Atmospheric re-entry, even when initiated from a circular low-Earth or
bit, requires heavy heat shields, ablative materials or radiative diss
ipation techniques. Semi-analytical and numerical simulations of the a
tmospheric re-entry from low-Earth orbits of a capsule with a 20-km, a
ttached, heat resistant tether have shown that the thermal input flux
on the capsule is reduced by more than one order of magnitude with res
pect to a comparable re-entry without tether. Long tethers have low ba
llistic coefficients and a large surface for heat dissipation. Moreove
r, a long tether is stabilized by gravity gradient and consequently te
nds to maintain a high angle of attack with respect to the wind veloci
ty. The exposed surface of a 20-km-long l-mm diameter tether is 20 m(2
), which is much larger than the cross section of a re-entry capsule.
The resulting strong drag decelerates the capsule during re-entry like
a conceivable hypersonic parachute would do. This paper describes the
methods and results of the simulation of the SEDS endmass re-entry wi
th different tethers.