Antarctic ecosystems are undergoing change at unprecedented levels. In this lesson, students will use real data to evaluate the effect of climate change on Antarctic fish. Denise Hardoy created this lesson plan after joining Dr. Anne Todgham’s team studying Antarctic Fish Development Under Future Ocean Conditions in October/November of 2019.
Denise Hardoy created this resource after spending five weeks embedded with Dr. Anne Todgham’s team studying the effects of climate change on Antarctic fishes in 2019. This lesson addresses one of the most difficult aspects of science for students - making sense of data.
Objectives
Success Criteria
* Given a graph, students will write an analysis paragraph of a
I believe it is important to show my students what real science is… and that is how I found myself in Antarctica studying Antarctic Fish Development Under Future Ocean Conditions.
The PolarTREC program pairs teachers with research scientists for a symbiotic expedition. Scientists get a voice and a larger audience through the educator, and the educator
My experience at McMurdo Station involved the study of neutrons caused by cosmic radiation from the sun. The sun can be very active. Changes in the sun's active surface can result in the ejection of high energy particles (from solar flares, coronal mass ejections, or related phenomena). Some of these particles can get sent toward the earth
Presentation prepared for the Rochester Community Schools Board of Education related to the PolarTREC 2017 Neutron Monitors for Solar Study expedition.
Students will examine sunspots and track them at different latitudes on the Sun.
This activity is adapted from the Tracking Sunspots activity on NASA’s Solar and Heliocentric Observatory (SOHO) website (2009): https://soho.nascom.nasa.gov/classroom/for_students.html.
Objectives:
Students begin to familiarize themselves with solar activity by tracking sunspots at different latitudes on the Sun.
This activity is designed to get students thinking about
When radioactive elements decay they emit high-speed particles. These can be detected by use of a cloud chamber. The cloud chamber was invented by Charles Thomson Rees Wilson in 1911. The chamber works by saturating the air inside with alcohol vapor. Cooling the chamber with dry ice supersaturates the air. The energetic particles produced by the radioactive decay ionize
This is a suite of labs created by Michigan State University and the Joint Institute for Nuclear Astrophysics (JINA). It provides a number of lessons and activities in nuclear physics. It can be used to demonstrate the types of reactions typical in cosmic ray interactions and the interactions that the CosRay neutron monitors depend on.
The Energetic Ray Global Observatory (ERGO) is a program that will provide students and teachers with a small detector that is capable of detecting the cosmic rays in a manner very similar to CosRAY and IceCube. The unit is small and will allow data to be exported automatically to Google Maps.