Like a cosmic light bulb on a dimmer switch
Saturn emitted gradually less energy each year from 2005 to 2009, according to observations by NASA’s Cassini spacecraft. But unlike an ordinary bulb, Saturn’s southern hemisphere consistently emitted more energy than its northern one.
On top of that, energy levels changed with the seasons and differed from the last time a spacecraft visited in the early 1980s.
These never-before-seen trends came from an analysis of comprehensive data from the Composite Infrared Spectrometer (CIRS), an instrument built by NASA’s Goddard Space Flight Center in Greenbelt, Md., as well as a comparison with earlier data from NASA’s Voyager spacecraft. When combined with information about the energy coming to Saturn from the sun, the results could help scientists understand the nature of Saturn’s internal heat source.
The findings were reported November 9 in the Journal of Geophysical Research-Planets by Liming Li of Cornell University in Ithaca, N.Y. (now at the University of Houston), and colleagues from several institutions, including Goddard and NASA’s Jet Propulsion Laboratory in Pasadena Calif., which manages the Cassini mission. “The Cassini CIRS data are very valuable because they give us a nearly complete picture of Saturn,” says Li. “This is the only single data set that provides so much information about this planet, and it’s the first time that anybody has been able to study the power emitted by one of the giant planets in such detail.”
The planets in our solar system lose energy in the form of heat radiation in wavelengths that are invisible to the human eye. The CIRS instrument picks up wavelengths in the thermal infrared region, which is beyond red light, where the wavelengths correspond to heat emission.
“In planetary science, we tend to think of planets as losing power evenly in all directions and at a steady rate,” says Li. “Now we know Saturn is not doing that.” (Power is the amount of energy emitted per unit of time.)
Instead, Saturn’s flow of outgoing energy was lopsided, with its southern hemisphere giving off about one-sixth more energy than the northern one, Li explains. This effect matched Saturn’s seasons: during those five Earth years, it was summer in the southern hemisphere and winter in the northern one. (A season on Saturn lasts about seven Earth years.) Like Earth, Saturn has these seasons because the planet is tilted on its axis, so one hemisphere receives more energy from the sun and experiences summer while the other receives less energy and is shrouded in winter. Saturn’s equinox, when the sun was directly over the equator, occurred in August 2009.
In the study, Saturn’s seasons looked Earth-like in another way: in each hemisphere, its effective temperature, which characterizes its thermal emission to space, started to warm up or cool down as a change of season approached. Because Saturn’s weather is variable and the atmosphere tends to retain heat (called heat inertia), the temperature changes in complicated ways throughout the atmosphere. “The effective temperature provides us a simple way to track the response of Saturn’s atmosphere, as a system, to the seasonal changes,” says Li. Cassini’s observations in the northern hemisphere revealed that the effective temperature gradually dropped from 2005 to 2008 and then started to warm up again by 2009. In Saturn’s southern hemisphere, the effective temperature cooled from 2005 to 2009, as the equinox started to approach.
The emitted energy for each hemisphere rose and fell along with the effective temperature. Even so, during this five-year period, the planet as a whole seemed to be slowly cooling down and emitting less energy.
more via sciencedaily.com