ASTR 120 Problem Set 04

Lectures 07-08: Airless worlds and Mars water evidence

Due and Scope

Due: [insert date]. Submit calculations, evidence tables, and concise interpretations.

Learning objectives: interpret craters, rays, regolith, and density on airless worlds; use lunar samples as chronology anchors; evaluate geomorphic and mineral evidence for water on Mars without overclaiming life.

Instructions: Carry units through calculations, distinguish past from present water, and identify observation versus inference. Revisions may be resubmitted with a change note.

Problems

1. Airless-World Crater Chronology 25 points

Two lunar image tiles each cover \(2.0\times10^4\,\mathrm{km^2}\). Tile H in the highlands contains 260 craters larger than 1 km. Tile M in a mare basalt plain contains 52 craters larger than 1 km, plus bright rays from a nearby young crater crossing the tile.

  1. Compute crater density for each tile in craters per \(10^4\,\mathrm{km^2}\).
  2. Compute the density ratio \(H/M\).
  3. Rank the highland surface, mare basalt, and bright rays from oldest to youngest.
  4. Explain why lunar sample ages are needed to turn relative crater density into an absolute chronology.

Deliverables: density table, age sequence, and chronology explanation.

2. Moon-Mercury Density Comparison 25 points

Use \(\rho=M/(4\pi R^3/3)\). The Moon has \(M=7.35\times10^{22}\) kg and \(R=1737\) km. Mercury has \(M=3.30\times10^{23}\) kg and \(R=2440\) km.

  1. Compute both mean densities in g cm\(^{-3}\).
  2. Which object is more metal-rich by inference? Defend the answer.
  3. Explain how a giant impact can plausibly help explain both the Moon's low iron fraction and Mercury's high metal fraction.

Deliverables: density calculations and a 150-200 word interpretation.

3. Mars Water Evidence Ranking 25 points

Rank the following observations for the claim "Mars had sustained liquid water at the surface in the past": valley networks, hydrated clay minerals, polar ice, recurring slope lineae, and a delta deposit in an ancient crater lake basin.

  1. Create a ranking from strongest to weakest for the stated claim.
  2. For each observation, mark whether it best supports past liquid water, present ice, present brines, or general volatile inventory.
  3. State one ambiguity or alternative explanation for each observation.
  4. Explain why evidence for water is not automatically evidence for life.

Deliverables: ranked evidence table and interpretation paragraph.

4. Delta Volume and Minimum Water Transport 25 points

A fan-shaped deposit in a martian crater covers \(45\,\mathrm{km^2}\) and has average exposed thickness \(20\) m. Assume the deposit is sediment with porosity 0.35 and grain density \(3000\,\mathrm{kg\ m^{-3}}\).

  1. Compute the bulk volume of the deposit in m\(^3\).
  2. Compute the solid-grain volume and sediment mass.
  3. If only 2% of suspended sediment carried by water is finally preserved in this deposit, estimate the minimum transported sediment mass.
  4. Explain why this supports sustained transport better than a single isolated channel image.

Deliverables: volume and mass calculations with units and geologic interpretation.

OpenStax Companion Practice

Recommended for additional practice: OpenStax Astronomy 2e, Chapter 9, Review Questions 10, 11, 13, 16, and 20; Thought Questions 21, 27, and 31; Figuring for Yourself 32-35; Chapter 10, Review Questions 4, 6, and 12; Thought Questions 19, 23, and 27; Figuring for Yourself 28 and 32. Verify numbering against the adopted PDF before LMS release.

References and Data Sources