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 lesson focuses on adaptations as a driving force in evolutionary diversity. Adaptations are characteristics within a species that enhance its chances of survival and reproduction. Adaptations can be behavioral, structural, or functional. Students must understand that these adaptations are not acquired in the course of the organism’s lifetime, but are inherited traits that have been passed down
Note: This event was not for our typical classroom-based education audience.
WAIS Divide (West Antarctic Ice Sheet), where the Velvet Ice team conducted its research, has recently be found to be one of the most vulnerable areas of Antarctica to global climate change. If recent predictions hold true, major glaciers in WAIS could collapse within 100 years, triggering massive shifts
This one hour event is an introduction to the expedition with Yamini Bala and her team. They address life at McMurdo and what it will be like at their remote field site at WAIS Divide (West Antarctic Ice Sheet).