Self-Assessment Quiz: Space Debris, Space Law, and Sustainability
Twenty questions on the Kessler syndrome, the debris environment, mitigation and disposal, active removal, space law, and traffic management. Answer each before opening the key. Aim for 16 or more. Use $\mu = 3.986\times10^{5}\ \text{km}^3/\text{s}^2$ where needed.
Question 1
The Kessler syndrome is best described as:
A) a dense wall of debris that instantly traps humanity on Earth B) a self-sustaining collision cascade in which debris breeds more debris C) the gradual re-entry of all low-orbit satellites D) the loss of a satellite to a single micrometeoroid
Question 2
A $1\ \text{cm}$ aluminum sphere ($\sim 1.4\ \text{g}$) at a $10\ \text{km/s}$ closing speed carries roughly the kinetic energy of:
A) a falling raindrop B) a rifle bullet C) a small car in a low-speed crash D) a tonne of TNT
Question 3
The orbital-collision rate scales with the number of objects $N$ as:
A) $N$ B) $\sqrt{N}$ C) $N^2$ D) $\ln N$
Question 4
The "lethal non-trackable" debris population is dangerous mainly because objects $1$–$10\ \text{cm}$ are:
A) too slow to cause damage B) too small to shield against yet too small to track and dodge C) already all de-orbited D) only found above GEO
Question 5
Roughly how many objects larger than $10\ \text{cm}$ are currently tracked? (Tier 2)
A) ~360 B) ~3,600 C) ~36,000 D) ~36,000,000
Question 6
Passivation at end of mission means:
A) turning the satellite so its solar panels face the Sun B) removing all stored energy (venting propellant, safing tanks and batteries) so it cannot later explode C) painting the satellite to reduce radiation pressure D) transferring control to another operator
Question 7
Historically, the single largest source of orbital debris (before the 2007/2009 events) was:
A) micrometeoroids B) astronaut tools lost on spacewalks C) explosions of abandoned, un-passivated rocket stages D) paint flecks
Question 8
A geostationary satellite disposes of itself by:
A) de-orbiting into the atmosphere B) boosting a few hundred km up to a graveyard orbit C) drifting east until it leaves the belt D) waiting for drag to bring it down
Question 9
The delta-v to raise a GEO satellite $\sim 300\ \text{km}$ to a graveyard orbit is closest to:
A) $\sim 11\ \text{m/s}$ B) $\sim 190\ \text{m/s}$ C) $\sim 1{,}500\ \text{m/s}$ D) $\sim 3{,}000\ \text{m/s}$
Question 10
Natural atmospheric decay is a "free" disposal method only:
A) at all altitudes equally B) below roughly $600\ \text{km}$, where lifetimes are short enough to meet the rules C) above $1{,}000\ \text{km}$ D) in geostationary orbit
Question 11
A drag sail shortens a derelict's orbital lifetime because it:
A) raises the ballistic coefficient $\beta$ B) lowers the ballistic coefficient $\beta = m/(C_D A)$, and $\tau \propto \beta$ C) adds thrust D) changes the orbital period
Question 12
The modeling result behind active debris removal is that, to stabilize the crowded shells, we must remove roughly:
A) all debris within one year B) 5–10 large derelicts per year C) one satellite per decade D) nothing — mitigation alone suffices
Question 13
The foundational treaty of international space law, and its year, is:
A) the Registration Convention, 1976 B) the Moon Agreement, 1979 C) the Outer Space Treaty, 1967 D) the Artemis Accords, 2020
Question 14
Under the Outer Space Treaty, a nation's ownership and jurisdiction over a space object it registered:
A) ends the moment the object is abandoned B) is retained indefinitely, even after the object becomes debris C) transfers automatically to the UN D) applies only while the object is operational
Question 15 (True/False, justify)
"Because no nation may own outer space, orbit is effectively a lawless free-for-all." True or false? Justify.
Question 16 (True/False, justify)
"Doubling the number of satellites in a shell roughly doubles the collision risk." True or false? Explain.
Question 17 (True/False, justify)
"A satellite at $800\ \text{km}$ will re-enter on its own soon enough to satisfy the 25-year disposal rule." True or false? Say roughly how long it actually takes and why.
Question 18 (Short answer)
Distinguish mitigation from active debris removal, and explain why models say mitigation alone cannot stabilize the most crowded orbital shells.
Question 19 (Short answer)
A satellite with area $A = 10\ \text{m}^2$ flies $t = 5$ years through a flux $\Phi = 1\times10^{-5}\ \text{m}^{-2}\text{yr}^{-1}$ of $>1\ \text{cm}$ debris. Compute the expected number of impacts and the approximate probability of at least one.
Question 20 (Short answer)
Explain in two or three sentences why orbital sustainability is a "tragedy of the commons," and name one policy idea meant to fix it.
Answer Key
| Q | Ans | Note |
|---|---|---|
| 1 | B | Debris breeds debris once production outpaces drag removal; it is a cascade, not an instant wall. |
| 2 | C | $E = \tfrac12(0.0014)(10^4)^2 = 70\ \text{kJ}$ ≈ a $\sim 700\ \text{kg}$ car at $\sim 50\ \text{km/h}$. |
| 3 | C | Risk lives in pairs; pairs $= N(N-1)/2 \approx N^2/2$. |
| 4 | B | Too energetic to shield, too small to catalog and avoid — the "lethal non-trackable" band. |
| 5 | C | ~36,000 tracked ($>10\ \text{cm}$); ~1 million in the $1$–$10\ \text{cm}$ band (modeled). |
| 6 | B | Removing stored energy stops later explosions/ruptures — the top historical debris source. |
| 7 | C | Un-passivated stage explosions; passivation is the cheap, high-value fix. |
| 8 | B | Graveyard raise ($\sim 11\ \text{m/s}$); de-orbiting from GEO would cost $\sim 1{,}500\ \text{m/s}$. |
| 9 | A | $\Delta v \approx \tfrac{v}{2}\tfrac{\Delta h}{a} = \tfrac{3070}{2}\tfrac{300}{42164} \approx 11\ \text{m/s}$. |
| 10 | B | Below $\sim 600\ \text{km}$, decay is decades or less; higher, it is centuries. |
| 11 | B | Bigger $C_D A$ → smaller $\beta$ → shorter lifetime ($\tau \propto \beta$). |
| 12 | B | ~5–10 large derelicts/yr stabilizes the supercritical shells (NASA modeling, Tier 2). |
| 13 | C | The Outer Space Treaty, in force 1967. |
| 14 | B | Article VIII: jurisdiction, control, and ownership retained indefinitely. |
| 15 | False | Space is a governed commons: states are responsible (OST Art. VI), liable (Liability Convention), and must register objects — the problem is under-governance, not lawlessness. |
| 16 | False | Risk scales as $N^2$, so doubling the population roughly quadruples the collision rate. |
| 17 | False | At $800\ \text{km}$ natural decay takes centuries; it fails both the 25-year and 5-year rules, so active de-orbit or a drag device is needed. |
| 18 | — | Mitigation prevents new debris (disposal rules, passivation); ADR removes existing objects. Even with zero launches, collisions among objects already in crowded shells keep the population growing (supercritical), so removal is required. |
| 19 | — | $N = \Phi A t = (10^{-5})(10)(5) = 5\times10^{-4}$; $P \approx 5\times10^{-4} = 0.05\%$ (about 1 in 2,000). |
| 20 | — | Each operator gains a launch's full benefit but bears only a fraction of the collision risk it creates, so all over-use the finite, shared orbits. Fixes price the externality: orbital-use fees, debris bonds / deposit-refund for on-time de-orbit, real liability. |
Topics to review by question
| Questions | Topic | Section |
|---|---|---|
| 1, 3, 16, 21-style | Kessler syndrome & $N^2$ scaling | §35.1, §35.6 |
| 2, 4, 5 | The debris environment & energy | §35.1, §35.2 |
| 19 | Collision-probability estimate | §35.2 |
| 6, 7, 8, 9, 10, 17 | Mitigation & disposal delta-v/lifetime | §35.3 |
| 11, 12 | Active debris removal | §35.4 |
| 13, 14, 15, 22-style | Space law | §35.5 |
| 18, 20 | Sustainability & the commons | §35.4, §35.6 |