Our Sun emits most of its radiation at a wavelength of 550 nm. If a star were 3.50 times hotter than our Sun, it would emit most of its radiation at a wavelength of nm

The wavelength of the radiation emitted by the star is 183 nm.

Explanation:

As per Wien's displacement law, the product of emitted wavelength and temperature of the star will be equal to 2.898 × 10⁻³ mK.

So if the wavelength of the emitted radiation by Sun is given as 550 nm, then the temperature of the Sun will be

Then if the temperature of star is said to be 3.5 times hotter than Sun, then the temperature of Star = 3.5×5.27×10³ = 15.81×10³ K.

With this temperature, the wavelength of the emitted radiation can be found as follows:

So, the wavelength of the radiation emitted by the star is 183 nm.

the displacement produced by the body.  

the amount of force subjected to the body.  

the angle between the direction of force and displacement

float.

archimedes' principle

denser than water sinks in water.

denser than mercury would sink in it