Astronomers Discover a Planet of Boiling Lava With an Eight-Hour Year

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Aug. 20 2013 10:30 AM

A Boiling Lava Planet With an Eight-Hour Year

artwork of an exoplanet
Artwork depicting an exoplanet close to its parent star.

Artwork by ESO/L. Calçada

Another really weird planet orbiting another star has been found, and it’s a world of extremes: The orbital period—its year—is only 8½ hours long, and it’s so hot it must have a molten surface of boiling lava. Not only that, but it’s roughly the same size as Earth!

Phil Plait Phil Plait

Phil Plait writes Slate’s Bad Astronomy blog and is an astronomer, public speaker, science evangelizer, and author of Death from the Skies!  

The planet is called Kepler-78b and is located about 700 light-years from Earth. The parent star, called just Kepler-78, is slightly smaller, cooler, and lower mass than the Sun. It’s less than 1 billion years old, making it far younger than the Sun as well.

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The planet was detected using the transit method. If a planet’s orbit is edge-on as seen from Earth, it blocks a tiny bit of light from the star every time it orbits (like a bug flying between you and a light). The star is relatively bright—about 11th magnitude, visible in a small telescope—which means it was extremely well-observed, and even though the amount of light blocked by the planet was tiny, it boomed right out of the observations:

kepler78b_lightcurve
The change in light from the star Kepler-78 as the planet moves around it.

Plot by Sanchis-Ojeda et al.

That diagram is from the announcement paper for the planet. When I saw it, I was stunned. It’ll take a moment to explain why, but bear with me. This is cool.

First, the graph plots light from the star and planet over time; about 12 hours is covered. The big dip is from when the planet is directly between us and the star. The units on the left are parts per million, so the planet blocks about 200 one-millionths of the star’s light, or 0.02 percent. That’s a teeny tiny amount, but clearly seen.

The black dots plot the starlight over one planetary orbit, and it repeats at about the seven-hour mark. (It’s plotted this way to make it easy to see the repeating pattern in the light.) The diagram inset in the middle shows the relative size of the star, planet, and the planet’s orbit (dashed line). That’s to scale: The planet circles the star, staying just three times the star’s own radius from the surface! That means the planet is boiling hot, with a surface temperature of about 4,800 degrees Celsius (8,700 degrees Fahrenheit).

But it’s the middle part of the graph that blew me away. If the light we saw were steady, then that would be a flat line between transits. But it’s not: You can see it rises a bit, then there is a second, much shallower dip starting at the 3½-hour mark, then it drops slowly again.

What you’re seeing there is the light from the planet itself, changing like the phases of the Moon as it orbits the star, and then getting blocked as it passes behind the star.

That’s astonishing. I mean, seriously, we’re seeing the changing phase of the planet itself! Here’s an animation made for a similar discovery in 2009, showing how this works:

When the planet is directly between the star and us, we see its unlit half. As it orbits around the star, we see gradually more of it, lit like a crescent Moon, so it gets brighter. Then we see it half full, three-quarters full … and just as we’d see it becoming fully lit, it passes behind the star itself, and we get that little dip in the light. So what you’re seeing there is actually the combined light of the star and the planet, too. We’re probably seeing reflected starlight off the planet, like the Moon is lit from the Sun. But again, note the small change: It only adds up to about 10 parts per million! The star is hundreds of thousands of times brighter, but the planet makes itself get noticed in all that blaring light.

Kepler-78b is a pretty spectacular place. While we can’t determine its mass very well, it’s certainly less than about eight times the Earth’s mass, most likely close to Earth’s own heft. It’s only about 1.2 times the radius of the Earth, so it’s very close to our size. But Earth it ain’t. Poking around the Web, I didn’t find any common metals that are solid at 4,800 degrees Celsius, which means no matter what, the surface of this planet is molten. If it has an atmosphere at all, it’ll be vaporized rock and metals.

And on top of it all, its year is only a few hours long. Only a handful of planets known orbit their stars more rapidly. That close to the star it’s probably tidally locked, too, so it always shows the same face to the star; one side of the planet is infernally hot and the other would be somewhat cooler. But even so, the whole surface would be a world-spanning ocean of churning liquid rock and metal. Crazy.

This is yet more evidence that the Universe is more clever than we are when it comes to creating worlds. But we’re clever, too, and we can find them. And the more we see, the better we understand how they form, how they exist, and the more we are able to understand about our own blue-green—and very temperate—planet.