Introductory Astronomy Complete University Course - Understanding Redshift: The Key to Cosmic Expansion

This video is part of a comprehensive series initially developed for William Paterson University and CUNY Hunter, aimed at supporting online classes and course materials for introductory astronomy. By engaging with all the videos within this series, you will effectively complete a full undergraduate course in astronomy, equipping yourself with the knowledge and skills necessary to navigate the night sky with confidence, learning all the basics and many advanced topics! Cosmic redshift, the relationship between a galaxy’s speed of recession and the redshift of its light, is explored. This delves into the mathematics behind redshift and measurement principles in cosmology. Atoms and molecules vibrate, generating electromagnetic waves called photons. Electrons primarily create these waves, but a proton vibrating can be used as an analogy. A charged particle’s vibration disturbs the electromagnetic field, emitting a photon. A photon is a wave packet with a beginning, middle, and end. Its wavelength is the distance between successive wave crests. As the universe expands, these crests stretch, causing redshift. To measure cosmic distances, we use a metric describing a uniformly expanding universe with isotropy and homogeneity. Simplifying this metric allows us to focus on photons traveling towards us, assuming a flat universe. This approach provides insights into the redshift-distance relationship. The redshift equation begins with the simplified metric, concentrating on the scale factor a(T) that varies over time. By integrating contributions of time and distance from emission to observation, we derive an integral expression for the scale factor. Examining wave crest differences yields an equation showing that the observed wavelength divided by the emitted wavelength equals the inverse ratio of scale factors at those temporal points. The redshift, z, is intrinsically linked to the Hubble expansion, directly related to the galaxy’s velocity via the speed of light. This relationship allows us to measure distances and velocities, reinforcing Hubble’s Law, which posits the universe’s expansion. This connects the observable universe to fundamental cosmological principles. The scale factor derived from redshift provides valuable information about the universe’s state. Defining the scale factor today as one simplifies calculations, enabling us to understand cosmic distances and times based on redshift observations, connecting theoretical models with empirical data. We now have a robust method for measuring a galaxy’s redshift by comparing emitted and observed wavelengths, determining distances and velocities through Hubble’s Law. This understanding of redshift emerges naturally from the expanding universe as described by the Friedman-Robertson-Walker metric. #Redshift #CosmicExpansion #HubbleLaw #Astronomy #Universe #Photons #Astrophysics #SpaceTime #Cosmology #Galaxies #LightWave #CosmicDistance #ObservableUniverse #FriedmanRobertsonWalker