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<Dark Matter>

ASTROID. <Dark Matter>. Lesson Plan Guided Research Model Dr. Christian Reimers reimers@astro.univie.ac.at http://www.virtuelleschule.at/cosmos/. [1]. [2]. [1] Gravitational Lens, HST observation of Abell 2218 [2] Rotation curve (observed and theoretical), SuW 1/2005 S.32ff.

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<Dark Matter>

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  1. ASTROID <Dark Matter> Lesson PlanGuided ResearchModel Dr. Christian Reimersreimers@astro.univie.ac.athttp://www.virtuelleschule.at/cosmos/ [1] [2] [1] Gravitational Lens, HST observation of Abell 2218 [2] Rotation curve (observed and theoretical), SuW 1/2005 S.32ff.

  2. <Dark Matter> • General InformationThe scenario aims to illustrate one of the evidences for dark matter. This includes the study of the rotational curves of spiral galaxies. • Duration: 3 x 50 min. • Vocabulary: dark matter, galaxies, rotation curve • Tools and Materials: PC with Internet connection, Paper, work sheets (excel, diagram), Pencil • Aims and Objectives: Students should ...- ... be able to plot data- ... learn basics on the structure and detection of matter • Students‘ Misconception: - confusing types of matter - visible parts of galaxies are dominant

  3. <Dark Matter> • Educational Phase 1: Stimulation • Presentation/Discussion:motivation by emotion (pictures of galaxies) [1] HST observation of M51 „Whirlpool Galaxy“ [2] HST observation of M104 „Sombrero Galaxy“

  4. <Dark Matter> • Educational Phase 2: Scientific Prediction • Discuss list of possible dark matter candidates and their interactions with measurable quantities / indirect detection • Draw up a list on the blackboard with various proposed methods and missions to detect dark matter • Finding pictures of galaxies and their rotation curves(internet research) [3] Doppler image of M33 [1] Illustration of the galaxies rotation (Sextans A) [2] Interactive Applet on the Doppler effect

  5. <Dark Matter> • Educational Phase 3: Experimental Activities • Kepler rotation in the Solar System (central point mass) • Applet with M(r) => v(r) [in development] [1] Work sheet: Kepler rotation in the Solar System [2] „rotcurve“-Applet of real galaxieshttp://burro.cwru.edu/JavaLab/RotcurveWeb/main.html

  6. <Dark Matter> • Educational Phase 4: Abstraction of the finding • Prediction Compared to Results:v2(r) = G * (Mvisible(r) + Mdark(r)) / rIf existing matter is only the observed (visible) matter, the rotation curves of spiral galaxies could not be described.Mtot > Mvisible => Mdark thus Mtot = Mvisible + MdarkWith assistance of Tutorials and Links. • Discussion: Short discussion on detection methods and theoretical issues.

  7. <Dark Matter> • Educational Phase 5: Consolidation • Quiz/Multiple-Choice-Test with Feedback • Exercises/Tasks: • Comparing simple calculations and self-composed diagrams with obtained data • Talk: Thoeretical background ist provided to find information on the internet to start a talk about types of dark matter • Discussion: Change of paradigm of matter over the centuries [1] Multiple-Choice-Test (ASTROID)

  8. <Dark Matter> • Ressources: • Worksheet (solar system; xls) • Worksheet (diagram; pdf) • Simulation (rotation curve; Applet) • Glossary (of related terms; pdf) • Examples with solutions and diagrams (for teachers; pdf) • Informationsheet (types of matter; pdf) • Informationsheet (posibilities of types of DM; pdf) • Informationsheet (internetlinks and further infos; pdf)

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