Star Systems and Galaxies
    Star Systems
        Open Clusters
 tens to thousands of young stars  
                individual stars  
                easily seen or verified that they exist (resolved)  
               Pleiades in the constellation Taurus 
 

        Globular Clusters
 
 Old stars  
            contain 100,000 to 1,000,000 stars,  
            High density in the center  
            individual stars from earth-based telescopes difficult to see  
            appear as a "glob" of light  
            Globular Cluster M15 see from Earth 
 

    Binary Stars
        Double stars
 
 
 
Kepler's laws  
                    elliptical orbit  
                    are on opposite sides of the center of mass. 
 
        The Sirius Binary System
 
Main sequence(Sirius A) and a white dwarf companion (Sirius B).  
                        orbits are drawn to scale, but not the sizes  
                        Sirius A is considerably larger than the Sun  
                        white dwarf Sirius B is about the size of the Earth  

 animation (scroll down)

 

Galaxies
        Spiral Galaxies
 presence of gas in the disk  
                stars still forming  
                low density galactic field  
                labeled Sa-d,m 
        Barred Spiral
developed bar in the interior region of the spiral arms  
             SBa-d,m 
 
        Elliptical
categories E0-7  
            depending on their degree of ellipticity  
            uniform luminosity  
            similar to the bulge in a spiral galaxy, with no disk  
            stars -old and - no gas  
          in the high density field,  
            at the centre of clusters. 
 

    Irregular
small galaxies 
        labeled Irr 
        no bulge 
        an ill-defined shape. 
        The Magellenic clouds