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E. E. BARNARD
E. E. BARNARD
USA (1857 - 1923)
Best known for his discovery of Barnard's star in 1916, Edward Emerson Barnard was a gifted astronomer who grew up with little formal education. In 1876, he purchased his first telescope, a 5-inch refractor and discovered his first comet in 1881. In 1892, he discovered Amalthea, the fifth moon of Jupiter, making him the first to discover a new Jovian moon since Galileo in 1609. After joining Yerkes Observatory at the University of Chicago in 1895, Barnard spent great amounts of time photographing the Milky Way. Posthumously, his photographs were published in 1927 as A Photographic Atlas of Selected Regions of the Milky Way.
 

Disfrute estos perspicaces y educacionales videoclips obtenidos de más de 70 horas de entrevistas con las más notables figuras en astronomía tomadas durante la filmación del documental 400 Años del Telescopio.

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Taft E. Armandroff

Adaptive vs. active optics at Keck
Taft E. Armandroff - W. M. Keck Observatory

Active optics compensate for slowly varying influences on the telescope optical system, so the mirrors and the mechanical systems that hold the mirrors into place. So these change rather slowly over the course of the night with the direction of telescopes pointed or with temperature.

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Taft E. Armandroff

Keck telescopes overview
Taft E. Armandroff - W. M. Keck Observatory

The Keck telescopes are the two largest fully stirrable optical infrared telescopes in the world. They were the first of the new generation of large telescopes.

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Taft E. Armandroff

Astronomy answers at Keck
Taft E. Armandroff - W. M. Keck Observatory

How do stars form and evolve? How does the galaxy form and evolve nearby galaxies? What are the real influences? What makes one galaxy a spiral and another an elliptical? What makes one star live a hundred thousand years and another live sixteen billion years?

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Taft E. Armandroff

Segmented mirror technology
Taft E. Armandroff - W. M. Keck Observatory

Jerry Nelson developed a revolutionary technique for instead of having one mirror as all telescopes had before Keck and following the prescription of say, the classic telescopes like the Palomar 200 inch, the Mt. Wilson 100 inch, and the Kitt Peak and Cerra Tololo four meters to make it much more achievable in terms of issues like weight, in terms of cost to break the mirror into segments.

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Taft E. Armandroff

The 30-meter telescope
Taft E. Armandroff - W. M. Keck Observatory

The 30-meter telescope plans to use segmented mirror technology just like Keck, and between Keck and 30 meter telescope we have a great interchange of technical knowledge on topics like controls systems, for keeping the mirrors precisely positioned, working on illuminizing the segments and adaptive optic systems.

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