Thursday, 11 June 2015

Observatory: Saturn’s Ring of Dust and ‘Soccer Balls’

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The planet’s enormous outer ring is made up of an unusual combination of fine dust and rocks the size of soccer balls, scientists have discovered.








via New York Times

Licensing agreement reached on brilliant new blue pigment discovered by happy accident

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A brilliant new blue pigment – discovered serendipitously by Oregon State University chemists in 2009 – is now

The post Licensing agreement reached on brilliant new blue pigment discovered by happy accident has been published on Technology Org.

 
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Closest ever look at dwarf planet Ceres

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NASA's Dawn mission is observing the dwarf planet Ceres from 2,700 miles above its surface, and this week released a new image of Ceres.
via Science Daily
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'Sunscreen' layer detected on distant planet

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NASA's Hubble Space Telescope has detected a stratosphere, one of the primary layers of Earth's atmosphere, on a massive and blazing-hot exoplanet known as WASP-33b.
via Science Daily
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Hubble Telescope Detects 'Sunscreen' Layer on Distant Planet


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Researchers using NASA's Hubble Space Telescope have detected a stratosphere and temperature inversion in the atmosphere of a planet several times the mass of Jupiter, called WASP-33b. Earth's stratosphere sits above the troposphere, the turbulent, active-weather region that reaches from the ground to the altitude where nearly all clouds top out. In the troposphere, the temperature is warmer at the bottom ground level and cools down at higher altitudes. The stratosphere is just the opposite: There, the temperature rises at higher altitudes. This is called a temperature inversion, and it happens because ozone in the stratosphere absorbs some of the sun's radiation, preventing it from reaching the surface and warming this layer of the atmosphere. Similar temperature inversions occur in the stratospheres of other planets in our solar system, such as Jupiter and Saturn. But WASP-33b is so close to its star that its atmosphere is a scathing 10,000 degrees Fahrenheit, and its atmosphere is so hot the planet might actually have titanium oxide rain.


via HubbleSite NewsCenter -- Latest News Releases
http://hubblesite.org/newscenter/archive/releases/2015/25/

Stonehenge at Night Posters

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


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ImageID: AX028971 / M. Dillon / CORBIS / Stonehenge at Night /

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Graphene promise for body armour

Science Focus

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The "wonder material" graphene could be used to make bulletproof armour, new research suggests. 
#science 
 » see original post http://www.bbc.co.uk/news/science-environment-30246089#sa-ns_mchannel=rss&ns_source=PublicRSS20-sa
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First technical stop for the LHC

LHC operators in the CERN Control Centre during the first day of the Run 2 for physics on 3 June 2015.

In a few days’ time, the Large Hadron Collider (LHC) and its experiments will be taking a short break. This five-day breather is the first of three technical stops scheduled for the accelerator during the 2015 operating period, before a slightly longer stop during the end-of-year holidays.

Although physics data only started to be collected at the LHC on 3 June, progressive recommissioning of the machine with beam actually began on 5 April. And even at the end of 2014, the machine had already been cooled and all of its equipment had begun operating.

Restarting the LHC involves much more than just pressing a button. The accelerator is made up of thousands of components that all have to work together harmoniously and need to be retuned at regular intervals. Each year of LHC operation therefore includes five-day technical stops every ten weeks or so. The experiments take advantage of these intervals to carry out their own maintenance work.

The first technical stop in 2015 will also allow LHCf to dismantle its detectors. LHCf is one of the LHC’s three smallest experiments and operates with beams that are not very concentrated, to avoid damage to its detectors. The operators of the LHC have therefore planned a special run this week, with beams that are less dense at the collision points. The other experiments will also use this opportunity to take data, in particular to calibrate their detectors.

After this first technical stop, several days will be dedicated to the scrubbing of the beam pipes ready to increase the machine's luminosity, i.e. to increase the number of bunches of protons. The LHC will then restart for physics with more bunches overall and a greater concentration of bunches at the collision points. Physics data collection will continue until the next technical stop, scheduled for the end of August.


via CERN: Updates for the general public
http://home.web.cern.ch/about/updates/2015/06/first-technical-stop-lhc

Monogram - Enlarged Region of The Omega Nebula Classic Round Sticker

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


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Galaxies, Stars and Nebulae series Like the fury of a raging sea, this bubbly ocean of glowing hydrogen, oxygen, and sulphur gas lies in the extremely massive and luminous molecular nebula Messier 17.
This Hubble photograph captures a small region within Messier 17 (M17), a hotbed of star formation. M17, also known as the Omega or Swan Nebula, is located about 5500 light-years away in the Sagittarius constellation.
Ultraviolet radiation is carving and heating the surfaces of cold hydrogen gas clouds and the warmed surfaces glow orange and red. The intense heat and pressure causes some material to stream away from the surface, creating the glowing veil of even hotter green-coloured gas that masks background structures. The colours in the image represent various gases. Red represents sulphur; green, hydrogen; and blue, oxygen.

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image code: eroton

Image credit: NASA, the ACS Science Team

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The Light, the Dark, and the Dusty

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This colorful skyscape spans about three full moons (1.5 degrees) across nebula rich starfields along the plane of our Milky Way Galaxy in the royal northern constellation Cepheus. Near the edge of the region's massive molecular cloud some 2,400 light-years away, bright reddish emission region Sharpless (Sh) 155 lies at the upper left, also known as the Cave Nebula. About 10 light-years across the cosmic cave's bright rims of gas are ionized by ultraviolet light from hot young stars. Dusty blue reflection nebulae also abound on the interstellar canvas cut by dense obscuring clouds of dust. The long core of the Lynds Dark Nebula (LDN) 1210 anchors the scene at lower right. Astronomical explorations have revealed other dramatic signs of star formation, including the bright red fleck of Herbig-Haro (HH) 168. Directly below the bright Cave Nebula, the Herbig-Haro object emission is generated by energetic jets from a newborn star.

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The Orion Nebula iPad Air Cases

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

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Seeing the Action Inside of a Cell

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Cells are biological wonders. Throughout billions of years of existence on Earth, these tiny units of life have

The post Seeing the Action Inside of a Cell has been published on Technology Org.

 
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Planets of the Solar System Posters

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


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ImageID: CB061976 / Corbis / Planets of the Solar System/ /

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Crab Pulsar Time Lapse - Neutron Star Square Sticker

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Galaxies, Stars and Nebulae series

Multiple observations made over several months with NASA's Chandra X-ray Observatory and the Hubble Space Telescope captured the spectacle of matter and antimatter propelled to near the speed of light by the Crab pulsar, a rapidly rotating neutron star the size of Manhattan.

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Image code: crbplsr

Image credit: NASA's Chandra X-ray Observatory and the Hubble Space Telescope

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Nebula in Turquoise iPad Air Powis Case iPad Air Covers

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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Nebula in Turquoise iPad Air Powis Case Personalize

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