THE BIRTH OF TAAF
During the formation of the Volar System, protoplanets wandered all around Vol, it used to be a very extensive system, spanning over 30 astronomical units from Vol - but the orbital instability of the gas giants made them swing each other around the system. During these planetary migrations, other planets were ejected while also triggering a period of great collisions.
During this epoch, Paart were in co-orbital configuration with two other minor planets aside from dozens of large asteroids. These co-orbital planets were shepherded by Paart over the course of thousands of years, until they collided with each other very close to our main planet.
This offset impact, merged and broke the planets core apart into 3 major blobs of metal, and a million pieces of their mantles were sprayed away - the result was that the material started to orbit Paart at the right distances for a couple more hundred million years, giving the planet a temporary record-breaking number of moons. Taaf which was the densest of all, ejected the smaller one, and de-orbited the second largest moon - which was shortly ground to dust and meteorites by it's gravity.
The fallen moon, had great portions of iron, and it's mass has been incorporated in the planet's mantle and core ever since.
26,08 sextillion kg
(0,03x Earth's)
Mean Diameter
(0,319x Earth's)
5,1g/cm³
(0,92x Earth's)
2,90 m/s²
(0,296x Earth's)
70% metals ; 30% silicates
surface is covered in silicates and titanium/aluminum compounds
Paart's rotation rate in hours can be defined at any point by (4*PMA^0.182).
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