With the Herschel/Planck telescopes now on their way -- the successful launch took place at 1312 UTC from the European Space Agency's launch pad at Kourou, and the two spacecraft are now on separate trajectories -- we can take a breather to reflect on what a busy time it's been of late for space telescopes. The ongoing Hubble repairs are a fascinating story in and of themselves, but we've also got Kepler to think about as its hunt for Earth-like planets around other stars now gets underway. Shaking out the instrumentation has taken some time, but the Kepler operations team slowed the pace of communications about a week ago to eighteen hours per day, a number that will drop to six as science observations now proceed. For the balance of the mission, according to JPL project manager Jim Fanson, communications will occur only twice per week as Kepler sends home precious data. "Now the fun begins," said William Borucki, Kepler science principal investigator at NASA's Ames Research Center,...
Reflections on the New Star Trek
by Athena Andreadis This morning I have the pleasure of introducing my friend Athena Andreadis, who will give us her thoughts on the recent Star Trek film. Dr. Andreadis is Associate Professor of Cell Biology at the University of Massachusetts Medical School, and the author of To Seek Out New Life: The Biology of Star Trek. In her basic molecular neurobiology research, she studies the fundamental gene regulatory mechanism known as alternative splicing. The long-term goal of her research is to understand how the brain works, and contribute to the struggle against mental retardation and dementia. When not conjuring in the lab, Athena writes essays on science and science fiction, while writing her own SF/F fiction, some of which appears at the site Starship Reckless, which she founded. We Now Interrupt Our Regular Programming… … so that, stepping into Paul's hospitable parlor, I can hold forth on the Star Trek reboot (henceforth ST||, for parallel timeline). I assume that...
Thursday Launch for Herschel and Planck
While we're thinking about space telescopes like the aging but potentially repairable Hubble, let's not forget the launch now scheduled for Thursday from the Guiana Space Centre in Kourou. The European Space Agency's Herschel instrument will be lifted into an orbit 1.5 million kilometers from Earth, stationed at the second Lagrange point (L2) so that Sun, Moon and Earth can all be hidden behind a sunshade to afford the instrument a clear view without disturbance from its celestial neighbors. Image: About 0.5 hours after launch, Herschel separates from the launcher upper stage and starts its cruise to L2 (the second Lagrangian point), situated at about 1.5 million kilometers from Earth. Credit: ESA/D. Ducros, 2009. Along with Herschel goes Planck, also scheduled for the L2 point (the two satellites will separate shortly after launch and reach L2 independently). Herschel is the largest infrared telescope ever launched, with a 3.5-meter primary mirror made of silicon carbide that is...
New Missions for Hubble and Spitzer
With all eyes on the mission to service the Hubble telescope, it's fascinating to see that technology created for the James Webb Space Telescope is going to be used to enhanced Hubble's Advanced Camera for Surveys (ACS). The particular Application-Specific Integrated Circuit, or ASIC, design in question mirrors that of the Webb instrument and also equipment recently installed at the 2.2-meter University of Hawaii telescope on Mauna Kea, where it is part of the Charge-Coupled Device (CCD) detection system. An ASIC is a small, specialized integrated circuit, and the one about to go into Hubble could be transformative. That's because new spectrographic instruments going into Hubble will work with the repaired and upgraded ACS instrument in the study of dark energy and distant galaxies, a truly enhanced imaging capability for the aging workhorse. The ASIC next goes into space on the Webb telescope, leading one to ponder what a repair mission to that instrument would look like. After all,...
Freezing Out the Dark Energy Field
A testable prediction about dark energy? Such is the promise of a new formulation from Sourish Dutta and Robert Scherrer (Vanderbilt University), whose dark energy model interacts with normal matter and has observable results, including a prediction about the expansion rate of the universe. Astronomical surveys in the next decade should be able to detect the slowdown in the expansion rate predicted by this model, if it exists. Think 'quintessence,' a new field with the unique property that it can act like antigravity, forcing nearby objects to move away from each other rather than pulling them together. The quintessence field as developed by Dutta and Scherer likely went through a phase transition somewhere around 2.2 billion years after the Big Bang. 'Freezing out' as the universe cooled creates a scenario where the energy density of the field remained high until, with the phase transition, it dropped abruptly to a level it retains to this day. Another result: The release of some of...
A Look Back at Star Trek’s Biology
The appearance of the new Star Trek film has inspired Athena Andreadis to revisit the epilogue of her 1998 book To Seek Out New Life: The Biology of Star Trek (Random House). Andreadis (University of Massachusetts) is a frequent commenter on issues of space exploration on this and other sites, including her own Astrogator's Logs, where you'll find the updated epilogue. It's well worth reading in the context of how and why we explore. Sharply critical of the Star Trek franchise, Andreadis nonetheless commends its celebration of the human thirst for knowledge, something she believes may be the one thing we have in common with whatever extraterrestrial beings we find out there. This is bracing stuff, even for those of us who leaned more toward Heinlein than Star Trek in our youths. Here, the author speaks about dreaming of possibilities and making them accessible: Scientific understanding does not strip away the mystery and grandeur of the universe; the intricate patterns only become...
New Title on Gravitational Focus Mission
Claudio Maccone's new book is out, an extension and re-analysis of the material in two earlier titles that examined the author's innovative ideas on deep space systems. Maccone is best known to Centauri Dreams readers as the major proponent of a mission to the Sun's gravitational focus where, at 550 AU and beyond, a spacecraft could take advantage of lensing properties that would allow detailed observations of distant stars and their planets. The Italian physicist, formerly associated with Alenia Spazio and now working independently on deep space matters, has developed the idea as an interstellar precursor mission loaded with good science. But in the second part of Deep Space Flight and Communications: Exploiting the Sun as a Gravitational Lens (Springer, 2009), he also examines the mathematics of what is known as the Karhunen-Loève Transform (KLT), analyzing the tools that seem to offer the best choices for optimized communications as we eventually develop star-faring capabilities....
EGR: A ‘Hail Mary’ Pass to the Stars
EGR, standing for Embryo/Gestation/Rearing, is the name of a mission presented by John Hunt on Tibor Pacher's PI Club site, where Tibor encourages the development of what he calls 'crazy ideas.' Crazy, that is, in terms of brainstorming, getting concepts out there for comment and growth. Hunt's is likely to be controversial on several levels, although its goal -- an insurance policy for the species -- is one this site can endorse. Why an insurance policy? As we've discussed recently, the number of existential threats facing our species makes the Fermi question pointed. Self-destruction would be an ignominious end for any culture, but one not inconsistent with factors as diverse as incoming asteroids, nuclear war or biological weaponry run amok. Hunt prefers to focus on a specific threat: Advances in the area of biotech, nanotech, and artificial intelligence are accelerating. Molecular manufacturing will also bring us the ability to produce chemicals which are entirely novel and...
Wired Looks at Advanced Propulsion
Wired has picked up on our Frontiers of Propulsion Science book with just published interviews of Marc Millis and Eric Davis, co-editors of the volume. Interviewer Sharon Weinberger had a tough assignment, dealing with a 739 page collection of technical and scientific papers aimed, as she notes, at scientists and university students. But her questions were well chosen, particularly in drawing out why a book like this was necessary. Defining the Terms Marc Millis, founder of the Tau Zero Foundation, noted the need for a single, defining reference point outlining the current status of research and the opportunities presented. Thus the motivation: To clear the way for progress, my colleagues and I decided to compile this one document covering the status, issues, and unresolved questions behind a variety of known concepts, and to link the ideal goals back to real physics details. To the extent possible, we endeavored to treat these subjects impartially; showing both their visionary...
Cosmic Inflation: Evidence and Perspective
I want to talk about an exciting project to find traces of cosmic inflation today, but first, a bit of housekeeping. Regulars will know that server issues a couple of weekends ago caused me to change the software this site uses to a temporary Wordpress theme while I worked to install a more permanent solution. The new look is now in place, with a wider page, changes in fonts and, behind the scenes, all kinds of useful tools that will make maintaining and upgrading Centauri Dreams a far less arduous proposition. The new server configuation seems stable as well, so I'm hopeful that those recent issues are past us. No Web site is ever complete, and I have numerous tweaks to phase in over the coming months, but having a stable platform is obviously the first task. Now, to that inflation story. Over the weekend at the American Physical Society meeting in Denver, Ki Won Yoon (National Institute of Standards and Technology) described an experimental collaboration that is using incredibly...
Black Holes Wandering the Galaxy?
Do rogue black holes wander through the distant outskirts of the Milky Way? A new theory suggests one way to find out: Look for small clusters of stars that should accompany such objects. The idea is that low-mass proto-galaxies with black holes at their center would have merged, creating a gravitational kick that would send the now larger black hole outward fast enough to escape the host dwarf galaxy, but not fast enough to leave the overall galactic halo. Image: This artist's conception shows a rogue black hole floating near a globular star cluster on the outskirts of the Milky Way. New calculations by Ryan O'Leary and Avi Loeb suggest that hundreds of massive black holes, left over from the galaxy-building days of the early universe, may wander the Milky Way. Fortunately, the closest rogue black hole should reside thousands of light-years from Earth. Credit: David A. Aguilar (CfA). The 'kick' comes from the emission of gravitational waves as the black holes merge, carrying away...
A Solar Sail Manifesto
I was startled to see the Breakthrough Propulsion Physics project make the pages of The Atlantic in its current issue. Novelist Thomas Mallon, in an essay largely devoted to solar sailing and The Planetary Society's efforts in that direction, gives vent to some of the frustration, if not exasperation, many of us feel as we see basic research losing out to short-term missions whose purpose is by no means clear. "American politicians now mostly avoid the old conditional trope 'If we can put a man on the moon' — because we can't, not anymore," writes Mallon, who goes on to lament the passage of the BPP project and, five years later, NASA's Institute for Advanced Concepts. Questioning Why We Explore In Mallon's view, the sense of exploration is itself under attack: Even the most spectacular unmanned successes of the American space program — from the Voyager probes of the '70s to the Galileo and Cassini missions of the '90s — seem to belong to a fading worldview. A...
Renewed Challenge to the Dinosaur Killer
Some scientific hypotheses seem too perfect to be anything but true. Long before we understood the processes behind plate tectonics, the natural fit between the coasts of Africa and South America made the notion of their original linkage seem obvious. Although dismissed in many quarters as mere coincidence, the piecing together of earlier continents would follow. The hypothesis of continental movement, whatever the cause, was almost too obvious not to be true. But does science really work so neatly? Writing about his work on the evident 'dinosaur killer' event at the Cretaceous/Tertiary boundary, Walter Alvarez once said: "Much of the work we do as scientists involves filling in the details about matters that are basically understood already, or applying standard techniques to new specific cases. But occasionally there is a question that offers an opportunity for a really major discovery." And the K/T impact seemed, like the continental coastlines, to be an obvious fit, a...
Eccentric Orbits and Bold Predictions
The 100th edition of the Carnival of Space is now up at the One-Minute Astronomer site, where I learned of the existence of Christopher Crockett's Innumerable Worlds blog. Christopher's story on two gas giants around subgiant stars is well worth reading. He's a UCLA graduate student now working at Lowell Observatory who offers a good deal of background material in his posts, as in this comment on the new planets' unusually eccentric orbits: How planets end up on such crazy orbits is a matter that is currently being researched. These two worlds aren't alone; many of the new worlds we're finding sit on highly eccentric orbits. The leading hypothesis is that interactions between closely spaced planets might affect their orbits. If two planets get too close, the lighter one can get ejected from the planetary system entirely while the remaining, more massive, world is left behind on a very elliptical orbit. This is the same principle we use to slingshot probes out into deep space by...
Pushing Past Redshift Eight
No one has ever seen an object further away than the one at the center of the image below. It's a gamma-ray burst known as GRB 090423, spotted by the Swift satellite on April 23rd and quickly observed by the Gemini Observatory and United Kingdom Infrared Telescope, both on Mauna Kea (Hawaii). The source is visible at longer wavelengths but disappears at the 1 micron level, all of which corresponds to a distance of about thirteen billion light years. Image: The fading infrared afterglow of GRB 090423 appears in the center of this false-color image taken with the Gemini North Telescope in Hawaii. The burst is the farthest cosmic explosion yet seen. Credit: Gemini Observatory/NSF/AURA, D. Fox and A. Cucchiara (Penn State Univ.) and E. Berger (Harvard Univ.) Spectacular, no? Numerous telescopes around the planet went on to observe the GRB's afterglow, allowing the infrared light's spectrum to confirm the highest redshift ever measured: z = 8.2. The object in question was probably a...
Getting Closer to an Exomoon Detection
Finding moons around extrasolar planets is an invigorating quest. After all, at least three moons around gas giants right here in our own system -- Europa, Enceladus and Titan -- are considered of high astrobiological interest. What about gas giants in the habitable zone of some distant star? The image below shows what a moon of such a planet one might look like, as imagined by astronomer Dan Durda (Southwest Research Institute). Could such worlds be? As we learn more, bear in mind that the hunt for 'exomoons' has already begun. The CoRoT spacecraft is searching for transit timing variation signals (TTV) -- variations in the time it takes a planet to transit its star -- as described by Sartoretti and Schneider in a 1999 paper. David Kipping (University College London) has been developing a second method called transit duration variation (TDV), which works in conjunction with the first. The TDV signal is brought about by velocity changes as the planet/moon 'system' is observed over...
Upcoming Beamed Propulsion Conference
A note from Eric Davis (Institute of Advanced Studies at Austin) fills me in on the details of the upcoming 6th International Symposium on Beamed Energy Propulsion, to be held in Scottsdale, AZ during the first week of November. Much of the program is of interest to interstellar studies, ranging from the basic science and technology of laser, microwave and particle beam propulsion to specifics relating the topic to beamed interstellar missions. The latter subject will always be associated with Robert Forward, whose studies of beaming technology and sails made us understand that reaching the stars was not necessarily impossible. Lasers were the key, as Forward learned through his work with Ted Maiman at Hughes Research Laboratory. Years later he recalled his 'eureka' moment: "I knew a lot about solar sails, and how, if you shine sunlight on them, the sunlight will push on the sail and make it go faster. Normal sunlight spreads out with distance, so after the solar sail has reached...
Asteroid Deflection by Tether
Diverting incoming asteroids is a high priority item, and so is a mission to a nearby asteroid for a close-up study of its composition and a shakeout of operating technologies. Think about the movie Deep Impact. Nukes are used to break up an incoming object, in this case a comet, but the resultant deadly chunks are still headed toward Earth. The planet suffers one disastrous collision, but it turns out to be survivable due to quick thinking and the willingness of a spacecraft crew to sacrifice themselves by blowing up the remaining impactor. Get past the Hollywood cliffhanger elements and Deep Impact had its moments (in any case, I'll sign off on any movie with Robert Duvall in it). The use of nuclear weapons in the movie does raise a legitimate question -- do we know enough about what might hit us to predict what would happen if we did try to destroy it this way? That's one reason we need early missions to study Earth-crossing asteroids, and it's also a reminder that keeping our...
Ubiquitous Brown Dwarfs: A Dark Matter Solution?
Three brown dwarfs with masses that push up against the boundary between star and planet have been identified in IC 348, a star-forming region some 1000 light years from Earth in the direction of the constellation Perseus. The dwarfs do not appear to be gravitationally bound to a star although they are bound by the cluster, and they're useful as we try to broaden our understanding of the mass distribution in newly formed stellar populations. Andrew Burgess (Observatoire de Grenoble) has this to say about the find: "There has been some controversy about identifying young, low mass brown dwarfs in this region. An object of a similar mass was discovered in 2002, but some groups have argued that it is an older, cooler brown dwarf in the foreground coinciding with the line of sight. The fact that we have detected three candidate low-mass dwarfs towards IC 348 supports the finding that these really are very young objects." Image: IC 348, the star-forming region where the brown dwarfs were...
Water World Around Gliese 581?
Gliese 581, the star that teased us a few years back with reports of a 'super-Earth' planet in the habitable zone, is back in the news. Michel Mayor's Geneva team has located a fourth planet in the system, Gliese 581 e, which weighs in at a mere 1.9 Earth masses, making it the least massive exoplanet ever detected. Orbiting its primary in 3.15 days, the newly found world is too close to the star to be in the habitable zone, but the other shoe that drops here is that Gl 581 d may itself be. Image: By refining the orbit of the planet Gliese 581 d, first discovered in 2007, a team of astronomers has shown that it lies well within the habitable zone, where liquid water oceans could exist. This diagram shows the distances of the planets in the Solar System (upper row) and in the Gliese 581 system (lower row), from their respective stars (left). The habitable zone is indicated as the blue area, showing that Gliese 581 d is located inside the habitable zone around its low-mass red star....