Potentially Habitable Exoplanet Confirmed Around Nearest Star!

Article written: 24 Aug , 2016
Updated: 25 Aug , 2016
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For years, astronomers have been observing Proxima Centauri, hoping to see if this red dwarf has a planet or system of planets around it. As the closest stellar neighbor to our Solar System, a planet here would also be our closest planetary neighbor, which would present unique opportunities for research and exploration.

So there was much excitement when, earlier this month, an unnamed source claimed that the ESO had spotted an Earth-sized planet orbiting within the star’s habitable zone. And after weeks of speculation, with anticipation reaching its boiling point, the ESO has confirmed that they have found a rocky exoplanet around Proxima Centauri – known as Proxima b.

Located just 4.25 light years from our Solar System, Proxima Centauri is a red dwarf star that is often considered to be part of a trinary star system – with Alpha Centauri A and B. For some time, astronomers at the ESO have been observing Proxima Centauri, primary with telescopes at the La Silla Observatory in Chile.

Their interest in this star was partly due to recent research that has shown how other red dwarf stars have planets orbiting them. These include, but are not limited to, TRAPPIST-1, which was shown to have three exoplanets with sizes similar to Earth last year; and Gliese 581, which was shown to have at least three exoplanets in 2007.

The ESO also confirmed that the planet is potentially terrestrial in nature (i.e. rocky), similar in size and mass to Earth, and orbits its star with an orbital period of 11 days. But best of all are the indications that surface temperatures and conditions are likely suitable for the existence of liquid water.

It’s discovery was thanks to the Pale Red Dot campaign, a name which reflects Carl Sagan’s famous reference to the Earth as a “pale blue dot”. As part of this campaign, a team of astronomers led by Guillem Anglada-Escudé – from Queen Mary University of London – have been observing Proxima Centauri for signs of wobble (i.e. the Radial Velocity Method).

After combing the Pale Red Dot data with earlier observations made by the ESO and other observatories, they noted that Proxima Centauri was indeed moving. With a regular period of 11.2 days, the star would vary between approaching Earth at a speed of 5 km an hour (3.1 mph), and then receding from Earth at the same speed.

Artist’s impression of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri. The double star Alpha Centauri AB is visible to the upper right of Proxima itself. Credit: ESO

Artist’s impression of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri. The double star Alpha Centauri AB is visible to the upper right of Proxima itself. Credit: ESO

This was certainly an exciting result, as it indicated a change in the star’s radial velocity that was consistent with the existence of a planet. Further analysis showed that the planet had a mass at least 1.3 times that of Earth, and that it orbited the star at a distance of about 7 million km (4.35 million mi) – only 5% of the Earth’s distance from the Sun.

The discovery of the planet was made possible by the La Silla’s regular observation of the star, which took place star  between mid-January and April of 2016, using the 3.6-meter telescope‘s HARPS spectrograph. Other telescopes around the world conducted simultaneous observation in order to confirm the results.

One such observatory was the San Pedro de Atacama Celestial Explorations Observatory in Chile, which relied on its ASH2 telescope to monitor the changing brightness of the star during the campaign. This was essential, as red dwarfs like Proxima Centauri are active stars, and can vary in ways that would mimic the presence of the planet.

Guillem Anglada-Escudé described the excitement of the past few months in an ESO press release:

“I kept checking the consistency of the signal every single day during the 60 nights of the Pale Red Dot campaign. The first 10 were promising, the first 20 were consistent with expectations, and at 30 days the result was pretty much definitive, so we started drafting the paper!”

This infographic compares the orbit of the planet around Proxima Centauri (Proxima b) with the same region of the Solar System. Proxima Centauri is smaller and cooler than the Sun and the planet orbits much closer to its star than Mercury. As a result it lies well within the habitable zone, where liquid water can exist on the planet’s surface.

Infographic comparing the orbit of the planet around Proxima Centauri (Proxima b) with the same region of the Solar System. Credit: ESO/M. Kornmesser/G. Coleman

Two separate papers discuss the habitability of Proxima b and its climate, both of which will be appearing soon on the Institute of Space Sciences (ICE) website. These papers describe the research team’s findings and outline their conclusions on how the existence of liquid water cannot be ruled out, and discuss where it is likely to be distributed.

Though there has been plenty of excitement thanks to words like “Earth-like”, “habitable zone”, and “liquid water” being thrown around, some clarifications need to be made. For instance, Proxima b’s rotation, the strong radiation it receives from its star, and its formation history mean that its climate is sure to be very different from Earth’s.

For instance, as is indicated in the two papers, Proxima b is not likely to have seasons, and water may only be present in the sunniest regions of the planet. Where those sunny regions are located depends entirely on the planet’s rotation. If, for example, it has a synchronous rotation with its star, water will only be present on the sun-facing side. If it has a 3:2 resoncance rotation, then water is likely to exist only in the planet’s tropical belt.

In any case, the discovery of this planet will open the door to further observations, using both existing instruments and the next-generation of space telescopes. And as Anglada-Escudé states, Proxima Centauri is also likely to become the focal point in the search for extra-terrestrial life in the coming years.

This picture combines a view of the southern skies over the ESO 3.6-metre telescope at the La Silla Observatory in Chile with images of the stars Proxima Centauri (lower-right) and the double star Alpha Centauri AB (lower-left) from the NASA/ESA Hubble Space Telescope. Proxima Centauri is the closest star to the Solar System and is orbited by the planet Proxima b, which was discovered using the HARPS instrument on the ESO 3.6-metre telescope.

A view of the southern skies over the ESO 3.6-metre telescope at the La Silla Observatory in Chile, showing the location of Proxima Centauri in the sky. Credit: Y. Beletsky (LCO)/ESO/ESA/NASA/M. Zamani

“Many exoplanets have been found and many more will be found, but searching for the closest potential Earth-analogue and succeeding has been the experience of a lifetime for all of us,” he said. “Many people’s stories and efforts have converged on this discovery. The result is also a tribute to all of them. The search for life on Proxima b comes next…”

As we noted in a previous article on the subject, Project Starshot is currently developing a nanocraft that will use a laser-driven sail to make the journey to Alpha Centauri in 20 years time. But a mission to Proxima Centuari would take even less time (19.45 years at the same speed), and could study this newly-found exoplanet up-close.

One can only hope they are planning on altering their destination to take advantage of this discovery. And one can only imagine what they might find if and when they get to Proxima b!

A paper describing this milestone finding will be published in the journal Nature on August 25th, 2016, titled “A terrestrial planet candidate in a temperate orbit around Proxima Centauri“.

Further Reading: ESO

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19 Responses

  1. Robert Walker says

    Just a typo – article says 11 hours for the orbital period – it’s 11.2 days of course.

  2. FarAwayLongAgo says

    Mercury is tidally locked to the Sun and only shows one and the same side to it all of the time.
    Oh, wait! No, that is not true!
    It took radar from Arecibo in the 1960s to discover that a tidally locked planet can rotate as it orbits its star. But they seem to know more about this exoplanet than about Mercury. Fantastic!

    • Torbjorn Larsson OM says

      Tidal lock refers to 1:1 resonances I think, so Mercury which is in a 3:2 resonance orbit isn’t locked. Models results in such a Mercury in 1/3 of cases, so it isn’t rare – IIRC ~ 50 % of M star habitables would be in similar resonances.

      • FarAwayLongAgo says

        Do you know if it is possible for a planet to have such an eccentric orbit as Mercury, and still be synchronously tidally locked to its star? (Mercury is asynchronously tidally locked, still tidally locked, to be picky about the messy terminology of astronomy).

  3. crocodilebomb says

    “Habitable… confirmed”! I, for one, welcome our new xray-proof overlords.

  4. Torbjorn Larsson OM says

    Unfortunately a bit too large for comfort, and they haven’t seen any transits yet. So habitability and searching foe biosignatures is a bit optimistic speculation yet. On the other hand Proxima C is not (at present) any more active than our relatively calm Sun, which is promising.

    But Starshots would fix the observation problem if there are no transits, and even a gas giant so close would be valuable.

  5. crocodilebomb says

    Wikipedia: “Proxima Centauri’s quiescent X-ray luminosity, approximately (4–16) × 10^26 erg/s ((4–16) × 10^19 W), is roughly equal to that of the much larger Sun. The peak X-ray luminosity of the largest flares can reach 10^28 erg/s (10^21 W.)” The cited paper from 2003 mentions a very large flare. So recent flares 100 times the xray flux of the sun, and situated *extremely* close. Seems like a particularly nasty neighborhood to visit, even in a lead box.

    • FarAwayLongAgo says

      So, you won’t need to go to the hospital to see if you have fracture. 😈

    • Very true! When it comes to exploring this one, searching for life on it, and potentially colonizing it, radiation is the big buzzkill. Not sure yet what it will mean for this lovely rock next door.

  6. Beth Kuda says

    Good information, and an exciting find.

    This is a fairly informative, decently written article, with one exception, as follows:
    “It’s discovery was…” You are a journalist. Stop destroying your own credibility with improper grammar. LEARN the difference between “It’s” which is a contraction of IT IS, and “Its” which is the possessive form of IT. Don’t expect a spell checker to do it for you. You’re better than this, Mr. Williams.

  7. SteveZodiac says

    Looks like the James Webb is going to be on a mission

  8. Underlings says

    In a tidelocked world, doesn’t all the water on the sunward side eventually and inevitably end up precipitating on the dark side, never to return? Thus resulting in a planet almost devoid of useful water for supporting life?

    • weeasle says

      I read some articles here citing studies on habitabilty of red dwarf tidally locked planets. To paraphrase, computer models suggested that with sufficient atmosphere, planetary mass and density of terrain (course materials / mountainous) that wind circulation would spread precipitation to both the day and night sides (with the night side colder / and possibly icy). How the ice/snow would evaporate and return to the atmosphere wasnt specified and i did not read the paper mentioned in the article here on UT..

  9. Member
    David Gell says

    I find it of passing interest that the central character in Robert L. Forward’s hard SciFi novel “Timemaster” made man’s first interstellar voyage to the Centauri system. He found no habitable planets around Alpha Centauri A or B, but did find one around Proxima Centauri — with a 3:2 rotation, I believe. I seem to recall that it orbited in about 4 days.

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