Title: Enabling Ice Core Science on Mars and Ocean Worlds
Authors: Alexander G. Chipps, Cassius B. Tunis, Nathan Chellman, Joseph R. McConnell, Bruce Hammer, Christopher E. Carr
First Author’s Institution: School of Mechanical Engineering, Georgia Institute of Technology, Atlanta, Georgia
Status: Available on arXiv
One of my favorite episodes of The X-Files is “Ice,” from the show’s first season. Our intrepid protagonists, Special Agents Fox Mulder and Dana Scully, have been summoned to a remote Alaskan research station, where a group of geophysicists analyzing ice cores sent out a distress call. The pair eventually discovers that the scientists had accidentally released alien parasites: worms embedded in the ice by a meteorite impact a quarter million years before.
Even though it’s fantastical, the episode gets a few things right. First, ice cores really do act as excellent records of Earth’s past, encoding climate variations and, yes, traces from some celestial events. Second, they do sometimes preserve the remains of simple organisms (though not necessarily parasitic worms!). Both of these facts make them exciting tools for studying not just Earth, but other bodies with known ice deposits and the potential to have hosted life, like Enceladus and Europa. Closer to home for humans is Mars, whose own ice reserves formed the basis of a pivotal Doctor Who episode not unlike “Ice.”
Today’s article is a white paper outlining the design of an instrument to aid in the analysis of Martian ice cores.The Melter-Sublimator for Ice Science, or MSIS, methodically melts and sublimate ice samples. With humans likely to visit the Red Planet in the coming decades, exploring ice-rich areas like its South Pole, now seems an excellent time to test out the MSIS. Let’s dive into how it works!
An ice scan in a box
MSIS is a compact object, less than 4 inches across and less than 9 inches high. Shown in Figure 1, it consists of two separate components, the Melter on top and the Sublimator beneath it. When combined, they allow the controlled initial processing of an ice core or smaller ice fragments, turning a sample ice into either vapor or meltwater, after which specialized tools could be used to perform a detailed analysis, perhaps searching for concentrations of isotopes or the signatures of microorganisms.
The Melter, centered around a heating plate and meltwater disposal pipe, allows the MSIS operator to carefully melt an ice core from the inside out, separating the sample into three distinct layers. This is important because the exterior of a core is most prone to contamination, whereas the center is the most pristine. The outermost layer, comprising ~70% of the core by volume, would ideally be discarded, with the inner two layers (10% and 20%) used for compositional analyses requiring different levels of purity.
The Sublimator allows the operator to pre-concentrate samples containing organic materials or other compounds of interest, followed by precision melting of the small sample remaining. This would be quite useful for a mission involving sample return to Earth, a goal that has long been in the works for rock and soil samples excavated by the Perseverance rover.
One sticking point for MSIS operations is that its current design requires a human to operate it. An astronaut is required to gather an ice core, load it into the device, choose the proper settings, clean MSIS, and, in sublimation mode, judge when adequate processing has been completed. Some of these tasks could be automated and potentially integrated into a robotic rover system, but this would require more testing and work.
The waters of Mars
What information could be locked in hundred-million-year-old ice cores? The MSIS designers envision three main areas of interest which could be aided by its preprocessing:
- Volcanism. While Mars currently experiences no volcanic activity, its surface has extensive lava fields and the famous but inactive Olympus Mons. Previous eruptions across the planet would have spewed out sulfur dioxide, which would have oxidized and absorbed by the water that later froze into ice.
- Climate. For approximately 3 billion years, Mars has experienced a cold, dry period known as the Amazonian. Nonetheless, scientists expect that there were miscellaneous variations in climate over that time, which would be reflected in ice deposits. Polar deposits might stretch back only a few million years but could be close to contiguous, whereas ice at lower latitudes might be piecemeal but could stretch back farther into the Amazonian.
- Life. Life on Mars has long been a trope of science fiction – just ask any Doctor over the last half century. Scientifically speaking, though, it’s quite possible that the Red Planet once sustained life. If Martian microorganisms ever existed, subsurface ice deposits could preserve their remains or the organics associated with them.
These are just a few of the compelling reasons to explore Mars, and with plenty of missions to the planet in progress or on the horizon, MSIS has the potential to be quite useful. Adding increased autonomy to the device would give it increased flexibility and the capacity to operate autonomously, a valuable option for uncrewed missions. The design has already undergone successful laboratory tests on artificial ice cores; the next step would be tests on cores from Antarctica or Greenland.
Just not, ideally, from a certain fictional Alaskan research station.
Astrobite edited by: Sasha Warren
Featured image credit: ESA/K. Oldenburg
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