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Thrust into Space Maxwell W. Hunter, II
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Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Dec 16, 2015

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Page 1: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Thrust into SpaceMaxwell W. Hunter, II

Page 2: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Newton’s 3rd Law of Motion

•Momentum is conserved, equation 1-1

mGVG =mBVB

Page 3: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Force

• Force, equation 1-2

•Weight, equation 1-3

F =ma

w =mg0

Page 4: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Energy

• Kinetic energy, equation 1-4

•Ratio of kinetic energy of gun to bullet, equation 1-5

KE =mV2

2=

wV2

2g0

KEG

KEB

=VG

VB

=wB

wG

Page 5: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Guns as Rockets

• Paris Gun, WW I

•Change in velocity, equation 1-6

ΔV = ve 1−wF

wI

⎝⎜⎞

⎠⎟

Page 6: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Rocket Engines

• Thrust, equation 1-7

T =

&wve

g0

+ pe−pat( )Ae

Page 7: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Rocket Nomenclature

• Figure 1-1

Page 8: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Fuel Consumption

• Specific impulse of engine, equation 1-8

• Effective exhaust velocity, equation 1-9

I sp =

T&w

vef =g0I sp

Page 9: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Power

• Power expended, equation 1-10

• Effective power, equation 1-11

Pe =

&wve2

2g0

Pef =

&wvef2

2g0

=Tvef

2=

g0I spT2

Page 10: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Internal Energy Release

• Exit velocity, equation 1-12

•Combustion temperature, equation 1-13

• Velocity of molecule, equation 1-14

ve = 2g0J h=224 h

Tco :

MV 2

2

V :

2Tco

M

Page 11: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Rocket Energy Efficiency

• Figure 1-2

Page 12: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Nozzle Altitude Effect

• Figure 1-3

Page 13: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Nozzle Altitude Performance

• Figure 1-4

Page 14: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Pump Power

• Pump power, equation 1-15

• Pump power for both propellants, equation 1-16

Ppu =

144Δp&wρ

Ppu =144ΔpTρI sp

Page 15: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Rocket Equation

•Change in velocity, equation 1-17

• Impulsive velocity, equation 1-18

ΔV = vef lnwI

wF

⎝⎜⎞

⎠⎟= g0I sp ln

wI

wF

⎝⎜⎞

⎠⎟

ΔV = ′λ vet lnwI

wF

⎝⎜⎞

⎠⎟

Page 16: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Rocket Equation

• Figure 1-5

Page 17: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Useful Load

•Useful load, equation 1-19 wI =wUL +

wpr

′λ

Page 18: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Rocket Equation

• Figure 1-6

Page 19: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Energy Efficiency

• Kinetic energy of useful load, equation 1-20

• Total energy expended by exhaust, equation 1-21

KEUL =wULΔV2

2g0

KEet =wprvet

2

2g0

Page 20: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

External Energy Efficiency

• Figure 1-7

Page 21: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Effect of Initial Velocity

• Increase of kinetic energy of useful load, equation 1-22

• Total kinetic energy expended, equation 1-23

KEUL =wUL VF

2 −VI2( )

2g0

=wUL ΔV2 +2ΔVVI( )

2g0

KEet =wpr vet

2 +VI2( )

2g0

Page 22: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

External Energy Efficiency

• Figure 1-8

Page 23: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Ballistics

• Flat earth, no drag

• From Newton’s Laws of Motion, equations in 2-1

•Range vs. velocity, equation 2-2

s =Vhtf tf =2Vv

g h=

Vv2

2g

s =V2

g

Page 24: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Energy

• Potential energy, equation 2-3

•Ratio of kinetic energy increase to initial kinetic energy, equation 2-4

PE =mgh=wh

ΔKE

ΔKE0=1+ 2

VI

ΔV

Page 25: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Forces During Motor Burning

• Velocity loss due to gravity, equation 2-5

• Figure 2-1

ΔVg = −gtb sinγ

Page 26: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Airplane Lift/Drag Ratio

• Airplane energy, equation 2-6

•Cruising efficiency, equation 2-7

• Velocity equivalent of energy used, equation 2-8

EA =Ds

EA =ws

L / D

ΔVEN2 =

2g0s

L /D=2g0tbV

L /D

Page 27: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Airplane Lift/Drag Ratio

• Figure 2-2

Page 28: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Automobile Lift/Drag Ratio

• Figure 2-3

Page 29: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Ship Lift/Drag Ratio

• Figure 2-4

Page 30: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Solid-Propellant Rockets

• Figure 2-5

Page 31: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Solid Rockets

• Acceleration of guns or rockets, equation 2-9

•Honest John Missile

a =ΔV2

2g0s

Page 32: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Required Acceleration

• Figure 2-6

Page 33: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Four Decades of Development

• Figure 2-7

Page 34: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Theoretical Propellant

PerformanceVacuum ε = 40Vacuum ε = 40 Sea Sea

LevelLevel

OxidizerOxidizer FuelFuel Mixture Mixture RatioRatio

Specific Specific GravityGravity IIspsp (sec) (sec) IIspsp (sec) (sec)

NH4ClO4 20% Al 1.74 314 266

H2O2 N2H4 2.09 1.26 325 287

N2O4 N2H4 1.40 1.22 324 292

O2 (cyro)Kerosen

e2.67 1.02 324 300

O2 (cyro) N2H4 0.95 1.07 343 313

Page 35: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Elliptical Orbit Nomenclature

• Figure 3-1

Page 36: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Circular Orbits•Gravity as a

function of distance, equation 3-1

• Velocity of satellite, equation 3-2

• Period, equation 3-3

• Period, equation 3-4

g =g0

Rr

⎛⎝⎜

⎞⎠⎟2

Ve = gr =g0R

2

r

Pe =2πrVe

=2π rg

Pe =2πr3/2

g0R2

Page 37: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Potential Energy

• Potential energy, equation 3-5

•Maximum potential energy, equation 3-6

PE =wR 1−Rr

⎛⎝⎜

⎞⎠⎟=wR

hR+h

⎛⎝⎜

⎞⎠⎟

PEmax =wR, r→ ∞

Page 38: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Escape Velocity

• Escape velocity, equation 3-7 VE = 2gr =

2g0R2

r

Page 39: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Vis-Vita Law• Kinetic and potential

energy, equation 3-8

• Conservation of angular momentum, equation 3-9

• Perigee velocity vs. escape velocity at perigee, equation 3-10

• Velocity, equation 3-11

KE +PE =wV2

2g0

+wR 1−Rr

⎛⎝⎜

⎞⎠⎟

Vara =Vprp

Vp2

VEp2 =

rara + rp

=2raa

V 2 =g0R2 2

r−1a

⎛⎝⎜

⎞⎠⎟

Page 40: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Vis-Vita Law

• Velocity and circular velocity, equation 3-12

•Orbital period, equation 3-13

V

Vc0

⎝⎜

⎠⎟

2

=2

r / R−

1a / R

⎛⎝⎜

⎞⎠⎟

Por =2πa3/2

g0R2

Page 41: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Optimum Ballistic Missile Trajectories

• Figure 3-2

Page 42: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Global Rocket Velocities

• Figure 3-3

Page 43: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Hohmann Transfer

• Figure 3-4

Page 44: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Velocities Required to Establish Orbit

• Figure 3-5

• Potential energy and kinetic energy, equation 3-14

PE +KE =R 1−R2r

⎛⎝⎜

⎞⎠⎟

Page 45: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Planet Escape Velocities and Radii

PlanetPlanetEscape Escape VelocityVelocity

(feet/sec)(feet/sec)

Radius Radius (Earth = 1.0)(Earth = 1.0)

Earth 36,700 1.0

Venus 33,600 0.97

Pluto 32,700 1.1

Mars 16,400 0.53

Mercury 13,700 0.38

Page 46: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Satellite Escape Velocities and Radii

Satellite Satellite (Planet)(Planet)

Escape Escape VelocityVelocity

(feet/sec)(feet/sec)

RadiusRadius(Earth = (Earth =

1.0)1.0)Triton (Neptune) 10,400 0.31Ganymede (Jupiter)

9,430 0.39

Titan (Saturn) 8,900 0.39Io (Jupiter) 8,250 0.26Moon (Earth) 7,800 0.272Callisto (Jupiter) 7,450 0.37Europa (Jupiter) 6,900 0.23

Page 47: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Gravity Losses

• Effective gravity, equation 3-15

gef =g−Vh

2

r=

Vc2 −Vh

2

r

Page 48: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Large, Solid Propellant Motors

• Figure 3-6

Page 49: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Planets Orbital Data

PlanetPlanet Semi-Major Semi-Major Axis AUAxis AU

PerihelioPerihelion AUn AU

Aphelion Aphelion AUAU

Mercury 0.387 0.308 0.467

Venus 0.723 0.718 0.728

Earth 1.000 0.983 1.017

Mars 1.524 1.381 1.666

Jupiter 5.203 4.951 5.455

Saturn 9.539 9.008 10.070

Uranus 19.182 18.277 20.087

Neptune 30.058 29.800 30.315

Page 50: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Planets Orbital Data

Mean Celestial LongitudeMean Celestial Longitude

PlanetPlanetOff Off

Ascending Ascending NodeNode

of of PerihelioPerihelio

nn

Epoch, Epoch, 1/1/19961/1/1996

Mercury 47.93° 76.93° 210.29°

Venus 76.38 131.1° 84.87°

Earth 102.12° 98.89°

Mars 49.3° 335.44° 324.31°

Jupiter 100.11° 13.5° 87.32°

Saturn 113.42° 91.5° 347.57°

Uranus 73.9° 168.65° 166.43°

Neptune 131.4° 53° 230.02°

Page 51: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Planets Orbital Data

InclinationInclination

PlanetPlanet Orbital to Orbital to EclipticEcliptic

Equatorial to Equatorial to OrbitOrbit

Mercury 7.00

Venus 3.39

Earth 23.45

Mars 1.85 25.20

Jupiter 1.31 3.12

Saturn 2.49 26.75

Uranus 0.77 97.98

Neptune 1.77 29

Page 52: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Planets Orbital Data

PlanetPlanetOrbital Velocity Orbital Velocity

About Sun About Sun (ft/sec)(ft/sec)

Period of Period of Revolution Revolution

(years)(years)Mercury 157,000 0.240

Venus 114,800 0.615

Earth 97,600 1.0

Mars 79,100 1.881

Jupiter 42,800 11.86

Saturn 31,600 29.46

Uranus 22,200 84.02

Neptune 17,800 164.78

Page 53: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Solar System Data

Jupiter’Jupiter’s s

MoonsMoons

DiametDiameter er

(miles)(miles)

SurfaSurface ce

GravitGravityy

PerioPeriod d

(days(days))

Escape Escape Velocity Velocity

(fps)(fps)

Io 2,060 0.195 1.77 8,250Europa 1,790 0.156 3.55 6,900Ganymede

3,070 0.170 7.15 9,430

Callisto 2,910 0.112 16.69 7,450

Page 54: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Outer Solar System

• Figure 4-1

Page 55: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Hyperbolic Excess Velocity

• Vis-Viva Law, hyperbolic excess velocity, equation 4-1

• Equation 4-2

• Equation 4-3

V∞2 =−

g0R2

a

V 2 =VE2 +V∞

2

V∞ = V2 −VE2

Page 56: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Hyperbolic Excess Velocity

• Figure 4-2

Page 57: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Solar System Hyperbolic Excess

Velocity

• Figure 4-3

Page 58: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Hohmann Transfer Velocities

• Figure 4-4

Page 59: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Hohmann Transfer Travel Time

• Figure 4-5

Page 60: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Synodic Period of Planets

• Synodic period, equation 4-4

• Figure 4-6

PS =1

1P1

−1P2

Page 61: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Solar Probe Type Missions with Two Impulse Transfers

• Figure 4-7

Page 62: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Elastic Impact Analogy for the Use of

Planetary Energy

• Figure 4-8

Page 63: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Use of Planetary Energy

•Weight of vehicle, equation 4-5

• Equation 4-6

wV V∞ +VPI( )+wV V∞ −VPF( ) =wP VPI−VPF( )

wV 2V∞( ) =wP ΔVP( )

Page 64: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Planetary Swing-Around Angle

• Figure 4-9

Page 65: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Distance from Center of Sun (Astronomical Units) Solar

Probe Velocity Requirements

• Figure 4-10

Page 66: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Out-of-Ecliptic Velocity

Requirements

• Figure 4-11

Page 67: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Solar System Travel Times

• Figure 4-12

Page 68: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Planetary Arrival Velocities

• Figure 4-13

Page 69: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Planetary Capture Velocities

• Figure 4-14

Page 70: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Payload Velocity Requirements

• Figure 4-15

Page 71: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Selected Comets

CometComet PeriheliPerihelion (AU)on (AU)

AphelioAphelion (AU)n (AU)

PerioPeriod d

(year(years)s)

PerihelioPerihelion Timen Time

Encke 0.339 4.09 3.301967-9-

12

Forbes 1.545 5.36 6.421967-12-

21

D’Arrest 1.378 5.73 6.701967-6-

17

Faye 1.652 5.95 7.411969-12-

29

Halley 0.587 35.0 76.031910-4-

20

Page 72: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Earth-Mars Launch Windows

• Figure 4-16

Page 73: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Earth-Mars Launch Windows

• Figure 4-17

Page 74: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Round Trip Synodic Period Effects

• Figure 4-18

Page 75: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Theoretical Liquid Propellant Performance

Equilibrium FlowVacuumVacuum Sea Sea

LevelLevel

OxidizerOxidizer FuelFuel Mixture Mixture RatioRatio

Specific Specific GravityGravity IIspsp IIspsp

Oxygen Hydrogen 4.5 0.31 456 391

Fluorine Hydrogen 9.0 0.50 475 411

Fluorine Ammonia 3.31 1.12 416 360O2-Difluoride

Kerosene 3.8 1.28 396 341

Hydrazine Diborate 1.16 0.63 401 339

HydrazinePentaborane 1.26 0.79 390 328

Page 76: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

High-Performance Chemical Rockets

• Figure 4-19

Page 77: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

New Types of Engines

•Wall stress, equation 4-7

• Engine chamber weight, equation 4-8

σ =pr

2t

wco : Acot :

Acopr

Page 78: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

New Engine Types

• Figure 4-20

Page 79: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Nuclear Thermal Rockets

• Einstein’s famous equation 4-9

• Kiwi-A rocket engine

E =mc2

Page 80: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Graphite Solid-Core Engine

• Figure 4-21

Page 81: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Isotopic Heat Sources

Parent Parent IsotopeIsotope

Half-Half-Life Life

(year(years)s)

Type Type of of

DecaDecayy

Specific PowerSpecific Power(watts/gm)(watts/gm)

ShieldiShieldingngPurePure Fuel Fuel

CompoundCompound

Cesium-137 30 β/γ 0.42 0.067 Heavy

Plutonium-238

89 α 0.56 0.39 Minor

Curium-244 18 α 2.8 2.49Moderat

e

Polonium-210

0.38 α 141 134 Minor

Cobalt-60 5.3 β/γ 17.4 1.7 Heavy

Page 82: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Nuclear Vehicle Shielding

Comparison

• Figure 4-22

Page 83: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Required Fuel Weights for Single-Stage Space

Launch Vehicles

• Figure 4-23

Page 84: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Heavy Velocity Rockets and Gravity

Fields• Travel time, equation 5-1

•Minimum travel time in terms of inner and outer distance, equation 5-2

•Maximum travel time, equation 5-3

t f =57AUΔV

100,000⎛⎝⎜

⎞⎠⎟

t f =144 AUo −AUi( )

ΔV100,000

⎛⎝⎜

⎞⎠⎟

t f =144 AUo +AUi( )

ΔV100,000

⎛⎝⎜

⎞⎠⎟

Page 85: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Minimum Travel Times from Earth Including

Braking Requirements

• Figure 5-1

Page 86: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Average Travel Times from Earth Including

Braking Requirements

• Figure 5-2

Page 87: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Solar System Synodic Periods

• Figure 5-3

Page 88: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Travel Times Between Planets

• Figure 5-4

Page 89: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Escape with Low Acceleration

• Velocity required to escape, equation 5-4

• For launch from circular orbit, equation 5-5

ΔV =Ve +V∞

ΔV = 2Vc2 +V∞

2 −Vc

Page 90: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Total Velocity to Escape

• Figure 5-5

Page 91: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Heliocentric Velocity Requirements

• Time to generate velocity at constant acceleration, equation 5-6

• Figure 5-6

tb =0.036a / g0( )

ΔV100,000

⎛⎝⎜

⎞⎠⎟

Page 92: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Specific Impulse From Nuclear

Reactions

• Figure 5-7

Page 93: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Typical Gaseous Core

Engines

• Figure 5-8

• Power output, equation 5-7

Pr =0.501T

1,000⎛⎝⎜

⎞⎠⎟

4

Page 94: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Cost of Nuclear Fission Fuel and

Propellant

• Figure 5-9

Page 95: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Cooling Limitations

• Amount by which gaseous heating raises specific impulse, equation 5-8

I sp =I sps

f

Page 96: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Thrust/Weight Ratio of Gaseous Fission

Engines

• Figure 5-10

Page 97: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Types of Electrical Rocket

Thrusters

• Figure 5-11

Page 98: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Electric Rocket Performance

•Characteristic velocity, equation 5-9

• For perfect efficiency, weight of power supply relates to weight of propellant, equation 5-10

Vch =64,100tbα

wαVch2 =wpvef

2

Page 99: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Electrical Rocket Performance

• Figure 5-12

Page 100: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Single-Stage Spaceship Fuel and

Propellant Costs

• Figure 5-13

Page 101: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Transportation vs. Ammunition Re-Use

Assumptions

• Figure 5-14

Page 102: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Spaceship Payload Capability

• Figure 5-15

Page 103: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Single-Stage Spaceship Fuel, Propellant, and

Structure Costs

• Figure 5-16

Page 104: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Single-Stage Spaceship Fuel, Propellant, and

Structure Costs

• Figure 5-17

Page 105: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Dose to Ground Observer from

Gaseous Core Rockets

• Figure 5-18

Page 106: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Gaseous Fission Powered Spaceship

• Figure 5-19

Page 107: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Acceleration Distance

• Figure 5-20

Page 108: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Near Stars

• Figure 6-1

Page 109: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

The Galaxy

• Figure 6-2

Page 110: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Hypothetical Galactic Community

• Figure 6-3

Page 111: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Time Dilation

• Ship time, equation 6-1 ts =tEA 1− V / c( )

2

Page 112: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Interstellar Travel Time Dilation

Effects

• Figure 6-4

Page 113: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Fusion Rockets

• Initial weight vs. final weight, equation 6-2

•Rocket braking on arrival, equation 6-3

wI

wF

=1+

ΔVc

1−ΔVc

⎢⎢⎢

⎥⎥⎥

c/2vef

wI

wF

=1+

ΔVc

1−ΔVc

⎢⎢⎢

⎥⎥⎥

c/vef

Page 114: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Fusion Starship Weight Ratio

• Figure 6-5

Page 115: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Fusion Starship Power

• Figure 6-6

Page 116: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Cost of Nuclear Rocket Fuel and

Propellant

• Figure 6-7

Page 117: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Photon Rockets

• Effective exhaust velocity, equation 6-4

•Relativistic rocket equation 6-5

• Exhaust power of photon beam, equation 6-6

vef =εc

wI

wF

=1+

ΔVc

1−ΔVc

⎢⎢⎢

⎥⎥⎥

1/2ε

Pef =Tc

Page 118: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Starship Weight Ratio

• Figure 6-8

Page 119: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Mass Annihilation Rockets

•Mass annihilation rocket equation 6-7

•Mass annihilation rocket braking equation 6-8

wI

wF

=1+

ΔVc

1−ΔVc

⎢⎢⎢

⎥⎥⎥

1/2

wI

wF

=1+

ΔVc

1−ΔVc

⎢⎢⎢

⎥⎥⎥

Page 120: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Starship Power

• Figure 6-9

Page 121: Thrust into Space Maxwell W. Hunter, II. Newton’s 3rd Law of Motion Momentum is conserved, equation 1- 1.

Mass Annihilation Rockets

•Overall time dilation effect, equation 6-9

•Relation between time dilation achieved and rocket weight, equation 6-10

• Equation 6-11

ts =tEA 1+Vc

⎛⎝⎜

⎞⎠⎟

1−Vc

⎛⎝⎜

⎞⎠⎟

=tEA 2 1−Vc

⎛⎝⎜

⎞⎠⎟

wI

wF

=2

1−ΔVc

⎢⎢⎢

⎥⎥⎥

wI

wF

=2tEA

ts

⎝⎜⎞

⎠⎟

2