For the first time, scientists have determined the color of a planet outside our solar system.
Astronomers using the Hubble Space Telescope have for the first time determined the true color of a planet outside our solar system. The planet, known as HD 189733b, has seemingly earned the HD in its functional title, having proved to be a high-definition-like azure blue.
That deep blue color came as surprise, since scientists had expected the planet to be either dark or white. One prediction was that HD 189733b was swaddled in sodium gases that would absorb most of the visible light, leaving it dark. Another was that the atmosphere was instead laced with silicates that would reflect the light, making it white.
“The blue color was totally unexpected,” said Frédéric Pont, senior lecturer in astrophysics at The University of Exeter.
Dr. Pont proposes that the blue color could be the result of "glass rain." Silicate particles in the planet's atmosphere could scatter the bluish wavelengths coming from its star, just as tiny particles in Earth's atmosphere do with light from our sun, which our oceans then reflect back into space.
This is all conjecture, however. “I wouldn’t bet my house on the silicate explanation,” said Pont.
Discerning an alien planet’s color is a difficult and time-consuming process, and it is only at present possible for a handful of exoplanets. To determine HD 189733b’s color, scientists had to isolate the planet's light from the starlight, using Hubble's Space Telescope Imaging Spectrograph to look at how light reflected from the planet before, during, and after it passed behind its host star in orbit.
When the planet slunk behind the star, the light reflected from the planet was blocked and the amount of light observed from the entire sun-planet system dropped. But the drop in light was not uniform across the color spectrum – it was the blue part of the spectrum that dropped, while all other colors remained constant, suggesting that the planet is blue.