Something Exquisite for the Weekend

NGC 6543 is called the Cat's Eye Nebula; it was one of the first planetary nebulae to be discovered. This gorgeous view from Hubble shows that it is also one of the most complex nebulae ever studied. You're looking at a Sun-like star at the very end of its life, losing its outer gaseous layers to create concentric clouds in ways that are still mysterious. Each bright ring is actually the edge of a spherical bubble of gas. Hubble used its Advanced Camera for Surveys (ACS) to make this image.

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A Self-Sustaining Robot

An interstellar robotic probe will need robotic systems that are completely autonomous. Think about it: the Jet Propulsion Laboratory was able to solve the rover Spirit's problems on Mars by sending it a series of commands and a software patch. Spirit's computer was crashing whenever it tried to access its data storage, forcing a series of reboots that were running down the rover's batteries. By deleting a backlog of files that were clogging the system's flash memory, JPL got the rover back on track. But Mars is virtually next-door compared to Alpha Centauri. Even the Galileo probe, which experienced a tape recorder malfunction and a reprogramming forced by the failure of its high-gain antenna, could be fixed from Earth because the radio delay was only eighty minutes round-trip. Imagine what will happen with an 8.6 year round-trip delay and you can see why robotic repair systems will have to function on their own. Of course, not all progress on robot autonomy is related to space...

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A Martian Baltic Sea

A University of Colorado study, using data from the Mars Global Surveyor and Mars Odyssey orbiters, has concluded that the area surrounding the rover Opportunity's landing site once contained a huge body of water -- up to 330,000 square kilometers. That makes this Martian sea comparable to the Baltic or, as investigator Brian Hynek of the Laboratory for Atmospheric and Space Physics puts it, 'all of the Great Lakes combined.' Hynek's paper on the Martian sea ("Implications for hydrologic processes on Mars from extensive bedrock outcrops throughout Terra Meridiani") appears in the September 9 issue of Nature, and you can find CU's press release on his work here. The physicist used the thermal emission imaging system on-board Mars Odyssey to infer the size of rocks, studying how larger and smaller particles change temperature at different rates in daylight and at night. His thermal maps show wide areas of bedrock, and tell him that water once extended far beyond the landing area. To...

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Whoops!

Well, David Brin wrote a novel called Sundiver, which wouldn't have been a bad name for the end of this mission. Genesis may still have some salvageable science on-board, but it's hard to see how much of the solar wind experiment could have survived its crash. Here's a link to the BBC's coverage. No deployment on the drogue chute!

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Sunfall

Use NASA's Genesis mission page to monitor the progress of the first sample return mission since Apollo 17. Coverage will be broadcast live and on the Internet (links available at the NASA site). Although snagging the Genesis return capsule in mid-air (using helicopters piloted by stunt flyers) should be spectacular, what interests interstellar theorists is what we may learn about the solar wind. This stream of charged particles and magnetic fields moving up to 500 kilometers per second may eventually be used to push a magnetic sail like M2P2 (Mini-Magnetospheric Plasma Propulsion), which the University of Washington's Robert Winglee designed in a study for NASA's Institute for Advanced Concepts. A NASA page on the Winglee design can be found here. From the article: There is enough power in the solar wind to accelerate a 136 kg (300 lb) spacecraft to speeds of up to 288,000 km/h (180,000 mph) or 6.9 million km (4.3 million mi) a day. By contrast, the space shuttle travels at about...

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Planetary Systems in the Billions

Planet-hunter Geoff Marcy is quoted in this story in The Oklahoman on the prevalence of planetary systems around other stars. His estimate: 20 billion systems in the Milky Way alone, and that's the lower end of the range. In fact, fully half of the galaxy's 200 billion stars may be capable of supporting planets. From the article: Marcy said astronomers may spot a rocky Earth-like planet as soon as five years from now, but will have to hypothesize about its life-sustaining possibilities until a robotic probe can be sent to the extrasolar planetary system. Exactly so, at least for close-up studies, but missions like Terrestrial Planet Finder may be able to analyze planetary atmospheres closely enough to find the methane and ozone signature of life. We'll need those missions (along with the earlier Kepler and Space Interferometry Mission projects) to help us choose our first targets for interstellar probes. Given the magnitude of the enterprise, we'll want our destination star to be...

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Slow Boat to Centauri?

Sending a golden disc filled with the sights and sounds of Earth, as we did with the Voyager spacecraft, may have been a pretty efficient way to communicate with extraterrestrial civilizations. That's the view of Christopher Rose, a professor of electrical and computer engineering at Rutgers, the State University of New Jersey. Rose and physicist Gregory Wright have the cover of the September 2 issue of Nature with a paper called ""Inscribed matter as an energy-efficient means of communication with an extraterrestrial civilization." Their thesis grew out of Rose's studies of wireless commnications and what he calls the 'energy budget' of sending a signal. Would ET really use radio, or would an advanced civilization scatter artifacts in more physical form? You can read the Rutgers press release about Rose and Wright's work here. And here is a quote: Rose is in favor of listening for that close encounter, but he thinks researchers should have their eyes open, too. Rose speculates that...

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Continuing Work on Solar Sail Deployment

Here is a press release first seen on Science Blog that details NASA's latest work on solar sails, and that of two key subcontractors. L'Garde's solar sail deployment occurred in July, using a 100-foot in diameter vacuum chamber at NASA's Glenn Research Center in Ohio. The test included temperatures of minus 112 Fahrenheit to mimic actual space conditions, and used inflatable booms that become rigid once deployed. Able Engineering has also tested a solar sail deployment at NASA's Langley Research Center in Hampton, VA using a graphite boom that is extended by remote control. Able's boom supports a sail made of an aluminized material called CP-1, produced by SRS Technologies of Huntsville. Deploying a solar sail is an enormous challenge, particularly when you start talking about sails considerably larger than these test models (we'll need sails kilometers in diameter when and if we start talking about interstellar missions). Moktar Salama of the Jet Propulsion Laboratory, who has been...

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More on SETI@Home Signal

The BBC talked to SETI@Home researchers and others this morning re the possible SETI reception discussed below. The verdict: "It's all hype and noise," said its chief scientist, Dr Dan Wertheimer. "We have nothing that is unusual. It's all out of proportion." And Dr Paul Horowitz, of Harvard University, who specialises in hunting for possible alien contacts added: "It's not much of anything at all. We're not investigating it further." What will bear investigating is what caused what seems to have been a spurious signal. Should be a good chance to sort out a possible bug in the Arecibo receiving equipment. Check here for more.

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SETI@Home’s Odd Catch

New Scientist is carrying the news of a singular find by SETI@Home, the distributed computing project that uses data from the Arecibo radio telescope to look for extraterrestrial radio signals. What is being described as 'the best candidate yet for a contact by intelligent aliens in the nearly six-year history of the SETI@home project' has been detected, emmanating from a source that may or may not be located somewhere between the constellations Pisces and Aries. Dubbed SHGb02+14a, the signal is weak and may in fact be the result of either an unknown natural phenomenon or an artifact in or near the Arecibo dish itself. Centauri Dreams' take: the odd drift in the 1420 MHz signal argues for a local anomaly at Arecibo. Yes, it could be a transmitter on a rapidly spinning planet, but what confounds researchers is that each observation starts at exactly 1420 MHz and then sees the signal begin to drift. What we need are independent observations from other dishes to confirm whether...

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More on Small Extrasolar Planets

The National Science Foundation's press release on the twin planetary discoveries recently announced by NASA can be found here. In it, Geoff Marcy suggests that while lower-mass planets are much harder to detect than the kind of gas giants that have so far dominated extra-solar planetary discovery, they may be much more common. And the implication from that is that Earth-size worlds may be 'downright abundant.' Re the Gliese 436 planet, the primary instruments were the two Keck telescopes at Mauna Kea, which monitored 950 nearby stars, 150 of which were tiny M-class red dwarfs: The effort paid off in July 2003, when the astronomers noticed a periodic wobble in Gliese 436, an M dwarf star that lies about 33 light-years from Earth in the direction of the constellation of Leo. Another 12 months of data-taking confirmed the result: Gliese 436 has a Neptune-sized planet of at least 21 Earth masses that goes whipping around in its circular orbit once every 2.64 days. That corresponds to an...

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Brighter Than 200 Million Suns

It looks bright enough to be a foreground star, but this supernova, called SN 2004dj, is 11 million light years away in a galaxy known as NGC 2403. Not particularly germane to interstellar propulsion or finding candidates for robotic probes, but simply too remarkable a sight to ignore. You can read more about this Hubble photograph here. From the press release issued by the Space Telescope Science Institute: The heart of NGC 2403 is the glowing region at lower left. Sprinkled across the region are pink areas of star birth. The myriad of faint stars visible in the Hubble image belong to NGC 2403, but the handful of very bright stars in the image belong to our own Milky Way Galaxy and are only a few hundred to a few thousand light-years away. This image was taken on Aug. 17, two weeks after an amateur astronomer discovered the supernova. What we're seeing here is the creation of heavy chemical elements like calcium, iron and gold, all of which, on Earth and elsewhere, came from...

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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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