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Magnetic Fields on Solar-Type Stars

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The Sun rotates slowly, about once every 24 days at its equator although the hot gas at every latitude rotates at a slightly different rate. Rotation helps to drive the mechanisms that p...

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...
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