\documentclass[11pt]{article} \usepackage[margin=1in]{geometry} \usepackage{amsmath} \usepackage{amssymb} \usepackage{graphicx} \usepackage{booktabs} \usepackage{tikz} \usepackage{pgfplots} \pgfplotsset{compat=1.18} \usepackage[colorlinks=true, linkcolor=black, citecolor=black, urlcolor=blue]{hyperref} % --- skin palette: iron rust, graphite, ember gold --------------------------- \definecolor{iron}{HTML}{B5502C} \definecolor{irondeep}{HTML}{8A3A1E} \definecolor{graphite}{HTML}{3A4652} \definecolor{ember}{HTML}{9C7418} \definecolor{ilarblue}{HTML}{2A6FB0} \definecolor{ykarust}{HTML}{C1502E} \definecolor{clubviolet}{HTML}{6A4BC4} \title{The Iron Ball at the Center of the Earth Keeps Changing Its Skin} \author{The Science Journaling Club} \date{Field Notes --- Paper Analysis --- Geophysics} \begin{document} \maketitle \begin{abstract} Nobody has ever touched Earth's inner core, and nobody ever will. Every fact about it arrives secondhand, carried the last 5,150 kilometres by a seismic wave. In February 2025, John Vidale and four co-authors re-examined a dataset of 121 repeating earthquakes near the South Sandwich Islands, recorded between 1991 and 2023 by two seismic arrays in the far north, and asked a narrower question than usual: when the inner core's own drifting rotation brings it back to a position it already occupied years earlier, do the two recordings match \cite{vidale2025}? At Yellowknife (YKA), whose waves graze the inner core's outer few hundred kilometres, some pairs recorded between 2004 and 2008 did not match. At Eielson (ILAR), whose waves bottom out deep near the centre, the same pairs matched fine \cite{vidale2025}. The natural reading is that whatever changed did not change everywhere --- it changed near the boundary, on a timescale of a few years, while the deep interior stayed put. We rebuild the ray geometry that makes this comparison possible, lay out why a solid iron sphere is not supposed to behave this way, and then do the club's own arithmetic: the inner core is about 35\% the volume of the Moon, and a "mushy," structurally softer layer reported elsewhere on the same boundary by an unrelated 2017 study is only about 0.3--0.7\% of the inner core's radius --- a few kilometres of restless skin wrapped around twelve hundred kilometres of otherwise very patient iron. \end{abstract} %============================================================================ \section{A Solid Ball That Keeps Not Acting Like One} About 5,150 kilometres beneath your feet, at a pressure of roughly 330 gigapascals and a temperature north of 5{,}000 kelvin, the molten iron-nickel alloy of the outer core freezes. It has been freezing, slowly, for well over half a billion years, growing a solid ball out from the centre of the planet one crystal at a time. That ball is the inner core: almost pure iron, laced with a little nickel and a scatter of lighter elements, and by every reasonable definition of the word, solid. Solid things are supposed to be boring on human timescales. The inner core has spent thirty years failing to be boring. Since Xiaodong Song and Paul Richards first reported in 1996 that its seismic signature seemed to drift relative to the rest of the planet \cite{song1996}, a small, argumentative subfield has grown up around exactly how a two-thousand kilometre-wide iron sphere, floating in a sea of its own molten parent material, actually behaves. Hrvoje Tkal\v{c}i\'{c} and colleagues extended the same repeating-earthquake logic in 2013 to argue the rotation was not smooth but ``shuffling'' --- speeding, slowing, occasionally reversing \cite{tkalcic2013}. Yaolin Yang and Xiaodong Song reported in 2023 that the apparent rotation itself varies over multiple decades rather than proceeding at one steady rate \cite{yang2023}. A 2014 review by Arwen Deuss catalogues the competing rotation-versus-local-change explanations as one of the field's oldest open questions \cite{deuss2014}. The 2025 paper by Vidale and four co-authors does not resolve that fight by picking a winner. It resolves it by showing both sides were half right, using a dataset built specifically to catch the inner core doing whichever one it does \cite{vidale2025}. ``Later on,'' Vidale told reporters after publication, ``I'd realize I was staring at evidence the inner core is not solid'' --- not liquid, he means, but not perfectly rigid either \cite{physorg2025}. %============================================================================ \section{How You Take the Pulse of Something You Will Never Touch} You cannot drill to the inner core; the deepest hole ever bored, the Kola Superdeep Borehole, reached 12.3 km, about a thousandth of the way down. Everything known about Earth's centre is inferred from how vibrations move through it. The wave that matters here is \textbf{PKIKP}: a P-wave leaves the earthquake, crosses the mantle, refracts into the liquid outer core (K), continues into the solid inner core (I), refracts back out (K), and crosses the mantle a second time to a distant seismometer (P). Only sources and receivers more than about $110^{\circ}$ apart produce a PKIKP arrival at all, which is why this literature almost always pairs an earthquake near one pole with a receiver near the other --- South Sandwich Islands events, recorded in Alaska and northern Canada, sit close to opposite ends of a chord through the planet's centre \cite{vidale2025,song1996,tkalcic2013}. The second trick is what makes the measurement possible at all. Some faults keep rupturing in almost exactly the same way, in almost exactly the same place, years apart --- \emph{repeating earthquakes}, or doublets. Two members of a doublet have, to a good approximation, an identical source and an identical receiver. Whatever differs between their seismograms has to come from whatever lies on the ray path between them and changed in the meantime. For a wave diving through the inner core, that difference is a direct readout of the inner core changing. \begin{figure}[htbp] \centering \begin{tikzpicture}[line width=0.9pt, font=\footnotesize] \draw[graphite, line width=1.6pt] (0,0.4) .. controls (0.6,0.9) and (0.9,-0.1) .. (1.5,0.4) .. controls (2.1,0.9) and (2.4,-0.1) .. (3.0,0.4) .. controls (3.6,0.9) and (3.9,-0.1) .. (4.5,0.4) .. controls (5.1,0.9) and (5.4,-0.1) .. (6.0,0.4); \draw[graphite, line width=1pt, dashed] (0,0.42) .. controls (0.6,0.82) and (0.9,0) .. (1.5,0.42) .. controls (2.1,0.82) and (2.4,0) .. (3.0,0.42) .. controls (3.6,0.82) and (3.9,0) .. (4.5,0.42) .. controls (5.1,0.82) and (5.4,0) .. (6.0,0.42); \node[anchor=west, iron, font=\bfseries\small] at (0,1.3) {A matching doublet (e.g.\ ILAR)}; \draw[ykarust, line width=1.6pt] (0,-0.7) .. controls (0.6,-0.2) and (0.9,-1.2) .. (1.5,-0.7) .. controls (2.1,-0.2) and (2.4,-1.2) .. (3.0,-0.7) .. controls (3.6,-0.2) and (3.9,-1.4) .. (4.4,-0.85); \draw[ykarust, line width=1pt, dashed] (0,-0.68) .. controls (0.6,-0.22) and (0.9,-1.18) .. (1.5,-0.68) .. controls (2.1,-0.22) and (2.4,-1.18) .. (3.0,-0.68) .. controls (3.5,-1.5) and (3.7,0.1) .. (4.0,-1.6) .. controls (4.3,0.2) and (4.5,-1.6) .. (6.0,-0.9); \node[anchor=west, ykarust, font=\bfseries\small] at (0,0.15) {A mismatching doublet (e.g.\ YKA)}; \node[anchor=north, font=\scriptsize] at (3.0,-1.9) {solid/dashed: two recordings of the same repeating pair, years apart}; \end{tikzpicture} \caption{Schematic, not real seismograms. Our redrawing of the logic the paper runs on real waveform pairs: a match means nothing detectable changed along that ray path; a mismatch means something did. The paper classifies each real pair this way, station by station \cite{vidale2025}.} \label{fig:doublet} \end{figure} %============================================================================ \section{Two Stations, Two Very Different Views Through the Same Ball} The paper leans on two seismic arrays in the far north: ILAR, at Eielson Air Force Base near Fairbanks, Alaska, and YKA, near Yellowknife in Canada's Northwest Territories \cite{vidale2025}. Because Fairbanks and Yellowknife sit at slightly different distances and azimuths from the South Sandwich Islands, their PKIKP rays cut through the inner core along different chords. The ILAR path bottoms out deep, near the planet's centre. The YKA path is shallower --- in the paper's own words, ``inner-core-grazing'' --- skimming the outer part of the inner core rather than plunging toward its heart \cite{vidale2025}. \begin{figure}[htbp] \centering \begin{tikzpicture}[line width=0.9pt] \draw[graphite!40, line width=1pt] (0,0) circle (3.0); \filldraw[iron!12, draw=graphite] (0,0) circle (1.7); \filldraw[iron!85, draw=irondeep, line width=1.2pt] (0,0) circle (0.6); \node[font=\tiny, white, font=\bfseries] at (0,0) {inner core}; \node[font=\scriptsize] at (0,2.2) {liquid outer core}; \node[font=\scriptsize] at (0,2.8) {mantle}; \node[ykarust, font=\Large] at (0,3.0) {$\times$}; \node[font=\scriptsize] at (0,3.35) {South Sandwich Is. quake}; % YKA path: shallow chord grazing inner core \draw[ykarust, line width=1.8pt] (0,3.0) -- (-1.35,1.15) arc[start angle=140,end angle=250,radius=0.6] -- (-2.6,-2.2); \node[ykarust, font=\bfseries\small] at (-2.9,-2.55) {YKA}; \node[font=\scriptsize] at (-2.9,-2.85) {grazes the rim}; % ILAR path: deep chord \draw[ilarblue, line width=1.8pt] (0,3.0) -- (-0.55,1.05) arc[start angle=150,end angle=280,radius=0.65] -- (1.9,-2.3); \node[ilarblue, font=\bfseries\small] at (2.15,-2.65) {ILAR}; \node[font=\scriptsize] at (2.15,-2.95) {bottoms deep}; \end{tikzpicture} \caption{Why two stations can disagree about the same inner core. The YKA ray skims the outer part of the inner core; the ILAR ray bottoms out much closer to the centre. If something changes only near the boundary, YKA's grazing path should register it and ILAR's deep path should not --- exactly the pattern reported for pairs recorded 2004--2008 \cite{vidale2025}. Schematic, not to true angular scale.} \label{fig:geometry} \end{figure} %============================================================================ \section{The Trick That Lets You Compare the Same Rock Twice} Comparing any two repeating earthquakes years apart is not, by itself, a clean experiment: if the inner core is rotating relative to the mantle, a ray that grazed one patch of the boundary in 1995 may graze different rock entirely by 2010. A mismatch would then tell you nothing. The team's direct predecessor paper, published in \emph{Nature} in 2024, solved this for the rotation question. Working from 121 repeating earthquakes between 1991 and 2023 --- 143 distinct pairs, some belonging to sixteen ``multiplet'' families --- Wei Wang, Vidale, Guanning Pang, Keith Koper and Ruoyan Wang found that the inner core \textbf{super-rotated} (drifted faster than the mantle) from roughly 2003 to 2008, then \textbf{sub-rotated}, moving back the other way, from 2008 onward --- two to three times more slowly than it had advanced \cite{wang2024}. Because the return drift is slower, the inner core eventually swings back through a rotational position it held years before, handing a wave recorded today a free repeat of a past experiment. \paragraph{Club arithmetic: a sanity check, not a measurement.} If the inner core super-rotated for five years (2003--2008) and crept back at ``two to three times'' slower, simple ratio arithmetic predicts 10--15 years to retrace the same rotational ground. The reported sub-rotation window, 2008--2023, is fifteen years --- right at the top of that range, consistent with a slowdown factor near $3\times$. This is not a result from either paper; it is only a check that the two headline numbers in the 2024 abstract are arithmetically compatible \cite{wang2024}. They are. \begin{figure}[htbp] \centering \begin{tikzpicture} \begin{axis}[ width=12.5cm, height=6.5cm, xmin=1991, xmax=2024, ymin=-0.3, ymax=1.3, xlabel={year}, ylabel={inner core position rel.\ mantle (arb.\ units)}, ymajorgrids=true, grid style={dashed, gray!30}, ytick=\empty, legend style={font=\scriptsize, at={(0.02,0.05)}, anchor=south west} ] \addplot[graphite, line width=1.4pt, mark=none] coordinates { (1991,0.42)(1997,0.42)(2003,0.42)(2004,0.55)(2005,0.68)(2006,0.80)(2007,0.90) (2008,0.97)(2010,0.82)(2012,0.68)(2014,0.58)(2016,0.51)(2018,0.47)(2020,0.44) (2022,0.42)(2023,0.41)(2024,0.41) }; \addlegendentry{schematic rotational offset} \addplot[ykarust, fill=ykarust, fill opacity=0.12, draw=none] coordinates { (2004,-0.3)(2004,1.3)(2008,1.3)(2008,-0.3) } \closedcycle; \addlegendentry{YKA mismatch window, 2004--2008} \draw[ember, dashed, line width=1pt] (axis cs:1991,0.42) -- (axis cs:2013,0.42); \node[ember, font=\scriptsize, anchor=south west] at (axis cs:2013.3,0.44) {position re-occupied}; \end{axis} \end{tikzpicture} \caption{The shape of the rotation history that makes the method work, redrawn schematically from the qualitative result in the 2024 backtracking paper \cite{wang2024}: five years of super-rotation (2003--2008), then roughly three times as many years of slower sub-rotation (2008--2023). The vertical axis is deliberately unlabelled in physical units --- the source papers report timing and a rate ratio, not a plottable single number --- but the shape and the 2004--2008 mismatch window are drawn from the papers' own reported years \cite{vidale2025,wang2024}.} \label{fig:rotation} \end{figure} That is the engine behind the 2025 paper. Vidale and colleagues extended the catalogue with seven more recent events, adding twenty-five more pairs, and searched specifically for pairs recorded when the backtracking history says the inner core had returned to a shared position \cite{vidale2025}. If pure rotation were the whole story, those pairs should match at \emph{both} stations. Any mismatch surviving this control is not about rotation any more --- it has to be about the rock itself. \begin{figure}[htbp] \centering \begin{tikzpicture} \begin{axis}[ ybar, width=11.5cm, height=6cm, symbolic x coords={Events,Pairs,Multiplets}, xtick=data, ylabel={count}, legend style={font=\scriptsize, at={(0.02,0.97)}, anchor=north west}, nodes near coords, every node near coord/.append style={font=\scriptsize} ] \addplot[fill=ilarblue] coordinates {(Events,121) (Pairs,143) (Multiplets,16)}; \addplot[fill=ilarblue!45] coordinates {(Events,128) (Pairs,168) (Multiplets,16)}; \legend{2024 paper \cite{wang2024}, 2025 paper, extended \cite{vidale2025}} \end{axis} \end{tikzpicture} \caption{Repeating earthquakes are rare enough that every study here is a slow accumulation. The 2024 paper worked from 121 South Sandwich Islands earthquakes forming 143 usable pairs in 16 multiplet families \cite{wang2024}; the 2025 paper added seven more events and twenty-five more pairs on the same catalogue \cite{vidale2025}. Real counts from the two papers.} \label{fig:growth} \end{figure} %============================================================================ \section{What Turned Up Between 2004 and 2008} Comparing repeaters recorded when the inner core had cycled back to a shared position, the paper found YKA waveforms that did not match --- among pairs spanning parts of the 2004--2008 window --- while the equivalent ILAR recordings, for the same earthquake pairs, matched fine \cite{vidale2025}. One example the paper documents at length, ``pair 31,'' is a repeating sequence tracked from 2004 to 2017. Only one geometry explains both observations at once. ILAR's deep ray kept sampling structure that had not changed. YKA's shallow ray sampled structure that had. The paper states the conclusion directly: the changes ``most likely'' originate in the shallow inner core, showing up more strongly on ray paths that spend more of their length near the inner-core boundary \cite{vidale2025}. \begin{table}[htbp] \centering \small \begin{tabular}{lll} \toprule \textbf{ILAR (deep)} & \textbf{YKA (shallow)} & \textbf{Implication} \\ \midrule matches & matches & pure rotation return; nothing changed \\ matches & \textbf{differs} & \textbf{shallow-only change --- what was observed, 2004--2008} \\ differs & differs & bulk / deep change (would reach toward the centre) \\ differs & matches & not observed; no simple mechanism for this \\ \bottomrule \end{tabular} \caption{The logic that localises the change. Only one of the four possible combinations was reported \cite{vidale2025}. Table is the club's own layout of the paper's reasoning.} \label{tab:logic} \end{table} %============================================================================ \section{``Annual-Scale'' Does Not Mean ``Ticks Like a Clock''} The title's ``annual-scale variability'' does not mean a fixed one-year cycle. It means the process unfolds over single-digit years rather than the thousands or millions of years geology usually needs. The YKA/ILAR divergence window is about four years wide (2004--2008); the documented example pair spans thirteen years (2004--2017) \cite{vidale2025}. Geological processes that reshape solid rock --- recrystallisation, slow creep, phase change under pressure --- are the textbook example of something too slow to notice. The inner core, iron under pressure high enough to make steel look like putty, is not an obvious candidate for a process fast enough to leave a mark inside two decades of seismic records. Something near its boundary evidently is. %============================================================================ \section{Why Solid Iron Is Allowed to Do This At All} ``Solid'' does the least useful amount of work here that a word can do. Materials under extreme pressure and heat, sitting a few hundred degrees below their melting point, can flow slowly by viscous creep --- the same mechanism that lets glaciers move and lets the solid mantle convect over millions of years, potentially operating far faster near the inner core's edge. Bruce Buffett's 1997 geodynamic estimate placed the inner core's effective viscosity somewhere between a very stiff solid and something that, over the right timescale, behaves almost like a very slow fluid \cite{buffett1997}; mineral-physics work on iron's strength at core pressures has since pushed some estimates toward a mechanically weaker inner core than earlier models assumed \cite{gleason2013}. The paper offers two candidate mechanisms and is honest that it cannot yet distinguish them \cite{vidale2025}. One: bumps in the inner-core boundary's topography are gravitationally coupled to mantle density anomalies, and slow rotation flexes a given patch as it passes a fixed mantle feature. Two: the outer core is a vigorously convecting liquid-metal ocean whose motion simply drags --- exerts traction --- on the solid surface it touches. Either mechanism only needs to act on a thin near-surface layer to reproduce the observed pattern. Separately, using an unrelated seismic method, Dongdong Tian and Lianxing Wen reported in 2017 that the inner-core boundary is not uniform everywhere: beneath the southwest Okhotsk Sea, reflected compressional waves revealed a patch, 4--8 km thick, with seismic properties between the solid inner core and the liquid outer core --- consistent with a genuinely ``mushy,'' partially molten transition \cite{tian2017}. That is a different location and a different method, almost certainly not the same patch the South Sandwich Islands rays sample. What it establishes is that the boundary is independently known to be capable of local structural softness at all. %============================================================================ \section{Club Arithmetic: How Big Is the Ball, and How Thin Is the Skin} \label{sec:club} Two numbers do a lot of intuitive work here, and neither is stated outright in the paper. \paragraph{Size, against something you can picture.} The PREM reference Earth model puts the inner core's radius at 1{,}221.5~km \cite{prem1981}; the ak135 travel-time model, which this very paper's own reference list leans on for seismic velocities, gives a slightly different figure, close to 1{,}217~km \cite{kennett1995}. As a sphere, \begin{equation} V_{\text{ic}} = \tfrac{4}{3}\pi r^3 \approx 7.63\times10^{9}\ \text{km}^3 \qquad (r = 1{,}221.5\ \text{km}). \end{equation} NASA's published lunar volume is $2.1968\times10^{10}\ \text{km}^3$ \cite{nasamoon}. The ratio is \begin{equation} \frac{V_{\text{ic}}}{V_{\text{Moon}}} \approx 0.35 , \end{equation} about 35\% of the Moon's volume. \paragraph{Thinness, against the whole radius.} Tian and Wen's mushy-zone thickness of 4--8~km \cite{tian2017}, divided by the PREM radius, gives \begin{equation} \frac{4\text{--}8\ \text{km}}{1{,}221.5\ \text{km}} \approx 0.33\text{--}0.65\% . \end{equation} We are \emph{not} claiming this is the thickness of the specific patch that changed at YKA between 2004 and 2008 --- the 2025 paper gives no depth figure for that patch, only that it is shallower than ILAR's ray path. This arithmetic shows the right order of magnitude for how thin a seismically soft layer at this boundary can be and still be measurable and published elsewhere on the same ball. \begin{figure}[htbp] \centering \begin{tikzpicture}[line width=0.9pt] \draw[graphite!50] (0,0) circle (1.9); \node[font=\scriptsize] at (0,-2.25) {the Moon, $r=1{,}737.4$ km \cite{nasamoon}}; \filldraw[clubviolet, opacity=0.8, draw=irondeep] (0,0) circle (1.336); \node[white, font=\tiny\bfseries] at (0,0) {inner core}; \node[font=\small, clubviolet, font=\bfseries] at (0,-2.7) {$\approx$ 35\% of the Moon's volume}; \begin{scope}[xshift=6.5cm] \draw[iron, fill=iron, opacity=0.82] (0,-2.2) rectangle (0.6,2.2); \draw[ember, line width=1.6pt] (0,2.2) -- (0.6,2.2); \node[anchor=west, font=\scriptsize, ember] at (0.8,2.1) {up to 8 km, ``mushy'' \cite{tian2017}}; \node[anchor=west, font=\scriptsize] at (0.8,-2.2) {1{,}221.5 km radius \cite{prem1981}}; \node[anchor=north, font=\scriptsize, align=center] at (0.3,-2.55) {not to true scale --- \\ the real sliver is far thinner}; \end{scope} \end{tikzpicture} \caption{Club arithmetic, not paper data. Left: the inner core drawn to scale beside the Moon. Right: the full inner-core radius as a bar, with the outer few kilometres called out at roughly the thickness a real 4--8~km mushy layer would occupy if drawn honestly --- thinner than this figure can actually render, which is itself the point.} \label{fig:club} \end{figure} %============================================================================ \section{The Old Debate, and Why ``Tentatively Both'' Is the Right Answer} For three decades the argument has run along one fault line: is temporal variability in PKIKP waveforms caused by the inner core physically \emph{rotating}, so a fixed ray samples new material over time, or by the boundary itself \emph{changing shape} under a fixed or slowly rotating ray? Vidale and colleagues' answer, stated in their own abstract, is ``tentatively both'' \cite{vidale2025}. The 2024 result established a real rotation signal with a measurable 2008 reversal \cite{wang2024}; the 2025 result shows that once rotation is controlled for, a genuine residual mismatch survives at the shallow-sampling station and not the deep one. Untangling how much of the historical literature's disagreements trace to one effect or the other is, per the authors, a project for more data, not a question this paper alone closes \cite{vidale2025}. %============================================================================ \section{Why Any of This Matters Above Ground} The inner core is not an inert curiosity. Its growth releases latent heat and light elements into the base of the liquid outer core, one of the main engines believed to drive the convection that generates Earth's magnetic field. A boundary that flexes or couples mechanically to mantle structure overhead is a boundary condition on that convection, not a bystander to it. Cao, Masson and Romanowicz's 2007 mapping of short-wavelength inner-core boundary topography treated the shape of this surface as geodynamically relevant for exactly this reason \cite{cao2007}. A boundary that changes shape on a timescale of years, rather than only over the hundreds of millions of years the inner core took to grow, is a different kind of boundary condition than most geodynamo models have assumed. %============================================================================ \section{What Would Make Us More Confident} The result rests on a genuinely small number of qualifying comparisons: the specific repeating pairs recorded during a window when the backtracking model says the inner core had cycled back to a shared position, at just two stations. More repeating earthquakes, especially along different azimuths, would sample different chords and either corroborate a genuinely localised shallow change or reveal the YKA pattern as more station-specific than global. The 2025 paper's own extension --- seven new events, twenty-five new pairs \cite{vidale2025} --- is exactly this kind of incremental strengthening, and the underlying earthquake sequence is still active. A harder test would be an independent geometry, a different source region and receivers, that also brackets a shallow-versus-deep contrast and checks whether it reproduces a shallow-only signal on a comparable timescale. %============================================================================ \section{What We Would Tell Someone Who Only Read the Headline} Three things. First, nobody found a hidden ocean or a crack in the inner core; ``mushy'' is a term of art borrowed from a different, unrelated study of a different patch of the same boundary \cite{tian2017}, describing a seismic property between solid-like and liquid-like, not an actual slush. Second, ``annual-scale'' describes how fast the process unfolds, not a strict yearly cycle. Third, and most important: the paper does not claim the inner core is secretly liquid. It claims something narrower and more interesting --- that the outermost sliver of a two-thousand-kilometre solid iron sphere is soft enough, at the right pressure and temperature and given enough time, to visibly deform within a human research career, while the deep interior a few hundred kilometres further in shows no such thing. %============================================================================ \begin{thebibliography}{99} \bibitem{vidale2025} Vidale, J.~E., Wang, W., Wang, R., Pang, G. \& Koper, K. (2025). Annual-scale variability in both the rotation rate and near surface of Earth's inner core. \textit{Nature Geoscience} 18, 267--272. doi:10.1038/s41561-025-01642-2 \bibitem{wang2024} Wang, W., Vidale, J.~E., Pang, G., Koper, K.~D. \& Wang, R. (2024). 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Short wavelength topography on the inner-core boundary. \textit{Proceedings of the National Academy of Sciences} 104, 31--35. doi:10.1073/pnas.0609035104 \bibitem{buffett1997} Buffett, B.~A. (1997). Geodynamic estimates of the viscosity of the Earth's inner core. \textit{Nature} 388, 571--573. doi:10.1038/41544 \bibitem{gleason2013} Gleason, A.~E. \& Mao, W.~L. (2013). Strength of iron at core pressures and evidence for a weak Earth's inner core. \textit{Nature Geoscience} 6, 571--574. doi:10.1038/ngeo1858 \bibitem{deuss2014} Deuss, A. (2014). Heterogeneity and anisotropy of Earth's inner core. \textit{Annual Review of Earth and Planetary Sciences} 42, 103--126. doi:10.1146/annurev-earth-060313-054658 \bibitem{kennett1995} Kennett, B.~L.~N., Engdahl, E.~R. \& Buland, R. (1995). Constraints on seismic velocities in the Earth from traveltimes. \textit{Geophysical Journal International} 122, 108--124. doi:10.1111/j.1365-246X.1995.tb03540.x \bibitem{prem1981} Dziewonski, A.~M. \& Anderson, D.~L. (1981). Preliminary reference Earth model. \textit{Physics of the Earth and Planetary Interiors} 25, 297--356. doi:10.1016/0031-9201(81)90046-7 \bibitem{nasamoon} NASA Goddard Space Flight Center, National Space Science Data Center (2024). \textit{Moon Fact Sheet}. nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html \bibitem{physorg2025} \textit{Phys.org} (2025). Earth's inner core is less solid than previously thought: Study reveals structural transformation. News report on \cite{vidale2025}, including comment from J.~E.~Vidale. \end{thebibliography} \end{document}