Spheres Of Eudoxus Model With Serial Key Version 1.0.1, 04 December 2009, Leonid Samkov -------------------------------------------------------------------- Spheres of Eudoxus Model is a Java application designed to illustrate the system created by the Ancient Greek astronomer Eudoxus to model the motion of the planets. The model consists of four nested concentric spheres. The axis of each sphere is attached to the surface of the next sphere out. The planet itself is located on the surface of the innermost sphere. The outermost sphere rotates with the daily (apparent) rotation of the stars. The Spheres Frame shows the four spheres of the model. The axis of the inner (red) sphere can be tilted relative to that of the middle (blue) sphere using a slider to adjust the angle. The red sphere automatically rotates with angular velocity +1.0 (in arbitrary units). The angular velocities of the blue and green spheres can be adjusted using sliders. Note that the axis of the blue sphere is attached to the equator of the green sphere. This is a crucial part of Eudoxus' model. The equator of the green sphere is in the plane of the ecliptic. The outermost (white) sphere is essentially the Celestial Sphere containing the fixed stars (or at least it rotates about the same axis and at the same rate as the Celestial Sphere). The Sky View Frame shows the motion of the planet (relative to the stars) as seen from the earth, which sits at the center of the concentric spheres in the model. By tilting the red sphere relative to the blue sphere, setting the angular velocity of the blue sphere opposite that of the red sphere, and giving the green sphere a sufficiently small angular speed, Eudoxus was able to qualitatively reproduce the observed retrograde motion of the planets using this model. spheres eudoxus model 1.0.2.jar, 08 March 2010, Adam Blome ------------------------------------------------------------------ Spheres of Eudoxus Model is a Java application designed to illustrate the system created by the Ancient Greek astronomer Eudoxus to model the motion of the planets. The model consists of four nested concentric spheres. The axis of each sphere is attached to the surface of the next sphere out. The planet itself is located on the surface of the innermost sphere. The outermost sphere rotates with the daily (apparent) rotation of the stars. The Spheres Frame shows Spheres Of Eudoxus Model Crack+ With Registration Code X64 Install the program and open the program by double-clicking on the file. The first window of the program displays the model. The second window shows the Celestial Sphere. The third window contains buttons to change and modify the model. The fourth window shows the sky for the date and time indicated by the button in the third window. To set the model and the desired date and time, set the date and time in the small window on the right. To set the angular velocities of the blue and green spheres, set the values in the corresponding sliders. To change the date, click on the calendar button in the third window. To change the date, click on the calendar icon at the top of the calendar popup. To set the time, click on the clock button at the top of the popup. To set the time, click on the clock icon at the top of the popup. To add/remove a planet from the model, click on the planets tab. To add/remove an earth-like body from the Celestial Sphere, click on the earth tab. To add/remove a moon from the Celestial Sphere, click on the moon tab. To add/remove a satellite from the Celestial Sphere, click on the satellite tab. To change the speed of the rotation of the innermost (red) sphere, click on the rotation tab. To change the angle of the axis of the innermost (red) sphere, click on the tilt tab. To change the date and time, click on the button at the bottom of the popup. To set the time zone, click on the time zone button at the bottom of the popup. To set the latitude and longitude of the Celestial Sphere, click on the lat lon tab. To change the rotational axis of the innermost (red) sphere, click on the rotation axis tab. To change the angle of the rotational axis of the innermost (red) sphere, click on the tilt axis tab. To change the direction of the rotation of the innermost (red) sphere, click on the direction tab. To change the direction of the rotation of the innermost (red) sphere, click on the tilt axis tab. To change the color of the innermost (red) sphere, click on the color tab. To change the scale of the innermost (red) sphere, click on the scale tab. To add/remove a background, click 77a5ca646e Spheres Of Eudoxus Model Crack+ License Code & Keygen The Spheres Model application demonstrates the use of the classic model for planet motion, created by Eudoxus (4th Century BCE). The system consists of four nested concentric spheres, the axis of each sphere being attached to the surface of the next sphere out. The planet is located on the surface of the innermost sphere. The outermost sphere rotates with the daily (apparent) rotation of the stars. Note that the axis of the inner sphere is parallel to the plane of the equator of the outer sphere. Thus, the red sphere is a polar sphere with a pole parallel to the equator of the blue sphere. The axis of the blue sphere is tilted relative to that of the green sphere. The angular velocity of the blue sphere is adjusted to opposite that of the red sphere by rotating the green sphere. Thus, the blue sphere is moving in the same direction as the equatorial plane of the green sphere. The green sphere rotates about a fixed point, the center of its sphere. The blue sphere and green sphere move in the same direction as the axis of the outermost sphere. The blue sphere rotates about a fixed point. The green sphere rotates about a fixed point. Note that the outermost sphere moves in the same direction as the axis of the blue sphere, and the blue sphere moves in the same direction as the axis of the green sphere. The application demonstrates the use of a simple model for planet motion, created by Eudoxus (4th Century BCE), to qualitatively reproduce the observed retrograde motion of the planets. Eudoxus' model consists of four nested concentric spheres. The axis of each sphere is attached to the surface of the next sphere out. The planet is located on the surface of the innermost sphere. The outermost sphere rotates with the daily (apparent) rotation of the stars. The Sky View Frame shows the motion of the planet (relative to the stars) as seen from the earth, which sits at the center of the concentric spheres in the model. The application consists of the four nested spheres of the model, the axis of each sphere being attached to the surface of the next sphere out. The planet is located on the surface of the innermost sphere. The outermost sphere rotates with the daily (apparent) rotation of the stars. The Spheres Model Files: The application consists of six application modules, each of which is a separate Java class. These classes implement functionality for the Sp What's New In Spheres Of Eudoxus Model? =========== Eudoxus' System of Spheres Model is a Java application designed to illustrate the system created by the Ancient Greek astronomer Eudoxus to model the motion of the planets. The model consists of four nested concentric spheres. The axis of each sphere is attached to the surface of the next sphere out. The planet itself is located on the surface of the innermost sphere. The outermost sphere rotates with the daily (apparent) rotation of the stars. The Spheres Frame shows the four spheres of the model. The axis of the inner (red) sphere can be tilted relative to that of the middle (blue) sphere using a slider to adjust the angle. The red sphere automatically rotates with angular velocity +1.0 (in arbitrary units). The angular velocities of the blue and green spheres can be adjusted using sliders. Note that the axis of the blue sphere is attached to the equator of the green sphere. This is a crucial part of Eudoxus' model. The equator of the green sphere is in the plane of the ecliptic. The outermost (white) sphere is essentially the Celestial Sphere containing the fixed stars (or at least it rotates about the same axis and at the same rate as the Celestial Sphere). The Sky View Frame shows the motion of the planet (relative to the stars) as seen from the earth, which sits at the center of the concentric spheres in the model. By tilting the red sphere relative to the blue sphere, setting the angular velocity of the blue sphere opposite that of the red sphere, and giving the green sphere a sufficiently small angular speed, Eudoxus was able to qualitatively reproduce the observed retrograde motion of the planets using this model. Usage: ====== 1. Start the application by clicking the "Spheres" button. 2. Click the "Spheres Frame" button to access the Spheres Frame. 3. Click the "Spheres" button to access the Spheres Frame again. 4. Set the angular velocity of the red sphere relative to the blue sphere. 5. Drag the green sphere to the desired angular velocity. 6. Run the application. 7. Click the "Sky View Frame" button to access the Sky View Frame. 8. Run the application. 9. If necessary, set the axes of the red sphere relative to the blue sphere using the sliders. 10. Run the application again. 11. Select the "Graphical" button. 12. Select the "Ticks" button. 13. Click the "Graphical" button again to stop the rotation of the red sphere. 14. Click the "Graphical" button to cancel the display of the Spheres Frame. 15. Click the "Spheres" button to return to the Spheres Frame. 16. Click the " System Requirements: Windows: - Windows 10 - 32-bit and 64-bit - Minimum: 1 GHz processor - 1 GB RAM - 500 MB free disk space - DirectX 9.0c compatible video card with 256 MB video RAM (8MB available for video memory to be used for OpenGL) Mac: - Mac OS X 10.7 or later
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