Measuring the Pioneer Anomaly

The so-called 'Pioneer Effect' continues to trigger study. Both Pioneer 10 and 11, as discussed in these pages back in November, have shown changes in their expected trajectories since they moved 20 AU beyond the Sun. In fact, since 1980 radio signals from the Pioneers have been slowly shifting to shorter wavelengths, which seems to imply a slight but interesting deceleration. This has led to at least one proposal for a mission to investigate the Pioneer effect. Both Galileo and Ulysses data have been examined for evidence of a similar effect; while Galileo's data were too limited for use, Ulysses did show a provocative, though extremely slight, change to its own acceleration (though at a much smaller distance from the Sun). Now a new paper notes the difficulties in measuring the Pioneer anomaly, and discusses a way of using asteroids and comets to measure gravitational effects in the outer Solar System. The paper is by computer scientists Gary Page and John Wallin (George Mason...

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Oort Cloud Explorer: Fast Mission to the Comets

How do you build an interstellar solar sail? Back in the 1980s, two studies of sail design set parameters that before then had remained largely unanalyzed. Gregory Matloff and Eugene Mallove were able to show in their papers "Solar Sail Starships: Clipper Ships of the Galaxy" and the later "The Interstellar Solar Sail: Optimization and Further Analysis," that a so-called 'sundiver' trajectory coud produce exit velocities from the Solar System on the order of 1000 kilometers per second, even for large payloads. Both papers appeared in the Journal of the British Interplanetary Society, which remains the leading venue for interstellar studies. A sundiver maneuver is tricky stuff; the spacecraft is established on a hyperbolic solar orbit that swings close to the Sun; at perihelion (closest approach), the sail is exposed to sunlight (having, perhaps, been shielded until now by an occulting object, such as a small asteroid). Make the sail reflective enough and the accompanying linkages to...

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Shielding an Interstellar Probe

Project Daedalus, a probe to Barnard's Star that was the first complete design study of a starship, included among its other innovations a dust shield made of beryllium. Driven by a nuclear-pulse engine using internal confinement fusion, Daedalus was so large that its 50 ton shield (nine millimeters thick over a radius of 32 meters) represented only a fraction of its enormous payload. But it was a critical part of the design. For the Daedalus team realized that at 12 percent of the speed of light, an encounter with even a tiny object could destroy their vehicle. Working in the 1970's and made up of members of the British Interplanetary Society, the starship designers knew that most of the interstellar medium is gaseous, primarily hydrogen and about 25 percent helium. Dust is rare, no more than one dust particle for every trillion atoms, but the faster a spacecraft moves, the more stray protons and electrons it will encounter. At a significant percentage of the speed of light, such...

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European Space Agency Eyes Europa

With the Jupiter Icy Moons Orbiter (JIMO) on hold, NASA is talking to the European Space Agency about a possible joint mission to Europa. A BBC story reports that a prime driver for ESA is the need to use radioisotope thermal generators (RTGs) on the mission, a power source with which the Europeans have little experience. RTGs are needed on missions to the outer planets because they increase the power available to the spacecraft, allowing for a wider range of experiments with more sophisticated instruments. Solar panels remain an option in Jupiter space, but aren't nearly as effective. The other driver, of course, is the recent success of the Cassini/Huygens combined mission, whose stunning images of the Saturnian system and data from the Titan descent and landing have many scientists now thinking of Europa. The moon's cracked ice seems to have been shaped by tidal forces from Jupiter, with reason to believe that an ocean of liquid water might be found beneath an ice crust tens of...

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Pluto/Charon Mission Taking Shape

January 11 to February 14, 2006 marks the launch window for NASA's New Horizons mission to Pluto and the Kuiper Belt. At the moment, New Horizons is in pieces, or as principal investigator Alan Stern puts it in an update on the mission, it's in "...boards, boxes and a spacecraft bus on the cleanroom floor at the Johns Hopkins Applied Physics Laboratory..." The high-gain antenna is being checked, and the main computer system installed. According to Stern: The bird also received a guidance, navigation and control software load, and the first testing of the autonomy system (that provides for fault protection) has taken place. Coming soon to the spacecraft are the redundant flight computer, the gyros and the Ralph remote-sensing package. We are now approaching the time - only weeks away - when the last avionics box goes on the spacecraft and New Horizons is dressed in thermal blankets for environmental testing in a large vacuum chamber at NASA Goddard Space Flight Center. New Horizons...

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Voyager Interstellar Mission in Jeopardy

Nature is reporting that the two Voyager missions -- recently discussed here as our first active probes of the interstellar medium, if they live long enough to cross the heliospheric boundary -- may be terminated in October. The decision is not yet final, and there is always the hope that it will spur enough reaction among space scientists and others to force a reprieve. But if these missions end (along with six others, including Ulysses), the loss to science would be severe. Voyager 1 is the fastest man-made object, now leaving the Sun behind at over 17 kilometers per second, at a current distance of approximately 94 AU (14 billion kilometers from Earth). Voyager 2 is roughly 76 AU out. Both spacecraft should be able to continue transmitting until 2020 or later. At $4.2 million per year, the Voyager program catches NASA's eye as the agency ponders budgetary cutbacks. But to shut down two operational spacecraft as they approach the interstellar medium for the first time in history is...

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Charting the Boundaries of the Heliosphere

Has Voyager 1 left the heliosphere? The question is a reminder that the Voyagers are our first interstellar probes; they'll still be returning data when they move into the interstellar medium. The heliosphere is a kind of bubble created by the solar wind from the Sun, that stream of high-speed charged particles constantly blowing into space at roughly 400 kilometers per second. Observing how Voyager 1 makes the transition across the boundary of the heliosphere will provide our first in situ study of interstellar space. Some scientists believe that at roughly 90 AU from the Sun, Voyager 1 has already pushed up against the 'termination shock,' that region where the speed of the solar wind drops to subsonic levels. Now new data studied by French and Finnish researchers indicate that the shape of the heliosphere may be distorted, further complicating the question of just where the true interstellar medium begins. Rosine Lallement and colleagues used data collected by the Solar and...

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A Quote for the Weekend

"It was only a few centuries ago that people began to realize that those points of light in the night sky were suns, like our Sun, and like our Sun, they might have planets around them. Many visionaries then dreamed and wrote of visiting those other planets in ships that traveled between the stars. Later, when astronomers were able to estimate the distance to the nearer stars, others concluded that, because interstellar distances were so immense and human life so short, interstellar travel was impossible. "Travel to the stars will be difficult and expensive. It will take decades of time, gigawatts of power, kilograms of energy and trillions of dollars. Recently, however, some new technologies have emerged and are under development for other purposes, that show promise of providing propulsion systems that will make interstellar travel feasible within the forseeable future -- if the world community decides to direct its energies and resources in that direction. Make no mistake --...

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Interstellar Boundary Explorer Chosen by NASA

Our first interstellar mission won't be a long jump to Alpha Centauri or Barnard's Star. In fact, we've already launched not one but several interstellar missions -- the two Pioneer probes, and the two Voyagers that followed them, will all exit the Solar System; i.e., they will eventually cross the boundaries of the heliosphere to emerge into pure interstellar space. Some scientists believe that Voyager 1 is already pushing up against the so-called 'termination shock,' where the speed of the solar wind of gas and charged particles from the Sun drops to subsonic levels. But we need far more information than the Voyagers, with their rapidly fading signals, can tell us. The next mission designed to explore the outer limits of the Sun's influence will be the Interstellar Boundary Explorer (IBEX). Under development at Southwest Research Institute, IBEX is designed to explore how the solar wind interacts with the interstellar medium through which our entire Solar System moves. IBEX won't...

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Kepler and the Search for Terrestrial Worlds

In Finding Other Worlds, Edna DeVore of the SETI Institute zeroes in on the importance of the Kepler Mission. Scheduled for an October 2007 launch, Kepler is likely to discover hundreds of extrasolar planets. And as DeVore writes, "Kepler is the first observatory capable of finding Earth-size worlds in the habitable zone of distant Suns. In other words, Kepler may find 'good places to live.'" Some key points about Kepler: To find planets, the mission will use the transit method, looking for the dimming of a star caused by repeated transits of a planet across its face. The size of a planet can be calculated from changes in the star's brightness, and the size of its orbit can be measured. The parameters of the mission are the most challenging ever attempted for extrasolar detection. Kepler is designed to survey nearby stars to determine how often terrestrial and larger planets occur in the habitable zone of different types of star. This, in turn, will allow the follow-on Space...

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Looking Back at Project Orion

"'I think there is absolutely no doubt -- and we did some experiments later; still quasi-classified, related to Casaba-Howitzer -- that the propulsion system would have worked. We knew what we were doing in designing it. We could send 85 percent of the momentum in one direction that we wanted it to go in, and there were enough experiments -- and there have been enough experiments -- done on the protection of the pusher plate, to have no doubt that it would have worked. Between those two things there is a tremendous amount of engineering detail to be worked out, but I think it was engineering detail. It could have worked. Now, could it have been done economically, could it have been done in time? Those were all different questions, but I think all of those things could have been solved. Today, people ask me, 'Was it really a joke, Pyatt, or was it serious?' It was dead serious. If we wanted to do it, if there were any good reason for wanting to have high specific impulse and high...

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Aerocapture: A Spectacular, Flaming Arrival

The nuclear-electric mission to Neptune discussed here on the 14th is one of two now being studied by NASA. The other is powered by chemical rockets and, like Cassini, would use gravity assists to reach Neptune in considerably less time. Its team, led by Andrew Ingersoll of the California Institute of Technology, is working on a design that, like University of Idaho professor David Atkinson's nuclear-electric mission, will be submitted to NASA in mid-2005. A faster mission has many advantages, but a major question arises: how do you stop when you get there? Unlike Voyager, the Neptune missions are to be capable of orbiting the planet and dispatching probes to both it and its largest moon, Triton. One answer Ingersoll's team is studying is aerocapture, which uses the destination planet's atmosphere to alter the spacecraft's trajectory, putting it into orbit after a single pass. If this sounds familiar, you may recall the aerocapture maneuver in the film 2010, a spectacular, flaming...

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Tracking Near-Earth Asteroids

An asteroid called 2004 TP1 came within 13 LD of Earth on November 2 -- LD stands for 'lunar distance,' and is the average distance between the Earth and the Moon (238,855 miles, or 384,401 kilometers). Asteroid 2004 RZ164 will come even closer, at 7 LD on December 8. Both objects are considered Potentially Hazardous Asteroids (PHAs, as acronym-obsessed scientists like to call them). That means they are larger than 100 meters in diameter and come too close to Earth for comfort. 653 Potentially Hazardous Asteroids are now known. We've discussed such objects as perhaps the most significant reason for building up a space-based infrastructure that could ward off a potential strike. A good place to track them is the NASA-sponsored site Spaceweather.com, which bills itself as 'News and Information about the Sun-Earth Environment.' The site likewise tracks solar wind conditions (currently moving at 493.7 kilometers per second, based on data transmitted from the Advanced Composition Explorer...

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An Anomaly from the Edge of the Solar System

Those of us with still fresh memories of Voyager 2's encounter with Neptune in 1989 find it gratifying that both Voyager probes are still returning good science. It's even more remarkable that the Pioneer 10 and 11 probes are still in the thick of things, but anomalies in their journeys beyond the orbit of Pluto offer tantalizing clues of some unexplained phenomenon in the far ranges of the Solar System. As this article in Nature points out, since 1980 the Pioneers have been returning radio signals that have kept shifting to shorter and shorter wavelengths. The implication: both spacecraft are decelerating, even if only by the slightest amount. Some are calling this the 'Pioneer anomaly,' and it may just point to a new principle in physics, perhaps involving exotic forces or undiscovered forms of matter. On the other hand, it may have a much more mundane explanation, such as a fuel leak that could be affecting the probes' progress. Either way, engineers faced with designing...

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Cassini and the Kuiper Belt

When it comes to interstellar work, don't forget the Kuiper Belt. Although amateur astronomer Kenneth Edgeworth was the first to predict its existence, the Belt was named for Gerard Kuiper, who analyzed it in 1951. It is a region of thousands (and perhaps millions) of small, icy moons and cometary debris that exists from the orbit of Neptune well into deep space. Our first interstellar missions will be explorations of this area and the vast Oort cloud of comets that may extend as much as a light year out from the Sun. And yes, in a true sense, the Voyager probes could be considered interstellar missions, still reporting data as they move on toward the heliopause. But we may learn a good deal about Kuiper Belt objects by studying the findings of a spacecraft considerably closer, the Cassini Saturn orbiter. Cassini's Ultraviolet Imaging Spectrometer tells us that Phoebe, a tiny world about one-fifteenth the diameter of Earth's moon, is probably itself a Kuiper Belt object that was...

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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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Jupiter Icy Moons Orbiter

NASA has just announced that it has selected Northrop Grumman Space Technology as the contractor for co-designing its proposed Jupiter Icy Moons Orbiter. JIMO will be designed to orbit and explore three of the most interesting Jovian moons: Callisto, Ganymede and Europa. All three may possess water, organic material and a source of energy, leading to the possibility of some form of life evolving there. Image: The surface of Europa as seen by the Galileo orbiter. Note the crustal blocks on the left that seem to have once broken apart, and then 'rafted' into their current positions. They're evidence of what may be a sub-surface ocean. Credit: Planetary Image Research Laboratory, University of Arizona. Studying these moons closely will involve long periods in orbit around each before moving on to the next target. The propulsion system envisioned here is nuclear electric. NASA's Deep Space 1 spacecraft has already demonstrated the principle, in which electrically charged particles are...

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Jupiter Icy Moons Orbiter: Reactor Options

Worth noting in relation to the JIMO story above (and for the broader issue of generating power for deep space probes): "A Power Conversion Concept for the Jupiter Icy Moons Orbiter," by Lee S. Mason (Journal of Propulsion and Power Vol. 20 No. 5, 1 September 2004, pp. 902-910). From the abstract: "An analytical study was performed to compare design options for a reactor power system that could be utilized on a Jupiter Icy Moons Orbiter mission employing nuclear electric propulsion."

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More Power for Deep Space Missions

Scottish minister Robert Stirling developed an engine in the 19th Century that used heated air instead of steam as the motive force for a piston engine. Now an acoustical version of the principle has emerged. As described in an article in a recent issue of Applied Physics Letters, a joint team from Los Alamos National Laboratory and Northrop Grumman Space Technology have created TASHE -- the "thermoacoustic-Stirling heat engine." The work of LANL scientist Scott Backhaus and Emanuel Tward and Mike Petach from Northrop Grumman, TASHE would be used to generate electricity aboard spacecraft, and would be quite a step up from the thermoelectric devices now used, which convert roughly 7 percent of their heat energy into electricity using heat from the decay of a radioactive fuel. By contrast, TASHE converts up to 18 percent of its heat source energy into usable electricity. The expansion of helium gas inside the engine drives the process, as described in a recent issue of Physics News...

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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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