ASTR 210 Problem Set 03: Light Curves and Astrometry

Analyze differential photometry and derive a plate scale and rate of motion from astrometric data.

Problems

1. Differential magnitude 15 points

At a given time, target flux = 0.945 and comparison flux = 0.998 (both normalized). Compute Δm = −2.5log10(F_target/F_comp).

2. Dip depth 15 points

Using the baseline Δm = 0.0054 mag (from t = 0.00 in Lab 04), compute the dip depth relative to baseline for the Δm found in Problem 1.

3. Plate scale 15 points

Two images of the same field show a pixel separation of 20.4 px for an object that moved 16.8 arcsec on the sky between exposures. Compute the plate scale in arcsec/pixel.

4. Rate of motion and classification 15 points

If the two images in Problem 3 were separated by 12 minutes, compute the object’s angular rate of motion in arcsec/minute and state whether this rate is more consistent with a main-belt asteroid or a fast-moving near-Earth object.

Due and Scope

Submit a clear solution with equations, units, labeled quantities, and a short narrative interpretation for each problem. Show every reduction step and state your assumptions explicitly; a correct final number without visible work receives partial credit at most.

OpenStax Companion Reading

Verify against OpenStax Astronomy 2e Chapter 17.1 (magnitudes) and Chapter 19.2 (astrometry) before instructional release.

References and Data Sources