Answer:
A 70 kg box is slid along the floor by a 400 n force. The coefficient of friction between the box and the floor is 0. 50 when the box is sliding
Because they behave just like all the electromagnetic waves of the spectrum. Same equations, just shorter wavelengths and more energy.
Hope you get it :)
Answer:
f = 632 Hz
Explanation:
As we know that for destructive interference the path difference from two loud speakers must be equal to the odd multiple of half of the wavelength
here we know that
![\Delta x = (2n + 1)\frac{\lambda}{2}](https://tex.z-dn.net/?f=%5CDelta%20x%20%3D%20%282n%20%2B%201%29%5Cfrac%7B%5Clambda%7D%7B2%7D)
given that path difference from two loud speakers is given as
![\Delta x = 5.80 m - 3.90 m](https://tex.z-dn.net/?f=%5CDelta%20x%20%3D%205.80%20m%20-%203.90%20m)
![\Delta x = 1.90 m](https://tex.z-dn.net/?f=%5CDelta%20x%20%3D%201.90%20m)
now we know that it will have fourth lowest frequency at which destructive interference will occurs
so here we have
![\Delta x = 1.90 = \frac{7\lambda}{2}](https://tex.z-dn.net/?f=%5CDelta%20x%20%3D%201.90%20%3D%20%5Cfrac%7B7%5Clambda%7D%7B2%7D)
![\lambda = \frac{2 \times 1.90}{7}](https://tex.z-dn.net/?f=%5Clambda%20%3D%20%5Cfrac%7B2%20%5Ctimes%201.90%7D%7B7%7D)
![\lambda = 0.54 m](https://tex.z-dn.net/?f=%5Clambda%20%3D%200.54%20m)
now for frequency we know that
![f = \frac{v}{\lambda}](https://tex.z-dn.net/?f=f%20%3D%20%5Cfrac%7Bv%7D%7B%5Clambda%7D)
![f = \frac{343}{0.54} = 632 Hz](https://tex.z-dn.net/?f=f%20%3D%20%5Cfrac%7B343%7D%7B0.54%7D%20%3D%20632%20Hz)
Kepler's third law is used to determine the relationship between the orbital period of a planet and the radius of the planet.
The distance of the earth from the sun is
.
<h3>
What is Kepler's third law?</h3>
Kepler's Third Law states that the square of the orbital period of a planet is directly proportional to the cube of the radius of their orbits. It means that the period for a planet to orbit the Sun increases rapidly with the radius of its orbit.
![T^2 \propto R^3](https://tex.z-dn.net/?f=T%5E2%20%5Cpropto%20R%5E3)
Given that Mars’s orbital period T is 687 days, and Mars’s distance from the Sun R is 2.279 × 10^11 m.
By using Kepler's third law, this can be written as,
![T^2 \propto R^3](https://tex.z-dn.net/?f=T%5E2%20%5Cpropto%20R%5E3)
![T^2 = kR^3](https://tex.z-dn.net/?f=T%5E2%20%3D%20kR%5E3)
Substituting the values, we get the value of constant k for mars.
![687^2 = k\times (2.279 \times 10^{11})^3](https://tex.z-dn.net/?f=687%5E2%20%3D%20k%5Ctimes%20%282.279%20%5Ctimes%2010%5E%7B11%7D%29%5E3)
![k = 3.92 \times 10^{-29}](https://tex.z-dn.net/?f=k%20%3D%203.92%20%5Ctimes%2010%5E%7B-29%7D)
The value of constant k is the same for Earth as well, also we know that the orbital period for Earth is 365 days. So the R is calculated as given below.
![365^3 = 3.92\times 10^{-29} R^3](https://tex.z-dn.net/?f=365%5E3%20%3D%203.92%5Ctimes%2010%5E%7B-29%7D%20R%5E3)
![R^3 = 3.39 \times 10^{33}](https://tex.z-dn.net/?f=R%5E3%20%3D%203.39%20%5Ctimes%2010%5E%7B33%7D)
![R= 1.50 \times 10^{11}\;\rm m](https://tex.z-dn.net/?f=R%3D%201.50%20%5Ctimes%2010%5E%7B11%7D%5C%3B%5Crm%20m)
Hence we can conclude that the distance of the earth from the sun is
.
To know more about Kepler's third law, follow the link given below.
brainly.com/question/7783290.