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exoplanets

‘Sunscreen snow’ falls on hot planet’s dark side

Using the Hubble Space Telescope, astronomers have discovered that a blistering-hot, giant planet outside our solar system has “snow” made of titanium dioxide—the active ingredient in sunscreen.

These Hubble observations are the first detections of this “snow-out” process, called a “cold trap,” on an exoplanet. This discovery, and other observations made by the same team, provide insight into the complexity of weather and atmospheric composition on exoplanets, and may someday be useful for gauging the habitability of Earth-size planets.

“In many ways, the atmospheric studies we’re doing now on these gaseous ‘hot Jupiter’ kinds of planets are test beds for how we’re going to do atmospheric studies of terrestrial, Earth-like planets,” says Thomas Beatty, assistant research professor of astronomy at Penn State and the lead author of the study.

Kepler-13ab size diagram
This is an artist’s impression of the gas giant planet Kepler-13Ab as compared in size to several planets in our solar system. The behemoth exoplanet is six times more massive than Jupiter. (Credit: NASA, ESA, and A. Feild (STScI) via Penn State)

“Understanding more about the atmospheres of these planets and how they work will help us when we study smaller planets that are harder to see and have more complicated features in their atmospheres.”

The hottest exoplanet

Beatty’s team targeted planet Kepler-13Ab because it is one of the hottest of the known exoplanets. Its dayside temperature is nearly 5,000 degrees Fahrenheit.

In a system 1,730 light-years from Earth, Kepler-13Ab is so close to its parent star that it is tidally locked, so one side always faces the star while the other side is in permanent darkness.

The team discovered that the “sunscreen snowfall” happens only on the planet’s permanent nighttime side. Any visitors to this exoplanet would need to bottle up some of that sunscreen, because they won’t find it on the sizzling-hot daytime side.

Kepler 13 illustration
This illustration shows the seething hot planet Kepler-13Ab that circles very close to its host star, Kepler-13A. In the background is the star’s binary companion, Kepler-13B, and the third member of the multiple-star system is the orange dwarf star Kepler-13C. (Credit: NASA, ESA, and G. Bacon (STScI) via Penn State)

The astronomers didn’t go looking for titanium oxide specifically. Instead, their studies revealed that this giant planet’s atmosphere is cooler at higher altitudes—which was surprising because it is the opposite of what happens on other hot Jupiters. Titanium oxide in the atmospheres of other hot Jupiters absorbs light and reradiates it as heat, making the atmosphere grow warmer at higher altitudes. Even at their much colder temperatures, most of our solar system’s gas giants also have warmer temperatures at higher altitudes.

Intrigued by this discovery, researchers concluded that the light-absorbing gaseous form of titanium oxide has been removed from the dayside of planet Kepler-13Ab’s atmosphere. Without the titanium oxide gas to absorb incoming starlight on the daytime side, the atmospheric temperature there grows colder with increasing altitude.

The astronomers suggest that powerful winds on Kepler-13Ab carry the titanium oxide gas around, condensing it into crystalline flakes that form clouds. Kepler-13Ab’s strong surface gravity—six times greater than Jupiter’s—then pulls the titanium oxide snow out of the upper atmosphere and traps it in the lower atmosphere on the nighttime side of the planet.

Gas ‘monster’ challenges how planets form

“Understanding what sets the climates of other worlds has been one of the big puzzles of the last decade,” says Jason Wright, associate professor of astronomy and one of the study’s coauthors. “Seeing this cold-trap process in action provides us with a long sought and important piece of that puzzle.”

Confirming a theory

The team’s observations confirm a theory from several years ago that this kind of precipitation could occur on massive, hot planets with powerful gravity.

“Presumably, this precipitation process is happening on most of the observed hot Jupiters, but those gas giants all have lower surface gravities than Kepler-13Ab,” Beatty explains. “The titanium oxide snow doesn’t fall far enough in those atmospheres, and then it gets swept back to the hotter dayside, revaporizes, and returns to a gaseous state.”

The researchers used Hubble’s Wide Field Camera 3 to conduct spectroscopic observations of the exoplanet’s atmosphere in near-infrared light. Hubble made the observations as the distant world traveled behind its star, a transit event called a secondary eclipse. This type of transit yields information on the temperature of the components of the atmosphere on the exoplanet’s dayside.

“These observations of Kepler-13Ab are telling us how condensates and clouds form in the atmospheres of very hot Jupiters, and how gravity will affect the composition of an atmosphere,” Beatty explains. “When looking at these planets, you need to know not only how hot they are, but also what their gravity is like.”

Spot exoplanets from Earth with new telescope add-on

The research appears in the Astronomical Journal.

Additional researchers contributing to the work are from Penn State, the University of Cambridge, the University College London, and the California Institute of Technology.

NASA and the Penn State Center for Exoplanets and Habitable Worlds funded the research.

The Hubble Space Telescope is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, Inc., in Washington, DC.

Source: Penn State

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