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— CH. 1 · INTRODUCTION —

RP-1

10 min listen · Ch. 1 of 7
7 sections
  • RP-1 is what put human beings on the moon, and it smells like diesel. Known formally as Rocket Propellant-1 or Refined Petroleum-1, this highly processed kerosene sits at the heart of some of the most consequential machines humanity has ever built. The Saturn V carried astronauts toward the moon on its first stage burning RP-1. The Falcon 9 lifts satellites into orbit on it. The Soyuz has used it for decades. Yet RP-1 is, at its core, just petroleum. The question worth asking is: what does it take to turn oil from the ground into something capable of reaching space? And why, in an era of methane engines and hydrogen fueled rockets, does kerosene keep showing up at the launchpad?

  • During and immediately after World War II, large liquid-fueled rockets commonly burned alcohols, primarily ethanol and occasionally methanol. Those fuels had a practical advantage. Their high heat of vaporization prevented regeneratively-cooled engines from melting, partly because the alcohol was often blended with several percent water. But engineers recognized that switching to hydrocarbon fuels would improve efficiency. Hydrocarbon molecules carry no oxygen atom, have negligible water content, and are slightly denser. Each of those properties boosts performance at the margins, and in rocketry, margins matter enormously.

    The transition to kerosene came with an unexpected problem. As burn times grew longer and combustion chamber pressures climbed higher, engine walls grew thinner and lighter. Raw kerosene used as coolant began to break down under heat. It would dissociate and polymerize, forming gas bubbles that caused cavitation and waxy deposits that blocked cooling passages. Once a passage narrowed, temperatures rose further. Higher temperatures caused more polymerization, which narrowed passages further. The cycle escalated rapidly, a condition engineers called thermal runaway, and it ended in engine wall ruptures or mechanical failures. The problem persisted even when the entire coolant flow consisted of kerosene. By the mid-1950s, rocket designers had run out of engineering solutions and turned to chemists instead.

  • Sulfur, as a chemical, attacks metals at high temperatures. Even trace amounts assist the polymerization that hardens seals and tubing. So sulfur and its compounds are held to a minimum in RP-1. Unsaturated compounds, including alkenes, alkynes, and aromatics, are also kept at low levels because they polymerize both at high temperatures and during long periods of storage. At one point, engineers anticipated that kerosene-fueled missiles might sit in storage for years before being activated. That function was eventually handed off to solid-fuel rockets, but the thermal stability requirements remained.

    Beyond removing unwanted compounds, chemists actively selected for the right ones. Linear alkanes were reduced in favor of cyclic and highly branched alkanes. The reasoning parallels the octane-rating logic of automotive fuel: cyclic and branched molecules significantly increase thermal stability. The most desirable forms are polycyclics such as ladderanes. The remaining hydrocarbons in RP-1 are at or near C12 mass. That careful selection gives RP-1 a high flash point, making it less of a fire hazard than ordinary petrol.

    The result is that RP-1 costs far more than common kerosene. Any petroleum can theoretically be refined into RP-1 with enough processing, but in practice rocket-grade kerosene is sourced from a small number of oil fields with high-quality base stock, or it is synthesized artificially. Military specifications for RP-1 are covered in MIL-R-25576, and its chemical and physical properties are documented in NISTIR 6646.

  • Russia and other former Soviet countries developed their own rocket kerosene formulations, called T-1 and RG-1. Their density is slightly higher than RP-1, sitting at 0.82 grams per milliliter compared to RP-1's 0.81. That small difference reflects a broader Soviet engineering philosophy of squeezing every possible unit of performance from a given fuel volume.

    Soviet engineers discovered they could push density even higher by chilling the kerosene before loading it into the rocket's tanks. The approach partially contradicted the original appeal of kerosene, which could be stored at ambient temperatures unlike the super-chilled propellants it competed against. But Soviet launch facilities already had infrastructure for managing cryogenic liquid oxygen and liquid nitrogen, both of which are far colder than kerosene. The launcher's central kerosene tank was surrounded on four sides and the top by liquid oxygen tanks, with a liquid nitrogen tank at the bottom. The four side boosters had relatively small kerosene tanks, each sitting between a liquid oxygen and a liquid nitrogen tank. Once chilled, the kerosene stayed cold long enough to complete launch preparations. The Soviets would eventually abandon the practice, but decades later SpaceX revisited the idea for the Falcon 9. All versions since the Falcon 9 Full Thrust have used sub-cooled RP-1, chilled to 20 degrees Fahrenheit, which delivers a 2.5 percent density increase.

  • Kerosene and liquid hydrogen represent opposite ends of a performance spectrum, and RP-1 sits firmly at the high-thrust end. Hydrogen engines achieve a specific impulse around 370 seconds in vacuum conditions. Kerosene engines land in the range of 270 seconds. Specific impulse measures how efficiently a propellant produces thrust from a given mass of fuel, so hydrogen looks like the obvious winner. But thrust also matters, particularly deep inside a gravity well at the moment of liftoff.

    Density is where kerosene makes up ground. Because RP-1 packs considerably more energy into a given volume than liquid hydrogen, it enables higher thrust relative to engine mass. That trade-off points toward a practical engineering solution: use kerosene in the first stage where raw thrust is needed most, then switch to hydrogen in upper stages where efficiency becomes the priority. Both the Saturn V and the Atlas V follow this dual-fuel architecture.

    Methane has increasingly drawn attention as a middle ground between hydrogen and kerosene. It offers middling molecular mass, middling efficiency, and density only slightly worse than kerosene. Because methane's handling difficulties are roughly comparable to those of liquid oxygen, a methane-oxygen rocket is nearly as straightforward to operate as a kerolox rocket. That balance makes methane better suited for a single-fuel rocket design, which tends to be more economical than dual-fuel designs because of reduced complexity. Starship, New Glenn, the first stage of Vulcan, and Zhuque-2 all use methalox.

  • When a rocket engine shuts down, fuel flow drops to zero almost instantly while the engine itself remains extremely hot. Whatever RP-1 is trapped in that hot hardware can polymerize or even carbonize. Beyond the shutdown moment, heavy fuels like kerosene leave petroleum residues over time, the same phenomenon visible in gasoline, diesel, or jet fuel tanks that have been in service for years. Rocket engines run for only minutes or even seconds over their entire cycle lifetimes, which prevents truly heavy deposits. But rockets are far more sensitive to deposits than ordinary engines, because the same narrow passages and precise tolerances that make rocket engines work also make them vulnerable to blockage.

    The practical consequence is that kerosene systems require more frequent teardowns and overhauls than hydrogen or methane systems would. This creates ongoing operations and labor expenses for both expendable and reusable engines. Even cold-flow tests, in which propellants flow through the engine without being ignited, can leave residues behind.

    Below a chamber pressure of about 1000 psi, kerosene produces sooty deposits on the inside of a nozzle and chamber liner that act as meaningful insulation, cutting heat flow into the wall by roughly a factor of two. Most modern hydrocarbon engines operate above that pressure threshold, so this bonus insulation effect is not significant for most engines currently in service. ABL Space Systems took a different approach with their E2 engine, which can run on either RP-1 or standard Jet-A, bypassing some of the supply constraints that affect the more tightly refined formulation.

  • Robert H. Goddard's earliest rockets ran on gasoline, not kerosene, a reminder that the path to RP-1 was not inevitable. While the RP-1 specification was still being developed, the propulsion company Rocketdyne was experimenting with a compound called diethyl cyclohexane. Tests indicated it was superior to RP-1. But its formulation was not finished before the Atlas and Titan I rockets, both designed around RP-1, moved into development. RP-1 became the standard, not because it was the best possible hydrocarbon fuel, but because it was ready when the hardware needed it.

    The Soviet Union briefly used a higher-energy formulation called syntin, chemically described as 1-methyl-1,2-dicyclopropyl cyclopropane, in upper stages. Russia is also working toward switching the Soyuz-2 from RP-1 to a formulation called naftil or naphthyl. After the RP-1 standard was established, a follow-on specification called RP-2 was developed, differing primarily in having an even lower sulfur content. Because most users found RP-1 acceptable, there was little commercial incentive to produce and stock a second, rarer, and more expensive variant. The OTRAG group launched test vehicles on more common fuel blends, and at least one of their rockets ran on diesel fuel, though no OTRAG vehicle came close to reaching orbit. The Indian Space Research Organisation is currently developing an RP-1 fueled engine designated SE-2000 for future rockets, suggesting the fuel's role in space launch is not finished.

Common questions

What is RP-1 rocket fuel made of?

RP-1 is a highly refined kerosene formulation. It is processed to stricter standards than aviation or heating kerosene, with tighter density and volatility ranges and significantly lower sulfur, olefin, and aromatic content. The remaining hydrocarbons are at or near C12 mass.

Which rockets use RP-1 as fuel?

RP-1 has powered a wide range of rockets, including the Saturn V, Saturn I and IB, Atlas, Falcon, Soyuz, Zenit, Electron, Antares, Delta I through III, and Energia. The Indian Space Research Organisation is also developing an RP-1 engine designated SE-2000 for future vehicles.

Why was RP-1 developed instead of using regular kerosene?

Raw kerosene breaks down under the heat and pressure of rocket engines, forming gas bubbles and waxy deposits that block cooling passages and trigger thermal runaway leading to engine failure. In the mid-1950s, rocket designers turned to chemists to create a heat-resistant hydrocarbon formulation, resulting in RP-1.

How does RP-1 compare to liquid hydrogen as a rocket fuel?

Hydrogen engines achieve a specific impulse around 370 seconds in vacuum while kerosene engines reach roughly 270 seconds, meaning hydrogen is more fuel-efficient. However, RP-1's higher density delivers greater thrust relative to engine mass, making it preferred for first stages where lift performance matters most.

What is the difference between RP-1 and the Russian rocket fuel RG-1?

RG-1 and T-1 are the primary rocket kerosene formulations used in Russia and former Soviet countries. Their density is slightly higher at 0.82 grams per milliliter compared to RP-1's 0.81. Soviet engineers also developed techniques for chilling the kerosene before loading to increase density further.

Why does SpaceX chill RP-1 for the Falcon 9?

All Falcon 9 versions since the Falcon 9 Full Thrust use sub-cooled RP-1, chilled to 20 degrees Fahrenheit, which delivers a 2.5 percent density increase. SpaceX revisited a technique the Soviets had developed and later abandoned, using existing cryogenic infrastructure at the launch site to keep the kerosene cold during countdown.

All sources

14 references cited across the entry

  1. 3BookStages to Saturn: A Technological History of the Apollo/Saturn Launch VehiclesRoger E. Bilstein — NASA — 1996
  2. 5BookHistory of Liquid Propellant Rocket EnginesGeorge Paul Sutton — American Institute of Aeronautics and Astronautics — 2006
  3. 9-340 F in this case. Deep cryo increases density and amplifies rocket performance. First time anyone has gone this low for O2. RP-1 chilled from 70F to 20 FElon Musk — 17 December 2015
  4. 11BookIgnition! an informal history of liquid rocket propellantsJ. D. Clark et al. — Rutgers University Press — 1972