Metric
A metric is a standard of measurement or a function that defines distance or similarity in a space. The term is used across various disciplines to quantify, compare, or evaluate phenomena. In measurement and standards, a metric refers to a system of units, most notably the International System of Units (SI), also known as the metric system, which provides a decimal-based framework for physical quantities using seven base units: metre (length), kilogram (mass), second (time), ampere (electric current), kelvin (temperature), mole (amount of substance), and candela (luminous intensity). Detailed coverage of the metric system, including its history and adoption, is provided in the "International Metric System (SI Units)" subsection.[1] In mathematics, a metric is a distance function on a set, satisfying properties like non-negativity and the triangle inequality, forming the basis of metric spaces essential in topology and analysis. Advanced structures, such as Riemannian metrics, are explored in geometry. In the natural sciences, metrics appear in physics as tools like spacetime metrics in general relativity, and in biology and chemistry for quantifying biodiversity or reaction rates. Engineering and applied sciences employ metrics for performance evaluation, such as efficiency ratios in design or code quality measures in software development. In business and social sciences, metrics denote key performance indicators (KPIs) for assessing economic growth, statistical significance, or organizational effectiveness. Finally, in the arts and humanities, metrics relate to rhythmic structures, as in musical meter or prosodic patterns in linguistics and poetry.Measurement and Standards
Core Concepts of Metrics in Measurement
A metric serves as a quantitative standard or scale for assessing size, amount, or degree of a physical quantity, enabling consistent comparison and evaluation across observations.[2] The term originates from the Greek word "metron," meaning "measure," which underscores its foundational role in systematizing quantification.[3] The historical evolution of metrics traces back to ancient civilizations, where early systems emerged to facilitate trade, construction, and agriculture. In ancient Egypt around 3000 BCE, the cubit—defined as the length from elbow to fingertip—served as a primary unit for measuring land and building monuments like the pyramids, while Babylonian systems from the 2nd millennium BCE introduced sexagesimal divisions for lengths and weights, influencing later Mesopotamian standards.[4] These localized metrics varied by region, leading to inconsistencies in commerce until the Enlightenment era prompted standardization; in the 1790s, French scientists developed the metric system based on decimal divisions and natural references, such as the Earth's meridian, to create universal units.[5] Central to effective metrics are key principles that ensure reliability in measurement processes: accuracy, which measures how closely a result aligns with the true value; precision, indicating the consistency of repeated measurements; reproducibility, allowing independent verification under similar conditions; and calibration, which traces instruments back to reference standards to minimize errors.[6] These principles, formalized in metrology practices, underpin the trustworthiness of quantitative data across disciplines.[7] Basic metrics include length, measured by the meter; mass, by the kilogram; and time, by the second, which collectively form the foundation for derived units through multiplication or division, such as area from length squared or density from mass per volume.[2] In everyday quantification, these enable practical applications like speed in kilometers per hour, combining length and time, or temperature in degrees Celsius, scaling thermal expansion relative to water's freezing and boiling points.[8] This conceptual framework evolved into the formal International System of Units, providing a cohesive global standard.[2]International Metric System (SI Units)
The International System of Units, abbreviated as SI from the French Système International d'Unités, is the modern form of the metric system and serves as the world's most widely used framework for measurement in science, industry, and commerce. It was formally established in 1960 by the 11th General Conference on Weights and Measures (CGPM) through Resolution 12, which defined the SI as a coherent system based on six initial base units (later expanded to seven) and introduced standardized prefixes for multiples and submultiples.[9] The SI's development traces back to the Metre Convention of 1875, a treaty signed by 17 nations in Paris that created the International Bureau of Weights and Measures (BIPM) to maintain global measurement standards and promote the metric system internationally.[10] The SI comprises seven base units, each defined precisely since the 2019 revision to ensure invariance and universality by linking them to fundamental physical constants rather than artifacts or physical prototypes. These units cover the fundamental quantities of length, mass, time, electric current, thermodynamic temperature, amount of substance, and luminous intensity. The definitions, adopted via CGPM Resolution 1 in 2018 and effective from May 20, 2019, are as follows:| Quantity | Base Unit | Symbol | Definition |
|---|---|---|---|
| Length | metre | m | The distance traveled by light in vacuum in 1/299,792,458 of a second, with the speed of light fixed at exactly 299,792,458 m/s. |
| Mass | kilogram | kg | Defined by fixing the Planck constant to exactly 6.626 070 15 × 10⁻³⁴ J s. |
| Time | second | s | The duration of 9,192,631,770 periods of radiation corresponding to the transition between two hyperfine levels of the caesium-133 atom at rest at 0 K. |
| Electric current | ampere | A | Defined by fixing the elementary charge to exactly 1.602 176 634 × 10⁻¹⁹ C. |
| Thermodynamic temperature | kelvin | K | Defined by fixing the Boltzmann constant to exactly 1.380 649 × 10⁻²³ J/K. |
| Amount of substance | mole | mol | Defined by fixing the Avogadro constant to exactly 6.022 140 76 × 10²³ mol⁻¹. |
| Luminous intensity | candela | cd | Defined by fixing the luminous efficacy of monochromatic radiation at 540 × 10¹² Hz to exactly 683 lm/W. |
Mathematics
Metric Spaces and Distance Functions
A metric space is a fundamental mathematical structure consisting of a set X equipped with a metric d: X \times X \to [0, \infty), which is a function that quantifies the distance between elements of X. This concept provides an abstract framework for studying notions of distance, convergence, and continuity without relying on specific coordinate systems or embeddings in higher-dimensional spaces.[14][15] The metric d must satisfy four axioms for all x, y, z \in X:- Non-negativity: d(x, y) \geq 0, with equality if and only if x = y (identity of indiscernibles).
- Symmetry: d(x, y) = d(y, x).
- Triangle inequality: d(x, z) \leq d(x, y) + d(y, z).