Astronomers making visible-light observations with NASA's Hubble Space
Telescope have deduced the actual color of a planet orbiting another star 63
light-years away.
The planet is HD 189733b, one of the closest exoplanets that can be seen
crossing the face of its star.
Hubble's Space Telescope Imaging Spectrograph measured changes in the color
of light from the planet before, during and after a pass behind its star. There
was a small drop in light and a slight change in the color of the light. "We saw
the light becoming less bright in the blue but not in the green or red. Light
was missing in the blue but not in the red when it was hidden," said research
team member Frederic Pont of the University of Exeter in South West England.
"This means that the object that disappeared was blue."
This artist's concept shows exoplanet HD 189733b
orbiting its yellow-orange star, HD 189733. NASA's Hubble Space Telescope
measured the actual visible-light color of the planet, which is deep
blue.
Image Credit: NASA, ESA, and G. Bacon (STScI)
Earlier observations have reported evidence for scattering of blue light on
the planet. The latest Hubble observation confirms the evidence.
If seen directly, this planet would look like a deep blue dot, reminiscent of
Earth's color as seen from space. That is where the comparison ends.
On this turbulent alien world, the daytime temperature is nearly 2,000
degrees Fahrenheit, and it possibly rains glass -- sideways -- in howling,
4,500-mph winds. The cobalt blue color comes not from the reflection of a
tropical ocean as it does on Earth, but rather a hazy, blow-torched atmosphere
containing high clouds laced with silicate particles. Silicates condensing in
the heat could form very small drops of glass that scatter blue light more than
red light.
Hubble and other observatories have made intensive studies of HD 189733b and
found its atmosphere to be changeable and exotic.
HD 189733b is among a bizarre class of planets called hot Jupiters, which
orbit precariously close to their parent stars. The observations yield new
insights into the chemical composition and cloud structure of the entire
class.
This plot compares the colors of planets in our
solar system to exoplanet HD 189733b. The exoplanet's deep blue color is
produced by silicate droplets, which scatter blue light in its
atmosphere.
Image Credit: NASA, ESA, and A. Feild (STScI)
Clouds often play key roles in planetary atmospheres. Detecting the presence
and importance of clouds in hot Jupiters is crucial to astronomers'
understanding of the physics and climatology of other planets.
HD 189733b was discovered in 2005. It is only 2.9 million miles from its
parent star, so close that it is gravitationally locked. One side always faces
the star and the other side is always dark.
In 2007, NASA's Spitzer Space Telescope measured the infrared light, or heat,
from the planet, leading to one of the first temperature maps for an exoplanet.
The map shows day side and night side temperatures on HD 189733b differ by about
500 degrees Fahrenheit. This should cause fierce winds to roar from the day side
to the night side.
Text issued as NASA Headquarters release
No. 13-202
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