SOFIA Finds Hidden Clues in Pluto’s Haze
Observations made with the Stratospheric Observatory for Infrared Astronomy (SOFIA) — a Boeing 747SP jetliner modified to carry a 106-inch diameter telescope — help explain how Pluto’s haze is formed and how the distant Sun affects the dwarf planet from 3.7 billion miles away.
When the New Horizons spacecraft passed by Pluto in 2015, its images revealed that this small, frigid world in the distant solar system has a hazy atmosphere. Now, new data from SOFIA helps explain how Pluto’s haze is formed from the faint light of the Sun 3.7 billion miles away as it moves through an unusual orbit.
Remote observations of Pluto by NASA’s airborne observatory SOFIA, show that the thin haze enshrouding Pluto is made of very small particles that remain in the atmosphere for prolonged periods of time rather than immediately falling to the surface. SOFIA’s data clarify that these haze particles are actively being replenished — a discovery that is revising predictions on the fate of Pluto’s atmosphere as it moves into even colder areas of space on its 248-Earth-year orbit around the Sun. The results are published in the scientific journal Icarus.
“Pluto is a mysterious object that is constantly surprising us,” said Michael Person, the lead author of the paper and director of Massachusetts Institute of Technology’s Wallace Astrophysical Observatory. “There had been hints in earlier remote observations that there might be haze, but there wasn’t strong evidence to confirm it really existed until the data came from SOFIA. Now we’re questioning if Pluto’s atmosphere is going to collapse in the coming years — it may be more resilient than we thought.”
SOFIA studied Pluto just two weeks before New Horizon’s flyby in July 2015. The modified Boeing 747 flew over the Pacific Ocean and pointed its nearly 9-foot telescope at Pluto during an occultation, an eclipse-like event in which Pluto cast a faint shadow on Earth’s surface as it passed in front of a distant star.
SOFIA observed the middle layers of Pluto’s atmosphere in the infrared and visible light wavelengths, and soon after, the New Horizons spacecraft probed its upper and lower layers using radio waves and ultraviolet light. These combined observations from SOFIA and New Horizons, taken so close in time, have provided the most complete picture yet of Pluto’s atmosphere.
Blue, Hazy Atmosphere
Created as surface ice vaporizes under the distant light of the Sun, Pluto’s atmosphere is predominantly nitrogen gas, along with small amounts of methane and carbon monoxide. Haze particles form high up in the atmosphere, more than 20 miles above the surface, as methane and other gases react to sunlight, before slowly raining down to the icy surface.
New Horizons found evidence of these particles when it sent back images showing a blue-tinted haze to Pluto’s atmosphere. Now, SOFIA’s observations fills in even more details by discovering that the particles are extremely small, just 0.06-0.10 micron thick, or 1,000 times smaller than the width of a human hair. Because of their small size, they scatter blue light more than other colors as they drift toward the surface, creating the blue tint.
With these new insights, scientists are reevaluating their predictions on the fate of Pluto’s atmosphere. Many forecasts indicated that as the dwarf planet moved away from the Sun, less surface ice would be vaporized — creating fewer atmospheric gases while losses to space continued — eventually leading to atmospheric collapse. But rather than collapsing, the atmosphere appears to change on a shorter cyclical pattern.
Applying what they learned from SOFIA to reanalyze previous observations, researchers found that the haze thickens and then fades in a cycle lasting just a few years. This indicates that the tiny particles are being created relatively quickly. The researchers suggest that Pluto’s unusual orbit is driving the changes in the haze and therefore may be more important in regulating its atmosphere than its distance from the Sun.
“There’s still a lot we don’t understand, but we’re forced now to reconsider earlier predictions,” said Person. “Pluto’s atmosphere may collapse more slowly than previously predicted, or perhaps not at all. We have to keep monitoring it to find out.”
Chasing Pluto’s Shadow
SOFIA was uniquely positioned to study Pluto from afar by taking advantage of a rare moment when Pluto passed in front of a distant star, casting a faint shadow across the Earth’s surface. Momentarily backlit by the star, Pluto’s atmosphere could be analyzed.
Traveling at 53,000 miles per hour, Pluto’s shadow was expected to appear for a brief two minutes over the Pacific Ocean near New Zealand. SOFIA charted its course to intercept, but two hours before the occultation an updated prediction placed the shadow 200 miles to the north.
“Capturing that shadow required a bit of scramble. SOFIA has the benefit of being mobile, but the revised flight plan had to be cleared by air traffic control,” said William Reach of Universities Space Research Association and SOFIA’s associate director for science operations. “There were a few tense moments, but the team worked together, and we got clearance. We reached Pluto’s shadow at exactly the right time and were very happy to have made it!”
Remote observations like these allow scientists to monitor planetary bodies in between spacecraft flybys, which can often be separated by many years. Such unique observations gathered remotely by SOFIA and New Horizons’ close flyby confirms that occultation observations from Earth can provide high quality and complementary data between spacecraft observations and flybys.
“Similar complementary capabilities of SOFIA in tandem with other ground-based and space-based astronomical observatories have been demonstrated and will continue to be explored in future,” said Margaret Meixner, USRA’s Director of SOFIA Mission Operations.
Reference:
“Haze in Pluto’s atmosphere: Results from SOFIA and ground-based observations of the 2015 June 29 Pluto occultation,” Michael J. Person et al., 2020, to appear in Icarus [https://doi.org/10.1016/j.icarus.2019.113572].
About USRA:
Founded in 1969, under the auspices of the National Academy of Sciences at the request of the U.S. Government, the Universities Space Research Association (USRA, https://www.usra.edu) is a nonprofit corporation chartered to advance space-related science, technology and engineering. USRA operates scientific institutes and facilities, and conducts other major research and educational programs, under Federal funding. USRA engages the university community and employs in-house scientific leadership, innovative research and development, and project management expertise.
About SOFIA:
SOFIA, the Stratospheric Observatory for Infrared Astronomy, is a Boeing 747SP jetliner modified to carry a 106-inch diameter telescope. It is a joint project of NASA and the German Aerospace Center, DLR. NASA’s Ames Research Center in California’s Silicon Valley manages the SOFIA program, science and mission operations in cooperation with the Universities Space Research Association headquartered in Columbia, Maryland, and the German SOFIA Institute (DSI) at the University of Stuttgart. The aircraft is maintained and operated from NASA’s Armstrong Flight Research Center Building 703, in Palmdale, California.
