DESIGNATE @int(1001:10099) CENTER @body REFERENCE PLANETOCENTRIC (2:3){ LATITUDE @number | LONGITUDE @number | @options | RADIUS @number } (0:3){ FROM @calendar | TO @calendar | EPOCH @calendar }
DESIGNATE @int(1001:10099) CENTER @body REFERENCE PLANETOCENTRIC (2:3){ LATITUDE (1:2)@number | LONGITUDE (1:2)@number | @options | RADIUS (1:2)@number } EPOCH @calendar (0:2){ FROM @calendar | TO @calendar }
When creating a designated object in this system, you must specify the
latitude and longitude of the object. The radius is optional, and defaults to
the largest semi-major axis of the tri-axial ellipsoid used to model the
body.
In planetocentric coordinates, the z-axis points toward the north pole of the
reference body. The x-axis is defined by the intersection of the equator and
prime meridian of the body. The origin is at the center of the body.
Let P be a point in space, and let V be the position vector from the origin of the planetocentric frame to P.
The planetocentric latitude of P is the angle between the equator and V. North latitudes are positive, south latitudes are negative.
The planetocentric longitude of P is the angle between the x-axis and the projection of V onto the x-y plane, positive from x toward y.
The planetocentric radius of P is the distance from the center of the reference body to P (the magnitude of V).
; ; Define a name for the designated object (the Great Dark Spot ; on Neptune). ; DEFINE 1001 NEPTUNE_SPOT; ; ; Provide the location of the spot. Note that the longitude ; changes with time. ; DESIGNATE NEPTUNE_SPOT CENTER NEPTUNE REFERENCE PLANETOCENTRIC LATITUDE -25 DEGREES; LONGITUDE 175 DEGREES -2 DEGREES/HOUR RADIUS 24270 KM EPOCH 23 MAY 1991 10:11:05; ; ; Find intervals when the spot is in transit across Neptune ; (that is, when it is visible from Earth). ; FIND VISIBLE TRANSIT OF NEPTUNE_SPOT ACROSS NEPTUNE FROM EARTH;