Answer:
Explanation:
fundamental frequency, f = 250 Hz 
Let T be the tension in the string and length of the string is l ans m be the mass of the string initially. 
the formula for the frequency is given by 
 .... (1)
    .... (1) 
Now the length is doubled ans the tension is four times but the mass remains same. 
let the frequency is f' 
 .... (2)
    .... (2) 
Divide equation (2) by equation (1) 
f' = √2 x f 
f' = 1.414 x 250 
f' = 353.5 Hz
 
        
             
        
        
        
Hello,
The answer is option A "Venus".
Reason:
The planet Venus spins the wrong way many scientists are not sure why. Its not options B, C, or D because these planets spin the same way the as each other. (besides Venus) Therefore the answer is option A.
If you need anymore help feel free to ask me!
Hope this helps!
~Nonportrit
        
                    
             
        
        
        
Answer:
Explanation:
Block A sits on block B and force is applied on block A . Block A will experience two forces 1) force P and 2 )  friction force in opposite direction of motion . Block B will experience one force that is force of friction in the direction of motion . 
Let force on block A be P . friction force on it will be equal to kinetic friction, that is μ mg , where μ is coefficient of friction and m is mass of block A 
friction force = .4 x 2.5 x 9.8 
= 9.8 N 
net force on block A = P - 9.8 
acceleration = ( P - 9.8 ) / 2.5 
force on block B = 9.8 
acceleration = force / mass 
= 9.8 / 6 
for common acceleration 
 ( P - 9.8 ) / 2.5  = 9.8 / 6
( P - 9.8 ) / 2.5 = 1.63333
P = 13.88 N . 
 
        
             
        
        
        
You could certainly have some good easy going carefree conversation with your sister or your cousin at dinner or at a movie, but relative dating is not an effective way to get serious and find a life partner.
        
             
        
        
        
Everything starts from spectroscopy. Astronomers only have concentrated information at wavelengths that are emitted from the stars. What they do with this information is to obtain the frequency range of the stars and through spectroscopes they are responsible for dividing the radiation beams and determining the coincidence with the emission of those same waves, of chemical elements. From these observation techniques it is possible to obtain the composition and according to the color, obtaining characteristics such as temperature. The spectrum of stars consists of dark and bright lines called Fraunhofer lines. This spectrum is compared to the spectrum of different elements to find the composition of the stars. This is possible because the elements emit or absorb only specific wavelengths.