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SCIENCE · INVESTIGATE AND EXPLAIN

Separate common calibration from scatter

Compare shared distance rescaling with wider conditional feasible bounds.

Learning outcome: Predict inverse slope scaling and distinguish feasibility from probability.

Starting recap

Changing an analysis assumption does not create new observations.

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Try

Multiplying all distances by 1.2 divides the central fitted slope by 1.2.

Open the experiment

Predict

Will wider distance bounds move the unchanged central fit?

Experiment

Compare baseline, distances 20% larger and wider distance bounds for D; calculate conditional interval endpoints.

Compare galaxy spectra, distance and expansion evidence

Fictional controlled comparisons · separate historical observations · Six original fictional records with artificial vacuum references. Low-redshift cz is a proxy, not an exact cosmological speed. Distance and peculiar-motion bounds are stipulated feasible ranges, not confidence intervals. A separate historical observed panel preserves all 24 raw Hubble 1929 Table 1 records. Neither fit is a current H0 estimate; Hubble time is not cosmic age.

Reset keeps your prediction, captures and practice history.

Original diagrams, not telescope images · same constructed galaxy, two viewsFace-on diskEdge-on diskHaloBulgeDiskStars, gas and dust occupy different distributions; dark matter is inferredfrom gravitational evidence. The dashed halo boundary is a layout guide.Unresolved spot: could be a star or a distant compact system. More evidence needed.

A galaxy is a gravitationally bound system of stars and other matter. Disk galaxies can include a central bulge and an extended halo; gas, dust and stellar populations need not share the same shape. Smooth elliptical and irregular appearances also occur. A viewing angle can change the appearance of one object without changing its physical identity. These schematic regions do not establish a galaxy's distance, age, stellar count or dark-matter distribution.

Try sketching the same disk from two directions, then list what a picture alone cannot determine. Morphological categories are not a universal evolutionary sequence. The NASA galaxy overview supplies background; the drawings here are original teaching constructions.

Controlled experiment: six fictional records

Selected D: Irregular. Appearance is supplied, not classified by the browser. All six records are original teaching cases. Selecting one highlights its evidence; it does not change the sample. The separate historical panel below supplies actual published observations.

The independent-method model distance is 40.00 Mpc and angular diameter is 15 arcseconds. With the small-angle local approximation, projected diameter is 2.90888 kpc. Mpc means million parsecs; kpc means thousand parsecs. One arcsecond is 1/3600 of a degree. These deliberately equal-size examples do not establish a real standard ruler.

Fictional virtual features · vacuum nm · no real element identificationReferenceRaw recordCorrectedLamp knownLamp raw400450500550600650Both lamps imply raw minus known = +2 nm. Subtract 2 nm to correct.Current analysis uses corrected wavelengths.
Selected virtual features; z = used wavelength / reference − 1
Reference nmRaw nmCorrected nmUsed nmFractional shift z
400406.002769404.002769404.0027690.010006923
500507.003461505.003461505.0034610.010006923
600608.004154606.004154606.0041540.010006923

Consistent virtual-line shifts under the selected calibration; fictional local approximation. Accepted common z: 0.010006923; accepted cz proxy: 3000.000 km/s. The 10⁻¹⁰ consistency tolerance suppresses arithmetic noise in exact constructed lines; it is not instrument precision or a confidence interval.

Fictional controlled comparison · cz proxy (km/s), not exact cosmological speedHorizontal bars: stipulated distance bounds · square: selected · circles: other records01000200030004000500060006500ABCDEF020406080100110Independent-method model distance (Mpc)Fixed axes for every analysis case. No synthetic point is an observed galaxy.
Full six-record sample; intervals are conditional feasibility bounds, not probabilities
RecordDistance MpcDistance bounds MpcAccepted cz km/scz/d (km/s/Mpc)Residual km/sFeasible H km/s/Mpc
A5.004.50–5.5050.00010.000-303.0930.000–77.778
B10.009.00–11.001000.000100.000293.81463.636–144.444
C20.0018.00–22.001100.00055.000-312.37136.364–77.778
D (selected)40.0036.00–44.003000.00075.000175.25861.364–91.667
E60.0054.00–66.004000.00066.667-237.11356.061–79.630
F80.0072.00–88.005800.00072.500150.51562.500–84.722

Descriptive slope H = 70.61856 km/s/Mpc. The calculation minimizes unweighted squared proxy residuals while forcing zero intercept. It is not an errors-in-variables analysis or a modern H₀ estimate. Wider bounds leave the central fit unchanged; multiplying all distances by 1.2 lowers the fitted slope by 1/1.2. A calibration change is not a new independent sample.

Connect the local approximation and conditional bounds

For each identified virtual feature, z = λused/λreference − 1. Multiplying by c = 299792.458 km/s expresses redshift as a proxy cz. The approximation cz ≈ Hd + u includes a prescribed line-of-sight peculiar-motion term u. It omits relativistic cross terms and distinctions between distance definitions. Neither cz as a speed nor cz/H as a distance is generally valid at high redshift without more cosmological assumptions.

The fitted slope is Σ(d × cz)/Σd²; Σ means add over all six records. The stated distance bounds and |u| ≤ 300 km/s give, for these positive proxies, Hlow = max(0, (cz − 300)/dhigh) and Hhigh = (cz + 300)/dlow. This is compatibility with rectangular assumptions and H ≥ 0, not a probability statement. No observational error bars are inferred from decimal precision.

Projected diameter in kpc ≈ 1000 × distance in Mpc × angular diameter in arcseconds / 206264.806. This uses the small-angle approximation and local angular-diameter distance. The distance and angular-size calculation remains available even when spectral inference fails.

For purely cosmological redshift of comoving sources, 1 + zcos = aobserve/aemit, where a is cosmic scale factor. A measured redshift may contain peculiar motion and other contributions, so this exercise's mixed proxy does not uniquely measure that scale-factor ratio.

Inspect how the fictional sample was constructed

The six central proxies were prescribed as 70 × distance plus offsets −300, +300, −300, +200, −200 and +200 km/s. These offsets are not random draws or population statistics. The model distances were supplied independently of the resulting proxies. Artificial references at 400, 500 and 600 nm are multiplied by 1 + z, then a +2 nm instrument offset is added. All six angular sizes were chosen to give the same nominal projected diameter. These choices teach controlled comparisons; they do not measure real expansion.

Observed reference: Hubble's 1929 Table 1

These 24 published historical distance–velocity pairs are observations, separate from the fictional calibration experiment. Its controls do not alter this panel. Distances use the obsolete historical calibration; velocities are the table's measured values before the fitted solar-motion correction used in the paper's Figure 1. These descriptive fits are neither a reproduction of that corrected figure nor a modern expansion measurement.

Actual historical records · outdated distance scale · uncertainties unavailableVelocity (km/s) · circle: other objects; diamond: common-distance Virgo groupSolid: through origin · dashed: free intercept · neither fit is current H₀-3000300600900120000.511.52Historical distance (million parsecs, numerically Mpc)No invented error bars. Nearby negative velocities coexist with the overall pattern.Full records below include identifiers and every published distance/sign.
All 24 original Table 1 pairs; uncertainty unavailable, not zero
ObjectHistorical distance MpcMeasured velocity km/sGroup note
Small Magellanic Cloud0.032170—
Large Magellanic Cloud0.034290—
NGC 68220.214-130—
NGC 5980.263-70—
NGC 2210.275-185—
NGC 2240.275-220—
NGC 54570.45200—
NGC 47360.5290—
NGC 51940.5270—
NGC 44490.63200—
NGC 42140.8300—
NGC 30310.9-30—
NGC 36270.9650—
NGC 48260.9150—
NGC 52360.9500—
NGC 10681920—
NGC 50551.1450—
NGC 73311.1500—
NGC 42581.4500—
NGC 41511.7960—
NGC 43822500Common Virgo distance
NGC 44722850Common Virgo distance
NGC 44862800Common Virgo distance
NGC 464921090Common Virgo distance
Fits describe this historical table; units km/s per historical Mpc
DescriptionSlopeIntercept km/s
All 24, forced through origin423.937320 imposed
All 24, fitted intercept454.15844-40.78365
Grouping sensitivity: omit four Virgo rows446.352010 imposed

The full sample remains the default evidence. The four common-distance objects are not automatically four independent distance calibrations. The disclosed omission is a sensitivity comparison, not a way to choose a preferred result. Neither fit models distance error, sample selection or the author's solar-motion solution.

Reproduce the historical arithmetic and provenance

For distance r and velocity v, the through-origin descriptive slope is Σrv / Σr². Here n = 24, Σr = 21.873, Σv = 8955, Σr² = 29.517795 and Σrv = 12513.695. Each Σ means add over all rows. Dividing 12513.695 by 29.517795 gives about 423.9373. A free-intercept line also estimates where the line crosses the velocity axis; changing that assumption changes its slope.

Table 1 used stellar/luminosity distance criteria; Table 2 instead inferred distances from velocity and is excluded. Using the latter to verify the same velocity–distance relation would be circular. The table is not a random, volume-complete survey. Scatter and missing individual error estimates limit inference.

Primary scan, printed page 169 · Original paper DOI. Retrieved 2026-10-26. The numerical transcription preserves every row and sign; normalized identifiers replace historical typography. Local record SHA-256: c7d41a68838eec76e7bcb539c77f2db39a28aa304cd8d376b86abce84c746ff5.

Calculate Hubble time without claiming cosmic age

For a hypothetical present rate of 70 km/s/Mpc, 1/H corresponds to 13.96846 Gyr using 1 Mpc = 3.085677581491367 × 10¹⁹ km and a Julian year of 31557600 seconds. This is Hubble time, not the age of the universe. A present rate does not determine the past expansion history. Neither these six fictional cases nor the historical table establishes dark energy, a cosmic edge, a privileged center or the entire Big Bang model.

For scale-factor and distance definitions, see Hogg's redshift derivation. Bound galaxies and solar systems do not simply grow according to the background expansion relation.

Fictional six-record descriptive slope 70.6186 km/s/Mpc; selected galaxy D has z=0.0100069.

Consistent virtual-line shifts under the selected calibration; fictional local approximation. Independent-distance angular-size estimate 2.9089 kpc. Historical observations are a separate fixed dataset; uncertainty envelopes are conditional, not probabilities.

Captures preserve the fictional galaxy selection and analysis assumptions. Historical observations remain fixed. Replay supplies conditional comparisons, not new observations or a current expansion-rate measurement.

Understand

Distinguish a common scale from wider uncertainty

A distance calibration can shift every inferred distance together. An uncertainty bound can widen without moving the central estimate. These are different changes, and neither creates a fresh set of observed galaxies. Predict their effects before using the analysis-case selector.

Start with Calibrated wavelengths; baseline distances. Keep galaxy D highlighted while all six rows remain in the fit. Its central distance is 40 Mpc, its redshift proxy is 3000 km/s and its baseline distance bounds are 36–44 Mpc. The bounds are stipulated teaching assumptions, not observational confidence intervals.

Rescale all distances together

Switch to Calibrated wavelengths; distances 20% larger. D moves to central distance 48 Mpc, with bounds 43.2–52.8 Mpc. The spectra, redshifts and angular diameters do not change. The experiment changes a shared distance-calibration assumption, not the physical galaxies during a click.

Let s denote a common distance multiplier. The through-origin fit is sum(d × cz)/sum(d²). Multiplying every d by s multiplies its numerator by s and its denominator by s², so the fitted slope divides by s. For s = 1.2, baseline 70.618557 becomes approximately 58.848797 km/s/Mpc.

On paper compare dividing by 1.2 with subtracting 20 percent. The former gives about 83.33 percent of the original slope, not 80 percent. Capture baseline and rescaled cases and write which raw evidence stayed fixed. Treating the rescaled rows as independent observations would count the same information twice.

Widen bounds without moving the central fit

Return to baseline, then choose Calibrated wavelengths; wider distance bounds. D still has central distance 40 Mpc, but bounds widen to 32–48 Mpc. The central six-point slope remains approximately 70.619 because neither central distances nor cz values changed.

The exercise also stipulates a local-motion bound of magnitude at most 300 km/s. Its local relation is cz = Hd + u, where H is nonnegative and u is the unknown bounded contribution. For positive cz in these records, feasible H runs from max(0, (cz − 300)/dhigh) to (cz + 300)/dlow.

With D’s baseline bounds, calculate lower 2700/44 ≈ 61.364 and upper 3300/36 ≈ 91.667 km/s/Mpc. With wider bounds the endpoints become 2700/48 = 56.25 and 3300/32 = 103.125. These ranges describe compatibility with rectangular assumptions. They do not mean a stated probability that the real Hubble constant lies inside them.

Compare fractional sensitivity and real uncertainties

For nearby A, the lower numerator is negative and the H ≥ 0 condition clips the lower bound to zero. Its baseline feasible range is 0–77.778. For F the range is approximately 62.5–84.722. The same local-motion bound has different relative importance. Do not use the positive-cz shortcut unquestioningly for a new negative record.

Hogg’s cosmographic discussion supplies broader definitions; the lab remains a first-order local exercise. It omits spectral noise and a full correlated statistical model. The unweighted central fit is not an errors-in-variables inference.

Keep the historical Hubble panel separate: its unavailable uncertainties are not replaced by our fictional ten-percent bounds. Likewise, the published NGC 4258 maser distance has distinct statistical and systematic terms. A common calibration effect does not generally disappear by averaging more objects. Do not combine those terms or assign a confidence level without a justified statistical contract.

Transfer: recalibrate downward

An unfamiliar method revises every central distance downward by ten percent while leaving redshift estimates unchanged. Predict the new slope multiplier. Explain whether that recalibration gives another independent sample or a probability interval.

Check the distance-uncertainty transfer

The distance multiplier is 0.9, so the slope multiplier is 1/0.9, approximately 1.1111. The increase is about 11.11 percent, not exactly ten percent. It is a common recalibration of the same sample, not new independent observations or a confidence statement.

Apply

The displayed feasible H ranges are:

Public practice checks a specific claim. It does not establish independent mastery.

Distinguish common systematic effects, central estimates and nonprobabilistic feasible bounds.

Continue

Completion requires a saved prediction, at least one capture and a reflection. Presence checks do not grade your reasoning.

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