Satellite: Astrogator Values: Keplerian Elems
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. |