Take a look at NGC 4565, a spiral galaxy seen edge-on. Spiral galaxies viewed at this angle often show dark dust lanes, the result of dust from dying stars mixing with interstellar gas. We've discussed the problem of interstellar dust in terms of objects moving at relativistic speeds between stars, but recent quasar studies are showing us that entire galaxies may expel dust to distances of several hundred thousand light years. In terms of the NGC 4565 image, that would be ten times farther than the visible edge of the galaxy. Image: Spiral galaxies seen edge-on often show dark lanes of interstellar dust blocking light from the galaxy's stars, as in this image of the galaxy NGC 4565. The dust is formed in the outer regions of dying stars, and it drifts off to mix with interstellar gas. Credit: Sloan Digital Sky Survey (SDSS-II). The astronomers who did this work talk of intergalactic space being filled with a haze of fine dust particles, a haze that can be examined by analyzing light...
Space Voyaging a Century Out
A nice, tidy liftoff for Kepler, and like all night launches, well worth watching. The mission is generating a satisfying amount of attention in the press and a slew of news releases, from one of which which I'll quote Geoff Marcy: "In part, learning about other Earths -- the frequency of them, the environment on them, the stability of the environment on other Earths, their habitability over the eons -- is going to teach us about our own Earth, how fragile and special it might be. We learn a little bit about home, ironically, by studying the stars." And of course it's hard to argue with that, although the focus for most of us will only be tangentially here and most emphatically there -- just how many terrestrial worlds are out there, and how likely are the chances for their being in the habitable zone? Marcy gets preferential treatment here simply because, along with Paul Butler and a team of exoplanet hunters spread out over the globe, he has been involved in almost half of our...
Ceres: A Possible Source of Life?
The Kepler countdown proceeds and, naturally, will preoccupy many of us during the day. I won't try to keep up with the minutiae, as we're not set up to be a news site at that level of granularity. Go instead to the Kennedy Space Center's countdown page, where you'll find live video feeds, or the Kepler portal. You can track the Kepler feed on Twitter here, although it's been quiet all morning. The launch is scheduled for 10:49 EST (03:49 UTC) and the clock, as they say, is running. NASA TV should kick in about two hours before launch. If you want a Kepler diversion, try Astrobiology Magazine's story on Ceres as a possible source for life on Earth. What's not to like about yet another candidate for life in the outer Solar System? Even so, this one seems to be quite a stretch. The story focuses on a theory from Joop Houtkooper (University of Giessen), who sees the 'dwarf planet' (I think that's the right IAU terminology these days) as a potentially living world, a place a bit like...
Kepler, SETI and Ancient Probes
We've already speculated here that if the Kepler mission finds few Earth-like planets in the course of its investigations, the belief that life is rare will grow. But let's be optimists and speculate on the reverse: What if Kepler pulls in dozens, even hundreds, of Earth-sized planets in the habitable zones of their respective stars? In that case, the effort to push on to study the atmospheres of such planets would receive a major boost, aiding the drive to launch a terrestrial planet hunter with serious spectroscopic capabilities some time in the next decade. Budget problems? Let's fold Darwin and whatever Terrestrial Planet Finder design wins approval into the same package, and make this a joint NASA/ESA mission. Finding numerous Earth-like planets will be a driver, as will gradual economic recovery. Finding Many Earths The discovery of numerous 'Earths' would also galvanize public interest in interstellar flight, which offers a useful educational opportunity. Even the short-lived...
New Life in an Ancient Lake?
If we're looking for pristine environments for life, Antarctica offers much. More than 150 subglacial lakes have been discovered beneath the ice sheet, isolated from the surface for long periods and possibly home to species that have never before been observed. From November 2007 to February 2008, a subglacial lake named Lake Ellsworth was studied by a four-person team that used seismic and radar surveys to map the lake's depth and take other measurements that made clear its potential for exploration. Their blog is archived here, and it makes for good reading. Image: A DeHavilland Dash-7 flying near the British Antarctic Survey research station at Rothera. The station is 1630 kilometers southeast of Punta Arenas, Chile, and served as a staging area for the Lake Ellsworth studies of 2007-2008. Credit: Natural Environment Research Council. Europa, anyone? Well, there are certain resemblances. If the thickness of the ice on Europa is still controversial, we know for a fact that Lake...
Temperature Inversion on Pluto
With an atmospheric pressure one hundred thousand times less than that on Earth, Pluto becomes an even more intriguing object than usual when it moves closer to the Sun in its 248-year orbit. This period, occurring now, causes the temperature of the surface to increase, and that causes what had been frozen nitrogen (with trace amounts of methane and, probably, carbon dioxide) to sublimate into gas. Studying these matters with ESO's Very Large Telescope, astronomers have now found unexpectedly large amounts of methane in that atmosphere. Image: Artist's impression of how the surface of Pluto might look, according to one of the two models that a team of astronomers has developed to account for the observed properties of Pluto's atmosphere. The image shows patches of pure methane on the surface. At the distance of Pluto, the Sun appears about 1000 times fainter than on Earth. Credit: ESO/L Calçada. A second discovery: The atmosphere of the distant ice world is some forty degrees Celsius...
A Planetary Migration?
With the Kepler launch scheduled for no earlier than Friday, I'm keeping one eye on the mission site while I develop today's material. Kepler launches aboard a Delta II, but engineers are now having to check common hardware between that rocket and the Taurus XL launch vehicle that failed to get NASA's Orbiting Carbon Observatory into orbit last week. Thus the March 5 launch date slips to March 6, which itself is still tentative. Meanwhile, an unusually interesting story in Nature also has my attention, dealing not with exoplanets but with the early Solar System and what may have been a period of planet migration that caused heavy asteroidal bombardment of the inner planets. This one comes out of the University of Arizona, where scientists have been looking at the distribution of asteroids with diameters greater than fifty kilometers. UA's David Minton and Renu Malhotra ran simulations beginning with a uniform asteroid belt to see how the present-day gaps in the belt may have arisen...
Imagining Alien Ecospheres
A Europan Scenario Between living dirigibles on gas giants and potential organisms under the ice, we've had quite a week in terms of exotic life-forms. I didn't have space in yesterday's review of Unmasking Europa to talk about the book's chapter on biology, but here's an interesting glimpse of a not implausible biosphere on that moon, as presented by physicist Richard Greenberg: Brisk tidal water sweeps over creatures clawed into the ice, bearing a fleet of jellyfish and other floaters to the source of their nourishment. As the water reaches the limits of its flow, it picks oxygen up from the pores of the ice, oxygen formed by the breakdown of frozen H2O and by tiny plants that breath it out as they extract energy from the sun. The floating creatures absorb the ocygen and graze on the plants for a few hours. The water cools quickly, but before more than a thin layer can freeze, the ebbing tide drags the animals deep down through cracks in the ice to the warmer ocean below. Most of...
Unmasking Europa: Of Ice and Controversy
You wouldn't think the thickness of ice on a distant moon of Jupiter could emerge as something of a political hot-button, but that seems to be what has happened in the ongoing investigation of Europa. Thick ice or thin? The question is more complicated than it looks, because by 'thin' ice we don't mean just a few inches, but perhaps ten kilometers, perhaps five. The key question is not a specific measurement, but whether the ice is thin enough to allow the surface and the global ocean beneath to be connected, in the form of occasional cracks, melt-throughs or other events. Much hinges on the answer. As Richard Greenberg shows in Unmasking Europa: The Search for Life on Jupiter's Ocean Moon (Springer, 2008), the small world quickly fell under the scrutiny of scientists with a geological bent after first Voyager and then Galileo imagery became available. The latter was a problem, for the failure of the spacecraft's high-gain antenna meant the total number of images was sharply reduced,...
HD 80606b Transit Bagged
An email from Greg Laughlin confirms that the planet HD 80606b has indeed been caught in a transit, a roughly 15 percent probability now turned into hard data. Laughlin (UCSC) and team recently wrote up their Spitzer infrared observations of this mutable gas giant, a world with an orbit so eccentric that it almost mimics a comet, swinging out to 0.85 AU from its star, then rushing in to a breathtaking 0.03 AU for a brief, searing encounter. The possibility of a transit has been on his mind ever since. "If you could float above the clouds of this planet, you'd see its sun growing larger and larger at faster and faster rates, increasing in brightness by almost a factor of 1,000," Laughlin said at the end of January in this JPL news release. His team captured what happens on this world as its atmosphere heats rapidly and produces 5 kilometer per second winds that create vast storm systems, gradually easing as the planet moves away from its star. I've already run the resultant image...
Edwin Salpeter and the Gasbags of Jupiter
By Larry Klaes 'The Gasbags of Jupiter' sounds for all the world like the title of an early 1930s novel that would have run in a venue like Science Wonder Stories. In fact, as Larry Klaes tells us below, the idea grew out of Carl Sagan's speculations about free-floating life-forms that might populate the atmospheres of gas giant planets like Jupiter. Cornell physicist Edwin Salpeter had much to do with the evolution of that concept, helping Sagan produce a paper that was a classic of informed imagination (and one that led to numerous science fiction treatments as the idea gained currency). Larry's celebration of Salpeter's life gives a nod to that paper but also notes his deep involvement in the study of the most distant celestial objects. On March 14, the Department of Astronomy at Cornell University will commemorate the life of one of their most prestigious faculty members: Edwin E. Salpeter, the James Gilbert White Distinguished Professor of Physical Sciences Emeritus. Salpeter...
Gamma-Ray Burst Exceeds All Others
Adam Goldstein must be living right. Here's a grad student (University of Alabama, Huntsville) who's on his first day on the job working with the Fermi Gamma-ray Space Telescope. He's given the task of monitoring the Gamma-ray Burst Monitor (GBM) instrument, which routinely detects bursts, about one a day. This time, though, when the phone rings, it is to flag a burst like no other, 700 times longer in duration than the average. We already knew that GRBs were exotic events. Many astronomers believe that they occur when, out of its nuclear fuel, a massive star collapses into a black hole, creating jets of material that interact with gaseous debris previously shed by the star. But this one, detected in mid-September last year, was a true behemoth, with a red shift pegging its point of origin as twelve billion light years from Earth, in the constellation Carina. GRB 080916C turns out to be the most powerful gamma-ray event ever detected. Image: GRB 080916C's X-ray afterglow appears...
Notes & Queries 2/23/09
Prioritizing the Outer System Europa or Titan? Jupiter or Saturn? NASA and the European Space Agency, faced with the dilemma of choosing between competing missions, apparently settled on both, with the Europa Jupiter System Mission likely to be implemented first. Here we're talking about two robotic orbiters, launched on separate spacecraft in 2020, with arrival in Jupiter space in 2026. The two orbiters will orbit Europa and Ganymede respectively, while the later Titan Saturn System Mission would include a NASA orbiter and an ESA lander and research balloon. Both missions thus move forward for further study. I note all this in the context of what will surely be ever increasing interest in Europa following the publication of Richard Greenberg's Unmasking Europa: The Search for Life on Jupiter's Ocean Moon. I'll be talking to Greenberg tomorrow and reporting on our conversation soon, but I do want to quote him on a particular point right away, relevant as it is to mission planning:...
Orion and Digital Science
The 91st Carnival of Space offers up Brian Wang's look at Project Orion, with links to photos and videos relating to nuclear pulse propulsion, one of which I embed here from the This is Rocket Science site. For those who like to take potentially workable ideas up to gigantic scales, Brian discusses the Super-Orion, all eight million tons of it, with the capacity to take three million tons of cargo anywhere in the Solar System. The pusher plate would have reached a diameter of 400 meters. Brian notes the scale: 400 meters in diameter means that the area (footprint) is about 30 football fields. 4 football fields long by 8 football fields wide. The height of the super-orion is about the height of skyscraper like Taipei 101 or Petronas Towers. The base of the Great Pyramid forms a nearly perfect square with about 230 m (756 feet) on a side. When newly completed, the Great Pyramid rose 146.7 m (481.4 ft)—nearly 50 stories high. Super-Orion would have had the volume of about 10 Great...
Kepler and the Odds
The Kepler launch is coming up on March 5, marking the first time we will have the ability to find a true Earth analogue around another star; i.e., a planet of about Earth's mass in the habitable zone where water can exist in liquid form on the surface. Which is not to say that COROT may not come close, though Kepler's enormous star-field (100,000 targets in the Cygnus-Lyra region) and incredibly sensitive camera -- a 95-megapixel array of charged coupled devices (CCDs) -- is optimized for planets down to Earth size rather than larger 'super-Earths.' Image (click to enlarge): Kepler's target region, the Milky Way ni the Cygnus region, with the instrument's field of view superimposed. Each rectangle indicates the specific region of the sky covered by each CCD element of the Kepler photometer. There are a total of 42 CCD elements in pairs, each pair comprising a square. Credit: NASA/Carter Roberts (1946-2008). We just looked at Alan Boss' remarkable statement that there could be 100...
STEREO: Into the Lagrangian Points
I love it when we find uses for instruments that they were never intended for. In deep space terms, we can go back to Voyager 2, which carried a plasma wave instrument that was designed to measure the charged particles inside the magnetic fields of the gas giant planets it would pass. Voyager 2 was able to tell us much about dust impacts on a fast-moving spacecraft when it was realized that the plasma wave instrument would be able to sense the plasma created by vaporized particles. In other words, the instrument became a de facto dust detection device. Now I see that the two STEREO spacecraft may be pressed into service to study what's lurking in the L4 and L5 Lagrangian points, each 150 million kilometers from Earth, with L4 60 degrees in front of our planet and L5 60 degrees behind. Balancing the gravitational field of the Sun with that of Earth, the Lagrange points are interesting places, possibly a junkyard of debris from the early Solar System. It's known that such points appear...
Finding ‘Weird Life’ on Earth
Just how many forms of life are there? We often speculate here about life on other worlds, but Paul Davies (Arizona State) is currently exploring the question from a different perspective entirely. Davies would like to know whether a 'second genesis' might have occurred, producing a fundamentally different form of life that would have evolved right here on Earth and might still occupy our planet. Life may, in other words, have started many times, perhaps with significantly different results we just haven't uncovered yet. Call it a 'shadow biosphere,' a concept the physicist calls for exploring: "...[It] is still just a theory. If someone discovers shadow life or weird life it will be the biggest sensation in biology since Darwin. We are simply saying, 'Why not let's take a look for it?' It doesn't cost much (compared to looking for weird life on Mars, say), and, it might be right under our noses." Finding these alternate life forms, if they exist, may be tricky, as they could be...
One Hundred Billion Trillion Habitable Planets
Alan Boss, whose new book The Crowded Universe will soon be on my shelves (and reviewed here), has driven the extrasolar planet story to the top of the news with a single statement. Speaking at the American Association for the Advancement of Science's annual meeting in Chicago, Boss (Carnegie Institution, Washington) said that the number of Earth-like planets in the universe might be the same as the number of stars, a figure he pegged at one hundred billion trillion. A universe teeming with life? Inevitably. The Telegraph quoted Boss on the matter in an early report on his presentation: "If you have a habitable world and let it evolve for a few billion years then inevitably some sort of life will form on it," said Dr Boss. "It is sort of running an experiment in your refrigerator - turn it off and something will grow in there. "It would be impossible to stop life growing on these habitable planets." Few Centauri Dreams readers would disagree with the notion that life may be common in...
Cosmic Inflation in Context
Cosmic inflation, first proposed by Alan Guth (MIT) in 1979, seems about as intractable a subject as dark energy. How to study it? Inflation does something mind-bending to spacetime by making it expand far faster than the speed of light. Oddly, this doesn't contradict anything Einstein said, because while nothing we know can travel faster than light through spacetime, there is no restriction implied in these equations on the expansion of spacetime itself. This is why Miguel Alcubierre's 'warp drive' notions can fit within an Einsteinian universe. After all, what Alcubierre proposed in his 1994 paper was that a spacecraft that could create the right kind of spacetime distortion would at no point in its journey go faster than the speed of light. Compressing spacetime in front while expanding spacetime behind, it would itself remain within a 'bubble' of normal spacetime. Of course, the amount of energy required to achieve this feat (and it's negative energy, at that) may render the...
Fireball Linked to Cometary Debris
Comet C/1919 Q2 Metcalf catches the attention. The intriguing object was discovered in August of 1919 and remained visible until early 1920, but no subsequent observations have been made. In 1973, Allan Cook discovered that the Omicron Draconids meteor stream seemed to be following the orbit of the earlier comet. Suspicion is strong that the comet broke up and that the Omicron Draconids are simply the result of that event, a manifestation of cometary debris. All of which makes the fireball that streaked through European skies last July a bit more interesting than your average bolide. A new paper will suggest that the boulder that caused it -- probably a meter across and massing 1.8 tons -- was a chunk of the original comet, a boulder that broke apart from the original ice and rock nucleus as C/1919 Q2 Metcalf disintegrated. That would mean we have comet fragments out there waiting to be discovered. Josep M. Trigo-Rodríguez (Institute of Space Sciences, CSIC-IEEC, Spain) explains: "If...