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I conducted more test with different orders/degrees, inclinations, altitudes. Didn't find problems. Simulates definitely much closer to GMAT than with default Orbiters' model based on JCoeffs. For example, a polar orbit with EGM96:
And the default model:
An Impressive difference.
I wasn't able to find file with spherical harmonic coefficients in correct format for Earth, so I made one from egm96_to360.ascii (EGM96 360x360 model) that is available on the Internet. The file is in the attachment.
Did a comparison with GMAT. Fits perfectly:
It was "tacc 1000" with 10 Hz in FlightData settings. Without graphics engines it gives relatively small steps < 1s and I didn't expect any problems.
Looks like the step increased due to unknown reasons and that affected precision (just huge step itself or with Orbit Stabilization).
I test both...
It should be recording FlightData.log every ~100 simulated seconds and there were two gaps:
...
121789.83 170.3096
121890.15 170.1104
122111.46 169.8282
122211.78 169.7923
...
128134.28 169.9225
128234.44 169.5184
128771.03 168.9129
128879.17 169.1444
...
which seemingly...
Excellent job!
I did some test and compared the new improved gravity model in OpenOrbiter with GMAT's models (even made a script for converting *.tab files to GMAT's *.cof files).
Orbiter and GMAT are very close now.
An orbit around Mars for example:
But once, only once, I got a strange...
Look here:
https://orbiter-forum.com/threads/improved-tesseral-gravity-model.40266/post-602936
Kernels\orbiter.mrg is the config file for spkmerge tool (from SPICE toolkit) that creates *.bsp form other *.bsp.
Original kernels are here:
https://naif.jpl.nasa.gov/pub/naif/generic_kernels/spk/
Orbiter now has an API for implementing any ephemerides. It's just a matter of packaging and perhaps revising some existing plugins, such as the SPICE module.
However, an API for utilizing better rotation models still needs to be implemented in the OpenOrbiter core, preferably as an extension of...
You need to use the minor view for the eject function and the maneuver has to minimize R.Inc and DeltaV:
https://orbitermars.co.uk/txmanfneject2.htm
It may or may not be the prograde burn relative to Earth. Depends on your parking orbit and your current position on the orbit.
I would also recommend SPICE module:
https://www.orbiter-forum.com/threads/spice-module.1108/
I've uploaded the latest ready-to-use build with all configs and SPICE kernels here:
https://mega.nz/file/Vmxh2YyQ#IvMlr1d1NvgnE8im4Bk4oFvdlgUlEaZ9Z8N7HJidutg
For x64 version of Orbiter you need to...
I don't think so. The difference in the moon's orientation for MJD 52006 between GMAT's (MOON_PA) and Orbiter ~0.001 rad.
Have you compared results with GMAT\data\gravity\luna\grgm900c.cof model?
Yes, for example if you try to get elliptical osculating elements for Earth for an arbitrary date from Horizons System ( https://ssd.jpl.nasa.gov/horizons/app.html#/ ) using J2000 reference frame you get almost random LAN between 0 and 360 deg. :)
Yes, I can confirm, there are course corrections before Nov 14-15, but after that it's ballistics.
I was even able to find some parameters for solar radiation pressure model to get almost the same POS/VEL after propagating Nov 15 - Dec 14:
HORIZONS (Moon body center, Ecliptic of J2000.0 )...
Yes, I used GMAT.
And yes, according to GMAT as well as Orbiter CAPSTONE with this POS/VEL from HORIZONS escapes Moon just soon after 14 Dec. Moreover, it looks like it's already way off NRHO, so I think there should be corrections before this date (and after 14 Nov) which were not included in...
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