The possibility of having a high-inclination out-of-the-ecliptic probe complemented by a second probe going from Jupiter to the sun along a rectilinear path (at least for the segment from 0.3 a.u. inward to the sun) is theoretically examined. Orbit calculations of spacecraft trajectories are included.
An alternative option to the dual-probe out-of-ecliptic mission via Jupiter swingby
01.03.1976
Aufsatz (Konferenz)
Keine Angabe
Englisch
Jupiter swingby missions to the outer planets.
AIAA | 1966
|Jupiter swingby missions to the outer planets.
NTRS | 1966
|Jupiter swingby missions to the outer planets
AIAA | 1966
|Trajectories to the outer planets via Jupiter swingby
NTRS | 1968
|