Astronomy · Unit 3: The Solar System · Project 3.1.3

Deep Dive: Habitability Report

🔬 Deep Dive
Two new factors, plus a scorecard for building your own comparison.
Synthesis · 3.1.1 + 3.1.2 + newConcept

The Habitability Framework

"Habitable" isn't one number — it's a balance of several factors, and a real habitability argument weighs all of them together rather than picking a winner off just one dramatic fact. Three of these five factors you already have from Activities 3.1.1 and 3.1.2. Two are new here.

Atmosphere &TemperatureRadiationShieldingSurfaceStabilityGravityWater &ResourcesAll five, weighed together — not just the one that sounds most dramatic
Atmosphere · Radiation shielding · Surface stability · Gravity · Water & resources
💡No world in this comparison set wins on all five. That's exactly the point — a real habitability report has to say which factors matter most for the specific mission you're proposing, not just declare an obvious winner.
New factorConcept

Gravity and the Human Body

Surface gravity is usually given as a fraction of Earth's own (1 g). It's never come up yet in this unit because it doesn't affect a planet's geology or atmosphere the way size and heat do — but it matters enormously for an actual human visitor. Long-term exposure to low gravity is linked to bone density loss and muscle atrophy, among other effects; nobody yet knows exactly how a human body would adapt to spending years at a fraction of Earth gravity, since no one has done it.

WorldSurface gravity
Mercury0.38 g
Venus0.90 g
Earth1.0 g
Mars0.38 g
The Moon0.17 g
⚠️Common mix-up: "lower gravity" isn't automatically a plus just because it sounds easier to move around in. For a long-term human presence, it's a real open health question, not a convenience.
New factorConceptExample

Water and Resources

Water is one of the heaviest, most expensive things to launch from Earth — so a world that already has some is a genuinely huge practical advantage for any future mission, both for drinking and for splitting into hydrogen and oxygen as fuel and breathable air.

The surprise: water ice has been confirmed not just on Mars, but in permanently shadowed craters at both poles of the Moon — and at Mercury's poles too. Two airless worlds that bake under direct sunlight are, in specific hidden pockets that never see the Sun at all, cold enough to have held onto ice for billions of years.

Confirmed water/ice: Earth, Mars, the Moon, and Mercury — not Venus
SynthesisSkill

Putting Together a Comparison

Use the scorecard below to pull real numbers for any two worlds — this is exactly the data your own project deliverable will draw on.

Build your comparison

Pick any two worlds to compare — this is the exact data you'll need for your own report.

FactorMarsMoon
Gravity0.38 g0.17 g
Distance1.52 AU~1.0 AU (orbits Earth)
Day length~24.6 hours~29.5 Earth days
AtmosphereThin CO₂, <1% Earth's pressureNone
Temperature~-63°C average-173°C to 127°C swings
Magnetic fieldNone todayNone
WaterPolar ice caps, some subsurface iceIce in permanently shadowed polar craters
GeologyAncient highlands next to young volcanic TharsisAncient cratered highlands + younger volcanic maria
ExampleGuided Example — Mars vs. the Moon for a First Outpost

Weigh Mars against the Moon as a target for a first long-term human outpost.

Step 1 — Distance and travel time
The Moon is about 3 days away; Mars takes roughly 6–9 months one way — a massive practical advantage for the Moon.
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