Astronomers said that a shower of charged particles from the heavens drives the northern lights of Saturn. However, some of its auroras show only when violent winds rage across the north pole, like a gust of wind stoking a cosmic flame.
Experts believe the weather system powers the system from Saturn's thermosphere, with ionosphere wind rates reaching three kilometers per second.
Researchers detailed the study, "Saturn's Weather-Driven Aurorae Modulate Oscillations in the Magnetic Field and Radio Emissions," in Geophysical Research Letters.
IN SPACE - MAY 21: In this handout image provided by the National Aeronautics and Space Administration (NASA), the shadow of Saturn on the rings is seen in visible light with the Cassini spacecraft wide-angle camera on May 21, 2016. The moon Mimas is seen near the lower left. The view was obtained at a distance of approximately 2.0 million miles from Saturn. Between April and September 2017, Cassini will plunge repeatedly through the gap that separates the planet from the rings. The Cassini mission is a cooperative project of NASA, ESA (the European Space Agency) and the Italian Space Agency.
Swirling Winds Cause Saturn And Jupiter's Aurora
The interaction of energized particles streaming from the planet's magnetosphere into its atmosphere mainly causes auroras. Charged particles from the sun fuel auroras on Earth, but charged particles from volcanic eruptions on the planets' moons power auroras on Jupiter and Saturn. This new sort of aurora spotted on Saturn is unique in that the planet's own atmospheric winds cause it.
The researchers studied the type of winds swirling around Saturn's upper atmosphere using the W. M. Keck Observatory on Mauna Kea, Hawai'i Island. The Near-Infrared Spectrograph (NIRSPEC) at the observatory detected infrared emissions from this region, which the scientists utilized to map the planet's weather currents.
Their findings show that the thermosphere powers Saturn's weather system, with winds in the ionosphere (below the magnetosphere) generating the planet's brilliant auroras.
Space.com said the planet's swirling winds appear to be responsible for the planet's irregular rate of rotation, which has made it impossible for experts to calculate how long the day lasts on the ringed world.
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Why Experts Had a Challenging Time Knowing Saturnian Day
Cassini attempted to address this question by tracing emission "pulses" from the planet's atmosphere. Still, it appeared that the planet's speed had changed since the last measurement taken by Voyager 2 in 1981. Researchers eventually used a new approach to determine the rate, which was 10 hours, 33 minutes, and 38 seconds.
Researchers said Saturn's intrinsic rotation rate must be constant. However, researchers have known for decades that various periodic features associated with the planet alter throughout time.
Leicester researcher Nahid Chowdhury said in a statement that there are independent periodic characteristics found in the northern and southern hemispheres, which vary throughout the course of a season on the globe.
Scientists have long questioned the origins of these lights, theorizing that they could be created by Enceladus' volcanic moon or interactions with Titan's thick atmosphere.
Dr. Kevin Baines, a member of the Cassini Science Team and co-author of the paper, said in the statement that the recent findings clear up a lot of the mystery around Saturn's mass rotation rate and the duration of the day on Saturn by establishing the source of the enigmatic variability in radio pulses.
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