Taking Measure of the Universe: How Big? How Old? How Do We Know?

Details Taking Measure of the Universe: How Big? How Old? How Do We Know? Taking Measure of the Universe: How Big? How Old? How Do We Know?

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kpls.confe...3k&link_type=abstract

Presented at the KITP: Public Lecture Series, Nov 12, 1997, Kavli Institute for Theoretical Physics, University of California, S

Physics

Scientific paper

Supernovae, exploding stars that shine as brightly as a billion Suns, areastonishing events which offer the best method for measuring the size andshape of the universe. Professor Kirshner explains how stars explodeand how astronomers piece together clues from these brilliant disastersto understand the age, shape, and fate of the Universe. Click here for more info.Robert P. Kirshner is Professor of Astronomy at Harvard University,where he chaired the department from 1990 to 1997. In Fall 1997 he was onsabbatical at the Institute for Theoretical Physics at the University ofCalifornia, Santa Barbara.Kirshner's scientific work has centered on supernova explosions andtheir application to measuring t he Universe. The author of over 150scientific publications, Kirshner is Principal Investigator for SINS, theSupernova Intensive Study with the Hubble Space Telescope. He is a memberof the American Academy of Arts and Sciences.At Harvard, Kirshner teaches a large core curriculum coursecalled Matter in the Universe. Dubbed "the David Letterman of astronomy"by his colleagues for his entertaining lecture manner, he has writtenpopular articles for National Geographic, ScientificAmerican, Natural History, Sky and Telescope, and theWorld Book Encyclopedia.

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