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Nuptse

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2. Gerlinde Kaltenbrunner Makes Pure Ascent Of Nuptse

In May, German climber Gerlinde Kaltenbrunner, the first woman to climb all fourteen 8000-meter peaks without supplemental oxygen, made an unusual ascent of Nuptse along with climbing partner David Gottler. The pair climbed the 7861-meter (25,791 ft) mountain (located in Nepal, not far from Everest) in the alpine style, without the use of Sherpa support, fixed ropes, or bottled oxygen. Each of those elements is crucial to most expeditions in the Himalaya these days, and to go without any of them is almost unheard of. But Kaltenbrunner and Gottler eschewed all of those comforts in pursuit of a more challenging, yet pure, ascent, making it one of the most impressive climbs of the year.

-- Kraig Becker

Image: Gerlinde Kaltenbrunner during her and partner David Gottler's alpine style ascent of Nuptse (Credit: Gerlinde Kaltenbrunner)


Paraglide

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3. Ueli Steck Climbs and Paraglides Three Alpine Peaks in a Single Day

Swiss mountaineer Ueli Steck is amongst the best climbers in the world and he often finds interesting projects to test his set of unique skills. This year he also discovered a love for paragliding, and his two passions came together in impressive fashion on one day in August. On that day, Steck managed to string together a series of summits on the Jungfrau, Mönch, and Eiger by speed climbing each of the mountains and paragliding from one to the next. The expedition began early in the morning and Steck glided from the summit of the Eiger back to his car by 5:00 PM, getting him home in time for dinner.

-- Kraig Becker

Image: Ueli Steck prepares to paraglide between climbs (Credit: Ueli Steck).

Second Seven Summits

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4. Italian Mountaineer Becomes First To Climb “Second Seven Summits”

At first glance, one wouldn’t think that summiting the 4851-meter (15,916 ft) Mt. Tyree, located in Antarctica, would make a list of the most impressive climbs of 2012. But when Italian climber Hans Kammerlander did it last January he also completed his quest to climb the “Second Seven Summits” – the second tallest mountains on each of the seven continents. For years, climbing the Seven Summits has been a badge of honor amongst climbers, but it turns out the Second Seven are even more challenging to complete. The list includes Mt. Kenya (Africa, 17,057'), K2 (Asia, 28,251'), Dykh-Tau (Europe, 17,076'), Mt. Logan (North America, 19,550'), Ojos del Salado (South America, 22,614'), Puncak Trikora (Australasia, 15,617'), and Mt. Tyree. Kammerlander became the first to accomplish the feat, earning his spot in mountaineering history in the process.

-- Kraig Becker

Image: Hans Kammerlander on the summit of Mt. Tyree, Antarctica. (Credit: Hans Kammerlander)

Mazeno Ridge

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5. First Ascent of the Mazeno Ridge

No climb in 2012 was as big or bold as the first ascent of the Mazeno Ridge, an 8-mile long route that culminates at the summit of Pakistan’s Nanga Parbet, the ninth tallest mountain in the world at 8126 meters (26,660 ft). The ridge features eight sub-summits of more than 7000 meters (22,965 ft) in height, and completing the route was a harrowing marathon for climbers Sandy Allan and Rick Allen, who faced incredibly bad weather and treacherous snow conditions on their way to the top. The climb was expected to take eight days to complete, but the expedition actually stretched to 18; by the time the two men stood on top, they were out of food, fuel and water. The descent was equally difficult, due to exhaustion and a lack of supplies, but when Allan and Allen returned to Base Camp, they had completed the most impressive mountaineering accomplishment in the past decade or more.

-- Kraig Becker

Image: The Mazeno Ridge (Credit: Doug Scott)

Jan 1, 2013

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Star Formation in Milky Way

This image displays a spectacular three-colour composite image of RCW38, obtained through three near-infrared filters. This is a region in the Milky Way at a distance of about 5,000 light years, where stars which have recently formed in clouds of gas and dust are still heavily obscured and cannot be observed in the visible part of the spectrum. Contrarily, as this image shows, they are very well seen at infrared wavelengths where the obscuration is substantially lower. The diffuse radiation is a mixture of starlight scattered by the dust and gas in the area, and atomic and molecular hydrogen line emission.

Image: ESO [high-resolution]

Caption: ESO

Jan 2, 2013

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Galactic Bar and Ring

The NASA/ESA Hubble Space Telescope provides us this week with a spectacular image of the bright star-forming ring that surrounds the heart of the barred spiral galaxy NGC 1097. In this image, the larger-scale structure of the galaxy is barely visible: its comparatively dim spiral arms, which surround its heart in a loose embrace, reach out beyond the edges of this frame.

This face-on galaxy, lying 45 million light-years away from Earth in the southern constellation of Fornax (The Furnace), is particularly attractive for astronomers. NGC 1097 is a Seyfert galaxy. Lurking at the very centre of the galaxy, a supermassive black hole 100 million times the mass of our Sun is gradually sucking in the matter around it. The area immediately around the black hole shines powerfully with radiation coming from the material falling in.

The distinctive ring around the black hole is bursting with new star formation due to an inflow of material toward the central bar of the galaxy. These star-forming regions are glowing brightly thanks to emission from clouds of ionised hydrogen. The ring is around 5000 light-years across, although the spiral arms of the galaxy extend tens of thousands of light-years beyond it.

NGC 1097 is also pretty exciting for supernova hunters. The galaxy experienced three supernovae (the violent deaths of high-mass stars) in the 11-year span between 1992 and 2003. This is definitely a galaxy worth checking on a regular basis. However, what it is really exciting about NGC 1097 is that it is not wandering alone through space. It has two small galaxy companions, which dance “the dance of stars and the dance of space” like the gracious dancer of the famous poem The Dancer by Khalil Gibran.

The satellite galaxies are NGC 1097A, an elliptical galaxy orbiting 42 000 light-years from the centre of NGC 1097 and a small dwarf galaxy named NGC 1097B. Both galaxies are located out beyond the frames of this image and they cannot be seen. Astronomers have indications that NGC 1097 and NGC 1097A have interacted in the past. This picture was taken with Hubble’s Advanced Camera for Surveys using visual and infrared filters. A version of this image was submitted to the Hubble’s Hidden Treasures image processing competition by contestant Eedresha Sturdivant.

Image: NASA/ESA/Hubble [high-resolution]

Caption: Hubble Heritage Team

Mandelbrot's Vision

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Mandelbrot's Vision

Mandelbrot assembled this collage as a suggested cover design for his 1975 treatise Fractals: Form, Chance, and Dimension. The profusion of straight lines is an abstract interpretation of stars, while at right are the natural forms Mandelbrot tried to simulate with his own mathematics.

"My idea is that he put these two things together to show the difference between straight lines, Euclidean geometry, and his new invention which was fractal geometry, the broken lines," speculated Samuel. "It was not taken. The editors said, 'This is too much image. It looks too crazy!'"

Image: Benoît Mandelbrot. Collection Aliette Mandelbrot.[high-resolution]

The Importance of Drawing

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The Importance of Drawing

Often Mandelbrot and his peers — the drawing above was penned by Adrien Douady and John Hubbard, who made vital contributions to the mathematics which took Mandelbrot's name — eschewed computers in favor of drawing by hand. Though computer limitations played a role in this choice, there was something cognitively powerful about having a direct, manual connection to their work.

"In order to relate the visual shapes that appeared on a computer's screen to mathematical theory, they had to be worked with," explained Samuel. "The hand was used to understand the structure."

Image: Adrien Douady & John Hubbard. Private collection. [high-resolution]


Becoming the Mandelbrot Set

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Many people know Benoît Mandelbrot from the computer screensavers of a pre-LCD era. Others have a deeper understanding of his mathematics, the repeating geometries that earned him the sobriquet Father of Fractals. Less appreciated, though, is the process underlying his work: Mandelbrot relied as much for guidance on visual imagery as whiteboard formulae. Primitive computer printouts were his maps to uncharted mathematical terrain, their dot-matrix patterns a "here be dragons" for the exploration of dynamical systems and chaos theory.

In 2008, fascinated by the interplay between imagery and scientific investigation, art historian Nina Samuel spent two weeks interviewing Mandelbrot in his Cambridge, Massachusetts home. After Mandelbrot passed away in 2010, she was allowed entry to his office, collecting some 300 printouts, sketches and notebook scribbles now on display in The Islands of Benoît Mandelbrot: Fractals, Chaos, and the Materiality of Thinking, an exhibition at the Bard Graduate Center in Manhattan.

"There is such an organic quality to these images," said Samuel. "These are the images the scientists used when they were working, and not what was found on magazine covers or popularized in screensavers."

The exhibition runs until Jan. 27, but for readers not fortunate enough to visit, Samuel took Wired on a guided virtual tour. Each entry is followed by links to high-resolution versions of the images.

Below:

Becoming the Mandelbrot Set

The image below comes from a series of 120 prints, some composed of seemingly stray dots and others almost completely blank, that preceded Mandelbrot's discovery of the fractal set that bears his name (visualized above, as produced by a modern pattern generator).

"If you look at the shadows, you can see the resemblance," Samuel said of the early image. "Later on, he could have seen the shapes that became famous." But at the time, Mandelbrot saw only an undefined something, a hint of what needed next to be done.

"Mandelbrot would never say that an image was a proof, but an image would lead to conjecture, open up the imagination, and then you could prove something with formulas," said Samuel.

Images: 1) Geek3/Wikimedia Commons [high-resolution] 2) Benoît Mandelbrot and Mark Laff, programmer. Collection Aliette Mandelbrot. [high-resolution]

Jan 3, 2012

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Vesta Crater in 3D

This composite-color view from NASA's Dawn mission shows Cornelia Crater, streaked with dark materials, on the giant asteroid Vesta. The data were obtained by Dawn's framing camera during the mission's high-altitude mapping orbit, about 420 miles (680 kilometers) above the surface. The images were integrated into a mosaic and wrapped on a topographical model of Vesta's surface.

Scientists colorized the picture by assigning red to the 0.75-micron wavelength, green to the 0.92-micron wavelength and blue to the 0.98-micron wavelength.

The Dawn mission to Vesta and Ceres is managed by NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, for NASA's Science Mission Directorate, Washington. UCLA is responsible for overall Dawn mission science. The Dawn framing cameras were developed and built under the leadership of the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, with significant contributions by DLR German Aerospace Center, Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig. The framing camera project is funded by the Max Planck Society, DLR, and NASA/JPL.

Image: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA [high-resolution]

Caption: NASA

Jan 4, 2013

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Prominent Solar Flare

A solar eruption gracefully rose up from the sun on Dec. 31, 2012, twisting and turning. Magnetic forces drove the flow of plasma, but without sufficient force to overcome the sun’s gravity much of the plasma fell back into the sun. The length of the eruption extends about 160,000 miles out from the Sun. With Earth about 7,900 miles in diameter, this relatively minor eruption is about 20 times the diameter of our planet.

See video and relative size of Earth to eruption on 'Solar Ballet on the Sun' feature.

Image: NASA/SDO [high-resolution]

Caption: NASA

Jan 5, 2013

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Colorful Lunar Mare

Galileo false-color image of the Mare Tranquillitatis and Mare Serenitatis areas of the Moon. The picture was made from four exposures taken during Galileo's second Earth/Moon flyby. The colors are enhanced to highlight compositional differences.

Mare Tranquillitatis at left appears blue due to titanium enrichment. Orange soil in Mare Sarenitatis at lower right indicates lower titanium. Dark purple areas at left center mark the Apollo 17 landing site, composed of explosive volcanic deposits. Red lunar highlands indicate low iron and titanium. Mare Serenitatis is roughly 1300 km across and North is at 5:00. The 95 km diameter crater Posidonius, centered at 32 N, 30 E, is at the middle of the bottom of the frame.

Image: NASA [high-resolution]

Caption: NASA

Dot Physics

The Extremo Files

Rocket Shop


Superbug

Social Dimension

Beyond Apollo

Elemental

Eruptions

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