g (b) Now instead assume that the Sun is pure, ionized He in the center. Find the analogous m and compute the pressure, PHeI I I, for this case

3.71 × 10^16 pascal

Explanation:

So, from the question above we are given the following condition or assumptions:

[1]. The sun is pure, and [2]. presence of ionized H in the center.

We have the sun's central density= 150 gcm^-3 and the central temperature = 1.5 * 10^7.

Without mincing words, let us dive straight into the solution to this question.

The pressure PHeI I I, for this case = 2 × 150 × 10³ × 1.38 × 10^-23 × 1.5 × 10^7/ 1.67 × 10^-27 = 3.71 × 10^16 pascal.

c is the answer because when something is left after something evaporates that shows the chemical change.