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Abstract:

This lecture provides an in-depth exploration of the Milky Way galaxy, focusing on historical discoveries, its structure, and dynamics. It recounts the pivotal "Great Debate" of 1920, explaining how the understanding of Cepheid variable stars revolutionized distance measurements, establishing that "nebulae" like Andromeda are independent external galaxies. The speaker details how the distribution of globular clusters revealed the Milky Way's disk shape and the Sun's off-center position. A significant portion of the talk is dedicated to galactic rotation, explaining the concept of differential rotation and the use of Oort constants to calculate the Sun's orbital speed. The lecture highlights the crucial role of radio astronomy, particularly the 21 cm hydrogen line, in mapping the galaxy's rotation curve, which surprisingly exhibits a flat velocity profile beyond the central region. This observed flat rotation curve, contrary to predictions based solely on visible matter, leads to the fundamental implication of dark matter within the galaxy.

Exploring the Milky Way: Unveiling Our Galaxy's Structure and Dynamics

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