Answer: f=150cm in water and f=60cm in air.
Explanation: Focal length is a measurement of how strong light is converged or diverged by a system. To find the variable, it can be used the formula:
 = (nglass - ni)(
 - 
).
nglass is the index of refraction of the glass;
ni is the index of refraction of the medium you want, water in this case;
R1 is the curvature through which light enters the lens;
R2 is the curvature of the surface which it exits the lens;
Substituting and calculating for water (nwater = 1.3):
 = (1.5 - 1.3)(
 - 
)
 = 0.2(
)
f = 
 = 150
For air (nair = 1):
 = (1.5 - 1)(
 - 
)
f = 
 = 60
In water, the focal length of the lens is f = 150cm.
In air, f = 60cm.
 
        
                    
             
        
        
        
It would be: 40 + 272 = 313 K
In short, Your Answer would be Option A
Hope this helps!
        
             
        
        
        
Answer:Twice of given mass
Explanation:
Given
Two Particles of Equal mass placed at the base of an equilateral Triangle 
let mass of two equal masses be m and third mass be m'
Taking one of the masses at origin
Therefore co-ordinates of first mass be (0,0)
Co-ordinates of other equal mass is (a,0)
if a is the length of triangle
co-ordinates of final mass 
Given its center of mass is at midway between base and third vertex therefore






 
        
             
        
        
        
Answer:
The angle between two just-resolvable stars for the Arecibo telescope is 
.
Explanation:
The resulting image in a telescope obtained from an object is a diffraction pattern.
That diffraction pattern is obtained because the light encounters different obstacles on its path inside the telescope (interact with the walls and edges of the instrument).
The diffraction pattern is composed by a central disk, called Airy disk, and diffraction rings.     
  
The angular resolution is defined as the minimal separation at which two sources can be resolved one for another, or in other words, when the distance between the two diffraction patterns maxima is greater than the radius of the Airy disk.
The angular resolution can be determined in an analytical way by means of the Rayleigh criterion.          
   (1)
Where 
 is the wavelength and D is the diameter of the telescope. 
Notice that it is necessary to express the wavelength in the same units than the diameter. 
 ⇒ 
 
Finally, equation 1 can be used.
 
              
Hence, the angle between two just-resolvable stars for the Arecibo telescope is