BSTAR

BSTAR is a way of modeling aerodynamic drag on a satellite in the simplified general perturbation model 4 satellite orbit propagation model.

Traditionally, aerodynamic resistance ("drag") is given by

FD=12ρCdAv2

where ρ is the air density, Cd is the drag coefficient, A is the frontal area, and v is the velocity.

The acceleration due to drag is then

aD=FDm=ρCdAv22m

In aerodynamic theory, the factor

B=CdAm

is the inverse of the ballistic coefficient, and its unit is area per mass. Further incorporating a reference air density and the factor of two in the denominator, we get the starred ballistic coefficient:

B∗=ρ0B2=ρ0CdA2m

thus reducing the expression for the acceleration due to drag to

aD=ρρ0B∗v2

As it can be seen, B∗ has a unit of inverse length. For orbit propagation purposes, there is a field for BSTAR drag in two-line element set (TLE) files, where it is to be given in units of inverse Earth radii. The corresponding reference air density is given as 0.15696615 kg/(m2⋅REarth). One must be very careful when using the value of B∗ released in the TLEs, as it is fitted to work on the SGP4 orbit propagation framework and, as a consequence, may even be negative as an effect of unmodelled forces on the orbital determination process.

References

  1. ↑ "BSTAR Drag Term". Retrieved November 8, 2022.
  2. ↑ Kelso, T.S. "Frequently Asked Questions: Two-Line Element Set Format". Retrieved November 8, 2022.
  3. ↑ Hoots, Felix R.; Roehrich, Ronald L. (December 1980). SPACETRACK Report No. 3 Models for Propagation of NORAD Element Sets (PDF) (Report). Retrieved November 8, 2022.
  4. ↑ Vallado, David A., and Paul J. Cefola. "Two-line element sets-Practice and use." 63rd International Astronautical Congress, Naples, Italy. 2012.