Jupiter was observed with SOFIA by stepping the FORCAST spectroscopic slit across the planet. The left-hand panel shows a visible-light image of Jupiter with blue rectangles illustrating the orientation and size of the FORCAST slit. For each pointing of the telescope, the spectrum was made at every position along the slit. The two right-hand panels show SOFIA images of Jupiter made from combining the wavelengths in two of the slits. Jupiter’s Great Red Spot is evident and has rotated between the different observations. The total information content is full images of Jupiter at all wavelengths between 17.9 and 32.9 microns, or equivalently, spectra at each position. Credit: Visible light image: Anthony Wesley. FORCAST slitscan: NASA/SOFIA/Fletcher et al. For the first time since the twin Voyager spacecraft missions in 1979, scientists have produced far-infrared maps of Jupiter using NASA’s Stratospheric Observatory for Infrared Astronomy, SOFIA. These maps were created from the researchers’ studies of the circulation of gases within the gas giant planet’s atmosphere. Infrared observations provide details not possible at other wavelengths. When gas planets like Jupiter are studied with visible light, they can only see the light reflecting from the top of the gas clouds that make up the atmosphere. Using infrared light allows scientists to see past the clouds and into the deep layers of the atmosphere, providing a three-dimensional view of the planet and the ability to study how gasses circulate within the atmosphere.
Leigh N. Fletcher from the University of Leicester, England, led a team of researchers that used the SOFIA telescope and data from the Faint Object infraRed Camera for the SOFIA Telescope, known as FORCAST, to make these observations. Fletcher’s team was looking for the two types of molecular hydrogen, called ”para” and ”ortho” – differentiated by whether their protons have aligned or opposite spins. The fraction of hydrogen in the ”para” flavor is a good indicator for gasses upwelling from deep within the planet’s atmosphere. This interaction of gas molecules was observed at infrared wavelengths between 17 and 37 microns, a spectrum range that is largely inaccessible to ground-based telescopes.
Much of the current understanding of Jupiter’s circulation patterns are based on results from space-based missions of the past, including the Voyager mission, Galileo mission (1989–2003), and the Cassini spacecraft, which flew past Jupiter in 2000. SOFIA’s airborne location, above more than 99 percent of Earth’s infrared-blocking water vapor, combined with the powerful FORCAST instrument, provides one of the only current facilities capable of studying Jupiter’s overall atmospheric circulation. These new SOFIA observations allow comparisons of how Jupiter’s atmospheric circulation has changed over time.
Images from SOFIA reveal several interesting features. The cold, red spot in the southern hemisphere indicates an upwelling of gas that is cooling the atmosphere. The belt zone structure near the equator shows that the equator is cold and surrounded by warm belts of sinking gas. The atmospheric heating from Jovian aurora in the northern reaches of the planet indicates the presence of methane and ethane in the stratosphere. SOFIA’s unique observations of the comparison between ortho and para hydrogen reveal a gradual trend from the equatorial to polar regions.
Based upon earlier observations, Fletcher’s research team assumed that Jupiter should have equilibrium everywhere in its atmosphere, but they found that at low latitudes in the tropics there is significant mixing. Aureoles may be affecting this mixing, but further observations are necessary to better understand the processes over time. The results from the Fletcher team’s observations were recently published in the journal Icarus.
”These results demonstrate that from Earth we can now capture a similar quality of spatially resolved observations as we can obtain from space missions like Voyager,” said Fletcher. ”These SOFIA observations will fill the gap in the wavelength coverage of current and future space-based observatories and provide spatial and temporal context for them.”
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More information: Leigh N. Fletcher et al, Jupiter’s para-H2 distribution from SOFIA/FORCAST and Voyager/IRIS 17–37 µm spectroscopy, Icarus (2016). DOI: 10.1016/j.icarus.2016.10.002