Astronomers Discover Exoplanet With Triple Sunrises and Sunsets

This graphic shows the orbit of the planet in the HD 131399 system (red line) and the orbits of the stars (blue lines). The planet orbits the brightest star in the system, HD 131399A. Credit: ESO
This graphic shows the orbit of the planet in the HD 131399 system (red oval) and the orbits of the stars (blue arcs). The planet orbits the brightest star in the triple system, HD 131399A with a period of about 550 years. Credit: ESO

In the famous scene from the Star Wars movie “A New Hope” we recall young Luke Skywalker contemplating his future in the light of a binary sunset on the planet Tatooine. Not so many years later in 2011, astronomers using the Kepler Space Telescope discovered Kepler-16b, the first Tatooine-like planet known to orbit two suns in a binary system. Now astronomers have found a planet in a triple star system where an observer would either experience constant daylight or enjoy triple sunrises and sunsets each day, depending on the seasons, which last longer than human lifetimes.

They used the SPHERE instrument on the European Southern Observatory’s Very Large Telescope to directly image the planet, the first ever found inside a triple-star system. The three stars are named HD 131399A, HD 131399B and HD 131399C in order of decreasing brightness; the planet orbits the brightest and goes by the chunky moniker HD 131399Ab.

This annotated composite image shows the newly discovered exoplanet HD 131399Ab in the triple-star system HD 131399. The image of the planet was obtained with the SPHERE imager on the ESO Very Large Telescope in Chile. This is the first exoplanet to be discovered by SPHERE and one of very few directly-imaged planets. With a temperature of around 580 degrees Celsius and an estimated mass of four Jupiter masses, it is also one of the coldest and least massive directly-imaged exoplanets. This picture was created from two separate SPHERE observations: one to image the three stars and one to detect the faint planet. The planet appears vastly brighter in this image than in would in reality in comparison to the stars. Credit: ESO/K. Wagner et al.
This composite image shows the newly discovered exoplanet HD 131399Ab in the triple-star system HD 131399. The image of the planet was obtained with the SPHERE imager.  This is the first exoplanet to be discovered by SPHERE and one of very few directly-imaged planets. This picture was created from two separate SPHERE observations: one of the three stars and one to detect the faint planet. The planet appears vastly brighter in this image than in would in reality in comparison to the stars. Credit: ESO/K. Wagner et al.

Located about 320 light-years from Earth in the constellation of Centaurus the Centaur HD 131399Ab is about 16 million years old, making it also one of the youngest exoplanets discovered to date, and one for which we have a direct image. With a temperature of around 1,075° F (580° C) and the mass about four times that of Jupiter, it’s also one of the coldest and least massive directly-imaged exoplanets.

This infrared image of Saturn’s largest moon, Titan, was one of the first produced by the SPHERE instrument soon after it was installed on ESO’s Very Large Telescope in May 2014. This picture shows how effective the adaptive optics system is at revealing fine detail on this tiny disc (just 0.8 arc seconds across). Credit: ESO/J.-L. Beuzit et al./SPHERE Consortium
This infrared image of Saturn’s largest moon, Titan, was one of the first produced by the SPHERE instrument soon after it was installed on ESO’s Very Large Telescope in May 2014. This picture shows how effective the adaptive optics system is at revealing fine detail on this tiny disc (just 0.8 arc seconds across). Credit: ESO/J.-L. Beuzit et al./SPHERE Consortium

To pry it loose from the glare of its host suns, a team of astronomers led by the University of Arizona used a state of the art adaptive optics system to give razor-sharp images coupled with SPHERE, an instrument that blocks the light from the central star(s) similar to the way a coronagraph blocks the brilliant solar disk and allows study of the Sun’s corona. Finally, the region around the star is photographed in infrared polarized light to make any putative planets stand out more clearly against the remaining glare.

The planet, HD 131399Ab, is unlike any other known world — its orbit around the brightest of the three stars is by far the widest known within a multi-star system. It was once thought that planets orbiting a multi-star system would be unstable because of the changing gravitational tugs on the planet from the other two stars. Yet this planet remains in orbit instead of getting booted out of the system, leading astronomers to think that planets orbiting multiple stars might be more common that previously thought.

This artist's impression shows a view of the triple star system HD 131399 from close to the giant planet orbiting in the system. The planet is known as HD 131399Ab and appears at the lower-left of the picture. Credit: ESO / L. Calcada
This artist’s impression shows a view of the triple star system HD 131399 from close to the giant planet orbiting in the system. The planet is known appears at the lower-left of the picture. Credit: ESO / L. Calcada

HD 131399Ab orbits HD 131399A, estimated to be 80% more massive than the Sun. Its double-star companions orbit about 300 times the Earth-Sun distance away. For much of the planet’s 550 year orbit, all three stars would appear close together in the sky and set one after the other in unique triple sunsets and sunrises each day. But when the planet reached the other side of its orbit around its host sun, that star and the pair would lie in opposite parts of the sky. As the pair set, the host would rise, bathing HD 131399Ab in near-constant daytime for about one-quarter of its orbit, or roughly 140 Earth-years.


Click to see a wonderful simulation showing how the planet orbits within the trinary system

Planets in multi-star systems are of special interest to astronomers and planetary scientists because they provide an example of how the mechanism of planetary formation functions in these more extreme scenarios. Since multi-star systems are just as common as single stars, so planets may be too.

How would our perspective of the cosmos change I wonder if Earth orbited triple suns instead of a single star? Would the sight deepen our desire for adventure like the fictional Skywalker? Or would we suffer the unlucky accident of being born at the start of a multi-decade long stretch of constant daylight? Wonderful musings for the next clear night under the stars.

6 Replies to “Astronomers Discover Exoplanet With Triple Sunrises and Sunsets”

  1. Seen from Pluto the Sun is barly distinguishable from the background stars. The distance Sun – Pluto is 40 AU.
    The distance HD 131399Ab – HD 131399 B is more than 200 AU when the star is between the suns. So how can there be daylight if the star is barely visable?

    1. Actually, the Sun from Pluto at aphelion still presents an apparent magnitude of brighter than -18… more than 280,000x brighter than the Full Moon (dimmer than -13). A fun image search to do is for NASA’s “Pluto Time” public outreach project, where prior to New Horizon’s fly-by people sent in images of their own local sky at the time when the level of ambient sunlight matched that of high noon on Pluto’s surface: you might be surprised at just how bright that actually is! And since the exoplanet’s primary is 80% bigger than Sol, we can expect it to be somewhat brighter than Sol as well (not necessarily by 80%), so it’ll certainly be brighter than the Sun appears in Saturn’s orbit (~ -21 mag.), four times closer in than Pluto.

      It’s true the article doesn’t mention how big/bright the smaller co-orbiting binary pair is, but if we assume for imagination’s sake that they combine to produce only 50% of Sol’s visible output, then even at 200AU they should still shine ~ -14 mag… more than 2.5x brighter than the fullest of Full Moons seen from Earth. While one might not get a good bronzing at that level, the average human being would still see in color, and with an Earth-like atmosphere (let’s say, on a hypothetical Earth-sized exo-moon?) they’d have trouble seeing any but the very brightest of stars with just that pair up in the sky. With all three up, I imagine we’d have better luck stargazing during daytime here on Earth!

      1. Yes, I Know these pictures. Everybody knows the pictures New Horizons made of Pluto. Unless Nasa has really big spotlights everybody should know that there is enough light on Pluto to take pictures.

        To write that the star is barely visible was a big exaggeration. Of course it is very visible. In fact it would be the brightest star at the sky. But only a star. About .2 arcminutes wide if the bigger star is as big as the sun and the smaller is behind it.

        And here we allready have the first problem. The Position of the two stars. At the moment the smaller star is hidden. If he is right or left of the other star there would be more light.

        I guess that the bigger one is smaller than the sun. That’s why they gave it a redish color. The smaller one is a red dwarf at best, so its not that much light anyway.

        We don’t know how elliptic the planet is moving. The distance is at least 4x Sol-Pluto. That means there is only 1/16 of the light, probably less.
        Edit: If you can see in color at all, maybe an hour at noon on the equator. But I doubt that. Pluto has 2.5 times the light of a full moon. 1/20 * 2.5 equls 0.105 the light of a full moon. I just can’t imagine enough light to call it day.

        I really hope Bob will follow up on the story and show us the actual data. It would be really interesting to know.

  2. Almost sounds like the planetary system the Game of Thrones is depicted in.

  3. Just amazing Bob. I remember when the best image of Mars looked like that image of Titan. And to directly image another solar system 320 light years away is more than amazing. Hard to believe Ab won’t get kicked out.

Comments are closed.