Answer:
The depth and acceleration are 0.1919291 ft and 3.61 m/s².
Explanation:
Given that,
Density of block 
Density of fluid 
We need to calculate the depth
Using balance equation
....(I)
We know that,
The density is


Put the value of m in equation (I)



Put the value into the formula



We need to calculate the acceleration
Using formula of net force



....(II)
Put the value in the equation (II)


Hence, The depth and acceleration are 0.1919291 ft and 3.61 m/s².
Heat the tea because the heat make the tea's particles move around more dissolving the sugar quicker
The answer is axial precession. Axial precession refers to
the very slow motion of the Earth’s axis, which almost requires twenty-six
thousand (26,000) years to complete a full rotation. This Axial Precession is
caused by the effects of gravitational pull from the Sun and the Moon towards
the Earth.
Answer:
Solar eclipses may be classified as either total, in which the Moon completely covers the Sun, or annular, in which the Moon obscures all but an outer ring of the Sun.
The answer is going be desert.