How Old Is It - 04 - How Old are Stars
Text at http://howfarawayisit.com/wp-content/uploads/2019/10/How-Old-Is-It-03-Stars.pdf
Credits at http://howfarawayisit.com/wp-content/uploads/2019/10/How-Old-Is-It-05-Credits-and-Research.pdf
Music Free Version at https://www.youtube.com/watch?v=6Wv4a5ln1pQ&list=PLpH1IDQEoE8TVy4gIXoua9IcYLB5uCjHJ
at 23:26 calculation error. S.B. 40.1N = 9.01 pounds
In this chapter of the “How Old Is It” video book, we’ll cover stars – second generation stars. We start with giant molecular clouds and what may trigger their collapse into star clusters. We’ll follow their size, density, and temperature as they move from hydrostatic equilibrium to fragments to stars. We’ll then follow the collapse of a fragment capable of creating a star like our Sun. We’ll cover how circumstellar disks around central massive objects are formed. We’ll cover the Protostar phase and examine a few like the ones in the Eagle Nebula and Orion. We’ll cover T-Tauri stars, their properties, and examine several including T Tauri itself, XZ Tauri, and others. We’ll cover how these giant molecular clouds form Open and Globular clusters and how Field Stars like our Sun have left their starting clusters. We’ll follow stars as they start burning hydrogen and migrate to the Main Sequence on the H-R Diagram. We’ll take a deep dive into the hydrogen fusion that powers stars. With a focus on our Sun, we’ll compute proton collision and fusion rates. In order to understand the mass-luminosity relationship better, we’ll cover the Coulomb Barrier and how Tunneling through it works. And finally, we’ll examine what happens to a star once it runs out of hydrogen fuel.
Music:
@00:00 Giordani, Giuseppe: “Caro Mio Ben” - from the album “Meditation: Classical Relaxation” 2010
@06:56 Chopin, Fryderyk: “Prelude in E Minor, Op. 28, No. 4” – from the album “Chopin: The Romantic World Of Chopin's Piano, Vol. 3” 2000
@10:39 Puccini, Giacomo: La rondine: “La rondine, Act I: Doretta's Aria (arr. for flugelhorn and brass band)” - Grimethorpe Colliery RJB Band with Peter Parkes from the album Grimethorpe Colliery Band: Melody Shop (The) 1998
@14:09 Gluck, Christoph Willibald: “Dance Of The Blessed Spirits (from Orpheus and Eurydice)” conductor Herbert Kegel from the album “Meditation: Classical Relaxation” 2010
@24:33 Schubert, Franz: “Andante con moto (from Symphony No. 8)” – Conductor Janos Kovacs; from the album “Meditation: Classical Relaxation” 2010
Видео How Old Is It - 04 - How Old are Stars канала David Butler
Credits at http://howfarawayisit.com/wp-content/uploads/2019/10/How-Old-Is-It-05-Credits-and-Research.pdf
Music Free Version at https://www.youtube.com/watch?v=6Wv4a5ln1pQ&list=PLpH1IDQEoE8TVy4gIXoua9IcYLB5uCjHJ
at 23:26 calculation error. S.B. 40.1N = 9.01 pounds
In this chapter of the “How Old Is It” video book, we’ll cover stars – second generation stars. We start with giant molecular clouds and what may trigger their collapse into star clusters. We’ll follow their size, density, and temperature as they move from hydrostatic equilibrium to fragments to stars. We’ll then follow the collapse of a fragment capable of creating a star like our Sun. We’ll cover how circumstellar disks around central massive objects are formed. We’ll cover the Protostar phase and examine a few like the ones in the Eagle Nebula and Orion. We’ll cover T-Tauri stars, their properties, and examine several including T Tauri itself, XZ Tauri, and others. We’ll cover how these giant molecular clouds form Open and Globular clusters and how Field Stars like our Sun have left their starting clusters. We’ll follow stars as they start burning hydrogen and migrate to the Main Sequence on the H-R Diagram. We’ll take a deep dive into the hydrogen fusion that powers stars. With a focus on our Sun, we’ll compute proton collision and fusion rates. In order to understand the mass-luminosity relationship better, we’ll cover the Coulomb Barrier and how Tunneling through it works. And finally, we’ll examine what happens to a star once it runs out of hydrogen fuel.
Music:
@00:00 Giordani, Giuseppe: “Caro Mio Ben” - from the album “Meditation: Classical Relaxation” 2010
@06:56 Chopin, Fryderyk: “Prelude in E Minor, Op. 28, No. 4” – from the album “Chopin: The Romantic World Of Chopin's Piano, Vol. 3” 2000
@10:39 Puccini, Giacomo: La rondine: “La rondine, Act I: Doretta's Aria (arr. for flugelhorn and brass band)” - Grimethorpe Colliery RJB Band with Peter Parkes from the album Grimethorpe Colliery Band: Melody Shop (The) 1998
@14:09 Gluck, Christoph Willibald: “Dance Of The Blessed Spirits (from Orpheus and Eurydice)” conductor Herbert Kegel from the album “Meditation: Classical Relaxation” 2010
@24:33 Schubert, Franz: “Andante con moto (from Symphony No. 8)” – Conductor Janos Kovacs; from the album “Meditation: Classical Relaxation” 2010
Видео How Old Is It - 04 - How Old are Stars канала David Butler
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