What is the difference between a protostar and a pre-main sequence star?
A protostar is a stage in the formation of a star, when it is still in the process of accumulating matter from its surrounding cloud of gas and dust. At this stage, the temperature and pressure in the core of the protostar are not yet high enough to initiate nuclear fusion reactions, which would produce the energy that powers a star. As the protostar continues to accumulate matter, it becomes denser and its temperature increases until it reaches the point where nuclear fusion can begin. This marks the transition to the next stage in the star's evolution, the pre-main sequence.
A pre-main sequence star is a young star that has just begun nuclear fusion in its core. At this stage, the star is not yet in hydrostatic equilibrium, meaning that the inward force of gravity is still greater than the outward pressure produced by the fusion reactions. This causes the star to contract, which increases its temperature and luminosity until it reaches a point of equilibrium. Once the star has reached this point, it enters the main sequence stage, where it will spend the majority of its life.
- What Is The Difference Between Postgresql And Mysql
- What Is A Lunar Eclipse
- What Is The Fee For Traveling With A Musical Instrument On My Hawaiian Airlines Flight
- What Are The Key Differences Between Ally Bank And Discover Bank
- Which Animal Can Breathe Through Its Skin
- How Do You Set Up A Landline Phone In A Home Office
- What Was The Most Significant Moment In The History Of Barney And Robins Romantic Wedding On How I Met Your Mother
- Which Series Has Better Exploration Of Politics And Power Lord Of The Rings Or Game Of Thrones
- How Do Movies Get Selected To Be Shown In Film Festivals
- What Are The Most Common Types Of Computer Viruses And How Do You Protect Against Them