occur on the dayside given a dense enough...

read more

Odd Hexagon at Saturn’s Pole

Shrouded in the night of a 15-year winter, Saturn's north pole demands specialized instruments to yield its secrets. Enter Cassini's visual and infrared mapping spectrometer, whose data on the region have disappointed no one. A six-sided honeycomb-shaped feature has emerged that was first found by the Voyager 1 and 2 spacecraft over twenty years ago. Now Cassini has, for the first time, captured the entire hexagon in a single image. What exactly is it? Think of Earth's polar regions, where winds move in a circular pattern around the pole, but ponder this difference: Saturn's vortex is a hexagon nearly 25,000 kilometers across. Four Earths would fit inside it. Click here for a QuickTime movie of the odd feature. This makes Saturn possibly the Solar System's most intriguing object when it comes to polar anomalies. The south pole sports an enormous hurricane, while the north is dominated by clouds moving along the hexagon at great rate. Indications are that the hexagon extends fully 100...

read more

Asia Emerging II

by Gregory & Elisabeth Benford We left February 17, 2007 on a considerable, month-long trip, starting with Hong Kong, where we caught the Lunar New Year Celebration (Chinese New Year). Then on to Colombo, Sri Lanka, to visit Arthur Clarke. Arthur has post polio syndrome and thus very little memory or energy. He turns 90 this December and wants to keep in touch with the outer world, mostly through the Internet. He has few friends left in Colombo. Arthur took us to the Swimming Club for lunch, a sunny ocean club left over from the British days (commonly called the Raj). Members swam in the pool and enjoyed buffet lunch. It felt somehow right to watch the Indian Ocean curl in, breaking on the rocks, and speak of space: the last, greatest ocean. Image: Elisabeth, Arthur C. Clarke, and Greg in ACC's home study in Colombo. Our hotel with a similar ocean view, the Galle Face, is the oldest grand Raj hotel east of the Suez Canal, dating from before the Civil War, and reeks of atmosphere. On...

read more

Asia Emerging

by Gregory Benford Centauri Dreams is pleased to present the travels of Gregory Benford, just returned from a multi-week journey that took him to Sri Lanka to see Arthur C. Clarke, around the southern Indian coast all the way to Bombay, thence to Jaipur, Delhi and finally on to Singapore. The well-known physicist and science fiction author portrays lands awash in history but laden with potential for a possible future off-planet. Will a China/India space race revitalize manned spacecraft technologies? Enjoy the journey and be sure to check the Benford & Rose site for the author's recent essays and commentaries. We left February 17, 2007 on a considerable, month-long trip, starting with Hong Kong. We caught the Lunar Celebration at Chinese New Year—huge crowds, spectacular fireworks. Then on to Colombo, Sri Lanka, to visit Arthur C. Clarke. Arthur has post polio syndrome and thus very little memory or energy. He turns 90 this December and wants to keep in touch with the outer...

read more

OSIRIS: Asteroid Sample Return

A little bit of asteroid 1999 RQ36 may wind up on Earth in 2017. That's assuming that NASA's OSIRIS mission launches in 2011, with the aim of investigating the properties of such Earth-crossing bodies. And while an asteroid sample may help us understand much about the early Solar System, OSIRIS offers a potentially greater benefit. It can help us sharpen our tracking skills so we can plot asteroid orbits with much greater precision. How? You'll recall that we recently discussed the the Yarkovsky Yarkovsky-O'Keefe-Radzievskii-Paddack effect. YORP is the minute push that an asteroid receives over time as it absorbs sunlight and emits heat -- let's call it the Yarkovsky Effect for short. It's a tricky thing to measure because of the uneven nature of asteroidal surfaces, and the varying wobble and rotation of each. Trying to predict an asteroid's orbit as it approaches Earth demands that we take the Yarkovsky Effect into account. And OSIRIS is tasked with measuring the effect for the...

read more

Charter

In Centauri Dreams, Paul Gilster looks at peer-reviewed research on deep space exploration, with an eye toward interstellar possibilities. For many years this site coordinated its efforts with the Tau Zero Foundation. It now serves as an independent forum for deep space news and ideas. In the logo above, the leftmost star is Alpha Centauri, a triple system closer than any other star, and a primary target for early interstellar probes. To its right is Beta Centauri (not a part of the Alpha Centauri system), with Beta, Gamma, Delta and Epsilon Crucis, stars in the Southern Cross, visible at the far right (image courtesy of Marco Lorenzi).

Now Reading

Recent Posts

On Comments

If you'd like to submit a comment for possible publication on Centauri Dreams, I will be glad to consider it. The primary criterion is that comments contribute meaningfully to the debate. Among other criteria for selection: Comments must be on topic, directly related to the post in question, must use appropriate language, and must not be abusive to others. Civility counts. In addition, a valid email address is required for a comment to be considered. Centauri Dreams is emphatically not a soapbox for political or religious views submitted by individuals or organizations. A long form of the policy can be viewed on the Administrative page. The short form is this: If your comment is not on topic and respectful to others, I'm probably not going to run it.

Follow with RSS or E-Mail

RSS
Follow by Email

Follow by E-Mail

Get new posts by email:

Advanced Propulsion Research

Beginning and End

Archives