100 Exoplanet Validation Study
This page presents a completed 100-row validation sample using NASA Science exoplanet catalogue entries with published orbital radius / semi-major axis values in AU.
Each planet is tested against the same predefined Fibonacci Index Table used elsewhere on PlanetaryHarmonics.net. The nearest Fibonacci match is selected by finding the ideal semi-major axis closest to the observed orbital radius.
Selection note: This is a curated NASA-catalogue validation sample assembled to complete the first 100-row test table. It should be treated as a substantial validation stage, not as a complete statistical survey of all 6,000+ known exoplanets. A stricter future study should use an automated NASA Exoplanet Archive TAP query with a fully reproducible selection rule.
Result Summary
100Planets tested
93Pass
7Fail
93.0%Pass rate
Validation Table
| Planet | Discovery Year | Observed SMA AU | Nearest N | N³ | Ideal SMA AU | Proximity | Status | Source |
|---|---|---|---|---|---|---|---|---|
| TOI-1232 b | 2026 | 0.117 | 0.055 | 0.000166375 | 0.1136 | 103.02% | Pass | NASA |
| GJ 3378 b | 2026 | 0.09673 | 0.055 | 0.000166375 | 0.1136 | 85.17% | Pass | NASA |
| HIP 54515 b | 2026 | 24.8 | 89 | 704,969 | 28.9763 | 85.59% | Pass | NASA |
| KMT-2025-BLG-0481L b | 2026 | 2.18 | 3 | 27 | 2.2795 | 95.63% | Pass | NASA |
| TOI-1752 c | 2026 | 0.1614 | 0.089 | 0.000704969 | 0.1629 | 99.05% | Pass | NASA |
| TOI-7384 b | 2026 | 0.0439 | 0.013 | 0.000002197 | 0.0385 | 114.03% | Pass | NASA |
| DMPP-9 b | 2026 | 0.1097 | 0.055 | 0.000166375 | 0.1136 | 96.59% | Pass | NASA |
| KMT-2025-BLG-1616L b | 2026 | 1.6 | 2 | 8 | 1.6818 | 95.14% | Pass | NASA |
| GJ 3090 c | 2026 | 0.0997 | 0.055 | 0.000166375 | 0.1136 | 87.79% | Pass | NASA |
| TOI-2071 b | 2026 | 0.0635384228693 | 0.021 | 0.000009261 | 0.0552 | 115.18% | Pass | NASA |
| KMT-2024-BLG-1281L b | 2025 | 1.96 | 2 | 8 | 1.6818 | 116.54% | Pass | NASA |
| L 98-59 f | 2025 | 0.1052 | 0.055 | 0.000166375 | 0.1136 | 92.63% | Pass | NASA |
| KMT-2023-BLG-0830L b | 2025 | 1.7 | 2 | 8 | 1.6818 | 101.08% | Pass | NASA |
| KMT-2024-BLG-2059L b | 2025 | 2.55 | 3 | 27 | 2.2795 | 111.87% | Pass | NASA |
| HD 28471 b | 2025 | 0.042 | 0.013 | 0.000002197 | 0.0385 | 109.09% | Pass | NASA |
| AU Microscopii e | 2025 | 0.170199395307 | 0.089 | 0.000704969 | 0.1629 | 104.45% | Pass | NASA |
| KMT-2023-BLG-1896L b | 2025 | 2.86 | 5 | 125 | 3.3437 | 85.53% | Pass | NASA |
| TOI-6223 b | 2025 | 0.04018 | 0.013 | 0.000002197 | 0.0385 | 104.36% | Pass | NASA |
| TOI-2322 c | 2025 | 0.1362 | 0.055 | 0.000166375 | 0.1136 | 119.92% | Pass | NASA |
| TOI-1846 b | 2025 | 0.03646 | 0.013 | 0.000002197 | 0.0385 | 94.70% | Pass | NASA |
| TOI-1224 b | 2024 | 0.0355 | 0.013 | 0.000002197 | 0.0385 | 92.21% | Pass | NASA |
| TOI-2420 b | 2024 | 0.0684 | 0.034 | 0.000039304 | 0.0792 | 86.39% | Pass | NASA |
| TOI-4504 d | 2024 | 0.2219 | 0.144 | 0.002985984 | 0.2338 | 94.93% | Pass | NASA |
| TOI-2458 b | 2024 | 0.0482 | 0.021 | 0.000009261 | 0.0552 | 87.37% | Pass | NASA |
| TOI-762 A b | 2024 | 0.03418 | 0.013 | 0.000002197 | 0.0385 | 88.78% | Pass | NASA |
| AU Microscopii d | 2023 | 0.0852732191678 | 0.034 | 0.000039304 | 0.0792 | 107.70% | Pass | NASA |
| HD 63433 d | 2023 | 0.0503 | 0.021 | 0.000009261 | 0.0552 | 91.18% | Pass | NASA |
| HD 110067 c | 2023 | 0.1039 | 0.055 | 0.000166375 | 0.1136 | 91.48% | Pass | NASA |
| TOI-5205 b | 2023 | 0.0199 | 0.005 | 0.000000125 | 0.0188 | 105.83% | Pass | NASA |
| TOI-700 e | 2023 | 0.134 | 0.055 | 0.000166375 | 0.1136 | 117.99% | Pass | NASA |
| TOI-2025 b | 2022 | 0.0892 | 0.034 | 0.000039304 | 0.0792 | 112.66% | Pass | NASA |
| AB Aurigae b | 2022 | 93.9 | 377 | 53,582,633 | 85.5571 | 109.75% | Pass | NASA |
| HD 114082 b | 2022 | 0.5109 | 0.377 | 0.053582633 | 0.4811 | 106.19% | Pass | NASA |
| LP 890-9 b | 2022 | 0.01875 | 0.005 | 0.000000125 | 0.0188 | 99.72% | Pass | NASA |
| GJ 1002 c | 2022 | 0.0738 | 0.034 | 0.000039304 | 0.0792 | 93.21% | Pass | NASA |
| TOI-1422 b | 2022 | 0.107 | 0.055 | 0.000166375 | 0.1136 | 94.21% | Pass | NASA |
| LTT 1445 A c | 2022 | 0.02661 | 0.008 | 0.000000512 | 0.0267 | 99.48% | Pass | NASA |
| CoRoT-35 b | 2022 | 0.342 | 0.233 | 0.012649337 | 0.3354 | 101.98% | Pass | NASA |
| CoRoT-36 b | 2022 | 0.0725 | 0.034 | 0.000039304 | 0.0792 | 91.56% | Pass | NASA |
| GJ 1002 b | 2022 | 0.046 | 0.013 | 0.000002197 | 0.0385 | 119.48% | Pass | NASA |
| AU Microscopii c | 2021 | 0.119 | 0.055 | 0.000166375 | 0.1136 | 104.78% | Pass | NASA |
| KMT-2020-BLG-0414L b | 2021 | 2.07 | 3 | 27 | 2.2795 | 90.81% | Pass | NASA |
| HD 22496 b | 2021 | 0.051 | 0.021 | 0.000009261 | 0.0552 | 92.45% | Pass | NASA |
| Kepler-1854 b | 2021 | 0.20894 | 0.144 | 0.002985984 | 0.2338 | 89.38% | Pass | NASA |
| GJ 486 b | 2021 | 0.01714 | 0.005 | 0.000000125 | 0.0188 | 91.16% | Pass | NASA |
| TIC 172900988 b | 2021 | 0.90281 | 1 | 1 | 1.0000 | 90.28% | Pass | NASA |
| TOI-1749 d | 2021 | 0.0707 | 0.034 | 0.000039304 | 0.0792 | 89.29% | Pass | NASA |
| G 264-012 b | 2021 | 0.022 | 0.005 | 0.000000125 | 0.0188 | 117.00% | Pass | NASA |
| G 264-012 c | 2021 | 0.045 | 0.013 | 0.000002197 | 0.0385 | 116.88% | Pass | NASA |
| BD+45 564 b | 2021 | 0.83 | 0.610 | 0.226981 | 0.6902 | 120.25% | Fail | NASA |
| TOI-700 b | 2020 | 0.0677 | 0.034 | 0.000039304 | 0.0792 | 85.50% | Pass | NASA |
| TOI-700 d | 2020 | 0.1633 | 0.089 | 0.000704969 | 0.1629 | 100.22% | Pass | NASA |
| TOI-849 b | 2020 | 0.0155 | 0.005 | 0.000000125 | 0.0188 | 82.43% | Pass | NASA |
| AU Microscopii b | 2020 | 0.07 | 0.034 | 0.000039304 | 0.0792 | 88.41% | Pass | NASA |
| HD 216520 c | 2020 | 0.528 | 0.377 | 0.053582633 | 0.4811 | 109.74% | Pass | NASA |
| WD 1856+534 b | 2020 | 0.0204 | 0.005 | 0.000000125 | 0.0188 | 108.49% | Pass | NASA |
| GJ 1061 c | 2020 | 0.0342 | 0.013 | 0.000002197 | 0.0385 | 88.83% | Pass | NASA |
| GJ 251 b | 2020 | 0.0808 | 0.034 | 0.000039304 | 0.0792 | 102.05% | Pass | NASA |
| KOI-1783.02 | 2020 | 0.86695 | 1 | 1 | 1.0000 | 86.69% | Pass | NASA |
| CoRoT-30 b | 2020 | 0.084 | 0.034 | 0.000039304 | 0.0792 | 106.09% | Pass | NASA |
| G 9-40 b | 2019 | 0.0418 | 0.013 | 0.000002197 | 0.0385 | 108.57% | Pass | NASA |
| EPIC 212737443 c | 2019 | 0.28 | 0.144 | 0.002985984 | 0.2338 | 119.78% | Pass | NASA |
| L 98-59 b | 2019 | 0.0223 | 0.005 | 0.000000125 | 0.0188 | 118.60% | Pass | NASA |
| DMPP-1 b | 2019 | 0.1423 | 0.089 | 0.000704969 | 0.1629 | 87.33% | Pass | NASA |
| WASP-190 b | 2019 | 0.0663 | 0.021 | 0.000009261 | 0.0552 | 120.18% | Fail | NASA |
| DMPP-2 b | 2019 | 0.06638 | 0.021 | 0.000009261 | 0.0552 | 120.33% | Fail | NASA |
| V1298 Tauri b | 2019 | 0.1685 | 0.089 | 0.000704969 | 0.1629 | 103.41% | Pass | NASA |
| Epsilon Indi A b | 2019 | 11.55 | 21 | 9,261 | 9.8099 | 117.74% | Pass | NASA |
| Beta Pictoris c | 2019 | 2.72 | 3 | 27 | 2.2795 | 119.32% | Pass | NASA |
| DMPP-3 A b | 2019 | 0.0662 | 0.021 | 0.000009261 | 0.0552 | 120.00% | Fail | NASA |
| HD 180617 b | 2018 | 0.343 | 0.233 | 0.012649337 | 0.3354 | 102.28% | Pass | NASA |
| K2-237 b | 2018 | 0.03552 | 0.013 | 0.000002197 | 0.0385 | 92.26% | Pass | NASA |
| K2-288 B b | 2018 | 0.164 | 0.089 | 0.000704969 | 0.1629 | 100.65% | Pass | NASA |
| LHS 1140 c | 2018 | 0.027 | 0.008 | 0.000000512 | 0.0267 | 100.94% | Pass | NASA |
| PDS 70 b | 2018 | 20.8 | 55 | 166,375 | 20.1963 | 102.99% | Pass | NASA |
| HATS-59 b | 2018 | 0.06112 | 0.021 | 0.000009261 | 0.0552 | 110.79% | Pass | NASA |
| DE Canum Venaticorum b | 2018 | 1.29 | 1 | 1 | 1.0000 | 129.00% | Fail | NASA |
| BD+48 740 b | 2018 | 1.89 | 2 | 8 | 1.6818 | 112.38% | Pass | NASA |
| EPIC 246851721 b | 2018 | 0.08 | 0.034 | 0.000039304 | 0.0792 | 101.04% | Pass | NASA |
| Gamma Librae b | 2018 | 1.24 | 1 | 1 | 1.0000 | 124.00% | Fail | NASA |
| GJ 3323 b | 2017 | 0.03282 | 0.013 | 0.000002197 | 0.0385 | 85.25% | Pass | NASA |
| KELT-12 b | 2017 | 0.06708 | 0.021 | 0.000009261 | 0.0552 | 121.60% | Fail | NASA |
| GJ 273 b | 2017 | 0.091101 | 0.034 | 0.000039304 | 0.0792 | 115.06% | Pass | NASA |
| Tau Ceti h | 2017 | 0.243 | 0.144 | 0.002985984 | 0.2338 | 103.95% | Pass | NASA |
| LHS 1140 b | 2017 | 0.0946 | 0.034 | 0.000039304 | 0.0792 | 119.48% | Pass | NASA |
| K2-18 c | 2017 | 0.06 | 0.021 | 0.000009261 | 0.0552 | 108.76% | Pass | NASA |
| TRAPPIST-1 e | 2017 | 0.02925 | 0.008 | 0.000000512 | 0.0267 | 109.35% | Pass | NASA |
| K2-3 d | 2017 | 0.2086 | 0.144 | 0.002985984 | 0.2338 | 89.24% | Pass | NASA |
| K2-3 c | 2017 | 0.14 | 0.089 | 0.000704969 | 0.1629 | 85.92% | Pass | NASA |
| K2-3 b | 2017 | 0.077 | 0.034 | 0.000039304 | 0.0792 | 97.25% | Pass | NASA |
| Kepler-816 b | 2016 | 0.0895 | 0.034 | 0.000039304 | 0.0792 | 113.04% | Pass | NASA |
| Kepler-1606 b | 2016 | 0.6421 | 0.610 | 0.226981 | 0.6902 | 93.03% | Pass | NASA |
| Kepler-1598 b | 2016 | 0.05207 | 0.021 | 0.000009261 | 0.0552 | 94.39% | Pass | NASA |
| KELT-4 A b | 2016 | 0.04317 | 0.013 | 0.000002197 | 0.0385 | 112.13% | Pass | NASA |
| Proxima Centauri b | 2016 | 0.04848 | 0.021 | 0.000009261 | 0.0552 | 87.88% | Pass | NASA |
| TRAPPIST-1 b | 2016 | 0.01154 | 0.005 | 0.000000125 | 0.0188 | 61.37% | Fail | NASA |
| HR 2562 b | 2016 | 22.2 | 55 | 166,375 | 20.1963 | 109.92% | Pass | NASA |
| BD+20 594 b | 2016 | 0.241 | 0.144 | 0.002985984 | 0.2338 | 103.10% | Pass | NASA |
| K2-18 b | 2015 | 0.1429 | 0.089 | 0.000704969 | 0.1629 | 87.70% | Pass | NASA |
| GJ 1132 b | 2015 | 0.0157 | 0.005 | 0.000000125 | 0.0188 | 83.50% | Pass | NASA |
Pass criterion: 80% ≤ proximity ≤ 120%. Proximity is observed SMA ÷ ideal SMA × 100.
Interpretation
This 100-row validation sample produced 93 passes and 7 fails. The result is notable, but it should still be presented cautiously. Planetary Harmonics investigates whether a measurable relationship exists between observed orbital distances and a Fibonacci-based spacing model; it does not claim that Fibonacci numbers cause planetary formation.
The next scientific improvement would be to repeat this test using a directly exported NASA Exoplanet Archive table and publish the exact query used to select the planets.