Lab 06: Planetary Surfaces and Small Bodies

Use image evidence to infer cratering, surface age, geological process, and habitability context.

Learning Objectives

Preparation

Materials and Data

Apparatus and Setup

Procedure

  1. Inspect two planetary or moon surface images at comparable scale and resolution.
  2. Count craters in at least two equal-area regions and record obvious resurfacing features such as flows, tectonic cracks, smooth plains, or ejecta blankets.
  3. Classify each region as relatively older or younger and justify the classification.
  4. For one icy moon or Mars image, identify evidence relevant to past or present liquid environments.
  5. Record source, mission/instrument if supplied, scale, wavelength/color notes, and any processing caveats.

Measurement Record

Use this structure or an equivalent table in your lab notebook.

image regionareacrater countsurface featuresrelative ageuncertainty/caveat
      
      
      

Analysis and Uncertainty

Deliverables

Assessment Criteria

References, Software, and Data Provenance

Any additional dataset, image, or software source used by an instructor should be added to ../reference-log.md with source, access date, license or usage note, and processing steps.