For astronomical objects, the time period can be calculated using:
T² = (4π²a³)/GM
where T is time in Earth years, a is distance in Astronomical units, M is solar mass (1 for the sun)
Thus,
T² = a³
a = ∛(29.46²)
a = 0.67 AU
1 AU = 1.496 × 10⁸ Km
0.67 * 1.496 × 10⁸ Km
= 1.43 × 10⁹ Km
Answer:
d.
Explanation:
the arrow is starts at 0,0 and ends at 2,2
Answer:
it is a constant value that does not depend on the observer
Explanation:

<h3><u>L</u><u>A</u><u>P</u><u>L</u><u>A</u><u>C</u><u>E</u><u> </u><u>L</u><u>A</u><u>W</u><u> </u><u>:</u><u>-</u></h3>
Laplace's law for the gauge pressure inside a cylindrical membrane is given by
<h3>ΔP = γ/r</h3>
<u>W</u><u>h</u><u>e</u><u>r</u><u>e</u>
γ => surface tension
r => the radius of the cylinder
Note : there is an inverse relation between the pressure and the radius.