Use the equation below: __ yd*3 ft 1 yd=? ft
D = M/V Density = Mass divided by Volume
Speed = Distrance / time
If you know the distance then you use the equation d = x0 + v0t = 1/2 at2 if the object starts from rest then v0 = 0 If the object starts at zero distance the x0 = 0 d = 1/2 at2 Squareroot(2d/a) = t
because we use it to calculate/measure things in science for example we use maths to calculate the distance of stars from the earth
To calculate distance with velocity and weight, you can use the equation for work: Work = Force x Distance. The force can be calculated by multiplying the weight with gravity. Velocity can then be used to determine the time it takes for the object to travel that distance using the equation Distance = Velocity x Time.
To calculate the position of an image formed by a lens or mirror, you can use the thin 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. By solving this equation, you can determine the image position relative to the lens or mirror.
Use the equation Absolute magnitude=Apparent Magnitude+5 -(5x Log x Distance)
Use the equation below: __ yd*3 ft 1 yd=? ft
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I can remember a bit of this. You have to use the equation : Velococity = Distance divided by time. You have to use a device called a hydroprop. You place it in the water and time how long it takes for the propeller to move from one distance to another. Then you meausere the distance and use the equation. This is one of the best ways to do this but you can use many others which may be not as good. such as a ruber duck and time it over a set distance. Thanks
It depends on how long a distance you want to measure!
yea
Use the Equation of State (EOS) in combination with the Antoine's Equation to determine vapor pressure.
The equation to calculate object momentum is: p = m * v where p is momentum, m is mass of the object, and v is the velocity of the object.
To calculate the image position when given magnification by a concave mirror, you can use the mirror equation: 1/f = 1/d_o + 1/d_i, where f is the focal length of the mirror, d_o is the object distance, and d_i is the image distance. Magnification, M, is also given by -d_i/d_o. By substituting the values of magnification and focal length into the mirror equation, you can solve for the image distance and then determine the image position.
Scientists would use the Doppler Effect to calculate the distance to a Star which had the newly-discovered planet.