Researchers studying nearby stars have found a giant Jupiter-like planet circling a tiny red dwarf star 31 light years away, an unusual pairing that stretches the boundaries of our understanding of planet formation.
The exoplanet, called GJ 3512 b, is about half as massive as Jupiter (and 150 times more massive than Earth), while its host star, GJ 3512, is little more than one-tenth the mass of the Sun.
“Around such stars there should only be planets the size of the Earth or somewhat more massive Super-Earths,” said Christoph Mordasini, professor at the University of Bern and member of the National Centre of Competence in Research (NCCR) PlanetS. “GJ 3512b, however, is a giant planet with a mass about half as big as the one of Jupiter, and thus at least one order of magnitude more massive than the planets predicted by theoretical models for such small stars.”
The Spanish-led team who first spotted the planet 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 planets — 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.”
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.
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 transit method 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 stars for sampling and so added a few at the last minute.
