martes, 31 de marzo de 2026

mecánica-lunar

Principio: [ orbital de cuerpo celeste ]

I_{c}·d_{t}[w]^{2} = pq·k·(1/R)

Ley

Órbita lunar:

B(d_{t}[w]) = qk·(1/r)^{2}·( (1/I_{c})·pq·k·(1/R)·)^{(1/2)}

Alunizar:

E(w) = qk·(1/r)^{2}·( (1/I_{c})·pq·k·(1/R)·)^{(1/2)}·t

Ley:

x(t) = pqk·(1/r)^{2}·( (1/I_{c})·pq·k·(1/R)·)^{(1/2)}·(1/6)·t^{3}+( (1/I_{c})·pq·k·(1/R)·)^{(1/2)}·ht+h

d_{t}[x] = pqk·(1/r)^{2}·( (1/I_{c})·pq·k·(1/R)·)^{(1/2)}·(1/2)·t^{2}+( (1/I_{c})·pq·k·(1/R)·)^{(1/2)}·h