Bright Meteoroid Explosion Above Jupiter’s Clouds Observed By Juno Spacecraft’s Instrument

“Jupiter undergoes a huge number of impacts per year, much more than the Earth, so impacts themselves are not rare,” said SwRI’s Dr. Rohini Giles, lead author of a paper outlining these findings in Geophysical Research Letters. “However, they are so short-lived that it is relatively unusual to see them. Only larger impacts can be seen from Earth, and you have to be lucky to be pointing a telescope at Jupiter at exactly the right time. In the last decade, amateur astronomers have managed to capture six impacts on Jupiter.”

During the course of a 30-second spin, UVS observes a swath of the planet. The UVS instrument has occasionally observed short-lived, localized ultraviolet emissions outside of the auroral zone, including a singular event on April 10, 2020.

“This observation is from a tiny snapshot in time — Juno is a spinning spacecraft, and our instrument observed that point on the planet for just 17 milliseconds, and we don’t know what happened to the bright flash outside of that time frame,” Giles said, “But we do know that we didn’t see it on an earlier spin or a later spin, so it must have been pretty short-lived.”

Previously, UVS had observed a set of eleven bright transient flashes that lasted 1 to 2 milliseconds. They were identified as Transient Luminous Events (TLEs), an upper atmospheric phenomenon triggered by lightning. The team initially thought this bright flash might be a TLE, however, it was different in two key ways. While it was also short-lived, it lasted at least 17 milliseconds, much longer than a TLE. It also had very different spectral characteristics. Spectra of TLEs and auroras feature emissions of molecular hydrogen, the main component of Jupiter’s atmosphere. This bolide event had a smooth “blackbody'” curve, which is what is expected from a meteor.

“The flash duration and spectral shape match up well with what we expect from an impact,” Giles said. “This bright flash stood out in the data, as it had very different spectral characteristics than the UV emissions from Jupiter’s auroras. From the UV spectrum, we can see that the emission came from a blackbody with a temperature of 9600 Kelvin, located at an altitude of 140 miles above the planet’s cloud tops. By looking at the brightness of the bright flash, we estimate that it was caused by an impactor with a mass of 550-3,300 pounds.”

Comet Shoemaker-Levy was the largest observed Jupiter impactor. The comet broke apart in July 1992 and collided with Jupiter in July 1994, which was closely observed by astronomers worldwide and the Galileo spacecraft. An SwRI-led team detected impact-related X-ray emissions from Jupiter’s northern hemisphere, and prominent scars from the impacts persisted for many months.

“Impacts from asteroids and comets can have a significant impact on the planet’s stratospheric chemistry — 15 years after the impact, comet Shoemaker-Levy 9 was still responsible for 95% of the stratospheric water on Jupiter,” Giles said. “Continuing to observe impacts and estimating the overall impact rates is therefore an important element of understanding the planet’s composition.”

Written by Eddie Gonzales Jr. – MessageToEagle.com Staff