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Mars Snooper

Missiles and Rockets, Jan 26, 1959

Image credit: ARMA

Image source: Internet Archive

Orion Vehicles 2/2

Lunar Ferry Vehicles

Fig. 3.13 — Exploration vehicle configuration for Jupiter moon landing mission, 20-m propulsion module

Fig. 3.15 — Various payload configurations on basic 20-m propulsion module (with departure weights for given missions)

Fig. 3.16 — Earth-orbit-to-lunar-orbit ferry vehicle

Fig. 3.18 — Lunar-ferry-vehicle command module

Fig. 3.19 — Reference-design passenger module

Fig. 3.20 — Earth-orbit-to-lunar-surface ferry vehicle

Fig. 3.21 — Lunar passenger ferry

Fig. 3.22 — Lunar cargo shuttle

Fig. 3.23 — Solid-propellant-boosted earth-launched lunar logistic vehicles

Lunar Logistics Vehicles

Fig. 3.24 — S-IC boosted earth launched lunar logistics vehicle

Fig. 3.15 — Orbit launched lunar logistics vehicle

source

From:

Nuclear Pulse Space Vehicle Study

Vol. III — Conceptual Vehicle Designs and Operational Systems (U)

Orion at Atomic Rockets

Image credit: General Atomics

File Source: Cornell

Orion Vehicles 1/2

Personnel Accommodations

Fig. 3.2 — Factors that influence the location of the shielded powered flight station

Fig. 3.4 — Powered flight station-escape vehicle for 8-man exploration missions with 10-m configurations

Fig. 3.5 — Powered flight station-escape vehicle for 20-man exploration missions with 20-m configurations

Fig 3.6 — Exploration-mission personnel accommodations for an 8-man complement

Fig 3.7 — Exploration-mission personnel accommodations for a 20-man complement

Fig 3.8 — General arrangement of payload spine and magazine payload support columns

Planetary Exploration Vehicles

Fig. 3.11 — Exploration vehicle for Mars orbital capture mission using 10-m propulsion module

Fig. 3.12 — Various payload configurations on basic 10-m propulsion module (with departure weights for 72, 850 fps Mars mission)

source

From:

Nuclear Pulse Space Vehicle Study

Vol. III — Conceptual Vehicle Designs and Operational Systems (U)

Orion at Atomic Rockets

Image credit: General Atomics

File Source: Cornell

Figure 2.

Unmanned probe approaching Pluto. Probe is powered by thermionic radioisotope power generator. The laser beams for surface illumination, with optical sensors slaved to the beams. Other equipment comprises radiation counters as well as field, plasma and particle sensors.

Image credit: Krafft Ehricke Papers

Image source: NASM

Figure 7.

Earth-moon based planetary space port in 1988. Spacecraft are nuclear propelled interplanetary vehicles, launched by solid propellant lift-off rockets side-mounted around center section which, like the cylinders at the spacecraft’s center section, contain nuclear pulse units. In background a large antenna, belonging to the lunar deep space network is visible.

Image credit: Krafft Ehricke Papers

Image source: NASM

Solar Transportation

I find writing excruciating, which is why I usually let the Astronautix guy or Winchell Chung do the talking. Neither were available this morning, so context for the next couple of posts is by yours truly. Apologies in advance.

Solar Transportation was a presentation given by Krafft Ehrikke at the American Astronautical Society in 1966. In essence, the lecture describes how our solar system might be navigated in the year 2000. As reprinted in the book by Marsha Freeman, it’s a surprisingly enjoyable read.

The summary includes a wish list of propulsion systems to be developed.

Late 70s and most of the 80s

  • Solid core nuclear reactors, especially NERVA

Late 80s and 90s

  • Nuclear pulse (NP) (non-steady nuclear fission and fusion drive)
  • Controlled thermonuclear reactor (CTR) (steady nuclear fusion drive) or, if neither one of these developments is undertaken,
  • Nuclear-electrostatic drive.

Ehrikke then presents a timetable, representing a “sensible and likely” evolution of manned helionautical missions.

1970s

  • An orbital operations capability would be developed, facilitating cislunar and heliocentric excursion missions. 

1980s

  • In 1982, a 69 day Mars capture mission launches. The crew conducts intensive reconnaissance both from orbit, and using probes – including landers and returners – but no manned surface excursions are planned. A mission launched between 1984 is one-way, involving a 529 day stay on Mars. A follow-on mission in 1985 (via Venus) retrieves the crew.
  • By the end of the ’80s, a capability is established for a Venus landing. A solar physics laboratory is erected on Mercury. These missions are based on the NP and CTR drives.

I990s

  • Regular transfers begin between Earth and Mars.
  • Exploration of Jupiter and Saturn and their moons.
  • Manned missions to asteroids and comets.
  • Beginning of utilization of the raw material resources of asteroids and planets of the inner solar system.

Solar Transportation then goes back the future and the fall of the year 2000, looking back at the events that led to the interplanetary travel we enjoy at the dawn of the new millennium. The interplanetary corridors  between Mercury and Saturn are alive with manned vehicles. Unmanned probes have reached the Sun. Food is grown on Mars and it is expected that exports to Earth will begin within fifty years. An orbital supply and rescue station is established at Venus, acting as a helionautical coast guard station. But like I said already, go and read it yourself.

Image credit: Krafft Ehricke Papers

Image source: NASM

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Fusion Designs at Atomic Rockets

Image credit: Krafft Ehricke Papers

Image source: NASM

Explorer Party Lands on Jupiter VII

Fusion Designs at Atomic Rockets

Image credit: Krafft Ehricke Papers

Image source: NASM

Over Midnight Point of Mercury

Fusion Designs at Atomic Rockets

Image credit: Krafft Ehricke Papers

Image source: NASM