
The rate at which an object covers distance, a scalar quantity.Speed is the rate at which an object covers distance, defined as the distance traveled divided by the time taken. It is a scalar quantity, meaning it has magnitude but no direction, unlike velocity which includes direction. In everyday life, speed is what a car's speedometer shows, and in physics it is fundamental to describing motion, from a falling apple to a speeding photon.
The concept of speed has been used since antiquity, but Galileo Galilei in the early 17th century formalized the relationship between distance, time, and speed, laying groundwork for classical mechanics.
Speed is calculated as the total distance traveled divided by the elapsed time, giving an average speed. Instantaneous speed is the limit of this ratio as the time interval approaches zero, which is the magnitude of the instantaneous velocity vector. In uniform motion, speed is constant; in accelerated motion, it changes over time.
Speed is used in navigation, traffic engineering, sports analytics, and in physics to calculate kinetic energy (½mv²) and to determine travel times in space missions.
The speed of light in a vacuum is exactly 299,792,458 meters per second, a fixed constant that defines the meter itself since 1983.
| k | variable | thermal conductivity — thermal conductivity watt per metre per kelvin |
| C | variable | heat capacity per unit volume — volumetric heat capacity joule per cubic metre per kelvin |
| v | variable | average particle speed — speed metre per second |
| l | variable | mean free path — mean free path metre |
| \Omega | variable | Berry curvature — berry curvature square metre |
| m | variable | electron mass — mass kilogram |
| c | variable | speed of light in vacuum — speed metre per second |
| r_H | variable | Accretion horizon radius — radius metre |
| \dot{M} | variable | Mass accretion rate — mass flow rate kilogram per second |
| \rho | variable | Mass density of accreting material — mass density kilogram per cubic metre |
| c_s | variable | Sound speed in accreting material — speed metre per second |
| c_coord | variable | Coordinate speed of light — speed metre per second |
| c | variable | Speed of light in vacuum — speed of light metre per second |
| g_tt | variable | Time-time component of metric tensor — metric tensor component |
| g_rr | variable | Radial-radial component of metric tensor — metric tensor component |
| √ | operator | Square root operation — square root operator |
| \Gamma_1 | variable | First adiabatic index — adiabatic index |
| M | variable | Mass of the star — mass kilogram |
| R | variable | Radius of the star — radius metre |
| c | variable | Speed of light — speed metre per second |
| G | constant | Newtonian gravitational constant — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared |
| k | constant | Numerical constant of order unity depending on stellar structure — structure constant = 1 |
| L_{\rm Edd} | variable | Eddington luminosity — luminosity watt |
| M | variable | Mass of the object — mass kilogram |
| c | variable | Speed of light — speed metre per second |
| G | constant | Newtonian gravitational constant — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared |
| \kappa | constant | Opacity of the stellar material — opacity = 0.034 square metre per kilogram |






