Oftentimes called “ghost particles,” neutrinos can travel through nearly everything (the sun, the earth, you!) undetected. Because they are nearly massless, gravitational fields do not affect neutrinos; Similarly, because they are chargeless, electric and magnetic fields do not con affect neutrinos. This lack of interaction is advantageous for IceCube researchers – when they detect a neutrino, it is a
In this lesson, students will be introduced to the Standard Model, learning key vocabulary such as Fermions, Hadrons, Mesons, Baryons, Quarks, Leptons, particles, and anti-particles. In particular, students will come to understand what a neutrino is and why it is such a unique particle. This understanding connects to the IceCube Neutrino Observatory’s search for neutrinos in an effort to
Students will develop research questions that will help them develop an ecosystem profile (species/conditions etc.) of a local pond. Their results will be compared with data from the McMurdo Dry Valley Lakes in Antarctica. Discussions about climate and energy dynamics will be conducted as conclusions are drawn. A map and key for the local pond (species/locations/conditions) will be
During this lesson, students will learn basic glacial features and how to interpret Topographic maps and satellite images in order to create a model replica of a glacier valley. The Dry Valleys of Antarctica have classic glacial features, both in the barren valleys and in the remaining glaciers in the area. The glaciers are a major contributor to