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Jovian Moons Applet
        
      
| The Galilean
                      moons are the four moons of Jupiter discovered by
                      Galileo Galilei in January 1610: Io, Europa,
                      Ganymede and Callisto. They revolve around Jupiter with periods of 1.77 to 16.69 days, and have apparent magnitudes between 4.6 and 5.6 when Jupiter is in opposition with the Sun, and are about one unit of magnitude dimmer when Jupiter is in conjunction.  | 
            
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                 Check your time zone offset and select the local standard time.  | 
            
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                 Click the applet first! 52.51° N, 13.41° E is Berlin, Germany.  | 
            
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                 You may use the keys "m", "d", "h", "n" to increase the month, date, hour, minute, or Shift key and "m", "d", "h", "n" to decrease the month, date, hour, minute !  | 
            
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              The sizes of
                  the moons are drawn according to their visual
                  magnitudes (accuracy about +/- 0.1 mag). The angular distances from Jupiter, and the angle from inferior conjunction are at right.  | 
            
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              With "Orbit"
                  selected from the "View" menu the illumination of
                  Jupiter can be shown. | 
            
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              The radii of
                  Jupiter and the orbital radii of the satellites are
                  drawn to scale. | 
            
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              Blue: Jupiter
                  visible in the local sky. | 
            
| The
                  simplified calculations used by the applet (according
                  to Jean Meeus: Astronomical Algorithms) is neglecting
                  the inclinations of the orbits of the satellites on
                  the equatorial plane of Jupiter (0.04° for Io, 0.51°
                  for Callisto): mutual occultations can not be
                  calculated with certainty. For 1610 the accuracy of times of inferior conjunctions of Callisto was tested by comparison with CalSky, and the deviations were found to be less than 2 minutes.  | 
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          Select "Diagram Moons" from the "View" menu:
        

        
Select
          "Ecliptic Plane" from the "View" menu:
        

        
The three
          inner moons—Io, Europa, and Ganymede—are in a 4:2:1 orbital
          resonance with each other.
          The Laplace resonance involving Io–Europa–Ganymede includes
          the following relation locking the orbital phase of the moons:
Select "Sky"
          from the "View" menu:
        Jupiter's
altitude
          and azimuth on the first of the month, 2 hours after sunset
      

      
      
Extreme
          visual magnitudes of the Galilean Moons:
        

        
        Extreme
          angular distances of the Galilean Moons from Jupiter (arc
          minutes):
        

        
Galilei's observations of
            1610 January at Padova (45.4° N, 11.9° E) were published in
            "Nuncius Sidereus"
            in Venice in March 1610.
        
The
year
          1610 can be selected from the "Year" menu:
        

Jan 07:
          Sunset 15:47 UT
        
  
          
          Credit:
              Linda Hall Library of Science, Engineering and Technology,
              [Page 17 [sic].]*
        
Simulation at 17:00 UT:

        
Jan 08:
          Callisto missing
        
          
          
        Credit:
Linda
Hall
Library
of
Science,
Engineering
                and Technology, [Page 18 [sic].]*
      
Simulation at 17:00 UT:

Jan 10:

                Credit: Linda Hall Library of Science, Engineering and
                Technology, [Page 18 [sic].]* 
          
        
          Simulation at 17:00 UT:
        

        
Jan 13:
          

          Credit:
Linda
Hall
Library
of
Science,
Engineering
                and Technology
      
Simulation at 17:00 UT:

        Sufficient
separation
          for Galilei's perspicillum to observe four moons.
        
Jupiter seen without moons:
        
2009 Sep 3, 5:30 UT:
          Io occulted/eclipsed,
          Europa and Ganymede in transit,
          Callisto in eclipse/transit.
          Next event: 2019 Nov 9
        

        
Jupiter seen with one satellite
            only:
          
This event is occurs far more frequently.
2010
Mar
          19 at 14:00 UT:
        

        
        Io transit, Europa occulted/eclipsed, Ganymede
          occulted.
      
2010
Oct
          27 at 15:00 UT:
        

        
Io
          occulted, Europa transit, Ganymede eclipse.
        
          Orbital Periods as published by Simon Marius in 1614
        
| Simon
              Marius | 
            Wikipedia | 
            Diff. | 
          ||
| (I)  Io | 
            1 d 18 h 28 min 30 s | 
            = 1.7698 d | 
            1.76914 d | 
             1 min 0.2 s = 0.04 % | 
          
| (II)   Europa | 
            3 d 13 h 18 min | 
            = 3.5542 d | 
            3.55118 d | 
             4 min 16 s = 0.08 % | 
          
| (III)   Ganymede | 
            7 d 3 h 56 min 34 s | 
            = 7.1643 d | 
            7.15455 d | 
            3 min 57 s = 0.14 % | 
          
| (IV)   Callisto | 
            16 d 18 h 9 min 15 s | 
            = 16.75642 d | 
            16.68902 d | 
            1 h 37 m = 0.40 % | 
          
          
        
| Books | 
| Simon Marius: Mundus Jovialis -
                  Die Welt des Jupiter - Die Entdeckung der Jupitermonde
                  durch den fränkischen Hofmathematiker und Astronimen
                  Simon Marius im Jahr 1609 - lateinisch und deutsch. Herausgegeben und bearbeitet von Joachim Schlör, Schrenk-Verlag, Gunzenhausen, 1988. ISBN 3-924270-14-7 Wolfschmidt, Gudrun (Hg.): Simon Marius, der fränkische Galilei, und die Entwicklung des astronomischen Weltbildes. Tredition, Hamburg 2012. ISBN 978-3847238645 Galileo Galilei: Sidereus Nuncius - Nachricht von neuen Sternen. Hg. Hans Blumenberg, Suhrkamp 1980. ISBN 978-3518279373  | 
            
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                 The Mundus Jovialis of Simon Marius: Jovian Satellite Fact Sheet (NASA) Jovian system simulator (high accuracy) Jupiter's Moon (simulation, Sky &
                      Telescope) Phenomena
                      of the Galilean Satellites of Jupiter (IMCE) Galilei: Nuncius Sidereus (Linda
Hall
                          Library of Science, Engineering and
                          Technology) From
Occhiale
                        to Printed Page: The Making of Galilei's Nuncius
                        Sidereus Jupiter satellite events and GRS
                          times for 2012-2013 Orbital
                        resonance (Wikipedia) Paita,
                        F. et al.: Element history of the Laplace
                        resonance: a dynamical approach Laplace,
                          P.-S.: Traite de Mecanique Celeste Vol. IV,
                          Paris 1805, chez Courcier.  | 
            
Last Modified: 2023, Oct 05
© 2010-2023 Juergen Giesen