![earth earth](https://blogs.esa.int/rocketscience/files/2016/03/esa_esoc_flight_dynamics_exomars-TGO_heliocentric_travelled_distance.jpg)
When calculating the angular velocity of the Earth as it completes a full rotation on its own axis (a solar day), this equation is represented as: ω avg = 2πrad/1day (86400 seconds), which works out to a moderate angular velocity of 7.2921159 × 10 -5 radians/second. Mathematically, the average angular velocity of an object can be represented by the following equation: ω average= Δθ/Δt, where ω is the radians/revolutions per second (on average), Δ is the change in quantity, θ is the velocity, and t is time. In addition, when an object rotating about an axis, every point on the object has the same angular velocity.
![earth earth](https://media.cheggcdn.com/media%2Fbb6%2Fbb6fe5bc-23e7-4a3a-89a5-20cde445aa0b%2Fimage.png)
However, it is sometimes also called the rotational velocity and its magnitude – the rotational speed – is typically measured in cycles or rotations per unit time (e.g. A full radian is 360 degrees, hence we know that the Earth performs two radians when performing a full rotation around an axis. A radian, by definition, is a unit which connects the radius of an arc, the length of the arc and the angle subtended by the arc. and is usually represented by the symbol omega (ω, rarely Ω). The SI unit of angular velocity is radians per second, although it may be measured in other units such as degrees per second, revolutions per second, etc. In physics, the angular velocity is a vector quantity which specifies the angular speed of an object and the axis about which the object is rotating. This applies equally to the Earth rotating around the axis of the Sun and the center of the Milky Way Galaxy. When it comes to the Earth rotating on its axis, a process which takes 23 hours, 56 minutes and 4.09 seconds, the process is known as a sidereal day, and the speed at which it moves is known as the Earth’s Angular Velocity. In each case, scientists have striven to calculate not only the time it takes, but the relative velocities involved.
![earth earth](https://www.science.org/cms/10.1126/sciadv.abe1358/asset/1a48415a-84d9-4673-8f62-ca1ab0822284/assets/graphic/abe1358-f1.jpeg)
The planet Earth has three motions: it rotates about its axis, which gives us day and night it revolves around the sun, giving us the seasons of the year, and through the Milky Way along with the rest of the Solar System.