Hayabusa in the Shadows

The Japanese Hayabusa spacecraft has always seemed to have a couple of strikes against it, at least in terms of media coverage. Never much in the spotlight, the ambitious attempt to explore and bring back samples from the asteroid Itokawa has been all but eclipsed by China's recent manned orbital ventures. And Centauri Dreams suspects that's a primary problem: robotic missions don't draw the public eye the way risky manned flights do, even if the scientific payback from the former is often immeasurably greater. Now Hayabusa is encountering a different set of problems. The Minerva robot was to have landed on Itokawa last week, but disappeared after its release. A lower profile issue has been solar flare damage to the spacecraft's solar panels and continuing problems with its positioning control system. And now we have word of a mission-endangering glitch: Hayabusa failed to touch down on the tiny asteroid when the attempt was made on Sunday. "I don't think it landed," project leader...

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Tracking the Falcon

Centauri Dreams focuses on the long-term, which almost always means deep space missions and interstellar possibilities. But building an industrial infrastructure in the outer Solar System also means finding much less expensive ways into space, a fact illuminated by the upcoming launch of SpaceX's Falcon rocket from Kwajalein atoll in the Pacific. CEO Elon Musk talks about building the 'Ford of space,' and as noted by Michael Belfiore, Musk went on to say this in a personal interview: "Ford didn't invent the internal combustion engine. But he found out how to make one at low cost." Similarly, "We didn't invent the rocket engine; what we're trying to do is figure out how to make it low-cost." Belfiore's weblog is a good place to monitor as we approach launch, which is set to occur at 1300 PST on November 25. Also be aware of Jim White's postings from Kwajalein; White is a member of the FalconSAT-2 satellite team and is reporting on final preparations. Finally, Jeff Foust provides...

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Photon Pressure Affects Japanese Spacecraft

The Japanese spacecraft Hayabusa, now in a 'parking orbit' above the asteroid Itokawa, is providing good evidence of just how useful the pressure of solar photons can be. Japan's Institute of Space and Aeronautical Science (ISAS) reports that the force being experienced by the spacecraft is 1/100th of the thrust produced by its ion engines, but fully ten times larger than the gravity of Itokawa itself. The effect is consequential enough that it must be factored into Hayabusa's descent close to Itokawa's surface; the spacecraft will deploy a small surface 'hopper' called MINERVA to take measurements on the asteroid. Hayabusa (once known as MUSES-C and renamed for a Japanese rocket pioneer) thus becomes both a testbed for current technologies and a reminder of a future one. Its electric propulsion or ion drive engines have met the challenge of asteroid rendezvous, although their performance was degraded by solar panel damage from solar flares in 2003. The spacecraft also carries an...

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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...

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Plasma Propulsion Under Scrutiny at MSFC

A team of NASA and university-based investigators is studying the physics of magnetic nozzles, devices that could be used in plasma-based propulsion systems that would sharply reduce the length of journeys within the Solar System. The project began in April and is led by the University of Texas, with support from Marshall Space Flight Center in Huntsville (AL), along with the University of Alabama at Huntsville and NASA's Johnson Space Center in Houston. "The technology we're pursuing could play an important role in NASA's exploration of the Moon, Mars and the rest of the Solar System," said Dr. Greg Chavers, a plasma physicist at Marshall and co-investigator for the new project. "Magnetic nozzles enable a new type of plasma-based propulsion system that could significantly reduce travel times to different planetary destinations, providing a new means of exploring space." Plasma forms when a hot gas is ionized, causing the atoms to lose their electrons and take on a positive charge....

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The Roadmap to Epsilon Eridani

Sending a probe to another star would be NASA's greatest adventure, but how do we lay the groundwork for such a mission? The agency likes 'roadmaps,' spelling out clear and specific objectives and beginning with missions not so far beyond those we could fly today. NASA's Interstellar Probe Science and Technology Definition Team (IPSTDT) recently prepared studies on a solar sail mission into nearby interstellar space, reaching approximately 400 AU from the Sun in 20 years of flight time. Think of it as a logical follow-on to the Voyager probes. But Ralph McNutt and colleagues at Johns Hopkins' Applied Physics Laboratory have been defining a more ambitious mission. As worked out in several recent papers, McNutt's probe would approach the Sun to within 4 solar radii before a fifteen minute engine burn would establish its high-speed escape trajectory from the Solar System. At this point all acceleration would end; unlike the IPSTDT design, no sail would be deployed. The McNutt mission...

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Plasma in a Bubble

Sonoluminescence -- the emission of light from bubbles in a liquid that has been excited by sound -- is a mystery. How does a sound wave put enough energy into such a small volume as to cause light to be emitted? The concentration of energy needed is something like a factor of one trillion, according to this Los Alamos National Laboratory introduction to the phenomenon. And not only that; the spectrum of the emitted light implies extremely high temperatures. Fusion, anyone? Well, not yet. But the slang term for sonoluminescence, 'star in a jar,' seems a little closer to reality now that the first direct measurements of the phenomenon are in. They show that the temperature inside a collapsing bubble can reach 20,000 degrees Kelvin, which is four times the temperature of the surface of the Sun. This work, by Ken Suslick and David Flannigan (University of Illinois at Urbana-Champaign), comes two years after controversial findings by an Oak Ridge National Laboratory team that found...

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Continuing Success for Ion Thrusters

The Japan Aerospace Exploration Agency's Hayabusa spacecraft (formerly known as MUSES-C) is demonstrating the advantages of ion propulsion in its mission to land on the asteroid Itokawa and return samples of its surface to Earth in 2007. When it performed an Earth flyby in May, Hayabusa became the first spacecraft to accomplish such a maneuver using an ion engine as its main thruster. In cruise mode, the craft's four ion engines were designed to burn throughout the flight. JAXA's recent announcement that Hayabusa's engines had marked 20,000 hours of 'accumulated operational time' points out the ion advantage: the spacecraft's engines consumed a mere 20 kilograms of propellant during that time. You can see the JAXA news release here. Ion engines operate continuously for long periods because their thrust levels are low, but their high efficiency makes them ideal for deep space missions. Hayabusa uses ionized xenon gas sent through a strong magnetic field and expelled at high speed as...

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The NEXT Generation of Ion Propulsion

Can ion propulsion really lead the way to the outer planets? No one can know for sure, but recent advances in solar-electric propulsion surely make ion methods a prime candidate. Not only has SMART-1 conducted a thorough ion engine shakedown on its lengthy and circuitious route to the Moon, but a variety of new studies are showing the way to more powerful ion thrusters that will eventually lead to the nuclear-electric systems we'll need for deep space missions. Today's standard ion engine is called NSTAR (it's a short acronym for a long term: the NASA Solar Electric Propulsion Technology Application Readiness thruster). The agency used one of these on its highly successful Deep Space 1 mission. In tests at the Jet Propulsion Laboratory, an NSTAR thruster was operated for a continuous 30,352 hours. That's almost five years of operation for an engine whose design life was only 8,000 hours. You can read more about that test in this NASA news release (PDF warning). Image: This xenon ion...

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To the Peak of Eternal Light

It used to be said that the Sun never set on the British Empire. Those days may be long gone, but there is still a place where the Sun forever shines, and it's on the Moon. The Peak of Eternal Light is a mountain at the lunar south pole that is always in view of the Sun. Its year-round temperature is a comparatively mild (by lunar standards) -20C, making it possibly useful as a site for a future lunar base. The possibility of water ice in nearby craters, though not proven, could be an attractive bonus. No wonder the European Space Agency is fascinated with the Peak of Eternal Light. Fascinated enough to make it a prime survey target for SMART-1, the ion-powered spacecraft that entered lunar orbit on Monday. SMART-1's studies of the Moon's south pole will surely be fascinating, as will its look at the South Pole-Aitken Basin, a huge impact crater that punches deep into the Moon's mantle. At stake may be new theories about the Moon's formation. But for deep-space enthusiasts, the...

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Slingshot to the Outer Planets?

The conference of the Division for Planetary Sciences of the American Astronomical Society continues in Louisville. Among the papers presented at today's Advanced Propulsion session were three of particular interest for interstellar advocates. Les Johnson, who heads up NASA's In-Space Propulsion Technology Program, gave an overview on the technology portfolio now being examined. "Some of the most promising technologies for achieving these goals use the environment of space itself for energy and propulsion and are generically called, 'propellantless' because they do not require on-board fuel to achieve thrust," Johnson wrote in a precis of the talk. "Propellantless propulsion technologies include scientific innovations such as solar sails, electrodynamic and momentum transfer tethers, aeroassist, and aerocapture." Both solar sails and aerocapture are candidates for flight validation as early as 2008. Two other presentations of particular note: "Solar Sail Propulsion: A Simple,...

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Promising Fusion Concepts

Fusion is often in the picture when interstellar propulsion systems are discussed, but so far we don't know how to sustain the process past the breakeven point. Ongoing research is intensive, however, and the latest in inertial confinement fusion (ICF) concepts will be examined in mid-November in Savannah, GA. That's when the American Physical Society's Division of Plasma Physics holds its 46th annual meeting. Inertial confinement fusion works by heating and compressing tiny fuel capsules with laser beams. Significant advances have been reported from the University of Rochester's Laboratory for Laser Energetics, whose researchers will present the results of their tests of OMEGA, a 60-beam laser facility that is designed for the National Ignition Facility, a fusion laser facility scheduled to be completed later in the decade. Image: Inertial confinement fusion at the Trident laser facility at Los Alamos National Laboratory. Here is a description of ICF from Los Alamos National...

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SMART-1 Final Course Correction

Keep an eye on ESA's SMART-1 mission, which recently completed a four-hour burn of its ion engine to correct its trajectory to the Moon. The next engine burn, lasting 4.5 days, won't occur until November 15 when the craft has reached lunar orbit. The final operational orbit will be polar elliptical, ranging from 300 to 3,000 kilometres above the Moon's surface. SMART-1 will perform a six-month survey of chemical elements on the lunar surface by way of examining various theories on how the Moon originally formed. What's interesting about SMART-1, in addition to the exotic series of spiraling orbits it is using to reach the moon, is its solar-electric propulsion system. This device uses electricity (generated from sunlight through solar panels) to accelerate xenon ions through an electric grid at huge velocity. So-called 'ion engines' like this create low thrust, but their specific impulse (ISP) is high. Their efficiency means a spacecraft can carry less fuel and be outfitted with more...

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X Prize Attempt Live from the Cockpit

The X Prize Foundation says it will provide live streaming video from the cockpit of SpaceShipOne tomorrow morning as Scaled Composites makes its first bid for the X Prize. The second, and potentially winning attempt, is scheduled for October 4. Coverage begins here at 9 am ET.

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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).

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