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Kareena Kapoor new sexy wallpapers

Written By AbhiShek Kap!L on Monday, 8 August 2011 | 05:21

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Riya Sen’s– Very Sexy at Tere Mere Sapne film event

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Madhuri Bhattacharya Hot Calendar photos

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Pictures: Six New Natural Landmarks Named

Written By AbhiShek Kap!L on Sunday, 7 August 2011 | 05:58

Lake Bill Chinook, part of The Island National Natural Landmark

Lake Billy Chinook, Oregon

A prairie in the new Kahlotus Ridgetop National Natural Landmark

Kahlotus Prairie, Washington

A picture of Hanging Lake, Colorado, part of the new Hanging Lake National Natural Landmark

Hanging Lake, Colorado

A picture of Barfoot Mountain, Arizona, part of the new Barfoot Park National Natural Landmark

Barfoot Park, Arizona

A picture of the new Round Top Butte National Natural Landmark

Round Top Butte, Oregon

A picture of a dinosaur footprint, part of the new Morrison-Golden Fossil Areas National Natural Landmark.\

Golden Fossil Areas, Colorado

NASA's Juno Spacecraft Headed to Jupiter Friday


An illustration of the Juno spacecraft.
An artist's rendering shows the Juno spacecraft in orbit above Jupiter.
Illustration courtesy NASA/Caltech
Brian Handwerk
Published August 4, 2011
This Friday a NASA spacecraft is slated to launch on a five-year journey toJupiter.
When it arrives, the craft will probe deeper into the gas giant planet than any previous mission, searching for the unseen core hidden below the thick atmosphere. It will also endure the solar system's strongest radiation zone to study the origins of the giant auroras that dance across Jupiter's poles.
The probe—dubbed Juno—will blast off from Florida aboard an Atlas V rocket, starting a 400-million-mile (644-million-kilometer) trek.
When it arrives at Jupiter in 2016, the spacecraft will spend about one Earth year making 33 elliptical polar orbits, skimming as close as 3,100 miles (5,000 kilometers) above the clouds.
Watch NASA video about the Juno mission.
Carrying a suite of eight main science instruments, Juno will collect data on Jupiter's atmosphere that may be key to understanding the birth of our cosmic neighborhood. (Also see "New Model of Jupiter's Core Ignites Planet Birth Debate.")
"We're really trying to understand the origins of Jupiter—how it formed, the role it played in the formation of the rest of our solar system, and what that can tell us about the solar systems that we're discovering around other stars now," said Juno's principal investigator, Scott Bolton, of the Southwest Research Institute (SwRI) in Colorado.
By delving far beneath the colorful zones and belts of Jupiter's high clouds, the Juno mission also aims to answer some fundamental questions about the planet's mysterious inner workings.
"It's as exciting as learning about the deep ocean," said Timothy Dowling, a planetary-atmosphere expert at the University of Louisville in Kentucky who's not part of the Juno team.
"It has that same feel. All that we see on Jupiter—the light and dark bands, the jets, the enormous storms—we'll explore the foundation underneath all of that."
Jupiter Water May Offer Clues to Planet Birth
Jupiter may already seem well studied, since spacecraft headed elsewhere in the solar system have taken countless pictures as they swung close to the planet to use its gravity like a slingshot. (Related: "Lightning Strikes, Changing Climate Revealed on Jupiter.")
But until now only one other probe, Galileo, has orbited the giant world and attempted to study its composition and activity.
As the largest planet in our solar system, Jupiter could help resolve theories for the process of planet formation.
Current theory states that the planets formed from a dusty disk of material that surrounded the newborn sun roughly 4.6 billion years ago. (Related: "Newborn Planet Found Orbiting Young Star.")
Scientists know that Jupiter is primarily made of hydrogen and helium, like the sun and most of the universe. But the planet is also enriched with heavier elements such as carbon and nitrogen—elements that became the building blocks for not only the rocky planets such as Earth and Mars but also for life.
One theory to explain the heavy elements in Jupiter is that water, in the form of ice, was one of the first multielement molecules to form inside the protoplanetary disk.
This ice clumped together and trapped heavy elements in the dust to make dirty snowballs called planetesimals. In Jupiter's case, an ice ball may have attracted gases as it swept through the disk, building up the planet's mass.
Juno will help test that theory using a device called a passive microwave radiometer, which will measure how much water is in Jupiter's deep atmosphere. In this region, gravity is so intense that much of the primordial solar material that formed the planets is probably still trapped.
"I think it's a very fundamental mission, in the sense that we're tying to go back and look at the first step in the solar system's history after the sun formed and investigate why the planets are the way they are," SwRI's Bolton said.
Juno Probing Jupiter's Depths
Other instruments on Juno will map the circulation, composition, temperature, and other features deeper in Jupiter's atmosphere than any previous experiments.
"Essentially we'll be unraveling basic aspects of how meteorology works in an alien environment, thereby extending our understanding of atmospheric circulation and climate beyond the confines of Earth," said Adam Showman, of the University of Arizona's Lunar and Planetary Laboratory.
"I think that's pretty exciting, especially because gas giants like Jupiter are among the most common planetary environments in the universe."
And while Jupiter is nearly all atmosphere, the planet should have some kind of solid core far beneath the swirling clouds, where atmospheric pressures are millions of times greater than at sea level on Earth.
By precisely measuring the way Juno gets pulled and pushed by the massive planet's gravity field, scientists may finally be able to detect and measure the planet's core.
"This mission is very unique," said the University of Louisville's Dowling. "We've never tried to probe into the heart of a planet like Jupiter. It's basically the first time we'll see an MRI of a gas giant."
Juno Needs "Radiation Vault" to Survive
In addition to peering far below Jupiter's surface, Juno will be gazing high above the clouds, studying the origins of the planet's intense magnetic field and how it interacts with the Jovian atmosphere.
The biggest and strongest magnetic dynamo in the solar system, Jupiter's magnetic field creates spectacular "hyperauroras," which Juno will see in unprecedented detail.
Juno will also sample the charged particles that create the auroras and will observe them in ultraviolet light. In addition, the spacecraft will capture color photos of the poles with its JunoCam—sure to be one of the mission's most popular features.
"That camera is really for the public, and the data will be immediately made available for the public—but I want to see a picture of the poles too," SwRI's Bolton said.
But the magnetic field that drives Jupiter's auroras also traps charged particles in a bubble around the planet, creating the strongest radiation zone in the solar system, something that would fricassee the spacecraft without special precautions.
"We basically have a radiation vault—a titanium box in the middle of the spacecraft—and the sensitive electronics are inside that box, like an armored tank going to Jupiter," Bolton said.
At Mission's End, Juno to Plunge Into Jupiter
In the end, Jupiter's radiation will degrade the solar cells on Juno's arrays, putting limits on the lifetime of the mission.
Unlike previous deep-space missions, which used nuclear power, Juno will operate entirely on sunlight. When it reaches Jupiter, it will be the most distant solar-powered spacecraft yet launched.
The craft's three superefficient arrays—each 9 by 30 feet (2.7 by 9.1 meters)—will allow it to work in sunlight that's about 25 times weaker than the light here on Earth.
When Juno's mission ends, NASA scientists will instruct the craft to deorbit over Jupiter so that Juno burns up in the giant planet's atmosphere. This way, the defunct spacecraft won't be left to wander the Jovian system and potentially crash on one of the planet's many moons, contaminating worlds such as Europa with watery habitats that possibly host life.
Ultimately, the Juno mission will provide scientists with a wealth of data for understanding not just our own solar system but also the scores of gas giants scattered across the galaxy.
"Jupiter is our prototype giant planet," the University of Arizona's Showman said. "So the understanding we gain from Juno about Jupiter will lend great insights to our understanding of the hundreds of giant planets being discovered around other stars."

Earth Had Two Moons, New Model Suggests


The moon, as seen by Apollo astronauts.
The near side of the moon (right) is much smoother than the far side.
Photograph courtesy NASA
Ker Than
Published August 3, 2011
Earth may have once had two moons, but one was destroyed in a slow-motion collision that left our current lunar orb lumpier on one side than the other, scientists say.
Astronomers have long been puzzled by the differences between the side of the moon that always faces Earth—the near side—and the side that always faces away, the far side. The topography of the near side is relatively low and flat, while that of the far side is high and mountainous with a much thicker crust.
According to a new computer model, this discrepancy can be explained if a smaller "companion moon" collided with our moon's far side early in its history. Such a collision would have left the far side splattered with especially hard rocky material that now forms the current lunar highlands.
For the theory to work, the smaller moon must have crashed into the larger one at about 4,400 miles (7,081 kilometers) an hour.
"This is the slowest possible collision the two massive bodies could have if they fell into each other’s gravity," explained study co-author Erik Asphaug, a planetary scientist at the University of California, Santa Cruz (UCSC).
At this relatively slow speed, the far-side collision wouldn’t have been energetic enough to melt rock or carve out a crater. But it would have been forceful enough to plaster material from the smaller moon onto the larger moon.
"It's like a car crash, where you have crumpled bumpers but you don't melt the cars as they're colliding," Asphaug said. "This is the same kind of phenomenon."
Moon Collision Created Meteor Shower
The new theory, by Asphaug and UCSC postdoctoral researcher Martin Jutzi, is detailed in the current issue of the journal Nature.
According to their model, the two moons coexisted peacefully for about 80 million years, each in its own stable orbit. The moons were the same color and composition, but one was about three times larger than the other, Asphaug said.
"Our moon looked like a big dinner plate in the sky ... and when it set, there was this other moon trailing it by about 60 degrees," he said.
This brief period of lunar harmony was shattered, according to the model, when natural gravitational interactions with Earth caused both moons to drift farther away from our planet. The sun's gravitational tug then destabilized the smaller moon’s orbit and caused it to fall into its larger sibling.
Though not very energetic, the collision would have ejected trillions of tons of lunar debris into space, obscuring both moons for several days.
"When the dust cleared, you had one moon that might have looked similar to our moon today," Asphaug said.
For up to a million years after the event, Earth would have been bombarded by moon bits of various sizes, the biggest of which could have been as much as 62 miles (100 kilometers) across.
"You'd have meteors raining down all over the sky for a long period of time," Asphaug said, though there probably would have been no life yet on Earth to witness the spectacular sky shows.
Lunar Smashup Opens Up "Cool Problems"
Astronomer Jeffrey Taylor of the University of Hawaii said the new moon theory is very interesting and worth further investigation.
Asphaug and Jutzi's model not only accounts for the moon's asymmetry, Taylor said, but the findings also explain the fates of the smaller, companion satellites that another theory predicts should have formed alongside our moon.
One of the leading theories for how our moon formed is that it was born after a Mars-size planet crashed into Earth shortly after the solar system's formation about 4.5 billion years ago. (See "Earth-Asteroid Collision Formed Moon Later Than Thought.")
Scientists think the earlier smashup created a ring of molten rock debris around Earth, which eventually coalesced into several bodies, including our current moon. (Related: "The Moon Has Shrunk, and May Still Be Contracting.")
But "if that's the case, what happened [to the smaller moons]? This is one thing that could have happened to them," said Taylor, who was not involved in the study.
The new theory isn't without its problems, however. For example, it doesn't explain why the lumpy far side of our moon shows a high concentration of aluminum, Taylor said.
If the two moons had formed from the same material, as is assumed, the companion moon—and its splatterings—should have been low in aluminum, like our own moon's interior.
However, this problem could be resolved by future lunar studies, Taylor said, and it's not a serious enough reason to dismiss the theory.
"If anything," he said, "it just opens up more cool problems to work on.

Android Honeycomb 3.1 - A Quick Breakdown


Google’s Android operating system for tablets has had mixed reactions.
Android Honeycomb 3.1 - A Quick Breakdown
Google’s Android operating system for tablets has had mixed reactions. On one hand, users seem to like Android for the mobile phone, and on the other hand, there’s Honeycomb 3.0 that lacks the finish and refinement seen in its primary competitor - iOS. Many of us agree that the OS is far from complete and there are some bugs that need to be ironed out. The iPad has been a runaway success and Google is hoping to catch up once Honeycomb matures. We just got news of Motorola launching Android 3.1 for the Xoom tablet and that’s something we’ll see across the board very soon. Here’s a quick look at what key features and enhancementsHoneycomb 3.1 has to offer.

Improved USB support
While tablets were designed to replace netbooks and notebooks, one of the key things stopping users from doing so was poor connectivity with other devices using the USB interface. Come Honeycomb 3.1, users will be able to use a wide variety of USB devices with their tablets.
USB open to a variety of devices; game controllers included
USB open to a variety of devices; game controllers included


This means, everything from keyboards, mice, other input devices and even digital cameras will be able to work with tablets. Imagine typing on a tablet using a portable, folding keyboard and transferring images from your camera or a card reader to your tablet, and viewing photos in real time. Google says that you can even use Bluetooth-based input devices with the tablet.

Resizable Widgets
Sure, this is something that third party window managers bring, but Android has never really had a built-in feature to do this. This means, anyone using Honeycomb had to be satisfied with the size of widgets. The new widget system lets you drag widgets into the screen of your choice and then adjust its width by holding it down, similar to what LauncherPro would let you do.

Improved Wi-Fi capabilities
Well technically, it’s not going to be faster or anything of that sort, but there will be bits and pieces added to the functionality. For example, users can now turn off the screen and the tablet will continue to stream content over the network for extended periods.
Wi-Fi optimized for longer battery life
Wi-Fi optimized for longer battery life


There’s also an option for users to use HTTP proxies for separate Wi-Fi networks, so you no longer have to switch networks and set a different HTTP proxy each time. Google claims that their new Preferred Network Offload (PNO) feature will help reduce battery drain during long Wi-Fi sessions.

App Updates
There are a bunch of Google apps that come bundled with any Google Android OS. Google has tweaked many of these for the 3.1 release. The browser, for example has an improved Quick Controls UI that’s bound to make navigation and multitasking between tabs easier. The browser has been upgraded to allow HTML5 video playback, so you no longer have to depend on Flash versions of Vimeo and Youtube videos.
UI tweaked and enhanced to allow easier navigation
UI tweaked and enhanced to allow easier navigation


Ability to save web pages for offline viewing is also a part of the browser now. Users should also notice some performance benefits, all thanks to hardware acceleration support through plugins for the browser. The Gallery now supports something called PTP (Picture Transfer Protocol). In simple terms, you can import photos from a camera to the Gallery easily. Other apps to receive enhancements are E-mail, Contacts and Calendar. 
ASUS Transformer - one of the tablets to get the 3.2 update
ASUS Transformer - one of the tablets to get the 3.2 update


Whether or not Google is successful in impressing users will only be known in the weeks to come, as manufacturers start rolling out these updates. Google has already started work on 3.2 andmanufacturers are announcing that the update should be available sometime in August.
 
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