Recycling and Synthesis in the Cosmos – Dr. Mike Bolte

(February 10, 2008) Dr. Mike Bolte from the University of California Observatories discusses the enormous advances being made in the study of stellar evolution and the genesis of elements from the simple to the complex. Bolte and his collaborators make observations of the oldest stars and star clusters in our Milky Way Galaxy to better understand the first epoch of star formation. Catch a glimpse of the complex methodology and modeling required to measure the chemistry of the cosmos using the Keck telescopes.

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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