Distance = (speed) multiplied by (time)
an object uniformly accerlerates over a distance of 100 m in 20 seconds. calculate the acceleration.
That number is what we call the object's "speed".
0.7848 meter
Speed = (distance traveled) divided by (time to cover the distance) Speed = (50 meters) / (2 seconds) Speed = 50 meters per 2 seconds Speed = 25 meters per second
Assuming the object starts from rest, the distance an object falls in 0.25 seconds can be calculated using the equation ( d = \frac{1}{2}gt^2 ), where (d) is the distance, (g) is the acceleration due to gravity (9.8 m/s²), and (t) is the time. Substituting the values, the object would fall approximately 0.31 meters in 0.25 seconds.
The equation to calculate the speed of an object is speed = distance / time. This equation gives the rate at which an object is moving over a given distance in a specific amount of time.
The kinematics equation for distance is: distance initial velocity time 0.5 acceleration time2. This equation is used to calculate the displacement of an object in motion by plugging in the values of initial velocity, time, and acceleration to find the total distance traveled by the object.
Speed=Distance travelled by the object /Time taken to cover the distance.
The focal length of a lens is related to the object distance and image distance by the lens equation: 1/f = 1/do + 1/di, where f is the focal length, do is the object distance, and di is the image distance. This equation describes how the lens focuses light rays from an object at a certain distance to form an image at a specific distance.
In optics, the relationship between image distance and object distance is described by the lens equation: 1/f 1/di 1/do, where f is the focal length of the lens, di is the image distance, and do is the object distance. This equation shows that as the object distance changes, the image distance also changes in a reciprocal manner.
The distance equation in kinematics is: distance initial velocity x time 0.5 x acceleration x time2. This equation is used to calculate the total distance traveled by an object in motion by taking into account the initial velocity, time elapsed, and acceleration of the object. By plugging in the values for these variables, one can determine the distance covered by the object during its motion.
Distance = (speed) multiplied by (time)
The magnification equation for a concave mirror is given by the formula: M = - (image distance) / (object distance), where M is the magnification, image distance is the distance from the mirror to the image, and object distance is the distance from the mirror to the object. Negative magnification indicates an inverted image.
The small angle formula is used for measuring the distance to a far away object when the actual size and angular size are known, or for finding out the actual size of a faraway object when the distance to the object and angular size are known. In arc-seconds: a = 206265 x D/d where a = the angular size of the object in arc-seconds D = the actual linear size of an object in km d = the distance to the object in km 206265 = the number of arc-seconds in a complete circle divided by 2pi In Radians: a = D/d where a = angular size of object in radians
To find the distance traveled in the first 5 seconds, we multiply the average velocity by the time traveled. If the object's velocity is constant, this distance is equal to the velocity multiplied by the time.
The thin lens equation is a relation that describes how the distance of an object from a thin lens, the distance of the image from the lens, and the focal length of the lens are related. The equation is given by 1/f = 1/do + 1/di, where f is the focal length of the lens, do is the object distance, and di is the image distance.