REVIEW 2 major objections 5 minor 18 references
Small telescopes and simple models still recover the speed of light from Io’s eclipses, just as Roemer did 350 years ago.
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · grok-4.5
2026-07-31 05:00 UTC pith:2VGLPVO2
load-bearing objection Clean didactic replication of Roemer with real multi-observer timings; the ~10% circular-model result is solid, the 298200 km/s headline is mostly a consistency check. the 2 major comments →
De mora luminis: Roemer's discovery 350 years later
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Roemer’s method remains valid under period-comparable visual conditions: the authors’ eye and camera timings of Io emersions, reduced with the simplest uniform-circular geometry, already give c within roughly 10 percent of the accepted value; feeding the same timings a synodic period taken from modern ephemerides produces the weighted average c = (298200 ± 1900) km s⁻¹.
What carries the argument
The linear relation between the increase in Earth–Jupiter distance after opposition and the accumulated delay in successive Io emersions; the slope of that line is the speed of light.
Load-bearing premise
The most precise quoted value treats Io’s average orbital period extracted from modern planetarium software as an independent input, even though that software already incorporates the known speed of light.
What would settle it
Re-reduce the same raw emersion times using an Io synodic period measured solely from dynamical models that contain no light-travel-time terms; if the resulting slope then departs significantly from 3 × 10⁸ m/s, the high-precision claim fails.
If this is right
- Undergraduate labs can measure c to ~10 % with an 80–120 mm refractor, a stopwatch, and circular-orbit arithmetic.
- Adding orbital eccentricity alone can worsen the answer; students must confront competing perturbations before trusting more complex models.
- The same data set can be re-used to compare human versus digital detection thresholds and atmospheric-error budgets.
- Roemer’s 1677 Great Red Spot timings supply an independent historical cross-check that light delay appears in Jupiter’s rotation as well as in Io’s eclipses.
Where Pith is reading between the lines
- The didactic design deliberately keeps telescope aperture and timing precision near 17th-century limits so that students experience the same systematic floor Roemer faced.
- Because the high-precision result is essentially a consistency test against modern ephemerides, the paper’s strongest first-principles claim remains the ~10 % circular-model recovery.
- A multi-year campaign spanning Jupiter’s full radial-velocity cycle would map how much the uncorrected circular result wanders, quantifying when simple models succeed or fail.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The authors re-observe Io eclipse emersions with eye and small telescopes comparable to late-17th-century instruments, plus one CMOS series, over ~70 orbits after the 2023 opposition. They recover c ≈ 2.6×10^5 km s⁻¹ (within ~10–14% of the modern value) from a uniform-circular model of Earth–Jupiter distance versus observed delay (Table 5), show that an ellipticity-only correction for Jupiter can over-correct and worsen the result, and obtain a weighted average c = (298200 ± 1900) km s⁻¹ when the Io synodic period is taken from modern ephemerides after light-time removal (Table 6). They argue the exercise has strong didactic value and report an archival note that Roemer in 1677 also timed Great Red Spot meridian transits as an independent check.
Significance. For a history-of-physics / physics-education venue the work is valuable and largely successful. The tabulated timings (Table 2), explicit cloud exclusions, eye-versus-CMOS scatter, and regression statistics make the observational claim reproducible. The demonstration that a more ‘realistic’ elliptical correction need not improve c is pedagogically useful and well supported by the data and by Appleton’s earlier analysis. The archival GRS confirmation from the Roemer–Huygens correspondence is a genuine historical contribution. Strengths include transparent data reduction, period-comparable instrumentation, and an explicit didactic framing that links hypothesis, prediction, observation and alternative explanations.
major comments (2)
- [Abstract; §III; Table 6; §IV] Abstract and §III (‘Calculation knowing the “exact” value of the synodic period’): tephemeris = 152917.1 s is obtained by subtracting light-travel times that already assume the modern value of c from Stellarium/VSOP87 positions, then feeding that period into the slope fit that recovers c = (298200 ± 1900) km s⁻¹ (Table 6). The body text acknowledges the presumption (‘we now presume to know the speed of light’), but the Abstract and Conclusions present the figure as a determination of c from modern ephemerides. The result is properly a high-precision consistency check of the observers’ timings against known physics, not an independent first-principles measurement. The Abstract, the final paragraph of §III, and §IV should state this limitation explicitly and relegate the number to a test of observational quality.
- [§III (Elliptical orbits model; Variability of Io’s synodic period)] §III, uniform-circular and elliptical analyses: the paper correctly notes that other perturbations (Io–Europa–Ganymede resonance, inclination) remain after the ellipticity correction, yet it never quantifies their expected contribution over the 2023–24 window or shows residual O–C after the circular-model fit. A short residual table or a one-paragraph comparison with Appleton’s full perturbation budget would make the claim that ‘increasing complexity does not necessarily bring results closer to c’ fully load-bearing rather than qualitative.
minor comments (5)
- [§III] §III, paragraph beginning ‘Let’s start counting…’: typographical error ‘Juiter’ for ‘Jupiter’.
- [Table 2] Table 2: the ‘Difference with Stellarium’ row mixes signed means with standard deviations; a clearer caption stating that negative RF values mean earlier detection would help non-specialist readers.
- [Figures 2 and 4] Figure 2 versus Figure 4: the zero-point of Δt differs (first FF observation vs first of each series). A single sentence in each caption would prevent confusion when comparing slopes.
- [Tables 5–6] The weighted-average procedure that produces 267270 ± 870 km s⁻¹ (Table 5) and 298200 ± 1900 km s⁻¹ (Table 6) is not stated (inverse-variance?); one sentence would suffice.
- [References] Reference [24] citation form is incomplete (‘(n.d.)’); the Huygens Oeuvres volume and page already given earlier can be repeated for consistency.
Circularity Check
Headline c=(298200±1900) km/s is recovered only after defining Io’s synodic period by subtracting light-times that already use modern c; the uniform-circular ~10% result is not circular.
specific steps
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self definitional
[§III “Calculation knowing the ‘exact’ value of the synodic period”; Table 4 tephemeris; Table 6; Abstract]
"we now presume to know the speed of light and the exact positions of Jupiter (or Io) and Earth using the ephemeris given by Stellarium. In this way, observing and timing the ends of eclipses, we can calculate when Io emerged from Jupiter’s shadow by subtracting the times needed for light to travel from Io to Earth. These are the local (Jupiter) times of emersions. Using the first ... and last ... local times of emersions, and dividing this time interval by the 70 orbits ... we obtained for the synodic period of Io a value tephemeris=152917.1 s. We then used this tephemeris period to calculate"
tephemeris is defined by removing light-travel delays computed with the known modern c (t_local=t_obs−d/c). The subsequent slope fit of modern Δx against delays measured relative to that same tephemeris therefore returns essentially the input c by construction (exactly at the endpoints; to within timing noise for intermediate points). The abstract’s c=(298200±1900) km/s is this consistency check renamed as a measurement, not an independent determination of c from the observations alone.
full rationale
The paper’s central non-circular claim holds: with adopted modern orbital radii/periods, a uniform-circular model, and purely observed emersion times, the slope of Δx vs light-delay yields c within ~10% (Table 5) without feeding modern c into the fit. The elliptical-orbit correction likewise does not use c. The load-bearing circular step is confined to §III “Calculation knowing the ‘exact’ value of the synodic period” and Table 6. There the authors explicitly presume modern c, subtract d/c from the observed Earth times to obtain local (Jupiter) emersion times, extract tephemeris=(t_local,last−t_local,first)/70=152917.1 s, then re-insert that period into the same slope procedure and recover c=298200±1900 km/s. For the endpoints this recovery is forced by construction: the period was defined by removing exactly the light-time delays that the slope is asked to measure. The abstract and conclusions still advertise this figure as a “noticeably accurate result” of Roemer’s method with modern ephemerides, without restating the presumption of c. No self-citation or uniqueness-theorem circularity is present; the historical GRS archival claim is independent. Overall: partial circularity on the headline high-precision number only.
Axiom & Free-Parameter Ledger
free parameters (3)
- Regression slope for c (per observer series) =
FF 258800; PG 261900; RF 267670 km/s (circular); weighted ephemeris average 298200±1900 km/s
- Cloud-compromised timing exclusions =
2 of 18 listed timings excluded
- Mental-count stopwatch delay (eye runs) =
3–5 s procedural delay, not subtracted
axioms (5)
- domain assumption Earth and Jupiter may be modelled to first order as uniform circular orbits with modern semi-major axes and sidereal periods when estimating Δx and mean Io synodic period.
- domain assumption Stellarium VSOP87 ephemerides supply sufficiently accurate Earth–Jupiter distances and reference emersion geometry for the campaign window.
- ad hoc to paper Io’s average synodic period over the observing span can be taken from ephemeris local emersion times after removing light travel time.
- domain assumption First unambiguous visual or first-frame CMOS detection is an adequate operational definition of emersion for differential timing across months.
- domain assumption Standard Euclidean light-time delay Δt = Δx/c with constant c in vacuum is the correct physical model for the observed schedule shifts.
read the original abstract
350 years from the 1676 announcement of the Roemer's discovery that light propagates with finite speed, we present our observations using eyes with telescopes having similar resolution compared to those in the late 17th century. We confirmed that Roemer's method is valid and gives reasonable values for the speed of light c, within about 10 per cent of the modern value for our measurements, even with the simplest modelling technique, using uniform circular motions. We found that increasing the complexity of the model, e.g., by taking into account the elliptical orbit of Jupiter, does not necessarily bring the results closer to the value of c due to the influence of other perturbations. Using modern ephemerides yields a noticeably accurate result of c=(298200+-1900) km/s. This experience can have great didactic value by showing the interconnections between formulation of hypotheses and the consequent predictions, making observations, reducing data, and searching for alternative explanations for the same phenomenon. Lastly, we also found, in the correspondence between Roemer and Huygens, that Roemer in 1677 searched for an independent confirmation of what he found during previous years observing Io's eclipses by making observations and reducing the data of the meridian transits of the Great Red Spot on Jupiter.
Figures
Reference graph
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