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Box 50

 Container

Contains 5 Results:

Sun (+ 4 inner planets)'s attractions on Jupiter with first difference, 1914 - 1960

 File — Box: 50
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: 1914 - 1960

Coordinates of Venus, Earth, Jupiter, and Saturn, n.d.

 File — Box: 50
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: n.d.

Herrick's Fable Book 2, n.d.

 File — Box: 50
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: n.d.

Rectilinear Calculations, n.d.

 File — Box: 50
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: n.d.

Betulia Computer Runs, 1969

 File — Box: 50
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: 1969