Lesson Plans:
Decoding Starlight
The student will use data collected from the Chandra X-ray Observatory
to calculate the average pixel intensity of X-ray emissions from a
supernova remnant.
Timing an X-Ray Pulsar
Using XTE observations of the Crab Pulsar, the student will be able
to:
Determine the period of the light intensity.
Interpret this period as the period of rotation of the object.
Identify this object as a neutron star.
Investigating the Crab Nebula
The student will review supernova phenomenon, predict the
characteristics of the Crab Nebula, and relate observations of the
Crab to the predictions.
Properties of Planetary Nebula
The student will examine many of the properties of planetary nebulae,
including their composition, size and evolution.
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