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SAO-Designed Solar Wall Featured at Cooper-Hewitt

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On Friday, Dec. 12, 1902, Andrew Carnegie moved into his just-finished home at 91st Street and Fifth Avenue, with his wife, Louise, and his 5-year-old daughter, Margaret, to whom he hande...

Eyes on Orion - An Interview with Jonathan McDowell

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On Friday, NASA successfully launched its next-generation spaceship farther than any astronaut has flown since the Apollo program of the 1960s. Though the Orion was unmanned during the te...

Twinkle, Twinkle New-Born Star

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Stars are born in dense, cool clouds of molecular gas and dust. When the local density is high enough, the matter can gravitationally collapse to form a new star, a so-called young stella...

Staying Warm: The Hot Gas in Clusters of Galaxies

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Most galaxies lie in clusters, groupings of a few to many thousands of galaxies. Our Milky Way galaxy itself is a member of the "Local Group," a band of about fifty galaxies whose other ...

Measuring the Ancient Solar Nebula's Magnetic Field

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Astronomical observations of young protostars indicate that early planetary systems evolved from the dust in a protoplanetary disk very quickly - in under five million years. Such short ...

The Future of Neutrino Cosmology

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One of the most remarkable aspects of modern cosmology is that the properties of the largest physical structures in the universe reveal the properties of the smallest. The largest struct...

The Role of Magnetic Fields in Star Formation

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Massive stars tend to form in clusters as the gas and dust in molecular clouds collapses and fragments under the influence of gravity. In the classic picture of star formation, gravity m...
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