Tag: exhibit
Event: Rare Spider Silk Textile Exhibit
by Lauren on Sep.23, 2009, under Science Event
| September 23, 2009 12:00 pm | to | September 24, 2009 5:44 am |
Um, this looks awesome. I would definitely go check this out!
Where: Museum of Natural History
When: September 23, 2009 10am-5:45pm
Event Exhibition Opening: Toward the Sentient City
by Lauren on Sep.16, 2009, under Science Event, Science Life
| September 17, 2009 6:00 pm | to | November 7, 2009 9:00 pm |
An exhibit about science, technology, urban architecture, and the future organized by the Architectural League of New York.
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Still want to set the world on fire
Science, media, art, movies, politics, and what else I find interesting tweeting and reading on the internet.
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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