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Interstellar oxygen

Oxygen found in the interstellar medium

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Interstellar oxygen refers to the presence of the element oxygen (atomic or molecular) found in interstellar space. Oxygen is common, being the third most abundant element in the universe after hydrogen and helium. It is often found as neutral or ionized atomic gas and as a constituent of molecular gas, volatile ices, and minerals in dust. Interstellar oxygen in dust is primarily found in the form of silicates. These molecules are created inside evolved stars which then eject it into space when they start to shed their outer layers. They are then incorporated into large molecular clouds that collapse to form star systems like the Solar System.

01Missing oxygen

The total amount of oxygen in the interstellar medium of the Milky Way galaxy is mostly unknown but studies have shown that there seems to be a depletion of oxygen. This missing oxygen problem is not solved and has been dubbed the ‘oxygen crisis’ or ‘O-crisis’. This problem can not be solved with the combined contributions of carbon monoxide, ices, and silicate and oxide dust. It's possible that a significant fraction of the missing oxygen is found in organic carbonate solids.

The Sun seems to have a slight overabundance of oxygen.

02Scientific importance

The study of oxygen located in interstellar space is important for a variety of reasons. Oxygen is abundant in the Solar System which it got from the Solar nebula which collapsed to form the Solar System.

The thermal or photolytic decomposition of carbonates may also form carbon dioxide in the interstellar medium.

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Sources and credits

This article is adapted from the Wikipedia article Interstellar oxygen, written by its contributors and licensed under CC BY-SA 4.0. Fathomly has changed the layout, removed citation markers, navigation and maintenance notices, and adjusted punctuation. This adapted version is shared under the same license. For references, see the original article.

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