SpaceEngineer & Strelok
Okay, let’s break this into layers. If you were to build a propulsion system that slashes delta‑v while keeping weight in check, what would be the first constraint you’d lock onto?
The first thing to lock onto is the propellant mass fraction – basically the mass ratio of propellant to the total vehicle mass. If you can’t keep that in check, the delta‑v you’re chasing will always come at the price of a heavier craft.
Good, but that’s just the headline. What’s the actual propellant? Liquid hydrogen? LOX? Or a solid grain? Each gives a different Isp, and that changes the mass ratio curve. Also, don’t forget structural mass – a light frame isn’t enough if the engine’s heavier than the fuel pack. Give me the numbers, and we’ll see if the design really holds together.
I’d start with a liquid bipropellant combo – LOX/H2 gives the best specific impulse, about 450 s for a modern cryogenic engine, but it’s a lot of weight in the tanks. A LOX/LCH4 mix drops the Isp to roughly 360 s but the propellant density is higher, so you can fit more mass in the same volume. For a solid grain you’re looking at 140–160 s, but the structural mass of the grain and casing adds another 15–20 % of the propellant mass. If you target a structural mass fraction of 10 % of the total, a liquid system with a lightweight composite pressure vessel can push that down to 8 %. So with LOX/H2, you’d have a propellant mass fraction of about 90 % and a structural mass fraction of 8 % – that’s the sweet spot for high delta‑v without a runaway weight penalty.
Nice numbers, but remember the tanks will be a weak point – cryo tanks need heavy insulation, which creeps up that 8 % structural figure. If the insulation takes another 2 %, you’re looking at 10 % again. Maybe tweak the methane mix for a lighter envelope and still keep Isp high enough. Keep a margin on the mass budget, or the whole thing will collapse on the first load test.
You’re right, insulation is a silent weight killer. With methane the tanks can be thinner, but you still need a decent thermal shield. I’d look at a high‑temperature composite lined with a lightweight vapor‑gap layer, which cuts the insulation mass by maybe 30 %. That brings the structural fraction back to about 8 %, and you still get a 360 s Isp. Adding a 5 % margin in the budget should give us a cushion for the first load test.
Sounds solid, but don’t forget the engine mass. Even with a lighter tank, a high‑performance methane engine will still add a few hundred kilos, and that pushes the overall mass fraction up. Keep an eye on the thrust‑to‑weight ratio for the first stage – if you’re still hunting 450 s, you’ll need an extra 10 % structural buffer or the vehicle will buckle under its own weight. Check the margins on the pressure vessel and the insulation thickness; a 5 % over‑design on those usually saves you from a first‑flight failure.
Engine mass is the real bottleneck; a high‑performance methane engine sits at around 200 kg, so the vehicle’s dry mass climbs fast. If we keep the pressure‑vessel and insulation to a 5 % over‑design, the total structural fraction stays near 9 %. That leaves just enough margin to hit a 4:1 thrust‑to‑weight on the first stage without the frame giving way. Keep tightening the propellant fill level and the tank shape – every gram saved there pushes the delta‑v up.
Nice, but “just enough margin” is a risky phrase. If the engine stalls on a mis‑tuned thrust curve or the tank leaks, that 4:1 ratio drops fast. Consider a staged approach—get the first burn to a clean 3.5:1 and then add a margin in the propellant load. Also, keep a contingency for thermal cycling; a single micrometeorite puncture could shift the whole balance. Tighten the shape is good, but don’t let the weight savings compromise the structural integrity under load.
You’re right, a 3.5:1 T/W baseline is safer. I’ll add an extra 8 % propellant load to cover any engine hiccup and give the tanks a thicker, but still lightweight, liner to survive a micrometeorite. The pressure‑vessel will be a double‑wall composite with a sacrificial buffer; that keeps the structural margin high while we still hit the delta‑v goal.
That extra 8 % is a nice safety net, but it also drags the dry mass up. Make sure the buffer layer doesn’t become a permanent weight penalty; you could use a single‑layer sacrificial film that tears off on impact, rather than a full second wall. Keep the T/W calculation tight and double‑check the thermal gradients—any asymmetry will create a bending moment that your double‑wall won’t cancel. And remember, the best weapon against micrometeorites is a predictable, symmetrical load, not a haphazard over‑design.
A single sacrificial film is the way to go; it lets the main composite keep its mass down and only loses a few grams if struck. I’ll model the load curve to stay within a 2 % symmetry tolerance so the bending moments stay negligible. That keeps the pressure‑vessel light but still able to handle the thermal cycling. And the extra 8 % propellant is kept in reserve, not as a permanent weight—withdraw it after the first burn if all goes as planned.