Artist David A. Hardy’s view of Pluto and Charon showing the possibility of haze, clouds and even cryovulcanism.
Credit: © David A. Hardy, www.astroart.org
You might guess that a small and distant world almost 40 times farther from the sun than the Earth is from the sun would not have an atmosphere, but in the case of Pluto, you’d be wrong. In fact, Pluto is a complex world, particularly when it comes to weather patterns. Gusty winds, clouds, haze, micro snowflakes and even ice volcanoes — cryovolcanism — could all be part of Pluto’s dynamic weather system. While such observations have come from Earth-based telescopes, many more surprises might be revealed as NASA’s New Horizons spacecraft makes its nearest approach to Pluto on July 14, 2015.
But no matter how you classify it, this icy and remote dwarf planet is an odd little world.
Evidence of Pluto’s atmosphere
Though Pluto was discovered by Clyde Tombaugh in 1930, it wasn’t until 1988 that scientists first detected an atmosphere on the dwarf planet during a stellar occultation. In a stellar occultation, a body such as a planet passes in front of a relatively bright star, and measuring the gradual dimming of starlight during such an event, scientists can amass a wide array of information about a planet, including its size, whether it has rings or if an atmosphere is present. Having theoretically worked out that Pluto should have an atmosphere, scientists set out to find it.
“When the 1988 stellar occultation occurred, scientists were out to detect the atmosphere, which had been expected on theoretical grounds for more than a decade,” Alan Stern, New Horizons principal investigator, said via email.
The June 9, 1988, stellar occultation by Pluto provided the first opportunity for astronomers using telescopes located in Australia, New Zealand, and the Kuiper Airborne Observatory flying over the ocean south of the Samoa islands to detect an atmosphere on the dwarf planet.
If an atmosphere on Pluto were not present, starlight would blink instantly off and then back on again at the end of the occultation. However, for a short time at the start and end of the occultation, Pluto’s atmosphere was backlit by the star, and the starlight dimmed more gradually. By modeling how the atmosphere refracted, or bent, the starlight, researchers detected that Pluto has a thin layer of atmosphere made of gaseous forms of the ices — nitrogen, methane, carbon monoxide and traces of others — that cover its surface.
“The occultation light curve shows a structured decline in intensity rather than a precipitous decline indicative of an atmosphere surrounding Pluto,” said Paul Delaney, a senior lecturer of physics and astronomy at York University in Toronto.
When astronomers graph the light data, a careful look at the gradual dimming of starlight shown in the occultation light curve reveals a “slight bend,” or “kink.” You can also see from the light curve that starlight does not penetrate all the way to Pluto’s surface. Starlight did not reach the surface, suggesting that obscuring clouds and/or haze might mask the surface.
“The symmetry and structure of the occultation light curve is suggestive of an atmosphere with structure, in comparison to the absence of an atmosphere surrounding Pluto,” Delaney noted. Hence, the presence of the same kink on either side of the curve suggests there is an atmosphere engulfing Pluto, he said.
The most recent Pluto occultation opportunity was on June 29, 2015, in the southern hemisphere, just two weeks before New Horizons makes its closest approach to the Pluto system. The only observatory able to position itself directly in the center of Pluto’s shadow, located off of New Zealand, was NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA), a Boeing 747SP jetliner modified to carry a 100-inch-diameter (2.5 meters) telescope.
“SOFIA observations of Pluto demonstrate a capability to make detailed measurements of Pluto’s atmospheric density and structure,” said Pamela Marcum, SOFIA program scientist at NASA’s Ames Research Center. “SOFIA conducted its first occultation observation, also involving Pluto, in July 2011. This flight adds to our understanding of how the atmosphere of Pluto evolves over multiple-year time scales as its elongated orbit takes it farther away from the sun.”
The comparative sizes of the atmospheres of Pluto and Earth.
Credit: Simulation Curriculum, www.PlutoSafari.com
Seasonal changes on Pluto
Once the existence of Pluto’s atmosphere was confirmed, scientists began to investigate how the atmosphere and the surface temperature change during Pluto’s 248-Earth-year journey around the sun. The orbit of Pluto follows a highly elliptical orbit that resembles a squashed circle. In fact, its orbit is so elliptical that during perihelion (its closest point to the sun), Pluto is only about 30 astronomical units (AU) from the sun, bringing it closer to the sun than to its closest neighbor, Neptune.
During aphelion (its farthest point from the sun), Pluto is about 50 AU from the sun. (One AU is about 150 million kilometers (93 million miles), defined as one Earth-sun distance.)
The large 20-AU difference between Pluto’s perihelion and aphelion distance results in interesting chemistry on Pluto’s surface and in its atmosphere. Pluto is a rocky body covered in ice. At perihelion, Pluto’s surface temperature increases to about minus 220 degrees Celsius (minus 364 degrees Fahrenheit), allowing the ice on its surface to sublimate — that is, transition directly from a solid to a gas. The resulting vapors form a layer of atmosphere made of molecular nitrogen (with trace amounts of carbon monoxide and methane).
Scientists originally thought that as Pluto recedes from the sun, and the temperature decreases to about minus 240 C (minus 400 F), the vapors freeze and fall back down to the dwarf planet’s surface. However, observations made as recently as 2013 and coordinated by the Portable High-Speed OccultationTelescope group from multiple sites including the 0.9 m astrograph at Cerro Tololo Inter-American Observatory (CTIO) and the 1 m Liverpool Telescope on the Canary Islands, indicate that Pluto’s atmosphere is not collapsing, but rather thickening.
So, although Pluto’s atmosphere gets thicker and thinner through its orbit of the sun, it may never completely freeze out and “collapse.”
Michael Summers, New Horizons co-investigator and member of the atmospheres science theme team, said it’s too early to tell whether Pluto’s atmosphere freezes out or persists through its orbit. This makes sense, as Pluto has made only one-tenth of an orbit around the sun since the discovery of its atmosphere in 1988.
Summers used a tangible analogy to explain what may be happening — one that we see daily on Earth. “There is a time delay between the highest temperature and the maximum heating. … The maximum heating from the sun during the day is when the sun is directly overhead, at noon,” he explained. “But the highest temperature usually occurs later, around 2 p.m. in the afternoon. The Earth continues to heat up from noon to 2 p.m. That is due to a thermal lag; it takes less time to heat up the atmosphere than it takes for it to cool off.
“I think, for Pluto, it just takes time for it to cool off,” Summers added. “In fact, it may still be heating up, sort of like we are still in the Earth’s, say 1 p.m., time frame for Pluto.”
Another interesting fact about Pluto’s atmosphere is that it evolves quickly. Work by a team led by Jane Greaves, an astrophysics researcher at the University of St. Andrews in Scotland, shows that the carbon monoxide density in Pluto’s atmosphere has increased in just a decade. Additionally, Greaves’ team found carbon monoxide extending out to more than 1,860 miles (3,000 kilometers) from Pluto’s surface. The molecules that reach such extents will likely escape, as solar winds will just carry them out into space.
When New Horizons arrives at the Pluto system, onboard science instruments such as Alice, a sensitive ultraviolet imaging spectrometer, will reveal even more about the composition and structure of the dwarf planet’s dynamic atmosphere. Continued observations of stellar occultations of Pluto will show us whether its atmosphere freezes out. Pluto last reached perihelion in 1989, and it will not reach perihelion again until 2237. Therefore, if its atmosphere does freeze out, scientists won’t observe this until somewhere around the year 2200.
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