Chances for life expand when passing stars push binaries together

A NASA graphic showing an Earth-sized planet inside, within, and outside of the habitable zone around a star. Credit: NASA

A NASA graphic showing an Earth-sized planet inside, within, and outside of the habitable zone around a star. Credit: NASA

Planetary systems can be harsh environments in their early history. The young worlds orbit suns in stellar nurseries, clusters of stars where violent encounters are commonplace. None of this makes it easy for life to get going, but now astronomers at the University of Sheffield find one positive of this tumultuous period. A model developed by undergraduate student Bethany Wootton and Royal Society Dorothy Hodgkin Fellow Dr. Richard Parker looks at how the habitable zone — the region around a star where the temperature allows liquid water to exist — changes around pairs of stars, so-called binary systems.

A diagram of two stars in a binary system, before and after an encounter with a third passing star. The stars are the yellow/orange dots (the yellow star is the same mass as our Sun, the orange star is just over half of the Sun’s mass) and the habitable zones are shown in blue. The ‘narrow’ habitable zone is the most pessimistic estimate for where water can exist as a liquid, and the cyan habitable zone is the most optimistic estimate. The diagram shows one star in an orbit, following the black path, around the other, and the size and shape of the orbit changes after the encounter. In this encounter the two stars have moved closer together, and both stars feel the extra warmth from each other. This has the effect of increasing the size of the habitable zones, especially around the lower mass star, and sometimes the habitable zones overlap. The grey dashed line shows the maximum distance a planet can be from the star and still remain on a stable orbit. Credit: Richard Parker / Bethany Wootton / University of Sheffield

A diagram of two stars in a binary system, before and after an encounter with a third passing star. The stars are the yellow/orange dots (the yellow star is the same mass as our Sun, the orange star is just over half of the Sun’s mass) and the habitable zones are shown in blue. The ‘narrow’ habitable zone is the most pessimistic estimate for where water can exist as a liquid, and the cyan habitable zone is the most optimistic estimate. The diagram shows one star in an orbit, following the black path, around the other, and the size and shape of the orbit changes after the encounter. In this encounter the two stars have moved closer together, and both stars feel the extra warmth from each other. This has the effect of increasing the size of the habitable zones, especially around the lower mass star, and sometimes the habitable zones overlap. The grey dashed line shows the maximum distance a planet can be from the star and still remain on a stable orbit. Credit: Richard Parker / Bethany Wootton / University of Sheffield

The two scientists discovered that an encounter with a passing third star may squeeze the binary pair together, expanding the habitable zone in the process. Their results appear in a new paper in the journal Monthly Notices of the Royal Astronomical Society.

The habitable zone, sometimes called the ‘Goldilocks zone’ as the temperature is not too hot and not too cold, is thought to be essential for the development of life on a planet. If a planet lies outside this zone, then the formation of the complex molecules needed for life is less likely to happen.

Around one third of stellar systems in our galaxy are thought to be made up of two or more stars, and this fraction is much higher when stars are young. If these stars are a relatively large distance apart, the size of the Goldilocks zone around each star is governed by the radiation from the individual star. If the two stars are closer, the size of the Goldilocks zone increases because each star feels additional warmth from the other and this increases the likelihood of a planet being located in the right place for life to develop.

Wootton and Parker looked at how this changed in stellar nurseries. They used computer simulations to model the interactions between young stars in these clusters, calculating how these encounters affected the binary pairs. In a typical stellar nursery with 350 binaries, the two researchers found that 20 would have their stars squeezed together, and their Goldilocks zones then expanded.

In a few cases, the habitable zones of widely separated stars actually overlapped, further increasing the prospect of any planets in orbit around one or both of the stars being in the right place for life to develop.

Artist’s impression of life on a planet in orbit around a binary star system, visible as two suns in the sky. Credit: Mark Garlick

Artist’s impression of life on a planet in orbit around a binary star system, visible as two suns in the sky. Credit: Mark Garlick

Wootton comments: “The search for life elsewhere in the universe is one of the most fundamental questions in modern science, and we need every bit of evidence we can find to help answer it.”

“Our model suggests that there are more binary systems where planets sit in Goldilocks zones than we thought, increasing the prospects for life. So those worlds beloved of science fiction writers — where two suns shine in their skies above alien life — look a lot more likely now.”

The next steps for this research are to use more computer models to understand whether the negative processes a young star experiences are outweighed by the positives. Parker and his research team are currently exploring whether internal heating within the Earth happens because our young Sun was born close to a supernova explosion of a massive star; this explosion would be catastrophic for life on Earth today, but may provide the necessary conditions for life to have developed on Earth in the first place.

Media Contacts:
Dr. Robert Massey
Royal Astronomical Society
+44 (0)20 7292 3979, cell: +44 (0)7802 877 699
press@ras.ac.uk

Dr. Morgan Hollis
Royal Astronomical Society
+44 (0)7802 877 700 (cell)
press@ras.ac.uk

Science Contacts:
Dr. Richard Parker
University of Sheffield
+44(0)114 22 23560, cell: +44 (0)7948 550 442
r.parker@sheffield.ac.uk

Ms. Bethany Wootton
University of York
+44 (0)7504 255 202 (cell)
bethany.wootton@york.ac.uk

Reference:
“Enlarging Habitable Zones Around Binary Stars in Hostile Environments,” B. A. Wootton & R. J. Parker, 2019 March 7, Monthly Notices of the Royal Astronomical Society: Letters [https://doi.org/10.1093/mnrasl/sly238].

Usman Zafar Paracha

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