Autonomous Navigation for Rovers
A significant challenge in deploying advanced robotics beyond Earth is the need for accurate traversal of unfamiliar terrain––Figure 4 shows the Perseverance rover and Ingenuity Helicopter currently deployed on Mars. Traditionally, this is achieved using human-in-the-loop (HITL) systems, where operators on Earth provide instructions or feedback. However, as the distance increases, communication delays become more pronounced. Even with radio waves––photons traveling at the speed of light, it can take up to 24 minutes for a signal to make a round trip between Earth and Mars. While this delay is negligible on Earth, it poses critical challenges on Mars. Space environments present numerous unique challenges that vary depending on the technology, location, and method of deployment. Key concerns include communication delays, the lack of a magnetic sphere, hazardous terrain––rocks, regolith, and cliffs––and lower gravity levels, all of which impact system performance. For example, unexpected changes in Martian wind conditions or terrain could render preloaded instructions ineffective. This requires the development of autonomous systems capable of real-time decision-making, such as smart navigation systems. This is where Artificial Intelligence methodologies come into play.
Figure 1
Perseverance and Ingenuity
Note. This image shows the remains of an ancient delta in Mars’ Jezero Crater, which NASA’s Perseverance Mars rover will explore for signs of fossilized microbial life (left) and This view of NASA’s Ingenuity Mars Helicopter was generated using data collected by the Mastcam-Z instrument aboard the agency’s Perseverance Mars rover. NASA/JPL-Caltech/ASU/MSSS (right) [53, 54].
Geography and surface features
Since early observations of Mars in the 1500s, astronomers have often interpreted the planet's terrain through the lens of their own biases and limitations. Using rudimentary telescopes, they created maps based on what they believed they saw through their lenses. However, these depictions were far from accurate. For instance, astronomers were unaware of the massive, planet-wide dust storms that regularly engulf Mars, obscuring its surface. Additionally, some mistakenly interpreted surface features as artificial canals, leading to further misconceptions about the planet's geography. It wasn’t until the 1960s and 1970s, with missions like Mariner 4, Mariner 9, and subsequent orbiters, that humanity obtained its first true images of Mars' surface, revealing its actual terrain.
Figure 2
Earth-Mars Comparison
Note. Earth-Mars Comparison: This composite image, from NASA Galileo and Mars Global Survey orbiters, of Earth and Mars was created to allow viewers to gain a better understanding of the relative sizes of the two planets. JPL [49].
Table 1
Earth-Mars Comparison
Note. A comparison between Earth and Mars. Key feature difference. Retrieved from NASA [64].
Physiology of Mars
Atmospheric conditions, temperature variations, and radiation exposure
It’s important to consider the differences between Earth and Mars––shown in Figure 2 and Table 1 despite both being rocky planets with some similarities, Mars’ atmospheric pressure is significantly lower than Earth’s, and its gravity is about 37% that of Earth. Combined with Mars’ thinner atmosphere and lack of a magnetic field, these differences pose significant challenges for deploying technologies. For instance, variations in atmospheric pressure affect the boiling and freezing points of substances, which has implications for managing resources and systems. Why does this matter? Considering the laws of thermodynamics, when a Neural Network is in its training phase, moving electrons through transistors generates heat. This occurs as particles release energy while transitioning from a lower to a higher entropy state. The more computational resources required, the more heat is generated––an issue intensified by Mars’ environmental constraints.
Lack of magnetic sphere
Earth protects us and our technology by shielding against harmful radiation, thanks to its active magnetic field, known as the magnetosphere. This magnetic field extends outward into space, forming a protective layer that deflects charged particles from the Sun and cosmic rays. Satellites in Low Earth Orbit (LEO) are positioned relatively close to Earth and benefit from this protection, but technologies deployed beyond Earth face harsher conditions. However, satellites at specific Lagrange points––positions in space where the gravitational forces of two large bodies (like Earth and the Sun) balance with the centrifugal force of a smaller object––may be less protected by the magnetosphere depending on their location. These satellites are crucial for modern communications but are still less exposed to radiation compared to technologies operating further away from Earth. Mars, by contrast, lacks a thick atmosphere and a magnetic field, leaving its surface exposed to high-energy particles, including photons, which can damage components. When designing technologies for deep space missions, engineers must account for the increased exposure to harmful radiation. This requires the use of radiation hardening, a process of designing and testing components to withstand the intense radiation environments encountered outside of Earth's protective magnetic field.
Figure 3
Jezero Crater
Note. This image shows the remains of an ancient delta in Mars’ Jezero Crater, which NASA’s Perseverance Mars rover will explore for signs of fossilized microbial life [55].
Mars’ extreme environment––shown in Figure 3––also presents other challenges, such as severe cold. For example, Curiosity tested dry lubricants to endure the cold, but they failed to meet durability requirements during rigorous testing. These conditions require advanced engineering solutions, such as the radiation hardening mentioned earlier, to ensure components can withstand both radiation and extreme temperatures, enabling long-term functionality in deep space. Understanding these challenges is essential for ensuring the longevity and functionality of space-based technologies.
Durability of hardware in extreme Martian conditions (Radiation Hardening)
Radiation hardening is a rigorous and time-intensive process. As a result, space missions often rely on older, proven components that have a track record of reliability in extreme conditions. However, this can lead to limitations, such as using older chips with far less computational power than modern consumer devices. For instance, your current smartphone likely has more processing power than the computers used to send the first manned mission to the Moon. In 1965, Gordon Moore predicted that the number of transistors on a chip would double every 10 years, revising it in 1975 to every 18-24 months––this became known as Moore’s Law. It has driven semiconductor advancements, but as transistors shrink below a certain threshold––there’s uncertainty around the actual size, they approach what’s known as the fuzzy quantum limit. At this scale, quantum effects such as electron tunneling and uncertainty disrupt the traditional flow of electrons through transistors, making further miniaturization impractical. Quantum computing seeks to overcome these limitations by leveraging quantum phenomena such as superposition and entanglement. However, returning to radiation-hardened components, their inherent limitations often mean they lack the advanced computational power necessary to run modern AI techniques on the Martian terrain.
Power consumption in AI systems
A critical consideration for AI systems in space is power consumption, an often-overlooked challenge that becomes crucial outside of Earth. On Earth, we have the luxury of scaling up compute power, resources, and energy as needed. On Mars, however, energy sources are limited solar and nuclear options. Solar power becomes unreliable during atmospheric events like dust storms, which can block sunlight and significantly reduce energy output, as well as regolith blocking the solar panels. Nuclear power––while more reliable and efficient––is primarily used to keep rovers operational by maintaining critical systems and protecting them from the extreme cold on Mars. This leaves little surplus energy for running power-intensive AI systems, making energy efficiency a key design priority.
The Foreseeable Future
For the foreseeable future, space exploration will rely heavily on robotic systems. While SpaceX has planned Mars missions, we remain far from sending humans to most celestial objects. Both the Moon and Mars are promising candidates for exploration—though only the Moon has hosted humans—but ensuring human safety requires advancements in artificial gravity, synthetic biology, and radiation-resistant spacecraft. Until these technologies are thoroughly tested and proven, society will remain cautious about placing humans in harm's way for what some consider a non-essential pursuit. Robotic systems continue to bridge this gap, as demonstrated by their successes in underwater, aerial, and space missions. These technologies allow us to test scenarios and develop smarter, more adaptive systems capable of interacting with their environments in innovative ways.
Humans often consider themselves the most intelligent species, yet our cognitive abilities are limited by the small window of visible light we perceive within the Electromagnetic Spectrum. For instance, bees can see ultraviolet light, which is invisible to us, due to their unique biology. Similarly, humans emit infrared radiation, which we cannot see without specialized tools. By leveraging wavelengths outside visible light, such as infrared, ultraviolet, and X-rays, we can explore the universe in entirely new ways. These tools enable us to better understand terrain, particularly on Mars, enhancing computational models with AI to create more detailed, multidimensional representations of the environment. However, challenges like energy efficiency, thermal output, Martian dust storms, and limited in situ resources persist. Overcoming these obstacles requires a multi-faceted approach, integrating incremental advancements across disciplines rather than relying on a single solution.
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