Vesta: Closing on a Protoplanet

As the Dawn spacecraft continues on its way to Vesta, which it will reach in July, mission controllers have been putting it through its paces with a series of maneuvers that test the vehicle's capabilities, a rehearsal for the high- and low-altitude mapping orbits it will operate in. It's interesting to consider Dawn's ion thrusters, which after more than 2.2 years of powered flight, continue to work flawlessly, now with a bit less than half of the original supply of xenon propellant (the spacecraft started with 425 kilograms of xenon). The velocity change in this period has been 5.7 kilometers per second, marking a record for on-board propulsion systems. Dawn's approach to Vesta is slow and spiraling, closing in on the asteroid at 0.7 kilometers per second as the orbital paths of target and spacecraft become more and more similar. In this mission report, chief engineer Marc Rayman (JPL) describes the trajectory, which is made possible by the high fuel efficiency of the ion...

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Under a Sri Lankan Moon

Looking to put things into perspective? The recent Kepler illustration of the 1235 candidate planets thus far identified, each shown in transit, is something to revel in. The image, shown below, offers a sweeping look at the range of stellar sizes that accomodate planets, and bear in mind that these are the planets that by the luck of the draw happen to be visible in transit, a small percentage of the stars Kepler is able to look at. We clearly live in a galaxy that is swarming with planets. Be sure to click on the image to blow it up to full size so you can have a better view of the distant Kepler worlds. Image: Kepler monitors a rich star field to identify planetary transits by the slight dimming of starlight caused by a planet crossing the face of its parent star. Here all of Kepler's planet candidates are shown in transit with their parent stars ordered by size from top left to bottom right. Simulated stellar disks and the silhouettes of transiting planets are all shown at the...

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Asteroid Mining: A Marker for SETI?

Having just finished Iain Banks' The Player of Games, I'm thinking about the 'orbitals' he describes in his series of novels about the Culture, a vast, star-crossing civilization that can build space habitats in the form of massive rings. Orbitals are smaller than the kind of 'ringworld' Larry Niven envisioned, but huge nonetheless, bracelets of super-strong materials housing billions who live on their inner surfaces as they orbit a parent star. The visual effects Banks pulls off in describing these habitats are spectacular. And now a new paper by Duncan Forgan (University of Edinburgh) and Martin Elvis (Harvard Smithsonian Center for Astrophysics) has me wondering about the kind of mining activities it would take to produce the raw materials for such constructs. Forgan and Elvis are interested in what they describe as a multi-wavelength, multi-signal approach to SETI. We're used to the idea of huge radio dishes listening for extraterrestrial signals, but SETI is evolving through the...

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Carnival of Space 190

Here's the latest in the weekly collection of space writing known as the Carnival of Space, in which people with their eyes on the stars go to work to explain the latest findings. Let's start with the Sun, for even as we push our investigations of distant exoplanets, we have much to learn about the nearest star, as our recent discussion of the Solar Probe Plus reminds us. Launching this week's Carnival, Vega 0.0 explains the plasma beta parameter, the ratio of gas pressure to magnetic pressure on the Sun, in an environment where plasma behaves like a fluid. In his Astroblog, the ever reliable Ian Musgrave offers up a review of Stellarium 0.10.6.1. Stellarium, for those not already acquainted with it, is a great, free photo-realistic planetarium program that amateurs should find helpful. Does Ian like it? Evidently so, given his description of the piece as an 'enthusiastic Fan Boi review.' And having worked with Stellarium myself, I can see why he's enchanted with its possibilities....

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Philosophy, Breakfast and Life Elsewhere

Because I'm immersed in Laura Snyder's wonderful book The Philosophical Breakfast Club (Broadway Books, 2011), I've been thinking lately about William Whewell. Long the master of Trinity College, Cambridge, Whewell helped bring sound, inductive methods to the fore in the science of his day, created models of international cooperation in scientific investigations through his studies of the tides, founded the discipline of mathematical economics, studied crystallography and, in one memorable episode, became involved in a 19th Century imbroglio over alien life. This morning I want to focus on that incident, but it's just one of the numerous episodes Snyder recounts in her history, which follows four remarkable men -- Whewell, mathematician Charles Babbage, astronomer John Herschel (son of William) and economist Richard Jones -- through a lifetime of friendship and scientific inquiry. What's fascinating about Whewell's brush with the topic of extraterrestrial life is that it reveals how...

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Pedal to the Metal

We have a long way to go before we can get a probe to another star in the space of a human lifetime. The figure always cited here is the heliocentric speed of Voyager 1, some 17.05 kilometers per second, which is faster than any of our outward bound spacecraft but would take well over 70,000 years to reach Alpha Centauri, assuming Voyager 1 were pointed in that direction. New Horizons is currently making 15.73 kilometers per second on its way to a Pluto/Charon flyby in July of 2015, impressive but not the kind of speed that would get us to interstellar probe territory. Interestingly, the fastest spacecraft ever built weren't headed out of the Solar System at all, but in toward the Sun. The Helios probes were West German vehicles launched by NASA, one in 1974, the other in 1976, producing successful missions to study conditions close to the Sun for a period of over ten years. The orbits of these two craft were highly elliptical, and at closest approach to the Sun, each reached speeds...

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Brown Dwarfs and Planets: A Blurry Boundary

With April approaching, my thoughts turn more and more to the release of the WISE data, which should tell us a great deal about brown dwarfs and other relatively cool objects in our stellar neighborhood. The Wide-Field Infrared Explorer mission hasn't gained the media attention of a Kepler or a CoRoT because it's not specifically a planet-hunter and isn't in the business of turning up small, rocky worlds. But if you've been following our discussions here, you know how important a mission this is. We'll get a bit more than half the data WISE has generated in April, and the rest of the dataset in 2012, by which time we may be able to identify, or else lay to rest the idea of, a gas giant ('Tyche') at 15000 AU, or a brown dwarf closer than Alpha Centauri. It's at the low end of the temperature range that so much interest is focusing these days, and the fact is that until we can get a read on how common brown dwarfs are, we won't have a good idea about what kind of stars are most common...

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Extraterrestrial Life: The Need for an Answer

An article in Time Magazine's latest issue caught my eye as I thumbed through it while waiting in line at the grocery store. The magazine is running a feature called '10 Ideas That Will Change the World,' and they tend toward being optimistic takes on huge problems. Thus the deficit gets an essay about how we're going to fix it, while Afghanistan gets a thumbs-up for progress in the right direction. The article finds gold in everything from direct mailings (OK because they help charities raise money) to modern airports, which are creating a new kind of community. And in the midst of this is a puzzling piece by Jeffrey Kluger called 'Relax: You Don't Need to Worry About Meeting E.T.', where the upshot is: 'Don't worry about contact with extraterrestrial civilizations. It will never happen.' Here's a quote: Humans and aliens haven't connected yet, but with 1022 stars out there (that's 1 with 22 zeros), it's just a matter of time — right? Wrong. If exobiologists have learned...

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Equatorial Rains on Titan

Rains have come to the equatorial regions of Titan, a vivid marker of the changing seasons on the distant Saturnian moon. A large storm system appeared in the equatorial regions in late September of last year as spring came to the low latitudes, and extensive clouds followed in October. When they dissipated, the Cassini orbiter was able to capture surface changes in a 500,000 square kilometer region along the southern boundary of the Belet dune field, along with smaller areas nearby, all of which had become darker. The likely cause: Methane rain. Tony Del Genio (Goddard Institute for Space Sciences) is a member of the Cassini imaging team: "These outbreaks may be the Titan equivalent of what creates Earth's tropical rainforest climates," says Del Genio, "even though the delayed reaction to the change of seasons and the apparently sudden shift is more reminiscent of Earth's behavior over the tropical oceans than over tropical land areas." That's an interesting take on these...

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Deadline Reminders: NASA Solicitations

Tau Zero practitioners should be aware that deadlines on the following solicitations are approaching quickly: (1) NASA Innovative Advanced Concepts (NIAC) - Early Stage Innovation DEADLINE for Notices of Intent: 29-March-2011 (Just 7 workdays away) DEADLINE for Proposals: 02-May-2011 (2) NASA Broad Agency Announcement (BAA): Technology Demonstration Missions (TDM) DEADLINE for Notices of Intent: 31-March-2011 (Just 9 workdays away) DEADLINE for Proposals: 31-May-2011 (3) NASA Broad Agency Announcement (BAA): Unique and Innovative Space Technology DEADLINE for Exec Summary: 30-Sept-2011 DEADLINE for White Paper: 01-Nov-2011 DEADLINE for Proposal: 03-Jan-2012

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The Flight of Icarus: Abridged

by Andreas Tziolas After a 15 minute main thruster burn early this morning (UTC), the MESSENGER spacecraft is now in orbit around Mercury. Congratulations to the entire MESSENGER team. As we look forward to much more from Mercury, I want to turn today's session over to Andreas Tziolas, for some thoughts on the mind-bending process of designing an interstellar spacecraft. Dr. Tziolas is a theoretical physicist and spacecraft engineer, currently serving as the Deputy Project Leader of Project Icarus. In his recent PhD (2009), he explored cosmologies resulting from brane collisions in string theory. He is currently the chief scientist for Variance Dynamical, an electronics prototyping company in Anchorage, Alaska developing radiation hardened electronics for use in space exploration. In this article, Dr. Tziolas talks to us about the legend of Icarus and offers some personal reflections from his experience as a part of the inspirational Project Icarus design team. There have been many...

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White Dwarfs and Habitable Planets

Before I get into today’s story, which is an interesting study on planets around white dwarfs that Andrew Tribick passed along, I want to say a few words about Japan. Centauri Dreams has many, many readers in that country, and the terrible images and stories coming out of there have haunted me these past few days. The suffering of those displaced by the earthquake and tsunami, and the continued problems in resolving the worsening situation at Fukushima, make it hard to focus on any other topic. Speaking for myself here at Centauri Dreams -- and I know I speak for the entire Tau Zero Foundation as well -- you Japanese readers remain in our thoughts and prayers, and will continue to do so until these great national wounds are healed. On the space front, today is the day when MESSENGER enters Mercury orbit. Below is the schedule for the events, which we’ll follow closely as orbital insertion occurs. White Dwarfs and Potential Planets But for now let’s talk about white dwarfs, those...

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MESSENGER’s Day in the Sun

We rarely talk about the inner planets here, and even Mars gets short shrift. That's because I decided at the outset that because there were so many excellent sites covering planetary exploration -- and especially Mars -- my only focus within our Solar System would be on the outer planets and, of course, what lies beyond them. But the MESSENGER mission is simply too fascinating to ignore, the first mission to Mercury since Mariner 10 way back in 1974, and beyond that, one of its project scientists is a man I deeply respect, Ralph McNutt (JHU/APL), who in addition to his MESSENGER duties also serves as one of the consultants for the Project Icarus starship design. In fact, McNutt's work in regions both near and far from the Sun is voluminous. For MESSENGER, he will be analyzing the planet's surface composition using data from the spacecraft's X-Ray Spectrometer and Gamma-Ray and Neutron Spectrometer instruments. But he's also a co-investigator for the New Horizons mission to...

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A Dark Energy Option Challenged

Having a constant named after you ensures a hallowed place in astronomical history, and we can assume that Edwin Hubble would have been delighted with our continuing studies of the constant that bears his name. It was Hubble who showed that the velocity of distant galaxies as measured by their Doppler shift is proportional to their distance from the Earth. But what would the man behind the Hubble Constant have made of the 'Hubble Bubble'? It's based on the idea that our region of the cosmos is surrounded by a bubble of relatively empty space, a bubble some eight-billion light years across that helps account for our observations of the universe's expansion. The theory goes something like this: We assume that the Hubble Constant should be the same no matter where it is measured, because we make the larger assumption that our planet does not occupy a special position in the universe. But suppose that's wrong, and that the Earth is near the center of a region of extremely low density. If...

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Fukushima: Reactors and the Public

All weekend long, as the dreadful news and heart-wrenching images from Japan kept coming in, I wondered how press coverage of the nuclear reactor situation would be handled. The temptation seemed irresistible to play the story for drama and maximum fear, citing catastrophic meltdowns, invoking Chernobyl and even Hiroshima, along with dire predictions about the future of nuclear power. My first thought was that the Japanese reactors were going to have the opposite effect than many in the media suppose. By showing that nuclear plants can survive so massive an event, they'll demonstrate that nuclear power remains a viable option. This is an important issue for the Centauri Dreams readership not just in terms of how we produce energy for use here on Earth, but because nuclear reactors are very much in play in our thinking about future deep space missions. Thus the public perception of nuclear reactors counts, and I probably don't have to remind any of you that when the Cassini orbiter...

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Antimatter: The Conundrum of Storage

Are we ever going to use antimatter to drive a starship? The question is tantalizing because while chemical reactions liberate about one part in a billion of the energy trapped inside matter -- and even nuclear reactions spring only about one percent of that energy free -- antimatter promises to release what Frank Close calls 'the full mc2 latent within matter.' But assuming you can make antimatter in large enough amounts (no mean task), the question of storage looms large. We know how to store antimatter in so-called Penning traps, using electric and magnetic fields to hold it, but thus far we're talking about vanishingly small amounts of the stuff. Moreover, such storage doesn't scale well. An antimatter trap demands that you put charged particles into a small volume. The more antimatter you put in, the closer the particles are to each other, and we know that electrically charged particles with the same sign of charge repel each other. Keep pushing more and more antimatter...

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The Rhetoric of Interstellar Flight

Isn't it fascinating how the Voyager spacecraft keep sparking the public imagination? When Voyager 2 flew past Neptune in 1989, the encounter was almost elegaic. It was as if we were saying goodbye to the doughty mission that had done so much to acquaint us with the outer Solar System, and although there was talk of continuing observations, the public perception was that Voyager was now a part of history. Which it is, of course, but the two spacecraft keep bobbing up in the news, reminding us incessantly about the dimensions of the Solar System, its composition, its relationship to the challenging depths of interstellar space the Voyagers now enter. In the public eye, Voyager has acquired a certain patina of myth, a fact once noted by NASA historian Roger Launius and followed up by author Stephen Pyne in his book Voyager: Seeking Newer Worlds in the Third Great Age of Discovery: ...the Voyager mission tapped into a heritage of exploration -- that was its cultural power. But there was...

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Enceladus: Heat Output a Surprise

What do we make of the ‘tiger stripes’? The intriguing terrain in the south polar region of Saturn’s moon Enceladus is geologically active and one of the most fascinating finds of the Cassini mission. The ‘stripes’ are actually four trenches, more or less in parallel, that stretch 130 kilometers, each about 2 kilometers wide. What Cassini showed us was that geysers of ice particles and water vapor are being ejected into space from the interior of the moon, setting off astrobiological speculations that elevated Enceladus to a new and deeply intriguing status. Is there liquid water under the surface? You could make that case based on recent work showing that some ice particles ejected from the moon are rich in salt, a sign that they may be frozen droplets from a saltwater ocean in contact with Enceladus’ mineral-rich core. Interesting place indeed -- we’ve got a serious possibility of liquid water and an energy source in the form of tidal effects from Enceladus’ orbit as it changes in...

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On Meteorites and Budgets

Two kinds of astrobiology stories are in the wind this morning. One of them has to do with the weekend eruption of stories concerning evidence of fossilized life inside a meteorite. The other deals with scientific investigation off-planet, and although sparsely covered, it's the one with the greater significance for finding life elsewhere. But first, let's get Richard Hoover's paper about meteorite life out of the way, for the growing consensus this morning is that there are serious problems with his analysis, especially as regards contamination of the sample here on Earth. I have no problems with the panspermia idea -- the notion that life just may be ubiquitous, and that planetary systems may be seeded with life not just from other planets within the system but from other stellar systems entirely. It's an appealing and elegant concept, but thus far we have no proof, and despite what Dr. Hoover is seeing in samples from three meteorites, we still can't definitively say that we've...

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NIAC: Bob Cassanova’s Mug

Last week turned into a major disruption for Centauri Dreams. Major server problems that have involved new hardware and all manner of delays struck late on the night of Sunday February 27 and kept the site offline until this past weekend. Sorry for this, and thanks to those of you who kept in touch via email or via the @centauri_dreams Twitter feed. Let's hope the situation is now under control. In any case, it's time to get back to work, which I'll begin with this piece on the return of NASA's Institute for Advanced Concepts. On my desk is a large black mug, too big for coffee despite the copious amounts of coffee I consume -- I've got it loaded with pens, yellow markers and the like. I take special pleasure in seeing it every day because it has a bold NIAC logo on it -- NASA Institute for Advanced Concepts -- blue and white on a black background, and on the other side is a favorite phrase of Bob Cassanova's: "Don't let your preoccupation with reality stifle your imagination." At...

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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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If you'd like to submit a comment for possible publication on Centauri Dreams, I will be glad to consider it. The primary criterion is that comments contribute meaningfully to the debate. Among other criteria for selection: Comments must be on topic, directly related to the post in question, must use appropriate language, and must not be abusive to others. Civility counts. In addition, a valid email address is required for a comment to be considered. Centauri Dreams is emphatically not a soapbox for political or religious views submitted by individuals or organizations. A long form of the policy can be viewed on the Administrative page. The short form is this: If your comment is not on topic and respectful to others, I'm probably not going to run it.

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