
Abstract:
One of the fundamental questions facing astronomers and astrophysicists is the origin of the elements that make up the universe around us. This investigation provides an opportunity to use data collected by scientists who work on answering that question. In the investigation the learner will first access Advance Composition Explorer (ACE) data to look for a correlation with known energetic solar events. Secondly, the learner will access ACE /SWEPAM data to determine if there is a correlation between the ratio of He++ to H+ ions as compared with electron and proton fluxes (rates of particle flow). The ratio of He++ to H+ found in the solar wind will also be compared to the ratio of He++ to H+ found in the Sun. And finally, the learner will compare the relative abundance of elements found in the Earth as a whole, to those found in the Sun, to those found in the solar wind. In a science classroom, the investigation can be tied in with a unit on the periodic table, fusion, stellar evolution, and a variety of other Earth and space science topics. The select accompanying Educational Brief: Fusion & Nucleosynthesis
Outcome:
PART ONE
PART TWO
Suggested Grade Level & Duration:
Grades 9-12; 1 to 2 fifty-minute periods.
Materials:
The learner will need a computer with Internet access, a browser, a scientific calculator, and a pencil and paper.
Background - Procedure - Standards - Credits