PEP-Part I: Callisto

What planet did my group choose and why?

Our group chose Callisto, one of Jupiter’s largest moons. It is covered in craters and ice, and its surface hasn’t changed much in billions of years (Schenk, 1995). Because it is far from Jupiter’s strong radiation, Callisto is safer for humans than some other moons, like Europa or Io (NASA Science, n.d.).

Scientists think there may be a subsurface ocean under Callisto’s icy surface, which could contain salts and chemicals that might support tiny life forms (Khurana et al., 1998). Its stable surface and relatively calm environment make it an excellent place for science research, exploring resources for human use, and for humans could live.

What opportunities does Callisto offer?

  • Craters and Surface History
    Callisto has over 1,000 craters larger than 10 km(Schenk, 1995). These craters are like a time capsule, saving information about asteroid and comet impacts that happened billions of years ago. By studying them, scientists can learn about the formation and changes of the Solar System.
  • Water and Ice Resources
    About 50% of Callisto’s surface is water ice (NASA Science, n.d.). This ice could be used for drinking water, oxygen production, or even hydrogen fuel, making it a valuable resource for long-term human habitation.
  • Chemical Composition
    Galileo spacecraft spectrometers detected carbon dioxide (~10^-6 bar), sulphur dioxide (~10^-7 bar), and small amounts of organic compounds on the surface (Hibbitts et al., 2000; McCord et al., 1997). These chemicals provide clues about the moon’s chemistry and could support microbial life in its subsurface ocean.
  • Gravity and Movement
    Callisto’s surface gravity is only 0.126 g which is roughly 12% of Earth’s gravity (Zimmer et al., 2000). This means a person weighing 70 kg on Earth would weigh just about 8.8 kg on Callisto. Low gravity makes walking and using tools more difficult, but it also makes transporting heavy equipment and moving large ice blocks easier, which could be helpful for building habitats or exploration bases.

Challenges for Humans

  • Extreme Cold: Average surface temperature is about -139°C (-218°F) (NASA Science, n.d.). This requires heated habitats and suits for human activity.
  • Thin Atmosphere: Callisto has almost no atmosphere, only a tiny amount of CO₂. Humans must live in pressurized habitats and wear suits to breathe and stay safe.
  • Rough Terrain: Craters, ridges, and fractured ice make the surface difficult to drive on, requiring specially designed vehicles (Schenk, 1995).
  • Low Gravity Effects: Muscles and bones weaken in low gravity, so habitats need exercise areas and routines to maintain health (Zimmer et al., 2000).

Vehicles and Habitats

  • Rovers and Transport: Vehicles need to be light, stable, and capable of moving on ice. Hovercraft or walkers may be more practical than traditional wheels (NASA Jet Propulsion Laboratory, n.d.). However it couldn’t be too light. Engineers would need to design it with a low center of gravity and maybe wide, flexible feet or treads to spread its weight. They might also add anchoring spikes or adjustable weights on the side to help it “stick” onto the terrain when moving or drilling.
  • Thermal Protection: Engines, batteries, and pipelines need insulation or heating to operate in the extreme cold.
  • Habitat Design: Homes could be buried underground for protection from cold, and radiation. Interiors need handholds, exercise equipment, and low-gravity design adaptations.

How Humans Could Survive on Callisto

Living on Callisto would be challenging but possible with the right technology. With almost no atmosphere and constant radiation from Jupiter, habitats would need to be underground or inside thick ice. The ice could also be melted for water and oxygen, reducing supplies from Earth.

Sunlight is weak, it is only 1/27th of Earth’s, so nuclear power would be the main energy source. Surface temperatures around –140 °C mean heated suits and vehicles are essential. Low gravity (1/8th of Earth’s) makes movement easier but can weaken muscles and bones, so daily exercise would be important.

How We Know About Callisto

Most of what scientists understand about Callisto comes from two major NASA missions: Voyager and Galileo.

  • Voyager 1 and 2 (1979)
    These spacecraft took the first detailed photos of Callisto’s surface, showing its huge craters, icy crust, and very old terrain. The images and mission data are publicly available through NASA’s Jet Propulsion Laboratory
  • Galileo Orbiter (1995–2003)
    Galileo gave scientists much deeper information using its scientific instruments:
  • Magnetometer: Detected changes in Jupiter’s magnetic field near Callisto, which suggested a subsurface ocean (Khurana et al., 1998; Zimmer et al., 2000).
  • Spectrometers: Found CO₂, SO₂, and organic molecules frozen in the surface ice (McCord et al., 1997; Hibbitts et al., 2000).
  • Surface Mapping: Helped scientists identify over 1,000 large craters and understand Callisto’s geologic history (Schenk, 1995).

APA references

Schenk, P. M. (1995). The geology of Callisto. Journal of Geophysical Research, 100(E9), 19011‑19022. https://ntrs.nasa.gov/citations/19970027091

Khurana, K. K., Kivelson, M. G., Stevenson, D. J., Schubert, G., Russell, C. T., Walker, R. J., & Polanskey, C. (1998). Induced magnetic fields as evidence for subsurface oceans in Europa and Callisto. Nature, 395(6704), 777–780. https://www.nature.com/articles/27394

Zimmer, C., Khurana, K. K., & Kivelson, M. G. (2000). Subsurface oceans on Europa and Callisto: Constraints from Galileo magnetometer observations. Icarus, 147(2), 329–347. https://www.sciencedirect.com/science/article/abs/pii/S001910350096456X?via%3Dihub

McCord, T. B., Carlson, R. W., Smythe, W. D., Hansen, G. B., Clark, R. N., Hibbitts, C. A., et al. (1997). Organics and other molecules in the surfaces of Callisto and Ganymede. Science, 278(5336), 271‑275. https://www.science.org/doi/10.1126/science.278.5336.271

Hibbitts, C. A., Schultz, P. H., et al. (2000). Distributions of CO₂ and SO₂ on the surface of Callisto. Journal of Geophysical Research: Planets, 105(E6), 15,255‑15,273. https://agupubs.onlinelibrary.wiley.com/doi/10.1029/1999JE001157

NASA Jet Propulsion Laboratory. (n.d.). View of Callisto from Voyager and Galileo. NASA / JPL. https://www.jpl.nasa.gov/images/pia01055-view-of-callisto-from-voyager-and-galileo/

NASA Science. (n.d.). Callisto facts. NASA. https://science.nasa.gov/jupiter/jupiter-moons/callisto

Use of AI

For this project I chose to use ChatGPT to help me with my research about Callisto. It helped me find reliable sources, summarize scientific information, and design a concept for an exploration vehicle.

Comments

3 Responses to “PEP-Part I: Callisto”

  1. mcrompton Avatar
    mcrompton

    Good job, Dean. I particularly like your use of in-text citations as a way of pointing directly to what articles/researchers are the source of the data that you share. Please make sure that your references are listed in alphabetical order so that the reader can find them easily. My big question is around your thinking about the effects of gravity and ice on your vehicle design. You say that your vehicle must be light, wide, and have some sort of traction that sticks it to the ice. Some of the ideas can be seen to be conflicting. Can you explain why you need a light vehicle? Why does it need to spread the qeight of the vehicle out? Why does it need to use something to stick it to the ice? Perhaps a heavier vehicle would counter Callisto’s low gravity? Can you respond to this question in the comments below?

    1. deans Avatar

      Thanks for your feedback Mr.Crompton.

      At first, my group went with a lightweight vehicle because we thought it would make the design more energy efficient. But after looking closer at Callisto’s low gravity (around 12–13% of Earth’s), I realized that being too light would actually make traction worse. So now I think a heavier vehicle is the better option, since the extra mass helps it stay grounded instead of sliding around on the ice while makuing it energy efficient.

      Callisto’s surface is a mix of ice, dust, and rocky areas, and the ice can be unpredictable in strength. By using wide tank tracks, the weight gets distributed over a larger area. That reduces the pressure on any single point and lowers the risk of slipping, sinking into softer patches, or cracking weaker ice. It also keeps the vehicle stable when climbing uneven terrain.

      The “sticking to the ice” idea came from an early plan related to resource collection, but since that’s not part of our mission anymore, we removed that system and kept things simpler.

      Do I also need to change my blog post base on the changes I made?

      1. mcrompton Avatar
        mcrompton

        No. Don’t edit the blog post, I prefer you replying to my comments. Thank you, Dean.

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