Ideal-model g with partial screening interval, k = 2
Refused: no defensible result
Calibrate the printed gauge before computing.
A paper gravimeter, with permission to say “not resolved”
Four printed strips become an 800.0 mm gauge. It sets a real pendulum’s pivot-to-bob-centre length, then the paper and a clock estimate gravity after this screen is switched off.
First, move one number. The curve below is not local weather for gravity. It is GRS80 normal gravity on a reference ellipsoid, recomputed from Moritz’s published constants. North and south give the same result; longitude does not enter this model.
GRS80 normal gravity at 37.8136°
9.7997662187 m/s²
0.0194394472 m/s² above the equator. This is not a measurement at your site.
Moritz prints γ(φ) = γe(1 + k sin²φ) / √(1 − e² sin²φ). The page uses the following table values directly, then recomputes the endpoints and Melbourne example rather than copying their outputs.
| quantity | published | recomputed here |
|---|---|---|
| γe | 9.7803267715 | |
| γp | 9.8321863685 | |
| e² | 0.00669438002290 | formula input |
| k | 0.001931851353 | formula input |
| pole − equator | derived | |
| Melbourne, |37.8136°| | derived |
gn = 9.80665 m/s² is shown only for contrast. JCGM calls it a conventional quantity value. It is not a measured local value and is not substituted into this model.
The mathematics is not the dominant uncertainty. The values below are explicit planning assumptions for this build, not measured household-performance facts. An irregular bob has no defensible result until its centre of mass and moment of inertia are independently established.
Choose the paper loaded in the printer, print at 100% / Actual Size, and disable “fit to page” and “shrink oversized pages”. All four sheets must be printed in the same job settings.
Not calibrated. This page cannot vouch for paper it has not seen measured. Measure both axes on every sheet; one entry here records the job, not four independent inspections.
The ideal plane pendulum’s period is multiplied by C(θ) = (2/π)K(sin(θ/2)). The calculator evaluates the complete elliptic integral, not merely the small-angle rule. It also distinguishes the pivot-to-centre distance h from equivalent simple-pendulum length.
Ideal-model g with partial screening interval, k = 2
Refused: no defensible result
Calibrate the printed gauge before computing.
GRS80 model comparison
No latitude claim permitted
The normal-gravity target and a partial interval cannot determine latitude or local g.
| amplitude | ideal C − 1 | raw g bias if ignored | θ⁴ series difference |
|---|
g = 4π² Leff C² / (t/N)² | Leff,sphere = h + 2r²/(5h) | (ug/g)² = (uL/L)² + (2ut/t)² + (2uC/C)² + umodel²
The result card may say whether a GRS80 target is numerically inside or outside the declared screening interval, but it makes no detection or latitude inference. The interval is incomplete, normal gravity is not site gravity, north and south are symmetric, and at 0° or 90° an endpoint match is true by construction.
At Melbourne’s latitude, the GRS80 value is only 0.19876% above the equator. The full pole-to-equator span is 0.53024%. One hundred swings divide a fixed start-stop error across many periods; they do not divide away an incorrect length.
Helmut Moritz, Geodetic Reference System 1980, supplies the constants and normal-gravity formula. JCGM VIM 2.12 identifies conventional g. Nelson and Olsson, DOI 10.1119/1.14703, treat the plane pendulum corrections and equivalent length. The 1968 NBS gravity record supplies the length and timing sensitivity and warns that precision alone does not establish accuracy.