Lunar Material and Momentum Supply

I am skeptical about high tech manufacturing in space, especially in the dusty lunar environment. Factories are big, and need a lot of PhDs to keep them running. 100 years from now, there will be many such factories in space, but for now, we have problems locating them in most countries around the world, where there is air and water and food and FedEx.

Assuming we can get material launched from the moon ( 5.5% of the escape energy and launch loop track length ), there are plenty of uses for deadweight mass in space, as ballast and as a source of momentum. Earth launch is expensive, and is deficient in angular momentum compared to destination orbits.

Earth and Moon and interesting orbits

Earth

\mu_e

Earth gravitational parameter

3.986004418e+14

m3/s2

r_E

Earth equatorial radius

6378137

m

E_e

Earth escape energy

-62.494807

MJ/kg

\omega_e

Earth angular frequency

7.29211515e-5

radians/s

Geostationary orbit

r_{GEO}

GEO radius

42164172.4

m

v_{GEO}

GEO velocity

3074.66

m/s

E_{GEO}

GEO Energy/kg

-1.41803E+07

J/kg

H_{GEO}

GEO Angular momentum/kg

1.2964E+11

m2/s

M288 Server Sky orbit

r_{288}

M288 radius

12788978

m

v_{288}

M288 velocity

5582.79

m/s

E_{288}

M288 energy/kg

-4.6751244E+07

J/kg

H_{288}

M288 angular momentum/kg

7.1398E+10

m2/s

Moon

\mu_m

Lunar gravitational parameter

4.9027779e+12

m3/s2

r_m

Lunar equatorial radius

1738140

m

E_{m-esc}

Lunar escape energy

2.8207037

MJ/kg

a_m

Lunar orbit semi-major axis

384399000

m

v_m

Lunar orbit velocity

1023.155

m/s

t_m

Lunar orbit period

2360591.5

seconds

\omega_m

Lunar orbit angular frequency

2.66169954e-6

radians/s

E_m

Lunar orbit energy/kg

-5.13522E+05

J/kg

H_m

Lunar angular momentum/kg

3.93300E+11

m2/s

Hohmann orbit, moon to GEO       r_a = a_m       r_p = r_{GEO}

a_{m-GEO}

Lunar-GEO semi-major axis

213281586

m

e_{m-GEO}

Lunar-GEO eccentricity

0.8023075

v_{a-m-GEO}

Lunar-GEO apogee velocity

452.7650

m/s

v_{l-m-GEO}

Lunar-GEO launch velocity

-2442.6935

m/s

v_{p-m-GEO}

Lunar-GEO perigee velocity

4127.7325

m/s

v_{i-m-GEO}

Lunar-GEO insertion velocity

-1053.0725

m/s

E_{m-GEO}

Lunar-GEO energy/kg

-9.34446E+05

J/kg

H_{m-GEO}

Lunar-GEO angular momentum/kg

1.74042E+11

m2/s

\omega_{m-G}

Lunar-GEO angular freq @ moon

1.17785E-06

radians/s

\omega_{G-m}

Lunar-GEO angular freq @ GEO

9.78967E-05

radians/s


Construction Orbit Apogee

Earth-Launchloop synchronous orbits "return to perigee" at multiples of an 86141 second sidereal day, facilitating synchronized additions of material from a launchloop. These ConstructionOrbits can be fed at apogee from lunar launches, though arrivals will be infrequent and asynchronous, especially due to the 23 degree inclnation of the Earth's orbit, and the extra 8 degrees north inclination of construction orbit apogees (launched from 8 degrees south.

Since the orbits are in a plane matching the launch loop's south latitude with respect to the Earth's center; a launch from the Moon that intersects with this plane will occur at the two times per month when the moon crosses this plane as well. That launch will generally be approximately collinear with 8 degrees south latitude on Earth.

A launch loop near the south pole of the Moon, launching approximately retrograde to the Moon's orbit, can harvest lunar ice in permanently shadowed craters, and connect to rotating photovoltaic arrays in contnuous sunlight. Although the Moon is tidelocked to the Earth, rotating once per sidereal month, a few degrees of north/south adjustment will be needed. Also, the lunar rotation axis is 1.5 degrees from the elliptic poles, and precesses in an 18.6 year cycle. As of this writing, it is pointed about 0.7 degrees away from Delta Doradus in the southern Dorado constellation, and about 24.4 degrees from the Earth's south celestial pole.

Actual mission planning will require much more precision than this. Loop launched surveying satellites and active retroreflectors will help us map the inner solar system to micrometer precision.

The following table is approximate, describing the apses, velocities, and times for construction orbits and in-plane trajectories (I wish ...). Plane changes (cheaper at apogee) require delta V's of 2 \sin( \delta / 2 ) V_{apogee}

construction orbit

Earth Loop launch

Moon launch to construction apogee

period

km

radius km

velocity m/s

velocity m/s

velocity m/s

ratio

sid.days

semi

peri.

apo.

peri.

apo.

peri.

apo.

insert

apo.

peri.

launch

insert

1

42164

8378

75950

9257

1021

10666

907

114.2

584.9

2961

2420

-1939

16.98

2

66931

8378

125484

9445

631

10835

558

72.9

714.4

2188

2399

-1558

21.36

3

87705

8378

167032

9519

477

10902

421

56.0

792.6

1824

2390

-1347

24.07

4

106247

8378

204116

9560

392

10939

346

46.3

848.1

1597

2385

-1205

26.01

5

123289

8378

238199

9588

337

10963

297

40.0

890.8

1437

2382

-1100

27.51

6

139223

8378

270068

9607

298

10980

263

35.5

925.1

1317

2380

-1019

28.73

7

154292

8378

300205

9621

269

10993

236

32.0

953.6

1221

2379

-953

29.74

8

168657

8378

328935

9633

245

11003

216

29.3

977.9

1143

2378

-897

30.60

9

182434

8378

356489

9642

227

11011

199

27.1

998.9

1077

2377

-851

31.35

10

195709

8378

383039

9650

211

11018

186

25.3

1017.4

1021

2377

-810

32.01

A higher construction orbit saves delta V, but with a ConstructionPort capture system, angular momentum from lunar delivery provides the insertion delta V needed for loop launch insertion. A lower construction orbit can be accessed from Earth more often, and is less perturbed by lunar tides. North/South delta V from the Moon is needed for plane matching, and that will be smaller if the transfer orbit apogee velocity is smaller.