Saturn's
aurora, a ghostly ultraviolet glow that illuminates the gas giant's
upper atmosphere near the poles, has a heartbeat that pulses in tandem
with the planet's radio emissions, scientists have discovered.
The pulsing auroras on Saturn occur about once every 11 Earth hours or
so ? the length of one day on the ringed planet, researchers found.
"This is an important discovery for two reasons,"
said study leader Jonathan Nichols of the University of Leicester in
England. "First, it provides a long-suspected but hitherto missing link
between the radio and auroral emissions, and second, it adds a critical
tool in diagnosing the cause of Saturn's irregular heartbeat."
Saturn's heartbeat
Like all magnetized planets, Saturn emits radio waves into space from its polar regions.
These emissions pulse at intervals of about 11 hours. During the twin
Voyager missions, both launched in 1977, the timing of the pulses were
thought to represent the planet's rotational period.
But,
observations over the years noted that the pulsing of the radio
emissions has varied. Since the rotation of a planet cannot easily
change speed, the source of Saturn's fluctuating radio period mystified
planetary scientists.
Similarly, the length of a day on Saturn
has generated debate, since traditional clocks are unreliable
timekeepers in determining the rotational period of a planet with no
solid surface for reference.
In a new study, researchers show that, not only do radio emissions pulse, the planet's auroras also beat in tandem.
Auroras on Saturn
Nichols and his team used images of Saturn's auroras from the Hubble
Space Telescope that were obtained between 2005 and 2009. The findings
of the study will be published in the Aug. 6 edition of the journal
Geophysical Research Letters.
On Earth, auroras are caused
when charged particles in space stream down the planet's magnetic field
lines toward the poles. The interaction of these particles with atoms of
nitrogen and oxygen in the Earth's atmosphere cause them to glow.
Auroras on Earth can occur when the planet's magnetic field is
bombarded by particles emitted by the sun. On Saturn, auroras can occur
when moons such as Enceladus or Io expel particulate material into the
near-planet space.
It was long suspected that Saturn's radio
waves were emitted by these charged particles as they traveled toward
the poles, but radio-like pulsing had not been observed in Saturn's
aurora. This puzzled astronomers, since the two phenomena were seemingly
related.
In this recent study, however, Nichols and his team
of researchers used the clock of Saturn's radio pulsing to organize the
planet's aurora data.
They also stacked the results from all of
Hubble's Saturn aurora images (obtained from 2005 to 2009) on top of
each other. By doing this, the aurora pulsing finally revealed itself.
"This confirms that the auroras and the radio emissions are indeed
physically associated, as suspected," Nichols said. "This link is
important, since it implies that the pulsing of the radio emissions is
being imparted by the processes driving Saturn's aurora, which in turn
can be studied by the NASA/ESA spacecraft Cassini, presently in orbit
around Saturn. It thus takes us a significant step toward solving the
mystery of the variable radio period."
