Verify Lectures 1–8: fix Stokes velocity error, complete author lists

Phase 1c verification of all 8 foundational lectures:
- Fix Stokes settling velocity in L4 (was 0.04 m/s, correct is ~4 m/s)
- Fix Mars scale height temperature in L5 (210→215 K for consistency)
- Replace truncated author lists for Thomas2023 (49) and Farley2022 (114)
- Mark L1–8 as "Verified" in course development roadmap

Co-Authored-By: Claude Opus 4.6 <noreply@anthropic.com>

Author: timlichtenberg

book/04_differentiation_magnetospheres/differentiation_magnetospheres.md

@@ -19,7 +19,7 @@ $$
 v_{\mathrm{Stokes}} = \frac{2}{9} \frac{\Delta\rho \, g \, r^2}{\mu}
 $$ (eq:stokes-settling)
 
-where $\Delta\rho \approx 4000$ kg m$^{-3}$ is the density contrast between metal and silicate, $g$ is the gravitational acceleration, $r$ is the droplet radius, and $\mu$ is the dynamic viscosity of the silicate melt. For centimetre-sized iron droplets ($r \sim 0.01$ m) in a low-viscosity magma ocean ($\mu \sim 0.1$ Pa s, $g \sim 5$ m s$^{-2}$ for an Earth-sized body during formation), this gives $v_{\mathrm{Stokes}} \sim 0.04$ m s$^{-1}$, or about 4 cm per second. At this rate, droplets could traverse a magma ocean thousands of kilometres deep in a matter of **hundreds of years** — geologically instantaneous {cite:p}`Rubie2015`.
+where $\Delta\rho \approx 4000$ kg m$^{-3}$ is the density contrast between metal and silicate, $g$ is the gravitational acceleration, $r$ is the droplet radius, and $\mu$ is the dynamic viscosity of the silicate melt. For centimetre-sized iron droplets ($r \sim 0.01$ m) in a low-viscosity magma ocean ($\mu \sim 0.1$ Pa s, $g \sim 5$ m s$^{-2}$ for an Earth-sized body during formation), this gives $v_{\mathrm{Stokes}} \sim 4$ m s$^{-1}$. At this rate, droplets could traverse a magma ocean thousands of kilometres deep in a matter of **days** — geologically instantaneous {cite:p}`Rubie2015`.
 
 ### The Moon-forming giant impact
 

book/05_atmospheres_1/atmospheres_1.md

@@ -169,7 +169,7 @@ We can now compute scale heights for several bodies using their characteristic a
 |------|:-------:|:-----:|:-----------------:|:---------:|
 | Venus | 735 | 43.4 | 8.87 | 15.8 |
 | Earth | 288 | 28.97 | 9.81 | 8.5 |
-| Mars | 210 | 43.3 | 3.72 | 11.1 |
+| Mars | 215 | 43.3 | 3.72 | 11.1 |
 | Jupiter | 165 | 2.2 | 24.8 | 27 |
 | Titan | 94 | 28.6 | 1.35 | 21 |
 

book/references.bib

@@ -903,7 +903,7 @@ @article{Greene2023
 }
 
 @article{Thomas2023,
-    author  = {Thomas, Cristina A. and Naidu, Shantanu P. and Scheirich, Peter and Moskovitz, Nicholas A. and Pravec, Petr and Chesley, Steven R. and Rivkin, Andrew S. and Cheng, Andrew F. and Agrusa, Harrison F. and Raducan, Sabina D. and Daly, R. Terik and others},
+    author  = {Thomas, Cristina A. and Naidu, Shantanu P. and Scheirich, Peter and Moskovitz, Nicholas A. and Pravec, Petr and Chesley, Steven R. and Rivkin, Andrew S. and Osip, David J. and Lister, Tim A. and Benner, Lance A. M. and Brozovi{\'c}, Marina and Contreras, Carlos and Morrell, Nidia and Ro{\.z}ek, Agata and Ku{\v{s}}nir{\'a}k, Peter and Hornoch, Kamil and Mages, Declan and Taylor, Patrick A. and Seymour, Andrew D. and Snodgrass, Colin and J{\o}rgensen, Uffe G. and Dominik, Martin and Skiff, Brian and Polakis, Tom and Knight, Matthew M. and Farnham, Tony L. and Giorgini, Jon D. and Rush, Brian and Bellerose, Julie and Salas, Pedro and Armentrout, William P. and Watts, Galen and Busch, Michael W. and Chatelain, Joseph and Gomez, Edward and Greenstreet, Sarah and Phillips, Liz and Bonavita, Mariangela and Burgdorf, Martin J. and Khalouei, Elahe and Longa-Pe{\~n}a, Pen{\'e}lope and Rabus, Markus and Sajadian, Sedighe and Chabot, Nancy L. and Cheng, Andrew F. and Ryan, William H. and Ryan, Eileen V. and Holt, Carrie E. and Agrusa, Harrison F.},
     title   = {Orbital Period Change of {Dimorphos} Due to the {DART} Kinetic Impact},
     journal = {Nature},
     volume  = {616},
@@ -914,7 +914,7 @@ @article{Thomas2023
 }
 
 @article{Farley2022,
-    author  = {Farley, K. A. and Stack, K. M. and Shuster, D. L. and Horgan, B. H. N. and Hurowitz, J. A. and Tarnas, J. D. and Simon, J. I. and Sun, V. Z. and Scheller, E. L. and Moore, K. R. and McLennan, S. M. and others},
+    author  = {Farley, K. A. and Stack, K. M. and Shuster, D. L. and Horgan, B. H. N. and Hurowitz, J. A. and Tarnas, J. D. and Simon, J. I. and Sun, V. Z. and Scheller, E. L. and Moore, K. R. and McLennan, S. M. and Vasconcelos, P. M. and Wiens, R. C. and Treiman, A. H. and Mayhew, L. E. and Beyssac, O. and Kizovski, T. V. and Tosca, N. J. and Williford, K. H. and Crumpler, L. S. and Beegle, L. W. and Bell, J. F. and Ehlmann, B. L. and Liu, Y. and Maki, J. N. and Schmidt, M. E. and Allwood, A. C. and Amundsen, H. E. F. and Bhartia, R. and Bosak, T. and Brown, A. J. and Clark, B. C. and Cousin, A. and Forni, O. and Gabriel, T. S. J. and Goreva, Y. and Gupta, S. and Hamran, S.-E. and Herd, C. D. K. and Hickman-Lewis, K. and Johnson, J. R. and Kah, L. C. and Kelemen, P. B. and Kinch, K. B. and Mandon, L. and Mangold, N. and Quantin-Nataf, C. and Rice, M. S. and Russell, P. S. and Sharma, S. and Siljestr{\"o}m, S. and Steele, A. and Sullivan, R. and Wadhwa, M. and Weiss, B. P. and Williams, A. J. and Wogsland, B. V. and Willis, P. A. and Acosta-Maeda, T. A. and Beck, P. and Benzerara, K. and Bernard, S. and Burton, A. S. and Cardarelli, E. L. and Chide, B. and Clav{\'e}, E. and Cloutis, E. A. and Cohen, B. A. and Czaja, A. D. and Debaille, V. and Dehouck, E. and Fair{\'e}n, A. G. and Flannery, D. T. and Fleron, S. Z. and Fouchet, T. and Frydenvang, J. and Garczynski, B. J. and Gibbons, E. F. and Hausrath, E. M. and Hayes, A. G. and Henneke, J. and J{\o}rgensen, J. L. and Kelly, E. M. and Lasue, J. and Le Mou{\'e}lic, S. and Madariaga, J. M. and Maurice, S. and Merusi, M. and Meslin, P.-Y. and Milkovich, S. M. and Million, C. C. and Moeller, R. C. and N{\'u}{\~n}ez, J. I. and Ollila, A. M. and Paar, G. and Paige, D. A. and Pedersen, D. A. K. and Pilleri, P. and Pilorget, C. and Pinet, P. C. and Rice, J. W. and Royer, C. and Sautter, V. and Schulte, M. and Sephton, M. A. and Sharma, S. K. and Sholes, S. F. and Spanovich, N. and St. Clair, M. and Tate, C. D. and Uckert, K. and VanBommel, S. J. and Yanchilina, A. G. and Zorzano, M.-P.},
     title   = {Aqueously altered igneous rocks sampled on the floor of {Jezero} crater, {Mars}},
     journal = {Science},
     volume  = {377},

planning/course_development.md

@@ -403,14 +403,14 @@ All homework sheets are **ungraded formative practice**. Each contains 4–6 pro
 
 | # | Lecture | Status | Priority |
 |---|--------|--------|----------|
-| 1 | Introduction & history | Draft complete (figures added) | High |
-| 2 | Planet formation & orbital dynamics | Draft complete (figures added) | High |
-| 3 | Planetary heat & energy transport | Draft complete (figures added) | High |
-| 4 | Chemical differentiation & magnetospheres | Draft complete (figures added) | High |
-| 5 | Atmospheres I | Draft complete (figures added) | High |
-| 6 | Atmospheres II | Draft complete (figures added) | High |
-| 7 | Planetary surfaces | Draft complete (figures added) | High |
-| 8 | Planetary interiors | Draft complete (figures added) | High |
+| 1 | Introduction & history | Verified | High |
+| 2 | Planet formation & orbital dynamics | Verified | High |
+| 3 | Planetary heat & energy transport | Verified | High |
+| 4 | Chemical differentiation & magnetospheres | Verified | High |
+| 5 | Atmospheres I | Verified | High |
+| 6 | Atmospheres II | Verified | High |
+| 7 | Planetary surfaces | Verified | High |
+| 8 | Planetary interiors | Verified | High |
 | 9 | Rocky planets: Earth & Venus | Not started | Medium |
 | 10 | Rocky planets: Mercury & Mars | Not started | Medium |
 | 11 | Gas & ice giants | Not started | Medium |