Usually, gravitational collapse of the protostar is stopped after hydrogen fusion starts in the center. Then gravitational forces and radiation pressure are in equilibrium.
In order to get star coins in the game Star Stable, you will need to purchase the star coins. They are much like the games form of currency. You can purchase them via PayPal.
Star of the East
Nebula.
When a star explodes in a supernova, its core can collapse into either a neutron star or a black hole, depending on the mass of the original star. For stars with masses less than about 3 times that of the Sun, the core collapses into a neutron star, which is an extremely dense and compact object. For more massive stars, the core collapses further into a singularity, forming a black hole.
The main sequence stage is the most stable stage in a star's life cycle. During this stage, a star fuses hydrogen into helium in its core, maintaining a stable balance between gravity pulling inward and the energy produced by nuclear fusion pushing outward. This equilibrium allows the star to shine steadily for billions of years.
Unlike the sodium and chlorine, some atoms become more stable by sharing electrons and therefore form the ionic compounds.
The main reasons of atoms forming bonds are: * To become stable * to fulfill their outer shell * to form compounds
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Sulfur gains 2 electrons to become stable.
A chlorine atom needs one additional electron in order to become stable.
To become more stable, calcium is likely to lose two electrons to achieve a full outer shell of electrons, forming a positive 2+ ion.
An alkaline earth metal would typically lose two electrons to become stable. This would result in the metal forming a 2+ cation, as it will have the same electron configuration as the nearest noble gas.
78 percent of the material that did not go to the sun, went to jupiter.
A star that is forming is called a protostar.
Atoms become stable by gaining or losing electrons to achieve a full outer electron shell. This involves forming bonds with other atoms to share or transfer electrons. Once the outer shell is full, the atom is more stable and less likely to react with other atoms.
please define what kind of stability: chemical, physical and isotopic stability are different. assuming diatomic molecular nitrogen it is stable up to about 1000C at atmospheric pressures.