Melissa G. Trainer’s research while affiliated with Johnson Space Center and other places

What is this page?


This page lists works of an author who doesn't have a ResearchGate profile or hasn't added the works to their profile yet. It is automatically generated from public (personal) data to further our legitimate goal of comprehensive and accurate scientific recordkeeping. If you are this author and want this page removed, please let us know.

Publications (28)


Science Autonomy using Machine Learning for Astrobiology
  • Preprint

April 2025

·

16 Reads

·

Bethany Theiling

·

Eric Lyness

·

[...]

·

Caroline Freissinet

In recent decades, artificial intelligence (AI) including machine learning (ML) have become vital for space missions enabling rapid data processing, advanced pattern recognition, and enhanced insight extraction. These tools are especially valuable in astrobiology applications, where models must distinguish biotic patterns from complex abiotic backgrounds. Advancing the integration of autonomy through AI and ML into space missions is a complex challenge, and we believe that by focusing on key areas, we can make significant progress and offer practical recommendations for tackling these obstacles.


Laboratory Studies on the Influence of Hydrogen on Titan-like Photochemistry
  • Article
  • Full-text available

December 2024

·

24 Reads

·

1 Citation

ACS Earth and Space Chemistry

Laboratory investigations of photochemical reactions in simulated Titan-like atmospheric systems provide insight into the formation of gas and aerosol products and the influence of different environmental parameters on the types of organic molecules generated. Studying the gas-phase products as a function of reaction time provides further insight into the reaction pathways that lead to organic production. The stable isotopes in the reactants and products serve as tracers and help to disentangle these reaction pathways. We report a time study on the chemical composition and relative abundance of the evolved gas-phase products formed by far-ultraviolet reactions between 5% CH4 and N2 in a closed system. Two experimental setups are used, where one fully removes hydrogen from the experimental system using a palladium membrane (hydrogen-poor experiments) and the other does not remove hydrogen during the experiment (hydrogen-rich experiments). Carbon isotope values (δ¹³C) of CH4, C2H6, and C3H8 are also reported and are used, along with the gas-phase composition and relative abundance measurements, to constrain the chemical reactions occurring during our experiments. The gas-phase products C2H6, C3H8, n-C4H10, iso-C4H10, n-C5H12, iso-C5H12, C2H2, C2H4, HCN, and CH3CN were detected, with some variations between both sets of experiments. The hydrogen-poor experiments highlight the importance of hydrogen in the formation of HCN, n-C5H12, iso-C5H12, and CH3CN. By monitoring the chemical composition and the carbon isotopic ratios of the gas phase during CH4/N2 photochemistry, especially under a hydrogen-poor and hydrogen-rich environment, the photochemical reaction pathways and the influence of hydrogen on these pathways in a Titan-like atmosphere can be better understood.

Download





FIGURE 1 | A variety of miniaturized mass analyzers that have been flown and will fly on planetary missions. (A) A magnetic sector MS was carried on the Viking landers. (B) A quadrupole MS was carried on board the Curiosity rover. (C) A time-of-flight MS was flown on the Rosetta/Philae lander (as part of the COSAC instrument suite). (D) An ion trap MS as part of the MOMA instrument suite will be flown on board the Rosalind Franklin rover. Reprinted with permission from Levin et al. (2000) and from Dr. Fred Goesmann.
FIGURE 2 | (A) Figurative biomarker tree of Terran life representing the diversity of chemical biosignatures detectable via mass spectrometry. (B) Figurative biomarker tree of exotic life representing our lack of knowledge on the biochemical ancestry and thus potential chemical biosignatures of exotic life.
FIGURE 3 | Possible agnostic biosignatures detectable using mass spectrometry. (A) Molecular assembly measurements of a molecule, correlated to the number of fragments in its mass spectra. (B) The uniform distribution of compounds found in non-life versus the discrete distribution of compounds found in life, potentially the result of the Lego principle. Adapted from McKay (2008).
FIGURE 4 | The miniaturized Orbitrap mass analyzer of the Characterization of Ocean Residues And Life Signatures (CORALS) instrument, one of the next generation mass spectrometers currently being developed for spaceflight. Adapted from Willhite et al. (2021).
Planetary Mass Spectrometry for Agnostic Life Detection in the Solar System

October 2021

·

550 Reads

·

39 Citations

Frontiers in Astronomy and Space Sciences

For the past fifty years of space exploration, mass spectrometry has provided unique chemical and physical insights on the characteristics of other planetary bodies in the Solar System. A variety of mass spectrometer types, including magnetic sector, quadrupole, time-of-flight, and ion trap, have and will continue to deepen our understanding of the formation and evolution of exploration targets like the surfaces and atmospheres of planets and their moons. An important impetus for the continuing exploration of Mars, Europa, Enceladus, Titan, and Venus involves assessing the habitability of solar system bodies and, ultimately, the search for life—a monumental effort that can be advanced by mass spectrometry. Modern flight-capable mass spectrometers, in combination with various sample processing, separation, and ionization techniques enable sensitive detection of chemical biosignatures. While our canonical knowledge of biosignatures is rooted in Terran-based examples, agnostic approaches in astrobiology can cast a wider net, to search for signs of life that may not be based on Terran-like biochemistry. Here, we delve into the search for extraterrestrial chemical and morphological biosignatures and examine several possible approaches to agnostic life detection using mass spectrometry. We discuss how future missions can help ensure that our search strategies are inclusive of unfamiliar life forms.


Science Autonomy and the ExoMars Mission: Machine Learning to Help Find Life on Mars

October 2021

·

42 Reads

·

6 Citations

Computer

We use Mars Organic Molecule Analyzer engineering model data to develop mass-spectrometry-focused machine learning techniques. Initial results show that the preliminary categorization could permit autonomous operations, such as prioritizing example data and decisions about retuning parameters for specific samples.


Science Goals and Objectives for the Dragonfly Titan Rotorcraft Relocatable Lander

July 2021

·

657 Reads

·

162 Citations

The Planetary Science Journal

NASA’s Dragonfly mission will send a rotorcraft lander to the surface of Titan in the mid-2030s. Dragonfly's science themes include investigation of Titan’s prebiotic chemistry, habitability, and potential chemical biosignatures from both water-based “life as we know it” (as might occur in the interior mantle ocean, potential cryovolcanic flows, and/or impact melt deposits) and potential “life, but not as we know it” that might use liquid hydrocarbons as a solvent (within Titan’s lakes, seas, and/or aquifers). Consideration of both of these solvents simultaneously led to our initial landing site in Titan’s equatorial dunes and interdunes to sample organic sediments and water ice, respectively. Ultimately, Dragonfly's traverse target is the 80 km diameter Selk Crater, at 7° N, where we seek previously liquid water that has mixed with surface organics. Our science goals include determining how far prebiotic chemistry has progressed on Titan and what molecules and elements might be available for such chemistry. We will also determine the role of Titan’s tropical deserts in the global methane cycle. We will investigate the processes and processing rates that modify Titan’s surface geology and constrain how and where organics and liquid water can mix on and within Titan. Importantly, we will search for chemical biosignatures indicative of past or extant biological processes. As such, Dragonfly, along with Perseverance, is the first NASA mission to explicitly incorporate the search for signs of life into its mission goals since the Viking landers in 1976.



Citations (15)


... However, various space agencies have been investing in technologies for detecting molecules in situ, known as bio-signatures 47 . Advances in mass spectrometry applied to space exploration actively contribute to the development of more robust equipment in terms of sensitivity, resolution, and the ability to analyze molecules of different sizes, making the use of complex organic molecules as bio-signatures a powerful tool for detecting evidence of extraterrestrial life 48,49 . The search for complex molecules as evidence of life beyond Earth turns out to be a very promising approach, as many of these molecules are produced exclusively by biotic processes, such as long-chain unsaturated lipids, polypeptides, and other molecules resulting from secondary metabolism 47 . ...

Reference:

Survival strategies of Rhinocladiella similis in perchlorate-rich Mars like environments
Planetary Mass Spectrometry for Agnostic Life Detection in the Solar System

Frontiers in Astronomy and Space Sciences

... In addition, samples measured by the Pyr-GC-MS instruments on the Mars Viking lander and the Curiosity rover (34, 43, 52) deserve new evaluation. While our method must first be calibrated to the specific thermal ramping and maximum temperature conditions of those instruments, these and other machine-learning methods hold promise for the evaluation of the biogenicity of samples of extraterrestrial provenance before they are returned to Earth (53). Of special interest in this regard is the possible role of environmental chemicals, such as perchlorate on Mars (54), as well as radiationaltered molecular suites (55), which might significantly influence the properties of the resulting molecular mixtures. ...

Science Autonomy and the ExoMars Mission: Machine Learning to Help Find Life on Mars
  • Citing Article
  • October 2021

Computer

... Understanding the interaction and alteration of organics on these icy worlds is a key scientific objective in both NASA's and ESA's space exploration programs, presenting a unique combination of organic molecules and ice in a radiation environment. The Saturn's moon Titan will be explored by the NASA's Dragonfly mission (Barnes et al. 2021), set to sample the moon's atmosphere and surface composition at different landing sites to assess Titan's potentially prebiotic organic chemistry. While the interpretation of spectroscopic data from the JUNO mission (Bolton et al. 2017) revealed the presence of organics on the surface of Ganymede ), NASA's Europa Clipper (Pappalardo et al. 2024) and ESA's Jupiter Icy Moons Explorer (JUICE, Grasset et al. 2013) are scheduled to reach the Jovian system in 2030 and 2031, respectively, with Europa, Ganymede, and Callisto as their primary targets. ...

Science Goals and Objectives for the Dragonfly Titan Rotorcraft Relocatable Lander

The Planetary Science Journal

... Payload masses for small flyby, probe, and orbital missions are reported in Table 1. Orbiter missions 68 to characterize ionosphere 9,19 plasma 57 and magnetic structure, continue studies of igneous rock geology with remote sensing 63 , improve geodesy 61 , determine trace gas flux and variation 28 , probe the stratigraphy of the upper 10-m subsurface in the mid-latitude ice regions 13,60 , perform global atmospheric observations 50 22 for in-situ measurements of isotopic ratios 43 or to determine the habitability of the cloud layer 42 . Payload masses beyond those reported in Table 1 are enabled through small spacecraft aerocapture 4 capabilities. ...

Mars Trace Gas Fluxes: Critical Strategies and Implications for the Upcoming Decade

... The Mars Organic Molecule Analyzer (MOMA) is a dualsource (laser desorption and gas chromatography) massspectrometer that will launch onboard the European Space Agency's ExoMars rover in 2022 to analyze soil samples for signs of past or current life on the surface or subsurface of Mars [49], [50]. However, low bandwidth and high time of interplanetary data transfer will limit the downlink of all raw MOMA-collected data to Earth [50]. ...

Science Autonomy and the ExoMars Mission: Machine Learning to Help Find Life on Mars
  • Citing Conference Paper
  • January 2020

... Finally, these data point towards the idea that similar atmospheric effects exist and could be measured on other planetary bodies with dense atmospheres. For example, if a scintillator detector such as CsI, CLYC, or CeBr 3 were flown on a landed mission to Venus or Titan [27,28], and if the sensors were turned on during descent, these instruments would measure a count-rate profile similar to those reported here for Earth-based measurements. Since the atmospheric altitude of the RP maximum is dependent on atmospheric density, the operation of such an instrument during descent could provide a measure of atmospheric density by just measuring the altitude location of the RP maximum. ...

DRAGONFLY: A ROTORCRAFT-LANDER TO EXPLORE TITAN'S PREBIOTIC CHEMISTRY AND HABITABILITY
  • Citing Conference Paper
  • January 2018

... The Ingenuity Mars Helicopter was the first aircraft to fly on another world with a total of 72 flights over its 1.5 year mission, Ref. [1]. The New Frontiers Dragonfly lander is now under development as the next rotorcraft to be launched from Earth and will explore Saturn's largest moon Titan, Ref. [2]. Such rotorcraft explorers enable 2 science campaigns to be conducted across geographically diverse regions and in locations that rovers cannot easily access. ...

Dragonfly: A rotorcraft lander concept for scientific exploration at titan

... Transient liquid water environments are expected to persist in cryovolcanic flows and impact melt pools 5 (Figure 1) 6,7 for hundreds to possibly tens of thousands of years prior to refreezing. 8−11 Numerous impact craters and several candidate cryovolcanic features have been identified on Titan's surface by the Cassini spacecraft 7,12−15 ( Figure 1); thus, transient surface melts of predominately liquid water have existed on Titan in the past and will occur again. ...

Strategies for Detecting Biological Molecules on Titan
  • Citing Article
  • May 2018

Astrobiology

... MGS-1 was based on the chemical and mineralogical composition of Rocknest (RN) soil in the Gale crater on Mars that was extensively analyzed by the Curiosity rover [9]. Bish et al. [10] considered that based on Alpha Particle X-ray Spectrometer (APXS) chemical analyses, the RN aeolian bedform is representative of global basaltic soil at Gale Crater [5][6][7] and typical of Martian soils [9][10][11]. ...

X-ray Diffraction Results from Mars Science Laboratory: Mineralogy of Rocknest at Gale Crater
  • Citing Article
  • September 2013

... The CB sample used in the OD experiment was drilled in the Sheepbed mudstone on Sol 279 of the mission, and a fresh triple portion (~135 ± 31 mg) was added on top of a previously pyrolyzed CB single portion sample (3,40). This fresh triple portion sample was left inside SAM for about 1,260 sols and accumulated MTBSTFA vapor present in the SMS during the traverse from Yellowknife Bay to the base of Mt. ...

Volatile and Organic Compositions of Sedimentary Rocks in Yellowknife Bay, Gale Crater, Mars.
  • Citing Article
  • January 2013