Letcher Lunar Distance Calculator

J. S. Letcher Jr. method  ·  Starpath School of Navigation

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Sight Data
Date / /
Lat-s ° '
Lon-s ° '
Ts (UTC) h m s
Hm (Moon alt) ° '
Hb (Body alt) ° '
D (SD-corrected) ° '
Almanac Data
Moon
Gm− (GHA at T−) ° '
Dm− (Dec at T−) ° '
Gm+ (GHA at T+) ° '
Dm+ (Dec at T+) ° '
HP Moon arcmin
Body (Sun / Star / Planet)
Gb− (GHA at T−) ° '
Db− (Dec at T−) ° '
Gb+ (GHA at T+) ° '
Db+ (Dec at T+) ° '
Clear the Lunar
y
P
x
R
Dc
Find UTC & Longitude
D−
D+
Tc
dUTC
dLon
Equations (J. S. Letcher Jr.)
y [cos(D)·sin(Hm) − sin(Hb)] / sin(D) dimensionless
P HP · { y + 0.000145·HP·cot(D)·[cos²(Hm) − y²] } arcmin  (HP in arcmin from almanac)
x 0.5 · [sin(Hm)/sin(Hb) + sin(Hb)/sin(Hm)] dimensionless
R 1.90 · (x − cos D) / sin D arcmin
Dc D + (P + R) / 60 degrees  (P and R converted from arcmin)
arccos[sin(Dm±)·sin(Db±) + cos(Dm±)·cos(Db±)·cos(Gm± − Gb±)] geocentric LD at T− and T+
Tc T− + (Dc − D−) / (D+ − D−) T− = INT(Ts) ; result in decimal hours
dUTC Ts − Tc [× 3600 → seconds] + = Ts fast ; − = Ts slow
dLon dUTC [sec] × 0.25′ arcmin of longitude ; 0.25′ per 1 sec of UTC error
Notes
  1. Ts is the best estimate of a common UTC for the lunar distance and altitude measurements.
  2. D is the lunar distance corrected for semidiameters.
  3. Hm and Hb can be observed (Ho) or computed (Hc) altitudes.
  4. T− and T+ are the whole UTC hours bracketing Ts: T− = INT(Ts), T+ = INT(Ts) + 1.
  5. P and R are in arcmin; Dc = D + (P + R)/60 adds them to D in degrees.
  6. dUTC > 0 (Ts fast): true UTC is earlier than Ts. dUTC < 0: Ts is slow.
  7. dLon = dUTC [sec] × 0.25′ ; equivalently 15′ per 1 minute of UTC error.
  8. For discussion and references see Lunar Distance by Calculator: The Letcher Method.