Making it Big in Astronomy – Dr. Jerry Nelson

(December 19, 2007) In 1977 Jerry Nelson was physicist at UC’s Lawrence Berkeley Laboratory, and he was asked to join a group to vision the future of US astronomy. For Nelson it was a once-in-a-lifetime chance to design a major apparatus with “cosmic implications.” His work translated into the revolutionary twin 10-meter Keck telescopes. Decades later, Nelson’s gift for devising solutions to large technical challenges continues to make its mark in astronomical innovation.
Science Standards: How Information is Collected and Analyzed; How a Telescope Works

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UCLA observers will work with MOSFIRE tonight. And UCI/UCB observers will work with NIRC2-LGS/NIRC2-NGS. Sun set 05:59:00pm rise 06:12:00am
Observers from UCR will use MOSFIRE on Keck 1, while on Keck 2, UCI observers will use DEIMOS. Sun set 06:00:00pm rise 06:12:00am
On Keck 1, we have UCR observers using LRIS-ADC. On Keck 2, we have Swinburne observers using ESI. Sun set 06:00:00pm rise 06:11:00am
CIT observers will use LRISP-ADC on Keck 1, and UCSC observers will use ESI on Keck 2 tonight. Sun set 06:01:00pm rise 06:11:00am
Our guests tonight are observers from UCSC and Swinburne, using LRISP-ADC and DEIMOS respectively. Sun set 06:02:00pm rise 06:10:00am