#Virtual moon atlas mac mac os x
Version for Windows and Mac OS X are also available.
#Virtual moon atlas mac drivers
OpenGL and graphic drivers supporting hardware acceleration Linux system i386 or x86-64 with 32bit libraries compatibility (ia32-libs) if you receive a message about cannot load libplan404.so try the following: if the program do not start, try from a console to look at the error messages look at your desktop menu if an icon is present under Education/Sciences run the command displayed at the end of the installation or just atlun vmapro_install.sh TexturesClementine.tgz take a note of the command given to run the program make the script executable: chmod +x vmapro_install.sh download the installer script vmapro_install.sh, the base package vmapro5.tgz and any additional package you want, for example TexturesClementine.tgz. create a symbolic link to libplan404.so in a folder already in /etc/ld.so.conf add the /usr/local/lib folder path to /etc/ld.so.conf run the full command given at the end of the installation, including the LD_LIBRARY_PATH section, change the icon to include this command. cd to the installation directory ( cd /usr/local ) other missing prerequesite, run ldd /usr/local/bin/atlun to get a full list of prerequesite for your system. I want a deb, rpm, mypreferedsystempackages. This is enough work for me to already make package for Linux, Mac and Windows for all this data. So I take the simplest, most portable solution for Linux to avoid to multiplicate them.īut you can build the packages yourself. tgz contain the classic bin, lib, share structure. This is easy to build any specific package you want from the extracted data.
#Virtual moon atlas mac 64 Bit
Why no 64 bit version ? no PPC version ?Īgain I want to avoid to multiplicate the packages I need to maintain. If you really need it (the program run fine in 32 bit compatibility) you can get the source codeĪnd the FreePascal/Lazarus compiler to build a native 64 bit version.This animation is an example of parallax. As the viewpoint moves side to side, the objects in the distance appear to move more slowly than the objects close to the camera. In this case, the white cube in front appears to move faster than the green cube in the middle of the far background. Parallax is a displacement or difference in the apparent position of an object viewed along two different lines of sight, and is measured by the angle or semi-angle of inclination between those two lines. Due to foreshortening, nearby objects show a larger parallax than farther objects when observed from different positions, so parallax can be used to determine distances. To measure large distances, such as the distance of a planet or a star from Earth, astronomers use the principle of parallax. Here, the term parallax is the semi-angle of inclination between two sight-lines to the star, as observed when Earth is on opposite sides of the Sun in its orbit. These distances form the lowest rung of what is called "the cosmic distance ladder", the first in a succession of methods by which astronomers determine the distances to celestial objects, serving as a basis for other distance measurements in astronomy forming the higher rungs of the ladder.
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