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{{convert|100|lb|kg}} → 100 pounds (45 kg) The unit-codes should be treated as case-sensitive: {{convert|100|Mm|mm}} → 100 megametres (1.0 × 10 11 mm) The output of {{convert}} can display multiple converted units, if further unit-codes are specified after the second unnamed parameter (without the pipe separator). Typical combination ...
Template talk:Convert • Questions on using the convert template, or discussion of any problems encountered, or proposals to add units or change convert; Wikipedia:Help desk • General questions; Module talk:Convert • Discussion concerning the convert modules (however, discussions relating to units should occur at Template talk:Convert)
Converts measurements to other units. Template parameters [Edit template data] This template prefers inline formatting of parameters. Parameter Description Type Status Value 1 The value to convert. Number required From unit 2 The unit for the provided value. Suggested values km2 m2 cm2 mm2 ha sqmi acre sqyd sqft sqin km m cm mm mi yd ft in kg g mg lb oz m/s km/h mph K C F m3 cm3 mm3 L mL cuft ...
Template documentation For the unit conversion template, see Template:Convert . Editors can experiment in this template's sandbox ( create | mirror ) and testcases ( create ) pages.
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[3] [5] Use of the gal was deprecated by the standard ISO 80000-3:2006, now superseded. The gal is a derived unit, defined in terms of the centimeter–gram–second (CGS) base unit of length, the centimeter, and the second, which is the base unit of time in both the CGS and the modern SI system. In SI base units, 1 Gal is equal to 0.01 m/s 2.
The factor–label method can convert only unit quantities for which the units are in a linear relationship intersecting at 0 (ratio scale in Stevens's typology). Most conversions fit this paradigm. An example for which it cannot be used is the conversion between the Celsius scale and the Kelvin scale (or the Fahrenheit scale). Between degrees ...
Stripping out unit conversion and uniform scaling, the formulae may be written: x = R λ y = 2 R sin φ {\displaystyle {\begin{aligned}x&=R\lambda \\y&=2R\sin \varphi \end{aligned}}} where λ {\displaystyle \lambda } is the longitude from the central meridian (in radians), φ {\displaystyle \varphi } is the latitude, and R is the radius of ...