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[[File:Soyuz TMA-18 launching.jpg|thumb|150px|[[Rockets]], which lose significant amounts of mass as fuel during flight, are an example of a variable-mass system.]]
 
In [[mechanics]], a '''variable-mass system''' is a collection of [[matter]] whose [[mass]] varies with [[time]]. [[Newton's second law]] of motion cannot directly be applied to such a system because it is valid for constant mass systems only.<ref name="Plastino">{{cite journal|last=Plastino|first=Angel R.|coauthors=Muzzio, Juan C.|year=1992|title=On the use and abuse of Newton's second law for variable mass problems|journal=Celestial Mechanics and Dynamical Astronomy|publisher=Kluwer Academic Publishers|location=Netherlands|volume=53|issue=3|pages=227–232|issn=0923-2958|doi=10.1007/BF00052611|bibcode=1992CeMDA..53..227P|url=http://articles.adsabs.harvard.edu/full/seri/CeMDA/0053//0000227.000.html|accessdate=2011-12-30}}</ref><ref name="Basavaraju">{{cite book|last1=Basavaraju|first1=G|last2=Ghosh|first2=Dipin|title=Mechanics and Thermodynamics|date=1985-02-01|publisher=[[Tata McGraw-Hill]]|isbn=978-0-07-451537-2|pages=162–165}}</ref> Instead, the time dependence of the mass ''m'' can be calculated by rearranging Newton's second law and adding a term to account for the [[momentum]] carried by mass entering or leaving the system. The general equation of variable-mass motion is written as
 
:<math>\mathbf{F}_{\mathrm{ext}} + \mathbf{v}_{\mathrm{rel}}\frac{\mathrm{d} m}{\mathrm{d}t} = m {\mathrm{d} \mathbf v \over \mathrm{d}t}</math>
 
where '''F'''<sub>ext</sub> is the [[net force|net external force]] on the body, '''v'''<sub>rel</sub> is the [[relative velocity]] of the escaping or incoming mass with respect to the [[center of mass]] of the body, and '''v''' is the [[velocity]] of the body.<ref name="Plastino" />  In [[astrodynamics]], which deals with the mechanics of [[rocket]]s, the term ''v''<sub>rel</sub> is often called the [[effective exhaust velocity]] and denoted ''v''<sub>''e''</sub>.<ref name="NASA">{{cite web|url=http://microgravity.grc.nasa.gov/education/rocket/rktpow.html|title=Ideal Rocket Equation|last=Benson|first=Tom|publisher=[[NASA]]|accessdate=30 December 2011}}</ref>
 
== Derivation ==
There are different derivations for the variable-mass system motion equation, depending on whether is mass is entering or leaving a body (in other words, whether the moving body's mass is increasing or decreasing). To simplify calculations, all bodies are considered as [[particle]]s.
 
=== Mass accretion ===
[[File:Variable-mass system derivation.svg|thumb|300px|At instant 1, a mass d''m'' with relative velocity '''u''' is about to collide with the main body of mass ''m'' and velocity '''v'''.  After a time d''t'', at instant 2, both particles move as one body with velocity '''v'''&nbsp;+&nbsp;d'''v'''.]]
The following derivation is for a body that is gaining mass ([[Accretion (astrophysics)|accretion]]).  Let a body of time-varying mass ''m'' moves at a velocity '''v''' at an initial time ''t''.  Meanwhile, at this instant, let a particle of mass dm moves with velocity '''u'''.  The initial [[momentum]] can be written as<ref name="Cveticanin">{{cite book|last=Cveticanin|first=L|title=Dynamics of Machines with Variable Mass|edition=1|date=1998-10-21|publisher=[[CRC Press]]|isbn=978-90-5699-096-1|pages=15–20|accessdate=2011-12-25}}</ref>
 
:<math>\mathbf{p}_{\mathrm{1}} = m\mathbf{v} + \mathbf{u}\mathrm{d}m</math>
 
Now at a time ''t'' + d''t'', let both the main body and the particle accrete into a body of velocity '''v''' + d'''v'''.  Thus the new momentum of the system can be written as
 
:<math>\mathbf{p}_{\mathrm{2}} = (m + \mathrm{d}m)(\mathbf{v} + \mathrm{d}\mathbf{v}) = m\mathbf{v} + m\mathrm{d}\mathbf{v} + \mathbf{v}\mathrm{d}m + \mathrm{d}m\mathrm{d}\mathbf{v}</math>
 
Since d''m''d'''v''' is the product of two small values, it can be ignored, meaning during d''t'' the momentum of the system varies for
 
:<math>\mathrm{d}\mathbf{p} = \mathbf{p}_{\mathrm{2}} - \mathbf{p}_{\mathrm{1}} = (m\mathbf{v} + m\mathrm{d}\mathbf{v} + \mathbf{v}\mathrm{d}m) - (m\mathbf{v} + \mathbf{u}\mathrm{d}m) = m\mathrm{d}\mathbf{v} - (\mathbf{u} - \mathbf{v})\mathrm{d}m</math>
 
Therefore, by [[Newton's second law]]
 
:<math>\mathbf{F}_{\mathrm{net}} = \frac{\mathrm{d}\mathbf{p}}{\mathrm{d}t} = \frac{m\mathrm{d}\mathbf{v} - (\mathbf{u} - \mathbf{v})\mathrm{d}m}{\mathrm{d}t} = m\frac{\mathrm{d}\mathbf{v}}{\mathrm{d}t} - (\mathbf{u} - \mathbf{v})\frac{\mathrm{d}m}{\mathrm{d}t}</math>
 
Noting that '''u''' - '''v''' is the velocity of d''m'' [[relative velocity|relative]] to ''m'', symbolized as '''v'''<sub>rel</sub>, this final equation can be arranged as<ref name="Giancoli">{{cite book|last=Giancoli|first=Douglas C.|title=Physics for Scientists & Engineers|edition=4, illustrated|volume=2|year=2008|publisher=Pearson Education|isbn=978-0-13-227359-6|pages=236–238}}</ref>
 
:<math>\mathbf{F}_{\mathrm{ext}} + \mathbf{v}_{\mathrm{rel}}\frac{\mathrm{d} m}{\mathrm{d}t} = m {\mathrm{d} \mathbf v \over \mathrm{d}t}</math>
 
=== Mass ablation/ejection ===
 
In a system where mass is being ejected or [[ablation|ablated]] from a main body, the derivation is slightly different.  At time ''t'', let a mass ''m'' travel at a velocity '''v''', meaning the initial momentum of the system is
 
:<math>\mathbf{p}_{\mathrm{1}} = m\mathbf{v}</math>
 
Since the main body will be losing mass, d''m'' will be negative, meaning that at a time ''t'' + d''t'' the momentum of the system becomes
 
:<math>\mathbf{p}_{\mathrm{2}} = (m + \mathrm{d}m)(\mathbf{v} + \mathrm{d}\mathbf{v}) + \mathbf{u}(-\mathrm{d}m) = m\mathbf{v} + m\mathrm{d}\mathbf{v} + \mathbf{v}\mathrm{d}m + \mathrm{d}m\mathrm{d}\mathbf{v} - \mathbf{u}\mathrm{d}m</math>
 
where '''u''' is the velocity of the ejected mass.  Thus during d''t'' the momentum of the system varies for
 
:<math>\mathrm{d}\mathbf{p} = \mathbf{p}_{\mathrm{2}} - \mathbf{p}_{\mathrm{1}} = (m\mathbf{v} + m\mathrm{d}\mathbf{v} + \mathbf{v}\mathrm{d}m - \mathbf{u}\mathrm{d}m) - (m\mathbf{v}) = m\mathrm{d}\mathbf{v} - (\mathbf{u} - \mathbf{v})\mathrm{d}m</math>
 
This is the same d'''p''' as found in the mass accretion case above, meaning that the same conclusion holds.<ref name="Cveticanin" />
 
== Forms ==
[[File:Inflated rocket balloon.jpg|thumb|100px|When released, this rocket [[toy balloon|balloon]] ejects a significant amount of its mass as air, causing a large acceleration.]]
By the definition of [[acceleration]], '''a''' = d'''v'''/d''t'', so the variable-mass system motion equation can be written as
 
:<math>\mathbf{F}_{\mathrm{ext}} + \mathbf{v}_{\mathrm{rel}}\frac{\mathrm{d}m}{\mathrm{d}t} = m\mathbf{a}</math>
 
In bodies that are not treated as particles '''a''' must be replaced by '''a'''<sub>cm</sub>, the acceleration of the [[center of mass]] of the system, meaning
 
:<math>\mathbf{F}_{\mathrm{ext}} + \mathbf{v}_{\mathrm{rel}}\frac{\mathrm{d}m}{\mathrm{d}t} = m\mathbf{a}_{\mathrm{cm}}</math>
 
Often the force due to [[thrust]] is defined as <math>\mathbf{F}_{\mathrm{thrust}} = \mathbf{v}_{\mathrm{rel}}\frac{\mathrm{d}m}{\mathrm{d}t}</math> so that
 
:<math>\mathbf{F}_{\mathrm{ext}} + \mathbf{F}_{\mathrm{thrust}} = m\mathbf{a}_{\mathrm{cm}}</math>
 
This form shows that a body can have acceleration due to thrust even if no external forces act on it ('''F'''<sub>ext</sub> = 0).  Note finally that if one lets '''F'''<sub>net</sub> be the sum of '''F'''<sub>ext</sub> and '''F'''<sub>thrust</sub> then the equation regains the usual form of Newton's second law:
 
:<math>\mathbf{F}_{\mathrm{net}} = m\mathbf{a}_{\mathrm{cm}}</math>
 
=== Ideal rocket equation ===
[[File:Rocket mass ratio versus delta-v.svg|thumb|right|Rocket [[mass ratio]]s versus final velocity calculated from the rocket equation]]
{{main|Tsiolkovsky rocket equation}}
The [[Tsiolkovsky rocket equation|ideal rocket equation]], or the [[Konstantin Tsiolkovsky|Tsiolkovsky]] rocket equation, can be used to study the motion of vehicles that behave like a [[rocket]] (where a body accelerates itself by ejecting part of its mass, a [[propellant]], with high speed). It can be derived from the general equation of motion for variable-mass systems as follows: when no external forces act on a body ('''F'''<sub>ext</sub> = 0) the variable-mass system motion equation reduces to<ref name="Basavaraju" />
 
:<math>\mathbf{v}_{\mathrm{rel}}\frac{\mathrm{d}m}{\mathrm{d}t}= m \frac{\mathrm{d}\mathbf{v}}{\mathrm{d}t}</math>
 
If the velocity of the ejected propellant, '''v'''<sub>rel</sub>, is assumed have the opposite direction as the rocket's acceleration, d'''v'''/d''t'', the [[scalar (mathematics)|scalar]] equivalent of this equation can be written as
:<math>-v_{\mathrm{rel}}\frac{\mathrm{d}m}{\mathrm{d}t} = m{\mathrm{d} v \over \mathrm{d}t}</math>
 
from which d''t'' can be canceled out to give
 
:<math>-v_{\mathrm{rel}}\mathrm{d}m = m\mathrm{d}v \,</math>
 
Integration by [[separation of variables]] gives
 
:<math>-v_\mathrm{rel}\int_{m_0}^{m_1} \frac{\mathrm{d}m}{m} = \int_{v_0}^{v_1} \mathrm{d}v</math>
 
:<math>v_\mathrm{rel}\ln{\frac{m_0}{m_1}} = v_1 - v_0</math>
 
By rearranging and letting Δ''v'' = ''v''<sub>1</sub> - ''v''<sub>0</sub>, one arrives at the standard form of the ideal rocket equation:
 
:<math>\Delta v = v_\mathrm{rel} \ln \frac {m_0} {m_1}</math>
 
where ''m''<sub>0</sub> is the initial total mass, including propellant, ''m''<sub>1</sub> is the final total mass, ''v''<sub>rel</sub> is the [[effective exhaust velocity]] (often denoted as ''v''<sub>''e''</sub>), and Δ''v'' is the maximum change of speed of the vehicle (when no external forces are acting).
 
== References ==
{{reflist|colwidth=33em}}
 
[[Category:Classical mechanics]]
[[Category:Mechanics]]

Revision as of 14:02, 9 August 2013

Rockets, which lose significant amounts of mass as fuel during flight, are an example of a variable-mass system.

In mechanics, a variable-mass system is a collection of matter whose mass varies with time. Newton's second law of motion cannot directly be applied to such a system because it is valid for constant mass systems only.[1][2] Instead, the time dependence of the mass m can be calculated by rearranging Newton's second law and adding a term to account for the momentum carried by mass entering or leaving the system. The general equation of variable-mass motion is written as

𝐅ext+𝐯reldmdt=md𝐯dt

where Fext is the net external force on the body, vrel is the relative velocity of the escaping or incoming mass with respect to the center of mass of the body, and v is the velocity of the body.[1] In astrodynamics, which deals with the mechanics of rockets, the term vrel is often called the effective exhaust velocity and denoted ve.[3]

Derivation

There are different derivations for the variable-mass system motion equation, depending on whether is mass is entering or leaving a body (in other words, whether the moving body's mass is increasing or decreasing). To simplify calculations, all bodies are considered as particles.

Mass accretion

At instant 1, a mass dm with relative velocity u is about to collide with the main body of mass m and velocity v. After a time dt, at instant 2, both particles move as one body with velocity v + dv.

The following derivation is for a body that is gaining mass (accretion). Let a body of time-varying mass m moves at a velocity v at an initial time t. Meanwhile, at this instant, let a particle of mass dm moves with velocity u. The initial momentum can be written as[4]

𝐩1=m𝐯+𝐮dm

Now at a time t + dt, let both the main body and the particle accrete into a body of velocity v + dv. Thus the new momentum of the system can be written as

𝐩2=(m+dm)(𝐯+d𝐯)=m𝐯+md𝐯+𝐯dm+dmd𝐯

Since dmdv is the product of two small values, it can be ignored, meaning during dt the momentum of the system varies for

d𝐩=𝐩2𝐩1=(m𝐯+md𝐯+𝐯dm)(m𝐯+𝐮dm)=md𝐯(𝐮𝐯)dm

Therefore, by Newton's second law

𝐅net=d𝐩dt=md𝐯(𝐮𝐯)dmdt=md𝐯dt(𝐮𝐯)dmdt

Noting that u - v is the velocity of dm relative to m, symbolized as vrel, this final equation can be arranged as[5]

𝐅ext+𝐯reldmdt=md𝐯dt

Mass ablation/ejection

In a system where mass is being ejected or ablated from a main body, the derivation is slightly different. At time t, let a mass m travel at a velocity v, meaning the initial momentum of the system is

𝐩1=m𝐯

Since the main body will be losing mass, dm will be negative, meaning that at a time t + dt the momentum of the system becomes

𝐩2=(m+dm)(𝐯+d𝐯)+𝐮(dm)=m𝐯+md𝐯+𝐯dm+dmd𝐯𝐮dm

where u is the velocity of the ejected mass. Thus during dt the momentum of the system varies for

d𝐩=𝐩2𝐩1=(m𝐯+md𝐯+𝐯dm𝐮dm)(m𝐯)=md𝐯(𝐮𝐯)dm

This is the same dp as found in the mass accretion case above, meaning that the same conclusion holds.[4]

Forms

When released, this rocket balloon ejects a significant amount of its mass as air, causing a large acceleration.

By the definition of acceleration, a = dv/dt, so the variable-mass system motion equation can be written as

𝐅ext+𝐯reldmdt=m𝐚

In bodies that are not treated as particles a must be replaced by acm, the acceleration of the center of mass of the system, meaning

𝐅ext+𝐯reldmdt=m𝐚cm

Often the force due to thrust is defined as 𝐅thrust=𝐯reldmdt so that

𝐅ext+𝐅thrust=m𝐚cm

This form shows that a body can have acceleration due to thrust even if no external forces act on it (Fext = 0). Note finally that if one lets Fnet be the sum of Fext and Fthrust then the equation regains the usual form of Newton's second law:

𝐅net=m𝐚cm

Ideal rocket equation

Rocket mass ratios versus final velocity calculated from the rocket equation

Mining Engineer (Excluding Oil ) Truman from Alma, loves to spend time knotting, largest property developers in singapore developers in singapore and stamp collecting. Recently had a family visit to Urnes Stave Church. The ideal rocket equation, or the Tsiolkovsky rocket equation, can be used to study the motion of vehicles that behave like a rocket (where a body accelerates itself by ejecting part of its mass, a propellant, with high speed). It can be derived from the general equation of motion for variable-mass systems as follows: when no external forces act on a body (Fext = 0) the variable-mass system motion equation reduces to[2]

𝐯reldmdt=md𝐯dt

If the velocity of the ejected propellant, vrel, is assumed have the opposite direction as the rocket's acceleration, dv/dt, the scalar equivalent of this equation can be written as

vreldmdt=mdvdt

from which dt can be canceled out to give

vreldm=mdv

Integration by separation of variables gives

vrelm0m1dmm=v0v1dv
vrellnm0m1=v1v0

By rearranging and letting Δv = v1 - v0, one arrives at the standard form of the ideal rocket equation:

Δv=vrellnm0m1

where m0 is the initial total mass, including propellant, m1 is the final total mass, vrel is the effective exhaust velocity (often denoted as ve), and Δv is the maximum change of speed of the vehicle (when no external forces are acting).

References

43 year old Petroleum Engineer Harry from Deep River, usually spends time with hobbies and interests like renting movies, property developers in singapore new condominium and vehicle racing. Constantly enjoys going to destinations like Camino Real de Tierra Adentro.

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