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The light hydrogen and helium gasses were swept out of the inner solar system by the intense solar wind of the young sun. The outer planets retained the hydrogen and helium as the solar wind diminished with distance.

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Q: Why did the inner planets lose their hydrogen and helium?
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What did the planets near the sun lose because of the sun's temperature?

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.


How many electrons does it take for hydrogen and helium to become stable?

Helium is already stable. Hydrogen should gain or lose one electron to be stable.


What element has 1 protons 1 neutrons and 2 electrons?

It is hydrogen element. It is tritium isotope of hydrogen.


What will happen if Jupiter dies?

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.


What element has two electrons?

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.


Do acids lose or gain hydrogen ions?

Acids lose hydrogen ions when they donate them in a chemical reaction, making them stronger acids.


What is the most likely charge on an ion when hydrogen forms an ion?

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.


Why are the inner planets composed of heavy elements and outer planets composed of gas?

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.


Why did early earth lose most of the hydrogen and helium that most likely made up the first atmosphere?

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.


What rule are hydrogen and helium excepted from?

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.


What separates the terrestrial and jovian planets?

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.


Why are the inner planets dense and small while the outer planets are gas giants?

The inner planets are dense and small because they formed closer to the Sun where high temperatures caused heavier materials to condense. The outer planets are gas giants because they formed farther from the Sun where it was colder, allowing lighter gases like hydrogen and helium to dominate their composition.