The precious expandable cargo is itself a simple test article, (or as those in the industry are keen to refer to it, a “pathfinder technology demonstrator”), which was manufactured by Bigelow Aerospace right here in Las Vegas, Nevada. Aptly titled the Bigelow Expandable Activity Module, or BEAM, the craft is designed to attach to the ISS and stay put for at least two years to see how it behaves.
Now, media outlets large and small, having caught wind of this impending technological departure from the streampunk-like status quo, (where hulking, submarine-like cylindrical pressure vessels serve as our spacecraft shells), are repeating the same, few details with great enthusiasm. However, general curiosity about BEAM’s design, structural elements, and expected performance is going generally unanswered.
Well, no more. There’s no question too big or too small to answer, here! So, for the intrepid of spirit, I hereby present the following 5-point breakdown of Everything You Wanted to Know About BEAM but Were Afraid to Ask… (using public-domain material, of course.)
1] What are BEAM’s pair of small, antennae-like protrusions for, anyway?
2] What about the sleek, wavy metal collar on the ‘hatch’ side of BEAM?
3] So, what are BEAM’s walls actually made of?
In the article, the walls of the expandable Bigelow “Nautilus” module under development at the time (later to be rechristened the B330 spacecraft) were described as having the following basic structure:
- “Five outer layers of graphite-fiber composites separated by foam spacers” that function as a micrometeorite and orbital debris (MMOD) shield.
- Moving inward, this is followed by a critical, intermediate layer known as the “restraint layer,” which serves as the load-bearing portion of the structure. This layer is described as “a web of interwoven straps made of high-strength fiber.”
- Finally, the innermost layer, called the “air bladder,” is a “plastic film” that “keeps the internal atmosphere from escaping into space.”
Admittedly, it has been some time since the article was written, and details may have shifted somewhat in the intervening years. -But, in a general sense, BEAM could be reasonably expected to follow the same sort of structural format.
For something a little more recent, one can also argue for a fairly close approximation of BEAM’s softgoods in another, modern inflatable spacecraft design. European aerospace titan Thales Alenia Space (TAS), (responsible for the design and manufacture of the rigid shell backbones of the European Space Agency’s Automated Transfer Vehicle supply ships as well as the Cygnus cargo freighters, and others), has its own inflatable spacecraft design known as REMSIM.
In landmark 2009 research presented at the International Symposium on Materials in a Space Environment, led by TAS researcher Roberto Destefanis, the REMSIM layers are revealed (and put through their paces).
So, odds are, if you want to know what’s inside BEAM’s collapsible/expandable spacecraft skin, the REMSIM “stack” isn’t a bad place to start.
4] Can BEAM really shield well against micrometeorite and orbital debris strikes?
Well, much like a Kevlar vest has no problem stopping a bullet, it turns out that expandable spacecraft have no problem holding their own against impinging space chunks. While specific information on how well BEAM’s softgoods hold up under punishment is proprietary, we can return once again to REMSIM for a good example.
So, again returning to the 2009 Destefanis paper, REMSIM softgoods test articles boasted surviving getting blasted with half-inch aluminum spheres at speeds exceeding 15,000 miles per hour. (This agrees with claims made in the aforementioned 2005 Popular Science article, which reports that Bigelow softgoods withstood a half-inch aluminum sphere impacting at better than 14,000 miles per hour.) Not too shabby at all, and according to the research, meets or exceeds the debris protection performance of rigid ISS modules using traditional “stuffed” Whipple Shields.
This implies that BEAM’s protection factor against micrometeorites and debris is just fine, if not outright superior to rigid modules.
5] What sort of radiation protection should we expect from BEAM?
This has been a big question, and one NASA has expressed particular interest in. In fact, it’s one of the primary functions of BEAM to determine just how favorable the radiation protection qualities of a softgoods spacecraft are.
The problem with space radiation is that it is generally more massive and highly energetic compared to ionizing radiation encountered on Earth’s surface, which makes it difficult to shield.
The problem with talking about space radiation shielding is that it depends on a boatload of variables — the more active our Sun, the more it deflects even more damaging radiation from exploding stars in our own Galaxy (and beyond) but trades it for an increased risk of being hit with lower-energy but overwhelming solar storms.
Keeping all of this in mind, if we return to the 2009 Destefanis study one final time, we find it has something to say about this as well.
By placing test articles meant to represent different types of spacecraft and spacecraft materials in front of particle accelerators powerful enough to fling atoms as large and fast as those fired into the cosmos by exploding stars, researchers can reliably predict how materials will shield against space radiation. This is exactly what the Destefanis study reports, using an iron-atom slinging accelerator at Brookhaven National Lab.
In a big-picture sense, the chart also reveals that REMSIM shields only 10% as well against heavy GCR as a fully-outfitted ISS module (3% versus 28.7%). While this might sound terrible at first glance, this is due largely to the fact that Columbus is currently far from empty, ringed with equipment racks, piping, tubing, cabling, and supplies. All of this extra material serves as supplemental shielding for astronauts located within.
By contrast, the basic REMSIM in this study is (like BEAM) completely empty, making the “10%” claim a somewhat unfair apples-to-oranges comparison. However, numbers like these more closely match the current situation between BEAM and the rest of ISS.
So, ultimately, if the REMSIM-BEAM comparison holds, one might expect a similar ratio between GCR-radiation shielding measurements made in BEAM and parallel readings taken across the rest of the ISS. And while the numbers might sound grim to the uninitiated, numbers like these are going to be exactly what NASA is looking for.
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I hope the information compiled in this post has been helpful at least to some, and as always, feedback is welcome.
Semper Exploro!
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