Answer:
Reflection is like bouncing a tennis ball, and absorption is like water soaking into a paper towel.
Explanation:
So first of all a simile uses the words "like" or "as" to compare things. Reflection is like bouncing a tennis ball, and absorption is like water soaking into a paper towel.
 
        
                    
             
        
        
        
Answer:
C. Cohesion of molecules 
Explanation:
Cohesion is the interaction of molecules of the same substance together. By the force of cohesion if two drops of water come together they form one. Water has high rates of cohesion due to hydrogen bonds.  
This phenomenon also called surface tension and is what allows small insects to stand on water.
Cohesion along with adhesion of water to the walls of the narrow tube generate what is called capillarity. This allows liquids to ascend inside the narrow tubes. As long as the cohesion is less than the adhesion, the liquid will rise until both forces are equal.
 
        
             
        
        
        
Answer:
The answer is below
Explanation:
The possible phenotypes of the mother can be any of the following
AA - A phenotype
AB - AB phenotype (here the mother must have contributed an A gene for it to be possible)
AO - A phenotype (here the mother may have contributed any of the A or O gene.)
BO - B phenotype (here, the mother would only need to contribute O gene for this to be possible)
 
        
             
        
        
        
D. the <span>stomata close to preserve water and gas exchange decreases.</span>
        
             
        
        
        
Stellar evolution is the process by which a star undergoes a sequence of radical changes during its lifetime. Depending on the mass of the star, this lifetime ranges from only a few million years (for the most massive) to trillions of years (for the less massive), considerably more than the age of the universe. ^ 
Small, relatively cold, low mass red dwarfs burn hydrogen slowly and will burn for hundreds of billions of years 
Massive hot supergiants will live for just a few million years. 
A mid-sized star like the Sun will remain on the main sequence for about 10 billion years. Hope tis helps!!