Artist's impression of Kepler-16b,
discovered by NASA's Kepler mission and the first confirmed
circumbinary planet. It is a gas giant that orbits close to the edge of
its binary system's habitable zone.
Credit: T. Pyle / NASA / JPL-Caltech
Artificial intelligence is giving scientists new hope for studying the habitability of planets, in a study from astronomers Chris Lam and David Kipping. Their work looks at so-called ‘Tatooines’, and uses machine learning techniques to calculate how likely such planets are to survive into stable orbits. The study is published in the journal Monthly Notices of the Royal Astronomical Society.
Artificial intelligence is giving scientists new hope for studying the habitability of planets, in a study from astronomers Chris Lam and David Kipping. Their work looks at so-called ‘Tatooines’, and uses machine learning techniques to calculate how likely such planets are to survive into stable orbits. The study is published in the journal Monthly Notices of the Royal Astronomical Society.
Circumbinary planets are
those planets that orbit two stars instead of just one, much like the
fictional planet Tatooine in the Star Wars franchise. Tens of these
planets have so far been discovered, but working out whether they may be
habitable or not can be difficult.
Moving
around two stars instead of just one can lead to large changes in a
planet’s orbit, which mean that it is often either ejected from the
system entirely, or it crashes violently into one of its twin stars.
Traditional approaches to calculating which of these occurs for a given
planet get significantly more complicated as soon as the extra star is thrown into the mix.
“When
we simulated millions of possible planets with different orbits using
traditional methods, we found that planets were being predicted as
stable that were clearly not, and vice versa,” explains Lam, lead author
of the study and a recent graduate of Columbia University.
Planets
need to survive for billions of years in order for life to evolve, so
finding out whether orbits are stable or not is an important question
for habitability. The new work shows how machine learning can make accurate predictions even if the standard approach - based on Newton’s laws of gravity and motion - breaks down.
“Classification
with numerous complex, inter-connected parameters is the perfect
problem for machine learning,” says Professor Kipping, supervisor of the
work.
After
creating ten million hypothetical Tatooines with different orbits, and
simulating each one to test for stability, this huge training set was
fed into the deep learning network. Within just a few hours, the network
was able to out-perform the accuracy of the standard approach.
More circumbinary planets look set to be discovered by NASA’s Transiting Exoplanet Survey Satellite (TESS)
mission, and Lam expects their work to help: “Our model helps
astronomers to know which regions are best to search for planets around
binary stars. This will hopefully help us discover new exoplanets and
better understand their properties.”
Media contacts
Dr Morgan Hollis
Royal Astronomical Society
Mob: +44 (0)7802 877 700
mhollis@ras.ac.uk
Dr Robert Massey
Royal Astronomical Society
Mob: +44 (0)7802 877 699
rmassey@ras.ac.uk
Science contacts
Mr Chris Lam
Columbia University
Tel: +1 954 540 1339
cl3425@columbia.edu
Prof. David Kipping
Columbia University
dkipping@astro.columbia.edu
Video:
Prof. David Kipping explains why three-body systems are so tricky and how a neural network can save the day. Neural networks can capture borderline cases that are missed by even the most sophisticated mathematical solutions. He also highlights how neural networks might play an increasingly larger role in answering similarly complex science questions.
Credit: D. Kipping / Cool Worlds Lab
Further information
The new work appears in: "A machine learns to predict the stability of circumbinary planets", C. Lam & D. Kipping, Monthly Notices of the Royal Astronomical Society (2018) 476 (4): 5692-5697 (DOI: 10.1093/mnras/sty022).
A copy of the paper is available at: https://doi.org/10.1093/mnras/sty022
Notes for editors
The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organizes scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 4,000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others. The RAS accepts papers for its journals based on the principle of peer review, in which fellow experts on the editorial boards accept the paper as worth considering. The Society issues press releases based on a similar principle, but the organisations and scientists concerned have overall responsibility for their content. Follow the RAS on Twitter, Facebook and Instagram
Source: Royal Astronomical Society (RAS)
Media contacts
Dr Morgan Hollis
Royal Astronomical Society
Mob: +44 (0)7802 877 700
mhollis@ras.ac.uk
Dr Robert Massey
Royal Astronomical Society
Mob: +44 (0)7802 877 699
rmassey@ras.ac.uk
Science contacts
Mr Chris Lam
Columbia University
Tel: +1 954 540 1339
cl3425@columbia.edu
Prof. David Kipping
Columbia University
dkipping@astro.columbia.edu
Video:
Further information
The new work appears in: "A machine learns to predict the stability of circumbinary planets", C. Lam & D. Kipping, Monthly Notices of the Royal Astronomical Society (2018) 476 (4): 5692-5697 (DOI: 10.1093/mnras/sty022).
A copy of the paper is available at: https://doi.org/10.1093/mnras/sty022
Notes for editors
The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organizes scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 4,000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others. The RAS accepts papers for its journals based on the principle of peer review, in which fellow experts on the editorial boards accept the paper as worth considering. The Society issues press releases based on a similar principle, but the organisations and scientists concerned have overall responsibility for their content. Follow the RAS on Twitter, Facebook and Instagram