Lesson Plans:
Demonstrating
the Distances of Stars:
Students will: 1.study how stars may appear to be
equidistant from the Earth but are in actuality not, 2.use a model to
demonstrate the arrangement of stars, 3.study the importance of the
parallax effect in determining distance.Entropy
Demo:
This is an attention-grabbing introduction to cell energetics. Students
participate in building and knocking down a tower of paper cups which
represents an organized living system.
Animating Motion
Students will apply their knowledge of object motion by
animating sequences of pictures that model a set of physical conditions,
such as the orbital motion of planets and satellites, the effects of
gravity on a falling body, and motions of objects in inertial (moving)
frames of reference.
Astronomical Scales
Students understand how scaling
factors can be used to make representations of astronomical distances.
Earth and Beyond
Students will investigate one or more of the following
topics and develop a plan for the future regarding it: global warming,
lunar exploration, space travel, Mars exploration, or terraforming.
Exploration of Mars
For exploration of celestial
bodies, NASA has developed a three-phase strategy: reconnaissance,
surveillance, and in-depth study.
The
Future of the Milky Way
Students will speculate about the changes that are taking
place in our galaxy;
research the latest ideas on the future of the Milky Way; and
discuss the consequences of events that may happen in the future.
Galileo's Dialogue
Students will understand Galileo’s conclusions about the
position of Earth in the solar system raised objections from the Church.
Savage Sun
Students research the sun to find
out how it produces solar energy. They also research how nuclear energy
is produced in nuclear power plants.
A Star Is Born
Students use their knowledge of a
star’s behavior at various stages of its life to piece together a
picture of the star’s entire life.
Understanding Space Travel
Students design a city (on another planet) and will have
to work within the parameters of the unique conditions of the base
environment.
Stargazers
Students will understand the concept of redshift.
Eyes in the Sky
Students will understand the purpose of satellites.
Understanding the Universe
Students will understand the stages of evolution a star.
THE BEGINNING OF THE SCIENTIFIC REVOLUTION
Ptolemy, Copernicus, & the Church
Radioactive Decay: A Sweet Simulation of a Half-life
To demonstrate that the rates of decay of unstable nuclei
can be measured, that the exact time that a certain nucleus will decay
cannot be predicted, and that it takes a very large number of nuclei to
find the rate of decay.
|