Open research questions in Planetary Science and Exploration
217 unresolved questions extracted from the limitations and future-work sections of 1,760 Planetary Science and Exploration papers in our library. Each links back to the study that raised it.
What the literature leaves open
further evaluation of the TPMs using additional data sources, - investigation of the effects of surface roughness on the thermal infrared signal, - development of more accurate thermophysical models of the lunar surface
Vicarious Calibration of Thermal Infrared Imagers Using Thermophysical Models of the Lunar Surface · 2026 · DOILack of robust calibration and validation methodologies at high brightness temperatures. Uncertainties in surface properties, particularly in the mid-wave infrared. Need for a stable and widely available reference target for vicarious calibration.
Vicarious Calibration of Thermal Infrared Imagers Using Thermophysical Models of the Lunar Surface · 2026 · DOIThe origin and alteration history of the Margin unit are not well understood. The potential for preserving biosignatures in the Margin unit is of great interest but requires further research.
Lake- and groundwater-associated alteration of the olivine-rich Margin unit in Jezero crater, Mars · 2026 · DOIThe mid-to-late-stage evolution of the lunar magnetic field is poorly constrained, and thus, the existence of a long-lived lunar dynamo remains controversial.
The origin of these molecules remains uncertain, as they could be derived from either abiotic or biological sources.
However, the ocean hypothesis remains controversial due to the lack of conclusive evidence from the Martian subsurface.
However, the ability to detect all possible craters under different lighting and camera geometries has not been systematically studied except in a few limited cases.
Crater Detection Dependence on Resolution, Incidence Angle, Emission Angle, and Phase Angle · 2025 · DOIThis study explores an underexplored process: the role of seasonal frost in brine formation.
However, the extent to which both the current and primitive geodynamo influence the transport of terrestrial ions still remains unclear, and this uncertainty is further complicated by the enigmatic composition and poorly constrained location of the Eoarchean exosphere.
Terrestrial atmospheric ion implantation occurred in the nearside lunar regolith during the history of Earth’s dynamo · 2025 · DOIHowever, the precision of existing geochronology is insufficient to determine whether this peak represents a brief event or a more protracted period of magmatism occurring over tens of millions of years.
High-precision U-Pb zircon dating identifies a major magmatic event on the Moon at 4.338 Ga · 2024 · DOIThe existence of molecular H 2 O and evolution of solar wind–derived water on the lunar surface remain controversial.
Abstract Although a low temperature limit for life has not been established, it is thought that there exists a physical limit imposed by the onset of intracellular vitrification, typically occurring at ~−20 °C for unicellular organisms.
Preservation of Bacillus subtilis’ cellular liquid state at deep sub-zero temperatures in perchlorate brines · 2024 · DOIAlthough we understand how helium is delivered to the Moon, certain aspects of helium concentration processes on the surface remain unknown, such as why impact-generated glass aggregates contain more helium than equally sized soil grains of other types.
The sublimation of CO2 has been proposed as an alternative driver for sediment transport, but how this mechanism works remains unknown.
How, when and where current mass flows in Martian gullies are driven by CO2 sublimation · 2024 · DOIFuture research should focus on investigating the effects of impact events on the environment and the biosphere. The study of impactites and shock-metamorphic features should continue to provide reliable evidence of impact origin.
The paper identifies a gap in our understanding of the global inventory and uneven distribution of confirmed terrestrial impact structures. The study highlights the need to consider the potential effects of impact events on the environment and the biosphere.
Limited spatial resolution and fine-scale regolith heterogeneity produce mixed pixels with spectra that combine multiple materials. Nonlinear scattering effects and limited ground truth pose major challenges for hyperspectral unmixing of lunar intimate mixtures.
Craters of varying sizes and morphological characteristics. Limited performance of traditional computer vision methods. Inadequate ability of some deep learning models to identify large craters.
The performance of the CNN model is limited for large craters. The ResNet-50 model has inadequate ability to identify large craters. The dataset used is from NASA's publicly accessible archives, which may have limitations.
Future research should focus on further exploring the lunar interior and the formation of the low-viscosity zone. The development of new technologies for exploring the lunar interior is needed.
The ill-posed problem of monocular terrain reconstruction, characterized by solution ambiguity and ill-posedness. The inherent ambiguity in the physical imaging process, where the observed pixel intensity stems from the tightly coupled effects of intrinsic surface reflectance and illumination geometry. The lack of ground-truth Martian surface albedo data at HiRISE resolution.
PFMGAN: A Generative Adversarial Network with Physics Fusion for DTM Generation from Martian Monocular Images · 2026 · DOIThe simplified Lambertian model is insufficient to accurately capture the complex optical phenomena on the Martian surface, - Conventional deep learning approaches often struggle to derive robust solutions amidst inherent ambiguity, - The lack of ground-truth Martian surface albedo data at HiRISE resolution
PFMGAN: A Generative Adversarial Network with Physics Fusion for DTM Generation from Martian Monocular Images · 2026 · DOIThe duration and dynamic evolution of surface water on Mars are key to understanding its past habitability, but remain poorly constrained. Prior work has preserved mineralogical signatures of ancient aqueous activity, but these remain chronologically unconstrained.
Manganese (Hydr)oxides record the dynamic evolution of a million-year Hesperian Ocean in Utopia Planitia, Mars · 2026 · DOIFuture research should focus on the in-flight calibration of HVM^3 - Future research should investigate the use of HVM^3 to map water ice or other volatiles within most of the Moon's Permanently Shadowed Regions
Calibration and Performance of the High Resolution Volatiles and Minerals Moon Mapper (HVM 3 ) on Lunar Trailblazer · 2026 · DOIThere is a need to understand the form, abundance, and distribution of water on the lunar surface - There is a need to measure the distinct absorptions of water ice, adsorbed O, and OH/hydroxl
Calibration and Performance of the High Resolution Volatiles and Minerals Moon Mapper (HVM 3 ) on Lunar Trailblazer · 2026 · DOI
Most-cited papers in Planetary Science and Exploration
- Organic molecules in the Sheepbed Mudstone, Gale Crater, Mars · Journal of Geophysical Research Planets · 2015 · 439 citations
- Revised CRISM spectral parameters and summary products based on the currently detected mineral diversity on Mars · Journal of Geophysical Research Planets · 2014 · 409 citations
- Global Regolith Thermophysical Properties of the Moon From the Diviner Lunar Radiometer Experiment · Journal of Geophysical Research Planets · 2017 · 361 citations
- Albert Einstein – Science et Religion · Synthesis philosophica · 2006 · 306 citations
- Assessing the mineralogy of the watershed and fan deposits of the Jezero crater paleolake system, Mars · Journal of Geophysical Research Planets · 2015 · 285 citations
- Calcium sulfate veins characterized by ChemCam/Curiosity at Gale crater, Mars · Journal of Geophysical Research Planets · 2014 · 265 citations
- Structure, dynamics, and seasonal variability of the Mars‐solar wind interaction: MAVEN Solar Wind Ion Analyzer in‐flight performance and science results · Journal of Geophysical Research Space Physics · 2016 · 262 citations
- Mars Global Ionosphere‐Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere · Journal of Geophysical Research Planets · 2014 · 251 citations
- Asymmetric thermal evolution of the Moon · Journal of Geophysical Research Planets · 2013 · 249 citations
- Evolved gas analyses of sedimentary rocks and eolian sediment in Gale Crater, Mars: Results of the Curiosity rover's sample analysis at Mars instrument from Yellowknife Bay to the Namib Dune · Journal of Geophysical Research Planets · 2017 · 234 citations
Most recent work
- Life Detection in the Martian Subsurface: Advancements in Microbial Metabolic Research Under Mars Laboratory and Field-Analog Conditions since Viking · Astrobiology · 2026
- The Lunar Trailblazer Lunar Thermal Mapper Instrument · Journal of Geophysical Research Planets · 2026
- Calibration and Performance of the High Resolution Volatiles and Minerals Moon Mapper (HVM 3 ) on Lunar Trailblazer · Earth and Space Science · 2026
- A Fluvio‐Lacustrine Environment Preserved in the Jezero Crater Inlet Channel, Neretva Vallis, Mars · Journal of Geophysical Research Planets · 2026
- Heating of the Martian Upper Atmosphere by the Dissipation of Acoustic‐Gravity Waves · Journal of Geophysical Research Planets · 2026
- In Situ Carbonation of Sedimentary and Igneous Rocks of Ultramafic Composition in Jezero Crater, Mars · Journal of Geophysical Research Planets · 2026
- Revealing Space Weathering of the Moon Farside via Soft X-ray Emission Spectroscopy · The Journal of Physical Chemistry Letters · 2026
- A native sulfur deposit in Gale crater, Mars · Science · 2026
- Formation and Alteration of Olivine‐Carbonate Rocks Within Jezero Crater as Constrained by In Situ Visible/Near‐Infrared Multispectral Images · Journal of Geophysical Research Planets · 2026
- Describing the Global Gravity Field of Mars With Lithospheric Flexure and Deep Mantle Flow · Journal of Geophysical Research Planets · 2026
Find a gap in your own Planetary Science and Exploration sub-topic
This page shows what the Planetary Science and Exploration literature already flags as unresolved. To narrow it to your specific question, search the Research Gap Finder: the search is free with a free account and lists the papers closest to your topic first. Unlocking that topic (50 credits, charged once) fills the comparison table from our 4.5M-paper local library and writes the gaps from its rows.
Open the Research Gap Finder →