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Thedark side ofextrasolar planets sharesurprisinglysimilartemperatures

New study suggests thatthe nightsides ofhotJupitersshare cloudsmadeof minerals
Published: 26 August 2019

A new study by ֱUniversityastronomershas foundthatthe temperature on thenightsidesofdifferenthot Jupitersis surprisinglyuniform, suggesting thedark side of thesemassive gaseous planetshaveclouds made of minerals and rocks.

UsingdatafromtheSpitzer Space and the Hubble Spacetelescopes, the researchers from the ֱ Space Institutefoundthat the nightside temperature of 12 hot Jupiters they studied wasabout 800°C.

Unlike our familiar planet Jupiter, so-called hot Jupiters circleveryclose to their host star -- so close that it typically takes fewer than three days to complete an orbit. As a result, hot Jupiters have daysides that permanently face their host stars and nightsides that always face the darkness of space, similarly to how the same side of the Moon always faces the Earth.The tight orbit also means these planetsreceive more sunlight from their star, which is what makes themextremelyhot on the dayside. But scientists had previously measured significant amounts of heat on the nightside of hot Jupiters,as well, suggesting some kind of energy transfer from one side to the other.

“Atmospheric circulation models predicted that nightside temperatures should vary much more than they do,” said Dylan Keating, aPhysicsPhD student under the supervision ofֱ professorNicolas Cowan. “This is really surprising because theplanetswe studiedall receive different amounts of irradiation from their host starsand thedayside temperaturesamong them varies by almost 1700°C.”

Keating,thefirst author of a newNature Astronomystudy describing the findings, saidthenightside temperatures are probably the result ofcondensation of vaporized rock in these very hot atmospheres.

“The uniformity of the nightside temperatures suggests that clouds on this side of the planets arelikely verysimilar to one another in composition. Our data suggest that these clouds are likely made ofminerals such as manganese sulfide or silicates,orrocks,” Keating explained.

According to Cowan,because thebasic physics of cloud formation are universal,the study of the nightside clouds on hot Jupiters could give insight into cloud formation elsewhere in the Universe, including on Earth.Keating said that future space telescope missions - such as the James Webb SpaceTelescopeandthe European Space Agency’sARIELmission- could be used to furthercharacterize the dominant cloud composition on hot Jupiter nightsides, as well as to improve models of atmospheric circulation and cloud formationofthese planets. 

“Observinghot Jupitersat both shorter and longer wavelengths will help us determine what types of clouds are on the nightsides of these planets,” Keating explained.

“Uniformly hot nightside temperatures on short-period gas giants,” by Dylan Keatinget al.was published in.

Graphic: Schematic of clouds on the night side of a hot Jupiter exoplanet. The underlying atmosphere is over 800 C, hot enough to vaporize rocks. Atmospheric motion from the deep atmosphere or from the hotter dayside bring the rock vapour to cooler regions, where it condenses into clouds, and possibly rains down into the atmosphere below. These clouds of condensed rock block outgoing thermal radiation, making the planet's nightside appear relatively cool from space.

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