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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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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