15 October 2016

"A Continuing Aspect of Human Endeavor": Bellcomm's January 1968 Lunar Exploration Program

Lunar Exploration Program candidate landing sites. Of these, the Apollo Program would reach only Fra Mauro; Apollo astronauts would, however, visit five other sites not labeled here. Please click on image to enlarge. Image credit: NASA/Arizona State University/DSFPortree
Bellcomm, Inc., based near NASA Headquarters in Washington, DC, was carved out of Bell Labs in 1962 to provide technical advice to NASA's Apollo Program Director. NASA rapidly expanded Bellcomm's bailiwick to take in nearly all NASA Office of Manned Space Flight planning.

In a January 1968 report, Bellcomm planners N. Hinners, D. James, and F. Schmidt proposed a lunar mission series designed to bridge a gap in NASA plans they believed existed between the first piloted "Early Apollo" moon flights and sophisticated Apollo Applications Program (AAP) lunar expeditions. They declared that their Lunar Exploration Program was "based upon a reasonable set of assumptions regarding hardware capability and evolution, an increase in scientific endeavor, launch rates, budgetary constraints, operational learning, lead times, and interaction with other space programs," as well as "the assumption that lunar exploration will be a continuing aspect of human endeavor."

Hinners, James, and Schmidt envisioned a series of 14 lunar missions in four phases. Phase 1 would span the period from 1969 through 1971. The five Phase 1 missions were approximately equivalent to the Early Apollos. They would launch at least six months apart to give engineers and scientists adequate time to learn from each mission's successes and failures and enable them to apply their new knowledge to subsequent missions. Phase 1 would begin with Lunar Landing Mission (LLM)-1, the historic first Apollo moon landing.

The LLM-1 Lunar Module (LM) would alight on one of the moon's flat, relatively smooth basaltic plains. Called since the 17th century "maria" (Latin for "seas" - the singular is "mare"), they appear as mottled gray areas on the moon's white face. They cover about 20% of the moon's Earth-facing Nearside hemisphere, but are scarce on the hemisphere the moon turns always away from Earth (its Farside). LLM-1 and the other Phase 1 missions would each have several back-up near-equatorial Nearside mare landing sites, enabling them to land in safe places regardless of how their planned launch dates might slip.

Almost any mare would do for LLM-1, Hinners, James, and Schmidt argued, because the first piloted landing mission would emphasize engineering, not science. LLM-1 would test the LM, lunar space suits, and other Apollo systems ahead of more ambitious Phase 1 missions. If all went as planned, the LLM-1 crew would stay on the moon for 22 hours and carry out two short moonwalks.

LLM-1 would follow a "free-return" flight path that would guarantee that the Apollo Command and Service Module (CSM) could loop around the moon and return to Earth without propulsion in the event that its Service Propulsion System (SPS) main engine failed en route to the moon. The SPS was meant to adjust the CSM/LM combination's course during flight to and from the moon, slow the CSM and LM so that the moon's gravity could capture them into lunar orbit, and boost the CSM out of lunar orbit to return to Earth. The Bellcomm planners noted that use of the free-return trajectory would greatly limit the percentage of the moon's surface a lunar mission could reach.

The LMs constructed for Phase 1 missions would each be capable of delivering two astronauts. their space suits, and up to 300 pounds of payload to the lunar surface. This would include geologic tools for collecting up to 50 pounds of lunar rock and dust samples for return to Earth. Missions LLM-2 through LLM-5 would, in addition, each include an Apollo Lunar Scientific Experiment Package (ALSEP) – a cluster of geophysical experiments – for deployment on the moon. The ALSEPs would monitor the moon and return data after the astronauts returned to Earth.

LLM-2 through LLM-5 would see astronauts perform geological traverses on foot to spots up to several kilometers from the LM. Meanwhile, the CSM Pilot, alone in lunar orbit, would photograph the moon's surface through the CSM's small windows.

LLM-2, like LLM-1, would follow a free-return trajectory and remain for 22 hours at a mare landing site. It would, however, add a third moonwalk.

LLM-3 would abandon the free-return trajectory so that it could reach a fresh crater on a mare. The crater, the Bellcomm planners explained, would serve as a natural "drill hole." Studies of both natural and human-made craters on Earth had shown that the LLM-3 astronauts would find the oldest rocks – those excavated from deepest beneath the surface – on the crater's rim. The astronauts would explore the lunar surface for longer than 22 hours but less than 36 hours.

LLM-4 would be similar to LLM-3, but would be targeted to land at one of the many widely scattered mare "wrinkle ridges." In 1968, some scientists (notably, Nobel Laureate Harold Urey) still attributed these sinuous raised features to salty water escaping from reservoirs beneath the moon's surface, but today we know that they formed when lava that filled the mare nearly 4 billion years ago buckled as it cooled. Some may link or follow traces of ancient landscape drowned when the lava welled up from within the moon.

LLM-5, the final Phase 1 flight, would see an LM land at a mare site bordering a Highlands region. The Highlands of the moon, the light-colored areas on the moon's disk, are ancient cratered terrain. The LLM-5 astronauts would squeeze four moonwalks into their 36-hour mission.

The Bellcomm planners' four Lunar Exploration Program Phase 2 missions would commence about two years after LLM-5 and span 1972-1973. Upgrades to Apollo hardware and operations in Phase 2 would permit in-depth exploration of specific unique landing sites selected primarily for scientific interest. Among the upgrades that Hinners, James, and Schmidt proposed was variable Earth-to-moon flight time or time spent in lunar orbit prior to landing. This operational flexibility was intended to permit an Extended LM (ELM) spacecraft to reach its pre-planned target site even if launch from Earth were delayed for several days.

The Phase 2 lunar-surface astronauts would perform six moonwalks at each landing site. The ELM would land 1300 pounds of payload. Phase 2 CSMs would carry prototype remote sensors to test their feasibility ahead of their operational use in Phases 3 and 4.

The first Phase 2 mission, LLM-6, would see an ELM spend three days at Tobias Mayer in the extensive Oceanus Procellarum ("Ocean of Storms") mare region. Its crew would deploy an ALSEP and explore on foot a sinuous rille (canyon), a dome (possible volcano), and a fresh crater with a surrounding dark halo (possible volcanic vent). LLM-7 would be similar to LLM-6, but would land at a linear rille site designated I-P1.

LLM-8 would see the introduction of the Lunar Flying Unit (LFU), a one-person rocket flyer. Bellcomm targeted LLM-8 to the Flamsteed Ring, an ancient crater mostly submerged by lava during the formation of Oceanus Procellarum. At the time Hinners, James, and Schmidt selected it, the Flamsteed Ring was suspected of being an extrusive volcanic feature called a "ring dike."

LLM-9, similar to LLM-8, would visit Fra Mauro, a site known for its domes and rilles, which geologists interpreted as signs of recent volcanism. Fra Mauro would later come to be seen (correctly) as a large geologic unit made up of ejecta from the enormous impact that blasted out Mare Imbrium, the right "eye" of the "Man in the Moon." Cone crater, a natural drill hole in the Fra Mauro Formation, would become the target of Apollo 13 (and, after that mission failed to land on the moon, Apollo 14).

Phase 3 of Bellcomm's Lunar Exploration Program would comprise a single lunar-orbital survey mission in 1974. Because it would include no lunar landing, it received no LLM number. The mission would, for all practical purposes, mark the start of advanced AAP lunar flights. A solar-powered sensor module based on a planned AAP Earth-resources observation module design would replace the LM. By spending 28 days (one lunar day-night period) in lunar polar orbit, the mission's augmented CSM could pass over the entire lunar surface in daylight, enabling the crew to conduct global high-resolution film photography. When time came to return to Earth, the astronauts would load exposed film into their CSM, then undock from the sensor module and leave it behind in lunar orbit to function as an independent satellite.

Hinners, James, and Schmidt explained that Lunar Exploration Program Phases 1 and 2 missions would gather "ground truth" data on the composition and structure of the moon's surface. These data would enable scientists to interpret Phase 3 mission results in preparation for Lunar Exploration Program Phase 4, which would span 1975-1976.

Phase 4 would see two "Dual Launch" Lunar Surface Rendezvous and Exploration Missions. Each Dual Launch mission would require two Saturn V rockets, two augmented CSMs, an LM-derived unmanned Lunar Payload Module (LPM), and an augmented ELM bearing one LFU.

LLM-10 and LLM-11 together would make up the first Dual Launch mission. LLM-10 would deliver an unmanned LPM to either Hyginus Rille or the Davy crater chain. The LLM-10 crew, orbiting the moon in their augmented CSM, would remotely pilot the LPM's final approach to the landing site to help to ensure that it would set down within 100 meters of a predetermined target point. Before returning to Earth, the LLM-10 astronauts would "photo locate" the landed LPM from lunar orbit to aid the follow-on LLM-11 crew in finding it. They would also release a science subsatellite into lunar orbit.

LLM-11 would see two astronauts wearing advanced "hard" (mostly non-fabric) space suits land their augmented ELM near the pre-landed LPM for a two-week stay. They would draw on the LPM's 8000-pound payload to conduct in-depth exploration of their complex landing site.

The LPM payload would include lunar surface transportation systems: specifically, one LFU and a one-man, 2000-pound Local Scientific Survey Module (LSSM) moon rover. Other LPM cargo would include: a spare hard suit; a core drill attached to the LPM for obtaining a 100-foot drill core; an LSSM-transportable core drill for obtaining 10-foot cores at scattered sites; life support consumables for replenishing those on board LLM-11's ELM; and an advanced lunar-surface geophysical station with a 10-year design life.

Hinners, James, and Schmidt selected the Marius Hills as the landing site for LLM-12 and LLM-13, their second Dual Launch mission pair and the final missions of their Lunar Exploration Program. The Marius Hills were popular with planners for their many domes and other features of possible volcanic origin.

The Bellcomm planners anticipated that, after the LLM-13 crew returned to Earth, even more ambitious AAP moon missions would commence. These might lead to establishment of a lunar surface outpost. They were, of course, incorrect; it became clear soon after they completed their report that lunar exploration would not become "a continuing aspect of human endeavor."

This NASA map, published at the time of the Apollo 17 mission in December 1972, shows the six Apollo landing sites. All landings occurred within an area the size of the western United States between the Mississippi River and the Rocky Mountains (on a world with about as much surface area as Europe and North America combined). If Apollo 17 had landed in St. Louis, Missouri, Apollo 16 would have landed in northeastern Texas; Apollo 15 on the Kansas-Nebraska border; Apollo 14 and Apollo 12 in New Mexico; and Apollo 11 in Oklahoma.
The earliest Apollo landing missions (Apollo 11, Apollo 12, and Apollo 14) were roughly equivalent to Bellcomm's LLM-1, LLM-2, and LLM-3, though their crews performed fewer moonwalks. Apollos 15, 16, and 17, by contrast, were mainly shaped by the certain knowledge that Apollo lunar exploration would soon conclude. They became unlike any of Bellcomm's proposed missions as NASA sought to accomplish as much lunar exploration as possible at minimal cost before political support for the Apollo Program ran out.

The final Apollo lunar mission, Apollo 17 (December 1972), saw astronauts Eugene Cernan and Harrison Schmitt explore the Highlands-bordering Taurus-Littrow mare site for about three days. They drove an electric-powered Lunar Roving Vehicle (LRV). Meanwhile, Ron Evans, on board the Apollo 17 CSM in lunar orbit, used a suite of sensors to map a broad swath of the moon's surface and released a science subsatellite.


"A Lunar Exploration Program – Case 710," N. Hinners, D. James, and F. Schmidt, TM-68-1012-1, Bellcomm, 5 January 1968

To a Rocky Moon: A Geologist's History of Lunar Exploration, D. Wilhelms, University of Arizona Press, 1993

The Geologic History of the Moon, U.S. Geological Survey Paper 1348, D. Wilhelms, J. McCauley, and N. Trask, USGS, 1987

More Information

Apollo's End: NASA Cancels Apollo 15 & Apollo 19 to Save Station/Shuttle (1970)

Rocket Belts and Rocket Chairs: Lunar Flying Units

"Assuming That Everything Goes Perfectly Well in the Apollo Program. . ." (1967)

Harold Urey and the Moon (1961)


  1. This comment has been removed by the author.

    1. Some Bellcomm reports remain online at the NASA Technical Reports Server, tho not as many as in the past. Mostly I've obtained mine through nearly 30 years of digging in archives. Given the effort and cost that went into finding them, I wouldn't want to give them away for free. Perhaps they and other documents could serve as incentives for people to contribute to my eventual Patreon campaign.


  2. Phase 3 strikes me as an extremely expensive way to put a satellite into orbit around the moon, especially given NASA was able to put Mariner 9 into orbit around Mars by 1971.

    1. Obviously the main purpose of the lunar polar orbiter Phase 3 LEP mission would not be to place a satellite in lunar polar orbit. Lunar Orbiter I reached lunar orbit in August 1966, so even at the time this report was put together we knew we could place an automated spacecraft into lunar orbit.

      The module would carry film cameras - film in those days provided much higher resolution than the scanned film system used on Lunar Orbiter. The astronauts would expose film for 28 days, then separate from the module and bring the film home to Earth in the CSM. The module would continue to operate for some period in an automatic mode, performing unspecified experiments. In those days, just tracking it could have been an informative experiment.

      So, the Bellcomm folks didn't see this as a satellite delivery mission - they saw an opportunity to squeeze a little more utility out of a piloted module that would be abandoned in lunar orbit in any case.


    2. Another great article! Thank you for writing it.

      I wonder if the proposed enhanced versions of the Saturn V would have made the dual launches for Phase 4 unnecessary. Thus, they could have sent an augmented CSM, an ELM, and an LPM to the moon on one launch. (I think there was a similar concept to the LPM called the LM Truck.) Maybe the enhanced Saturns could eventually place a Lunar Exploration System for Apollo (LESA) shelter on the moon.

      If I recall correctly, there were proposals to cram three astronauts into the LM for lunar outpost missions, leaving the CSM in orbit alone until it was time to come home. I wonder how comfortable people would be with that idea. I know that space stations were left untended between missions for a long time, but the station is a destination, not the means to get home.

    3. I can't edit my post, so I have a follow-up: The similar concept I was thinking of was called the LM Shelter; the LM Truck used LM components to place a vehicle on the moon. I'm not completely sure the CSM would have been left unattended in lunar orbit; I just thought it would be if the LM was modified to accept three astronauts. I suppose you could have modified the CM to carry four astronauts so one could remain with the ship in orbit. I don't know how practical this would have been.

    4. Phil:

      You are welcome. This is the latest version of an old post - it's probably Rev 4.0. I think it appeared in its earliest crude form on my first spaceflight history blog, Romance to Reality. Back then, I wrote bulleted summaries with very little interpretation or context.

      NASA and its contractors studied many Apollo enhancements - basically everything you've described except perhaps the four-man Apollo with three astronauts on the moon. I don't recall that scenario.

      I do recall that they studied leaving two astronauts on the moon for extended periods while the CSM with lone pilot went home to Earth. This was typically part of a temporary lunar base scheme. A second CSM with lone pilot would have been launched from Earth to pick them up. As you might imagine, that scenario - which left the astronauts without an option to retreat to lunar orbit - didn't have many fans.

      Toward the end of AAP lunar planning, NASA was leaning toward a one-week stay on the moon by two astronauts with a single upgraded LM - usually called the Augmented LM (ALM). The CSM pilot would have stayed in orbit alone during that period.

      LOR is praised as the mission mode that made a man on the moon possible. The trouble was, it had limitations. Ultimately, had exploration of the moon become a "continuing aspect of human endeavor," I think we'd have seen a return to Direct Ascent. In the 1990s, when NASA looked at the cheapest way of achieving a lunar outpost, it naturally gravitated back to Direct Ascent as the cheapest, least constrained method of staying for extended periods on the moon at almost any site.


  3. Thank you for your response. This is where I got the idea that three astronauts could go to the surface in an upgraded LM. http://www.astronautix.com/a/apollolmtaxi.html I think the big First Lunar Outpost direct ascent lander would have been a lot more comfortable, in a lot of ways.

    1. Phil:

      I think I might not have expressed myself clearly. There was indeed a proposal to land three astronauts on the moon in the Apollo LM and leave the CSM vacant. What I do not recall is any scheme to fly four astronauts in the CSM, land three, and leave one on board. That's not to say that no one entertained the concept, only that I have yet to find it (or, if I did find it, I forgot it).

      One drawback of a four-person Apollo mission would be consumables - four astronauts would use more than three and leaving one on board the CSM for perhaps an extended period would use more than leaving the CSM vacant. Of course, one can imagine ways around that - they would have had to anyway if they had flown (for example) a 28-day lunar polar orbiter CSM + instrument carrier mission. Cutting one astronaut from the crew would have stretched their supplies, but from what I've read, not enough.

      Hopefully I'm not explaining to you things you thoroughly understand. My goal here is to be sure we are not talking past each other, not to talk down to you.


  4. I always appreciate your comments and willingness to discuss ideas. When I was growing up, I read brief references to more advanced projects we weren't able to pursue. Thanks to the wonder of the Internet and sites like yours, I'm finally able to learn about them.

    The idea of four astronauts in an Apollo spacecraft on a lunar mission is pure speculation on my part, but it is influenced by this passage from Voyage by Stephen Baxter:

    "...the Apollo system had been heavily upgraded in the past few years. Rockwell had stretched the original lunar flight design, making it more robust and reliable, and increasing its capacity; Apollo was mostly used as an orbital ferry craft for taking crews to and from the Skylabs, but even flying solo it was capable of supporting as many as four men for eight days in orbit."

    Thank you for bringing up the 28-day lunar photography mission. I always figured that would be a grueling mission, and I wondered if it was really workable.


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