Commercializing VASIMR

It's heartening to see that NASA has inked an agreement with a commercial firm to get its VASIMR (Variable Specific Impulse Magnetoplasma Rocket) technology into the private sector. Houston-based Ad Astra Rocket Company is actually located within the Johnson Space Center and, under the direction of president and CEO Franklin Chang-Diaz, focuses on the development of plasma rocket technologies. Its agreement with NASA should further work on a design widely thought to offer powerful advances over conventional chemical rockets. Chang-Diaz is a veteran of seven Shuttle flights who retired from NASA last July to focus on the Ad Astra/VASIMR connection. The design, which he conceived back in 1979, uses magnetic fields to channel a plasma exhaust that would melt conventional rocket nozzles. An additional beauty of the concept is that both thrust and specific impulse can be varied during the course of a mission. Ad Astra compares this to the transmission in an automobile; the exhaust...

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A Black Hole Boost into Intergalactic Space

What would fling a star out of the galaxy at over 1 million miles per hour? Warren Brown (Harvard-Smithsonian Center for Astrophysics) and colleagues have some thoughts on that, based on their own and other studies in Europe that have so far identified five stellar exiles, a group now called 'hypervelocity stars.' "These stars literally are castaways," says Brown. "They have been thrown out of their home galaxy and set adrift in an ocean of intergalactic space." Brown's team went after galactic escapees in a targeted manner, using computer models that showed such stars would be forced into their current trajectories by interactions in the galactic core. The idea is this: a binary star swings too close to the black hole at the galaxy's center. Its gravity tears the duo apart, in the process capturing one of the stars and ejecting the other one at high velocity. Evidence exists not only in the exiled stars themselves but in the other half of the binary pairs that once contained them;...

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The Ultimate SETI Signal

Robert Carrigan (Fermi National Accelerator Laboratory) drew quite a bit of attention last summer when he suggested that SETI signals could contain harmful information, perhaps created by a so-called 'SETI hacker.' Carrigan's article has now appeared in Acta Astronautica, and it's stuffed with beguiling ideas even if you find the premise unlikely. "...will a SETI signal be altruistic, benign or malevolent?" Carrigan asks. "It would help to understand the motivations of a message before reading too much of it. Like Odysseus, we may have to stuff wax in the ears of our programmers and strap the chief astronomer to the receiving tower before she is allowed to listen to the song of the siren star." That's fascinating stuff, recalling Fred Hoyle's A for Andromeda and Carrigan's own The Siren Stars, written with Nancy Carrigan and serialized in Analog in 1970. But this new paper is worth reading for reasons other than the hacker hypothesis; its author speculates widely on SETI itself....

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Thoughts on Microlensing

Some further thoughts on OGLE-2005-BLG-390Lb, the planet whose discovery portends numerous microlensing breakthroughs to come. Note the distance between the Sun and the red dwarf in question, which is variously reported as between 20,000 and 28,000 light years. The red dwarf is in the constellation Sagittarius and lined up between us and the center of the galaxy, a location that is a natural consequence of the microlensing method used to find the new world. For microlensing relies upon a closer star passing in front of one farther away, thus causing the gravitational effects used to pinpoint OGLE-2005-BLG-390Lb. To maximize the chances of seeing such an event, you need to point toward the largest possible field of stars, which is exactly what the OGLE project does. OGLE stands for Optical Gravitational Lensing Experiment, a study whose telescopes scan the central Milky Way each night. The scans are fruitful, for more than 500 microlensing events are discovered every year. Bear in...

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Rocky World Discovered Through Microlensing

The most Earth-like planet yet found has been discovered by a team of astronomers in a collaborative effort that involved 73 scientists in 12 countries. When astronomers use the term 'Earth-like' in this context, they're referring to planets whose mass is closer to Earth's than previous discoveries. They're also talking about surface conditions, for OGLE-2005-BLG-390Lb seems to have a rocky surface, and is only five times as massive as Earth. And what a fascinating find from the standpoint of technique. This is no relatively nearby gas giant found through observing the radial velocity changes it caused in its star's path through space. Instead, the new world, some 20,000 light years away, was found through microlensing, where the gravity of an intervening star magnifies the light of a more distant star. Close study of the brightening phenomenon can reveal defects that are the telltale sign of a companion object. In this case, as the star and its planet passed in front of the...

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Speaking Across Time and Space

Science writer Larry Klaes wrote last November with a thought about New Horizons that I've been pondering ever since. Klaes was troubled to learn that the spacecraft -- just the fifth mission ever launched that will eventually leave the Solar System -- was carrying little that could communicate information about its makers. Its major relic was a CD disc with signatures collected from those who signed up at a Web site, along with an image of the mission team. Klaes added that the CD would itself would be rendered unreadable within decades or, at most, a few centuries. Noting that the European Space Agency had included samples of 1000 human languages on its Rosetta comet probe, Klaes went on to say, "I think this is why an independent committee should be formed working with NASA and any other space agency that plans to launch probes into interstellar space to create messages/info carriers for those future vessels. This may help to avoid giving the mission teams any extra issues beyond...

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Solar Sail NEA Missions Proposed

If we chose to launch an interstellar probe using near-term technologies, it would almost surely be a solar sail, unfurled on a close approach to the Sun and flung outward at speeds that could get it to Alpha Centauri in perhaps 1000 years. That's the thinking of Gregory Matloff, author of Deep Space Probes: To the Outer Solar System and Beyond (Springer, 2005) and a leading proponent of interstellar studies. Later technologies might also use sails, driven by laser or microwave or even particle beams. But as we take incremental steps toward an interstellar future, solar sails have to be developed first. On that score, it's interesting to note the contributions of the Deutschen Zentrum für Luft- und Raumfahrt (DLR), Germany's aerospace research center and space agency. An early consolidation of sail studies, for example, came from a joint NASA/DLR feasibility study conducted in 1996-97. The working group recommended a demonstration mission that could help develop the basic principles...

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Toward a Self-Healing Spacecraft

Self-repair in spacecraft has always been a fascinating subject, one that comes to the fore as we launch missions to the outer Solar System. It's one thing to send commands to fix a stuck tape recorder, as was done with Galileo on the approach to Jupiter in 1995. In that situation, controllers worked with a 40-minute time lag -- eighty minutes for each confirmation that a command had been executed. But what happens if something goes awry in the Kuiper Belt, or the Oort Cloud, or a third of the way to Alpha Centauri? Clearly, probes beyond our Solar System will have to rely heavily on advances in robotics and autonomous computing that allow them to diagnose and fix their own problems. But they'll also have to make use of self-healing materials that can repair damage caused by temperature variations and external collisions. Small cracks caused by micrometeorites, for example, could weaken the spacecraft as they accumulate over the course of a long mission. But how about healing such...

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Lasers and Deep Space Communications

All but lost in the recent news of the Stardust sample return and New Horizons launch, the Messenger spacecraft continues on its journey to Mercury. And significant science has already occurred, particularly the laser link set up across a record 24 million kilometers (15 million miles) between the spacecraft and Earth. Laser communications with spacecraft are still in their infancy, but this test showed the potential of moving past microwaves into far more effective laser channels. The beauty of a laser signal is that it spreads much more slowly than conventional radio signals, a huge factor given the need to return significant data at maximum speed. Consider this: the Mars Pathfinder mission returned a radio signal that spread to hundreds of times the diameter of the Earth by the time it reached us. The 23-watt signal of the distant Voyagers broadcasts a beam now a thousand times the Earth's diameter. These numbers play havoc with signal strength. Voyager's signal to Earth during...

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A News Conference and a Launch

This is shaping up to be a busy day, starting with good news from the Stardust mission. Having opened the sample return capsule at Johnson Space Center in Houston, the science team found that the sample tray held numerous particles captured not only from comet Wild 2 but interstellar particles collected during the missions' seven year journey. Stardust principal investigator Donald Brownlee said it all: "The collection of cometary particles has exceeded our expectations. We were absolutely thrilled to see thousands of impacts on the aerogel." Coming up at 1100 EST (1600 GMT) is a news conference held by Stardust team members in Houston, with coverage on NASA TV (and I notice that NASA will offer video of the opening of the Stardust cannister at 1500 EST today). Also imminent is another attempt to launch New Horizons, now scheduled for 1308 EST (1808 GMT), and available both through NASA TV and useful pages like the ELV Countdown Portal at Kennedy Space Center. The New Horizons launch...

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A Wish for New Horizons

Yesterday's brief and unplanned exercise in 'liveblogging' was caused by an odd discovery: the only way for this observer to track the New Horizons launch was through the Internet. With over 200 channels available through cable television, I found that channel surfing through all of them yielded not one with live NASA coverage. Now ponder this. Centauri Dreams is based near North Carolina's Research Triangle Park, with three major universities within easy driving distance. The woods are full of PhDs, the area priding itself on high tech. With all these resources, there was not a single cable channel that could be devoted to the first mission to Pluto/Charon ever launched. You can imagine what kind of fare was available on many of the channels that were available. Around the same time, I also noted the slowdown in NASA servers as the launch progressed and received e-mails from people who were having trouble accessing NASA TV. Thus the attempt to post updates on the launch holds...

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New Horizons Launch Aborted

Centauri Dreams is not conceived as a streaming news site, but the NASA servers are slammed, so I'll update as needed until we get New Horizons off the ground. Update times are GMT (subtract 5 for EST). Update: 2022 Launch abort, with at least a 24-hour turnaround. Launch now scheduled for tomorrow at 1816 GMT (1316 EST). 2019: Countdown resumes at T-4 minutes. 2001: Launch now re-scheduled for 2023 GMT (1523 EST). We're nearing the outer edge of today's launch envelope. Ground-level winds are now problematic. 1950: Upper level winds remain a concern although launch is still set for 2005 GMT (1505 EST). No technical issues with the Atlas V; the problem is solely meteorological at this point. 1946: Launch time now set for 2005 GMT (1505 EST), due to a problem with the Deep Space Network that has now been resolved. An earlier delay had been caused by upper level winds. ----------- All eyes are on Launch Complex 41 this morning, and on the clock. The New Horizons launch is scheduled for...

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New Studies of Dark Matter

Catching up on news from the recently concluded American Astronomical Society meeting, I want to be sure to mention RAVE -- the Radial Velocity Experiment -- which is an all-sky spectroscopic survey of as many as a million stars passing near the Sun. Observations of stars in other galaxies show that only dark matter can explain their movement since there is not enough visible mass to keep them gravitationally bound. Early results from RAVE confirm that dark matter dominates the mass of the Milky Way as well. The survey will help to firm up our picture of the Milky Way's own dark matter and, by extension, its mass. "One important early application of RAVE aims to measure just how much stuff there is in our Milky Way galaxy — the collection of stars, gas and dark matter that is the home of our sun," said Rosemary Wyse (Johns Hopkins). "Newton's Law of Gravity allows us to figure out from the orbital motions of stars how much mass is holding them together. Faster motions need more...

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Of Missions and Deep Time

The successful return of the Stardust samples offers a chance to study cometary materials up close, surely deepening our understanding of the origins of the Solar System. But it also serves as a reminder of the time frames in which deep space missions must be flown. At that, Stardust has been a relatively swift mission, traveling some 2.88 billion miles in a seven-year journey. But ten years of planning also went into that journey, and design work goes back over 20 years. Thus Don Brownlee's comment on the mission's origin. "I have been waiting for this day since the early 1980s when Deputy Principal Investigator Dr. Peter Tsou of JPL and I designed a mission to collect comet dust," said Dr. Brownlee. "To see the capsule safely back on its home planet is a thrilling accomplishment." As well it must be, for Brownlee (University of Washington, Seattle) is principal investigator for the entire Stardust mission. Now thoughts turn to New Horizons, just over a day from launch. Scheduled to...

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Stardust Update

The return capsule from the Stardust probe landed successfully in the Utah desert at 1012 GMT. More on Monday; for now, this BBC story contains the details, and provides video of the landing. From the story: "'I'm very confident we will have samples in there that are the first returned from beyond the Moon,' former Stardust project manager, Ken Atkins, told the BBC News website." Well done!

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Stardust Just Hours from Earth

The Stardust spacecraft crossed the Moon's orbit at 1730 GMT on Saturday and will close the distance to Earth in sixteen and a half hours (an indication of how fast the vehicle is moving). The craft performed a final burn for course adjustment before passing the Moon's orbit. Approaching the Earth, it will deploy its return capsule for a scheduled landing at the Utah Test and Training Range on Sunday (the primary spacecraft will enter a Solar orbit after release). The capsule is scheduled to enter Earth's atmosphere over northern California at an altitude of 125 kilometers, traveling some 46,440 kilometers per hour (28,860 miles per hour). This is the fastest return of any man-made object on record. Landing is now expected at 1012 GMT on Sunday, after which the capsule will be taken to the U.S. Army Dugway Proving Ground (Utah); the collector grid (containing cometary and interstellar samples) will then be moved to NASA's Johnson Space Center in Houston. You can follow events at the...

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New Instrument Should Speed Exoplanet Hunt

Busy times. Centauri Dreams has three new Acta Astronautica papers waiting for review, but Stardust is about to return with cometary dust (and, we hope, interstellar materials), and, of course, New Horizons is just four days from liftoff. Add to that the usual flurry of news from the just concluded American Astronomical Society meeting and it's clear I'm going to be behind the curve for a week or so just trying to catch up. Bear with me, though, because fascinating stuff keeps rolling in, such as the singular exoplanet detection below. What's interesting is not just the new planet but the detection method. Normally, Doppler radial velocity measurements rely on spectographs mounted on large telescopes. A new instrument called the Exoplanet Tracker (ET) uses an interferometer instead, a device capable of more precise measurements because it can capture more light. Image: An artist's rendition shows a planet orbiting a very young, active star pocked with dark star spots and speckled...

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A Boost for Ion Propulsion

The European space agency is ramping up expectations for its Dual-Stage 4-Grid (DS4G) ion thruster. Using a concept developed by UK propulsion theorist David Fearn, the agency's test model, designed and built by a team from Australian National University, is said to be ten times more fuel efficient than the ion engine used on the SMART-1 lunar mission. In fact, says Roger Walker of ESA's Advanced Concepts Team, who is technical manager of the project, "Using a similar amount of propellant as SMART-1, with the right power supply, a future spacecraft using our new engine design wouldn't just reach the Moon, it would be able to leave the Solar System entirely." Walker calls the design "an ultra-ion engine," and ESA talks about using flight models to push into the Kuiper Belt and beyond, or deploying clusters of higher-power versions of the engine on manned Mars missions. All of which is exciting stuff, though it comes with a needed caveat. Currently at the stage of laboratory...

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A Warped, Vibrating Galaxy

If you go back 35 years, what we now call 'dark matter' was even more controversial than it is today. What was the stuff, if it really existed, and should we consider it a dim version of what we see around us elsewhere in the galaxy? Or was it something truly exotic, not yet explicable but traceable in the effects it had on galactic evolution? Whatever it was, we seemed to need it to explain a key observation: stars in the outer regions of the galaxy move faster than they ought to based on the observed mass of stars in the Milky Way. Today we still don't know what dark matter is, but an intriguing new study again reminds us of its extensive influence. As reported at the ongoing meeting of the American Astronomical Society, the Magellanic Clouds -- a pair of galaxies that orbit the Milky Way -- seem to be interacting with the galaxy's dark matter, creating a previously observed warp in the galactic disk. Using a new map of hydrogen gas emissions, researchers have found that the motion...

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Marc Millis on Hyperspace Propulsion

Centauri Dreams asked Marc Millis, former head of NASA's Breakthrough Propulsion Physics Project, for his thoughts on so-called hyperspace propulsion, as recently published in an article called "Take a Leap into Hyperspace" (New Scientist, 5 January 2006). The article has received wide coverage because of its sensational implication that we may be much closer to a breakthrough in interstellar propulsion than anyone realized. And as discussed here in the last few days, it draws on the work of the German theoretician Burkhard Heim and the later refinements of Walter Dröscher and Jochem Häuser. Millis' response follows. But he leads it off with this qualification: "My assessments below are only a cursory response rather than the result of a full technical review. If I had done a full technical review, I would have submitted it to a journal. Given the level of interest, however, and the habit that many of us have to jump to conclusions (pro or con), I thought I should comment." With that...

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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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