Planetary Ephemeris
Implement position and velocity of astronomical objects
- Library:
Aerospace Blockset / Environment / Celestial Phenomena
Description
The Planetary Ephemeris block uses Chebyshev coefficients to implement the position and velocity of the target object relative to the specified center object for a given Julian date. The Target parameter specifies an astronomical object. The block implements the ephemerides using the Center parameter for an astronomical object as the reference.
The block uses the Chebyshev coefficients that the NASA Jet Propulsion Laboratory provides.
Tip
For TJD
, Julian date input for the block:
Calculate the date using the Julian Date Conversion block or the Aerospace Toolbox
juliandate
function.Calculate the Julian date using some other means and input it using the Constant block.
This block implements the position and velocity using the International Celestial Reference Frame. If you require the planetary ephemeris position value relative to Earth in Earth-fixed (ECEF) coordinates, use the Direction Cosine Matrix ECI to ECEF block.
Ports
Input
Output
Parameters
References
[1] Folkner, W. M., J. G. Williams, D. H. Boggs. "The Planetary and Lunar Ephemeris DE 421." IPN Progress Report 42-178, 2009.
[2] Ma, C. et al. "The International Celestial Reference Frame as Realized by Very Long Baseline Interferometry." Astronomical Journal, Vol. 116, 516–546, 1998.
[3] Vallado, D. A. Fundamentals of Astrodynamics and Applications, New York: McGraw-Hill, 1997.
Extended Capabilities
Version History
Introduced in R2013a