Planet formation can be tricky business. Consider that our current models for core accretion show dust grains embedded in a protoplanetary disk around a young star. Mixing with rotating gas, the dust undergoes inevitable collisions, gradually bulking up to pebble size, then larger. As the scale increases, we move through to planetesimals, bodies of at least one kilometer in size, which are large enough to attract each other gravitationally. Some planetesimals break apart through subsequent collisions, but a few grow into protoplanets, then planets themselves. It's a reasonable theory that fits what we see around young stars as solar systems take hold. But what Alan Boss (Carnegie Institution for Science) has been working on is a question raised by the process: How do the dust grains and objects smaller than planetesimals keep from being drawn into the protostar before they can become large enough to attract the materials they need to grow? The pressure gradient of the gas in the disk...
A Planet Reborn?
Objects that seem younger than they ought to be attract attention. Take the so-called 'blue stragglers.' Found in open or globular clusters, they're more luminous than the cluster stars around them, defying our expectation that stars that formed at about the same time should develop consistent with their neighbors. Allan Sandage discovered the first blue stragglers back in 1953 while working on the globular cluster M3. Because blue stragglers are more common in the dense core regions of globular clusters, they may be binary stars that have merged, but a number of theories exist, most of them focusing on interactions within a given cluster. Image: The center of globular cluster NGC 6397, in an image taken by the Hubble Space Telescope. Credit: Francesco Ferraro (Bologna Observatory), ESA, NASA. Now we may have found a planet that seems to be younger than it ought to be. Michael Jura (UCLA) and team report on the results in the Astrophysical Journal Letters, making the case that a...
The Zoo Hypothesis as Thought Experiment
Imagine a civilization one million years old. As Nick Nielsen points out in today's essay, the 10,000 year span of our terrestrial civilization would only amount to one percent of the older culture's lifetime. The 'zoo hypothesis' considers extraterrestrials studying us as we study animals in controlled settings. Can a super-civilization study a planetary culture for the whole course of its technological development? Nielsen, an author and strategic analyst, runs a thought experiment on two possible courses of observation, asking how we would be perceived by outsiders, and how they might relate us to the history of their own development. by J. N. Nielsen In 1973 John A. Ball wrote a paper published in Icarus called "The Zoo Hypothesis" in which he posited an answer to the Fermi paradox involving the deliberate non-communication of advanced ETI (extraterrestrial intelligence) elsewhere in our universe: "…the only way that we can understand the apparent non-interaction between...
Beaming ‘Wafer’ Probes to the Stars
The last interstellar concept I can recall with a 20-year timeline to reach Alpha Centauri was Robert Forward's 'Starwisp,' an elegant though ultimately flawed idea. Proposed in 1985, Starwisp would take advantage of a high-power microwave beam that would push its 1000-meter fine carbon mesh to high velocities. As evanescent as a spider web, the craft would use wires spaced the same distance apart as the wavelength of the microwaves that drove it, which is how it could be so lightweight and yet maintain rigidity under the microwave beam. Throw in sensors and circuitry built-into the sail itself and you had no need for a separate probe payload -- Starwisp was its own payload. This was conceived as a flyby mission, in which the microwaves would again bathe the craft as it neared its target, providing just enough energy to drive its communications and sensor array to return data to Earth. What a mission: Starwisp would accelerate at 115 g's, its beam pushing it up to 20 percent of...
Capturing Sedna: A Close Stellar Encounter?
With New Horizons scheduled for its flyby of Pluto/Charon in a matter of weeks and a Kuiper Belt extended mission to follow, it’s interesting to note a new paper on objects well beyond Pluto’s orbit. Lucie Jílková (Leiden Observatory) and colleagues address the problem of Sedna and recently discovered 2012VP113. The problem they present is that even at their closest approach to the Sun, these two objects are outside the Kuiper Belt, while their aphelion distances are too short for them to be considered members of the Oort Cloud. So where do Sedna and 2012VP113 belong in our taxonomy of the Solar System? Thirteen such objects have now been discovered, a group collectively referred to as Sednitos. These objects have orbital elements in common: A large semi-major axis (with perihelion beyond 30 AU and aphelion beyond 150 AU), a common orbital inclination, and a similar argument of perihelion. A common origin seems likely. Jílková’s team is interested in the possibility that Sedna and...
Charon’s ‘Dark Pole’
An abrupt change: I'm holding today's post (about halfway done, on a stellar flyby that may have produced Sedna and other such objects long in our system's past) to turn to New Horizons' latest imagery, which is provocative indeed. We'll cover the Sedna story tomorrow. What we have from New Horizons is the work of the spacecraft's Long Range Reconnaissance Imager (LORRI) in a series of images that show Pluto and its largest moon Charon as they more than double in size between May 29 and June 19. There's plenty here to marvel at, but what stands out for me is the mysterious dark region that NASA's latest release refers to as 'a kind of anti-polar cap' on Charon. Have a look: Image: These recent images show the discovery of significant surface details on Pluto's largest moon, Charon. They were taken by the New Horizons Long Range Reconnaissance Imager (LORRI) on June 18, 2015. The image on the left is the original image, displayed at four times the native LORRI image size. After...
Yarkovsky and YORP Effect Propulsion for Long-life Starprobes
Centauri Dreams regular James Jason Wentworth wrote recently with some musings about Bracewell probes, proposed by Ronald Bracewell in a 1960 paper. Bracewell conceived the idea of autonomous craft that could monitor developments in a distant solar system, perhaps communicating with any local species that developed technology. Pondering how such a craft might manage station-keeping over the aeons, Jason hit on the idea of using a natural effect that would draw little attention to itself, one he explains below. An amateur astronomer and interstellar travel enthusiast who worked at the Miami Space Transit Planetarium and volunteered at the Weintraub Observatory atop the adjacent Miami Museum of Science, Jason now makes his home in Fairbanks (AK). He was the historian for the Poker Flat Research Range sounding rocket launch facility near Fairbanks. His space history and advocacy articles have appeared in Quest: The History of Spaceflight magazine and Space News. by James Jason Wentworth...
New Insights into Titan
It's hard to consider a place with surface temperatures of -180°C 'Earthlike,' but there are reasons why we see the term so often applied to Titan. The most striking of these is the presence of surface lakes and seas, a phenomenon found nowhere else in the Solar System. The temperatures are cold enough to make the circulating fluid liquid methane and ethane rather than water, but we see things in Cassini imagery that are strikingly familiar, including seas fed by river-like channels and large numbers of shallow lakes that appear in flatter areas. The European Space Agency's Thomas Cornet has been leading a team investigating Titan's surface features in greater detail. In particular, the lakes of Titan do not appear to be fed by rivers, making it likely that they are filled either by rainfall or by liquids welling up from below. Empty depressions can be found where lakes may once have been, and it is believed that some of the lakes dry out during Titan's thirty-year cycle of...
Kepler-138b: A Mars-Size Exoplanet
Astronomers at Penn State, NASA Ames, the University of Chicago and the SETI Institute are publishing news of an exoplanetary first: A planet smaller than Earth whose mass and size have both been measured. Kepler-138b is a Mars-sized world orbiting a red dwarf about 200 light years from Sol in the constellation Lyra. This is transit work, focusing on a system with two other transiting worlds, all three of which are too close to their parent star to make life a likely possibility. If we look back at how far exoplanet research has come in the last fifteen years, it's startling to realize that Kepler-138b, with a mass of about 6.7 percent that of the Earth, is 3000 times less massive than the first planet whose density was measured. That's the word from Eric Ford (Penn State), a co-author on the study, which is being published today in Nature, and I assume he's talking about HD 209458 b, whose size and density were first measured in 1999. Previous work on the Kepler-138 system had...
Interplanetary Updates: Philae and New Horizons
Given that the Philae lander has just come to life after seven months without communicating, it's no wonder that the mood among everyone involved with Rosetta's mission to comet 67P/Churyumov-Gerasimenko is exuberant. On the surface of the comet, conditions have been improving for Philae since March, meaning that with higher temperatures and better illumination, it was hoped that the lander might reactivate. That hope was realized on June 13 when Rosetta picked up 330 data packets from an earlier segment of the lander's mission. Stephan Ulamec (DLR), Philae lander project manager, has positive things to say: "We are still examining the housekeeping information at the Lander Control Centre in the DLR German Aerospace Center's establishment in Cologne, but we can already tell that all lander subsystems are working nominally, with no apparent degradation after more than half a year hiding out on the comet's frozen surface." Image: Processed NAVCAM image of Comet 67P/C-G taken on 5 June...
A Cometary Reawakening
In a summer already packed with interesting missions, we also have the unusual phenomenon of spacecraft ‘waking up’ after unexpected periods of dormancy. The European Space Agency’s Philae lander, which shut down on November 15, 2014 after operating on comet 67P/Churyumov-Gerasimenko for about sixty hours, came out of its hibernation on June 13. ESA reports more than 300 data packets have been received and are being analyzed. Image: Twitter lit up with news of Philae’s reappearance. Be sure to track @ESA_Rosetta to keep up with the latest. This first contact since November lasted for 85 seconds, and according to reports from ESA, made it apparent that the lander had been retrieving data during the time of communications blackout. This ESA update notes that there are more than 8000 data packets in Philae’s memory that can be accessed (we hope) on the next contact, giving us information about the lander’s most recent activity as the comet and orbiting Rosetta continue toward...
Pluto: Surface Features Emerging
New imagery from New Horizons continues to dazzle, with the images below taken by the spacecraft's Long Range Reconnaissance Imager (LORRI) instrument from May 29 to June 2. We're beginning to pick up bright areas mixed with dark terrain in what are clearly the best images ever obtained of the remote world. As before, mission scientists are using deconvolution to sharpen the raw images and are also teasing out further details with contrast adjustments. The processing can produce artifacts so that fine details will have to be checked at closer range. Image: These images, taken by New Horizons' Long Range Reconnaissance Imager (LORRI), show four different "faces" of Pluto as it rotates about its axis with a period of 6.4 days. All the images have been rotated to align Pluto's rotational axis with the vertical direction (up-down) on the figure, as depicted schematically in the upper left. From left to right, the images were taken when Pluto's central longitude was 17, 63, 130, and 243...
Ceres Up Close (and a Bit of Bradbury)
I know I'm going to remember the summer of 2015 for a long time. The confluence of deep space missions has brought new images every week, including the latest view of Ceres and its enigmatic bright spots, which appears below. I'm already bracing myself for that Voyager-like sense of deflation once New Horizons gets past Pluto/Charon and the long-anticipated targets dwindle. Pluto has a special place for some of us because we grew up with it being considered the ninth planet. Dwarf planet or not, it's the final act of a classic Solar System tour. Not that we won't be returning to many of these places, but the timing is uncertain and once Juno finishes its work at Jupiter, we'll have no missions on their way to the outer planets. That makes this summer both energizing and a bit poignant, but let's enjoy it while we can. This view of Ceres, taken on June 6, really is spectacular. We're seeing the dwarf planet from 4400 kilometers as Dawn flies its second mapping orbit. The resolution is...
Volcanism and Astrobiology
A question in a grad school astrobiology seminar at the University of Washington prompted Amit Misra to go to work on plate tectonics. The movement of huge blocks of a planetary surface is beneficial to life because it prompts recycling, as materials move back and forth between the inside of the planet and the atmosphere. We've learned a lot about plate tectonics on Earth, but the seminar question stuck with Misra. How could we detect plate tectonics on an exoplanet? The result is a paper in press at Astriobiology. Misra and colleagues make the case that transient sulfate aerosols produced by volcanic outgassing could provide just the signature scientists need. Explosive volcanic events produced by subduction at the edges of tectonic plates inject such aerosols directly into the atmosphere, where they can persist over periods of months to years. The paper argues that future instruments like the James Webb Space Telescope or the European Extremely Large Telescope (E-ELT) will be able...
Sail in View
The main post for today will be online around 1230 EDT (1630 UTC), but first I have to publish this image from LightSail, along with Jason Davis' description. Nice work! "The Planetary Society's LightSail test mission successfully completed its primary objective of deploying a solar sail in low-Earth orbit, mission managers said today [June 9]. During a ground station pass over Cal Poly San Luis Obispo that began at 1:26 p.m. EDT (17:26 UTC), the final pieces of an image showcasing LightSail's deployed solar sails were received on Earth. The image confirms the sails have unfurled, which was the final milestone of a shakedown mission designed to pave the way for a full-fledged solar sail flight in 2016." A second image may include a view of the Earth, according to Davis. What may happen next is a further tensioning, or 'walking out,' of the sail booms, which should further flatten the sail. Davis notes, too, that the 'fish-eye' lens of the camera produces a bit of distortion in the...
Mission Updates Far and Near
The Planetary Society's Emily Lakdawalla tells us (via Twitter) that she has a history with jigsaw puzzles, one that finally paid off in the image below. You're looking at her work on a partially de-scrambled image from LightSail, fragmentary because the entire image was not downloaded during a Cal Poly (San Luis Obispo) overflight on the afternoon of the 8th. The complete image should be downloaded later today, and perhaps shown at an upcoming press conference with LightSail engineering team leaders scheduled for Wednesday June 10 at 1730 UTC (1330 EDT). At any rate, LightSail's deployed sails are in view. Bill Nye, CEO of The Planetary Society, was on National Public Radio yesterday (audio here) in a brief spot in which he described the unfurling of the solar sail as a 'sail Mary pass,' a longshot required by circumstance as the spacecraft continued to tumble. If the phrase 'sail Mary pass' is inscrutable to you, you may not be familiar with American football, where 'hail Mary...
LightSail Deployment Apparently Successful
After a nerve-wracking week in which contact was repeatedly lost and then regained, The Planetary Society's LightSail has successfully charged its batteries and deployed its solar sail. Deployment began at 1947 UTC (1547 EDT) June 7, just off the coast of Baja California, with telemetry showing climbing motor counts and power levels consistent with ground testing. In a late afternoon update, Jason Davis also noted that the spacecraft's cameras were on (see Deployment! LightSail Boom Motor Whirrs to Life). If you're following this mission closely, you'll want to know about Ted Molczan's page LightSail-A: Estimated Post-Sail Deployment Orbital Elements, with early predictions on orbital decay with the sails extended. Bonnie Link (hflink.com) produced a map showing Monday's LightSail passes over North America that you can see below. Here the white boxes are UTC times. The green arcs are sunlit, the blue in shadow and thus not visible. Further confirmation of sail deployment came in a...
The View from Outside the Galaxy
The Russian Federal Space Agency (Roscosmos) has recently released a video (viewable here on YouTube) showing how a number of celestial objects might look if they were substantially closer to Earth than they are. The image of the Andromeda galaxy and its trillion stars projected against an apparent Earthscape is below. Unfortunately, this seems to be an astronomical image inserted into a view that purports to show what we would see in visible light. What we would actually see if we were standing in such a location is much different. After all, astronomical images are teased out of lengthy exposures in carefully chosen wavelengths. In reality the Andromeda galaxy is gigantic even when viewed from 2.5 million light years, but I doubt the average person has any idea where it is in the sky. Although considerably wider than the Moon as seen from Earth, M31 is visually faint, a fact that reminds us of the importance of photographs and charged coupled devices (CCDs) in light gathering as we...
Science Fiction: An Updated Solar System
Having written yesterday about the constellation of missions now returning data from deep space, I found Geoffrey Landis' essay "Spaceflight and Science Fiction" timely. The essay is freely available in the inaugural issue of The Journal of Astrosociology, the publication of the Astrosociology Research Institute (downloadable here). And while it covers some familiar ground -- Jules Verne's moon cannon, Frau im Monde, etc. -- it also highlights Landis' insights into the relationship between the space program and the genre that helped inspire it. My friend Al Jackson has written in various comments here (and in a number of back-channel emails) about Wernher von Braun's ideas and their relation to science fiction. As Landis notes, von Braun was himself a science fiction reader who credited an 1897 novel called Auf Zwei Planeten (Two Planets) by Kurd Lasswitz with inspiring his interest in rocketry. So, by the way, did Walter Hohmann, the German engineer who helped develop the area of...
Mission Data: An Early Summer Harvest
What a time for space missions, with data returning from far places and a nail-biter close at hand. On the latter, be advised that the LightSail mission team has decided to divide sail deployment into two operations, one of them starting today as the CubeSat's solar panels are released and an imaging session verifies the craft is ready for sail deployment. The actual deployment will then follow on Friday, and is currently scheduled for 1647 UTC (1247 EDT). From Jason Davis: The first indication the sail sequence has started should come from the spacecraft's automated telemetry signals, which include a motor revolution count for the boom system. The next few orbits will be used to check LightSail's health and status, transfer imagery from the cameras to flight computer, and begin sending home to Earth.The last contact of the day comes during a Cal Poly ground pass at 4:16 p.m. EDT (20:16 UTC). By then, the team hopes to at least part of a sail image on the ground. If not, the next...