Big world around tiny star puts new spin on planet formation

A planet that should not exist
Jupiter-like planet with a blueish colour orbiting a cool red dwarf. Credit: © CARMENES/RenderArea/J. Bollaín/C. Gallego

A giant world discovered around a tiny star is putting a new spin on how planets form.

Astronomers reported Thursday they've found a Jupiter-like planet orbiting a star that's a mere 12% the mass of our sun. There may even be another big gas planet lurking in this system 31 light-years away.

The Spanish-led team wrote in the journal Science that the newly confirmed planet did not form the usual, gradual way, where a solid core of merging particles takes shape before a gas buildup. Instead, in a surprise to scientists, the planet seems to have arisen straight from gas.

Lead author Juan Carlos Morales of the Institute of Space Studies of Catalonia said the planet may be almost as big as its star. A year there is about 200 days.

"It was very exciting finding this planet because it was completely unexpected," Morales wrote in an email. The results indicate "a new population of massive planets may also exist around low-mass stars."

Morales and his team maintain that gravitational instability in a young star's disk of gas and dust could, in some cases, result in the quick formation of huge gas —even when the star is minuscule. This new world is "an extraordinary candidate" for this process, said Hubert Klahr of Max Planck Institute for Astronomy in Germany, part of the research team. "This find prompts us to review our models."

  • A planet that should not exist
    Comparison of GJ 3512 to the Solar System and other nearby red-dwarf planetary systems. Planets around a solar-mass stars can grow until they start accreting gas and become giant planets such as Jupiter, in a few millions of years. But we thought that small stars such as Proxima, TRAPPIST-1, Teegardern’s star and GJ 3512, could not form Jupiter mass planets. Credit: Guillem Anglada-Escude - IEEC, SpaceEngine.org
  • A planet that should not exist
    Domes of different telescopes at the Calar Alto Observatory. CARMENES is installed on the 3.5-m telescope inside the dome at the right of the image. Credit: Pedro Amado/Marco Azzaro - IAA/CSIC

In a companion article, Yale University astronomer Greg Laughlin, who was not involved in the study, pointed out that more than 4,000 so-called exoplanets have been confirmed in solar systems outside our own. While another new one, by itself, is no longer particularly noteworthy, he said, "one that challenges current theories of planet formation can animate astronomers."

The planet orbiting this particularly small and cool red dwarf star, officially known as GJ 3512, is at least half the mass of Jupiter. Scientists are unable to measure its dimensions, but models indicate it may be comparable to Jupiter in size, according to Morales.

Artistic representation of the orbits of the planets around GJ 3512. The giant planet discussed in the paper is represented in the inner orbit, while the outer one corresponds to the long period signal also found in the data but for which confirmation is still needed. Credit: Guillem Anglada-Escude - IEEC/Science Wave, SpaceEngine.org

Using observatories in Spain, the researchers repeatedly studied the star's wobbling motion to disclose the planet in its lopsided orbit, rather than rely on the in which a brief, periodic dimming of starlight indicates a planet passing in front of its star.

The star is so faint it almost didn't make it into the group's survey. Scientists needed more small for sampling and so added a few at the last minute.

Simulation using current main-stream models for planet formation around a Sun-like star and a small star like GJ 3512. The current main-stream model (pebble accretion) can form large planets like Jupiter and Saturn around Sun-like stars (in black, 00:23), but it fails to produce planets like GJ 3512 b around small red-dwarfs (red dots, never climb up to become large gas giants, see end of simulation). Credit: Anders Johanson- Lund Observatory

"We were lucky to do so because otherwise we would have never made this discovery," Ignasi Ribas, director of the Catalonia space studies institute, said in a statement.

Morales and his colleagues continue to search for a second planet orbiting this dwarf star. There may have been a third planet that was ejected from the system long ago, they noted.


Explore further

New exoplanet too big for its stars

More information: J.C. Morales el al., "A giant exoplanet orbiting a very-low-mass star challenges planet formation models," Science (2019). science.sciencemag.org/cgi/doi … 1126/science.aax3198

"The world that came in from the cold," by G. Laughlin science.sciencemag.org/cgi/doi … 1126/science.aay7775

Journal information: Science

© 2019 The Associated Press. All rights reserved.

Citation: Big world around tiny star puts new spin on planet formation (2019, September 26) retrieved 17 October 2019 from https://phys.org/news/2019-09-big-world-tiny-star-planet.html
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Sep 26, 2019
well, so much for those futile hopes for a coherent intelligent design

chaos rules in implausible eccentricities

thanks for the link, castro

Sep 27, 2019
Thanks for the link, Castro !

Sep 27, 2019
It is not the first case of large planets around red dwarfs, see the paper [Fig, 2]. In fact, such systems can have much more massive brown dwarfs, which is often called "failed stars" but the present work labels "planet". And in general most systems are binaries - binary stars - all of which form by direct collapse.

In that respect this corner case - they are rare - looks like "a failed failed stars". It is arguable that they "challenge planet formation models" as they claim, rather they elucidate the border or overlap between the different formation mechanisms.

Sep 27, 2019
way i see it?
at least the universe is not a giant mimeograph machine

churning out endless copies of tha same damn tediously boring
asteroid, comet, planet. star, systems, clusters, galaxies

in an endless rote of deadly dull identical clones
full of the same old, same old,

instead, wherever we look?
we find the unexpected

even when it seems we have found similarities?
we also have an opportunity to discover unique features

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