Tuesday, November 23, 2010

Acer jumping into Android tablet market with three models

 Acer has decided to join the masses in rolling out a tablet for any and every demographic the company can possibly think of with a line of new 4.8", 7", and 10.1" tablets. The company introduced the products during the Acer global press conference Tuesday, all of which will eventually run Android 3.0 (Honeycomb) when they are released in 2011.
Acer started out its presentation by saying that everyone uses technology differently, and that the future showed a "variety of form factors and devices." Indeed, Acer seems to want to get into all of those markets at once with its new family of tablets, all of which will have dual-core Tegra CPUs and come with Acer's own UI. None of the products have a name yet, nor is their OS ready yet, but the company hopes to have them available to the public in the spring of next year.
The baby of the family will have a 4.8" screen with a resolution of 1024x480 which Acer described as "100 percent smartphone, 100 percent tablet." Those specs make it slightly larger than the already-large HTC Evo with its 4.3" screen, but quite a bit smaller than the 7" tablets out there. But don't worry, Acer has one of those too: the 7" Acer tablet will have a resolution of 1280x800 (just like its 10.1" counterpart). The 10.1" and 4.8" versions have front- and rear-facing cameras, though it was unclear from Acer's presentation whether the 7" version does or not.
According to Engadget's "hands-on" time with the devices, only one of the three would power on (apparently due to the lack of OS), and the one that did turn on was described as "very sluggish" aside from a blazing HD video.

With its new yet-to-be-named tablets, Acer will engage Samsung, RIM, Apple, and a slew of bottom feeders on the latest front of tablet wars. Research firm Strategy Analytics recently said that Apple currently owns 95 percent of the tablet market, but that number is sure to drop once the Android tablets start flooding store shelves.

Arstechnica.com


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Thursday, November 11, 2010

NASA's Fermi Telescope Finds Giant Structure in our Galaxy

WASHINGTON -- NASA's Fermi Gamma-ray Space Telescope has unveiled a previously unseen structure centered in the Milky Way. The feature spans 50,000 light-years and may be the remnant of an eruption from a supersized black hole at the center of our galaxy.
"What we see are two gamma-ray-emitting bubbles that extend 25,000 light-years north and south of the galactic center," said Doug Finkbeiner, an astronomer at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., who first recognized the feature. "We don't fully understand their nature or origin."

The structure spans more than half of the visible sky, from the constellation Virgo to the constellation Grus, and it may be millions of years old. A paper about the findings has been accepted for publication in The Astrophysical Journal.

Finkbeiner and his team discovered the bubbles by processing publicly available data from Fermi's Large Area Telescope (LAT). The LAT is the most sensitive and highest-resolution gamma-ray detector ever launched. Gamma rays are the highest-energy form of light.
Other astronomers studying gamma rays hadn't detected the bubbles partly because of a fog of gamma rays that appears throughout the sky. The fog happens when particles moving near the speed of light interact with light and interstellar gas in the Milky Way. The LAT team constantly refines models to uncover new gamma-ray sources obscured by this so-called diffuse emission. By using various estimates of the fog, Finkbeiner and his colleagues were able to isolate it from the LAT data and unveil the giant bubbles.

Scientists now are conducting more analyses to better understand how the never-before-seen structure was formed. The bubble emissions are much more energetic than the gamma-ray fog seen elsewhere in the Milky Way. The bubbles also appear to have well-defined edges. The structure's shape and emissions suggest it was formed as a result of a large and relatively rapid energy release - the source of which remains a mystery.

One possibility includes a particle jet from the supermassive black hole at the galactic center. In many other galaxies, astronomers see fast particle jets powered by matter falling toward a central black hole. While there is no evidence the Milky Way's black hole has such a jet today, it may have in the past. The bubbles also may have formed as a result of gas outflows from a burst of star formation, perhaps the one that produced many massive star clusters in the Milky Way's center several million years ago.
"In other galaxies, we see that starbursts can drive enormous gas outflows," said David Spergel, a scientist at Princeton University in New Jersey. "Whatever the energy source behind these huge bubbles may be, it is connected to many deep questions in astrophysics."
Hints of the bubbles appear in earlier spacecraft data. X-ray observations from the German-led Roentgen Satellite suggested subtle evidence for bubble edges close to the galactic center, or in the same orientation as the Milky Way. NASA's Wilkinson Microwave Anisotropy Probe detected an excess of radio signals at the position of the gamma-ray bubbles.
The Fermi LAT team also revealed Tuesday the instrument's best picture of the gamma-ray sky, the result of two years of data collection.
"Fermi scans the entire sky every three hours, and as the mission continues and our exposure deepens, we see the extreme universe in progressively greater detail," said Julie McEnery, Fermi project scientist at NASA's Goddard Space Flight Center in Greenbelt, Md.
NASA's Fermi is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden and the United States.
"Since its launch in June 2008, Fermi repeatedly has proven itself to be a frontier facility, giving us new insights ranging from the nature of space-time to the first observations of a gamma-ray nova," said Jon Morse, Astrophysics Division director at NASA Headquarters in Washington. “These latest discoveries continue to demonstrate Fermi's outstanding performance.”

NASA



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