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Chapters 12 and 13 The Sun & Measuring the Properties of Stars “We are star stuff” - Carl Sagan Reminder... • star: A self-luminous, gravitationally bound, ball of gas that shines or has shone because of nuclear reaction in its interior Brown Dwarfs- Failed Stars • Mass < 8% the mass of the Sun • And 10-80 times the mass of Jupiter • First detected in 1995 The Sun and other stars are huge and massive!!! Figure 11.1 Our Sun Sunspots • regions of the photosphere that are dark and relatively cool • corresponds to regions of intense magnetic fields • Galileo monitored their movement to determine the rotation period of the Sun= about 1 month Figure 11.16 Sunspots occur when the magnetic field loops out of the photosphere Figure 11.18a Prominences Filaments Flares and Coronal Mass Ejections flares coronal mass ejections The Earth’s magnetic field protects us! Sunspot Cycle Maximum number Minimum number Figure 11.23 Sun’s Rotation Babcock’s Magnetic Dynamo Theory Binary Stars binary stars: multiple systems bound by gravity and orbiting each other around their center of mass (double star) Contact Binary Stars Star Clusters Open Cluster Globular Cluster Open or Globular Cluster?