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N90 Art Print featuring the photograph Small Magellanic Cloud, Region N90 by Science Source

The watermark in the lower right corner of the image will not appear on the final print.

Frame

Top Mat

Top Mat

Bottom Mat

Bottom Mat

Dimensions

Image:

8.00" x 8.00"

Overall:

10.00" x 10.00"

 

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Small Magellanic Cloud, Region N90 Art Print

Science Source

by Science Source

$53.00

Product Details

Small Magellanic Cloud, Region N90 art print by Science Source.   Our art prints are produced on acid-free papers using archival inks to guarantee that they last a lifetime without fading or loss of color. All art prints include a 1" white border around the image to allow for future framing and matting, if desired.

Design Details

This new image taken with NASA's Hubble Space Telescope depicts bright, blue, newly formed stars that are blowing a cavity in the center of a... more

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3 - 4 business days

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Small Magellanic Cloud, Region N90 Photograph by Science Source

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Art Print Tags

art prints space art prints n90 art prints ngc 602 art prints n 90 art prints star cluster art prints galaxy art prints galaxies art prints star art prints star formation art prints stellar wind art prints radiation art prints nebula art prints nebulae art prints space exploration art prints hubble space telescope art prints

Photograph Tags

photographs space photos n90 photos ngc 602 photos n 90 photos star cluster photos galaxy photos galaxies photos star photos star formation photos stellar wind photos radiation photos nebula photos nebulae photos space exploration photos hubble space telescope photos

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Artist's Description

This new image taken with NASA's Hubble Space Telescope depicts bright, blue, newly formed stars that are blowing a cavity in the center of a star-forming region in the Small Magellanic Cloud. At the heart of the star-forming region, lies star cluster NGC 602. The high-energy radiation blazing out from the hot young stars is sculpting the inner edge of the outer portions of the nebula, slowly eroding it away and eating into the material beyond. The diffuse outer reaches of the nebula prevent the energetic outflows from streaming away from the cluster. Ridges of dust and gaseous filaments are seen towards the northwest (in the upper-left part of the image) and towards the southeast (in the lower right-hand corner). Elephant trunk-like dust pillars point towards the hot blue stars and are telltale signs of their eroding effect. In this region it is possible with Hubble to trace how the star formation started at the center of the cluster and propagated outward, with the youngest stars sti...

 

$53.00

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