'Mass luminosity' diaporamas de présentation

The Strange Universe

The Strange Universe. The Strange Universe Sanjay K. Ghosh Department of Physics Bose Institute Kolkata. Early Efforts Earliest astronomical records : 2000 - 1500 BC ? Mesopotamian priests : systematic astronomical records Sumarians, Babylonians, and Egyptians develop astronomy

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Chapter 10

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1 snapshots and timescales

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The structure and evolution of stars

The structure and evolution of stars. Lecture 7: The structure of main-sequence stars: homologous stellar models. Dr. Stephen Smartt Department of Physics and Astronomy S.Smartt@qub.ac.uk. Learning Outcomes. Student will learn:

344 views • 20 slides

The structure and evolution of stars

The structure and evolution of stars. Lecture 7: The structure of main-sequence stars: homologous stellar models. Learning Outcomes. Student will learn:

329 views • 20 slides

The structure and evolution of stars

The structure and evolution of stars. Lecture 7: The structure of main-sequence stars: homologous stellar models. Dr. Stephen Smartt Department of Physics and Astronomy S.Smartt@qub.ac.uk. Learning Outcomes. Student will learn:

200 views • 20 slides

The structure and evolution of stars

The structure and evolution of stars. Lecture 7: The structure of main-sequence stars: homologous stellar models. Learning Outcomes. Student will learn:

208 views • 20 slides

Announcements

Announcements. Homework: Supplemental Problems Next exam is scheduled for April 1. It will be delayed one week to April 8. A formula sheet for it has been posted. The HR Diagram shows that stars group together by type. Most stars are on the Main Sequence.

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