This statement was released by The Planetary Society at 13:30 EDT: "In the past twenty-four hours, the Russian space agency (RKA) has made a tentative conclusion that the Volna rocket carrying Cosmos 1 failed during the firing of the first stage. This would mean that Cosmos 1 is lost. While it is likely that this conclusion is correct, there are some inconsistent indications from information received from other sources. The Cosmos 1 team observed what appear to be signals, that looks like they are from the spacecraft when it was over the first three ground stations and some Doppler data over one of these stations. This might indicate that Cosmos 1 made it into orbit, but probably a lower one than intended. "The project team now considers this to be a very small probability. But because there is a slim chance that it might be so, efforts to contact and track the spacecraft continue. We are working with US Strategic Command to provide additional information in a day or so. "If the...
Solar Sail Fails to Reach Orbit
The Planetary Society's servers were slammed yesterday through the launch and aftermath of the Cosmos 1 mission, but the entries again available on Emily Lakdawalla's more or less official weblog make for grim reading this morning. For that matter, so does the silence that follows her post at 1915 EDT last night, saying that the search continued for Cosmos 1, but the ground stations that expected to receive the spacecraft's signal have come up empty. True, some signals have been detected, but are they the right ones? Project director Louis Friedman puts it this way: "That the weak signals were recorded at the expected times of spacecraft passes over the ground stations is encouraging, but in no way are they conclusive enough for us to be sure that they came from Cosmos 1 working in orbit." The Russian space agency indicated that the Volna rocket may have had a problem during its first or second stage firing. "This," Friedman noted, "would almost certainly have prevented the...
Protoplanetary Disks Apparently Common
How can a planetary disk form in a region as chaotic as the Orion Nebula? Ponder the disruptive force of stellar winds in the range of two million miles per hour and temperatures above 18,000 degrees Fahrenheit. The assumption would naturally be that until a place like this settles down, material trying to form into a new solar system would simply be scattered into space. Not so, according to new findings from the Submillimeter Array (SMA), a telescope on Mauna Kea which works at millimeter and submillimeter wavelengths, and can therefore study interstellar material like gas, dust and small rocks the likes of which ultimately form planetary systems. SMA actually sees into dense interstellar clouds to examine the birthing process of stars. What the array has found is that protoplanetary disks are more tenacious than first thought. In fact, many of the objects called "proplyds" -- first seen by Hubble in the 1990s as silhouettes on the nebular background -- already have clustered...
Reflections on Cosmos 1
We're a little over a day from the Cosmos 1 solar sail launch, testing the technologies that may one day make travel within the inner Solar System faster and far more efficient. Centauri Dreams has discussed the involvement of Ann Druyan's Cosmos Studios; the documentary film and entertainment company put $4 million into the project, which is led by The Planetary Society. But it's also important to acknowledge the major Russian contribution, and not just in the Volna rocket that will launch the satellite, or the Russian submarine from which it will be fired. No, the Russian involvement is deeper still: the space firm NPO Lavochkin is behind much of the design of Cosmos 1, and the Russian Academy of Science's Space Research Institute is a major player. All told, Cosmos 1 is a case of trans-national collaboration, a fact emphasized by the scattering of team members around the globe as the launch approaches. The Planetary Society's Viktor Kerzhanovich is now in the Marshall Islands,...
Solar Sail Close to Launch
As we near launch, let's run through the Cosmos 1 sail mission again. The vehicle is privately funded (by Ann Druyan's Cosmos Studios and The Planetary Society), and will be launched aboard a converted Russian ICBM. Once in orbit, the spacecraft will deploy eight mylar sails. The principle is straightforward: Photons have no mass but they do carry momentum. As solar photons strike the sail blades, Cosmos 1's orbit should change, providing a test of solar sailing that can be measured from the ground. A later microwave beaming experiment may be able to measure the effect beamed propulsion has on the spacecraft, though the primary mission goal remains to test the principles of solar sailing by photons alone. Launch is now scheduled for June 21 from a submerged Russian submarine in the Barents Sea. The mission will be controlled from the Lavochkin Association in Moscow and assisted by a project operations center at The Planetary Society's headquarters in Pasadena. Everyone will be...
Harvesting Antimatter in Space
Two studies stand out in the list of Phase 1 awards recently announced by NASA's Institute for Advanced Concepts (NIAC). Gerald Jackson of Hbar Technologies (Chicago) will work on "Antimatter Harvesting in Space," while James Bickford of Draper Laboratory (Cambridge, MA) will study "Extraction of Antiparticles Concentrated in Planetary Magnetic Fields." Both offer solutions to the huge antimatter production problem that currently has us extracting tiny amounts at fantastic price from particle accelerators here on Earth. Jackson's is a familiar name. He and Steve Howe at Hbar are well known in the antimatter community as proponents of a fascinating and evidently feasible antimatter sail concept that would be energized by minute amounts of antihydrogen (see this earlier Centauri Dreams story). Jackson's new work on antimatter harvesting suggests taking antimatter collection into space, snaring antiprotons produced by the collision of cosmic rays with dust and solar wind protons. "Just...
Probing Red Dwarf Habitability
With exquisite timing, the SETI Institute has announced the first of a series of workshops to study the habitability of planets around M-class red dwarfs. The issue became highly visible recently with the announcement of the rocky planet discovered around the red dwarf Gliese 876, some 15 light years from Earth. Although thought to be too hot for life as we know it, the new planet is a solid world orbiting a main sequence star, raising the question of genuinely terrestrial worlds around such stars. 'Main sequence' refers to stars that burn hydrogen in their cores, those that show up in a well-defined band on the famous Hertzsprung-Russell (HR) diagram, which plots the intrinsic brightness of stars against their surface temperatures (intrinsic brightness is the observed brightness of the star corrected for distance). Moving off the main sequence takes you into the domain of red giants, red and yellow supergiants, and white dwarfs. But way down on the lower right of the HR diagram, and...
Correction on Red Dwarf Lifespans
Yesterday's post "On Red Dwarf Stars and the Hunt for Life" incorrectly stated the lifespan of an M-class red dwarf star as 100 times that of the Sun. The correct figure is ten times as long, making an age limit of perhaps 100 billion years for the average red dwarf. G-class stars like the Sun are expected to live about ten billion years. The red dwarf Gliese 876 is about 11 billion years old, more than twice the age of the Sun.
New Horizons on Schedule for Pluto/Charon
New Horizons, the doughty spacecraft soon to be sent to Pluto, Charon and on into the Kuiper Belt, has been shipped from its birthplace -- the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, MD -- to NASA's Goodard Space Flight Center in nearby Greenbelt. At Goddard, New Horizons will begin another round of pre-launch tests, with liftoff scheduled for next January. What I hear from people associated with this project is that New Horizons is ready to go. As mentioned here earlier, APL's David Dunham gave a talk about upcoming missions at the recent New Trends in Astrodynamics conference in Princeton. I had been concerned about the review process that New Horizons must undergo, required because it carries a radioisotope thermoelectric generator (RTG) that produces energy from fissionable materials. The final environmental impact statement produced by this process is due in the summer, with final NASA decision on the mission in the fall. But when I talked to him at...
On Red Dwarf Stars and the Hunt for Life
'Normal' is a tricky word when you're talking about extrasolar objects. As in 'normal star,' a phrase used during yesterday's news briefing about the new planet detected around Gliese 876, and in much of the press coverage since. The planet's low mass (about 5.9 times the mass of Earth) rules out the possibility that it is in any sense Jupiter-like, and the natural assumption is that this is a rocky world in a tight orbit around an M-class red dwarf.
Small, Rocky Exoplanet Discovered Around Nearby Star
Finding a planet that resembles the Earth is the ultimate goal of our exoplanetary explorations. It implies the possibility of life on a world not so different from our own, and encourages the speculation that Earth-like worlds are out there in huge numbers. We certainly haven't found such a place yet, but we're getting closer. Which is why Gliese 876, a red dwarf some 15 light years from our Solar System, made news today at a National Science Foundation briefing. No planet yet found -- and that includes roughly 155 extrasolar planets to date -- is as similar to Earth as the one found here. Gliese 876 is in the direction of the constellation Aquarius, and it is known to possess two larger gas-giant worlds as well as this much smaller neighbor. Not that conditions on the newfound world would be exactly habitable by our standards. The planet, some seven and a half times the mass of Earth, orbits its host star once every 1.94 days, and it's only two million miles from it (about...
New Exoplanet Findings Tomorrow Afternoon
We should have some interesting news about exoplanets tomorrow afternoon. That's when a media briefing will be given to reporters at the National Science Foundation in Arlington VA. The briefing is titled "Scientists Make New Discovery About Planets Outside Our Solar System," and although I have a hunch what this one is about, I'm not confident enough to run with it here. But it's intriguing that Jack Lissauer (NASA Ames), who is participating in the briefing, has done groundbreaking work on planetary formation in binary systems, as discussed in these pages back in December. Other participants in the briefing include exoplanetary pioneers Geoff Marcy (University of California, Berkeley) and Paul Butler (Carnegie Institution), as well as Eugenio Rivera from Lick Observatory. Rivera has previously worked with Lissauer on the 'resonant' orbits of two planets around the red dwarf Gliese 876, some 15 light years from Earth. Michael Turner, who heads NSF's Directorate of Mathematical and...
The Case for Helium-3
"Fusion reactors powered by deuterium/helium-3 are a good candidate for a very advanced spacecraft propulsion. The fuel has the highest energy-to-mass ratio of any substance found in nature, and, further, in space the vacuum the reaction needs to run can be had for free in any size desired. A rocket engine based upon controlled fusion could work simply by allowing the plasma to leak out of one end of the magnetic trap, adding ordinary hydrogen to the leaked plasma, and then directing the exhaust mixture away from the ship with a magnetic nozzle. The more hydrogen added, the higher the thrust (since you're adding mass to the flow), but the lower the exhaust velocity (because the added hydrogen tends to cool the flow a bit). For travel to the outer solar system, the exhaust would be over 95 percent ordinary hydrogen, and the exhaust velocity would be over 250 km/s (a specific impulse of 25,000 s, which compares quite well with the specific impulses of chemical or nuclear thermal...
An Ice Volcano on Titan?
By now, our outer Solar System probes have brought us so many surprises that finding yet another one should be passé. But it never is, and imagine the wonders we'll find, for example, when New Horizons arrives at Pluto/Charon and moves on to the Kuiper Belt beyond. Now Cassini has once again made news with the discovery of what may be described as an 'ice volcano.' The beauty of the concept is that it may explain the presence of atmospheric methane on Titan. "Before Cassini-Huygens, the most widely accepted explanation for the presence of methane in Titan's atmosphere was the presence of a methane-rich hydrocarbon ocean," said Dr. Christophe Sotin, distinguished visiting scientist at NASA's Jet Propulsion Laboratory, Pasadena, Calif. That otherworldly ocean was the most exotic of constructs, creating images of the Huygens lander bobbing about amidst frigid swells as its batteries failed. What the probe parachuted into was quite different. In a way, it's a shame to lose the...
Supernova Remnants and Star Formation
Apropos to our earlier discussion about shielding an interstellar probe comes this new image from the Hubble Space Telescope (click to enlarge). This chaotic and expanding mass of gas and dust, known as LMC N 63A, is the result of the explosion of a massive star. It's found in the N 63 region of the Large Magellanic Cloud, an irregular galaxy 160,000 light years from the Milky Way that is visible in the southern hemisphere. Numerous studies have been made of star formation and supernova remnants in this region. Imagine the shielding requirements that would be needed to penetrate such a active patch of sky! Fortunately, the interstellar medium is rarely so dense, but images like these remind us that space is anything but empty. Instead, it houses to a greater or lesser extent gas and dust particles that have to be reckoned with. We've also looked recently at the growing evidence that Voyager 1 is at the edge of the heliosphere, that 'bubble' of relatively clear space blown by the...
Astrodynamics at Princeton
Ed Belbruno did a terrific job putting together the New Trends in Astrodynamics and Applications II conference, from which I returned yesterday. I chose to drive to Princeton because of my growing aversion to airline travel. It was a long but generally uneventful drive except for the usual delays around Washington DC -- over an hour to clear the Beltway because of construction on one of the access ramps. But driving through western New Jersey is, as anyone who has done it knows, a pleasant experience, beautiful farmlands giving way to small villages here and there, with Princeton itself an oasis of lovely architecture, fine restaurants and, of course, a great university. About the only thing that didn't cooperate was the weather -- we had a chill rain for the first two days -- but Peyton Hall is about half a mile from the Nassau Inn, Princeton's fine colonial-era hostelry, and it was an energizing walk even with umbrella. The conference sessions were intense; we generally ran from...
Getting Ready for Deep Impact
Deep Impact's arrival at Comet Tempel 1 should be spectacular. Due to reach the comet on July 4 of this year, the two-part probe will launch a 360 kg impactor designed to produce a crater on the comet's nucleus and a plume of gas and dust. Getting inside a comet is a key mission goal: the ejected material should tell us much about the early days of the Solar System. Right now astronomers are engaged in making baseline observations through Earth-based telescopes to characterize Tempel 1 as completely as possible. By examining its albedo (reflectivity), rotation period and size, the mission team will be able to differentiate between impact effects and the natural activity of the comet during the Deep Impact encounter. The photograph on the right (click to enlarge) shows an image of Tempel 1 together with a number of visual artifacts. What has happened here is that images were taken through various filters, one after the other. The motion of the comet against background objects accounts...
New Trends in Astrodynamics
Centauri Dreams will be in Princeton over the weekend for the New Trends in Astrodynamics conference (Web site here). Topics are to range from upcoming missions to low-energy trajectories (a specialty of conference organizer Edward Belbruno) and near-Earth object impact projections. Among the papers targeting advanced propulsion technologies: Gregory Matloff, "Phobos/Diemos Sample Return via Solar Sail" Marc Millis, "Assessing Potential Propulsion Breakthroughs" Edgar Choueiri, "Advanced Propulsion Concepts for High-Energy Space Exploration Missions" I will be presenting "The Interstellar Conundrum: A Survey of Concepts and Proposed Solutions." And it will be wonderful to have the chance to talk to two Italian theorists, Giancarlo Genta (Politecnico di Torino) and Claudio Maccone (Alenia Spazio), whose work I have long admired. It should be a rich and full weekend, busy enough to require a brief suspension of postings here. Centauri Dreams will resume its normal publication schedule...
Inside the Carina Nebula
Panoramas this stunning deserve a lingering look (and be sure to click the image for a higher resolution view). You're looking at more of the fruits of the Spitzer Space Telescope's remarkable labors, this time a false-color image showing a part of the star-forming region known as the Carina Nebula. Using infrared, Spitzer was able to penetrate the so-called 'South Pillar' region of the nebula to reveal yellow and white stars in their infancy, wrapped up inside pillars of thick pink dust. The hottest gases here are green; the foreground stars are blue, which shows up better in the enlargement. And note the bright area at the top of the frame, which is what this story is all about. The glow is caused by the massive star Eta Carinae, which is too bright to be observed by infrared telescopes. Stellar winds and ultraviolet radiation from this star are what have torn the gas cloud, leaving the tendrils and pillars visible here. It is this 'shredding' process that triggers the birth of the...
Microwave Beaming and the Cosmos Sail
We're closing in on the launch of the Cosmos 1 solar sail, the first free-flying spacecraft to be powered by the momentum of solar photons. Yes, there have been deployment experiments before this, such as the Russian Znamya missions and the Japanese deployment of a thin film just last summer. But Cosmos 1 will be a functioning spacecraft capable of returning data, and its launch thus marks an important first in sail development. The launch window opens on June 21. The spacecraft is to be launched into a near polar and circular 800 kilometer orbit, with sail deployment four days later. Cosmos 1 has been moved from the test facility in Moscow to Severomorsk; the plan calls for it to be launched by a converted Russian ICBM from a submerged submarine. If successful, the mission will be a landmark not only for sail propulsion but also for commercial space development. The vehicle was funded by Cosmos Studios, with donations from members of the Planetary Society, whose latest update on the...