Dorkbot Videos
by Greg on Nov.21, 2009, under Science Life Alert, Science Life Video
For you artists and people who like to mix their science and creativity jones and are looking for some inspiration, there are 11 (soon to be 12) Dorkbot presentations up on DorkBot’s Vimeo page. They range from electronic projects at elementary schools, personal indoor farms for nyc apartments, dolls mutated into sexy robots, and other incredibly interesting visions from artists all around. They were captured by me and edited by my good friend Joe Frey. We are calling this little thing of ours Content Content and will continue to bring you an archive of Dorkbot -NYC’s exciting presentations.
Dorkbot meets every the first Wednesday of every month at 7p at Location 1 in soho.
:content content, dorkbot
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Nasa's Image of the Day
Little Galaxy With a Tail
This infrared portrait of the Small Magellanic Cloud, taken by NASA's Spitzer Space Telescope, reveals stars and dust in this galaxy as never seen before. T The image shows the main body of the Small Magellanic Cloud, which is comprised of the "bar" and "wing" on the left and the "tail" extending to the right. The bar contains both old stars (in blue) and young stars lighting up their natal dust (green/red). The wing mainly contains young stars. The tail contains only gas, dust and newly formed stars. Spitzer data has confirmed that the tail region was recently torn off the main body of the galaxy. Two of the tail clusters, which are still embedded in their birth clouds, can be seen as red dots. The data in this image are being used by astronomers to study the lifecycle of dust in the entire galaxy: from the formation in stellar atmospheres, to the reservoir containing the present day interstellar medium, and the dust consumed in forming new stars. The dust being formed in old, evolved stars (blue stars with a red tinge) is measured using mid-infrared wavelengths. The present day interstellar dust is weighed by measuring the intensity and color of emission at longer infrared wavelengths. The rate at which the raw material is being consumed is determined by studying ionized gas regions and the younger stars (yellow/red extended regions). The Small Magellanic Cloud, and its companion galaxy the Large Magellanic Cloud, are the two galaxies where this type of study is possible. Image Credit: NASA/JPL-Caltech/STScI
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