Resources

determination of the half-life of radon-220

measuring the carriage of α particles through the air from a source with radium-226

gaining insight into the system dynamics of a predator-prey model with sheep and wolves from a modeling perspective

Our universe started as a fog of particles, but slight variations in density allowed the formation of stars, galaxies, and the large-scale structures of the universe. In this lesson, we’ll discuss early structure formation and fast-forward to today’s stars with planets.

Our universe started as a fog of particles, but slight variations in density allowed the formation of stars, galaxies, and the large-scale structures of the universe. In this lesson, we’ll discuss early structure formation and fast-forward to today’s stars with planets.

The Earth is warm because energy created in the core of the Sun is able to travel from the Sun’s Core to its surface, and then shine through space all the way to Earth. As it travels, the light is transformed from deadly high-energy particles to the nice warm light that keeps us alive. In this lesson, we will discuss the primary ways energy is transported: convection, conduction, and radiation.

The Earth is warm because energy created in the core of the Sun is able to travel from the Sun’s Core to its surface, and then shine through space all the way to Earth. As it travels, the light is transformed from deadly high-energy particles to the nice warm light that keeps us alive. In this lesson, we will discuss the primary ways energy is transported: convection, conduction, and radiation.

The Earth is warm because energy created in the core of the Sun is able to travel from the Sun’s Core to its surface, and then shine through space all the way to Earth. As it travels, the light is transformed from deadly high-energy particles to the nice warm light that keeps us alive. In this lesson, we will discuss the primary ways energy is transported: convection, conduction, and radiation.

inquire on the statistical character of radioactive phenomena

gaining insight into the system dynamics of how aspects of student life influence the amount of money you have from a modeling perspective

perceive the condensation tracks caused by α and β particles from a source with radium-226, and their decay products

getting acquainted with several aspects of X-ray computed tomography

getting acquainted with several aspects of X-radiation