Uh oh! A quarter of Sun-like stars probably gobble up planets

Publicly released:
Australia; International; VIC; ACT
NASA/Goddard Space Flight Center
NASA/Goddard Space Flight Center

International scientists, including Australians, say around a quarter of stars similar to our own Sun are probably engulfing planets from their solar systems. But don't worry too much, because they are talking about binary star systems, with two Sun-like stars, rather than our own, mercifully calm, solar system. The scientists' interest was piqued by the fact that the two stars in binary systems can be quite different in composition, so they set out to establish whether this was due to differences when the stars were born, or because one or other of the stars had been gobbling up planets during its life. Their research suggests the latter is true, and that there's a 20 - 35 per cent chance a Sun-like star will chomp down on a local planet. They say their findings could make it easier to identify habitable solar systems by looking at the composition of their stars.

Attachments

Note: Not all attachments are visible to the general public. Research URLs will go live after the embargo ends.

Research Springer Nature, Web page The URL will go live after the embargo ends
Journal/
conference:
Nature Astronomy
Research:Paper
Organisation/s: Monash University, ARC Centre of Excellence for All Sky Astrophysics in 3D (ASTRO 3D), INAF, Italy
Funder: This work has made use of observations collected at the ESO (programmes 188.C-0265, 0103.C-0785 and 0101.C-0275) and of data from the European Space Agency mission Gaia. We are grateful to K. Hawkins, and F. Liu for having shared with us tabular and spectroscopic data. L.S. thanks A. I. Karakas for her support and advice. L.S. also acknowledges financial support from the Australian Research Council (Discovery Project 170100521) and continuing support from the Italian Space Agency through contract 2018-24-HH.0 to the National Institute for Astrophysics (INAF). J.M. thanks FAPESP (2018/04055-8). A.R.C. is supported in part by the Australian Research Council through a Discovery Early Career Researcher Award (DE190100656). M.C. is supported by MIUR under PRIN programme 2017Z2HSMF. Parts of this research were supported by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013.
Media Contact/s
Contact details are only visible to registered journalists.