UCLAN astronomer discovers new way in which young giant planets evolve

New research into the early stages of planet formation, published  in the Monthly Notices of the Royal Astronomical Society, suggests that there may be more giant planets – most at least 10 times as big as Jupiter – orbiting at large distances from their host star than we previously thought.

Using supercomputers, researchers at the University of Central Lancashire (UCLan) and Nagoya University in Japan have analysed how young planets interact with their host protoplanetary disc – the rotating disc of dense gas and dust, from which planetary systems, like our own Solar System, form. They have discovered that the early evolution of giant planets is far more diverse than expected.

As giant planets form, they take gas from their protoplanetary discs over a few millions of years in order to grow. Research has previously focused on how, as they grew, these planets moved inwards towards their parent star, often getting destroyed by it in the process.

Using computer simulations performed with the UCLan High Performance Computing (HPC) facility and the UK DiRAC supercomputer facility, researchers have now discovered that when there are strong interactions with a heavy protoplanetary disc, the growing giant planet is likely to be dragged away from its parent star, while milder interactions with a less heavy, stable disc drag the planet towards its star.

Although some of the inward-migrating planets were likely to getshatteredby gravitational interactions with the disc and the host star, in both types of interactions, the growing planets may survive to reach adulthood. Interestingly, the researchers found that a significant fraction of giant planets may be outward-migrating, suggesting that there may be more giant planets orbiting at large distances from their host star than previously expected. These planets may end up orbiting at distances more than 10 to 40 times the distance of Jupiter from the Sun.

Commenting on the findings, Dr Dimitris Stamatellos, astrophysicist at UCLan, said: “There’s a lot about the early years of young planets that we don’t know. There is a very fine balance between the forces that push the planet towards its parent star and the forces that push the planet away from it.

“A planet’s survival is also difficult to predict. Many planets that formed initially may be destroyed, and only a few can survive to reach adulthood. This newly discovered insight into the diversity of how young giant planets evolve can help us to understand more about the formation of solar systems beyond our own.”

 

Figure: Computer simulation of a young planet that is being fed with gas from its parent protoplanetary disc (YouTube video)

 

Notes for editors

 

Simulations were performed using the UCLAN HPC facility and the COSMOS Shared Memory system at DAMTP, University of Cambridge operated on behalf of the STFC DiRAC HPC Facility (ST/J005673/1 and STFC grants ST/H008586/1, ST/K00333X/1). This work was supported from a Royal Society-Daiwa Foundation International Exchanges award (IE140640) between University of Central Lancashire, UK, and Nagoya University, Japan.  Dimitris Stamatellos was also partly supported from STFC Grant ST/M000877/1.

 

Related publications

 

“The diverse lives of massive protoplanets in self-gravitating discs”

Stamatellos, D. & Inutsuka, S-i, 2018, Monthly Notices of the Royal Astronomical Society, Volume 477, Issue 3, 1 July 2018, pages 3110-3135

 

https://doi.org/10.1093/mnras/sty827

https://arxiv.org/abs/1804.00583

 

 

Contact details

 

Dr Dimitris Stamatellos

Jeremiah Horrocks Institute for Mathematics, Physics, & Astronomy

University of Central Lancashire

Preston PR1 2HE, UK

Web: http://www.star.uclan.ac.uk/~dstamatellos

Email: dstamatellos@uclan.ac.uk