Astronomers have discovered a new Earth-sized planet, SPECULOOS-3b, orbiting a cold,
The ultracool dwarf that hosts the new planet is about one-tenth the size of, and 1,000 times dimmer than, the sun. The star is more similar in size to Jupiter and is twice as cold as the sun. Nevertheless, the dwarf star radiates an enormous amount of energy onto the planet’s surface due to the planet’s extremely close proximity: SPECULOOS-3b circles its star in just 17 hours. One year on the new planet, then, is shorter than one day on Earth.
Because it is so close to its star, the planet is blasted with 16 times more radiation per second compared to what the Earth receives from the sun. The team believes that such intense and relentless exposure has likely vaporized any atmosphere that the planet once held, leaving it an airless, exposed, blistering ball of rock.
If the planet lacks an atmosphere, scientists might soon be able to zero in on exactly what type of rocks are on its surface and even what sort of geological processes shaped its landscape, such as whether the planet’s crust experienced magma oceans, volcanic activity, and plate tectonics in its past.
“SPECULOOS-3b is the first planet for which we can consider moving toward constraining surface properties of planets beyond the solar system,” says study co-author Julien de Wit, associate professor of planetary sciences at
Lining Up
Astronomers observed the first inklings of the new planet in 2021, with observations taken by SPECULOOS — a network of six robotic, 1-meter telescopes (four in the Southern Hemisphere, and two in the Northern Hemisphere) that continuously observe the sky for signs of planets orbiting around ultracool dwarf stars. SPECULOOS is the parent project of the TRAPPIST (TRAnsiting Planets and PlanetesImals Small Telescope-South) survey, which discovered seven terrestrial planets — several potentially habitable — around a small cold star named TRAPPIST-1.
SPECULOOS aims to observe about 1,600 nearby ultracool dwarf stars. As these stars are small, any planets that orbit and cross in front of them should momentarily block their light, by a more noticeable amount compared to planets that orbit around larger, brighter stars. Ultracool dwarf stars, then, could give astronomers a better view of any planets that they host.
In 2021, a telescope in SPECULOOS’ network picked up some inconclusive signs of a transit, in front of one ultracool dwarf star about 55 light years away. Then in 2022, a close monitoring with MIT’s Artemis telescope changed the game.
“While there were structures in the 2021 data that didn’t look convincing, the 2022 Artemis data really got our attention,” recalls MIT’s Artem Burdanov, who manages the SPECULOOS Northern Observatory. “We started to analyze one clear transit-like signal in the Artemis data, quickly decided to launch a campaign around this star, and then things just started lining up.”
Dark Like the Moon
The team zeroed in on the star with MIT’s Artemis telescope, the rest of the SPECULOOS network, and several other observatories. The multipronged observations confirmed that the star did indeed host a planet, which appeared to orbit every 17 hours. Judging from the amount of light it blocked with each crossing, the scientists estimate that the planet is about the size of the Earth.
They were then able to estimate certain properties of the star and the planet based on analyses of the star’s light taken by MIT’s Benjamin Rackham, who has led a campaign using the Magellan telescopes in Chile and the DOI: 10.1038/s41550-024-02271-2
This research was supported, in part, by the European Research Council, the Simons Foundation, and the Heising-Simons Foundation.