Monday 5 January 2015

Dwarf Galaxy Holmberg IX iPad Mini 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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"This loose collection of stars is actually a dwarf irregular galaxy, called Holmberg IX. It resides just off the outer edge of M81, a large spiral galaxy in Ursa Major. This image was taken with Hubble's Advanced Camera for Surveys in early 2006. Holmberg IX is of the so-called Magellanic type of galaxy, as its size and irregularity in structure are similar to the Small Magellanic Cloud, a neighbor to our own Milky Way. Holmberg IX was first discovered by astronomer Sidney van den Bergh in 1959, and cataloged as DDO 66. The galaxy received its "Holmberg IX" naming when it was discussed in Eric Holmberg's study of groups of galaxies ten years later. It is suspected that the dwarf galaxy was created as a result of a galactic interaction between M81 and neighboring galaxy M82."

(qtd. from Hubblesite.org NewsCenter release STScI-2008-02)

Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

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Hubble Discovers that Milky Way Core Drives Wind at 2 Million Miles Per Hour



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At a time when our earliest human ancestors had recently mastered walking upright, the heart of our Milky Way galaxy underwent a titanic eruption, driving gases and other material outward at 2 million miles per hour. Now, at least 2 million years later, astronomers are witnessing the aftermath of the explosion: billowing clouds of gas towering about 30,000 light-years above and below the plane of our galaxy.




via HubbleSite NewsCenter -- Latest News Releases

http://hubblesite.org/newscenter/archive/releases/2015/03/

Hubble's High-Definition Panoramic View of the Andromeda Galaxy



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The largest NASA Hubble Space Telescope image ever assembled, this sweeping view of a portion of the Andromeda galaxy (M31) is the sharpest large composite image ever taken of our galactic neighbor. Though the galaxy is over 2 million light-years away, the Hubble telescope is powerful enough to resolve individual stars in a 61,000-light-year-long section of the galaxy's pancake-shaped disk. It's like photographing a beach and resolving individual grains of sand. And, there are lots of stars in this sweeping view over 100 million, with some of them in thousands of star clusters seen embedded in the disk. This ambitious photographic cartography of the Andromeda galaxy represents a new benchmark for precision studies of large spiral galaxies which dominate the universe's population of over 100 billion galaxies. Never before have astronomers been able to see individual stars over a major portion of an external spiral galaxy. Most of the stars in the universe live inside such majestic star cities, and this is the first data that reveal populations of stars in context to their home galaxy.




via HubbleSite NewsCenter -- Latest News Releases

http://hubblesite.org/newscenter/archive/releases/2015/02/

Hubble Goes High Def to Revisit the Iconic 'Pillars of Creation'



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Although NASA's Hubble Space Telescope has taken many breathtaking images of the universe, one snapshot stands out from the rest: the iconic view of the so-called "Pillars of Creation." The jaw-dropping photo, taken in 1995, revealed never-before-seen details of three giant columns of cold gas bathed in the scorching ultraviolet light from a cluster of young, massive stars in a small region of the Eagle Nebula, or M16.




via HubbleSite NewsCenter -- Latest News Releases

http://hubblesite.org/newscenter/archive/releases/2015/01/

Electromagnetic waves linked to particle fallout in Earth's atmosphere, new study finds

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In a new study that sheds light on space weather's impact on Earth, researchers show for the first time that plasma waves buffeting the planet's radiation belts are responsible for scattering charged particles into the atmosphere.

via Science Daily

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Atomic ‘mismatch’ creates nano ‘dumbbells’

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Like snowflakes, nanoparticles come in a wide variety of shapes and sizes. The geometry of a nanoparticle is

The post Atomic ‘mismatch’ creates nano ‘dumbbells’ has been published on Technology Org.

 
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New instrument reveals recipe for other Earths

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How do you make an Earth-like planet? The "test kitchen" of Earth has given us a detailed recipe, but it wasn't clear whether other planetary systems would follow the same formula. Now, astronomers have found evidence that the recipe for Earth also applies to terrestrial exoplanets orbiting distant stars.



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Stars' spins reveal their ages

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When you're a kid every birthday is cause for celebration, but as you get older they become a little less exciting. You might not want to admit just how old you are. And you might notice yourself slowing down over the years. You're not alone - the same is true of stars. They slow down as they age, and their ages are well-kept secrets. Astronomers are taking advantage of the first fact to tackle the second and tease out stellar ages.



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New analyses of Martian chemical maps suggest water bound to sulfates in soil

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A spatial association between the presence of sulfur and hydrogen found in Martian soil has been proposed by scientists. The team suggests that further observations by the Curiosity rover in Gale Crater could move forward models of aqueous processes on Mars. For example, recent analyses of "Rocknest" soil samples suggest complementary modes of soil hydration in the Gale Crater area.

via Science Daily

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Pinwheel Galaxy Spiral Space Print

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


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This is a NASA space photograph, showing the spiral Pinwheel Galaxy, also known as M101. This galaxy is located about 21 million light years from Earth, in Ursa Major (the Big Dipper). This composite image has pink, white, blue and yellow colours, and combines visible light, infrared light, ultraviolet light and x-ray data. Four of NASA's telescopes were involved: the Hubble Space Telescope, Spitzer Space telescope, Chandra X-Ray Observatory and the Galaxy Evolution Explorer (GALEX).

Image Credits: X-ray: NASA/CXC/SAO; IR & UV: NASA/JPL-Caltech; Optical: NASA/STScI

There are many more products with this space photo in The Astronomy Gift Shop store.

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The dark side of creativity

Science Focus

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Creativity — the generation of novel and useful ideas, products, or solutions — is seen as a valuable trait for people and organizations to possess.

Organizations harness it to develop innovative products, services, or processes, all of which promote profitability, long-term sustainability, and a competitive advantage. For the individual, research has shown that creativity is often associated with humor and altruism, more positive moods, and personal resiliency. Sharon Kim, a professor at Johns Hopkins University, Jack Goncalo, a professor at Cornell University, and I found that...

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 » see original post http://theweek.com/article/index/273682/the-dark-side-of-creativity
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AUDIO: HIV virus 'becoming less dangerous'

Science Focus

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A new study suggests HIV is becoming less infectious and deadly as it evolves, but virologist Prof David Dausey says caution has to be observed. 
#science 
 » see original post http://www.bbc.co.uk/news/health-30288524#sa-ns_mchannel=rss&ns_source=PublicRSS20-sa
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Why combining Mentos and Coke creates a sugary volcano, and other cool candy tricks

Science Focus

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How to make sparks fly in your mouth

We're issuing a science-based exception to the "don't chew with your mouth open" rule for this one. If you crunch Wint-O-Green Life Savers with your mouth open in the dark in front of a mirror, you should see some sparks start to fly. The light you see is due to a phenomenon called "triboluminescence."

When you chomp down on a mint, your teeth are fracturing crystals of sugar. This fracturing happens all the way down at the molecular level, where chemical bonds are broken. Because of the structure of the sugar crystal, the breaking of these chemical bonds...

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 » see original post http://theweek.com/article/index/270821/why-combining-mentos-and-coke-creates-a-sugary-volcano-and-other-cool-candy-tricks
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Butterfly Nebula in Scorpius Constellation Rectangular Sticker

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


tagged with: peel off, galaxies and stars, stellar winds, btbgneb, butterfly nebula, bug nebula, scorpius constellation, ngc 6302, sculptured gas clouds

Galaxies, Stars and Nebulae series NGC 6302, more popularly called the Bug Nebula or the Butterfly Nebula, lies within our Milky Way galaxy, roughly 3,800 light-years away in the constellation of Scorpius.
The central dying star cannot be seen because it's hidden within a doughnut-shaped ring of dust, which appears as a dark band pinching the nebula in the centre. The thick dust belt constricts the star's outflow, creating the classic "bipolar" or hourglass shape displayed by some planetary nebulae.
The nebula's reddish outer edges are largely due to light emitted by nitrogen, which marks the coolest gas visible in the picture. The white-coloured regions are areas where light is emitted by sulphur. These are regions where fast-moving gas overtakes and collides with slow-moving gas that left the star at an earlier time, producing shock waves in the gas (the bright white edges on the sides facing the central star).

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image code: btbgneb

image credit: NGC 6302 was imaged on 27 July 2009 with Hubble's Wide Field Camera 3 in ultraviolet and visible light. Filters that isolate emissions from oxygen, helium, hydrogen, nitrogen and sulphur were used to create this composite image.

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A Fox Fur, a Unicorn, and a Christmas Tree

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Zazzle Space Gifts for young and old

Helix Nebula, Beautiful Stars in the Galaxy Wall Decal

Here's a great wall decal featuring a beautiful image from deep space


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This infrared image from NASA's Spitzer Space Telescope shows the Helix Nebula, a cosmic starlet often photographed by amateur astronomers for its vivid colors and eerie resemblance to a giant eye. The nebula, located about 700 light-years away in the constellation Aquarius, belongs to a class of objects called planetary nebulae. Discovered in the 18th century, these colorful beauties were named for their resemblance to gas-giant planets like Jupiter. Planetary nebulae are the remains of stars that once looked a lot like our sun. When sun-like stars die, they puff out their outer gaseous layers. These layers are heated by the hot core of the dead star, called a white dwarf, and shine with infrared and visible colors. Our own sun will blossom into a planetary nebula when it dies in about five billion years. In Spitzer's infrared view of the Helix nebula, the eye looks more like that of a green monster's. Infrared light from the outer gaseous layers is represented in blues and greens. The white dwarf is visible as a tiny white dot in the center of the picture. The red color in the middle of the eye denotes the final layers of gas blown out when the star died. The brighter red circle in the very center is the glow of a dusty disk circling the white dwarf (the disk itself is too small to be resolved). This dust, discovered by Spitzer's infrared heat-seeking vision, was most likely kicked up by comets that survived the death of their star. Before the star died, its comets and possibly planets would have orbited the star in an orderly fashion. But when the star blew off its outer layers, the icy bodies and outer planets would have been tossed about and into each other, resulting in an ongoing cosmic dust storm. Any inner planets in the system would have burned up or been swallowed as their dying star expanded. So far, the Helix nebula is one of only a few dead-star systems in which evidence for comet survivors has been found. You can personalize the design further if you'd prefer, such as by adding your name or other text, or adjusting the image - just click 'Customize' to see all the options.

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Stunning Aqua Star Cluster iPad Mini Cover

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: cosmological, cosmos, space, hubble, telescope, magellanic, turquoise, aqua, blue, stars, outer space

A breathtaking blue and turquoise dance of heavenly clouds, Star Cluster NGC 2074 in the Large Magellanic Cloud as captured by the Hubble Space Telescope.

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Chasms and cliffs on Mars

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Space Science Image of the Week: Mars Express spots familiar geology near the volcanic Tharsis region on Mars

via ESA Space Science

http://www.esa.int/spaceinimages/Images/2015/01/Chasms_and_cliffs_on_Mars

Studies look at long-term aging of electronics in nuclear weapons

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Sandia National Laboratories is studying how environments, including radiation that originates from a nuclear weapon itself, could affect

The post Studies look at long-term aging of electronics in nuclear weapons has been published on Technology Org.

 
#materials 
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TEST PRINT

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


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teacher,professor,astronomy,sociology,psychology,economics,physics,biology,history,english,archaeology,geology,ornithology,paleontology,anthropology,accounting,marketing,computer,science,french,literature,management,exam,test,instructor,law,medicine,school,med,drama,engineerin,political,art

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Monogram Celestial Bauble - SXP1062 space picture Round Sticker

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


tagged with: monogram initials, sculptured gas clouds, hot young stars, star incubator, star galaxies, outer space picture, sxp1062, supernova remnant, small magellanic cloud, deep space astronomy, star factory, smc

Galaxies, Stars and Nebulae series In this composite image, X-rays from Chandra and XMM-Newton have been colored blue and optical data from the Cerro Tololo Inter-American Observatory in Chile are colored red and green. The flowering shape on the left is a star factory and on the right is the pulsar. Known as SXP 1062, it's the bright white source located on the right-hand side of the image in the middle of the diffuse blue emission inside a red shell. The diffuse X-rays and optical shell are both evidence for a supernova remnant surrounding the pulsar. The optical data also displays spectacular formations of gas and dust in a star-forming region on the left side of the image. A comparison of the Chandra image with optical images shows that the pulsar has a hot, massive companion.
Astronomers are interested in SXP 1062 because the Chandra and XMM-Newton data show that it is rotating unusually slowly - about once every 18 minutes. (In contrast, some pulsars are found to revolve multiple times per second, including most newly born pulsars.) This relatively leisurely pace of SXP 1062 makes it one of the slowest rotating X-ray pulsars in the SMC.
Two different teams of scientists have estimated that the supernova remnant around SXP 1062 is between 10,000 and 40,000 years old, as it appears in the image. This means that the pulsar is very young, from an astronomical perspective, since it was presumably formed in the same explosion that produced the supernova remnant.
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image code: sxp1062

Image credit: X-ray: NASA/CXC/Univ.Potsdam/L.Oskinova et al & ESA/XMM-Newton; Optical: AURA/NOAO/CTIO/Univ.Potsdam/L.Oskinova et al

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SpaceX’s Next Frontier: Landing a Rocket on Earth

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On Tuesday, the company hopes to upend the economics of space travel, by landing the first stage of a rocket intact on a barge floating in the Atlantic Ocean.















via New York Times

Nebula in shape of Horsehead in Pink Wall Skins

Here's a great wall decal featuring a beautiful image from deep space


tagged with: astronomy, galaxy, twinkle, planets, stars, science, geek, hubble telescope, outer space, emission nebula, celestial bodies, space, physics, cosmos, big bang theory, hubble, telescope, exploration, orion nebula, spitzer telescope, messier object, milky way, natural science, natural sciences, natural world, nebula, nobody, physical science, sciences, space exploration and research, taurus, zodiac, universe, constellation, night sky, hubb

The Horsehead Nebula (also known as Barnard 33 in emission nebula IC 434) is a dark nebula in the constellation Orion.[1] The nebula is located just to the south of the star Alnitak, which is farthest east on Orion's Belt, and is part of the much larger Orion Molecular Cloud Complex. The nebula was first recorded in 1888 by Scottish astronomer Williamina Fleming on photographic plate B2312 taken at the Harvard College Observatory. The Horsehead Nebula is approximately 1500 light years from Earth. It is one of the most identifiable nebulae because of the shape of its swirling cloud of dark dust and gases, which bears some resemblance to a horse's head when viewed from Earth. You can personalize the design further if you'd prefer, such as by adding your name or other text, or adjusting the image - just click 'Customize' to see all the options.

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