The Daily Croissant

Eclectic Perambulations in the Noosphere

  • Stellar Nursery in the Arms of NGC 1672

    • 29 Apr 2012
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    • April 29 2012 Astronomy Hubble
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    "The barred spiral galaxy NGC 1672, showing up clusters of hot young blue stars along its spiral arms, and clouds of hydrogen gas glowing in red. Delicate curtains of dust partially obscure and redden the light of the stars behind them. NGC 1672's symmetric look is emphasised by the four principal arms, edged by eye-catching dust lanes that extend out from the centre." 
    via spacetelescope.org

     

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  • New Panorama of 30 Doradus Celebrates Hubble’s 22nd Anniversary

    • 24 Apr 2012
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    • Anniversary April 24 2012 Astronomy Celebration Hubble
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    A new view of 30 Doradus, one of the largest mosaics ever assembled from Hubble photos, to celebrate HST's 22nd anniversary. Source: ESA’s Hubble website 

    "Happy birthday to the Hubble Space Telescope! On April 24, 1990, HST was launched into low Earth orbit. Now, nearly 22 years later, Hubble is still producing incredible, stunning images of the farthest reaches of the Universe. For this year’s anniversary, the Hubble team took a special panoramic view of 30 Doradus, a raucous stellar breeding ground, located in the heart of the Tarantula nebula. The image comprises one of the largest mosaics ever assembled from Hubble photos and consists of observations taken by Hubble’s Wide Field Camera 3 and Advanced Camera for Surveys, combined with observations from the European Southern Observatory’s MPG/ESO 2.2-metre telescope that trace the location of glowing hydrogen and oxygen. The Tarantula nebula is 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus."

    via universetoday.com

     

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  • A Lucky Observation of an Enigmatic Cloud

    • 13 Apr 2012
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    • April 13 2012 Astronomy Hubble
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    "The little-known nebula IRAS 05437+2502 billows out among the bright stars and dark dust clouds that surround it in this striking image from the Hubble Space Telescope. It is located in the constellation of Taurus (the Bull), close to the central plane of our Milky Way galaxy. Unlike many of Hubble’s targets, this object has not been studied in detail and its exact nature is unclear. At first glance it appears to be a small, rather isolated, region of star formation and one might assume that the effects of fierce ultraviolet radiation from bright young stars probably were the cause of the eye-catching shapes of the gas. However, the bright boomerang-shaped feature may tell a more dramatic tale. The interaction of a high velocity young star and the cloud of gas and dust may have created this unusually sharp-edged bright arc. Such a reckless star would have been ejected from the distant young cluster where it was born and would travel at 200 000 km/hour or more through the nebula." 
    via spacetelescope.org

     

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  • Pandora's Cluster – Clash of the Titans

    • 9 Apr 2012
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    • April 09 2012 Astronomy Hubble
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    "A team of scientists studying the galaxy cluster Abell 2744, nicknamed Pandora's Cluster, have pieced together the cluster's complex and violent history using telescopes in space and on the ground, including the Hubble Space Telescope, the European Southern Observatory's Very Large Telescope, the Japanese Subaru telescope, and NASA's Chandra X-ray Observatory.

    The giant galaxy cluster appears to be the result of a simultaneous pile-up of at least four separate, smaller galaxy clusters. The crash took place over a span of 350 million years.

    The galaxies in the cluster make up less than five percent of its mass. The gas (around 20 percent) is so hot that it shines only in X-rays (colored red in this image). The distribution of invisible dark matter (making up around 75 percent of the cluster's mass) is colored here in blue."

    via hubblesite.org

     

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  • Infrared Sombrero

    • 21 Mar 2012
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    • Astronomy Galaxies Hubble March 21 2012
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    The Sombrero Galaxy in Infrared : Credit: R. Kennicutt 

    "This floating ring is the size of a galaxy. In fact, it is part of the photogenic Sombrero Galaxy, one of the largest galaxies in the nearby Virgo Cluster of Galaxies. The dark band of dust that obscures the mid-section of the Sombrero Galaxy in optical light actually glows brightly in infrared light. The above image, digitally sharpened, shows the infrared glow, recently recorded by the orbiting Spitzer Space Telescope, superposed in false-color on an existing image taken by NASA's Hubble Space Telescope in optical light. The Sombrero Galaxy, also known as M104, spans about 50,000 light years across and lies 28 million light years away. M104 can be seen with a small telescope in the direction of the constellation Virgo."

    via apod.nasa.gov

     

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  • Warped Spiral Galaxy ESO 510 13

    • 17 Mar 2012
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    • Astronomy Hubble March 17 2012
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    "How did spiral galaxy ESO 510-13 get bent out of shape? The disks of many spirals are thin and flat, but not solid. Spiral disks are loose conglomerations of billions of stars and diffuse gas all gravitationally orbiting a galaxy center. A flat disk is thought to be created by sticky collisions of large gas clouds early in the galaxy's formation. Warped disks are not uncommon, though, and even our own Milky Way Galaxy is thought to have a small warp. The causes of spiral warps are still being investigated, but some warps are thought to result from interactions or even collisions between galaxies. ESO 510-13, pictured above digitally sharpened, is about 150 million light years away and about 100,000 light years across."
    via apod.nasa.gov

     

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  • Firestorm of Star Birth in Centaurus A

    • 15 Mar 2012
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    • Astronomy Hubble Interactive March 15 2012
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    Resembling looming rain clouds on a stormy day, dark lanes of dust crisscross the giant elliptical galaxy Centaurus A. Hubble's panchromatic vision, stretching from ultraviolet through near-infrared wavelengths, reveals the vibrant glow of young, blue star clusters and a glimpse into regions normally obscured by the dust. This image was taken in July 2010 with Hubble's Wide Field Camera 3.
    via hubblesite.org

     

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  • Martian Avalanche, Earth’s Spaghetti-Like Magnetosphere and Spirograph Nebula

    • 20 Feb 2012
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    • Astronomy Earth February 20 2012 HiRISE Hubble Magnetospere Mars
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    An avalanche on Mars captured by the HiRISE camera on the Mars Reconnaissance Orbiter on November 27, 2011.

     

     Supercomputer simulation showing the tangled magnetosphere surrounding Earth.

     

     

    Spirograph Nebula Courtesy of the Hubble Space Telescope

     

    via universetoday.com

     

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  • The barred spiral galaxy NGC 1073

    • 10 Feb 2012
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    • Astronomy February 10 2012 Hubble
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    "Is this what we look like? Astronomers don’t know for sure exactly what the Milky Way looks like, but searching out other barred spiral galaxies like this one is helping scientists to learn more about our home. Galaxy NGC 1073 is located in the constellation of Cetus (The Sea Monster).Most of the known spiral galaxies have a bar structure in their center, and this new image offer a stunning, if not clear view of one of these types of galaxies."
    via universetoday.com

     

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  • New Supernova Remnant Lights Up

    • 29 Jan 2012
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    • Astronomy Hubble January 29 2012
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    "This Hubble Space Telescope image of SN 1987A shows the brightening ring of supernova debris. The closest supernova explosion seen in almost 400 years is located in the Large Magellanic Cloud. "
    via hubblesite.org

     

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