BABYLONTHE LEARNING CENTREThe encyclopedia
BABYLON · EARTH EVIDENCE EXPLORER

Above us.
Beneath us.
How do we know?

Explore Earth’s layers through the measurements that reveal them. Begin with an actual balloon profile and an earthquake recorded around the world.

01 · MEASURE02 · INTERPRET03 · CROSS-CHECK

A sample, an instrument reading and an inferred structure answer different questions. Follow each connection back to the record.

A CROSS-SECTION YOU CAN QUESTION

Choose a layer. Open its evidence.

Above the surface

Below the surface

Illustrative Earth cross-section and expanded atmosphereNested interior regions and atmospheric arcs. The nearby buttons select a layer. Atmosphere and crust are enlarged for readability; boundaries are schematic.CrustMantleOuter coreInner coreAtmosphere and crust enlarged · not to scaleSelect a named layer to follow its evidence
Thermal atmosphere and compositional interior shown together schematically. The ionosphere overlaps thermal layers.
Above EARTH · Instruments carried through the air

Troposphere

Surface to roughly 12 km; varies with latitude and weather

Dense air, water vapour and suspended particles.

This is the lowest thermal layer, where most weather occurs. Its upper boundary is defined from atmospheric temperature structure, not from a solid surface.

What the measurements address
Balloon sensors report pressure and temperature as they rise. The Tateno pilot lets you inspect an actual vertical profile.
What this pilot checked
104 reported levels in one sounding; 16 have both temperature and geopotential height.
What remains open
This one ascent does not measure global gas composition, every cloud or the whole atmosphere.
A useful next test
Repeat with other dates and stations; check where the temperature gradient changes before labelling a local tropopause.
Read all nine layer notes
Above EARTH · Instruments carried through the air

Troposphere

Surface to roughly 12 km; varies with latitude and weather

Dense air, water vapour and suspended particles.

This is the lowest thermal layer, where most weather occurs. Its upper boundary is defined from atmospheric temperature structure, not from a solid surface.

What the measurements address
Balloon sensors report pressure and temperature as they rise. The Tateno pilot lets you inspect an actual vertical profile.
What this pilot checked
104 reported levels in one sounding; 16 have both temperature and geopotential height.
What remains open
This one ascent does not measure global gas composition, every cloud or the whole atmosphere.
A useful next test
Repeat with other dates and stations; check where the temperature gradient changes before labelling a local tropopause.
Above EARTH · Atmospheric profiles and optical measurements

Stratosphere

Roughly 12–50 km; boundaries vary

Thin air containing ozone and, at times, volcanic aerosols.

A thermal region in which temperature generally increases with height. Different instruments are needed to distinguish temperature, ozone and aerosol extinction.

What the measurements address
Radiosondes sample temperature and pressure; lidar and spectroscopy address particles and gases.
What this pilot checked
The Tateno height–temperature pairs reach 30.75 km geopotential height. Our separate 1982 study reviews historical aerosol lidar.
What remains open
This sounding contains no ozone profile or aerosol concentration. It cannot establish a volcanic effect by itself.
A useful next test
Align dated ozone/aerosol observations and wavelengths with the light path being tested.
Above EARTH · Research measurements beyond this pilot

Mesosphere

Approximately 50–80 km in the linked overview

Very thin atmospheric gases.

A thermal layer in which temperatures generally fall with height. Its name describes a region of gas.

What the measurements address
Sounding rockets and remote sensing extend coverage above ordinary balloon profiles.
What this pilot checked
The overview is reviewed; the Tateno pilot does not reach this layer.
What remains open
No original mesospheric measurement series is analysed here yet.
A useful next test
Choose a specific rocket or occultation dataset, verify altitude calibration and compare independent methods.
Above EARTH · Remote and in-situ upper-atmospheric measurements

Thermosphere

Approximately 80–700 km; strongly variable

Extremely sparse gases, with substantial ionization in overlapping regions.

Thermal and electrical classifications overlap. The ionosphere is not a separate solid shell stacked above this thermal layer.

What the measurements address
Particle measurements, spectroscopy and radio propagation respond to different properties.
What this pilot checked
Thermal and ionospheric explanations are linked; no original upper-atmosphere series is analysed in this pilot.
What remains open
A high particle temperature is not the same as the heating a person would feel in dense air.
A useful next test
Compare neutral density, electron density and temperature with their own units and instrument responses.
Above EARTH · Particle and light measurements interpreted with models

Exosphere

Outermost atmospheric region; no sharp universal top

Exceptionally sparse particles, including light gases.

The outer atmosphere becomes increasingly sparse. A conventional space boundary is not a detected material ceiling.

What the measurements address
Remote light measurements and spacecraft instruments constrain particle distributions.
What this pilot checked
A source-led explanation only; no original exospheric particle series analysed here.
What remains open
No single altitude is a fixed upper edge of every atmospheric component.
A useful next test
Specify the gas, detection threshold and instrument before asking where that component ends.
Below EARTH · Accessible samples plus geophysical inference

Crust

Variable thickness; oceanic and continental crust differ

Solid rock with different mineral and chemical compositions.

Outcrops and boreholes give physical samples. Locating the crust–mantle boundary at a particular place also requires geophysical evidence.

What the measurements address
Rock chemistry, field relationships, drilling and seismic changes constrain different aspects.
What this pilot checked
USGS explanatory sources reviewed. This explorer does not yet contain an original rock chemistry or borehole dataset.
What remains open
A surface sample does not identify every material at depth. Chemical crust and mechanical lithosphere are different concepts.
A useful next test
Choose one named borehole or rock specimen and align its laboratory record with local seismic observations.
Below EARTH · Multiple geophysical and laboratory constraints

Mantle

Below the crust to about 2,900 km depth

Predominantly solid silicate rock, able to deform slowly; local partial melting occurs.

Slow flow over geological time is compatible with rock transmitting seismic shear waves. The mantle is not a global ocean of liquid magma.

What the measurements address
Seismic velocities, mineral experiments at pressure, transported rock samples and heat-flow constraints contribute.
What this pilot checked
One earthquake’s catalogued arrival picks are available below, plus the USGS explanation. No mantle inversion or mineral experiment is reproduced here.
What remains open
Composition and temperature cannot be read directly from a single arrival-time curve.
A useful next test
Compare many paths and events, then check candidate mineral properties against laboratory data.
Below EARTH · Strong inference from converging measurements

Outer core

Below the mantle, surrounding the inner core

Liquid, predominantly iron alloy; lighter-element composition remains a research question.

The liquid interpretation is supported by seismic propagation and other physical constraints. It is not a retrieved sample of core material.

What the measurements address
Core-sensitive compressional phases, lack of ordinary shear transmission through liquid, rotation, magnetic field and laboratory properties.
What this pilot checked
The pilot includes catalogued PKP-family arrivals. A phase name already contains an interpretation; raw waveforms are the next check.
What remains open
This P-dominated product cannot be used as an independent demonstration that S waves are absent.
A useful next test
Recover waveforms and responses, compare predicted phase travel times and use events not used for fitting.
Below EARTH · Seismic and physical inference

Inner core

Central region; radius roughly 1,200–1,250 km

Solid, predominantly iron alloy in the standard model.

Deep interior structure is inferred from how signals travel, supported by other constraints. A cross-section is a model representation, not a photograph.

What the measurements address
Core-sensitive seismic phase behaviour and high-pressure material experiments.
What this pilot checked
The selected catalogue labels PKPdf arrivals; we have not independently verified those phase identifications or reconstructed the inner core.
What remains open
Fine structure, temperature and alloy composition need additional data and modelling.
A useful next test
Compare multiple phase branches, directions and earthquakes; examine whether alternative models explain them together.
ONE REAL PROFILE · TATENO, JAPAN

A journey through the air.

The archived profile is labelled 11 March 2011, nominal 00:00 UTC. Its release field says 23:30, interpreted here as the preceding UTC date. This is not a simultaneous column: the instrument ascends over time and drifts horizontally.

104reported levels
16height–temperature pairs
30.75 kmhighest paired geopotential height
Dots are reported pairs; no missing height is estimated. Geopotential height is not identical to geometric altitude. The chart does not measure atmospheric composition.

Missing values are kept missing. A/B flags record different climatological checks; a blank flag is not proof that a value is absent.

Inspect all 104 reported levels and flags
Tateno · nominal 2011-03-11 00 UTC · selected reported fields
LevelPressure hPaHeight m geopotentialTemperature °CFlags P / height / T
11013.0Missing4.6B / blank / B
21000.0128.02.8blank / B / B
3998.0Missing2.6blank / blank / B
4988.0MissingMissingblank / blank / blank
5985.0Missing3.4blank / blank / B
6925.0756.0-0.3blank / B / B
7905.0MissingMissingblank / blank / blank
8868.0Missing-3.9blank / blank / B
9850.01426.0-5.5blank / B / B
10827.0MissingMissingblank / blank / blank
11747.0Missing-14.5blank / blank / B
12746.0MissingMissingblank / blank / blank
13737.0MissingMissingblank / blank / blank
14710.0MissingMissingblank / blank / blank
15700.02911.0-17.9blank / B / B
16628.0MissingMissingblank / blank / blank
17624.0Missing-23.9blank / blank / B
18616.0Missing-22.9blank / blank / B
19605.0Missing-22.5blank / blank / B
20584.0MissingMissingblank / blank / blank
21542.0MissingMissingblank / blank / blank
22500.05360.0-32.3blank / B / B
23441.0Missing-39.3blank / blank / B
24432.0Missing-40.1blank / blank / B
25424.0MissingMissingblank / blank / blank
26400.06900.0-41.3blank / B / B
27367.0Missing-43.5blank / blank / B
28364.0Missing-42.7blank / blank / B
29353.0MissingMissingblank / blank / blank
30301.0MissingMissingblank / blank / blank
31300.08830.0-47.5blank / B / B
32298.0Missing-47.7blank / blank / B
33294.0Missing-47.1blank / blank / B
34281.0MissingMissingblank / blank / blank
35265.0Missing-50.9blank / blank / B
36261.0MissingMissingblank / blank / blank
37250.010020.0-48.3blank / B / B
38224.0Missing-46.1blank / blank / B
39212.0MissingMissingblank / blank / blank
40200.011500.0-48.1blank / B / B
41184.0MissingMissingblank / blank / blank
42173.0Missing-53.7blank / blank / B
43169.0MissingMissingblank / blank / blank
44156.0Missing-51.1blank / blank / B
45151.0MissingMissingblank / blank / blank
46150.013370.0-51.5blank / B / B
47112.0MissingMissingblank / blank / blank
48100.015970.0-55.5blank / B / B
4976.5MissingMissingblank / blank / blank
5075.1Missing-58.1blank / blank / B
5173.6MissingMissingblank / blank / blank
5270.8MissingMissingblank / blank / blank
5370.018230.0-55.5blank / B / B
5466.4MissingMissingblank / blank / blank
5565.2Missing-53.5blank / blank / B
5660.2MissingMissingblank / blank / blank
5754.8Missing-59.9blank / blank / B
5852.1MissingMissingblank / blank / blank
5951.0Missing-58.9blank / blank / B
6050.2Missing-56.1blank / blank / B
6150.020370.0-56.1blank / B / B
6248.0MissingMissingblank / blank / blank
6347.2Missing-58.5blank / blank / B
6444.8MissingMissingblank / blank / blank
6542.9MissingMissingblank / blank / blank
6641.5MissingMissingblank / blank / blank
6741.0Missing-52.5blank / blank / B
6840.1MissingMissingblank / blank / blank
6937.2MissingMissingblank / blank / blank
7034.0Missing-56.3blank / blank / B
7133.5MissingMissingblank / blank / blank
7231.6MissingMissingblank / blank / blank
7331.2MissingMissingblank / blank / blank
7430.5Missing-52.7blank / blank / B
7530.023630.0-53.1blank / B / B
7629.3MissingMissingblank / blank / blank
7727.2MissingMissingblank / blank / blank
7826.2MissingMissingblank / blank / blank
7924.6MissingMissingblank / blank / blank
8023.6MissingMissingblank / blank / blank
8121.6MissingMissingblank / blank / blank
8221.4Missing-50.7blank / blank / B
8321.2MissingMissingblank / blank / blank
8420.7MissingMissingblank / blank / blank
8520.2MissingMissingblank / blank / blank
8620.026260.0-51.5blank / B / B
8719.5MissingMissingblank / blank / blank
8818.9MissingMissingblank / blank / blank
8918.3MissingMissingblank / blank / blank
9015.4MissingMissingblank / blank / blank
9115.2Missing-55.5blank / blank / B
9214.9MissingMissingblank / blank / blank
9314.7Missing-52.3blank / blank / B
9414.2MissingMissingblank / blank / blank
9513.4MissingMissingblank / blank / blank
9611.5Missing-50.3blank / blank / B
9711.2Missing-50.9blank / blank / B
9810.9MissingMissingblank / blank / blank
9910.4MissingMissingblank / blank / blank
10010.030750.0-49.5blank / B / B
1019.7Missing-50.3blank / blank / B
1028.9Missing-45.1blank / blank / A
1037.7MissingMissingblank / blank / blank
1047.2Missing-40.1blank / blank / A

Reported geopotential heights are not geometric altitudes. Variable-pressure levels often lack height. Missing and QA-removed values become null, never zero. No intermediate height is invented; gaps between plotted levels are not new observations. Header coordinates are fixed-station catalogue coordinates, not a reconstructed balloon trajectory. No chemical composition or aerosol concentration is measured by this extract.

ONE EARTHQUAKE · MANY STATIONS

Listen through the ground.

The 2011 Great Tōhoku earthquake is catalogued at magnitude 9.1, with preferred origin time 05:46:24.120 UTC on 11 March. The selected reviewed product associates 657 arrival picks with that origin. Its reported depth is 29 km and is explicitly marked operator assigned. The assignment flag does not explain which constraints were used to choose the depth. The origin time, location and phase identifications are analysis outputs; they are not all direct instrument readings.

657associated arrival picks
541positive-weight arrivals
116zero-weight arrivals retained
Recorded pick time minus inferred origin time, versus catalogued angular distance. This is an arrival-time plot, not a raw waveform or a reconstruction of Earth’s interior.

657 associated arrivals

What do the phase labels mean?

P denotes compressional propagation; Pn a regional mantle-refracted branch; Pdif denotes diffraction near the core–mantle boundary. PKP-family labels describe interpreted paths involving the outer core; the df branch traverses the inner core. These are catalogue classifications to verify against waveforms, not material samples. The source spells the diffracted branch “Pdif”; we preserve that spelling.

This product is dominated by P-family picks. Its absence of S entries cannot by itself demonstrate a liquid outer core. Zero-weight picks are visible by default as outlined points. A zero catalogue weight does not mean the instrument recorded nothing.

These are catalogue picks associated with one preferred origin, not raw waveforms. Phase labels, distances, origin and residuals depend on catalogue analysis. Zero-weight picks remain present and are visibly distinct. Missing S picks in a P-dominated compilation do not demonstrate absence of S waves. Arrival count, distinct station labels and the origin reported station count are different fields. One earthquake does not independently establish core composition or reconstruct every interior layer.

HOW STRUCTURE BECAME HISTORY

Materials gather. Layers develop.
Rocks preserve clocks.

01 · ACCRETION

Building a planet

Material accumulated into larger bodies. Planet-formation models connect this process to evidence from meteorites and observations of young systems.

02 · DIFFERENTIATION

Separating materials

Heating and material properties allowed metal and silicate reservoirs to separate. That history is constrained through chemistry, physical experiments and models.

03 · DATING

Reading a mineral’s clock

Isotope ratios can constrain when a mineral formed or its isotope system was last reset. A mineral’s age and Earth’s formation age are different propositions.

Explore a clock’s behaviour

Illustration: uranium-235 remaining after a chosen time, using a 0.704-billion-year half-life. This is a decay calculation, not a new date measured from a sample.

100% of the original parent isotope remains at the start.

Fraction remaining = 2−time / half-life. Dating an actual specimen also requires measured isotope ratios, initial daughter constraints, contamination checks and assessment of whether the system stayed closed. The commonly estimated planetary age is about 4.54 billion years; this pilot has not independently reproduced a laboratory age.

MAKE THE CLAIM TESTABLE

Three witnesses to the same question.

For an interior claim, seismic behaviour, material experiments and gravity or rotation can supply different constraints. Three websites repeating one catalogue do not create three independent measurements. The two datasets here are introductory examples; their dates do not establish an atmosphere–earthquake connection.

State a prediction

What should an instrument record if the proposed layer or material exists? Give a location, depth or altitude, units and expected behaviour.

Compare alternatives

Would different materials or structures produce the same reading? Include instrument limitations and the established explanation in the comparison.

Check another method

Seek observations with different instruments and failure modes, then test predictions on records not used to fit the explanation.

If the question is a physical firmament

Specify its proposed material, altitude, extent and interactions with light, radio waves and objects. A material surface would need evidence distinguishing it from refracting gases, clouds and ionized plasma. Current atmospheric evidence supports an atmosphere that thins with height; this pilot supplies no evidence of a solid ceiling. A theological meaning and a physical material claim require different kinds of argument.

What would deepen this explorer?

  1. Retrieve original seismic waveforms, instrument responses and station metadata for selected arrivals, then verify phase picks.
  2. Compare additional earthquakes across different paths and hold out events from any model fitting.
  3. Add a named rock or borehole record with specimen identity and laboratory measurements.
  4. Add original ionosonde and particle-density records above balloon range.
  5. Add original isotope measurements and their uncertainty before reproducing a geological age.

These tasks remain open. No new interior inversion, global atmospheric reconstruction or geological date is claimed.

Follow the original records.

Reviewed 11 November 2026. Public observations, catalogue interpretations and explanatory references have separate roles.

  1. NOAA NCEI · IGRA station archive ↗

    One 104-level profile extracted from the station period-of-record file, nominal 2011-03-11 00 UTC. Original archive preserved privately; bounded profile extract published.

  2. NOAA · IGRA record format ↗

    Fixed-width units, missing values and processing flags used in extraction. A/B flags describe different climatological checks; blank does not mean unmeasured.

  3. NOAA · IGRA station metadata ↗

    Station identity and current catalogue coordinates; historic station location changes were not reconstructed.

  4. USGS · 2011 Great Tōhoku earthquake ↗

    Preferred event/origin metadata. The event is Mw 9.1; the selected phase product is a later reviewed catalogue product, not a contemporaneous raw recording.

  5. USGS · reviewed QuakeML phase product ↗

    657 associated arrivals, retained with original phase names, weights, pick UTC and residuals. Preferred origin depth is explicitly operator assigned.

  6. USGS · The Interior of the Earth ↗

    Historical explanatory overview of the combined seismic, gravity, magnetic, heat-flow and laboratory evidence. Not a raw dataset; older illustrative estimates require context.

  7. USGS · Inside the Earth ↗

    Crust, mantle, liquid outer core and solid inner core; mechanical lithosphere and asthenosphere are a different classification. Educational synthesis, not independent raw evidence.

  8. NASA · thermal layers of the atmosphere ↗

    Approximate, variable thermal layer ranges for the schematic. No sharp universal upper atmospheric surface is defined.

  9. NOAA · ionosphere ↗

    Charged particles and radio propagation; an overlapping electrical region rather than another solid or thermal shell.

  10. NASA · A Rocky Planet Forms ↗

    Accretion and differentiation as a formation explanation. Educational model, not a measurement made by this explorer.

  11. NIST · how radiometric dating works ↗

    Isotope decay and the approximate 4.54-billion-year planetary age. Slider is an illustration; no original laboratory isotope measurements analysed here.

  12. EarthScope · seismic data access ↗

    Next route to original waveforms and station responses. A free account may be needed; raw waveforms not downloaded in this pilot.

Learning in the Light

In Babylon, the Father’s light opens perspective, learning and a chosen next step. Your worth remains intact. Every person is sovereign, with dignity, freedom and room to grow.

Read the learning principle ↗

Follow Apollo 11 from launch to return

Compare the atmosphere, engine burns, outside radio observations and return engineering, with calculations, documented findings and an eight-track investigation map.

Follow Apollo 11 from launch to return ↗

Follow Starship Flight 4 through two returns

Compare the operator account, dated FAA records and outside infrasound observations, with a propagation-delay lesson and explicit research gaps.

Follow Starship Flight 4 through two returns ↗