Sextant noon sight in one offline app: Calculator reduces a meridian passage to latitude & longitude with an on-board solar ephemeris (truncated VSOP87D, Meeus Astronomical Algorithms ch. 25 higher-accuracy path, checked against JPL DE421 to ≤0,03′ — no almanac tables, any date works, 2026 included); Worked examples holds the four sights from the course deck, recomputed and corrected; Training is a graded sextant drill against a live GPS referee. Coordinates in Degrees Minutes,Decimal, e.g. 78° 48,2' N.
Enter at least 3 timed sextant altitudes taken around local noon.
A parabola is fitted by least squares through all entered points; its vertex gives the time of the true Sun
and the corresponding Hs to be used in Part 2.
Time = watch time HH:MM:SS, Hs = DD MM,M (or decimal degrees).
| Date: | ||
| DR Latitude: | N/S | |
| DR Longitude: | W/E | |
| Watch time: | h:m:s | |
| Zone corr. (zone − UTC): | h | |
| GMT (UT): | h:m:s |
GMT = watch time − zone correction. East zones positive (CET = +1, CEST = +2).
| Eye height: | m | |
| Limb: | ||
| Hs (Height Sextant): | ° ' | |
| IE (Index Error): | ' | |
| Dip −: | ' | |
| App. Alt: | ° ' | |
| Alt. Corr. + −: | ' | |
| Ho (Altitude): | ° ' |
| Declination: | N/S | |
| DR Latitude: | N/S | |
| Ho (Altitude): | ° ' | |
| ZD = 90° − Altitude: | ° ' |
| Lat > Dec, same N/S | Lat = ZD + DEC |
| Lat, Dec different N/S | Lat = ZD − DEC |
| Lat < Dec, same N/S | Lat = DEC − ZD |
| LATITUDE | ||
| DR / GPS: | ||
| Difference: | ||
| Mer. Pass. Greenwich: | GMT | |
| Difference (time) GMT − Mer.Pass: | h:m:s | |
| Time to Arc: | ° ' |
Mer. Pass. Greenwich = 12h − Equation of Time. Time is converted to arc at 15°/h (1h = 15°, 1m = 15', 4s = 1'). Observer west of Greenwich ⇒ transit after Greenwich noon.
| LONGITUDE | ||
| DR / GPS: | ||
| Difference: | ||
The four noon sights from the presentation, re-computed here with the on-board ephemeris. Load fills Part 2 of the Calculator tab with the sight; Worked solution shows every step. Where the deck contains a slip, the errata box says exactly what and why — the arithmetic below is the corrected one.
| IE (Index Error): | ' | |
| Eye height: | m | |
| Limb: | ||
| Mark delay (sight → entry): | s |
Mark delay = how long it takes you to lower the sextant and reach the phone. Pressing New reading stamps the sight that many seconds in the past and uses the GPS position from that same moment.
| GPS source: | ||
| Blind mode: | ||
—
| # | UT time | Hs (DD MM,M) | Δ vs GPS truth |
|---|
Δ = your Hs minus the Hs a perfect sextant would have read at the GPS position at that second (ephemeris altitude, corrections applied in reverse). Grading: ≤0,3′ perfect ≤0,8′ excellent ≤1,5′ good ≤3′ fair >3′ check that shot
| LATITUDE | |
| LONGITUDE |
| GPS at culmination: | ||
| Error Lat / Lon: | NM | |
| Total error: | NM |