Considered an ultra-hot Jupiter – a place where iron gets vaporized, condenses on the night side and then falls from the sky like rain – the fiery, inferno-like WASP-76b exoplanet may be even more sizzling than scientists had realized.
An international team, led by scientists at Cornell University, University of Toronto and Queen’s University Belfast, reports the discovery of ionized calcium on the planet – suggesting an atmospheric temperature higher than previously thought, or strong upper atmosphere winds.
The discovery was made in high-resolution spectra obtained with Gemini North near the summit of Mauna Kea in Hawaii.
Hot Jupiters are named for their high temperatures, due to proximity to their stars. WASP-76b, discovered in 2016, is about 640 light-years from Earth, but so close to its F-type star, which is slightly hotter than the sun, that the giant planet completes one orbit every 1.8 Earth days.
The research results are the first of a multiyear, Cornell-led project, Exoplanets with Gemini Spectroscopy survey, or ExoGemS, that explores the diversity of planetary atmospheres.
“As we do remote sensing of dozens of exoplanets, spanning a range of masses and temperatures, we will develop a more complete picture of the true diversity of alien worlds – from those hot enough to harbor iron rain to others with more moderate climates, from those heftier than Jupiter to others not much bigger than the Earth,” said co-author Ray Jayawardhana, Harold Tanner Dean of the College of Arts and Sciences at Cornell University and a professor of astronomy.
“It’s remarkable that with today’s telescopes and instruments, we can already learn so much about the atmospheres – their constituents, physical properties, presence of clouds and even large-scale wind patterns – of planets that are orbiting stars hundreds of light-years away,” Jayawardhana said.
The group spotted a rare trio of spectral lines in highly sensitive observations of the exoplanet WASP-76b’s atmosphere, published in the Astrophysical Journal Letters on September 28 and presented on October 5 at the annual meeting of the Division for Planetary Sciences of the American Astronomical Society.
“We’re seeing so much calcium; it’s a really strong feature,” said first author Emily Deibert, a University of Toronto doctoral student, whose adviser is Jayawardhana.
“This spectral signature of ionized calcium could indicate that the exoplanet has very strong upper atmosphere winds,” Deibert said. “Or the atmospheric temperature on the exoplanet is much higher than we thought.”
Since WASP-76b is tidally locked – in that one side of it always faces the star – it has a permanent night side that sports a relatively cool 2,400-degree Fahrenheit average temperature. Its day side, facing toward the star, has an average temperature at 4,400 degrees F.
Deibert and her colleagues examined the moderate temperature zone, on the planet’s limb between day and night. “The exoplanet moves fast on its orbit and that’s how we were able to separate its signal from starlight,” she said. “You can see that the calcium imprint on the spectra is moving quickly along with the planet.”
The ExoGemS survey – intended to study 30 or more planets – is led by Jake Turner, a Carl Sagan Fellow in NASA’s Hubble Fellowship program, who is in Cornell’s Department of Astronomy (A&S) and is also advised by Jayawardhana.
Astronomers continue to delve deeper to understand exoplanets – considered just a dream two decades ago. “Our work, and that of other researchers, is paving the way for exploring the atmospheres of terrestrial worlds beyond our solar system,” Turner said.
Reference: “Detection of Ionized Calcium in the Atmosphere of the Ultra-Hot Jupiter WASP-76b” by Emily K. Deibert, Ernst J. W. de Mooij, Ray Jayawardhana, Jake D. Turner, Andrew Ridden-Harper, Luca Fossati, Callie E. Hood, Jonathan J. Fortney, Laura Flagg, Ryan MacDonald, Romain Allart and David K. Sing, 28 September 2021, The Astrophysical Journal Letters.
Other authors on the paper include Ernst J. W. de Mooij of the Queen’s University Belfast; Luca Fossati of the Austrian Academy of Sciences; Callie E. Hood and Jonathan J. Fortney, both from University of California, Santa Cruz; Romain Allart of the University of Montreal; and David K. Sing of Johns Hopkins University. Cornellians included researchers Andrew Ridden-Harper and Laura Flagg, both in Jayawardhana’s group, and Ryan MacDonald. Portions of this research were funded by NASA.
Gemini North is part of the international Gemini Observatory, a program of National Science Foundation’s NOIRLab.