Infer a surface history without equating craters with age
An impact crater record reflects production and preservation. Volcanic resurfacing, erosion, burial and later impacts can remove or obscure older craters. Comparing surfaces therefore requires common counting criteria, area, size range and a calibrated production history; a larger raw count is not automatically an older surface.
Learning outcome: Keep production, loss, observation time and patch reset separate. Compare the mixed density with both component densities and state why a single-age inversion hides geological history.
Starting recap
Keep interior, thermal, surface-history, orbital and detection assumptions distinct before drawing a planetary inference.
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Try
For p=2, the unreset six-time-unit surface has density 10(1−e^−1.2)≈6.98806. A patch reset at time four has density 10(1−e^−0.4)≈3.29680. The 60:40 mixture is≈5.51155, lower than the unreset surface without changing the body’s formation time.
Open the experimentPredict
Does one mixed crater density imply one unique surface age?
Experiment
Keep production, loss, observation time and patch reset separate. Compare the mixed density with both component densities and state why a single-age inversion hides geological history.
Separate crater production, loss and partial resurfacing
Worked teaching model · synthetic values · Original expected crater inventory dN/dt=p−0.2N, initially 0, observed at time 6. A 40% area patch resets to 0 at supplied time b; remaining 60% does not. Expected mixed density is area weighted; inverse unreset age is conditional on known production/loss. No real crater catalog age, impact chronology or discrete realized count.
Reset keeps your prediction, captures and practice history.
Crater inventory depends on production and erasure, not only elapsed time.
A mixed-age surface can imitate a younger uniform surface under a mistaken inverse model. Real crater dating needs calibrated production, size selection, resurfacing and preservation evidence; this expected-value curve is not an observed impact chronology.
| Quantity | Value | Unit |
|---|---|---|
| Unreset surface expected density | 6.988058 | craters/area |
| Reset patch expected density | 3.296800 | craters/area |
| Area-weighted expected density | 5.511555 | craters/area |
| Age inferred under mistaken unreset model | 4.005393 | time |
| Actual supplied elapsed age | 6 | time |
| Patch elapsed time since reset | 2 | time |
Read exact plotted values
| Unreset elapsed time | Expected crater density |
|---|---|
| 0 | 0 |
| 0.5000000 | 0.9516258 |
| 1 | 1.812692 |
| 1.500000 | 2.591818 |
| 2 | 3.296800 |
| 2.500000 | 3.934693 |
| 3 | 4.511884 |
| 3.500000 | 5.034147 |
| 4 | 5.506710 |
| 4.500000 | 5.934303 |
| 5 | 6.321206 |
| 5.500000 | 6.671289 |
| 6 | 6.988058 |
Original supplied models, not actual planet observations or a unique interior, atmosphere or discovery claim.
Crater inventory depends on production and erasure, not only elapsed time.
A mixed-age surface can imitate a younger uniform surface under a mistaken inverse model. Real crater dating needs calibrated production, size selection, resurfacing and preservation evidence; this expected-value curve is not an observed impact chronology.
Captures preserve recipes and replay their calculated results. They are synthetic model evidence, not physical measurements.
Understand
Apply
Public practice checks a specific claim. It does not establish independent mastery.
Keep p=2 but reset the patch at time zero. What happens to both component histories and the inferred unreset age?
Continue
Completion requires a saved prediction, at least one capture and a reflection. Presence checks do not grade your reasoning.
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