Great Red Spot position when offset is given
Affects | Status | Importance | Assigned to | Milestone | |
---|---|---|---|---|---|
Stellarium |
Fix Released
|
Low
|
Alexander Wolf |
Bug Description
I am somewhat puzzled by line 718 of Planet.cpp and am wondering whether the call to qAbs is correct.
This is the routine for "drifting" the position of the Great Red Spot when an offset has been provided by the user.
The drift, apparently in degrees, seems to be 0.2483 * qAbs(JD - 2456172)
If I have understood it correctly, this seems to assert that the drift reversed direction in 2012. Other sources show a steady drift.
Also, I'm wondering about the coefficient 0.2483. The actual drift of the GRS is only about 0.04 degree per day relative to System II. The rest of the coefficient might come from the difference between System II (used for GRS measurements) and System III (used for the rotation period in ssystem.ini), but even then I'm not sure I understand its value.
tags: | added: solar-system |
Changed in stellarium: | |
status: | Fix Committed → Fix Released |
This is a legacy code to compensate for the drift of the GRS. I think we can use the approach of CdC planetarium and introduce explicit configurable options for the GRS as a special case.
P.S. Stellarium uses an inner coordinate system for all planets.