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.
Kepler-62 f · Kepler-62 · Transit
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 267.291 ± 0.005 | days | Borucki et al. 2013 |
| Planet radius | 1.41 ± 0.07 | Earth radii | Borucki et al. 2013 |
| Planet mass; provenance below | < 35 (upper limit) | Earth masses | Borucki et al. 2013 |
| Planet orbital semi-major axis | 0.718 ± 0.007 | AU | Borucki et al. 2013 |
| Catalog incident flux | 0.5 (meaningful uncertainty not supplied) | Earth flux | Fulton & Petigura 2018 |
| Star effective temperature; catalog entry | 4925 ± 70 | K | Borucki et al. 2013 |
| Star radius; catalog entry | 0.64 ± 0.02 | Solar radii | Borucki et al. 2013 |
| System distance | 300.874 ± 1.219 | parsecs | TICv8 |
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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
Discovery, orbital periods, planet radii and stellar parameters; does not establish surfaces or life.
Supports astronomical context; does not establish the illustrated biology or environment.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.
Kepler-442 b · Kepler-442 · Transit
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 112.3053 (+0.0024 / −0.0028) | days | Torres et al. 2015 |
| Planet radius | 1.34 (+0.11 / −0.18) | Earth radii | Torres et al. 2015 |
| Planet mass; provenance below | 2.36 (meaningful uncertainty not supplied) | Earth masses | Calculated Value |
| Planet orbital semi-major axis | 0.409 (+0.209 / −0.06) | AU | Torres et al. 2015 |
| Catalog incident flux | 0.66 (+0.23 / −0.41) | Earth flux | Torres et al. 2015 |
| Star effective temperature; catalog entry | 4402 ± 100 | K | Torres et al. 2015 |
| Star radius; catalog entry | 0.598 (+0.023 / −0.024) | Solar radii | Torres et al. 2015 |
| System distance | 365.965 (+2.763 / −2.724) | parsecs | TICv8 |
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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
Statistical validation, planet radius, orbital period and host properties; not atmospheric evidence.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.
TRAPPIST-1 e · TRAPPIST-1 · Transit
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 6.101013 ± 0.000035 | days | Agol et al. 2021 |
| Planet radius | 0.92 (+0.013 / −0.012) | Earth radii | Agol et al. 2021 |
| Planet mass; provenance below | 0.692 ± 0.022 | Earth masses | Agol et al. 2021 |
| Planet orbital semi-major axis | 0.02925 ± 0.0025 | AU | Agol et al. 2021 |
| Catalog incident flux | 0.646 ± 0.025 | Earth flux | Agol et al. 2021 |
| Star effective temperature; catalog entry | 2566 ± 26 | K | Agol et al. 2021 |
| Star radius; catalog entry | 0.1192 ± 0.0013 | Solar radii | Agol et al. 2021 |
| System distance | 12.42988881 ± 0.01870661 | parsecs | Gaia 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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
Transit timing and photodynamical constraints on the real system; no detection of this surface or life.
Supports astronomical context; does not establish the illustrated biology or environment.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.
TOI-700 d · TOI-700 · Transit
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 37.42396 (+0.00039 / −0.00035) | days | Gilbert et al. 2023 |
| Planet radius | 1.073 (+0.059 / −0.054) | Earth radii | Gilbert et al. 2023 |
| Planet mass; provenance below | 1.25 (meaningful uncertainty not supplied) | Earth masses | Calculated Value |
| Planet orbital semi-major axis | 0.1633 ± 0.0027 | AU | Gilbert et al. 2023 |
| Catalog incident flux | 0.85 (+0.09 / −0.1) | Earth flux | Gilbert et al. 2023 |
| Star effective temperature; catalog entry | 3459 ± 65 | K | Gilbert et al. 2023 |
| Star radius; catalog entry | 0.421 (+0.017 / −0.015) | Solar radii | Gilbert et al. 2023 |
| System distance | 31.1265 ± 0.0206 | parsecs | TICv8 |
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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
The paper introduces planet e and refines the system, including the quoted parameters for planet d. The illustration is assigned to d.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.
LHS 1140 b · LHS 1140 · Transit
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 24.73723 ± 0.00002 | days | Cadieux et al. 2024 |
| Planet radius | 1.73 ± 0.025 | Earth radii | Cadieux et al. 2024 |
| Planet mass; provenance below | 5.6 ± 0.19 | Earth masses | Cadieux et al. 2024 |
| Planet orbital semi-major axis | 0.0946 ± 0.0017 | AU | Cadieux et al. 2024 |
| Catalog incident flux | 0.43 ± 0.03 | Earth flux | Cadieux et al. 2024 |
| Star effective temperature; catalog entry | 3096 ± 48 | K | Cadieux et al. 2024 |
| Star radius; catalog entry | 0.2159 ± 0.003 | Solar radii | Cadieux et al. 2024 |
| System distance | 14.9861 (+0.0153 / −0.0152) | parsecs | TICv8 |
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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
Mass, radius, orbital and stellar constraints; interior interpretations are model-dependent.
Supports astronomical context; does not establish the illustrated biology or environment.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.
Kepler-62 e · Kepler-62 · Transit
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 122.3874 ± 0.0008 | days | Borucki et al. 2013 |
| Planet radius | 1.61 ± 0.05 | Earth radii | Borucki et al. 2013 |
| Planet mass; provenance below | < 36 (upper limit) | Earth masses | Borucki et al. 2013 |
| Planet orbital semi-major axis | 0.427 ± 0.004 | AU | Borucki et al. 2013 |
| Catalog incident flux | 1.352 ± 0.028 | Earth flux | Berger et al. 2018 |
| Star effective temperature; catalog entry | 4925 ± 70 | K | Borucki et al. 2013 |
| Star radius; catalog entry | 0.64 ± 0.02 | Solar radii | Borucki et al. 2013 |
| System distance | 300.874 ± 1.219 | parsecs | TICv8 |
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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
Discovery, orbital periods, planet radii and stellar parameters; does not establish surfaces or life.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.
Kepler-16 b · Kepler-16 · Transit
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 228.776 (+0.02 / −0.037) | days | Doyle et al. 2011 |
| Planet radius | 8.4493 ± 0.0291 | Earth radii | Doyle et al. 2011 |
| Planet mass; provenance below | 105.833 ± 5.085 | Earth masses | Doyle et al. 2011 |
| Planet orbital semi-major axis | 0.7048 ± 0.0011 | AU | Doyle et al. 2011 |
| Catalog incident flux | 0.2517 ± 0.0012 | Earth flux | Calculated Value |
| Star effective temperature; catalog entry | 4450 ± 150 | K | Doyle et al. 2011 |
| Star radius; catalog entry | 0.6489 ± 0.0013 | Solar radii | Doyle et al. 2011 |
| System distance | 75.0852 (+0.1541 / −0.1536) | parsecs | TICv8 |
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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
The two real stars and the circumbinary planet; the illustrated satellite is invented.
Supports astronomical context; does not establish the illustrated biology or environment.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.
Kepler-47 c · Kepler-47 · Transit
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 303.227 (+0.062 / −0.027) | days | Orosz et al. 2019 |
| Planet radius | 4.65 (+0.09 / −0.07) | Earth radii | Orosz et al. 2019 |
| Planet mass; provenance below | 3.17 (+2.18 / −1.25) | Earth masses | Orosz et al. 2019 |
| Planet orbital semi-major axis | 0.9638 (+0.0041 / −0.0044) | AU | Orosz et al. 2019 |
| Catalog incident flux | 0.9037 ± 0.0722 | Earth flux | Calculated Value |
| Star effective temperature; catalog entry | 5636 ± 100 | K | Orosz et al. 2012 |
| Star radius; catalog entry | 0.936 ± 0.005 | Solar radii | Orosz et al. 2019 |
| System distance | 1025.02 ± 30.6445 | parsecs | TICv8 |
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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
Revised system solution including the quoted values for outer planet c; the newly announced planet in this paper is d.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.
Kepler-1647 b · Kepler-1647 · Transit
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 1107.5923 ± 0.0227 | days | Kostov et al. 2016 |
| Planet radius | 11.8739 ± 0.1377 | Earth radii | Kostov et al. 2016 |
| Planet mass; provenance below | 483 ± 206 | Earth masses | Kostov et al. 2016 |
| Planet orbital semi-major axis | 2.7205 ± 0.007 | AU | Kostov et al. 2016 |
| Catalog incident flux | 0.5956 ± 0.0339 | Earth flux | Calculated Value |
| Star effective temperature; catalog entry | 6210 ± 100 | K | Kostov et al. 2016 |
| Star radius; catalog entry | 1.7903 ± 0.0055 | Solar radii | Kostov et al. 2016 |
| System distance | 1212.45 ± 22.335 | parsecs | TICv8 |
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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
Binary stars and the observed giant planet; does not establish a moon or its habitability.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.
HD 28185 b · HD 28185 · Radial Velocity
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| Quantity | Value and error | Unit | Source |
|---|---|---|---|
| Planet orbital period | 385.92 (+0.06 / −0.07) | days | Venner et al. 2024 |
| Planet radius | 12.8 (meaningful uncertainty not supplied) | Earth radii | Calculated Value |
| Planet mass; provenance below | 1859.29618095 ± 25.42627256 | Earth masses | Venner et al. 2024 |
| Planet orbital semi-major axis | 1.034 ± 0.006 | AU | Venner et al. 2024 |
| Catalog incident flux | 0.9073 ± 0.0207 | Earth flux | Calculated Value |
| Star effective temperature; catalog entry | 5602 ± 36 | K | Venner et al. 2024 |
| Star radius; catalog entry | 1.048 ± 0.015 | Solar radii | Venner et al. 2024 |
| System distance | 39.3809 (+0.0637 / −0.0636) | parsecs | TICv8 |
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.
Catalog measurements, errors, limits and parameter-specific source links. A composite catalog may combine different publications.
Revised orbital period and radial-velocity minimum mass for b; the paper’s outer-planet result concerns c.
Numerical values retained from the NASA composite snapshot dated 25 September 2026.
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.