Exploring Titan with Balloons and Landers

titan-haze.jpg

Last week - from Monday, February 27th to Wednesday, March 1st - NASA hosted the "

Planetary Science Vision 2050 Workshop

" at their headquarters in Washington, DC. In the course of the many presentations, speeches and panel discussions, NASA's shared its many plans for the future of space exploration with the international community.

Among the more ambitious of these was a proposal to explore

Titan

using an aerial explorer and a lander. Building upon the success of the ESA's

Cassini-Huygen

mission, this plan would involve a balloon that would explore Titan's surface from low altitude, along with a

Mars Pathfinder

-style mission that would explore the surface.

Ultimately, the goal a mission to Titan would be to explore the rich organic chemical environment the moon has, which presents a unique opportunity for planetary researchers. For some time, scientists have understood that Titan's surface and atmosphere have an abundance of organic compounds and all the prebiotic chemistry necessary for life to function.

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Artist depiction of Huygens landing on Titan. Credit: ESA

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The presentation, which was titled "

Aerial Mobility : The Key to Exploring Titan's Rich Chemical Diversity

" was chaired by Ralph Lorenz from the

Johns Hopkins Applied Physics Laboratory

, and co-chaired by Elizabeth Turtle (also from John Hopkins APL) and Jason Barnes from the

Dept. of Physics at the University of Idaho

. As Turtle explained to Universe Today via email, Titan presents some exciting opportunities for a next-generation mission:

For this reason, the exploration of Titan has been a scientific goal for decades. The only question is how best to go about exploring Titan's unique environment. During previous Decadal Surveys - such as the Campaign Strategy Working Group (CSWG) on Prebiotic Chemistry in the Outer Solar System, of which Lorenz was a contributor - has suggested that a mobile aerial vehicle (such as an airship or a balloon) would well-suited to the task.

However, such vehicles would be unable to study Titan's methane lakes, which are one of the most exciting draws of the moon as far as research into prebiotic chemistry goes. What's more, an aerial vehicle would not be able to conduct in-situ chemical analysis of the surface, much like what the

Mars Exploration Rovers

(

Spirit, Opportunity

and

Curiosity)

have been doing on Mars - and with immense results!

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The ESA's TALISE (Titan Lake In-situ Sampling Propelled Explorer) on the left, and NASA's Titan Mare Explorer (TiME) on the right. Credit: bisbos.com

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At the same time, Lorenz and his colleagues examined concepts for the exploration of Titan's hydrocarbon seas - like the proposed

Titan Mare Explorer

(TiME) capsule. As one of several finalists of NASA's 2010 Discovery competition, this concept called for the deployment of nautical robot to Titan in the coming decades, where it would study its methane lakes to learn more about the methane cycle and search for signs of organic life.

While such a proposal would be cost-effective and presents some very exciting opportunities for research, it also has some limitations. For instance, during the 2020s-2030s, Titan's northern hemisphere will be experiencing its winter season; at which point the thickness of its atmosphere will make direct-to-Earth communications and Earth views impossible. On top of that, a nautical vehicle would preclude the exploration of Titan's land surfaces.

These offer some of the most likely prospects for studying Titan's advanced chemical evolution, including Titan's dune sands. As a windswept region, this area likely has material deposited from all over Titan and may also contain aqueously altered materials. Much as the

Mars Pathfinder

landing site was selected so it could collect samples from a wide area, such as location would be an ideal site for a lander.

As such, Lorenz and his colleagues advocated the type of mission that was articulated in the

2007 Flagship Study

, which called for a Montgolfière balloon for regional exploration and a Pathfinder-like lander. This would provide the opportunity to conduct surface imaging at resolutions that are impossible from orbit (due to the thick atmosphere) as well as investigating the surface chemistry and interior structure of the moon.

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Artist's conception of a possible structure for underground liquid reservoirs on Saturn moon's Titan. Credit: ESA/ATG medialab[/caption]

So while the balloon would gather high-resolution geographical data of the moon, the lander could conduct seismological surveys that would characterize the thickness of the ice above Titan's internal water ocean. However, a lander mission would be limited in terms of range, and the surface of Titan presents problems for mobility. This would make multiple landers, or a relocatable lander, the most desired option.

"Potential targets include areas where we can measure solid surface materials, the composition of which is still not well known, Titan's dune sands, for example," said Turtle. "Detailed in situ analysis is required to determine their composition. The lakes and seas are also intriguing; however, in the nearer term (missions arriving in the 2030s) most of those will be in winter darkness. So, exploring them would likely have to wait until the 2040s."

This mission concept would also take advantage of several technological advances that have been made in recent years. As Lorenz explained in the course of the presentation:

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Updated maps of Titan, based on the Cassini imaging science subsystem. Credit: NASA/JPL/Space Science Institute

[/caption]

Lorenz, Turtle and Barnes will also be presenting these findings at the upcoming

48th Lunar and Planetary Science Conference

  • which will be taking place from March 20th to 24th in The Woodlands, Texas. There they will be joined by additional members of the Johns Hopkins APL and the University of Idaho, as well as panelists from NASA's

Goddard Space Flight Center

,

Pennsylvania State University

, and

Honeybee Robotics

.

However, addressing some additional challenges not raised at the 2050 Vision Workshop, they will be presenting a slight twist on their idea. Instead of a balloon and multiple landers, they will present a mission concept involving a "Dragonfly" qaudcopter. This four-rotor vehicle would be able to take advantage of Titan's thick atmosphere and low gravity to obtain samples and determine the surface composition in multiple geological settings.

This concept also incorporates a lot of recent advances in technology, which include modern control electronics and advances in commerical unmanned aerial vehicle (UAV) designs. On top of that, a quadcopter would do away with chemically-powered retrorockets and could power-up between flights, giving it a potentially much longer lifespan.

These and other concepts for exploring Saturn's moon Titan are sure to gain traction in the coming years. Given the many mysteries locked away on this world - with includes abundant water ice, prebiotic chemistry, a methane cycle, and a subsurface ocean that is likely to be a prebiotic environment - it is certainly a popular target for scientific research.

Further Reading: USRA

,

USRA (2)

,

USRA (3)

Matthew Williams

Matthew Williams

Matt Williams is a space journalist, science communicator, and author with several published titles and studies. His work is featured in The Ross 248 Project and Interstellar Travel edited by NASA alumni Les Johnson and Ken Roy. He also hosts the podcast series Stories from Space at ITSP Magazine. He lives in beautiful British Columbia with his wife and family. For more information, check out his website.