Apparatus Workshop: Bessemer Optomechanical Division
Fiducial Tolerance: ±0.05 arcsec
Drive System: Gravity Weight Clockwork
Clock: --:--:-- UTC

Primary Observing Equipment

Meridian Circle • No. 03

The 200 mm Repsold Transit Instrument

Mounted strictly along the North-South celestial meridian on monolithic granite piers. Utilizes twin silver circles read by four micrometer microscopes reading directly to tenths of an arcsecond.

Equatorial Coude • No. 01

The 380 mm Gautier Dual Refractor

An articulated folded-path refractor permitting the observer to remain stationary in a temperature-controlled room while the instrument sweeps the polar axis. Houses both visual and photographic tubes.

Photometric Benchmark • No. 07

The Hartmann Wedge Photometer

A neutral gray glass absorption wedge that optically dims an artificial comparison light source until extinction matches the targeted celestial body. Unaffected by electrical voltage fluctuations.

Optomechanical Specifications

Objective Glass Glass Type
Schott Borosilicate Crown (BK7) & Dense Flint (F2)
Drive Mechanism
Falling 80 kg lead ballast regulated by fly-ball governor
Filar Micrometer Wire
Natural Araneus diadematus dragline silk (4.5 μm diameter)
Pier Foundation
Sub-bedrock crystalline granite isolated from pavilion floors
Spider Silk Reticles

The filar cross-hairs of our meridian transits are strung exclusively with washed cocoon silk. Unlike metal wires, these fibers maintain perfect tension without sagging or breaking across severe sub-zero mountain temperatures.

Calibration and Collimation Log

Instrument Collimation Method Error Tolerable Cycle of Inspection Vault Custodian
Repsold Meridian 200 mm Nadir Mercury Basin Reflection ±0.04″ Weekly at Sunset Station Observer A
Gautier Coude 380 mm Opposed Horizontal Collimator Telescopes ±0.08″ Prior to Every Lunar Cycle Optical Engineer
Plate Measuring Engine Precision Lead Screw Interferometry ±0.5 μm Monthly Routine Chief Metrologist