That depends on the definition of T'2
Period = wavelength/speed
Well, let's see:Force of gravity = G M1 M2 / R2So G = (force) x (distance)2 / (mass)2 = (M L / T2) x (L2) / (M2) = (M L3) / (M2 T2) =(Length)3 (Mass)-1(Time)-2
the period is 2pi. period is 2pi/b and the formula is y=AsinBx.
The ratio of the quantity between two sets of time an equal period apart are the same. That is, the rate of growth over the same time is a constant. Suppose V(t) is the value of the variable V at time t. Then, if t1, t2, t3 and t4 are four times such that t2 - t1 = t4 - t3 then V(t2)/V(t1) = V(t4)/V(t3) whether V is compound interest or exponential growth.
by using the formula we will calculat time period of simple harmonic motion
Gay-Lussac's law states that the pressure of a gas is directly proportional to its temperature at constant volume. The formula is P1/T1 = P2/T2, where P1 and T1 are the initial pressure and temperature, and P2 is the final pressure.
The formula for pulley is T1/T2 = R1/R2, where T1 and T2 are the tensions in the ropes on each side of the pulley, and R1 and R2 are the radii of the pulley on each side.
V1/T1 = V2/T2 Where temperature must be in Kelvins 67C + 273 = 340 K So 140/340 = 50/T2 Find T2 340/140(50) = T2 T2 = 121 K or -152C
The Charles' Law formula is V1/T1 = V2/T2, where V is volume and T is temperature. This formula describes the relationship between the volume of a gas and its temperature at constant pressure.
To solve Gay-Lussac's Law, use the formula P1/T1 P2/T2, where P1 and T1 are the initial pressure and temperature, and P2 and T2 are the final pressure and temperature. Rearrange the formula to solve for the unknown variable.
Formula for the nth term of general geometric sequence tn = t1 x r(n - 1) For n = 2, we have: t2 = t1 x r(2 - 1) t2 = t1r substitute 11.304 for t2, and 2.512 for t1 into the formula; 11.304 = 2.512r r = 4.5 Check:
To calculate the orbital period of a planet, you can use Kepler's third law of planetary motion. The formula is T2 (42 r3) / (G M), where T is the orbital period, r is the average distance from the planet to the sun, G is the gravitational constant, and M is the mass of the sun. Simply plug in the values for r and M to find the orbital period of the planet.
There is a more complex formula that cannot be printed here, but for the sake of simplicity, you can consider the period T to be proportional to the square root of the length of the pendulum L. If L is halved, then T2 is proportional to the square root of 1/2, or approximately 0.707 times T1.
The formula to calculate the final temperature when equal masses of water are mixed is: Final temperature = (m1 x T1 + m2 x T2) / (m1 + m2), where m1 and T1 are the mass and initial temperature of the first sample of water, and m2 and T2 are the mass and initial temperature of the second sample of water.
Formula for the Payback Period. Payback period = Initial investment / Annual Cash inflows
The Combined Gas Law relates pressure (P), volume (V) and temperature (T). The appropriate SI units are P in atm, V in liters, and T in degrees Kelvin. The Combined Gas Law equation is (P1*V1)/T1 = (P2V2)/T2. Isolating for V2 the equation then becomes (P1V1T2)/(T1P2) = V2
T1 = 273.15K. T2 = 410.15K. V1 = 350mL. V2 = ? P1 = P2. Since pressure is constant you can use the formula. V1/T1 = V2/T2 Rearrange the formula to get: V2 = T2V1/T1