(CNN) — In a discovery that has been years in the making, researchers have confirmed the existence of a rocky planet named Proxima b orbiting Proxima Centauri, the closest star to our sun, according to a new study. It is the closest exoplanet to us in the universe.
Given the fact that Proxima b is within the habitable zone of its star, meaning liquid water could exist on the surface, it may also be the closest possible home for life outside of our solar system, the researchers said. Because of its location, the researchers hope that it provides an opportunity to “attempt further characterization via ongoing searches by direct imaging and high-resolution spectroscopy in the next decades, and possibly robotic exploration in the coming centuries.”
“The good news is that it is so close,” study author Ansgar Reiners said. “It is not only nice for having it in our neighborhood, but it’s a dream come true for astronomers if we think about follow-up observation.”
Proxima Centauri coexists with a binary star in Alpha Centauri, a well-studied star system that serves as a neighbor to our sun.
Proxima b is a mere 4.2 light-years away from our solar system, or 266,000 times the distance between the Earth and the sun, which are 92.96 million miles apart. Previous rocky exoplanet discoveries, like those orbiting ultracool red dwarf star TRAPPIST-1, were described as close at 40 light-years away.
“It’s not only the closest terrestrial planet found, it’s probably the closest planet outside our solar system that will ever be found because there is no star closer to the solar system than this one, and any planet around that star is the closest to our solar system,” said lead study author Guillem Anglada-Escudé.
“The only thing you can hope to find between that is Planet Nine, but that would a solar system object or a brown dwarf that hasn’t been discovered,” researcher Pedro Amado added.
Here is what we know about the planet, as well as the questions that researchers hope to be able to answer.
Meet Proxima b
Proxima b is a rocky, terrestrial planet with a surface — unlike a gas giant, such as Jupiter — that is 1.3 times the size of Earth and orbits its star every 11.2 days. It is in a close orbit of Proxima Centauri: only 5% of the distance between the Earth and the sun. They are even closer together than Mercury and the sun. But because its star is much cooler and fainter than our sun, Proxima b has a temperature that is suitable for liquid water to exist on the surface without evaporating.
Researchers estimate that if the planet has an atmosphere, which could be assumed but isn’t known, it may be between 86 to 104 degrees Fahrenheit on the surface. Without an atmosphere, it could be -22 to -40 degrees Fahrenheit. To put that in perspective, Earth would be -4 degrees if it didn’t have an atmosphere, Reiners said.
This also depends on the tidal locking of the planet, meaning some of its face is in light while some remains in shadow. Those light and dark faces could also have this positive to negative temperature range.
Given the proximity to its star, Proxima b is also subject to less pleasant factors like ultraviolet and X-ray flares that are 100 times the intensity of what Earth receives from the sun. In the paper, researchers estimated it to be 400 times the intensity, but recent research has caused them to create a new estimate, they said. If there is life on the planet, it would be affected by this radiation, but it is pure speculation as to what kind of effect.
If the Alpha Centauri system is well-studied and Proxima Centauri is our sun’s cozy star neighbor in the universe, why did it take so long to find Proxima b?
It comes down to an understanding of the star this planet orbits, as well as how data collection has evolved during the last 16 years.
Proxima Centauri is a low-mass red dwarf star, known as an M-class dwarf, that happens to be close to the bright binary star Alpha Centauri AB, which outshines its cool stepbrother, so to speak. All of these stars are within the faint Centaurus constellation, which can’t be seen with the unaided eye.
The cool star has a radius that is 14% of the sun’s, a mass of about 12% of the sun’s and a luminosity of .15% of the sun’s. It is moderately active, with a slow rotation period of 83 days.
M-class dwarves are not well understood in comparison with other types of stars, Reiners said. Because of that, researchers don’t know much about the history of these stars or their radiation in the early days.
“But within the field of exoplants, [researchers] have recently realized that looking for planets around M dwarves is what is going to be the most spectacular, because you can find these plants in the liquid water zone more easily than other stars,” Reiners said.
Because it’s an active star, Proxima Centauri can behave in varied ways that mimic the presence of a planet, according to the study. Researchers wanted to observe it for a long period of time and did so during the Pale Red Dot Campaign, a nod to the original “pale blue dot” image of Earth. The campaign, run by the researchers, included a public site and social media updates about their search for this exoplanet.
For the first half of this year, telescopes around the world were pointed at Proxima Centauri, including the High Accuracy Radial velocity Planet Searcher (HARPS) spectrograph at the European Southern Observatory’s La Silla observatory in Chile.
Rather than confirming this as a transiting planet candidate — they would have observed the light of the star to see a dip in its brightness as a planet passed in front of it — the researchers looked for a “Doppler wobble,” or back and forth wobble of Proxima Centauri that would be caused by the gravitational pull of a planet in orbit.
Using the Doppler effect, or watching for an increase or decrease in the frequency of the star’s light spectrum based on its velocity, the researchers saw the star approach Earth at 3 mph and recede at the same pace, repeating a pattern with a period of 11.2 days.
They combined these observations over 60 days in a row for 20 minutes a night with what they gathered from the other telescopes. This was combined with research, data and published studies of Proxima Centauri dating to 2000.
“The significance of the detection went sky high,” Anglada-Escudé said. “Statistically, there was no doubt. We have found a planet around Proxima Centauri.”
What we don’t know
The research around Proxima b will continue, and the researchers have more questions they want to answer. They don’t know whether there is water on the surface or if the planet has an atmosphere, although both are likely. They also don’t know whether, like Earth, the planet has a protective magnetic field to help with some of the radiation it receives.
Perhaps one of the biggest questions includes the history of the star and the planet. How did they form?
“What happened during the formation?” Reiners asked. “Was the star more active than the sun is today, and where during that phase was Proxima b located?”
This would indicate whether the plant was rich with water in its early days or started out dry, as well as whether there was any high-energy radiation that could have blasted away an atmosphere during formation of the planet.
There is also some debate over whether this planet is Earth-like, which comes with some connotations. Depending on its formation, perhaps it could be like Venus.
Learning the answers to these questions about formation are possible with research. The habitability of a planet like Proxima b is also “a matter of intense debate,” according to the study, due to arguments against it: tidal locking, strong stellar magnetic fields, strong flares, and high ultraviolet and X-ray fluxes. But, as they point out, none of those has been proved definitive, either.
