Calc Objects for the ephemeris of the
object, expressed in keplerian (i.e., instantaneous two-body)
elements. Each Calc Object allows a choice of element type
(Osculating elements, Kozai-Izsak Mean elements, Brouwer-Lyddane
Mean elements using only short period terms, and Brouwer-Lyddane
Mean elements using both short and long period terms). The default
is osculating.
Name |
Dimension |
Type |
Description |
Time |
DateFormat |
Real Number |
Time. |
Altitude_Of_Apoapsis |
DistanceUnit |
Real Number |
The difference between the radius of apoapsis and
the central body's equatorial radius. The Calc Object allows a
choice of a central body. The default is Earth. |
Altitude_Of_Periapsis |
DistanceUnit |
Real Number |
The difference between the radius of apoapsis and
the central body's equatorial radius. The Calc Object allows a
choice of a central body. The default is Earth. |
Argument_of_Latitude |
AngleUnit |
Real Number |
The sum of the argument of periapsis and true
anomaly. The Calc Object allows a choice of coordinate systems. The
default is Earth Centered Inertial. |
Argument_of_Periapsis |
AngleUnit |
Real Number |
The angle from the ascending node to the periapsis
vector measured in the orbit plane in the direction of the object's
motion. The periapsis vector locates the closest point of the
orbit. For a circular orbit, the value is defined to be zero (i.e.,
periapsis at the ascending node). The Calc Object allows a choice
of coordinate systems. The default is Earth Centered Inertial. |
Eccentric_Anomaly |
AngleUnit |
Real Number |
Not defined for this class of object. |
Eccentricity |
Unitless |
Real Number |
A measure of the shape of the orbit. Values <1
indicate an ellipse (where zero is a circular orbit) and values
>1 indicate a hyperbola. |
Inclination |
AngleUnit |
Real Number |
The angle between the orbit plane and the XY plane
of the coordinate system. |
Longitude_Of_Ascending_Node |
AngleUnit |
Real Number |
A measure of the right ascension of the ascending
node, made in the Fixed frame. The value is the detic longitude of
the orbit's ascending node. The ascending node crossing is assumed
to be at, or prior to, the current position in the orbit in the
same nodal revolution. The Calc Object allows a choice of a central
body. The default is Earth. |
MeanAnomaly |
AngleUnit |
Real Number |
A measure of the time past periapsis passing,
expressed as an angle. The Calc Object allows a choice of a central
body. The default is Earth. |
Mean_Motion |
AngleRateUnit |
Real Number |
Not defined for this class of object. |
Orbit_Period |
TimeUnit |
Real Number |
Time required for a complete revolution as computed
from osculating semi-major axis length. The Calc Object allows a
choice of a central body. The default is Earth. |
RAAN |
AngleUnit |
Real Number |
Not defined for this class of object. |
Radius_Of_Apoapsis |
DistanceUnit |
Real Number |
The magnitude of the apoapsis vector. The apoapsis
vector (defined only when the eccentricity is <1) locates the
position in the orbit furthest from the central body. The Calc
Object allows a choice of a central body. The default is
Earth. |
Radius_Of_Periapsis |
DistanceUnit |
Real Number |
The magnitude of the periapsis vector. The
periapsis vector locates the position in the orbit closest to the
central body. The Calc Object allows a choice of a central body.
The default is Earth. |
Semimajor_Axis |
DistanceUnit |
Real Number |
Not defined for this class of object. |
Time_Past_Asc_Node |
TimeUnit |
Real Number |
The elapsed time since passing the last ascending
node crossing based on assumed two-body motion.. The Calc Object
allows a choice of coordinate systems. The default is Earth
Centered Inertial. |
Time_Past_Periapsis |
TimeUnit |
Real Number |
The elapsed time since passing the last periapsis
crossing based on assumed two-body motion.. The Calc Object allows
a choice of a central body. The default is Earth. |
True_Anomaly |
AngleUnit |
Real Number |
Not defined for this class of object. |