First planet orbiting binary stars discovered

[Andrew J.]

From the New York Times:

NASA Detects Planet Dancing With a Pair of Stars
By DENNIS OVERBYE

From double sunrise to double sunset the show goes on, always changing.

Sometimes the orange sun rises first. Sometimes it is the red one, although they are never far apart in the sky and you can see them moving around each other, casting double shadows across the firmament and periodically crossing right in front of each other.

Such is life, if it were possible, on the latest addition to the pantheon of weird planets now known to exist outside the bounds of our own solar system. It is the first planet, astronomers say, that has been definitely shown to be orbiting two stars at once, circling the pair — which themselves orbit each other tightly — at a distance of some 65 million miles.

A team of astronomers using NASA’s Kepler planet-hunting spacecraft announced the discovery on Thursday in a paper published online in the journal Science, in a talk at a conference in Jackson Hole, Wyo., and in a news conference at NASA’s Ames Research Laboratory in Mountain View, Calif., Kepler’s headquarters.

The official name of the new planet is Kepler 16b, but astronomers are already referring to it informally as Tatooine, after the home planet of Luke and Anakin Skywalker in the George Lucas “Star Wars” movies, which also had two suns.

“Reality has finally caught up with science fiction,” said Alan P. Boss of the Carnegie Institution, a member of the research team.

Indeed, John Knoll, who is a visual effects supervisor at Industrial Light & Magic, which is part of Lucasfilm, and who worked on several of the “Star Wars” movies, joined the Ames news conference and showed a clip from the original movie.

“Again and again we see that the science is stranger and weirder than fiction,” Mr. Knoll said. “The very existence of this discovery gives us cause to dream bigger.”

While some double-star systems, of which there are billions in the galaxy, have been suspected to harbor planets, those smaller bodies have never been seen.

“This is a direct detection; it removes all doubt,” said Laurance Doyle of the SETI Institute in Mountain View, Calif., who led the discovery team.

Beyond the wow factor, astronomers said the discovery — as so many discoveries of so-called exoplanets have done — had thrown a wrench into another well-received theory of how planets can and cannot form. “In other words,” said Sara Seager, a planetary expert at the Massachusetts Institute of Technology who was not part of the discovery team, “people don’t really know how to form this planet.”

It was long thought, Dr. Seager said, that for its orbit to be stable, a planet belonging to two stars at once would have to be at least seven times as far from the stars as the stars were from each other. According to that, Kepler 16b would have to be twice as far out as it is to survive.

“This planet broke the rule,” she said.

Moreover, by timing all the eclipses and transits of the planet and stars in the system, the astronomers have been able to measure the sizes and masses of the stars and the planet to unusually high precision, calibrating models of stellar and planetary properties.

“I believe this is the best-measured planet outside the solar system,” Dr. Doyle said.

Technically, Tatooine is probably a ball of rock and gas about the size and density of Saturn living in a system about 200 light-years away, in the constellation Cygnus.

If you go, pack to wear layers. Because those suns move back and forth all the time, temperatures on the planet can change by 50 degrees or more over the course of a few Earth days, from minus 100 to minus 150 Fahrenheit. So the weather is like “a nippy day in Antarctica at best,” as Dr. Doyle put it.

Kepler, launched in 2009, is on a mission to determine the fraction of stars in the galaxy that have Earth-like planets. It scrutinizes a patch of some 155,000 stars in the constellations Cygnus and Lyra looking for dips in starlight when planets cross in front of their home stars.

In the case of the Kepler 16 system — home to Tatooine — there turned out to be a lot of dips. The two stars are about 20 million miles apart and produce two eclipses every 41 days as they take turns going in front of each other. One star is about two-thirds the mass of the Sun, the other about a fifth of the Sun.

In addition, there are smaller dips when the planet, which is about 65 million miles from the center of the system — about the distance of Venus from the Sun — passes in front of each of the stars in the course of its 229-day orbit.

The degree of dimming during the planetary transits — those times that a planet crosses the path of something else — usually allows Kepler astronomers to measure the size of a planet relative to the stars. As a result, uncertainties in the properties of stars propagate into uncertainties of as much as 25 percent in the mass of a planet — enough to blur the line between a rocky planet and a gaseous one.

But in the Kepler 16 system, by comparing slight variations in the timing of the transits with calculations of the positions of the stars and the gravitational nudges the bodies give one another, Dr. Doyle’s team could deduce the absolute masses and sizes of the stars and planets in the system. That is a tool, they say, that is becoming increasingly valuable for determining the masses of small planets in multiple-planet systems.

As a result, said Dr. Doyle, “it’s a laboratory for all sorts of physics and stellar evolution.”

The Tatooine laboratory will be available to a wide audience for at least a while longer. Dr. Doyle noted that amateur astronomers in northern Asia, equipped with as little as an eight-inch telescope and an off-the-shelf C.C.D. detector (an electronic device that cameras use to capture images), would be able to record the passage of the Tatooine planet across the brighter star in its system on June 28 next year.

But enjoy it while you can. Because of variations in the planet’s orbital plane, as seen from Earth, the planet will stop crossing one of the stars as soon as 2014 and cease transiting the other, brighter one in 2018. It will be around 2042 before the show starts up again for Earthlings.

[Guardsman Bass]

That's good news, even if the planet in question is a cold Saturn-sized gas giant. I'm hoping that the next step will be to find a "super-Earth" orbiting around a binary pair.

[Modax]

So once again we have to shift our estimate of the number of planets in the galaxy up. If planets form anywhere, even in binary star systems there must be trillions of them. To think that 20 years ago we had no evidence of the existence of exoplanets. Unbelievable.

[Lord Baal]

Hahaha.. in the face of all those fuckers that always said that was impossible.

[Iroscato]

*Begins humming John William's score*
Never thought this was possible, guess we were all wrong.

[Cykeisme]

That's crazy awesome.

My first thought before reading the article was "Tatooine", great to see the astronomers were thinking exactly the same thing!

[Korgeta]

Great news though would it possible for humans to survive on a 'earth like' planet with orbiting binary stars?

[Number Theoretic]

Depends. If the binary star has a habitable zone and the planet stays nicely into it, i see no fundamental reason, why this is impossible.

It would be funny, if this name sticks and everyone knows this planet as "Tatooine".

[madd0ct0r]

except in this case, the planet is firmly beyond the habitable zone, AND it's already much closer then previously believed possible.

So since that theory will have to be rewritten, I suppose the chance of a hab planet on a binary star might just be possible.

How close can the stars get to each other before falling in?

[starslayer]

The planet is not much closer than previously believed possible. The period of the binary is only 41 days (separation ~.2 AU, IIRC), and consists of a .7 solar mass and a .2 solar mass star. Although this does constitute a three-body problem, for a planet (assumed mass much less than that of either star) the ratio of binary separation radius to stable orbit radius has been known for quite some time: about 3:1. This ratio is affected by the mass ratio of the binary and other factors, but it works as a first approximation in most cases.