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The bigger fluctuations 295 m/s is an artefact of numercial approximation of the orbit.
I'm mot sure about 63 m/s, but NASA uses this ephemerides (like MAR097) in real missions, so it's definitely closer to the real orbit. But it's hard to say how accurate it is in this case.
Yes, apparently...
I've compared the default Phobos ephemeris module with SPICE module in Orbiter.
Yes, the default Phobos module has bigger amplitude and speed of apoapsis fluctuations.
With SPICE and mar097.bsp kernel it's 1.03 s (~63 m/s), not 1.14 s.
x - GMAT’s Modified Julian Date (it's one day - 2021-12-01)
y - AOP (argument of periapsis in degrees)
But I still can't get 295 m/s. Looks like AOP of Phobos is wobbling with speed 0-70 m/s.
Apoapsis and periapsis of Phobos are not stable and wobbling around some point.
There is a graph from GMAT (orbit of Phobos here is based on MAR097 ephemeris file):
Interesting. Using D3D9Client with DXVK ( https://github.com/doitsujin/dxvk ) I get ~20% more fps on Windows 10 than without DXVK.
There are some glitches though.
It will be difficult to use TransX with GMAT. TransX uses conic sections but this approach doesn't work well with GMAT.
Few years ago I added GMAT support to Keithth G's trajectory optimization python script here https://www.orbiter-forum.com/threads/pykep-to-transx-conversion.33685/ and...
I can only do this using GMAT and transfer position/velocity to Orbiter.
Yes, but you can tune GMAT propagator parameters close enough to the Orbiter propagator. So it gives good results for Orbiter too.
Try this, for example:
BEGIN_ENVIRONMENT
System Sol
Date MJD 60886.5011574074...
Incoming and outgoing trajectories generally are the same. In most cases your have to use tons of extra fuel to get into/from an interplanetary trajectory from/into an equatorial (or any arbitrary) LEO.
I doubt that an ideal LEO for the transfer station exists.
Your can aproach/departure a...
boogabooga
You can use https://ssd.jpl.nasa.gov/horizons.cgi to get accurate position/velocity of many objects.
For example 163348 (2002 NN4):
Current Settings
Ephemeris Type [change] : VECTORS
Target Body [change] : 163348 (2002 NN4)
Coordinate Origin [change] : Geocentric [500]
Time...
In Orbiter? There is an example from ScnEditor plugin:
oapiGetRelativePos (hV, hRef, &pos);
oapiGetRelativeVel (hV, hRef, &vel);
// map ecliptic -> equatorial frame
if (frm) {
MATRIX3 rot;
if (frm == 1) oapiGetPlanetObliquityMatrix (hRef, &rot);
else oapiGetRotationMatrix...
Really? Sounds like there is a bug in GMAT. It doesn't matter, though. I suspect radiation pressure and atmospheric models in Orbiter and GMAT are very different to include these details into import/export.
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