Hydrogen and helium are exceptions to the octet rule in chemical bonding. Hydrogen can either gain one electron to achieve a duet configuration or lose one electron to be left with a single electron. Helium is already stable with two electrons in its outer shell.
The terrestrial planets are closer to the sun, smaller in size, and have solid surfaces made of rock and metal. Jovian planets are further from the sun, larger in size, and primarily composed of hydrogen and helium gas with no solid surfaces.
Hydrogen has 1 electron in its outer shell. other elemnts also have just one electron in their outer shell, the alkali metals, group1; lithium, sodium potassium, rubidium, caesium, frankium the coinage metals, group 11; copper, silver, gold
Different planets have different atmospheres due to variations in their composition and distance from the sun. Factors like the planet's size, gravity, and proximity to the sun determine what gases are retained in the atmosphere, leading to unique compositions. Active processes like volcanic activity and biological activity can also contribute to the diversity of atmospheric compositions across planets.
Helium has 2 valence electrons and has completely filled orbitals / shells and helium is stable.
Planets near the sun likely lost lighter elements like hydrogen and helium due to the sun's high temperature and solar wind. These elements were blown away, leaving behind the heavier elements that make up the terrestrial planets closer to the sun.
Helium is already stable. Hydrogen should gain or lose one electron to be stable.
It is hydrogen element. It is tritium isotope of hydrogen.
Jupiter is a gas giant and does not "die" in the traditional sense. It is made up primarily of hydrogen and helium, similar to a star. If Jupiter were to somehow lose its gas and dissipate, it would not have a direct impact on our solar system, since it does not support life as we know it.
The only neutral atom with two electrons is helium; however, lithium will lose one electron when becoming an ion to have two electrons. Hydrogen can also gain an electron (compounds called hydrides) to have two electrons also.
Acids lose hydrogen ions when they donate them in a chemical reaction, making them stronger acids.
When hydrogen forms an ion, it is most likely to have a charge of +1, forming a hydrogen ion (H+). This is because hydrogen has one electron in its outer shell, so it tends to lose this electron to achieve a stable electron configuration similar to that of helium.
The inner planets are closer to the sun and the heat from the sun caused the lighter elements to be blown away, leaving behind heavier elements. The outer planets are further away from the sun, so the lighter gases were able to remain and accumulate to form gas giants.
Early Earth likely lost most of its hydrogen and helium because they are lightweight gases that could escape the planet's gravity due to their high kinetic energy. This loss likely occurred during the early stages of Earth's formation when the planet was still molten and experiencing intense heat.
Hydrogen and helium are exceptions to the octet rule in chemical bonding. Hydrogen can either gain one electron to achieve a duet configuration or lose one electron to be left with a single electron. Helium is already stable with two electrons in its outer shell.
The terrestrial planets are closer to the sun, smaller in size, and have solid surfaces made of rock and metal. Jovian planets are further from the sun, larger in size, and primarily composed of hydrogen and helium gas with no solid surfaces.
As stars grow older, they lose energy. The sun is growing older and it is losing hydrogen and helium (the gases on the outer region). When the sun loses all of its energy it explodes. It then becomes a black dwarf.