Thursday, April 2, 2026

Micro_G

 Copilot:

Deep Space; explain to me how micro-gravity works in a spacecraft. If there are two astronauts, are they attracted to each other at a certain distance, to the walls, can they push each other??

Deep Space; explain to me how micro-gravity works in a spacecraft. If there are two astronauts, are they attracted to each other at a certain distance, to the walls, can they push each other??

Here’s the fun part about “micro‑gravity” in a spacecraft: nothing magical is happening to gravity itself. What changes is the environment the astronauts are in — and that changes how their bodies behave.

Let’s break it down cleanly and intuitively.

🌌 What “micro‑gravity” really means

Inside a spacecraft in orbit, astronauts are in continuous free‑fall around Earth.

They’re falling with the spacecraft at the same rate, so they don’t feel the normal force that we feel standing on the ground.

Gravity at the altitude of the ISS is still about 90% as strong as on Earth.

But because everything is falling together, astronauts experience weightlessness.

This is why we call it micro‑gravity: not because gravity is tiny, but because the residual forces that remain are tiny.

So:

They are technically attracted to each other.

But the force is so tiny that air currents, ventilation fans, or even breathing will dominate.

In practice, astronauts do not drift toward each other due to gravity.


🧱 Are astronauts attracted to the walls?

Not by gravity.

But they can drift toward walls because of:

✔ Tiny air currents

Ventilation systems constantly move air to prevent CO₂ pockets. This airflow can gently push astronauts around.

✔ Initial motion

If you push off even slightly, you’ll drift until you hit something.

✔ Mass distribution

If the spacecraft rotates slightly, objects inside may drift toward the outer wall due to centrifugal effects — but spacecraft try to avoid rotation.

There is no gravitational pull from the walls that matters.


🤼 Can astronauts push each other?

Absolutely — and this is where micro‑gravity becomes fun.

Newton’s Third Law still rules:

If astronaut A pushes astronaut B,

B moves away, and A moves in the opposite direction.

Because there’s no friction with the floor or air resistance to slow them down, both astronauts will keep drifting until they hit something.

This is why astronauts move carefully — a careless push can send you drifting across the module.

If you want, we can go deeper into:

how spacecraft ventilation shapes movement

why astronauts sometimes “stick” to surfaces

how micro‑gravity affects fluids, tools, or the human body

Just tell me where you want to take this next — space is a great playground for physics.


How about - as is the case with Artemis - the spacecraft is very far from both departure and arrival planet?

When a spacecraft like Artemis is far from both Earth and the Moon — truly in deep space — the physics of “micro‑gravity” becomes even cleaner and more elegant. You’re no longer in orbit around a nearby planet, so you’re not in free‑fall around anything. Instead, you’re in a region where all gravitational pulls are weak and nearly uniform, and everything inside the spacecraft shares the same motion.

Let’s unpack what that means for astronauts floating inside.

🌌 1. What creates micro‑gravity in deep space?

Even far from planets, gravity never becomes zero. But:

The gravitational pull from Earth, Moon, and Sun becomes very small.

More importantly, the pull is almost the same everywhere inside the spacecraft.

This uniformity means there’s no “down” direction and no tidal stretching.

Everything — astronauts, tools, droplets — accelerates together under the same tiny gravitational field.

The result is true free‑floating conditions, often better than low‑Earth orbit.


🧲 2. Are astronauts attracted to each other?

Yes — but the effect is still microscopic.

The gravitational attraction between two 80‑kg astronauts 1 meter apart is:


𝐹 ≈ 4×10^−9newtons

That’s unchanged whether you’re near Earth or in deep space, because it depends only on their masses and distance.

In deep space, there’s less environmental noise (no strong ventilation currents, no orbital tidal forces), so in theory the attraction is more “pure” — but still far too small to matter.

They will not drift together due to gravity.

🧱 3. Are astronauts attracted to the walls?

Still no.

The spacecraft walls have mass, but the gravitational pull from a wall panel is so tiny it’s effectively zero.


What can move astronauts toward a wall:

Air currents (still present, though weaker than on ISS)

Residual spacecraft rotation

Their own initial motion

Vibrations from machinery

But gravitational attraction to the walls is negligible.


🤼 4. Can astronauts push each other?

Absolutely — and in deep space, the effect is even more pronounced.

With no planetary gravity gradients and minimal air drag:

A tiny push sends both astronauts drifting smoothly in opposite directions.

They will continue drifting until they hit a wall or grab something.

Motion is extremely predictable because there are fewer disturbances.

This is why deep‑space missions require careful body control — you don’t want to accidentally launch yourself across the cabin.

Deep space is actually closer to ideal micro‑gravity than orbit.


🧭 6. Does anything “pull” the astronauts in deep space?

Only extremely weak, uniform gravitational fields from:

Earth

Moon

Sun

Other planets (tiny)

But because these fields are nearly the same everywhere inside the spacecraft, they don’t create a sense of direction or weight.

The astronauts float because everything accelerates together.


🌙 7. What about near Lagrange points (like Artemis missions)?

Lagrange points (e.g., L1, L2) are regions where gravitational pulls from Earth and Moon balance in a way that allows stable or semi‑stable orbits.

Even there:

Gravity is not zero.

But the forces are balanced so that the spacecraft can “hover” with minimal fuel.

Inside the spacecraft, astronauts still experience micro‑gravity exactly as described above.


⭐ In short

Even far from planets:

Micro‑gravity persists because everything accelerates together under the same weak gravitational field.

Astronauts are technically attracted to each other, but the force is absurdly tiny.

They are not attracted to the walls.

They can push each other, and the resulting motion is clean and long‑lasting.


If you want, we can go deeper into:

how micro‑gravity affects fluids or tools in deep space

how spacecraft rotation changes the experience

why deep‑space missions sometimes create artificial gravity

Just tell me where you want to explore next — deep space physics is a beautiful rabbit hole.


So there is a fight over that last bag of peanuts during the Artemis flight, and one astronaut pushes the other away from the dispenser. Which astronaut is moving faster, the pusher or pushee? What is the consequence of a push with respect to the arm strength of the pusher?

Great scenario—space peanuts and Newtonian drama.

Who moves faster: pusher or pushee?

It all comes down to conservation of momentum.

When astronaut A pushes astronaut B:

Forces are equal and opposite (Newton’s Third Law).

The impulse (force × time) on each is equal and opposite.

So the change in momentum of each is equal in magnitude and opposite in direction.


𝑚𝐴v𝐴=−𝑚𝐵𝑣𝐵

If they have different masses:

The lighter astronaut ends up with the higher speed.

The heavier astronaut moves more slowly.

If they have the same mass:

They move off with equal speeds in opposite directions.

So: the “faster” one is the lighter one, not “the one who got pushed.”


What does arm strength change?

Arm strength doesn’t change the rules, it changes the numbers:

Stronger push → larger force or longer push time → bigger impulse

Δ𝑝=F⋅Δ𝑡

Bigger impulse means both astronauts get larger (but opposite) momentum.

So both end up moving faster (in opposite directions) than they would with a weaker push.


But:

The ratio of their speeds is still fixed by their masses:

𝑣𝐴𝑣𝐵=−𝑚𝐵𝑚𝐴

Arm strength can’t break conservation of momentum—it just scales the whole event up or down.

Intuitive picture

Same mass, strong shove: they blast apart equally fast in opposite directions.

Heavier pusher, lighter pushee: both get a big momentum change, but the lighter one shoots off faster; the heavier one recoils more slowly.

The pusher “pays” for a stronger shove with:

More muscle effort

More recoil speed (if they’re not much heavier)

A higher chance of ending up drifting into a wall or across the cabin.

If you want, we can plug in actual numbers—say 90 kg vs 70 kg—and compute their exact speeds for a realistic push.


So, on the rebound, who gets the peanuts?

Ah, the orbital peanut duel — a classic.

Let’s walk through it with the same physics we just built up, but now with a bit of tactical flair.

🥜 Who gets the peanut after the push?

It depends entirely on who ends up with the better trajectory toward the dispenser, not on who pushed or who was pushed.

But here’s the key insight:

⭐ The pusher usually loses the peanut.

Why?

Because when astronaut A pushes astronaut B away from the dispenser:

B moves away from the dispenser (obvious).

A recoils in the opposite direction — which is toward the dispenser.

So unless A misjudges the angle or overdoes the push, the pusher ends up drifting toward the peanut source.

This is the micro‑gravity equivalent of shoving someone backward while you fall forward.


🧠 But there’s a twist: mass matters

Let’s say:

Astronaut A (the pusher) = 90 kg

Astronaut B (the pushee) = 70 kg

After the push:

𝑚𝐴𝑣𝐴=−𝑚𝐵𝑣𝐵

So:

B moves away faster (because they’re lighter).

A moves toward the dispenser slower (because they’re heavier).

But direction is what matters for peanut acquisition, not speed.

If A pushes B away from the dispenser, A automatically moves toward it.

Even if A moves slowly, they’re still drifting in the right direction.


💪 What about arm strength?

Arm strength only changes the magnitude of the velocities:

Stronger push → both astronauts get more momentum.

But the ratio of their speeds stays fixed by their masses.

A stronger push means:

B shoots away faster.

A shoots toward the peanuts faster.

So a strong push actually helps the pusher reach the dispenser sooner — as long as they don’t overshoot or spin themselves.


🎯 Final verdict

The pusher gets the peanut.

Unless:

They push at a bad angle,

They impart unwanted rotation,

They overdo it and drift past the dispenser,

Or the pushee grabs a handhold and rebounds like a ninja.

But in a clean, straight-line shove, the pusher wins the snack.


If you want, we can model:

exact speeds for specific masses and push forces

how rotation complicates the peanut chase

how astronauts actually move around using handholds and foot loops

Space is a perfect playground for Newtonian mischief.


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source: La Presse

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Actual speed of push:





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