Hubble Uncovers a 'Heavy Metal' Exoplanet Shaped Like a Football:
Observations by NASA's Hubble Space Telescope reveal magnesium and iron gas streaming from the strange world outside our solar system known as WASP-121b. The observations represent the first time that so-called "heavy metals" -- elements heavier than hydrogen and helium -- have been spotted escaping from a hot Jupiter, a large, gaseous exoplanet very close to its star.
Normally, hot Jupiter-sized planets are still cool enough inside to condense heavier elements such as magnesium and iron into clouds.
But that's not the case with WASP-121b, which is orbiting so dangerously close to its star that its upper atmosphere reaches a blazing 4,600 degrees Fahrenheit[*]. The temperature in WASP-121b's upper atmosphere is about 10 times greater than that of any known planetary atmosphere. The WASP-121 system resides about 900 light-years from Earth.
"Heavy metals have been seen in other hot Jupiters before, but only in the lower atmosphere," explained lead researcher David Sing of the Johns Hopkins University in Baltimore, Maryland. "So you don't know if they are escaping or not. With WASP-121b, we see magnesium and iron gas so far away from the planet that they're not gravitationally bound."
Ultraviolet light from the host star, which is brighter and hotter than the Sun, heats the upper atmosphere and helps lead to its escape. In addition, the escaping magnesium and iron gas may contribute to the temperature spike, Sing said. "These metals will make the atmosphere more opaque in the ultraviolet, which could be contributing to the heating of the upper atmosphere," he explained.
The sizzling planet is so close to its star that it is on the cusp of being ripped apart by the star's gravity. This hugging distance means that the planet is football[**] shaped due to gravitational tidal forces.
[*] Approximately 2500° C
[**] American football; think of a rugby ball for our internationalists.
Journal Reference:
David K. Sing, et. al. The Hubble Space Telescope PanCET Program: Exospheric Mg ii and Fe ii in the Near-ultraviolet Transmission Spectrum of WASP-121b Using Jitter Decorrelation. The Astronomical Journal, 2019; 158 (2): 91 DOI: 10.3847/1538-3881/ab2986
(Score: 3, Interesting) by takyon on Friday August 02 2019, @11:51PM (1 child)
It's biased towards finding hot exoplanets with short orbital periods within the first two years of operations, except for narrow parts of the sky where it will observe for longer.
https://en.wikipedia.org/wiki/File:TESS_science_sector_suddivision.jpg [wikipedia.org]
After the first two years, they could change things up.
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(Score: 2) by takyon on Friday August 02 2019, @11:54PM
https://www.sciencedaily.com/releases/2019/07/190731125428.htm [sciencedaily.com]
[SIG] 10/28/2017: Soylent Upgrade v14 [soylentnews.org]