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
This event was a 1 hr overview of Marine Life Science in Antarctica by Annamarie Pasqualone for the CISE Fall 2011 course and other interested educators.
This PolarConnect live event is a one hour presentation by PolarTREC teacher Michael League and the research team studying Adaptations of Marine Worms in Antarctica. The team covers field logistics, what they have found, and what the next step is in the scientific process.
This PolarConnect Event was with teacher Michael League and a team of researchers in Antarctica. They are looking at adaptations of marine worms. The event focused on adaptations and biomes. Length: approximately one hour
This PolarConnect Event was with teacher Michael League and a team of researchers in Antarctica. They are looking at adaptations of marine worms. The presentation was given a part of a teacher training in energy curriculum. Length: approximately one hour.
This PolarConnect Event was with teacher Michael League and a team of researchers in Antarctica. They are looking at adaptations of marine worms. The presentation focused on where they are, what they are doing, and what they found.