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Rosette Seven Primary Ephemeris
Thursday, April 2nd 2009

This is the standard ephemeris for Rosette Seven system. The starting epoch date is January 1th, 3000. All seven planets orbit the primary star 0.5 AU from it.

The purpose of this ephemeris is to test the stability of a Klemperer Rosette with seven orbiting bodies.

The initial orbital velocity of all orbiting objects are calculated by assuming circular orbit on initial distance for case only the star and said orbiting object exist.

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Rosette Seven
Monday, January 4th 2010

Sistem planet fiktif ini dibuat untuk mensimulasikan dinamika benda langit di dalam sebuah Klemperer Rosette dengan 7 objek mengorbit sebuah objek sentral (bintang).

Bintang primer sistem planet ini adalah Rosette Tujuh yang memiliki massa 0.421 massa Matahari. Semua planet-planet di dalamnya Iritalia, Varthona, Uelahala, Vertinakaze, Varidmela, Palzeakazo dan Urevinhuaga memiliki massa 3.532 Massa Bumi. Semua gambar untuk planet-planet ini dibuat dengan menggunakan aplikasi Pembuat Planet Instan dari www.eldritch.org.

Orbit dari setiap planet bervariasi menurut ephemeris masing-masing.

Objects: All Objects, Rosette Seven ( Star ), Iritalia ( Planet ), Varthona ( Planet ), Uelahala ( Planet ), Vertinakaze ( Planet ), Varidmela ( Planet ), Palzeakazo ( Planet ), Urevinhuaga ( Planet )
Ephemeris:View All Ephemeris
Rosette Seven Primary Ephemeris - Wednesday, January 1st 3000
Rosette Seven modification Six-One - Wednesday, January 1st 3000
Keywords:klemperer rosette, sistem planet experimental
Status:This System is Non-Public - Non-Public Systems are subject to owner change and deletion. If you make an ephemeris or describe an object or ephemeris within a Non-Public system, they will also be deleted if the System Owner delete the system.