ES-01 practice — not an approved assessment

Rotating Earth and coordinate systems

Learning outcomes & permitted supports
  • Identify axes, poles, equator, meridians and parallels, and read any position as latitude and longitude.
  • Distinguish great circles from small circles and say why the difference matters for distance.
  • Compute DLat and DLong (shortest way, date-line safe) and convert longitude to miles through latitude.

Supports in this lab: interactive sphere, engine-computed differences and distances. No tables needed.

Glossary: latitude · longitude · DLat/DLong · great circle · small circle · nautical mile · declination

The sphere itself

NBA
Equator in teal — the only parallel that is a great circle. The green arc is the great-circle track A→B: notice it does not follow a parallel.

Coordinates & differences (engine)

A (vessel)18° 56.4′ N 072° 49.8′ E
B (destination)01° 21.0′ N 103° 49.2′ E
DLat A→B17° 35.4′ S
DLong A→B (shortest)030° 59.4′ E
Great-circle distance2105.3 nm
1′ of latitude1.0 nm (everywhere)
1° of longitude at 18° 56.4′ N56.8 nm

Slide A toward the pole and watch one fact do all the work: a minute of latitude is always a mile, but a degree of longitude shrinks with cos(lat) — longitude is an angle, never a distance. DLong is computed the shortest way round; drag B across the date line and watch it stay small while the raw difference would jump to 350°+.

My notebook — ES-01 (0)

All notes & standing →

Every interaction here is recorded as an ordered evidence trail — 0 events this attempt.