A rocket engine nozzle is a propelling nozzle (usually of the de Laval type) used in a rocket engine to expand and accelerate the combustion gases produced by burning propellants so that the exhaust gases exit the nozzle at hypersonic velocities.
Simply: the rocket (pumps and a combustion chamber) generates high pressure, a few hundred atmospheres. The nozzle turns the static high pressure high temperature gas into rapidly moving gas at near-ambient pressure.
History
The de Laval nozzle was originally developed in the 19th century by Gustaf de Laval for use in steam turbines. It was first used in an early rocket engine developed by Robert Goddard, one of the fathers of modern rocketry. It has since been used in almost all rocket engines, including Walter Thiel's implementation, which made possible Germany's V-2 rocket.
Atmospheric use
The
optimal size of a rocket engine nozzle to be used within the atmosphere
is achieved when the exit pressure equals ambient (atmospheric)
pressure, which decreases with altitude. For rockets travelling from the
Earth to orbit, a simple nozzle design is only optimal at one altitude,
losing efficiency and wasting fuel at other altitudes.
Just past the throat, the pressure of the gas is higher than
ambient pressure and needs to be lowered between the throat and the
nozzle exit by expansion. If the pressure of the jet leaving the nozzle
exit is still above ambient pressure, then a nozzle is said to be
"underexpanded"; if the jet is below ambient pressure, then it is
"overexpanded".
Slight overexpansion causes a slight reduction in efficiency, but
otherwise does little harm. However, if the exit pressure is less than
approximately 40% that of ambient, then "flow separation" occurs. This
can cause jet instabilities that can cause damage to the nozzle or
simply cause control difficulties of the vehicle or the engine.
In some cases it is desirable for reliability and safety reasons
to ignite a rocket engine on the ground that will be used all the way to
orbit. For optimal liftoff
performance, the pressure of the gases exiting nozzle should be at
sea-level pressure; however, if a rocket engine is primarily designed
for use at high altitudes and is only providing additional thrust to
another "first-stage" engine during liftoff in a multi-stage
design, then designers will usually opt for an overexpanded nozzle (at
sea-level) design, making it more efficient at higher altitudes, where
the ambient pressure is lower. This was the technique employed on the Space shuttle's main engines, which spent most of their powered trajectory in near-vacuum, while the shuttle's two solid rocket boosters provided the majority of the liftoff thrust.
Vacuum use
For
nozzles that are used in vacuum or at very high altitude, it is
impossible to match ambient pressure; rather, nozzles with larger area
ratio are usually more efficient. However, a very long nozzle has
significant mass, a drawback in and of itself. A length that optimises
overall vehicle performance typically has to be found. Additionally, as
the temperature of the gas in the nozzle decreases, some components of
the exhaust gases (such as water vapour from the combustion process) may
condense or even freeze. This is highly undesirable and needs to be
avoided.
Magnetic nozzles have been proposed for some types of propulsion (for example VASIMR), in which the flow of plasma or ions are directed by magnetic fields
instead of walls made of solid materials. These can be advantageous,
since a magnetic field itself cannot melt, and the plasma temperatures
can reach millions of kelvins.
However, there are often thermal design challenges presented by the
coils themselves, particularly if superconducting coils are used to form
the throat and expansion fields.
One-dimensional analysis of gas flow in rocket engine nozzles
The analysis of gas flow through de Laval nozzles involves a number of concepts and simplifying assumptions:
- The combustion gas is assumed to be an ideal gas.
- The gas flow is isentropic i.e., at constant entropy, as the result of the assumption of non-viscous fluid, and adiabatic process.
- The gas flow is constant (i.e., steady) during the period of the propellant burn.
- The gas flow is non-turbulent and axisymmetric from gas inlet to exhaust gas exit (i.e., along the nozzle's axis of symmetry)
- The flow behavior is compressible since the fluid is a gas.
As the combustion gas enters the rocket nozzle, it is traveling at subsonic
velocities. As the throat constricts, the gas is forced to accelerate
until at the nozzle throat, where the cross-sectional area is the least,
the linear velocity becomes sonic. From the throat the cross-sectional area then increases, the gas expands and the linear velocity becomes progressively more supersonic.
The linear velocity of the exiting exhaust gases can be calculated using the following equation
where: | |
, | exhaust velocity at nozzle exit (m/s) |
---|---|
, | absolute temperature of inlet gas (K) |
= 8314.5 J/kmol·K, universal gas law constant | |
, | the gas molecular mass or weight, (kg/kmol) |
, isentropic expansion factor | |
, | specific heat of the gas at constant pressure |
, | specific heat of the gas at constant volume |
, | absolute pressure of exhaust gas at nozzle exit (Pa) |
, | absolute pressure of inlet gas (Pa) |
Some typical values of the exhaust gas velocity ve for rocket engines burning various propellants are:
- 1.7 to 2.9 km/s (3800 to 6500 mi/h) for liquid monopropellants
- 2.9 to 4.5 km/s (6500 to 10100 mi/h) for liquid bipropellants
- 2.1 to 3.2 km/s (4700 to 7200 mi/h) for solid propellants
As a note of interest, ve is sometimes referred to as the ideal exhaust gas velocity because it based on the assumption that the exhaust gas behaves as an ideal gas.
As an example calculation using the above equation, assume that
the propellant combustion gases are: at an absolute pressure entering
the nozzle of p = 7.0 MPa and exit the rocket exhaust at an absolute pressure of pe = 0.1 MPa; at an absolute temperature of T = 3500 K; with an isentropic expansion factor of γ = 1.22 and a molar mass of M = 22 kg/kmol. Using those values in the above equation yields an exhaust velocity ve = 2802 m/s or 2.80 km/s which is consistent with above typical values.
The technical literature can be very confusing because many
authors fail to explain whether they are using the universal gas law
constant R which applies to any ideal gas or whether they are using the gas law constant Rs which only applies to a specific individual gas. The relationship between the two constants is Rs = R/M, where R is the universal gas constant, and M is the molar mass of the gas.
Specific impulse
Thrust is the force that moves a rocket through the air or space. Thrust is generated by the propulsion
system of the rocket through the application of Newton's third law of
motion: "For every action there is an equal and opposite reaction". A
gas or working fluid is accelerated out the rear of the rocket engine
nozzle, and the rocket is accelerated in the opposite direction. The
thrust of a rocket engine nozzle can be defined as:
and for perfectly expanded nozzles, this reduces to:
The specific impulse is the ratio of the thrust produced to the weight flow of the propellants. It is a measure of the fuel efficiency of a rocket engine. In English Engineering units it can be obtained as
where: , gross rocket engine thrust (N) , mass flow rate of exhaust gas (kg/s) , exhaust gas velocity at nozzle exit (m/s) , exhaust gas pressure at nozzle exit (Pa) , external ambient pressure, or free stream pressure (Pa) , cross-sectional area of nozzle exhaust exit (m²) , equivalent (or effective) exhaust gas velocity at nozzle exit (m/s) , specific impulse (s) , standard gravitational acceleration at sea level on Earth = 9.807 m/s²
In certain cases, where equals , the formula becomes
In cases where this may not be so, since for a rocket nozzle is proportional to , it is possible to define a constant quantity that is the vacuum for any given engine thus:
and hence:
which is simply the vacuum thrust minus the force of the ambient atmospheric pressure acting over the exit plane.
Essentially then, for rocket nozzles, the ambient pressure acting
on the engine cancels except over the exit plane of the rocket engine
in a rearward direction, while the exhaust jet generates forward thrust.
Aerostatic back-pressure and optimal expansion
As
the gas travels down the expansion part of the nozzle, the pressure and
temperature decrease, while the speed of the gas increases.
The supersonic nature of the exhaust jet means that the pressure
of the exhaust can be significantly different from ambient pressure –
the outside air is unable to equalize the pressure upstream due to the
very high jet velocity. Therefore, for supersonic nozzles, it is
actually possible for the pressure of the gas exiting the nozzle to be
significantly below or very greatly above ambient pressure.
If the exit pressure is too low, then the jet can separate from
the nozzle. This is often unstable, and the jet will generally cause
large off-axis thrusts and may mechanically damage the nozzle.
This separation generally occurs if the exit pressure drops below
roughly 30–45% of ambient, but separation may be delayed to far lower
pressures if the nozzle is designed to increase the pressure at the rim,
as is achieved with the SSME (1–2 psi at 15 psi ambient).
In addition, as the rocket engine starts up or throttles, the
chamber pressure varies, and this generates different levels of
efficiency. At low chamber pressures the engine is almost inevitably
going to be grossly over-expanded.
Optimal shape
The
ratio of the area of the narrowest part of the nozzle to the exit plane
area is mainly what determines how efficiently the expansion of the
exhaust gases is converted into linear velocity, the exhaust velocity,
and therefore the thrust of the rocket engine. The gas properties have an effect as well.
The shape of the nozzle also modestly affects how efficiently the
expansion of the exhaust gases is converted into linear motion. The
simplest nozzle shape has a ~15° cone half-angle, which is about 98%
efficient. Smaller angles give very slightly higher efficiency, larger
angles give lower efficiency.
More complex shapes of revolution are frequently used, such as Bell nozzles
or parabolic shapes. These give perhaps 1% higher efficiency than the
cone nozzle and can be shorter and lighter. They are widely used on
launch vehicles and other rockets where weight is at a premium. They
are, of course, harder to fabricate, so are typically more costly.
There is also a theoretically optimal nozzle shape for maximal
exhaust speed. However, a shorter bell shape is typically used, which
gives better overall performance due to its much lower weight, shorter
length, lower drag losses, and only very marginally lower exhaust speed.
Other design aspects affect the efficiency of a rocket nozzle.
The nozzle's throat should have a smooth radius. The internal angle that
narrows to the throat also has an effect on the overall efficiency, but
this is small. The exit angle of the nozzle needs to be as small as
possible (about 12°) in order to minimize the chances of separation
problems at low exit pressures.
Advanced designs
A number of more sophisticated designs have been proposed for altitude compensation and other uses.
Nozzles with an atmospheric boundary include:
- expansion-deflection nozzle,
- plug nozzle,
- aerospike,
- Single Expansion Ramp Nozzle (SERN), a linear expansion nozzle, where the gas pressure transfers work only on one side and which could be described as a single-sided aerospike nozzle.
Each of these allows the supersonic flow to adapt to the ambient
pressure by expanding or contracting, thereby changing the exit ratio so
that it is at (or near) optimal exit pressure for the corresponding
altitude. The plug and aerospike nozzles are very similar in that they
are radial in-flow designs but plug nozzles feature a solid centerbody
(sometimes truncated) and aerospike nozzles have a "base-bleed" of gases
to simulate a solid center-body. ED nozzles are radial out-flow nozzles
with the flow deflected by a center pintle.
Controlled flow-separation nozzles include:
- expanding nozzle,
- bell nozzles with a removable insert,
- Stepped nozzles, or dual-bell nozzles.
These are generally very similar to bell nozzles but include an
insert or mechanism by which the exit area ratio can be increased as
ambient pressure is reduced.
Dual-mode nozzles include:
- dual-expander nozzle,
- dual-throat nozzle.
These have either two throats or two thrust chambers (with
corresponding throats). The central throat is of a standard design and
is surrounded by an annular throat, which exhausts gases from the same
(dual-throat) or a separate (dual-expander) thrust chamber. Both throats
would, in either case, discharge into a bell nozzle. At higher
altitudes, where the ambient pressure is lower, the central nozzle would
be shut off, reducing the throat area and thereby increasing the nozzle
area ratio. These designs require additional complexity, but an
advantage of having two thrust chambers is that they can be configured
to burn different propellants or different fuel mixture ratios.
Similarly, Aerojet has also designed a nozzle called the "Thrust
Augmented Nozzle",
which injects propellant and oxidiser directly into the nozzle section
for combustion, allowing larger area ratio nozzles to be used deeper in
an atmosphere than they would without augmentation due to effects of
flow separation. They would again allow multiple propellants to be used
(such as RP-1), further increasing thrust.
Liquid injection thrust vectoring nozzles are another advanced
design that allow pitch and yaw control from un-gimbaled nozzles.
India's PSLV
calls its design "Secondary Injection Thrust Vector Control System";
strontium perchlorate is injected through various fluid paths in the
nozzle to achieve the desired control. Some ICBMs and boosters, such as
the Titan IIIC and Minuteman II, use similar designs.