Shuttle Education

Shuttle Education
In Orbiter Processing Facility-3 at NASA's Kennedy Space Center in Florida, members of the STS-130 crew view a demonstration on the maintenance of space shuttle Endeavour's thermal protection system.

From left are: Mission Specialist Kathryn Hire, Commander George Zamka, Mission Specialist Nicolas Patrick and Pilot Terry Virts.

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NASA Ames Plays Key Role in Proposed Space Missions

Computer simulated global view of VenusScientists at NASA’s Ames Research Center, Moffett Field, Calif., are contributing to proposed missions to probe the atmosphere and crust of Venus and return a piece of a near-Earth asteroid for analysis on Earth.

Ames has a role in two of the winning proposals NASA selected as candidates for the agency's next space venture to another celestial body in our solar system. NASA will select one proposal for full development in mid-2011 after detailed mission concept studies are completed and reviewed. The final project may provide a better understanding of Earth's formation or perhaps the origin of life on our planet.

Each winning proposal team initially will receive approximately $3.3 million in 2010 to conduct a 12-month mission concept study that focuses on implementation feasibility, cost, management and technical plans. Studies also will include plans for educational outreach and small business opportunities. The studies will begin this year, and the selected mission must be ready for launch no later than Dec. 30, 2018. Mission cost, excluding the launch vehicle, is limited to $650 million.

"These are projects that inspire and excite young scientists, engineers and the public," said Ed Weiler, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington. "These three proposals provide the best science value among eight submitted to NASA."

The Surface and Atmosphere Geochemical Explorer, or SAGE, mission to Venus would release a probe to descend through the planet's atmosphere. During descent, instruments would conduct extensive measurements of the atmosphere's composition and obtain meteorological data. The probe then would land on the surface of Venus, where its abrading tool would expose both a weathered and a pristine surface area to measure its composition and mineralogy. Scientists hope to understand the origin of Venus and why it is so different from Earth. Larry Esposito of the University of Colorado, Boulder, is the principal investigator.

Asteroid 951 GaspraTony Colaprete and Kevin Zahnle, both research scientists at NASA Ames, are SAGE science team co-investigators. Colaprete also is the principal investigator of the SAGE Atmospheric Structure Investigation (ASI) and instrument package. The ASI instrument package will measure pressure, temperature and wind as the probe descends from the top of its atmosphere, approximately 93 miles high, to the surface. NASA Ames also is responsible for the SAGE Instrument Control Module, which interfaces with each module and the lander. The instrument package will determine Venus's atmospheric structure, stability and composition, using sensors, including an Inertial Measurement Unit. The unit includes accelerometers and gyroscopes; a temperature and pressure measuring assembly, to measure temperature, dynamic and static pressure and determine the spacecraft's descent speed; and an anemometer to measure surface wind speed.

“We can build a coherent picture of Venus's atmospheric profile by taking direct measurements in unprecedented accuracy and resolution with a unique set of sensors as SAGE flies through the atmosphere,” Colaprete said. “Wind speed, direction and the rate at which the atmosphere overturns are critical to understanding the chemistry of the atmosphere and how it interacts with the surface.”

Zahnle is part of a team that will interpret the abundances of gases in Venus's atmosphere measured by SAGE as it descends to the planet's surface. Zahnle will focus on the presence of noble gases, such as helium and neon, but particularly xenon.

"Noble gases are both rare on planets like Earth and Venus and chemically inert, but they accumulate in the atmosphere," Zahnle said. "This makes them accessible to a probe like SAGE."

Some of the noble gases are made by radioactive decay of rock-forming elements like potassium and uranium, which enter the atmosphere through volcanic eruptions.

"Some noble gases can be used to determine the geologic history of Venus because radioactive decay acts as a kind of clock," Zahnle explained. "Other noble gases are primordial, in the sense that they formed before the planets, and can be used to determine the origin and earliest evolution of planets and their atmospheres."

The Origins Spectral Interpretation Resource Identification Security Regolith Explorer spacecraft, called OSIRIS-REx, would rendezvous and orbit a primitive asteroid. After extensive measurements, instruments would collect more than two ounces of material from the asteroid's surface for analysis on Earth. The returned samples would help scientists better understand and answer long-held questions about the formation of our solar system and the origin of complex molecules necessary for life. Michael Drake of the University of Arizona in Tucson, is the principal investigator.

Scott Sandford, research scientist at NASA Ames, an OSIRIS-REx science team co-investigator, will assess and control spacecraft contamination, particularly for organic particles that may appear during the design, construction, flight or recovery of the spacecraft.

While at the asteroid, the OSIRIS-REx will study the asteroid's shape, rotation and other features. Scientists then will analyze the sample to identify the minerals and organics that comprise the asteroid.

"We are hoping to find out what the true composition of organic-rich asteroids are and find out what sort of impact hazards and potential space resources they represent," said Sandford.

Sandford also will help organize and lead a portion of the Preliminary Examination Team that will study and analyze the organic particles present in the returned samples, as well as assess the cleanliness of the sample return capsule (SRC).

"When the SRC re-enters Earth's atmosphere, the spacecraft lets atmospheric air into the capsule," explained Sandford. "However, we don't want that air to also suck in contamination that will ruin the samples."

To prevent contamination, the SRC will be equipped with an air filter to protect the sample. Sandford brings his experience testing filter designs from his work on NASA's Stardust mission to collect comet dust and NASA's Genesis mission to collect solar wind particles.

Sandford also is part of another science team that will study a force that acts on rotating bodies in space, known as the Yarkovsky effect, which can cause asteroids to change their orbits. Data from the mission science instruments can also be compared with data from Earth-based telescopes. These comparisons will help scientists understand the nature of asteroids in our solar system.

"This is a key issue for being able to predict the orbits of asteroids and determine their dangers as impact hazards," said Sandford. "The science instruments also will measure the composition of the asteroid even before we get samples back."

After the samples have been analyzed, Sandford will work with the Astromaterials Research and Exploration Science Directorate at NASA's Johnson Space Center, Houston, to organize their distribution to various organizations and researchers.

In addition to science team support, the Human-Computer Interaction Group at NASA Ames is developing software for the science processing and operations center at the University of Arizona, Tuscon.

If OSIRIS-REx is selected as a mission, NASA Ames also will provide thermal protection systems support by completing heat shield and design testing and verification in the NASA Ames arc jet facilities.

The proposals were submitted to NASA on July 31, 2009, in response to the New Frontiers Program 2009 Announcement of Opportunity. New Frontiers seeks to explore the solar system with frequent, medium-class spacecraft missions that will conduct high-quality, focused scientific investigations designed to enhance our understanding of the solar system. The New Frontiers Program is managed by NASA's Marshall Space Flight Center, Huntsville, Ala., for NASA Headquarters.

The final selection will become the third mission in the program. New Horizons, NASA’s first New Frontiers mission, launched in 2006, will fly by the Pluto-Charon system in 2015, then target another Kuiper Belt object for study. The second mission, called Juno, is designed to orbit Jupiter from pole to pole for the first time, conducting an in-depth study of the giant planet's atmosphere and interior. It is slated for launch in August 2011.

For more information about the New Frontiers Program, visit the New Frontiers program site.

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NASA Reveals New Batch Of Space Program Artifacts

NASA is inviting eligible education institutions, museums and other organizations to examine and request space program artifacts online. The items represent significant human space flight technologies, processes and accomplishments from NASA's past and present space exploration programs.

NASA partnered with the General Services Administration to provide a first-of-its-kind, Web-based, electronic artifacts prescreening capability last year. On Oct. 1, 2009, the GSA launched a Web initiative for screening and requesting NASA's space shuttle artifacts. The first round ended Nov. 30, and all 913 artifacts were allocated.

A second Web-based screening opportunity begins Tuesday. It includes approximately 2,500 potential artifacts from NASA programs that include the space shuttle, Hubble Space Telescope, Apollo, Mercury, and Gemini. It is available at:

http://gsaxcess.gov/NASAWel.htm

Each artifact will be screened for 90 days. After the screening period closes, and at the completion of the allocation process, requestors will be notified about the status of their request.

Museums and schools will be screened for eligibility through an online registration process or through their state agency for surplus property. Eligible recipients may view the available artifacts and request specific items at the Web site. Prescreening allows potential recipients to identify specific items and provides the time to plan to transport, preserve and properly display artifacts.

Requesting an artifact through the prescreening process does not guarantee the item will be available. Nor does it provide a specific time when it will become available. Allocated artifacts will be incrementally released as they are no longer needed by NASA and in accordance with export control laws and regulations.

Although the artifacts are provided without charge, eligible recipients must cover shipping and any special handling costs. Shipping fees on smaller items will be relatively inexpensive, while larger items may involve extensive disassembly, preparation, shipping and reassembly costs. NASA will work closely with potential recipients, on a case-by-case basis, to address any unique special handling costs.

For information about NASA's space shuttle transition and artifacts, visit

http://www.nasa.gov/transition

For information about NASA and agency programs, visit:

http://www.nasa.gov

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The Cat’s Paw

The Cat's Paw (NGC 6334). Imaged at the ESO. Click for a larger version. Credit: ESO

Just look at this! The ESO has outdone themselves this time. I’m glad too because given my location it would be pretty much right on the horizon and throw in the local geography I’d probably never get to see it otherwise.  If you click on the ESO link below you will get more and larger versions of the image.

The ESO press release:

Few objects in the sky have been as well named as the Cat’s Paw Nebula, a glowing gas cloud resembling the gigantic pawprint of a celestial cat out on an errand across the Universe. British astronomer John Herschel first recorded NGC 6334 in 1837 during his stay in South Africa. Despite using one of the largest telescopes in the world at the time, Herschel seems to have only noted the brightest part of the cloud, seen here towards the lower left.

NGC 6334 lies about 5500 light-years away in the direction of the constellation Scorpius (the Scorpion) and covers an area on the sky slightly larger than the full Moon. The whole gas cloud is about 50 light-years across. The nebula appears red because its blue and green light are scattered and absorbed more efficiently by material between the nebula and Earth. The red light comes predominantly from hydrogen gas glowing under the intense glare of hot young stars.

NGC 6334 is one of the most active nurseries of massive stars in our galaxy and has been extensively studied by astronomers. The nebula conceals freshly minted brilliant blue stars — each nearly ten times the mass of our Sun and born in the last few million years. The region is also home to many baby stars that are buried deep in the dust, making them difficult to study. In total, the Cat’s Paw Nebula could contain several tens of thousands of stars.

Particularly striking is the red, intricate bubble in the lower right part of the image. This is most likely either a star expelling large amount of matter at high speed as it nears the end of its life or the remnant of a star that already has exploded.

This new portrait of the Cat’s Paw Nebula was created from images taken with the Wide Field Imager (WFI) instrument at the 2.2-metre MPG/ESO telescope at the La Silla Observatory in Chile, combining images taken through blue, green and red filters, as well as a special filter designed to let through the light of glowing hydrogen.

Giz Explains: SSDs and Why You Wish You Had One [Giz Explains]

Speed. Toughness. Efficiency. Silence. That's why we want solid-state drives in our computers. But we worry about the zoom-zoom performance degrading over time, and the fact that SSDs might eventually wear out. Here's what you need to know about 'em.

Why Solid-State Drives Are Awesome (Or At Least, Better Than Hard Drives)

To understand what's great about SSDs, let's start with HDDs (you know, old-fashioned hard drives). On a basic level, a hard disk drive works thusly: Inside is a magnetized recording surface called a platter that spins around really fast, with a head that zooms across disk to read and write data—think kinda like a record player, except the head never touches the surface, 'cause that would be very, very bad. So, you can see the problem with hard drives: They're fragile (don't drop your computer) and they're slow to access stuff because the head has to physically move to where the data is.


With an SSD, on the other hand, we're talking straight silicon. What's inside is a bunch of flash memory chips and a controller running the show. There are no moving parts, so an SSD doesn't need to start spinning, doesn't need to physically hunt data scattered across the drive and doesn't make a whirrrrr. The result is that it's crazy faster than a regular hard drive in nearly every way, so you have insanely quick boot times (an old video, but it stands), application launches, random writes and almost every other measure of drive performance (writing large files excepted). For a frame of reference, General Manager of SanDisk's SSD group, Doron Myersdorf, says an equivalent hard drive would have to spin at almost 40,000rpm to match an SSD. And, you can drop it—at least, a little.

Secrets of the SSD

Typically, what you've inside an SSD is a bunch of NAND flash memory chips for storage—the same stuff found in memory cards and USB thumb drives—along with a small cache of DRAM, like you'd find on most current hard drives. The DRAM is also flash memory, but the difference between the two is that the storage memory is non-volatile, meaning the data it holds won't go poof when it loses power, while the faster DRAM is volatile memory, so "poof" is exactly what happens to DRAM data when the power goes out. That's fine because it's the faster DRAM is just for caching things, holding them temporarily to make the whole system work faster.

So, let's talk a bit about flash memory itself. I'll try to keep it straightforward and not lose you, because it's key to the benefits and problems with solid-state storage.

Flash memory is made up of a bunch of memory cells, which are made up of transistors. There are two basic kinds of memory: With single-level cell (SLC) memory, one bit of data is stored per cell. (Bits, the basic building block of information, if you recall, have two states, 0 or 1.) The SLC type is fast as hell and lasts a long time, but it is too expensive for storing the dense amounts of data you'd want in a personal computer. SLC memory is really only used for enterprise stuff, like servers, where you need it to last for 100,000 write cycles.

The solution for normal humans is multi-level cell memory. Currently, up to 4 bits can be stored per cell. "Multi-level" refers to the multiple levels of voltage in the cell used to get those extra bits in. MLC SSD drives are much cheaper than SLC but are, as I mentioned, slower, and can wear out faster than their pricier counterpart. Still, for now and going forward into the foreseeable future, all of the SSDs you could come close to owning are of the MLC variety.

The Bad Stuff

Structurally, flash memory is divided into blocks, which are broken down further into pages. And now, we get into one of the major problems with flash. While data can be read and written at the individual page level, it can only be erased at the larger block level. In other words, suppose you have a 256k block and a 4k page, and you want to erase just one page worth of data, you have to erase the whole block, and then write all the rest of the data back to the block.

This is a huge problem, for one, because MLC flash memory wears out after 10,000 write cycles. Two, as the drive fills up, performance significantly degrades. (Anandtech has a pretty great illustration, amidst a massively deep dive on SSDs you should read if you're interested at all, showing this.) That's because without free blocks to write to, you've gotta go through that intensive erase and rewrite cycle, which, as you'd imagine, entails a lot of overhead. Problem numero three is that, according to SanDisk CEO Eli Harari, there's "a brick wall" in the near future, when storage at the chip level could stop increasing in the not-too-distant future.

Mitigating the Bad Stuff

The thing is, you actually probably still want an SSD in your next computer, to make it run awesomer. Because where there are problems, there are sorta solutions. Remember how I mentioned up above the other major component in an SSD, besides the flash memory, is the controller? They're a big part of what differentiates one company's SSD from another's. The controller is the secret sauce, as SanDisk's Myersdorf told me. Because the game, for now, is all about managing flash better, both physically and logically. In other words, it's about algorithms.

The first standard technique for long flash-memory life is wear leveling, which is simply not writing to the same area of the drive over and over again. Instead, the goal is to fill up the entire drive with stuff before you have to start erasing blocks, knowing that erasing and re-writing will use up precious cycles. The problem of "Write amplification"—say you have a 1MB document that ends up causing 4MB worth of writes to the drive because of the whole block and pages problem described above, where you wind up reading, erasing and re-writing a bunch of extra blocks and pages—that is being lowered, says Myersdorf, because drive management is shifting from being block-based to page-based. More granular algorithms with caching and prediction means there's less unnecessary erasing and writing.

The biggest thing is what's called TRIM. As you probably know, when you delete something from your computer, it isn't instantly vaporized. Your OS basically just marks the data as "Hey it's cool to pave over this with new stuff." Your hard drive has no real idea you deleted anything. With the TRIM function, when you delete something, the OS actually tells the SSD, "Hey you can scrub this crap." The SSD dumps the block to a cache, wipes the pages with the stuff you want gone, and copies the stuff you want to keep back to a new block, leaving you with clean pages for the next time you want to write something to the disk. This means better performance when you're saving new stuff, since it handles the read-erase-rewrite dance ahead of time. Windows 7 supports TRIM, and Myersdorf says Windows 8 will be even better for solid-state storage.

As for busting through the brick wall of limited storage, the number of electrons that can reside in a cell, increasing flash memory storage at a pace faster than Moore's Law, right now, Toshiba, who invented NAND flash, is currently the chip capacity king. The company just announced a new 64GB NAND flash module that combines 16 4GB NAND chips. This would seem to be closing in on that wall, which we don't want them to do, because we want the dollar-to-MB ratio to keep dropping. Myersdorf is optimistic (despite his boss's gloomy pronouncement), "There have been several walls in history of the [flash] industry—there was transition to MLC, then three bits per cell, then four—every time there is some physical wall, that physics doesn't allow you to pass, there is always a new shift of paradigm as to how we make the next step on the performance curve."

Okay, the big question then: When are SSDs gonna get seriously affordable? A 160GB version of one of the one of the most acclaimed SSDs, Intel's X25, retails for $470. OCZ's Colossus is a verifiable brick of solid-state storage, and the 1TB model has an MSRP of $2200, though it's going for much more. By contrast, a 1TB WD hard drive is like from a hundred bucks on a bad day. Myersdorf says it's hard to say when the dollar to byte is going to go down absolutely, mostly because of supply and demand, but he did predict that a lot of "mainstream" laptops are gonna have 256GB SSDs in the next 18 months. Oh good, I'll be due for a new laptop right around then.

Thanks to SanDisk for helping us out! Still something you wanna know? Send questions about solid states, solid snakes, or solid shakes here, with "Giz Explains" in the subject line.


Potato Chip Hand Solves the Chip/Keyboard Problem the Japanese Way [Japan]

The age old conundrum of how to eat chips at a keyboard without making a giant mess has finally been solved. So how do you keep your hands clean? By using another hand. A robotic hand.

As this lady demonstrates, you push the button on the shaft to clamp the hand around the chip, which you then shove in the direction of your face. It's soft enough to not completely crush through the chip—which is bad—but still stable enough to carry it without dropping. You might say that there was too much thought and engineering effort going into a problem that nobody needed solving, but you'd be wrong. Very wrong. [ITmedia via Crunchgear]


Poll: Which Is the Most Awesomely Bizarre Science Illustration? | Discoblog

Discoblog readers: We need your help.

If you’ve been reading the DISCOVER blogs this week, you might have caught 80beats’ coverage of the study out suggesting the ultra-tough shell of a deep-sea snail could inspire the next generation of body armor. For reasons that could only be described as “dropping the ball,” we didn’t include the illustration provided by the National Science Foundation. It’s not every day that you get to see a samurai attacking a giant snail, though he probably should’ve brought his Hattori Hanz? sword rather than this spear.

Samurai vs. Snail:

snail

Not to be outdone, the Nature study we covered today, arguing Madagascar’s mammals arrived there via flotilla, came with its own illustration. In it, the happy lemur wins the boat race to the Africa while the sad hippos and lions, too fat to ride, stay on the mainland.

The Great Animal Boat Race:

madagascar

More awesomely bizarre? Please, help us decide:

<br /> <a href=”http://answers.polldaddy.com/poll/2570157/” mce_href=”http://answers.polldaddy.com/poll/2570157/”>Which is the more awesomely bad science illustration?</a><span style=”font-size:9px;” mce_style=”font-size:9px;”>(<a href=”http://www.polldaddy.com” mce_href=”http://www.polldaddy.com”>surveys</a>)</span><br />

Related Content:
80beats: Could a Deep Sea Snail’s Shell Inspire Next-Gen Body Armor?
80beats: Study: Madagascar’s Weird Mammals Got There On Rafts

Images: NSF; Luci Betti Nash

YouTube Redesign Cuts the Chaff, Keeps the Ads [YouTube]

You may have already noticed YouTube looking a little different this week, but now it's official: the site's undergone a major redesign that aims to clear out the clutter.

YouTube's new pared-down look is opt-in at the moment, and up and running internationally. It's a little spartan, but it does make it easier to focus on the video you're watching—and the advertisements packaged with it. Gone is the five-star rating system, replaced with a gladiatorian thumbs up or down. Information about each clip's creator is tucked under the video, while you can view a list of their other offerings and choose to subscribe above it. Actions like sharing, saving, and flagging a video have been reduced to buttons, and you can search while continuing to watch whatever's on your current page.

On the right-hand side of the screen, the "Next UP" box now incorporates the search that brought you there and takes into account your subscriptions, instead of the previous one-video experience.

According to YouTube, the move was made to simplify the user experience and to create a video page that could accommodate a wide range of genres. This is good! What would be better—and what's coming eventually but not available now—is the ability to to customize your viewing page, using this design as a foundation.

One thing that's not going anywhere are the number and placement of ads. That's understandable—it's a business, after all—but I do wonder, if they were taking such a big axe to the design elements of the page, if there may have been a little room to cut those down as well.

It sounds as though there's still room for change, as YouTube monitors and measures user response over the next couple of weeks. But overall, it's a good clean look for all your Muppet music video needs. [YouTube]


Winduino II Instrument Updates The Humble Aeloian Harp To New Octaves [Instruments]

For all four minutes and 34 seconds of the video below, I just zoned out listening to the relaxing noise of wind passing through the Winduino II's Bluetooth board. I fell into a kind of blogger coma.

The Winduino II is made from an Adruino BT Bluetooth board, and is inspired by the Aeolian harp that was used in ye olden days. Hung outside, the wind makes the various sensors tinkle with harmonious sounds of music, and a USB port keeps it charged up if the solar panels on top aren't soaking up enough rays. [Fascination Workshop via Matrixsynth via MAKE]

The Winduino II from Fascination Workshop on Vimeo.


The Flashier the Tit, the Stronger the Sperm (No, Really) | Discoblog

Great-Tit-BirdFlashy tits equals stronger sperm–at least in the bird world.

A recent study of the birds known as great tits, by evolutionary ecologist Fabrice Helfenstein at the University of Bern, Switzerland, found that the more colorful and bright a male tit’s plumage, the stronger the bird’s sperm is.

The study, published in Ecology Letters, explains that the plumage of some birds contains caretenoids–important antioxidants that can help the bird combat cellular damage caused by stress from predators or feeding babies. A higher amount of caretenoids also results in intensely colored plumage in males, signaling the bird’s increased capacity to ward off stress and preserve its sperm from damage.

New Scientist reports:

[Fabrice Helfenstein] tested this by upping the parental workload of wild male great tits, Parus major – which have yellow breast plumage – by adding two extra chicks to their nests. After five days of looking after their big brood, males with paler plumage suffered a greater reduction in sperm motility than more colorful males. Supplementing the birds’ diet with carotenoids markedly improved the sperm quality of the paler males.

Related Content:
80beats: Male Cleaner Fish Punish Females Who Piss Off The Boss Fish
80beats: In Galpagos Finches, Biologists Catch Evolution in the Act
80beats: Rumors of Y Death Are Greatly Exaggerated; Male Chromosome Evolving Like Crazy
80beats: Study: The Chemical BPA, in High Doses, Causes Impotence

Image: iStockphoto

The Palm Pre Plus Can Run 50 (50!) Apps at Once [Palm]

As mentioned in our review, the added RAM in the Palm Pre Plus means you can run "a LOT" of apps. You know, like 10! Absurdist logic site PreCentral asks the obvious question: why not 50?

Anyway, I'm stuck on the third mission of GTA: Chinatown Wars on my iPhone, because I keep getting calls while I'm playing, which shuts down the game completely. So, my question is, is this Pre Plus making fun of me? Because it sure feels that way. [PreCentral]


The Apple Tablet: ‘A First-Generation iPhone That’s Met Its Match With a Rolling Pin’ [Rumor]

According to AppleInsider's sources, this flickr image is the closest mockup of the Apple Tablet that anyone has seen to date. And yes, it's essentially a big, first-gen iPhone that's "met its match with a rolling pin."

Rather than a plastic back, AI claims the Tablet will have the same, two-tone aluminum look of the original iPhone. But while this image is thought to be very close to Apple's final design, it doesn't sound like a full-fledged OS X will be on board. Why? The Tablet will have an iPhone-inspired Home button (along with a 10-inch screen, 3.5-mm stereo headphone jack, built-in speaker grills, a microphone, GPS, 3G connectivity and a 30-pin dock connector, if AppleInsider has it right).

Personally, I never grew tired of the iPhone's original look, and I'd love to see the design in tablet form. What about you? [AppleInsider and flickr]


Witnessing suffering | Cosmic Variance

While we’re on the topic of charities, it seems appropriate to note that this is a particularly opportune time to donate to an exceedingly worthwhile charity: Doctors Without Borders. They are doing amazing work around the world, and the current tragedy in Haiti is no exception.

port-au-prince exodus (Maggie Steber for NYT)Note that Doctors Without Borders (more generally known as Médecins Sans Frontières) is not the same as Doctors of the World (Médecins du Monde; now called HealthRight). It’s somewhat ironic, but the Doctors couldn’t agree about how to go about saving the world. So MDM split off in 1980 (and is roughly 1/40th the size). The critical issue was the degree to which “witnessing” was a part of their mission. On the one hand, if you want to be able to go anywhere that you’re needed, it’s wise to be explicitly apolitical. Your goal is simply to help the sick and relieve suffering. On the other hand, if you witness atrocities, it seems incumbent upon you to tell the world what has happened. If you are on the ground in the midst of genocide, is it really appropriate to stay silent? Both groups “bear witness” to atrocities, but MSF is more conservative, while MDM is more aggressive.

I think strong arguments can be made for both approaches, and I don’t think you can go wrong supporting either organization. As always, it makes sense to check out any intended recipient of largess on Charity Navigator. Both organizations get essentially identical, stellar scores (implying that the vast majority [~90%] of what you donate goes to people in need, and not to fatten the pay of executives, or into the pockets of Madison Avenue).

Haiti is a tragedy of epic proportions. Here is a way to help.


Study: Madagascar’s Weird Mammals Got There on Rafts | 80beats

madagascar425Just how did all the exotic mammals of Madagascar, like its unique collection of lemurs, originally reach the African island? Did they float there from the African mainland, or did nature provide a land bridge? The question has vexed biologists because both explanations have their problems. But a new study in Nature proposes an answer to the main problem posed by the floating-across-the-channel idea, suggesting that it is the most likely explanation.

Because of the narrow range of biology on Madagascar, most biologists favored the floating rafts hypothesis. But there has always been a problem with this notion: the currents swirling in the channel and the surrounding Indian Ocean would make it virtually impossible for a floating Noah’s Ark of vegetation to reach Madagascar’s shores [AFP]. Were those currents always this way, though? No, says a team led by Matthew Huber.

Huber and his colleagues employed the computer modeling techniques used in modern climate studies to predict backwards. 50 million years ago Africa and Madagascar sat about 1,000 miles (1,600 kilometers) south of their current positions due to continental drift…. By plugging data about the ocean and atmosphere of ancient Earth into modern climate models, Huber and Ali found that ocean currents around the two land masses once flowed eastward, toward Madagascar, after all [National Geographic].

Madagascar’s four groups of land mammals would’ve arrived on the island between 60 and 20 million years ago. The peculiar set of creatures that arrived had always suggested that migration opportunities probably were scarce—otherwise (as with a land bridge) a greater mammalian variety probably would’ve arrived. The rafting hypothesis also matches the reality that none of the mainland Africa’s very large mammals made it to Madagascar. As you can see in the illustrative yet strange image above, you just can’t fit an elephant or hippo in a dinghy… or a natural raft.

Related Content:
80beats: Madagascar Chameleon Makes the Most of a 4-Month Life
80beats: Scientists Find Oddball Right-Side-Up Bat in Madagascar
DISCOVER: A Bridge To Madagascar
DISCOVER: The Deadliest Carnivore, on Madagascar’s fossa

Image: Nature


Landlocked Swiss Hit the Beach at Lake Zurich

Sunbathing on the shores of Lake Zurich, Switzerland

Switzerland s a landlocked country. Whats more, Switzerland is a cold country; even in the middle of summer temperatures can be downright chilly. But the Swiss, stoic to a fault, don’t let the lack of a coastline or the brisk winds sweeping down from the snow-clad summer Alps hinder their summer beach outings. Instead of the ocean they head for the lakes, and one of the more popular places to spend a day at the beach is Lake Zurich.

This 24-mile long lake, which was gouged out by a glacier during the last Ice Age, sits in a densely populated region, surrounded by a beautiful pre-Alpine setting. Although almost a million inhabitants live around the shores of Lake Zurich, a third of the its shoreline is still freely accessible, and residents flock city beach resorts to swim and sunbathe, making the most of the country’s short summer season.

Giant Ferris wheel towers over city beach resort in Zurich

Strandbad Mythenquai resort, located in Zurich proper, offers a long stretch of sandy beach complete with diving platform, children’s playground, barbecue facilities, boutique, massage, aerobics, volleyball, and a good waterfront restaurant, all framed by the spectacular Alps. Close by, Seebad Enge is another popular lakeside resort that features floating rafts, designated women-only areas, massage, Yoga classes and saunas. There’s even a giant Ferris wheel at the resort, which at one time was the tallest in the world. Singapore claimed the title for highest Ferrris wheel in 2008, but Zurich’s wheel still provides stunning views across the lake.

Sunbathers stretch out on expansive lawns surrounding the lake shore

Tourist brochures insist that the lake water climbs to 68 degrees in the midst of summer, and that folks actually swim in it, but on the day I strolled along its shores few had ventured into the water. I am, however, willing to give them the benefit of the doubt – it was rather gray and drizzly that day. And even in these less-than-perfect conditions, scores of people were sprawled on lawns and splayed on docks jutting into the lake, as if daring the sun to peek through the cloud cover.

Photo Credits: Barbara Weibel

Article by Barbara Weibel of Hole In The Donut Travels

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Our ice is disappearing | Bad Astronomy

If you are a normal person trying to figure out who is right and who is wrong on an issue, it can be pretty confusing. When it comes to things like global warming, there are folks out there who twist, distort, and spin the facts so grievously that it’s hard to tell the difference between what they are doing and outright lying. And when one of them does it, a slew of others pick it up, making the chorus of nonsense self-reinforcing, muddying the waters even more.

We saw this happen with the CRU emails that were hacked — a situation which was nowhere near as important as so many trumped them up to be — and of course we will see it again and again.

To help staunch that, there are two points about global warming I’ve recently come across that I want to make sure are very clear.

1) Some global warming denialists obfuscate what’s going on with Antarctica, saying the ice there is actually growing, not melting. That is patently false. Where it really matters, Antarctic ice is melting.

antarctic_iceloss

As you can see by this NASA graphic from the linked page, Antarctica loses over 100 billion tons of ice per year, the equivalent of about a hundred cubic kilometers (more than 20 cubic miles) of ice. That number is hard to grasp, but it’s the equivalent to the volume of a mountain about 14,000 feet high — or, if you prefer, it’s like saying that one Colorado Rocky Mountain’s worth of ice disappears every year. Just in Antarctica alone.

You may note that the line fitted to the points in that graph is changing its slope, getting steeper with time. I wouldn’t extrapolate that too much, but if true, it means the loss rate is accelerating.

2) The IPCC report in 2007 was a landmark analysis of the current GW situation. It has been attacked repeatedly by denialists, of course. As it happens, in one part of the report they said that Himalayan glaciers may melt away completely by 2035. This turns out to have been based on a report that was not peer-reviewed, and most likely incorrect.

However, this does not mean the entire report is wrong, and it certainly doesn’t even mean that Himalayan glaciers are fine! Quite the opposite, in fact. A new study of Himalayan ice using satellite data shows that the ice is disappearing, and from 2003 to 2009 shrank at a rate of 47 billion tons per year. I’ll be careful to note that the uncertainty in this measurement is about 25% (12 Gt/year) and has a short baseline in time, but even considering that, the loss of Himalayan ice is definitely large and almost certainly increasing — perhaps twice as rapidly now as it was in the past 40 years before the study.

This is supported by a ground-based study of over 600 glaciers being monitored by Chinese scientists, which showed that between 1980 and 1995, 90% of those glaciers were retreating, and in the period of 1995 – 2005, 95% retreated. In other words, the vast majority of the glaciers studied were losing ice, and in more recent years the number of glaciers losing ice increased.

This is all consistent with global loss rates of ice: it’s disappearing faster now than it was in previous decades.

himalayan_glacier

Get a good look at Himalayan glaciers while you still can.

Expect to hear the antiglobal warming crowd crowing over this, and the media misreporting this to sow more doubt about global warming. But the important point to remember is this: the Himalayan ice really is shrinking, and the same thing is happening in Antarctica.

Global warming is real. It’s also getting worse. You can shout, you can scream until you’re red in the face, and you can deny the facts all you want. But facts are pesky: they exist whether you believe in them or not.

My thanks to expert glaciologists Drs. Lonnie Thompson and C. K . Shum for taking time to explain the Himalayan studies to me and for providing me with the numbers from the ground studies.

Glacier image from mckaysavage’s Flickr stream licensed under creative comons.


New (Possibly) Touchscreen BlackBerry Bold Spotted [BlackBerry]

RIM has already been moving away from the trackball to the trackpad, but this new image of a yet to be released device shows neither. All signs point to the first touchscreen BlackBerry Bold.

There's not much more information available beyond the picture, but it's certainly a relief to see an improvement over earlier touchscreen prototypes. And it's even better to see RIM continuing to innovate, although it's likely months before we see this—or the final version of it—in stores. With the BlackBerry Storm having had touchscreen capability for some time, it's only natural to see that technology infiltrate other brands.

But what do all you BlackBerry enthusiasts think? Is this sacrilege, or progress?

UPDATE: Crackberry is reporting that this is almost definitely an early Magnum prototype, which sounds right to me. So expect to see a lot of these design elements sometime this year, though probably not this exact design. [Cell Guru via FoneFrenzy]


Create Your Own Faked iPhone 4.0 Screenshots [Photoshop Contest]

People love trying to trick us with fake shots of unreleased Apple products. We recently received the shot above of the supposed iPhone 4.0 firmware, which we know for a fact is a fake. Can you do better?

It's really easy to fake a screenshot on the iPhone. Simply make what you want in Photoshop, load it onto your phone as a photo and take a photo of the phone with it on the screen. That's clearly what the person who made the above shot did. The above shot is a jailbreak app, but you get the idea.

So what do you hope to see in the iPhone 4.0 software? Go nuts! Send your best entries to me at contests@gizmodo.com with iPhone Fakes in the subject line. Save your files as JPGs or GIFs under 800k in size, and use a FirstnameLastname.jpg naming convention using whatever name you want to be credited with. Send your work to me by next Tuesday morning, and I'll pick three top winners and show off the rest of the best in our Gallery of Champions. Get to it!