Critical Initial Mass Function of the Sun

Critical Initial Mass Function of the Sun
Yesterday we discussed the question of what real creation is about. Our point was that the study of real creation involves the study of how time, space, and matter/energy came into existence. Those sciences are in the embryonic stage, but they point to there being a purpose that involves wisdom and contributes to our understanding of the nature of God. One important finding of the study of creation is the critical initial mass function of the Sun.

As we study the Sun, we see that much is unique about our star. It is not just an average star of the billions formed from the “big bang” and classified in the Hertzsprung-Russell diagram. As we watch stars forming today and, as we look at the composition of the galaxy we live in, much stands out in our understanding of the Sun. Our mathematics indicate that there is what we call a critical initial mass function of the Sun, or IMF for short. IMF is the mass needed for star formation to take place. When stars begin to form from the material in the creation, they must have enough mass to allow gravity to fuse hydrogen into helium. If that mass isn’t there, what you have is a brown dwarf. If the mass is .08 of the solar mass, a red dwarf will form.

There are roughly 400 billion stars in the Milky Way, and 300 billion of them are red dwarfs – also called M dwarfs because of their spectral identification. There are roughly 15,000 places in our Milky Way galaxy where we see stars forming, so we can watch the way in which the IMF functions. When our Sun was formed, an IMF had to be carefully chosen so that it would produce a spectral G type star. Other star types such as O, B or F types would be too hot, too active and have too short of a lifespan. The most numerous stars in our galaxy – the red dwarfs mentioned earlier – have similar difficulties with their activity including stellar flares and coronal mass ejections. None of these types of stars can be seen as possible solar systems where life could exist.

The critical initial mass function of the Sun seems to be fine-tuned for life to exist. While we may have believed that by faith for many years, we now have scientific evidence to support that belief.
–John N. Clayton © 2019

Reference: Astronomy February 2019, page 21-27.