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...
MEarth: Searching for Habitable ‘Super-Earths’
Will the first 'super-Earth' in the habitable zone of its star be found around a red dwarf? An M5-dwarf with both mass and radius about a quarter that of the Sun would have 1/200th Sol's luminosity. That's interesting for transit purposes, for a planet in the habitable zone around this star would be close in indeed, some 0.074 AU out, with an orbital period of 14.8 days. Its transit probability would correspondingly be raised by a factor of three compared to the Earth-Sun system. The result, as laid out by the transit survey called MEarth: Detecting such planets should be possible from the ground. Take a look at the live video of what MEarth is doing. Based at the Fred Lawrence Whipple Observatory on Mt. Hopkins in Arizona, the team works with 1976 nearby red dwarfs, visiting each repeatedly in hopes of snaring an ongoing transit, whose information would then be routed to larger instruments for confirmation. They're looking at targets spread over the entire celestial northern...
Deep Questions About an Impact
Things move around in the story queue here, but occasionally a particular item almost gets past me before I remember to cover it. Such is the recent work on the possible impact event some 12,900 years ago, which Richard Firestone (Lawrence Berkeley Laboratory) and colleagues have argued would have contributed to the extinction of such large mammals as woolly mammoths and mastodons, not to mention causing continent-wide wildfires that could have brought about the end of the Clovis culture in North America. The period in question comes at the beginning of the Younger Dryas, a 1300-year cold spell whose termination saw the temperature of Greenland warm by over 5°C in just a few decades (see comments below). We've speculated about the possibility of an asteroid or comet impact on Centauri Dreams (the most recent story is here), but new analysis casts doubt on the theory. Sandy Harrison (University of Bristol) has gone to work on charcoal and pollen evidence to study how wildfires...
Interstellar Strategy: Spreading the Word
by Tibor Pacher My friend Tibor Pacher is joined with me (until 2025, anyway) in our 'interstellar bet,' under the auspices of the Long Now Foundation. Trained as a physicist at the Eötvös University in Budapest and the University of Heidelberg, Dr. Pacher has been exploring ways to get across interstellar concepts to the public through venues like his peregrinus interstellar. Social networking is to some of us a new frontier, and I've asked Tibor to provide some background on what he is doing to make sure that an obscure wager develops an audience and becomes an effective teaching tool. Yesterday I watched the movie In the Shadow of the Moon. I must admit, this was not the first time, but I wanted to capture more details and - well, it is just a great film, and, I believe, not only for space heads a 'must.' Sober and emotional at the same time, for me it is a perfect example of how the public imagination can be captured about space, in a way which shows the deeply human nature of...
361 Civilizations in the Galaxy?
I promised a quick return to recent work on the Drake Equation, which helps us estimate the number of communicating civilizations in the galaxy, but a BBC story on Duncan Forgan has me back at it even sooner than I had intended. It's no surprise that the matters encapsulated in Drake's thinking should be in the news. After all, the era of Fermi and Drake was without firm knowledge of extrasolar worlds, of which we now know over three hundred. For that matter, the concepts of habitable zones around both stars and the galaxy itself had not come to fruition, nor had anyone ever heard of the 'rare Earth' hypothesis. We also work today with knowledge of Charles Lineweaver's studies of the median age of terrestrial planets in the Milky Way, which point to civilizations around other stars having had as much as two billion years-plus to emerge before our own Earth had even coalesced. Until we know more, I suspect we'll be adjusting Drake parameters for some time, as Duncan Forgan (University...
Dust Up Between the Stars
Almost four years ago I wrote a Centauri Dreams entry about Dana Andrews' views on shielding an interstellar spaceship. The paper is so directly relevant to our recent discussion on the matter that I want to return to it here. Andrews (Andrews Space, Seattle) believes that speeds of 0.2 to 0.3 c are attainable using beamed momentum propulsion. That being the case, he turns in his "Things to Do While Coasting Through Interstellar Space" paper to questions of human survival. Particles with a Punch Collision with interstellar dust becomes a major issue when you're traveling at speeds like these, a fact Andrews is quick to quantify. For a starship moving at 0.3 c, a typical grain of carbonaceous dust about a tenth of a micron in diameter should have a relative kinetic energy of 37,500,000 GeV. Our hypothetical star mission with human crew moving at a substantial fraction of light speed will run into about thirteen of these dust particles every second over every square meter of frontal...
Dissent on Drake
Centauri Dreams' recent post on the Drake Equation triggered a broad range of response, both in comments and back-channel e-mails, the latter of which produced a note from Kelvin Long quoting a rather controversial position on Drake by one leading scientist. Here it is. See if it raises your hackles: "I reject as worthless all attempts to calculate from theoretical principles the frequency of occurrence of intelligent life forms in the universe. Our ignorance of the chemical processes by which life arose on earth makes such calculations meaningless." The words are Freeman Dyson's, from his essay "Extraterrestrials" in Disturbing the Universe (Harper & Row, 1979), a book I re-read every few years as much to admire the author's rhetorical skills as to draw again on his insights. Kelvin has differing views on Drake and so do I, but I'm going to quote Marc Millis' reaction to the Dyson statement, reflecting as it does an approach toward scientific method that I share. Marc writes: "On...
Interstellar Flight: The Dust Conundrum
It would be helpful if space were a bit more empty. A key problem facing an interstellar probe would be encounters with dust in the planetary system it leaves and, as it reaches cruising speed, dust impact in space between the stars. Although our Solar System seems to be in an unusually sparse pocket of space, the galaxy-wide distribution of hydrogen is roughly one atom per cubic centimeter. Dust -- bits of carbon, ice, iron compounds, and silicates -- is far rarer still, but enough of a factor to a ship moving at a significant fraction of the speed of light that the designers of the Project Daedalus craft built in a payload shield 32-meters in radius to protect their starship. Then again, much depends on your location. Have a look at the image below. It's an area called the Red Rectangle some 2300 light years from Earth in the constellation Monoceros. Although the center of the image seems to be a single star, it's actually the double star system HD 44179. The Red Rectangle is a...