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Out of the Void Poster by Bebops
I hope to display a variety of animal images on this blog to delight us all. I have created many products featuring wildlife and pets for my Zazzle stores, Bebop's Place and Bebop's Weddings, using my original photographs and designs. I am also constantly amazed at the gorgeous animal products available from the rest of the Zazzle community. I am hoping others will enjoy this blog and even be moved to purchase some of these lovely items for gifts or just for the pleasure of having such beauty around.
Friday, September 5, 2014
Zazzle Poster from Bebops: Grazing Horses 2015 Calendar Poster
Thursday, September 4, 2014
Monogram, M106 Spiral Galaxy, Canes Venatici Lamp
A gorgeous something for Valentine's day to express your love and featuring a cute animal. Click to see, personalize and buy.
tagged with: star galaxies, outer space picture, deep space astronomy, hubble galaxy photography, supermassive black hole, spiral arms, seyfert ii galaxy, constellation canes venatici, hunting dog stars, hrbstslr m106cv, messier 106
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
»visit the HightonRidley store for more designs and products like this
The Zazzle guarantee: We promise 100% satisfaction. If you don't absolutely love it, we'll take it back!
tagged with: star galaxies, outer space picture, deep space astronomy, hubble galaxy photography, supermassive black hole, spiral arms, seyfert ii galaxy, constellation canes venatici, hunting dog stars, hrbstslr m106cv, messier 106
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.
more items with this image
more items in the Galaxies, Stars and Nebulae series
image code: m106cv
Image credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and R. Gendler (for the Hubble Heritage Team), J. GaBany
»visit the HightonRidley store for more designs and products like this
The Zazzle guarantee: We promise 100% satisfaction. If you don't absolutely love it, we'll take it back!
Zazzle Cake Pop from Bebop's Weddings: Springtime Wedding Cake Pops
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Wednesday, September 3, 2014
Stephans Quintet deep space star galaxy cluster Square Wallclocks
A gorgeous something for Valentine's day to express your love and featuring a cute animal. Click to see, personalize and buy.
tagged with: star galaxies, outer space picture, deep space astronomy, galaxy cluster, galaxy quintet, stephans quintet, hicksons compact group, spiral galaxy, eliptical galaxy, hrbstslr stkcg
Galaxies, Stars and Nebulae series A clash among members of a famous galaxy quintet reveals an assortment of stars across a wide color range, from young, blue stars to aging, red stars.
This portrait of Stephan's Quintet, also known as Hickson Compact Group 92, was taken by the new Wide Field Camera 3 (WFC3) aboard NASA's Hubble Space Telescope. Stephan's Quintet, as the name implies, is a group of five galaxies. The name, however, is a bit of a misnomer. Studies have shown that group member NGC 7320, at upper left, is actually a foreground galaxy about seven times closer to Earth than the rest of the group.
Three of the galaxies have distorted shapes, elongated spiral arms, and long, gaseous tidal tails containing myriad star clusters, proof of their close encounters. These interactions have sparked a frenzy of star birth in the central pair of galaxies. This drama is being played out against a rich backdrop of faraway galaxies.
The image, taken in visible and near-infrared light, showcases WFC3's broad wavelength range.
The colors trace the ages of the stellar populations, showing that star birth occurred at different epochs, stretching over hundreds of millions of years. The camera's infrared vision also peers through curtains of dust to see groupings of stars that cannot be seen in visible light.
NGC 7319, at top right, is a barred spiral with distinct spiral arms that follow nearly 180 degrees back to the bar. The blue specks in the spiral arm at the top of NGC 7319 and the red dots just above and to the right of the core are clusters of many thousands of stars. Most of the quintet is too far away even for Hubble to resolve individual stars.
Continuing clockwise, the next galaxy appears to have two cores, but it is actually two galaxies, NGC 7318A and NGC 7318B. Encircling the galaxies are young, bright blue star clusters and pinkish clouds of glowing hydrogen where infant stars are being born. These stars are less than 10 million years old and have not yet blown away their natal cloud. Far away from the galaxies, at right, is a patch of intergalactic space where many star clusters are forming.
NGC 7317, at bottom left, is a normal-looking elliptical galaxy that is less affected by the interactions.
Sharply contrasting with these galaxies is the dwarf galaxy NGC 7320 at upper left. Bursts of star formation are occurring in the galaxy's disk, as seen by the blue and pink dots. In this galaxy, Hubble can resolve individual stars, evidence that NGC 7320 is closer to Earth.
NGC 7320 is 40 million light-years from Earth. The other members of the quintet reside 290 million light-years away in the constellation Pegasus.
These farther members are markedly redder than the foreground galaxy, suggesting that older stars reside in their cores. The stars' light also may be further reddened by dust stirred up in the encounters.
Spied by Edouard M. Stephan in 1877, Stephan's Quintet is the first compact group ever discovered.
WFC3 observed the quintet in July and August 2009. 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.
These Hubble observations are part of the Hubble Servicing Mission 4 Early Release Observations. NASA astronauts installed the WFC3 camera during a servicing mission in May to upgrade and repair the 19-year-old Hubble telescope.
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image code: stkcg
Image credit: ASA, ESA, and the Hubble SM4 ERO Team
»visit the HightonRidley store for more designs and products like this
The Zazzle guarantee: We promise 100% satisfaction. If you don't absolutely love it, we'll take it back!
tagged with: star galaxies, outer space picture, deep space astronomy, galaxy cluster, galaxy quintet, stephans quintet, hicksons compact group, spiral galaxy, eliptical galaxy, hrbstslr stkcg
Galaxies, Stars and Nebulae series A clash among members of a famous galaxy quintet reveals an assortment of stars across a wide color range, from young, blue stars to aging, red stars.
This portrait of Stephan's Quintet, also known as Hickson Compact Group 92, was taken by the new Wide Field Camera 3 (WFC3) aboard NASA's Hubble Space Telescope. Stephan's Quintet, as the name implies, is a group of five galaxies. The name, however, is a bit of a misnomer. Studies have shown that group member NGC 7320, at upper left, is actually a foreground galaxy about seven times closer to Earth than the rest of the group.
Three of the galaxies have distorted shapes, elongated spiral arms, and long, gaseous tidal tails containing myriad star clusters, proof of their close encounters. These interactions have sparked a frenzy of star birth in the central pair of galaxies. This drama is being played out against a rich backdrop of faraway galaxies.
The image, taken in visible and near-infrared light, showcases WFC3's broad wavelength range.
The colors trace the ages of the stellar populations, showing that star birth occurred at different epochs, stretching over hundreds of millions of years. The camera's infrared vision also peers through curtains of dust to see groupings of stars that cannot be seen in visible light.
NGC 7319, at top right, is a barred spiral with distinct spiral arms that follow nearly 180 degrees back to the bar. The blue specks in the spiral arm at the top of NGC 7319 and the red dots just above and to the right of the core are clusters of many thousands of stars. Most of the quintet is too far away even for Hubble to resolve individual stars.
Continuing clockwise, the next galaxy appears to have two cores, but it is actually two galaxies, NGC 7318A and NGC 7318B. Encircling the galaxies are young, bright blue star clusters and pinkish clouds of glowing hydrogen where infant stars are being born. These stars are less than 10 million years old and have not yet blown away their natal cloud. Far away from the galaxies, at right, is a patch of intergalactic space where many star clusters are forming.
NGC 7317, at bottom left, is a normal-looking elliptical galaxy that is less affected by the interactions.
Sharply contrasting with these galaxies is the dwarf galaxy NGC 7320 at upper left. Bursts of star formation are occurring in the galaxy's disk, as seen by the blue and pink dots. In this galaxy, Hubble can resolve individual stars, evidence that NGC 7320 is closer to Earth.
NGC 7320 is 40 million light-years from Earth. The other members of the quintet reside 290 million light-years away in the constellation Pegasus.
These farther members are markedly redder than the foreground galaxy, suggesting that older stars reside in their cores. The stars' light also may be further reddened by dust stirred up in the encounters.
Spied by Edouard M. Stephan in 1877, Stephan's Quintet is the first compact group ever discovered.
WFC3 observed the quintet in July and August 2009. 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.
These Hubble observations are part of the Hubble Servicing Mission 4 Early Release Observations. NASA astronauts installed the WFC3 camera during a servicing mission in May to upgrade and repair the 19-year-old Hubble telescope.
more items with this image
more items in the Galaxies, Stars and Nebulae series
image code: stkcg
Image credit: ASA, ESA, and the Hubble SM4 ERO Team
»visit the HightonRidley store for more designs and products like this
The Zazzle guarantee: We promise 100% satisfaction. If you don't absolutely love it, we'll take it back!
Zazzle Cufflinks from Bebops: Cardinal Cufflinks
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Zazzle wood canvas from Northern World And Wildlife: Sheep Peak Lodge
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Zazzle Pet Clothing from Electrovista.com: Keep Calm and Eat Bacon
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