Session Date
Lesson Topic
White dwarfs
Lesson Outline
In today's second lesson, we continued with the fate of stars like our Sun. Once the star becomes unstable and loses its outer layers after the red giant phase, what's left behind is a very dense object known as a white dwarf. White dwarfs are only about the size of our Earth, but matter is packed in so densely that one spoonful of 'white dwarf matter' weighs as much an elephant. Matter is no longer in the form that we are used to here on Earth, and we need to invoke the Pauli Exclusion Principle to understand how the atoms are packed in so tight. We again covered a lot of material, and even if Jared had to sit through two hours of class today, he remained attentive and inquisitive right until the end.
Assignment
Find the answers to the questions brought up in class, e.g. how long does it take for a star to become a red giant
Session Minutes
60
Minutes Student Attended
60
Lesson Comments
We again covered a lot of material, and even if Jared had to sit through two hours of class today, he remained attentive and inquisitive right until the end. I'm starting to be a little stricter with Jared regarding his homework, and instead of resisting it, he himself is already writing down the questions that he has to research for homework before I even get to tell him, 'Write that down" !
Session Hours
1.00
Hours Attended
1.00
Entry Status
Review Status
Student Name(s)
Subject
School