Linear expansivity is a type of thermal expansion. It is described by a fraction that represents the fractional increase in length of a thin beam of a material exposed to a temperature increase of one degree Celsius. ... Linear expansivity is used in many real world applications.
Potential Energy (Initial one) = m * g * h
P.E. = 60 * 9.8 * 10
P.E. = 5880
Kinetic Energy (Final One) = 1/2 mv²
K.E. = 1/2 * 60 * (10)²
K.E. = 6000/2
K.E. = 3000
Lost Energy = 5880 - 3000 = 2880 J
In short, Your Answer would be 2880 Joules
Hope this helps!
The pressure exerted by the block on the table is given by:
![p=\frac{W}{A}](https://tex.z-dn.net/?f=%20p%3D%5Cfrac%7BW%7D%7BA%7D%20%20)
where W is the weight of the box, and A is the bottom surface area of the box.
The weight of the box is: ![W=mg=(7.5 kg)(9.81 m/s^2)=73.6 N](https://tex.z-dn.net/?f=%20W%3Dmg%3D%287.5%20kg%29%289.81%20m%2Fs%5E2%29%3D73.6%20N%20)
Substituting into the first equation, we find the pressure:
![p=\frac{W}{A}=\frac{73.6 N}{0.6 m^2}=122.7 Pa](https://tex.z-dn.net/?f=%20p%3D%5Cfrac%7BW%7D%7BA%7D%3D%5Cfrac%7B73.6%20N%7D%7B0.6%20m%5E2%7D%3D122.7%20Pa%20%20%20)
When supernova explodes
because of the collapsing cores, the core itself will become a neutron star or
a white dwarf without undergoing any kind of explosive transformation. The white
dwarf stars can also become supernova if they orbit another star in a binary
system and steal material from their companion. In addition, the end state of a
star, whether it will explode as a supernova become a black hole.