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Out of the Void Poster by Bebops
Tuesday, July 15, 2014
Zazzle Pair of Cufflinks from Bebops: Bird on a Branch Cuff Links
Zazzle Pair of Cufflinks from Bebops: Monarch Butterfly Abstract Cuff ...
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Monday, July 14, 2014
Eye - Stellar Nursery R136 on nebula background Square Sticker
tagged with: astronomy, envelope sealers, eye, stellar nursery, r136, 30 doradus nebula, massive stars, tarantula nebula, hrbstslr dorneblmc, galaxy stars, large magellanic cloud, star cluster, amazing hubble images
Galaxies, Stars and Nebulae series On a background of the Pelican and North American nebulae, an eye made from hundreds of brilliant blue stars wreathed by warm, glowing clouds appear in this the most detailed view of the largest stellar nursery in our local galactic neighborhood. The massive, young stellar grouping, called R136, is only a few million years old and resides in the 30 Doradus (or Tarantula) Nebula, a turbulent star-birth region in the Large Magellanic Cloud (LMC), a satellite galaxy of our Milky Way.
There is no known star-forming region in our galaxy as large or as prolific as 30 Doradus. Many of the diamond-like icy blue stars are among the most massive stars known. Several of them are over 100 times more massive than our Sun. These hefty stars are destined to pop off, like a string of firecrackers, as supernovas in a few million years. The image, taken in ultraviolet, visible, and red light by Hubble's Wide Field Camera 3, spans about 100 light-years.
The movement of the LMC around the Milky Way may have triggered the massive cluster's formation in several ways. The gravitational tug of the Milky Way and the companion Small Magellanic Cloud may have compressed gas in the LMC. Also, the pressure resulting from the LMC plowing through the Milky Way's halo may have compressed gas in the satellite. The cluster is a rare, nearby example of the many super star clusters that formed in the distant, early universe, when star birth and galaxy interactions were more frequent.
The LMC is located 170,000 light-years away and is a member of the Local Group of Galaxies, which also includes the Milky Way. The Hubble observations were taken Oct. 20-27, 2009. The blue color is light from the hottest, most massive stars; the green from the glow of oxygen; and the red from fluorescing hydrogen.
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image code: dorneblmc
image credit: Hubble's Wide Field Camera 3
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Zazzle Decal from Bebops: Princess Charming Think Green LED Window Dec...
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Carina Nebula in Argo Navis constellation Custom Jewelry
tagged with: jewelry, jewellery, carina nebula, argos navis constellation, carina the keel, star formation, gas clouds, galaxy stars, astronomy pictures, hrbstslr carnebngcttst, ngc 3372
Galaxies, Stars and Nebulae series Hubble's view of the Carina Nebula shows star birth in a new level of detail. The fantasy-like landscape of the nebula is sculpted by the action of outflowing winds and scorching ultraviolet radiation from the monster stars that inhabit this inferno. In the process, these stars are shredding the surrounding material that is the last vestige of the giant cloud from which the stars were born. The immense nebula is an estimated 7,500 light-years away in the southern constellation Carina the Keel (of the old southern constellation Argo Navis, the ship of Jason and the Argonauts, from Greek mythology).
The original image is a mosaic of the Carina Nebula assembled from 48 frames taken with Hubble Space Telescope's Advanced Camera for Surveys. The Hubble images were taken in the light of ionized hydrogen. Colour information was added with data taken at the Cerro Tololo Inter-American Observatory in Chile. Red corresponds to sulfur, green to hydrogen, and blue to oxygen emission.
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image code: carnebngcttst
Image credit: Hubble Space Telescope; colour data from the Cerro Tololo Inter-American Observatory, Chile
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Zazzle tile from arrayforhome: Running Giraffes
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