Chapter 15: By Leaps and Bounds, Part II: Staying a Little Longer.
(Elton John, Crocodile Rock)
“The Space Shuttle program was to define an era, delivering the promise of routine orbital access on a scale never before seen. The Shuttle Orbiter and STS would perform in tandem to allow on-orbit construction, continued and expanded planetary exploration and the delivery of countless humans into Earth-Orbit.”
- Author Unknown, 1972
With the discovery and eventual analysis of frozen water on the lunar surface, Apollo’s objectives and landing sites were subject to change. Apollo 20, however, would prove an exception. Originally scheduled for Apollo 18, Armstrong and Schmitt were transferred to Apollo 20, demonstrating the intermediate capabilities of the Lunar Module in a site chosen months prior: the Vallis Schröteri. The valley, believed to be a collapsed magma tube created in the result of long-dorman lunar volcanism, was chosen as it would provide scientists on the ground with ancient regolith samples, as well as a large variety of terrain feature analysis.
Apollo 20 was to be the first of as many as four K-Class lunar missions; While later missions aimed to stay on the surface for a month or more, the K-Class flights would demonstrate just a few of the many components necessary to pull this mission off. Foremost of these was the new L-Class Lunar Module; The L-Class upgrades, called earlier in their development the “LM-Taxi” were relatively extensive. The LMDE would receive a small bump in chamber pressure and thus increases in specific impulse and thrust, with fuel load increasing to match. The LM would also gain the capabilities to ferry 3 astronauts through the L-Class Ascent Module. Most importantly however, the Lunar Module would transition from battery power to fuel cells using hydrogen and oxygen stored in both stages, this allowing much longer duration stays and operation in a low-power mode. These changes would, of course, return some of the pesky mass that was removed during early development of the LM; This, however, was offset by the increase in TLI-payload allotted by the J-2S.
The L-Class Descent Module would also gain the ability to fly autonomously. This would, in eventuality, allow the delivery of unmanned supply landings by an S-IVC and LM, alongside semi-permanent base elements. These components, however, were not ready for flight, with only the L-Class Ascent and Descent module being ready by 1972. This, however, was anticipated. The K-class missions aimed to demonstrate L-Class LM hardware by landing a crew of two on the lunar surface for up to 7 days, allowing expanded exploration capabilities over the previous J-Class flights. Additionally, if schedules permitted, the latter K-Class missions were to demonstrate the upgraded S-IVC alongside its capabilities to deliver payloads to lunar orbit directly.
All the while, STS and Space Shuttle development was speeding up as planned. While many proposals had been put forward, ultimately it was Boeing’s proposal that won NASA over. Derived directly from the Saturn V, and promising more than 3 flights a month, the system won over NASA with more than just its cost. The design promised rapid reuse based on engine testing, demonstrating reuse of the J-2S and F-1 engines with little more than cleaning between firings.
The first stage of the Space Transportation System was to be derived closely from the S-IC, with some major changes. While initial design considerations toyed with the idea of a separable wing that would be mounted directly to a lightly modified S-IC, this was eventually decided to be needlessly complex. A staple feature of this design, however, was a split tail fin allowing improved stability at high angles of attack. Ultimately, this feature would be passed on to the fixed-wing alternative, leading to a small run of modified S-ICs.
These S-ICs, Dubbed the Reusable S-IC or RS-IC, were to employ the use of a metallic heatshield. This shielding, not dissimilar to that used on the X-15 by nasa years prior, promised to be lightweight, require minimal inspection and allow near-zero turnaround times. The RS-IC would have a single, monolithic delta wing protruding from its base, with split tail fins either side. This, alongside some simple reaction controls would allow the stage to easily descend from the hellish mach 7 plasma that was to engulf the stage as it fell through the atmosphere. The stage would utilize jet engines to maintain the crossrange capabilities necessary to return to the launch site; These engine’s configuration, however, was something of an internal debate.
(Initial wing-seated S-IC design)
(Initial Fixed-Wing design)
While most argued for jet engines mounted on the underside of the RS-IC’s wings, still others argued for engines to be mounted inside the wing, or even the nose; This, they argued, would allow the engines to be shielded more thoroughly than the alternatives. As contracts were assigned in 1972, the debate still raged, and it was one of the last major points of discussion. Alloys were chosen later that year, and an initial test flight was expected for 1977 or 1978.
(Boeing internal-diagram demonstrating nose-mounted engines)
The Space Transportation System was to utilize a semi-expendable upper stage, produced by North American Rockwell, derived from the S-II. This stage would consist of two primary components, the External Tank (ET) and the Engine Recovery Device (ERD). The STS External tank was to be a split-bulkhead design derived from the S-II stage, scaled up to the J-2S’ capabilities. This, it was hoped, would allow the stage to not only be more capable, but significantly cheaper. The validity of such claims, however, was in question to many of those at NASA. The tank would crossfeed propellants into the ERD, something that had not been demonstrated as of yet. If successful, many wondered, would it be cheap?
The ERD was to be the major cost-saving component of the second stage however, allowing nearly all essential components to be recovered. The Engine Recovery Device was a large, conical module capable of recovering the 5 J-2S engines alongside the stage’s avionics and flight computers. This would mean that all the STS expended in a single launch was the fuel tank, a component designed for mass production from the get go. The stage, collectively referred to as the S-IIB by designers, demonstrated the promise of the STS; Increased flight rate, increased redundancy, and routine access to space, all at a low cost.
(Early Concept art of the ERD in Low-Earth Orbit)
The stage was quite early in development, but was assigned alongside the contract to build the RS-IC, and the Shuttle in 1972. The final piece of the puzzle, the Shuttle, was the largest mystery though. A contract had been awarded to the Boeing and Martin Marietta companies to develop a large, lifting body orbiter. The orbiters were to regularly shuttle 8 crew to orbit alongside more than 20 tons of payload, as many as 24 times a year. These orbiters would ultimately become the backbone of the systems capabilities, acting as a universal utility craft capable of launching, retrieving and servicing a number of craft in orbit. The program had big goals, and the hope was that deriving many components from Apollo-era hardware would allow development to go relatively smoothly.
Nevertheless, Apollo continued his march onwards, and Apollo 20 lifted off that fall. The mission, a week long endeavour to the lunar surface, was the start of Phase-II for the program. This mission would, like Apollo 11 before it, be the proving ground for nearly all missions to come. The launcher lifted off without a hitch, and as the S-IC flamed out, the 5 J-2S’ on the second stage flared to life. The rocket had made it to orbit, and before long the S-IVB performed her TLI once again.
Armstrong: I got eyes on the Constitution-
Capcom: Roger that America, go for docking.
…
Schmitt: We’re docked.
Capcom: Roger that, Joe!
Apollo 20 extracted their lunar module, clearing it from the S-IVB and performing separation maneuvers. The crew continued onwards to the moon as had become routine over the past 4 years; Their 3 day trip was largely uneventful, with minor experiments and tests being run on the LM. At Perilune, the America CSM braked into lunar orbit, slowing her velocity down enough to release the LM. The S-IVB that had delivered them to TLI flew past the moon shortly on their heels, reporting nominal tank pressure as the stage exited the Earth’s sphere of influence shortly thereafter.
After some minor checkouts in lunar orbit, the lander was cleared for descent. Armstrong and Kerwin boarded the LM, leaving Eisele to pilot the CSM by himself. The two spacecraft separated with the signature thud and hiss of the tunnel venting. The LM fired her thrusters separating comfortably from the command module.
Armstrong: Alright, we’re separated, keep her warm for us Joe!
Kerwin: Of course boys!
The LM began her descent shortly thereafter; While the lander's mass had increased by over a ton, the engine’s thrust had increased similarly, allowing the lander to maintain a relatively consistent descent profile. As the lander came in closer to the surface the call was made-
Schmitt: Contact!
Armstrong: Engine off-
…
Armstrong: Houston, Constitution is down. Right on the mark!
Schmitt: This cobra’s got fangs, we can see a couple sharp looking boulders from where we’re at. Dodged a bullet there didn’t we Niel.
Armstrong: Sure did.
Capcom: Welcome to the Vallis Schröteri, 20.
Shortly after their landing, the crew began preparing for their rest period. After checking out the LM, and inflating their mattresses, the two men went to sleep; The crew awaited the grand adventure of a lifetime that was to face them in the days to come. After a restful night's sleep, the theme from 2001 a space odyssey rang over the Lunar Modules speakers, waking the crew from their rest. Spacecraft Communicator Karl Henize’s voice came over the intercom shortly after:
Capcom: Gooooooood morning Apollo 20!
Armstrong: I’m up, I’m up.
Schmitt: Sheesh… quite the entrance, Houston.
The men began deflating their mattresses shortly after, the mattresses stowing into the floorboards beneath them.
Capcom: How’d you sleep, boys?
Armstrong: Hell of a lot better than I did on 11, that’s for sure.
Early Apollo astronauts had complained about a lack of restful sleep; While this was largely a constraint of the LM’s small cabin, and was mitigated temporarily with the inclusion of hammocks, engineers decided to tackle the issue head on in the L-Series landers. The landers would include folding inflatable mattresses that could stow into the floorboards underneath a small hatch in the main standing-room and the main hallway; This allowing the astronauts to receive more restful sleep alongside the use of radiation-shielded facemasks.
Outside of the Earth’s protective magnetic field, NASA found that cosmic-rays, high energy particles emitted by distant suns, could impact and react with the optic nerve. This caused the astronauts to see flashes, clouds or small visual hallucinations. This, understandably made it difficult to sleep, facilitating the need for the face masks.
Capcom: Alright you two, you can begin EVA-1. We’re gonna go ahead and get that new LRV out for a spin!
Armstrong: Roger, depressurizing.
The LM hissed, and the hatch opened. As the crew descended down the ladder, they caught their first up-close glimpse of the lander. Constitution was dressed in a silver cladding, accenting her enlarged fuel tanks. As the men descended the ladder, their focus shifted rapidly to the LM’s rear bay.
(LM-13, Constitution, in the Vallis Schröteri, marking the first use of NASA’s new worm logo.)
The LRV, or Lunar Roving Vehicle, had received a series of minor upgrades preparing it for the K and L-Class flights ahead. The rover received rechargeable battery-packs, which would charge off the LM’s fuel cells. Additionally, the rover received far heavier batteries, over doubling its range; This impared the top speed of the rover slightly, but as was shown by Ronald Evans on Apollo 18, this wouldn’t be an issue. Evans had demonstrated, by accident or on purpose, the top speed of the LRV to be in excess of 13mph, or 21 kph. Boeing and GM disapproved of this, however, and the upgrades were actually anticipated to make the LRV harder to over-speed.
The mission’s plan was predominately the same as the J-Class missions before it; Explore the lunar surface, gather a few interesting looking rocks, and get your ass back home. This had become something of a routine over the past years, but the K-Class missions aimed to crank this formula to 11. With missions stretching as long as a week, this allowed far greater exploration. Setting out from their landing site in the center of the Valley, the crew headed north to the valley’s edge.
(Map of Apollo 20’s landing site. LEM shown in Blue, EVA-1 in red, EVA-2 in Teal, and EVA-3 in Green)
By day 3, however, mission controllers had gained enough confidence with the new LRV to push it to its limits. The crew set off that morning on a nearly 7 and a half hour, 100km drive through towards the Cobra’s Head. EVA-2 began and the crew headed to the North-West, slowly trekking through the lunar terrain and stopping periodically
Armstrong: Hell of a drive, eh?
Schmitt: No kidding, this thing can move pretty well.
Capcom: How are you coming along, boys?
Armstrong: The convertible’s zipping across the surface babe, not a worry in the world!
Schmitt: Wooohoo!
Capcom: Drive safe, you two. Last thing we need is to have to call a tow truck.
Armstrong: Roger that, no drifting.
Schmitt: What a bummer.
When the crew arrived at the mouth of the crater, Schmitt was overjoyed. This crater, believed to be an ancient volcano, was one of the most scientifically interesting sites visited thus far. Before long, a small cave was spotted and Schmitt began his stroll to the site of interest, Armstrong in tow.
Schmitt: Yippee
Armstrong: Slow down buddy-
Schmitt: I was strolling on the moon one day…
Scmitt: In the very mary month of-
Armstrong: September!
Schmitt: No, May!
After a jonty stroll across the collapsed lava tube, the crews arrived at the mouth of the small cave, and collected a few samples. In these samples, many volatile compounds would be found, having been shielded from the worst of the Sun’s rays; Among these were traces of ammonium, carbon dioxide, and of course, water. The crew returned to the LRV, looped around the rim of the crater, and began their journey home for the evening.
As the crew returned that afternoon, the LRV was loaded to the brim with surface samples. The mission’s capabilities were somewhat limited by the LM’s lack of a pressurized lab, but NASA hoped to have this sorted out in the coming years. Nevertheless, the crew remained on the surface for four more days, and conducted another long-distance EVA. All the while, NASA was gathering more and more data about how the lunar gravity affected astronauts, conducting a comparative study between Kerwin’s week in microgravity and that of Armstrong and Schmitt. Their mission over doubled Apollo 18’s previous endurance record, clocking in just over 7 days on the lunar surface. Before long though, the crew had to return to the CSM, and their lander began ascent.
Capcom: Okay, we have them in frame-
Armstrong: 3… 2… 1…
Schmitt: Ignition-
Armstrong: Liftoff!
Capcom: Roger liftoff, Constitution!
(Liftoff of the first L-Class LM from the lunar surface)
After a rapid ascent, the crews finally rendezvoused with the CSM, returning after their week-long mission.
Kerwin: They’re back, flight. And they brought a hell of a lot of rocks.
Schmitt: We sure did!
Kerwin: I told you to bring me back a souvenir, not some measly dirt!
Armstrong: Sorry boss, just followin’ orders.
Capcom: Joe may not appreciate it, but we sure will. Good work out there you two, let’s get you all back home.
The LM and CSM separated one final time, separating the two spacecraft permanently and starting the series of maneuvers necessary to return the three men safely to the Earth. Days later, the capsule separated from the service module, leaving it behind to burn in the hellfire of reentry. The heat shield protected the men and their precious cargo, and the spacecraft splashed down, just shy of 16 days after liftoff.
As Apollo 20 landed, preparations were underway for Apollo 21 and the mission that followed it: Skylab. Skylab 1 and 2 were being prepared in NASA’s vehicle assembly building alongside the far-off Apollo 22. Marking the first, but not final time that four missions were being prepared simultaneously in the complex. Skylab was to be the world’s first space station, following on the failed launch of Salyut 1 in december of 1972. Scheduled to lift off in May of 1973, the station was an incredibly ambitious undertaking.
Skylab, in development since the late 60’s, was to be a station derived from the S-IVB stage. The station was to house a number of scientific payloads, including the Apollo Telescope Mount. The ATM aimed to allow solar observation, and recording. Additionally, the station would demonstrate the costs-savings of the so-called dry-workshop method of hollowing out a fuel tank to turn into a habitation module. The station was to be the first in a series of laboratories, the next of which had gotten approval alongside the ASTP-II mission earlier that summer. As April showers faded across the floridian coast and gave way to the beating sun of summer, Skylab lifted off atop her launcher.