← Return to Before Names

Astronomy & references

Ten worlds, their measured astronomical settings, and the evidence behind each chapter. Numerical values retain the saved NASA snapshot; later papers are not silently substituted for its measurements.

Ten independently prompted illustrations depict six planetary surfaces and four explicitly invented moons, anchored to ten catalogued planets in nine host systems. Full-resolution originals live in World Images. Every scene has an image science companion, a registry assignment and a chapter. “Prehistoric” means an imagined world before recorded history; these are not reconstructions of discovered alien fossils.

Numerical properties are frozen from the NASA Exoplanet Archive composite snapshot retrieved 25 September 2026. Different parameters can come from different source papers and do not form a single self-consistent model. The companion pages retain source-specific errors, upper or lower limits and calculated-value provenance. Equilibrium temperature is not surface temperature; unknown is not zero.

Kepler-62 e and f have catalog mass upper limits, not those exact measured masses. Kepler-442 b and TOI-700 d have mass–radius-derived mass entries. HD 28185 b has a minimum mass and calculated radius. No scene uses those uncertain values as a measured gravity to certify giant animals. LHS 1140 b has measured central mass 5.6 Earth masses and radius 1.73 Earth radii: g/gEarth = 5.6/1.73² ≈ 1.87, a central estimate without uncertainty propagation.

For a spherical object of radius R at observer distance d, angular diameter is 2 asin(R/d). An invented Moon-sized body with R = 1,737 km gives approximately 4.98° at 40,000 km and 3.98° at 50,000 km. These distances illustrate a visual concept; they are not satellite detections, orbital-stability results or forecasts of tidal height. The Moon formed closer to Earth; the extreme early-Moon sky is not a reconstruction of Earth’s dinosaur era. The present recession rate must not be extrapolated unchanged through geological time.

The four satellite scenes assign images to their real parent planets: Kepler-16 b, Kepler-47 c, Kepler-1647 b and HD 28185 b. All satellite sizes, masses, orbits, atmospheres, histories and ecologies are invented. Their huge sky objects are the parent planets, not additional nearby confirmed worlds. Rings are invented only for the HD 28185 b scene. Gas-rich planets are never given ordinary exposed ground.

Binary systems support two real stellar sources, but sky position, apparent separation, phase and shadow geometry require an orbital model not supplied here. Catalog incident flux entries for binaries may not describe the time-varying combined irradiation; this book does not use them as complete climate budgets. Single-star nominal angular sizes use saved central stellar radii and orbital distances. The artwork is not a calibrated sky, and visual-review notes identify departures from prompt targets.

Each body plan was designed independently: an open body ring, a blade comb, many joined chambers, a deformable torus, an aquatic lattice, a mobile pleated fan, thermal bellows, an aerial chambered body, a radial strider and a perforated sheet. Proposed feeding, transport, sensing and locomotion mechanisms are fiction. No physiology, gravity, ecosystem, climate, lifting-gas budget or structural calculation proves that these giant forms could survive. Their colors and scale are creative choices.

The jacket reuses the opening scene with live typographic layout; it is not an eleventh world. The reader works offline, supports keyboard navigation, searchable contents, saved position, adjustable text, full-screen artwork with zoom, and printing of every chapter. Public copies use bounded WebP derivatives. This local build does not publish the site.

1. The open-bodied titans

Kepler-62 f · Kepler-62 · Transit

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period267.291 ± 0.005daysBorucki et al. 2013
Planet radius1.41 ± 0.07Earth radiiBorucki et al. 2013
Planet mass; provenance below< 35 (upper limit)Earth massesBorucki et al. 2013
Planet orbital semi-major axis0.718 ± 0.007AUBorucki et al. 2013
Catalog incident flux0.5 (meaningful uncertainty not supplied)Earth fluxFulton & Petigura 2018
Star effective temperature; catalog entry4925 ± 70KBorucki et al. 2013
Star radius; catalog entry0.64 ± 0.02Solar radiiBorucki et al. 2013
System distance300.874 ± 1.219parsecsTICv8

Mass constraint; preserve any upper/lower limit indicated in the table. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Borucki, W. J., et al. (2013). Kepler-62: A five-planet system with planets of 1.4 and 1.6 Earth radii in the Habitable Zone. Science, 340, 587–590.

    Discovery, orbital periods, planet radii and stellar parameters; does not establish surfaces or life.

  3. NASA · Formation of the Moon

    Supports astronomical context; does not establish the illustrated biology or environment.

  4. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

Open-bodied adult and smaller juvenile; continuous sensory pits and hanging feeding veils are visible. Peripheral supports overlap, so the exact designed limb count is not recoverable. One small host and one large left-lit fictional moon. Disk size is illustrative, somewhat larger than the nominal prompt target; tides and support mechanics are not modeled.

2. The walking weather-combs

Kepler-442 b · Kepler-442 · Transit

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period112.3053 (+0.0024 / −0.0028)daysTorres et al. 2015
Planet radius1.34 (+0.11 / −0.18)Earth radiiTorres et al. 2015
Planet mass; provenance below2.36 (meaningful uncertainty not supplied)Earth massesCalculated Value
Planet orbital semi-major axis0.409 (+0.209 / −0.06)AUTorres et al. 2015
Catalog incident flux0.66 (+0.23 / −0.41)Earth fluxTorres et al. 2015
Star effective temperature; catalog entry4402 ± 100KTorres et al. 2015
Star radius; catalog entry0.598 (+0.023 / −0.024)Solar radiiTorres et al. 2015
System distance365.965 (+2.763 / −2.724)parsecsTICv8

Mass estimated from a mass–radius relation; not an independent mass measurement. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Torres, G., et al. (2015). Validation of Twelve Small Kepler Transiting Planets in the Habitable Zone. The Astrophysical Journal, 800, 99.

    Statistical validation, planet radius, orbital period and host properties; not atmospheric evidence.

  3. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

Headless vascular blade-comb and smaller companion are visible in rain with a distant lightning branch. A single fictional crescent moon appears right-lit; the source is hidden by cloud, so its direction is not calibrated. Phase and disk size differ from the nominal half-moon prompt.

3. The many-centered migration

TRAPPIST-1 e · TRAPPIST-1 · Transit

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period6.101013 ± 0.000035daysAgol et al. 2021
Planet radius0.92 (+0.013 / −0.012)Earth radiiAgol et al. 2021
Planet mass; provenance below0.692 ± 0.022Earth massesAgol et al. 2021
Planet orbital semi-major axis0.02925 ± 0.0025AUAgol et al. 2021
Catalog incident flux0.646 ± 0.025Earth fluxAgol et al. 2021
Star effective temperature; catalog entry2566 ± 26KAgol et al. 2021
Star radius; catalog entry0.1192 ± 0.0013Solar radiiAgol et al. 2021
System distance12.42988881 ± 0.01870661parsecsGaia DR2

Mass constraint; preserve any upper/lower limit indicated in the table. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Agol, E., et al. (2021). Refining the transit timing and photometric analysis of TRAPPIST-1: Masses, radii, densities, dynamics, and ephemerides. The Planetary Science Journal, 2, 1.

    Transit timing and photodynamical constraints on the real system; no detection of this surface or life.

  3. NASA · What Webb is revealing about the TRAPPIST-1 system

    Supports astronomical context; does not establish the illustrated biology or environment.

  4. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

Joined translucent chambers, vascular interiors and many short contact lobes establish a distributed body plan. One warm stellar disk and no moons. The rendered stellar diameter is larger than the 2.17-degree central-value estimate; fog, pressure and synchronous rotation are scene assumptions.

4. The dune turners

TOI-700 d · TOI-700 · Transit

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period37.42396 (+0.00039 / −0.00035)daysGilbert et al. 2023
Planet radius1.073 (+0.059 / −0.054)Earth radiiGilbert et al. 2023
Planet mass; provenance below1.25 (meaningful uncertainty not supplied)Earth massesCalculated Value
Planet orbital semi-major axis0.1633 ± 0.0027AUGilbert et al. 2023
Catalog incident flux0.85 (+0.09 / −0.1)Earth fluxGilbert et al. 2023
Star effective temperature; catalog entry3459 ± 65KGilbert et al. 2023
Star radius; catalog entry0.421 (+0.017 / −0.015)Solar radiiGilbert et al. 2023
System distance31.1265 ± 0.0206parsecsTICv8

Mass estimated from a mass–radius relation; not an independent mass measurement. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Gilbert, E. A., et al. (2023). A Second Earth-Sized Planet in the Habitable Zone of the M Dwarf, TOI-700. The Astrophysical Journal Letters, 944, L35.

    The paper introduces planet e and refines the system, including the quoted parameters for planet d. The illustration is assigned to d.

  3. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

Muscular ring is visibly flattened at the sand contact; inner tissues and smaller related forms remain organic. One small pale stellar disk, dust front and no moons. Rolling tracks and tissue mechanics are suggestive rather than dynamically simulated.

5. The ocean’s open hearts

LHS 1140 b · LHS 1140 · Transit

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period24.73723 ± 0.00002daysCadieux et al. 2024
Planet radius1.73 ± 0.025Earth radiiCadieux et al. 2024
Planet mass; provenance below5.6 ± 0.19Earth massesCadieux et al. 2024
Planet orbital semi-major axis0.0946 ± 0.0017AUCadieux et al. 2024
Catalog incident flux0.43 ± 0.03Earth fluxCadieux et al. 2024
Star effective temperature; catalog entry3096 ± 48KCadieux et al. 2024
Star radius; catalog entry0.2159 ± 0.003Solar radiiCadieux et al. 2024
System distance14.9861 (+0.0153 / −0.0152)parsecsTICv8

Mass constraint; preserve any upper/lower limit indicated in the table. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Cadieux, C., et al. (2024). New Mass and Radius Constraints on the LHS 1140 Planets—LHS 1140 b Is Either a Temperate Mini-Neptune or a Water World. The Astrophysical Journal Letters, 960, L3.

    Mass, radius, orbital and stellar constraints; interior interpretations are model-dependent.

  3. Cadieux et al. 2024 · JWST/NIRISS transmission spectroscopy of LHS 1140 b

    Supports astronomical context; does not establish the illustrated biology or environment.

  4. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

Open muscular lattice, buoyancy nodes, feeding meshes and submerged connections are visible across a split waterline. One very small host disk is rendered below its nominal angular scale. The open ocean, ice, nodes, scale and feeding system are fictional; buoyancy is not quantitatively modeled.

6. The rain that walks

Kepler-62 e · Kepler-62 · Transit

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period122.3874 ± 0.0008daysBorucki et al. 2013
Planet radius1.61 ± 0.05Earth radiiBorucki et al. 2013
Planet mass; provenance below< 36 (upper limit)Earth massesBorucki et al. 2013
Planet orbital semi-major axis0.427 ± 0.004AUBorucki et al. 2013
Catalog incident flux1.352 ± 0.028Earth fluxBerger et al. 2018
Star effective temperature; catalog entry4925 ± 70KBorucki et al. 2013
Star radius; catalog entry0.64 ± 0.02Solar radiiBorucki et al. 2013
System distance300.874 ± 1.219parsecsTICv8

Mass constraint; preserve any upper/lower limit indicated in the table. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Borucki, W. J., et al. (2013). Kepler-62: A five-planet system with planets of 1.4 and 1.6 Earth radii in the Habitable Zone. Science, 340, 587–590.

    Discovery, orbital periods, planet radii and stellar parameters; does not establish surfaces or life.

  3. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

Mobile pleated fan, vascular ribs, a basal fringe and smaller fans are visible beneath heavy rain. The unintended bright celestial disk was removed in a targeted sky edit. The host is cloud-hidden; there are no moons or extra planets. Supporting foliage includes familiar frond-like shapes as imagined convergence.

7. The thermal breathers

Kepler-16 b · Kepler-16 · Transit

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period228.776 (+0.02 / −0.037)daysDoyle et al. 2011
Planet radius8.4493 ± 0.0291Earth radiiDoyle et al. 2011
Planet mass; provenance below105.833 ± 5.085Earth massesDoyle et al. 2011
Planet orbital semi-major axis0.7048 ± 0.0011AUDoyle et al. 2011
Catalog incident flux0.2517 ± 0.0012Earth fluxCalculated Value
Star effective temperature; catalog entry4450 ± 150KDoyle et al. 2011
Star radius; catalog entry0.6489 ± 0.0013Solar radiiDoyle et al. 2011
System distance75.0852 (+0.1541 / −0.1536)parsecsTICv8

Mass constraint; preserve any upper/lower limit indicated in the table. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Doyle, L. R., et al. (2011). Kepler-16: A Transiting Circumbinary Planet. Science, 333, 1602–1606.

    The two real stars and the circumbinary planet; the illustrated satellite is invented.

  3. Heller & Barnes 2013 · illumination and tidal heating of hypothetical moons

    Supports astronomical context; does not establish the illustrated biology or environment.

  4. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

Three prominent bellows-lobes with exchange membranes stand over a broad muscular sole in a steaming icy setting. Two small stellar sources and one left-lit banded parent planet are visible. A satellite, local heating and retained atmosphere are fictional; geometry is illustrative.

8. The low sky herds

Kepler-47 c · Kepler-47 · Transit

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period303.227 (+0.062 / −0.027)daysOrosz et al. 2019
Planet radius4.65 (+0.09 / −0.07)Earth radiiOrosz et al. 2019
Planet mass; provenance below3.17 (+2.18 / −1.25)Earth massesOrosz et al. 2019
Planet orbital semi-major axis0.9638 (+0.0041 / −0.0044)AUOrosz et al. 2019
Catalog incident flux0.9037 ± 0.0722Earth fluxCalculated Value
Star effective temperature; catalog entry5636 ± 100KOrosz et al. 2012
Star radius; catalog entry0.936 ± 0.005Solar radiiOrosz et al. 2019
System distance1025.02 ± 30.6445parsecsTICv8

Mass constraint; preserve any upper/lower limit indicated in the table. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Orosz, J. A., et al. (2019). Discovery of a Third Transiting Planet in the Kepler-47 Circumbinary System. The Astronomical Journal, 157, 174.

    Revised system solution including the quoted values for outer planet c; the newly announced planet in this paper is d.

  3. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

Three-chambered aerial adults have vascular skins and branched feeding structures above a lavender wetland. Two small hosts and one partially cropped parent disk are visible; cloud occlusion is present. Parent size exceeds the nominal prompt target. Atmospheric lift, tissue density and stable moon orbit are not established.

9. The sevenfold striders

Kepler-1647 b · Kepler-1647 · Transit

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period1107.5923 ± 0.0227daysKostov et al. 2016
Planet radius11.8739 ± 0.1377Earth radiiKostov et al. 2016
Planet mass; provenance below483 ± 206Earth massesKostov et al. 2016
Planet orbital semi-major axis2.7205 ± 0.007AUKostov et al. 2016
Catalog incident flux0.5956 ± 0.0339Earth fluxCalculated Value
Star effective temperature; catalog entry6210 ± 100KKostov et al. 2016
Star radius; catalog entry1.7903 ± 0.0055Solar radiiKostov et al. 2016
System distance1212.45 ± 22.335parsecsTICv8

Mass constraint; preserve any upper/lower limit indicated in the table. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Kostov, V. B., et al. (2016). Kepler-1647b: The Largest and Longest-period Kepler Transiting Circumbinary Planet. The Astrophysical Journal, 827, 86.

    Binary stars and the observed giant planet; does not establish a moon or its habitability.

  3. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

Headless hollow spindle, vascular slits, radial supports and patterned sensory belt are visible. The tallest adult is cropped by the upper edge; rear supports overlap, preventing an exact visible count of seven. Two small suns and one large partially cropped parent planet. Limb loads and sky geometry are illustrative.

10. The continent that breathes

HD 28185 b · HD 28185 · Radial Velocity

Open this illustrated chapter →

Saved measurements, uncertainties and original sources
QuantityValue and errorUnitSource
Planet orbital period385.92 (+0.06 / −0.07)daysVenner et al. 2024
Planet radius12.8 (meaningful uncertainty not supplied)Earth radiiCalculated Value
Planet mass; provenance below1859.29618095 ± 25.42627256Earth massesVenner et al. 2024
Planet orbital semi-major axis1.034 ± 0.006AUVenner et al. 2024
Catalog incident flux0.9073 ± 0.0207Earth fluxCalculated Value
Star effective temperature; catalog entry5602 ± 36KVenner et al. 2024
Star radius; catalog entry1.048 ± 0.015Solar radiiVenner et al. 2024
System distance39.3809 (+0.0637 / −0.0636)parsecsTICv8

Minimum mass m sin i; the true mass is not established by this value. For binary systems, the stellar rows describe one catalog entry, not both stars or their combined time-varying illumination. Calculated Value denotes an archive estimate, not a direct observation.

References

  1. NASA Exoplanet Archive. Planetary Systems Composite Parameters; local snapshot retrieved 25 September 2026. Individual measurement sources are retained in the astronomy tables.

    Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.

  2. Venner, A., et al. (2024). HD 28185 Revisited: An Outer Planet, Instead of a Brown Dwarf, On a Saturn-like Orbit. Monthly Notices of the Royal Astronomical Society, 535, 90–106.

    Revised orbital period and radial-velocity minimum mass for b; the paper’s outer-planet result concerns c.

  3. Complete scene measurements, uncertainties & assumptions

    Numerical values retained from the NASA composite snapshot dated 25 September 2026.

Visual assumptions

An integrated broad perforated sheet lifts above shoals on soft marginal paddles; several juveniles repeat its structure. One ringed parent, offshore cloud and faint auroral curtain are visible. Ring ellipse and disk overlap are visually coherent, but illumination, particle composition, satellite orbit and aurora are not calibrated.