Thank you very much in advantage for your recent created asteroid belt scripts for Epsilon Eridani's two asteroid belts.
Source of the post
I have made two asteroid belts for 'Eps Eri'.
But I do not know which 'Inclination' they must have. I gave them the same Inclination as the planet 'AEgir', but the orbit of the planet cuts the path of one belt. This seems me unlikely.
You are very correct in assuming that the orbital inclination of planet 'AEgir' is as same as that of the main asteroid belts. Hubble Space Telescope finds that orbit of AEgir at Epsilon Eridani is at same tilt as the star's circumstellar disk, 25 degrees- even though no inclination data was given in Wikipedia's Epsilon Eridani planetary system table.
In fact, the website of en.wikipedia.org/wiki/Epsilon_Eridani says about controversy nature of AEgir's orbital parameters:
"The frequently cited value of 0.7 for Epsilon Eridani b's eccentricity is inconsistent with the presence of the proposed asteroid belt at a distance of 3 A.U. If the eccentricity was actually this high, the planet would pass through the asteroid belt (A) and clear it out within about ten thousand years. If the belt has existed longer than this period, which appears likely, it imposes an upper limit on Epsilon Eridani b's eccentricity of about 0.10-0.15."
Moreover, the website of http://www.solstation.com/stars/eps-erid.htm
says more about this subject:
"Although some researchers previously suggested that 'Epsilon Eridani b' moves in an exaggerated ellipse ranging between 1 and 5 Astronomical Units around its host star, such an orbit could cross and quickly disrupt and 'clear out' the newly discovered innermost asteroid belt; hence, the Spitzer team of astronomers argues that planet b must have relatively circular orbit that keeps it just outside the inner asteroid belt, such as the eccentricity of e=0.25 +/-0.23 reported by Botieu et al in 2006."
Best solution for this problem is to change AEgir's orbital parameters and conform it with the inner asteroid belt.
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