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).
Analyze differential photometry and derive a plate scale and rate of motion from astrometric data.
At a given time, target flux = 0.945 and comparison flux = 0.998 (both normalized). Compute Δm = −2.5log10(F_target/F_comp).
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.
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.
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.
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.
Verify against OpenStax Astronomy 2e Chapter 17.1 (magnitudes) and Chapter 19.2 (astrometry) before instructional release.
materials/ASTR210/data/ where referenced above.