Wednesday, 3 June 2015

Two chaotically tumbling Pluto moons

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If you lived on one of Pluto's moons Nix or Hydra, you'd have a hard time setting your alarm clock. That's because you could not know for sure when, or even in which direction, the sun would rise. Comprehensive analysis of data from NASA's Hubble Space Telescope shows that two of Pluto's moons, Nix and Hydra, wobble unpredictably.
via Science Daily
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Hubble Finds Two Chaotically Tumbling Pluto Moons


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Two of the most reliable changes in the sky are the daily rising of the sun in the east and setting of the sun in the west. But if you lived on a couple of Pluto's moons you wouldn't know when the day would begin, or even what direction the sun would rise. That's because, unlike Earth's moon, at least two of Pluto's small moons, Hydra and Nix, are tumbling chaotically through space. Why? Because they orbit inside a dynamically shifting gravitational field caused by the system's two central bodies, Pluto and Charon, that are whirling around each other. The moons are also football shaped, and this contributes to the chaotic rotation.


via HubbleSite NewsCenter -- Latest News Releases
http://hubblesite.org/newscenter/archive/releases/2015/24/

Astronomers Describe Chaotic Dance of Pluto’s Moons

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On Nix, one of Pluto’s five moons, the sun could rise in the east and set in the north. The moons form a sort of miniature planetary system.








via New York Times

Pentagon Seeks Easing of Ban on Russian Rockets for U.S. Space Missions

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Additional Russian engines will be needed for at least a few more years, the Pentagon says, to assure access to space for the most delicate defense and intelligence technology.








via New York Times

I Need More Space Astronaut Poster

Here's a great poster featuring a beautiful image from deep space


tagged with: astronomy, science, cosmology, cosmos, funny, humor, nasa, spaceman, scientist, astronaut, galaxy, breaking up, breakup, boyfriend, girlfriend, relationship, exploration, dating

This astronaut wants to have a serious talk. Basically, he needs more space. He's feeling smothered. But it's not you, it's him.

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Brainstorm with DARPA on a “100x Zoom Lens” for Seeing Distant Space Objects More Clearly

Science Focus

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Imaging of Earth from satellites in space has vastly improved in recent years. But the opposite challenge—using Earth-based

The post Brainstorm with DARPA on a “100x Zoom Lens” for Seeing Distant Space Objects More Clearly has been published on Technology Org.

 
#physics 
 » see original post http://feedproxy.google.com/~r/TechnologyOrgPhysicsNews/~3/lF5hG8dcNS4/
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Keyhole Nebula and Digitus Impudicus Square Sticker

Here's a great sheet of stickers featuring a beautiful image from deep space


tagged with: kndigimp, envelope sealers, galaxies and stars, keyhole nebula, carina nebula, massive stars, hubble space telescope, digitus impudicus, complex structure

Galaxies, Stars and Nebulae series Details of a mysterious, complex structure within the Carina Nebula (NGC 3372) are revealed by this image of the 'Keyhole Nebula, ' obtained with the Hubble Space Telescope. The picture is a montage assembled from four different April 1999 telescope pointings with Hubble's Wide Field Planetary Camera 2, which used six different colour filters. The picture is dominated by a large, approximately circular feature, which is part of the Keyhole Nebula, named in the 19th century by Sir John Herschel. This region, about 8000 light-years from Earth, is located adjacent to the famous explosive variable star Eta Carinae, which lies just outside the field of view toward the upper right. The Carina Nebula also contains several other stars that are among the hottest and most massive known, each about 10 times as hot, and 100 times as massive, as our Sun.

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Image credit: Hubble's Wide Field Planetary Camera 2

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Flyby Image of Saturn's Sponge Moon Hyperion

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Zazzle Space Gifts for young and old

Orion Nebula iPad Air Case

Here's a great iPad case from Zazzle featuring a Hubble-related design. Maybe you'd like to see your name on it? Click to personalize and see what it's like!


tagged with: orion, nebula, space, image, nasa, hubble, astronomy

A lovely detail of an image of the Orion Nebula in infrared thanks to NASA/Hubble.

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LHC experiments back in business at record energy

In the CERN Control Centre, the LHC operations team as well as members of CERN management applaud the announcement of stable beams this morning at 10.40am (Image: Maximilien Brice/CERN) more images

The Large Hadron Collider (LHC) started delivering physics data today for the first time in 27 months. After an almost two year shutdown and several months re-commissioning, the LHC is now providing collisions to all of its experiments at the unprecedented energy of 13 TeV, almost double the collision energy of its first run. This marks the start of season 2 at the LHC, opening the way to new discoveries. The LHC will now run round the clock for the next three years.

“With the LHC back in the collision-production mode, we celebrate the end of two months of beam commissioning,” said CERN Director of Accelerators and Technology Frédérick Bordry. “It is a great accomplishment and a rewarding moment for all of the teams involved in the work performed during the long shutdown of the LHC, in the powering tests and in the beam commissioning process. All these people have dedicated so much of their time to making this happen.”

Today at 10.40am, the LHC operators declared “stable beams”, the signal for the LHC experiments that they can start taking data. Beams are made of “trains” of proton bunches moving at almost the speed of light around the 27 kilometre ring of the LHC. These so-called bunch trains circulate in opposite directions, guided by powerful superconducting magnets. Today the LHC was filled with 6 bunches each containing around 100 billion protons. This rate will be progressively increased as the run goes on to 2808 bunches per beam, allowing the LHC to produce up to 1 billion collisions per second.

For more information see the live blog that covered events as they unfolded.


via CERN: Updates for the general public
http://home.web.cern.ch/about/updates/2015/06/lhc-experiments-back-business-record-energy

Suspended monolayer graphene on cavities

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Nanoelectromechanical systems (NEMS), small brothers of microelectromechanical systems (MEMS), are entering mainstream technology through sensors and actuators in platforms as common as inkjet printers, accelerometers, displays, and optical switches. Worth several tens of billions USD, the MEMS and NEMS market is one that cannot be ignored.

NEMS relies on small vibrating membranes, which are sensitive to tiny forces. The membranes need to be lightweight and stiff, with a high Young's modulus - all parameters which graphene is known for. For example, the Young's modulus of graphene is about five times larger than that of silicon, the flagship material for MEMS. As such, graphene is among the most promising candidates for applications that require ultrathin membranes with excellent mechanical properties.

Image 1: Monolayer graphene membrane suspended over a microscopic cavity.

Already in 2013, the sensitivity of graphene NEMS was shown to overshadow silicon MEMS by up to an order of magnitude. The success of graphene NEMS ignited follow-up research across the world, with industrial interest closely following. In order to serve the growing field, Graphenea enhanced their product catalog with the addition of suspended monolayer graphene on cavities. Because all NEMS are different, the idea is that the customer makes their own cavities (tiny holes) in a substrate, and Graphenea uses a novel transfer method to cover the holes with high quality CVD graphene. This is an arrangement that has proven to be successful, as exemplified by publications that Graphenea shares with world-leading graphene NEMS research groups.

Image 2: Monolayer graphene membrane suspended over microcavities.

Graphenea is engaged in research of graphene NEMS within the EU FET Graphene Flagship initiative and also through the project GRAFOL. Suspended graphene membranes have other uses than NEMS, for example in optomechanical systems. Details of the substrate requirements and graphene film quality for this product are available in the Graphenea catalog.


via Graphenea

Live blog: LHC experiments to start taking data at 13 TeV

Today's the day! The Large Hadron Collider (LHC) is set to start delivering physics data to its experiments for the first time in 27 months.

After nearly two years of maintenance and repair, as well as several months of re-commissioning, the experiments at the world's largest particle accelerator are now ready to take data at the unprecedented energy of 13 teraelectronvolts (TeV) – almost double the collision energy of the LHC's first, three-year run. Data taking will mark the start of season 2 at the LHC, opening the way to new frontiers in physics.

For all the day's action, follow our Live Blog "LHC Season 2: New frontiers in physics" where we'll be posting all the latest from the CERN Control Centre.


via CERN: Updates for the general public
http://home.web.cern.ch/about/updates/2015/06/live-blog-lhc-experiments-start-taking-data-13-tev

Keyhole Nebula and Digitus Impudicus Rectangular Sticker

Here's a great sheet of stickers featuring a beautiful image from deep space


tagged with: kndigimp, peel off, galaxies and stars, keyhole nebula, carina nebula, massive stars, hubble space telescope, digitus impudicus, complex structure

Galaxies, Stars and Nebulae series Details of a mysterious, complex structure within the Carina Nebula (NGC 3372) are revealed by this image of the 'Keyhole Nebula, ' obtained with the Hubble Space Telescope. The picture is a montage assembled from four different April 1999 telescope pointings with Hubble's Wide Field Planetary Camera 2, which used six different colour filters. The picture is dominated by a large, approximately circular feature, which is part of the Keyhole Nebula, named in the 19th century by Sir John Herschel. This region, about 8000 light-years from Earth, is located adjacent to the famous explosive variable star Eta Carinae, which lies just outside the field of view toward the upper right. The Carina Nebula also contains several other stars that are among the hottest and most massive known, each about 10 times as hot, and 100 times as massive, as our Sun.

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image code: kndigimp

Image credit: Hubble's Wide Field Planetary Camera 2

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Click to customize.
via Zazzle Astronomy market place

Name, Barred Spiral Galaxy NGC 1672 Wrapping Paper

Get your out-of-this-world gift wrap here! Perfect for Christmas gifts for anyone who is fascinated by what the universe holds in store for us!


tagged with: star galaxies, deep space astronomy, barred spiral galaxy, bsgsst, starry space picture, galactic arms, supermassive black hole, dust lanes, star forming galaxy, outer space telescope images

Galaxies, Stars and Nebulae series: This NASA Hubble Space Telescope view of the nearby barred spiral galaxy NGC 1672 unveils details in the galaxy's star-forming clouds and dark bands of interstellar dust.
One of the most striking features is the dust lanes that extend away from the nucleus and follow the inner edges of the galaxy's spiral arms. Clusters of hot young blue stars form along the spiral arms and ionize surrounding clouds of hydrogen gas that glow red. Delicate curtains of dust partially obscure and redden the light of the stars behind them by scattering blue light.
Galaxies lying behind NGC 1672 give the illusion they are embedded in the foreground galaxy, even though they are really much farther away. They also appear reddened as they shine through NGC 1672's dust. A few bright foreground stars inside our own Milky Way Galaxy appear in the image as bright and diamond-like objects.
As a prototypical barred spiral galaxy, NGC 1672 differs from normal spiral galaxies, in that the arms do not twist all the way into the center. Instead, they are attached to the two ends of a straight bar of stars enclosing the nucleus. Viewed nearly face on, NGC 1672 shows intense star formation regions especially off in the ends of its central bar.
Astronomers believe that barred spirals have a unique mechanism that channels gas from the disk inward towards the nucleus. This allows the bar portion of the galaxy to serve as an area of new star generation.
NGC 1672 is also classified as a Seyfert galaxy. Seyferts are a subset of galaxies with active nuclei. The energy output of these nuclei can sometimes outshine their host galaxies. This activity is powered by accretion onto supermassive black holes.
NGC 1672 is more than 60 million light-years away in the direction of the southern constellation Dorado. These observations of NGC 1672 were taken with Hubble's Advanced Camera for Surveys in August of 2005. The composite image was made by using filters that isolate light from the blue, green, and infrared portions of the spectrum, as well as emission from ionized hydrogen.
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image code: bsgsst

image credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration

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Crab Nebula iPad Air Case

Here's a great iPad case from Zazzle featuring a Hubble-related design. Maybe you'd like to see your name on it? Click to personalize and see what it's like!


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This is a mosaic image, one of the largest ever taken by NASA's Hubble Space Telescope of the Crab Nebula, a six-light-year-wide expanding remnant of a star's supernova explosion. Japanese and Chinese astronomers recorded this violent event nearly 1,000 years ago in 1054, as did, almost certainly, Native Americans.

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