Editing Tsiolkovsky rocket equation

{{Short description|Mathematical equation describing the motion of a rocket}}
{{Astrodynamics |Preflight engineering}}
[[File:Tsiolkovsky rocket equation.svg|thumb|right|A rocket's required [[mass ratio]] as a function of [[effective exhaust velocity]] ratio]]

The '''classical rocket equation''', or '''ideal rocket equation''' is a mathematical equation that describes the motion of vehicles that follow the basic principle of a [[rocket]]: a device that can apply acceleration to itself using [[thrust]] by expelling part of its mass with high [[velocity]] and can thereby move due to the [[conservation of momentum]].
It is credited to [[Konstantin Tsiolkovsky]], who independently derived it and published it in 1903,<ref name="here">К. Ціолковскій, Изслѣдованіе мировыхъ пространствъ реактивными приборами, 1903 (available online [http://epizodsspace.airbase.ru/bibl/dorev-knigi/ciolkovskiy/sm.rar here] {{webarchive|url=https://web.archive.org/web/20110815183920/http://epizodsspace.airbase.ru/bibl/dorev-knigi/ciolkovskiy/sm.rar |date=2011-08-15 }} in a [[RAR (file format)|RARed]] PDF)</ref><ref name="ReactiveFlyingMachines">{{Cite web|last=Tsiolkovsky|first=K.|title=Reactive Flying Machines|url=http://epizodsspace.airbase.ru/bibl/inostr-yazyki/tsiolkovskii/tsiolkovskii-nhedy-t2-1954.pdf}}</ref> although it had been independently derived and published by [[William Moore (British mathematician)|William Moore]] in 1810,<ref name="moore1810">{{Cite journal|last=Moore|first=William|date=1810|title=On the Motion of Rockets both in Nonresisting and Resisting Mediums|url=https://www.biodiversitylibrary.org/page/36067032|journal=Journal of Natural Philosophy, Chemistry & the Arts|volume=27|pages=276–285}}</ref> and later published in a separate book in 1813.<ref name="moore">{{Cite book|last=Moore|first=William|url=https://books.google.com/books?id=nrVgAAAAcAAJ|title=A Treatise on the Motion of Rockets: to which is added, an Essay on Naval Gunnery, in theory and practice, etc|date=1813|publisher=G. & S. Robinson|language=en}}</ref> [[Robert Goddard]] also developed it independently in 1912, and [[Hermann Oberth]] derived it independently about 1920.

The maximum change of [[velocity]] of the vehicle, <math>\Delta v</math> (with no external forces acting) is:

<math display="block">\Delta v = v_\text{e} \ln \frac{m_0}{m_f} = I_\text{sp} g_0 \ln \frac{m_0}{m_f},</math>
where:
* <math>v_\text{e}</math> is the [[effective exhaust velocity]];
**<math>I_\text{sp}</math> is the [[specific impulse]] in dimension of time;
**<math>g_0</math> is [[standard gravity]];
* <math>\ln</math> is the [[natural logarithm]] function;
* <math>m_0</math> is the initial total mass, including [[propellant]], a.k.a. wet mass;
* <math>m_f</math> is the final total mass without propellant, a.k.a. dry mass.

Given the effective exhaust velocity determined by the rocket motor's design, the desired delta-v (e.g., [[orbital speed]] or [[escape velocity]]), and a given dry mass <math>m_f</math>, the equation can be solved for the required wet mass <math>m_0</math>:
<math display="block">m_0 = m_f e^{\Delta v / v_\text{e}}.</math> The required propellant mass is then <math display="block">m_0 - m_f = m_f (e^{\Delta v / v_\text{e}} - 1)</math>

The necessary wet mass grows exponentially with the desired delta-v.

== History ==
The equation is named after Russian scientist [[Konstantin Tsiolkovsky]] who independently derived it and published it in his 1903 work.<ref name="here"/><ref name="ReactiveFlyingMachines"/>

The equation had been derived earlier by the British mathematician [[William Moore (British mathematician)|William Moore]] in 1810,<ref name="moore1810"/> and later published in a separate book in 1813.<ref name="moore"/>

American [[Robert Goddard]] independently developed the equation in 1912 when he began his research to improve rocket engines for possible space flight. German engineer [[Hermann Oberth]] independently derived the equation about 1920 as he studied the feasibility of space travel.

While the derivation of the rocket equation is a straightforward [[calculus]] exercise, Tsiolkovsky is honored as being the first to apply it to the question of whether rockets could achieve speeds necessary for [[Spaceflight|space travel]].

== Experiment of the boat==
[[Image:Exp%C3%A9rience_de_Tsiolkovsky.gif|upright=2|thumb|Experiment of the boat by Tsiolkovsky.]]

In order to understand the principle of rocket propulsion, Konstantin Tsiolkovsky proposed the famous experiment of "the boat".{{cn|date=February 2025}} A person is in a boat away from the shore without oars. They want to reach this shore. They notice that the boat is loaded with a certain quantity of stones and have the idea of quickly and repeatedly throwing the stones in succession in the opposite direction. Effectively, the quantity of movement of the stones thrown in one direction corresponds to an equal quantity of movement for the boat in the other direction (ignoring friction / drag).

==Derivation==
===Most popular derivation===
Consider the following system:

[[File:Tsiolkovsky's Theoretical Rocket Diagram.png|thumb|Tsiolkovsky's theoretical rocket from t = 0 to t = delta_t]]

In the following derivation, "the rocket" is taken to mean "the rocket and all of its unexpended propellant".

[[Newton's second law of motion]] relates external forces (<math>\vec{F}_i</math>) to the change in linear momentum of the whole system (including rocket and exhaust) as follows:
<math display="block">\sum_i \vec{F}_i  = \lim_{\Delta t \to 0} \frac{\vec{P}_{\Delta t} - \vec{P}_0}{\Delta t}</math>
where <math>\vec{P}_0</math> is the momentum of the rocket at time <math>t = 0</math>:
<math display="block">\vec{P}_0 = m \vec{V}</math>
and <math>\vec{P}_{\Delta t}</math> is the momentum of the rocket and exhausted mass at time <math>t = \Delta t</math>:
<math display="block">\vec{P}_{\Delta t} = \left(m - \Delta m \right) \left(\vec{V}  + \Delta \vec{V} \right) + \Delta m \vec{V}_\text{e}</math>
and where, with respect to the observer:
* <math>\vec{V}</math> is the velocity of the rocket at time <math>t = 0</math>
* <math>\vec{V} + \Delta \vec{V}</math> is the velocity of the rocket at time <math>t = \Delta t</math>
* <math>\vec{V}_\text{e}</math> is the velocity of the mass added to the exhaust (and lost by the rocket) during time <math>\Delta t</math>
* <math>m</math> is the mass of the rocket at time <math>t = 0</math>
* <math>\left( m - \Delta m \right)</math> is the mass of the rocket at time <math>t = \Delta t</math>

The velocity of the exhaust <math>\vec{V}_\text{e}</math> in the observer frame is related to the velocity of the exhaust in the rocket frame <math>v_\text{e}</math> by:
<math display="block">\vec {v}_\text{e} = \vec{V}_\text{e} - \vec{V} </math>
thus,
<math display="block">\vec {V}_\text{e} = \vec{V} + \vec{v}_\text{e} </math>
Solving this yields:
<math display="block">\vec{P}_{\Delta t} - \vec{P}_0 = m\Delta \vec{V} + \vec{v}_\text{e} \Delta m - \Delta m \Delta \vec{V}</math>
If <math>\vec{V}</math> and <math>\vec{v}_\text{e}</math> are opposite, <math>\vec{F}_\text{i}</math> have the same direction as <math>\vec{V}</math>, <math>\Delta m \Delta \vec{V}</math> are negligible (since <math>dm \, d\vec{v} \to 0</math>), and using <math>dm = -\Delta m</math> (since ejecting a positive <math>\Delta m</math> results in a decrease in rocket mass in time),
<math display="block">\sum_i F_i = m \frac{dV}{dt} + v_\text{e} \frac{dm}{dt}</math>

If there are no external forces then <math display="inline">\sum_i F_i = 0</math> ([[momentum#Conservation|conservation of linear momentum]]) and
<math display="block">-m\frac{dV}{dt} = v_\text{e}\frac{dm}{dt}</math>

Assuming that <math>v_\text{e}</math> is constant (known as [[Tsiolkovsky's hypothesis]]<ref name="ReactiveFlyingMachines" />), so it is not subject to integration, then the above equation may be integrated as follows:
<math display="block">-\int_{V}^{V + \Delta V} \, dV = {v_e} \int_{m_0}^{m_f} \frac{dm}{m} </math>

This then yields
<math display="block">\Delta V = v_\text{e} \ln \frac{m_0}{m_f}</math>
or equivalently
<math display="block">m_f = m_0 e^{-\Delta V\ / v_\text{e}}</math> or
<math display="block">m_0 = m_f e^{\Delta V / v_\text{e}}</math> or
<math display="block">m_0 - m_f = m_f \left(e^{\Delta V / v_\text{e}} - 1\right)</math>
where <math>m_0</math> is the initial total mass including propellant, <math>m_f</math>  the final mass, and <math>v_\text{e}</math> the velocity of the rocket exhaust with respect to the rocket (the [[specific impulse]], or, if measured in time, that multiplied by [[gravity]]-on-Earth acceleration). If <math>v_\text{e}</math> is NOT constant, we might not have rocket equations that are as simple as the above forms. Many rocket dynamics researches were based on the Tsiolkovsky's constant <math>v_\text{e}</math> hypothesis.

The value <math>m_0 - m_f</math> is the total [[working mass]] of propellant expended.

<math>\Delta V</math> ([[delta-v]]) is the integration over time of the magnitude of the acceleration produced by using the rocket engine (what would be the actual acceleration if external forces were absent). In free space, for the case of acceleration in the direction of the velocity, this is the increase of the speed. In the case of an acceleration in opposite direction (deceleration) it is the decrease of the speed. Of course gravity and drag also accelerate the vehicle, and they can add or subtract to the change in velocity experienced by the vehicle. Hence delta-v may not always be the actual change in speed or velocity of the vehicle.

===Other derivations===

====Impulse-based====
The equation can also be derived from the basic integral of acceleration in the form of force (thrust) over mass.
By representing the delta-v equation as the following:
<math display="block">\Delta v = \int^{t_f}_{t_0} \frac{|T|}{{m_0}-{t} \Delta{m}} ~ dt</math>

where T is thrust, <math>m_0</math> is the initial (wet) mass and <math>\Delta m</math> is the initial mass minus the final (dry) mass,

and realising that the integral of a resultant force over time is total impulse, assuming thrust is the only force involved,
<math display="block">\int^{t_f}_{t_0} F ~ dt = J</math>

The integral is found to be:
<math display="block">J ~ \frac{\ln({m_0}) - \ln({m_f})}{\Delta m}</math>

Realising that impulse over the change in mass is equivalent to force over propellant mass flow rate (p), which is itself equivalent to exhaust velocity,
<math display="block"> \frac{J}{\Delta m} = \frac{F}{p} = V_\text{exh}</math>
the integral can be equated to
<math display="block">\Delta v = V_\text{exh} ~ \ln\left({\frac{m_0}{m_f}}\right)</math>

====Acceleration-based====
Imagine a rocket at rest in space with no forces exerted on it ([[Newton's laws of motion|Newton's first law of motion]]). From the moment its engine is started (clock set to 0) the rocket expels gas mass at a ''constant mass flow rate R'' (kg/s) and at ''exhaust velocity relative to the rocket v<sub>e</sub>'' (m/s). This creates a constant force ''F'' propelling the rocket that is equal to ''R'' × ''v<sub>e</sub>''. The rocket is subject to a constant force, but its total mass is decreasing steadily because it is expelling gas. According to [[Newton's laws of motion|Newton's second law of motion]], its acceleration at any time ''t'' is its propelling force ''F'' divided by its current mass ''m'':
<math display="block"> ~ a = \frac{dv}{dt} = - \frac{F}{m(t)} = - \frac{R v_\text{e}}{m(t)}</math>

Now, the mass of fuel the rocket initially has on board is equal to ''m''<sub>0</sub> – ''m<sub>f</sub>''. For the constant mass flow rate ''R'' it will therefore take a time ''T'' = (''m''<sub>0</sub> – ''m<sub>f</sub>'')/''R'' to burn all this fuel. Integrating both sides of the equation with respect to time from ''0'' to ''T'' (and noting that ''R = dm/dt'' allows a substitution on the right) obtains: 
<math display="block"> ~ \Delta v = v_f - v_0 = - v_\text{e} \left[ \ln m_f - \ln m_0 \right] = ~ v_\text{e}  \ln\left(\frac{m_0}{m_f}\right).</math>

==== Limit of finite mass "pellet" expulsion ====
The rocket equation can also be derived as the limiting case of the speed change for a rocket that expels its fuel in the form of <math>N</math> pellets consecutively, as <math>N \to \infty</math>, with an effective exhaust speed <math>v_\text{eff}</math> such that the mechanical energy gained per unit fuel mass is given by <math display="inline">\tfrac{1}{2} v_\text{eff}^2 </math>.

In the rocket's center-of-mass frame, if a pellet of mass <math>m_p</math> is ejected at speed <math>u</math> and the remaining mass of the rocket is <math>m</math>, the amount of energy converted to increase the rocket's and pellet's kinetic energy is
<math display="block">\tfrac{1}{2} m_p v_\text{eff}^2 = \tfrac{1}{2}m_p u^2 + \tfrac{1}{2}m (\Delta v)^2. </math>

Using momentum conservation in the rocket's frame just prior to ejection, <math display="inline"> u = \Delta v \tfrac{m}{m_p}</math>, from which we find 
<math display="block">\Delta v = v_\text{eff} \frac{m_p}{\sqrt{m(m+m_p)}}.</math>

Let <math>\phi</math> be the initial fuel mass fraction on board and <math> m_0</math> the initial fueled-up mass of the rocket. Divide the total mass of fuel <math>\phi m_0</math> into <math>N</math> discrete pellets each of mass <math>m_p = \phi m_0/N</math>. The remaining mass of the rocket after ejecting <math>j</math> pellets is then <math>m = m_0(1 - j\phi/N)</math>. The overall speed change after ejecting <math>j</math> pellets is the sum
<ref name="discreteproof">{{cite journal |last1=Blanco |first1=Philip |title=A discrete, energetic approach to rocket propulsion|journal=Physics Education |date=November 2019 |volume=54|issue=6 |pages=065001 |doi=10.1088/1361-6552/ab315b|bibcode=2019PhyEd..54f5001B |s2cid=202130640 }}</ref>
<math display="block"> \Delta v = v_\text{eff} \sum ^{j=N}_{j=1} \frac{\phi/N}{\sqrt{(1-j\phi/N)(1-j\phi/N+\phi/N)}} </math>

Notice that for large <math>N</math> the last term in the denominator <math>\phi/N\ll 1</math> and can be neglected to give
<math display="block"> \Delta v \approx v_\text{eff} \sum^{j=N}_{j=1}\frac{\phi/N}{1-j\phi/N} = v_\text{eff} \sum ^{j=N}_{j=1} \frac{\Delta x}{1-x_j} </math> where <math display="inline"> \Delta x = \frac{\phi}{N}</math> and <math display="inline"> x_j = \frac{j\phi}{N} </math>.

As <math> N\rightarrow \infty</math> this [[Riemann sum]] becomes the definite integral
<math display="block"> \lim_{N\to\infty}\Delta v = v_\text{eff} \int_{0}^{\phi} \frac{dx}{1-x} = v_\text{eff}\ln \frac{1}{1-\phi} = v_\text{eff} \ln \frac{m_0}{m_f} ,</math> since the final remaining mass of the rocket is <math> m_f = m_0(1-\phi)</math>.

===Special relativity===

If [[special relativity]] is taken into account, the following equation can be derived for a [[relativistic rocket]],<ref>Forward, Robert L. [https://web.archive.org/web/20240116083227/http://www.relativitycalculator.com/images/rocket_equations/AIAA.pdf "A Transparent Derivation of the Relativistic Rocket Equation"] (see the right side of equation 15 on the last page, with ''R'' as the ratio of initial to final mass and w as the exhaust velocity, corresponding to ''v''<sub>e</sub> in the notation of this article)</ref> with <math>\Delta v</math> again standing for the rocket's final velocity (after expelling all its reaction mass and being reduced to a rest mass of <math>m_1</math>) in the [[inertial frame of reference]] where the rocket started at rest (with the rest mass including fuel being <math>m_0</math> initially), and <math>c</math> standing for the [[speed of light]] in vacuum:
<math display="block">\frac{m_0}{m_1} = \left[\frac{1 + {\frac{\Delta v}{c}}}{1 - {\frac{\Delta v}{c}}}\right]^{\frac{c}{2v_\text{e}}}</math>

Writing <math display="inline">\frac{m_0}{m_1}</math> as <math>R</math> allows this equation to be rearranged as
<math display="block">\frac{\Delta v}{c} = \frac{R^{\frac{2v_\text{e}}{c}} - 1}{R^{\frac{2v_\text{e}}{c}} + 1}</math>

Then, using the [[identity (mathematics)|identity]] <math display="inline">R^{\frac{2v_\text{e}}{c}} = \exp \left[ \frac{2v_\text{e}}{c} \ln R \right]</math> (here "exp" denotes the [[exponential function]]; ''see also'' [[Natural logarithm]] as well as the "power" identity at [[Logarithm#Product, quotient, power, and root|logarithmic identities]]) and the identity <math display="inline">\tanh x = \frac{e^{2x} - 1} {e^{2x} + 1}</math> (''see'' [[Hyperbolic function]]), this is equivalent to
<math display="block">\Delta v = c \tanh\left(\frac {v_\text{e}}{c} \ln \frac{m_0}{m_1} \right)</math>

==Terms of the equation==

===Delta-''v''===
{{main article|Delta-v}}
Delta-''v'' (literally "[[Delta (letter)#Upper case|change]] in [[velocity]]"), symbolised as '''Δ''v''''' and pronounced ''delta-vee'', as used in [[flight dynamics (spacecraft)|spacecraft flight dynamics]], is a measure of the [[impulse (physics)|impulse]] that is needed to perform a maneuver such as launching from, or landing on a planet or moon, or an in-space [[orbital maneuver]]. It is a [[scalar (mathematics)|scalar]] that has the units of [[speed]]. As used in this context, it is ''not'' the same as the [[delta-v (physics)|physical change in velocity]] of the vehicle.

Delta-''v'' is produced by reaction engines, such as [[rocket engines]], is proportional to the [[thrust]] per unit mass and burn time, and is used to determine the mass  of [[rocket propellant|propellant]] required for the given manoeuvre through the rocket equation.

For multiple manoeuvres, delta-''v'' sums linearly.

For interplanetary missions delta-''v'' is often plotted on a [[porkchop plot]] which displays the required mission delta-''v'' as a function of launch date.

===Mass fraction===
{{main article|Propellant mass fraction}}
In [[aerospace engineering]], the propellant mass fraction is the portion of a vehicle's mass which does not reach the destination, usually used as a measure of the vehicle's performance. In other words, the propellant mass fraction is the ratio between the propellant mass and the initial mass of the vehicle. In a spacecraft, the destination is usually an orbit, while for aircraft it is their landing location. A higher mass fraction represents less weight in a design.  Another related measure is the [[payload fraction]], which is the fraction of initial weight that is payload.

===Effective exhaust velocity===
{{main article|Effective exhaust velocity}}
The effective exhaust velocity is often specified as a [[specific impulse]] and they are related to each other by:
<math display="block">v_\text{e} = g_0 I_\text{sp},</math>
where
*<math>I_\text{sp}</math> is the specific impulse in seconds,
*<math>v_\text{e}</math> is the specific impulse measured in [[metre per second|m/s]], which is the same as the effective exhaust velocity measured in m/s (or ft/s if g is in ft/s<sup>2</sup>),
*<math>g_0</math> is the [[standard gravity]], 9.80665{{nbsp}}m/s<sup>2</sup> (in [[Imperial units]] 32.174{{nbsp}}ft/s<sup>2</sup>).

==Applicability==
The rocket equation captures the essentials of rocket flight physics in a single short equation. It also holds true for rocket-like reaction vehicles whenever the effective exhaust velocity is constant, and can be summed or integrated when the effective exhaust velocity varies. The rocket equation only accounts for the reaction force from the rocket engine; it does not include other forces that may act on a rocket, such as [[aerodynamic force|aerodynamic]] or [[gravitation]]al forces. As such, when using it to calculate the propellant requirement for launch from (or powered descent to) a planet with an atmosphere, the effects of these forces must be included in the delta-V requirement (see Examples below). In what has been called "the tyranny of the rocket equation", there is a limit to the amount of [[Payload fraction|payload]] that the rocket can carry, as higher amounts of propellant increment the overall weight, and thus also increase the fuel consumption.<ref>{{Cite web|url=http://www.nasa.gov/mission_pages/station/expeditions/expedition30/tryanny.html|title=The Tyranny of the Rocket Equation|website=[[NASA.gov]] |language=en|access-date=2016-04-18|archive-url=https://web.archive.org/web/20220306084046/https://www.nasa.gov/mission_pages/station/expeditions/expedition30/tryanny.html|archive-date=2022-03-06}}</ref> The equation does not apply to [[Non-rocket spacelaunch|non-rocket systems]] such as [[aerobraking]], [[Space gun|gun launch]]es, [[space elevator]]s, [[launch loop]]s, [[tether propulsion]] or [[Solar sail|light sails]].

The rocket equation can be applied to [[orbital maneuver]]s in order to determine how much propellant is needed to change to a particular new orbit, or to find the new orbit as the result of a particular propellant burn. When applying to orbital maneuvers, one assumes an [[Orbital maneuver#Impulsive maneuvers|impulsive maneuver]], in which the propellant is discharged and delta-v applied instantaneously. This assumption is relatively accurate for short-duration burns such as for mid-course corrections and orbital insertion maneuvers. As the burn duration increases, the result is less accurate due to the effect of gravity on the vehicle over the duration of the maneuver. For low-thrust, long duration propulsion, such as [[Electrically powered spacecraft propulsion|electric propulsion]], more complicated analysis based on the propagation of the spacecraft's state vector and the integration of thrust are used to predict orbital motion.

==Examples==
Assume an exhaust velocity of {{convert|4500|m/s|ft/s|sp=us}} and a <math>\Delta v</math> of {{convert|9700|m/s|ft/s|sp=us}} (Earth to [[low Earth orbit|LEO]], including <math>\Delta v</math> to overcome gravity and aerodynamic drag).

*[[Single-stage-to-orbit]] rocket: <math>1-e^{-9.7/4.5}</math> = 0.884, therefore 88.4% of the initial total mass has to be propellant. The remaining 11.6% is for the engines, the tank, and the payload.
*[[Two-stage-to-orbit]]: suppose that the first stage should provide a <math>\Delta v</math> of {{convert|5000|m/s|ft/s|sp=us}}; <math>1-e^{-5.0/4.5}</math> = 0.671, therefore 67.1% of the initial total mass has to be propellant to the first stage. The remaining mass is 32.9%. After disposing of the first stage, a mass remains equal to this 32.9%, minus the mass of the tank and engines of the first stage. Assume that this is 8% of the initial total mass, then 24.9% remains. The second stage should provide a <math>\Delta v</math> of {{convert|4700|m/s|ft/s|sp=us}}; <math>1-e^{-4.7/4.5}</math> = 0.648, therefore 64.8% of the remaining mass has to be propellant, which is 16.2% of the original total mass, and 8.7% remains for the tank and engines of the second stage, the payload, and in the case of a space shuttle, also the orbiter. Thus together 16.7% of the original launch mass is available for ''all'' engines, the tanks, and payload.

==Stages==
In the case of sequentially thrusting [[staging (rocketry)|rocket stages]], the equation applies for each stage, where for each stage the initial mass in the equation is the total mass of the rocket after discarding the previous stage, and the final mass in the equation is the total mass of the rocket just before discarding the stage concerned. For each stage the specific impulse may be different.

For example, if 80% of the mass of a rocket is the fuel of the first stage, and 10% is the dry mass of the first stage, and 10% is the remaining rocket, then

<math display="block">
\begin{align}
\Delta v \ & = v_\text{e} \ln { 100 \over 100 - 80 }\\
           & = v_\text{e} \ln 5 \\
           & = 1.61 v_\text{e}. \\
\end{align}
</math>

With three similar, subsequently smaller stages with the same <math>v_\text{e}</math> for each stage, gives:

<math display="block">\Delta v \ = 3 v_\text{e} \ln 5 \ = 4.83 v_\text{e} </math>

and the payload is 10% × 10% × 10% = 0.1% of the initial mass.

A comparable [[Single-stage-to-orbit|SSTO]] rocket, also with a 0.1% payload, could have a mass of 11.1% for fuel tanks and engines, and 88.8% for fuel. This would give

<math display="block">\Delta v \ = v_\text{e} \ln(100/11.2) \ = 2.19 v_\text{e}. </math>

If the motor of a new stage is ignited before the previous stage has been discarded and the simultaneously working motors have a different specific impulse (as is often the case with solid rocket boosters and a liquid-fuel stage), the situation is more complicated.

==See also==
{{Portal| Spaceflight }}
* [[Delta-v budget]]
* [[Jeep problem]]
* [[Mass ratio]]
* [[Oberth effect]] - applying delta-v in a [[gravity well]] increases the final velocity
* [[Relativistic rocket]]
* [[Reversibility of orbits]]
* [[Robert H. Goddard]] - added terms for gravity and drag in vertical flight
* [[Spacecraft propulsion]]
* [[Stigler’s law of eponymy]]

==References==
{{Reflist}}

==External links==
*[http://ed-thelen.org/rocket-eq.html How to derive the rocket equation]
*[http://www.relativitycalculator.com/rocket_equations.shtml Relativity Calculator – Learn Tsiolkovsky's rocket equations]
*[http://www.wolframalpha.com/input/?i=Tsiolkovsky+rocket+equation Tsiolkovsky's rocket equations plot and calculator in WolframAlpha]

{{Orbits}}

{{DEFAULTSORT:Tsiolkovsky Rocket Equation}}
[[Category:Astrodynamics]]
[[Category:Eponymous equations of physics]]
[[Category:Konstantin Tsiolkovsky|Rocket Equation]]
[[Category:Single-stage-to-orbit]]
[[Category:Rocket propulsion]]