A paper gravimeter, with permission to say “not resolved”

The String That Weighs the Earth

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.

Latitude changes the target

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.

The published anchor, before the print button

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.

quantitypublishedrecomputed here
γe9.7803267715
γp9.8321863685
0.00669438002290formula input
k0.001931851353formula input
pole − equatorderived
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.

Error budget, before you measure

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.

Printed and assembled length: 4.0 mm minimum standard allowance
Four accepted 200 mm modules can each retain a ±0.5 mm reading floor, before cutting and joints. The calculator therefore refuses u(L) below 0.0040 m.
Bob model and other systematics: 0.10% minimum standard allowance
This is a declared screening floor, not proof that the build is accurate to 0.10%. It does not rescue an unknown irregular-bob inertia; that model is refused outright.
Start and stop: 0.283 s minimum standard allowance
This follows the stated model of independent 0.20 s start and stop uncertainties: √2 × 0.20 s. Repetition reduces random scatter, not scale, bob, drag, pivot or counting errors.
Amplitude history: 0.05% minimum relative standard allowance in C
The elliptic-integral factor is exact only for an ideal plane pendulum held at one amplitude. A real damped run needs an amplitude-history allowance; the calculator will not silently set it to zero.
Named, not corrected
String mass and stretch, pivot radius or slip, air buoyancy and drag, drafts, elliptic motion, paper humidity, cutting, butt joints and tape creep. Height changes normal gravity by roughly 0.003% per 100 m; terrain, tides, groundwater and local density anomalies are absent from GRS80 here.

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.

Measure one sheet’s local checks first

What the paper does

  1. On every sheet, measure the 100.0 mm horizontal line, 100.0 mm vertical line and 50.0 × 50.0 mm square. Reject and reprint if either axis is outside 99.5 to 100.5 mm. Do not average the axes.
  2. Cut each narrow module on its solid boundary. Butt module 1’s 200 datum against module 2’s zero datum on a flat surface. Tape across the back. Repeat without overlapping any calibrated span.
  3. Place the assembled zero cross at the actual support point. The four spans now locate an 800.0 mm target. This is not an instruction to cut 800 mm of free string.
  4. Tie a compact symmetric bob and adjust until its measured centre of mass aligns with the target. For a solid sphere, use the calculator’s inertia correction. Do not apply that sphere formula to nuts, coins, keys or hollow balls.
  5. Use the printed angle wedge. Release without pushing. One oscillation means return to the same side moving in the same direction. A centre crossing is half an oscillation.
  6. Time 100 complete oscillations, expected near 179.5 seconds, and repeat at least five times. Record every run. Then repeat at 10°, 15° and 20° to expose the amplitude drift.

Make the school-lab approximation answer back

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.

amplitudeideal C − 1raw g bias if ignoredθ⁴ 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

Let non-detection be a result

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.

The check, visible

Sources and what each establishes

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.