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Wednesday, May 28, 2014
Zazzle Stretched Canvas Print from Portraits Naturally: Secretive Afri...
Monday, May 26, 2014
Zazzle Stretched Canvas Print from arrayforart: Land of the Free
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Monday, May 19, 2014
Zazzle Stretched Canvas Print from Portraits Naturally: Musical Dancin...
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Friday, May 16, 2014
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Tuesday, May 13, 2014
Zazzle Stretched Canvas Print from Portraits Naturally: Blue-Throated ...
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Friday, May 9, 2014
Desiderata Poem - Lagoon Nebula in Sagittarius Gallery Wrapped Canvas
A gorgeous wrapped canvas from HightonRidley showing some of the beauty from deep space that surrounds us. Click to customize...
tagged with: full desiderata, wallart, desiderata poem, noise and haste, go placidly, lagnebme, sagitarius constellation, lagoon nebula, the archer, galaxy stars, stellar nursery, messier 18, nebulae
Inspirational Guidance series A gorgeous iPad Mini case featuring the full Desiderata by Max Ehrmann: Go placidly amidst the noise and haste... with an amazing accompanying image. Located in the constellation of Sagittarius (The Archer), this giant cloud of glowing interstellar gas (Messier 8) is a stellar nursery that is also known as the Lagoon Nebula.
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image code: lagnebme
Image credit: Advanced Camera for Surveys (ACS) on the Hubble Space Telescope
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tagged with: full desiderata, wallart, desiderata poem, noise and haste, go placidly, lagnebme, sagitarius constellation, lagoon nebula, the archer, galaxy stars, stellar nursery, messier 18, nebulae
Inspirational Guidance series A gorgeous iPad Mini case featuring the full Desiderata by Max Ehrmann: Go placidly amidst the noise and haste... with an amazing accompanying image. Located in the constellation of Sagittarius (The Archer), this giant cloud of glowing interstellar gas (Messier 8) is a stellar nursery that is also known as the Lagoon Nebula.
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image code: lagnebme
Image credit: Advanced Camera for Surveys (ACS) on the Hubble Space Telescope
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Thursday, May 8, 2014
Star Cluster Pismis 24, core of NGC 6357 Canvas Print
A gorgeous wrapped canvas from HightonRidley showing some of the beauty from deep space that surrounds us. Click to customize...
tagged with: galaxies, outer space, wallart, star cluster, pismis 24, sculpting ultaviolet ionisation, super massive stars, nebula ngc 6357, sclustpsms, astronomy photography, stretch frame
Galaxies, Stars and Nebulae series The star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 that extends one degree on the sky in the direction of the Scorpius constellation. Part of the nebula is ionised by the youngest (bluest) heavy stars in Pismis 24. The intense ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder. One of the top candidates for the title of "Milky Way stellar heavyweight champion" was, until now, Pismis 24-1, a bright young star that lies in the core of the small open star cluster Pismis 24 (the bright stars in the Hubble image) about 8,000 light-years away from Earth. Pismis 24-1 was thought to have an incredibly large mass of 200 to 300 solar masses. New NASA/ESA Hubble measurements of the star, have, however, resolved Pismis 24-1 into two separate stars, and, in doing so, have "halved" its mass to around 100 solar masses.
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image code: sclustpsms
Image credit: NASA/ESA Hubble
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tagged with: galaxies, outer space, wallart, star cluster, pismis 24, sculpting ultaviolet ionisation, super massive stars, nebula ngc 6357, sclustpsms, astronomy photography, stretch frame
Galaxies, Stars and Nebulae series The star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 that extends one degree on the sky in the direction of the Scorpius constellation. Part of the nebula is ionised by the youngest (bluest) heavy stars in Pismis 24. The intense ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder. One of the top candidates for the title of "Milky Way stellar heavyweight champion" was, until now, Pismis 24-1, a bright young star that lies in the core of the small open star cluster Pismis 24 (the bright stars in the Hubble image) about 8,000 light-years away from Earth. Pismis 24-1 was thought to have an incredibly large mass of 200 to 300 solar masses. New NASA/ESA Hubble measurements of the star, have, however, resolved Pismis 24-1 into two separate stars, and, in doing so, have "halved" its mass to around 100 solar masses.
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image code: sclustpsms
Image credit: NASA/ESA Hubble
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Wednesday, May 7, 2014
Emission Nebula NGC 2467 in Constellation Puppis Canvas Prints
A gorgeous wrapped canvas from HightonRidley showing some of the beauty from deep space that surrounds us. Click to customize...
tagged with: wallart, galaxies and stars, sculptured gas clouds, enebicp, constellation puppis, ngc 2467, the stern, hot young stars, star incubator, outer space pictures, stretch frame
Galaxies, Stars and Nebulae series A colourful star-forming region is featured in this stunning image of NGC 2467 located in the southern constellation of Puppis (The Stern). Looking like a roiling cauldron of some exotic cosmic brew, huge clouds of gas and dust are sprinkled with bright blue, hot young stars. Strangely shaped dust clouds, resembling spilled liquids, are silhouetted against a colourful background of glowing gas. Like the familiar Orion Nebula, NGC 2467 is a huge cloud of gas, mostly hydrogen, that serves as an incubator for new stars. Some of these youthful stars have emerged from the dense clouds where they were born and now shine brightly, hot and blue in this picture, but many others remain hidden.
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image code: enebicp
Image credit: NASA/ESA Hubble Space Telescope.
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tagged with: wallart, galaxies and stars, sculptured gas clouds, enebicp, constellation puppis, ngc 2467, the stern, hot young stars, star incubator, outer space pictures, stretch frame
Galaxies, Stars and Nebulae series A colourful star-forming region is featured in this stunning image of NGC 2467 located in the southern constellation of Puppis (The Stern). Looking like a roiling cauldron of some exotic cosmic brew, huge clouds of gas and dust are sprinkled with bright blue, hot young stars. Strangely shaped dust clouds, resembling spilled liquids, are silhouetted against a colourful background of glowing gas. Like the familiar Orion Nebula, NGC 2467 is a huge cloud of gas, mostly hydrogen, that serves as an incubator for new stars. Some of these youthful stars have emerged from the dense clouds where they were born and now shine brightly, hot and blue in this picture, but many others remain hidden.
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image code: enebicp
Image credit: NASA/ESA Hubble Space Telescope.
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Tuesday, May 6, 2014
M106 Spiral Galaxy, Canes Venatici, outer space Canvas Prints
A gorgeous wrapped canvas from HightonRidley showing some of the beauty from deep space that surrounds us. Click to customize...
tagged with: wallart, star galaxies, outer space picture, deep space astronomy, hubble galaxy photography, supermassive black hole, spiral arms, constellation canes venatici, hunting dog stars, m106cv, messier 106, seyfert ii galaxy
Galaxies, Stars and Nebulae series Messier 106 (also known as NGC 4258) is a spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781. M106 is at a distance of about 22 to 25 million light-years away from Earth. It is also a Seyfert II galaxy, which means that due to x-rays and unusual emission lines detected, it is suspected that part of the galaxy is falling into a supermassive black hole in the center.
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image code: m106cv
Image credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and R. Gendler (for the Hubble Heritage Team), J. GaBany
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tagged with: wallart, star galaxies, outer space picture, deep space astronomy, hubble galaxy photography, supermassive black hole, spiral arms, constellation canes venatici, hunting dog stars, m106cv, messier 106, seyfert ii galaxy
Galaxies, Stars and Nebulae series Messier 106 (also known as NGC 4258) is a spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781. M106 is at a distance of about 22 to 25 million light-years away from Earth. It is also a Seyfert II galaxy, which means that due to x-rays and unusual emission lines detected, it is suspected that part of the galaxy is falling into a supermassive black hole in the center.
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image code: m106cv
Image credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and R. Gendler (for the Hubble Heritage Team), J. GaBany
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Zazzle Stretched Canvas Print from Portraits Naturally: Heliconia Stri...
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