Alpha Centauri A – Our Closest Sun-Like Star – Has A New “Very Strong Candidate” Planet

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Alpha Centauri A – Our Closest Sun-Like Star – Has A New “Very Strong Candidate” Planet

Alpha Centauri A – Our Closest Sun-Like Star – Has A New “Very Strong Candidate” Planet

It’s not just Proxima Centauri that might be sporting planets.

Dr. Alfredo Carpineti headshot
In this concept, Alpha Centauri A is depicted at the upper left of the planet, while the other Sun-like star in the system, Alpha Centauri B, is at the upper right. Our Sun is shown as a small dot of light between those two stars.

This artist’s concept shows what the gas giant orbiting Alpha Centauri A could look like - the Sun is that small dot in between the stars!

Image Credit: Artwork: NASA, ESA, CSA, STScI, R. Hurt (Caltech/IPAC)

The closest exoplanets to the Solar System are around the red dwarf Proxima Centauri. This little star is orbiting two bigger Sun-like stars, which are known as Alpha Centauri A and B. For over a decade, people have proposed possible planets around either, with no confirmation. New observations now make a stronger case for a planet around Alpha Centauri A.

The candidate world believed to be orbiting  Alpha Centauri A, also known as Rigil Kentaurus, is in its habitable zone. If confirmed, this is the closest planet in the habitable zone of a Sun-like star. However, don’t shout aliens, just yet! The planet is estimated to be not a rocky world like Earth but a gas giant.

“At only 4 light-years away, Alpha Centauri is the nearest star most similar to our own Sun. The presence of a planet, possibly a habitable planet, around our nearest neighbor has been a matter of great scientific and science fiction speculation for decades,” co-lead author Charles Beichman, executive director of the NASA Exoplanet Science Institute at Caltech, told IFLScience. “The fact that we now have a very strong candidate for a planet, even if it is a Saturn-mass planet that could not itself be habitable, is an important milestone in the search.”

Crucial to this work have been the observations from the JWST mid-infrared instrument. The space observatory has a coronagraphic mask blocking the light of the star, but the challenge here is to get rid of the light of Alpha Centauri B, which is very close. The team had to do some incredible work to subtract the light of both to find the incredibly faint signal that suggests the presence of a planet.

This image shows the Alpha Centauri star system from several different ground- and space-based observatories: the Digitized Sky Survey (DSS), NASA’s Hubble Space Telescope, and NASA’s James Webb Space Telescope. Alpha Centauri A is the third brightest star in the night sky. The ground-based image from DSS shows the triple system as a single source of light, while Hubble resolves the two Sun-like stars in the system, Alpha Centauri A and Alpha Centauri B. The image from Webb’s MIRI (Mid-Infrared Instrument), which uses a coronagraphic mask to block the bright glare from Alpha Centauri A, reveals a potential planet orbiting the star.

It looks like there might be something there.

Image Credit: Science: NASA, ESA, CSA, STScI, DSS, A. Sanghi (Caltech), C. Beichman (JPL), D. Mawet (Caltech); Image Processing: J. DePasquale (STScI)

“This project started almost a decade ago when JWST was still many years away from launch. It took an international team of astronomers with differing areas of expertise to plan and execute the observations, to process the data carefully to reveal the planet, and to interpret the results. The JWST operations team were critical in making these challenging observations possible,” Beichman told IFLScience.

“JWST's great stability and sensitivity at infrared wavelengths inaccessible from the ground allowed the careful subtraction of the light from Alpha Centauri to reveal a planet more than 10,000 times fainter than the star.”

If this planet is confirmed, it would be the closest that has been visually discovered, and the first imaged around a star the same age and temperature as the Sun. The team will continue to follow the potential world with JWST, and use the upcoming Nancy Grace Roman Space Telescope and the European Extremely Large Telescope (E-ELT) to work out even more details about this world.

The work co-led by Aniket Sanghi, a Caltech graduate student, are reported in two papers accepted for publication in The Astrophysical Journal Letters and available on the ArXiv.


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