Arc measurement

The first known arc measurement was performed by Eratosthenes (240 BC) between Alexandria and Syene in what is now Egypt, determining the radius of the Earth with remarkable correctness. In the early 8th century, Yi Xing performed a similar survey.^[5]

The French physician Jean Fernel measured the arc in 1528. The Dutch geodesist Snellius (~1620) repeated the experiment between Alkmaar and Bergen op Zoom using more modern geodetic instrumentation (Snellius' triangulation).

Later arc measurements aimed at determining the flattening of the Earth ellipsoid by measuring at different geographic latitudes. The first of these was the French Geodesic Mission, commissioned by the French Academy of Sciences in 1735–1738, involving measurement expeditions to Lapland (Maupertuis et al.) and Peru (Pierre Bouguer et al.).

Struve measured a geodetic control network via triangulation between the Arctic Sea and the Black Sea, the Struve Geodetic Arc. Bessel compiled several meridian arcs, to compute the famous Bessel ellipsoid (1841).

Nowadays, the method is replaced by worldwide geodetic networks and by satellite geodesy.

 

• Al-Ma'mun's arc measurement
• Posidonius' arc measurement
• Swedish–Russian Arc-of-Meridian Expedition
• Picard's arc measurement
• Dunkirk-Collioure arc measurement (Cassini, Cassini, and de La Hire)
• Dunkirk-Collioure arc measurement (Cassini de Thury and de Lacaille)
• Meridian arc of Delambre and Méchain
• West Europe-Africa Meridian-arc
• De Lacaille's arc measurement
• Fernel's arc measurement
• Norwood's arc measurement
• Boscovich and Maire's arc measurement
• Maclear's arc measurement
• Hopfner's arc measurement
• Struve Geodetic Arc

Assume the astronomic latitudes of two endpoints, ${\displaystyle \phi _{s}}$  (standpoint) and ${\displaystyle \phi _{f}}$  (forepoint) are known; these can be determined by astrogeodesy, observing the zenith distances of sufficient numbers of stars (meridian altitude method).

Then, the empirical Earth's meridional radius of curvature at the midpoint of the meridian arc can then be determined inverting the great-circle distance (or circular arc length) formula:

${\displaystyle R={\frac {{\mathit {\Delta }}'}{\vert \phi _{s}-\phi _{f}\vert }}}$ 

where the latitudes are in radians and ${\displaystyle {\mathit {\Delta }}'}$  is the arc length on mean sea level (MSL).

Historically, the distance between two places has been determined at low precision by pacing or odometry. High precision land surveys can be used to determine the distance between two places at nearly the same longitude by measuring a baseline and a triangulation network linking fixed points. The meridian distance ${\displaystyle {\mathit {\Delta }}}$  from one end point to a fictitious point at the same latitude as the second end point is then calculated by trigonometry. The surface distance ${\displaystyle {\mathit {\Delta }}}$  is reduced to the corresponding distance at MSL, ${\displaystyle {\mathit {\Delta }}'}$  (see: Geographical distance#Altitude correction).

An additional arc measurement at another latitudinal band, delimited by a new pair of standpoint and forepoint, serves to determine Earth's flattening.

• Astrogeodesy
• Earth ellipsoid
• Geodesy
• Gradian § Relation to the metre
• History of geodesy
  • Spherical Earth § History
  • Meridian arc § History
  • Earth's circumference § History
• Meridian arc
• Paris Meridian