CoordinateSystem#
- class ansys.stk.core.stkutil.CoordinateSystem#
IntEnum
Overview#
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Represents coordinate system not supported by the Object Model. |
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Alignment at Epoch: an inertial system coincident with ECF at the Coord Epoch. Often used to specify launch trajectories. |
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B1950: X points toward the mean vernal equinox and Z points along the mean rotation axis of the Earth at the beginning of the Besselian year 1950 and corresponds to 31 December 1949 22:09:07.2 or JD 2433282.423. |
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Fixed: X is fixed at 0 deg longitude, Y is fixed at 90 deg longitude, and Z is directed toward the north pole. |
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J2000: X points toward the mean vernal equinox and Z points along the mean rotation axis of the Earth on 1 Jan 2000 at 12:00:00.00 TDB, which corresponds to JD 2451545.0 TDB. |
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Mean of Date: X points toward the mean vernal equinox and Z points along the mean rotation axis of the Earth at the Orbit Epoch. |
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Mean of Epoch: X points toward the mean vernal equinox and Z points along the mean rotation axis of the Earth at the Coord Epoch. |
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TEME of Date: X points toward the mean vernal equinox and Z points along the true rotation axis of the Earth at the Orbit Epoch. |
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TEME of Epoch: X points toward the mean vernal equinox and Z points along the true rotation axis of the Earth at the Coord Epoch. |
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True of Date: X points toward the true vernal equinox and Z points along the true rotation axis of the Earth at the Orbit Epoch. |
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True of Epoch: X points toward the true vernal equinox and Z points along the true rotation axis of the Earth at the Coord Epoch. |
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True of Ref Date: A special case of True of Epoch. Instead of the Coord Epoch, this system uses a Reference Date defined in the Integration Control page of the scenarioβs PODS properties. |
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ICRF: International Celestial Reference Frame. |
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Mean Earth. |
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uses an analytic formula not modeling lunar libration. |
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Fixed_IAU2003. |
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PrincipalAxes_421. |
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PrincipalAxes_403. |
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Inertial. |
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The mean ecliptic system evaluated at the J2000 epoch. The mean ecliptic plane is defined as the rotation of the J2000 XY plane about the J2000 X axis by the mean obliquity defined using FK5 IAU76 theory. |
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The true ecliptic system, evaluated at each given time. The true ecliptic plane is defined as the rotation of the J2000 XY plane about the J2000 X axis by the true obliquity defined using FK5 IAU76 theory. |
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PrincipalAxes_430. |
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TrueOfDateRotating: Like the Fixed system, but ignores pole wander. The XY plane is the same as the XY plane of the TrueOfDate system, and the system rotates about the TrueOfDate Z-axis. |
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EclipticJ2000ICRF: An ecliptic system that is a fixed offset of the ICRF system, found by rotating the ICRF system about its X-axis by the mean obliquity at the J2000 epoch (i.e., 84381.448 arcSecs). The ecliptic plane is the XY-plane of this system. |
Import detail#
from ansys.stk.core.stkutil import CoordinateSystem