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The Milky Way’s Bulge - From a Hypothesized Blob to a Remarkably Detailed Picture

Hubble Space Telescope via YouTube

Overview

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This course aims to provide a detailed understanding of the central bulge of the Milky Way galaxy, including the composition, formation processes, and implications for planet formation and life evolution. The course covers topics such as chemistry, metallicity, star distributions, and the significance of the bulge. Participants will learn about the ages and chemical abundances of stars in the bulge, as well as the complexities and gaps in current knowledge. The teaching method involves a recorded lecture by an expert in the field, supplemented with visual aids such as images and diagrams. This course is intended for individuals interested in astronomy, astrophysics, or space science, particularly those with a curiosity about the structure and evolution of our galaxy.

Syllabus

Introduction
Upcoming lectures
Observatory update
Webb delay
Omi
Omi January 2018
PDS 70
News from the Universe
Why the Bulge Matters
Part 1 Chemistry
Part 2 Metallicity
Hubble Tuning Fork Diagram
Bared Spiral Galaxy
Deep Rejected Model
MidInfrared Image
The X
Orbits
Bars
Metalrich Stars
First Evidence
Distributions of Stars
Shortage of Younger Stars
Stars Near the Sun
The Wrinkle
New Analysis
Conclusions

Taught by

Hubble Space Telescope

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