Tag: Mischel’s Marshmallows
Radiolab Saturday and delaying enjoyment
by Greg on Jul.25, 2009, under Science Life Musing
I have never read the works of Frank McCourt (author of popular books like Angela’s Ashes), but because he often graced my media staples like NPR, i had learned to appreciate and enjoy his take on America’s decadent persona. It is sad to see him and his insight go. He really put old cranky dudes like Andy Rooney to shame. I didn’t see his schtick reflect longing for the american idea of yesteryear (born in brooklyn, he grew up destitute in Ireland), but more of an indictment of materialism and its promise of easy joy.
Here is an interview i heard on NPR’s Studio 360 from McCourt on his ideas on how Americans raise their children. It’s a great listen: (continue reading…)
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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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