This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility:


peer-reviewed publication

trusted source


Astronomers propose a new stellar theory to explain the origin of phosphorus

Stellar theory to explain the origin of phosphorus
Artist's impression of this research. Credit: NAOJ

Astronomers have proposed a new theory to explain the origin of phosphorus, one of the elements important for life on Earth. The theory suggests a type of stellar explosion known as "ONe novae" as a major source of phosphorus.

After the Big Bang, almost all of the matter in the universe was comprised of hydrogen. Other elements were formed later, by inside or when stars exploded in events known as novae or supernovae. But there are a variety of stars and a variety of ways they can explode. Astronomers are still trying to figure out which processes were important in creating the abundances of elements we see in the universe.

In this study, Kenji Bekki, at The University of Western Australia, and Takuji Tsujimoto, at the National Astronomical Observatory of Japan, proposed a new model based on oxygen-neon novae, denoted as "ONe novae," to explain the abundance of phosphorus. The study has been published in The Astrophysical Journal Letters.

A ONe nova occurs when matter builds up on the surface of an oxygen-neon-magnesium rich white dwarf star and is heated to the point to ignite explosive run-away nuclear fusion.

The model predicts that a large amount of phosphorus will be released in a ONe nova and that the number of novae will depend on the , specifically the , of the stars. The researchers estimate that the rate of ONe novae peaked around 8 billion years ago, meaning that phosphorus would have been readily available when the solar system started to form around 4.6 billion years ago.

The model predicts that ONe novae will produce a chlorine enhancement similar to the phosphorus enhancement. There is not yet enough for chlorine to confirm this and it provides a testable hypothesis to check the validity of the ONe novae model. Future observations of stars in the outer part of the Milky Way galaxy will provide the data needed to see if the predicted iron dependency and chlorine enhancement match reality, or if a rethink is needed.

More information: Kenji Bekki et al, Phosphorus Enrichment by ONe Novae in the Galaxy, The Astrophysical Journal Letters (2024). DOI: 10.3847/2041-8213/ad3fb6

Journal information: Astrophysical Journal Letters

Citation: Astronomers propose a new stellar theory to explain the origin of phosphorus (2024, May 10) retrieved 25 May 2024 from
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.

Explore further

Q&A: How to catch a glimpse of a new star about to appear in the night sky


Feedback to editors