Orbit uncertainty after observation submissions
Each row is an independent Find_Orb reconstruction using only observations whose WAMO submission time is at or before that row. The uncertainty is evaluated at the nearest Find_Orb ephemeris minute to the exact submission UTC. Thus later observations cannot influence an earlier row. Missing values identify insufficient observations or a failed historical fit. Each object keeps its complete table and matching graph together.
00001AE
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-03 01:53:30 UTC | 3 | 3 | 327 — Peking Observatory, Xinglong Station | 6.300′ | fitted |
00001BL
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 02:09:09 UTC | 3 | 3 | 327 — Peking Observatory, Xinglong Station | 26.683′ | fitted |
00001Bx
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 02:09:09 UTC | 4 | 4 | 327 — Peking Observatory, Xinglong Station | 1.602′ | fitted |
00001CB
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 04:48:15 UTC | 3 | 3 | 327 — Peking Observatory, Xinglong Station | 2.983′ | fitted |
00001Ck
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 04:48:15 UTC | 3 | 3 | 327 — Peking Observatory, Xinglong Station | 12.717′ | fitted |
A11FPxB
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-08-19 19:56:00 UTC | 4 | 4 | M22 — ATLAS South Africa, Sutherland | 1.578′ | fitted |
| 2026-08-20 22:58:01 UTC | 3 | 7 | Y05 — SONEAR Wykrota-CEAMIG, Serra da Piedade | 0.041′ | fitted |
| 2026-08-21 18:23:55 UTC | 2 | 9 | M49 — IAS Remote Observatory, Hakos | 0.007′ | fitted |
| 2026-08-22 18:46:56 UTC | 2 | 11 | M49 — IAS Remote Observatory, Hakos | 0.005′ | fitted |
| 2026-08-23 16:03:49 UTC | 2 | 13 | Q64 — Siding Spring-LCO B | 0.006′ | fitted |
| 2026-08-23 16:20:05 UTC | 3 | 16 | Q62 — iTelescope Observatory, Siding Spring | 0.004′ | fitted |
| 2026-08-24 18:46:32 UTC | 2 | 18 | M49 — IAS Remote Observatory, Hakos | 0.004′ | fitted |
| 2026-08-26 16:04:26 UTC | 2 | 20 | X28 — Station name unavailable | 0.016′ | fitted |
| 2026-08-28 08:00:18 UTC | 3 | 23 | E42 — AUSTRALIA1/SRI, Swan Reach | — | fit-error |
| 2026-08-28 22:33:43 UTC | 2 | 25 | E62 — Slooh.com Australia, Coonabarabran | 0.004′ | fitted |
| 2026-08-31 22:09:45 UTC | 2 | 27 | E62 — Slooh.com Australia, Coonabarabran | 0.005′ | fitted |
| 2026-09-03 20:07:37 UTC | 3 | 30 | M49 — IAS Remote Observatory, Hakos | 0.003′ | fitted |
| 2026-09-04 14:09:31 UTC | 3 | 33 | 194 — Tivoli | 0.002′ | fitted |
| 2026-09-05 16:51:23 UTC | 3 | 36 | M49 — IAS Remote Observatory, Hakos | 0.003′ | fitted |
| 2026-09-09 20:31:38 UTC | 3 | 39 | 194 — Tivoli | 0.004′ | fitted |
| 2026-09-09 20:50:54 UTC | 2 | 41 | M21 — Schiaparelli Southern Observatory, Hakos | 0.004′ | fitted |
| 2026-09-12 04:45:05 UTC | 5 | 46 | Q63 — Siding Spring-LCO A | 0.003′ | fitted |
| 2026-09-12 18:52:05 UTC | 3 | 49 | M49 — IAS Remote Observatory, Hakos | 0.002′ | fitted |
| 2026-09-17 12:35:06 UTC | 2 | 51 | I47 — Pierre Auger Observatory, Malargue | 0.004′ | fitted |
| 2026-10-03 10:15:04 UTC | 3 | 54 | E94 — Possum Observatory, Gisborne | — | fit-error |
| 2026-10-04 12:17:37 UTC | 2 | 56 | M21 — Schiaparelli Southern Observatory, Hakos | 0.009′ | fitted |
A11H8ut
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-19 06:06:39 UTC | 5 | 5 | R17 — ATLAS-TDO | 0.293′ | fitted |
| 2026-09-19 10:52:56 UTC | 3 | 8 | 734 — Farpoint Observatory, Eskridge | 0.015′ | fitted |
| 2026-09-20 07:48:53 UTC | 3 | 11 | Y64 — Transient Survey Telescope (TST), Teide | 0.007′ | fitted |
| 2026-09-20 11:57:07 UTC | 4 | 15 | I52 — Steward Observatory, Mt. Lemmon Station | 0.004′ | fitted |
| 2026-09-20 12:55:38 UTC | 3 | 18 | V21 — Cewanee Observatory at DSNM | 0.004′ | fitted |
| 2026-09-21 06:12:50 UTC | 2 | 20 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.013′ | fitted |
| 2026-09-21 19:10:42 UTC | 3 | 23 | Q06 — Tarui Observatory, Tarui | 0.007′ | fitted |
| 2026-09-22 02:00:08 UTC | 2 | 25 | Q62 — iTelescope Observatory, Siding Spring | 0.012′ | fitted |
| 2026-09-22 03:04:33 UTC | 2 | 27 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.003′ | fitted |
| 2026-09-25 09:27:51 UTC | 3 | 30 | Y68 — Two-meter Twin Telescope, TTT3 | 0.003′ | fitted |
| 2026-09-25 09:52:15 UTC | 3 | 33 | R18 — Two-meter Twin Telescope, TTT4 | 0.002′ | fitted |
| 2026-09-26 02:20:05 UTC | 3 | 36 | 595 — Farra d'Isonzo | 0.002′ | fitted |
| 2026-09-26 05:26:44 UTC | 3 | 39 | R59 — Camarasa Observatory, Astrocamp Nerpio | 0.002′ | fitted |
| 2026-09-26 19:43:44 UTC | 3 | 42 | U95 — USA1/HCRO, Pie Town | 0.002′ | fitted |
| 2026-09-26 23:20:05 UTC | 2 | 44 | I47 — Pierre Auger Observatory, Malargue | 0.003′ | fitted |
| 2026-09-28 05:55:36 UTC | 3 | 47 | L06 — Sormano 2 Observatory, Bellagio Via Lattea | 0.003′ | fitted |
| 2026-09-29 15:51:52 UTC | 3 | 50 | R18 — Two-meter Twin Telescope, TTT4 | 0.004′ | fitted |
| 2026-09-29 18:15:39 UTC | 2 | 52 | K74 — Muensterschwarzach Observatory, Schwarzach | 0.004′ | fitted |
| 2026-09-30 06:11:15 UTC | 2 | 54 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.003′ | fitted |
| 2026-09-30 18:55:53 UTC | 3 | 57 | 900 — Moriyama | 0.003′ | fitted |
| 2026-10-01 02:59:02 UTC | 2 | 59 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.002′ | fitted |
A11HAVq
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 12:40:50 UTC | 4 | 4 | T05 — ATLAS-HKO, Haleakala | 0.838′ | fitted |
A11Htul
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-01 13:57:11 UTC | 4 | 4 | T08 — ATLAS-MLO, Mauna Loa | 7.317′ | fitted |
C1GE785
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
C1GFD95
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 07:37:21 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 0.758′ | fitted |
C1GFDH5
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 07:39:10 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 1.900′ | fitted |
C1LT2DP
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-11 22:53:34 UTC | 4 | 4 | G96 — University of Arizona Mt. Lemmon Survey | 15.433′ | fitted |
C1M0JJP
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-21 03:53:20 UTC | 4 | 4 | G96 — University of Arizona Mt. Lemmon Survey | 1.033′ | fitted |
C46K1R1
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-14 04:04:35 UTC | 4 | 4 | 703 — University of Arizona Catalina Sky Survey | 3.533′ | fitted |
| 2026-09-14 04:21:00 UTC | 4 | 8 | 703 — University of Arizona Catalina Sky Survey | 1.100′ | fitted |
| 2026-09-14 18:56:13 UTC | 3 | 11 | 595 — Farra d'Isonzo | 0.046′ | fitted |
| 2026-09-14 19:04:56 UTC | 3 | 14 | M26 — Zen Observatory, Scandicci | 0.037′ | fitted |
| 2026-09-14 19:08:14 UTC | 2 | 16 | 126 — Monte Viseggi L. Zannoni Observatory | 0.046′ | fitted |
| 2026-09-14 19:14:39 UTC | 4 | 20 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.046′ | fitted |
| 2026-09-14 19:17:16 UTC | 2 | 22 | 126 — Monte Viseggi L. Zannoni Observatory | 0.025′ | fitted |
| 2026-09-14 19:47:49 UTC | 3 | 25 | K74 — Muensterschwarzach Observatory, Schwarzach | 0.021′ | fitted |
| 2026-09-14 19:50:06 UTC | 2 | 27 | L06 — Sormano 2 Observatory, Bellagio Via Lattea | 0.015′ | fitted |
| 2026-09-14 20:20:06 UTC | 3 | 30 | G34 — Oberfrauendorf | 0.047′ | fitted |
| 2026-09-14 20:26:59 UTC | 3 | 33 | R48 — Centro Astronomico Alto Turia 2 | 0.006′ | fitted |
| 2026-09-14 20:29:10 UTC | 2 | 35 | M38 — Harsona Observatory, Nyiregyhaza | 0.004′ | fitted |
| 2026-09-14 20:38:21 UTC | 3 | 38 | R59 — Camarasa Observatory, Astrocamp Nerpio | 0.004′ | fitted |
| 2026-09-14 20:50:22 UTC | 3 | 41 | J87 — La Canada | 0.006′ | fitted |
| 2026-09-14 20:53:42 UTC | 3 | 44 | A71 — Stixendorf | 0.005′ | fitted |
| 2026-09-14 21:00:51 UTC | 2 | 46 | D31 — Osservatorio Aldebaran, Rivalba | 0.005′ | fitted |
| 2026-09-14 21:17:12 UTC | 3 | 49 | R93 — Sanse Observatory, San Sebastiano Curone | 0.005′ | fitted |
| 2026-09-14 21:24:27 UTC | 3 | 52 | R85 — Telescope Leonard de Vinci, GAPRA, Antibes | 0.004′ | fitted |
| 2026-09-14 21:52:47 UTC | 4 | 56 | C23 — Olmen | 0.003′ | fitted |
| 2026-09-14 22:25:17 UTC | 2 | 58 | 970 — Chelmsford | 0.004′ | fitted |
| 2026-09-15 00:01:24 UTC | 3 | 61 | P13 — Baihuashan Observatory, Beijing | 0.004′ | fitted |
| 2026-09-15 05:05:17 UTC | 3 | 64 | 215 — Buchloe | 0.012′ | fitted |
| 2026-09-15 05:05:53 UTC | 6 | 70 | L27 — 29PREMOTE Observatory, Dauban | 0.012′ | fitted |
| 2026-09-15 06:45:05 UTC | 3 | 73 | 718 — Tooele | 0.004′ | fitted |
| 2026-09-15 07:31:16 UTC | 3 | 76 | W62 — Comet Hunter Observatory2, New Ringgold | 0.005′ | fitted |
| 2026-09-15 08:02:41 UTC | 2 | 78 | U94 — iTelescope Observatory, Beryl Junction | 0.004′ | fitted |
| 2026-09-15 08:17:13 UTC | 5 | 83 | B96 — Brixiis Observatory, Kruibeke | 0.004′ | fitted |
| 2026-09-15 08:45:06 UTC | 2 | 85 | L06 — Sormano 2 Observatory, Bellagio Via Lattea | 0.004′ | fitted |
| 2026-09-15 11:45:05 UTC | 3 | 88 | U94 — iTelescope Observatory, Beryl Junction | 0.050′ | fitted |
| 2026-09-15 18:50:08 UTC | 3 | 91 | M32 — Sunny Transcarpathian, Mukachevo | 0.004′ | fitted |
| 2026-09-15 18:55:06 UTC | 3 | 94 | K88 — GINOP-KHK, Piszkesteto | 0.004′ | fitted |
| 2026-09-15 18:58:04 UTC | 3 | 97 | A71 — Stixendorf | 0.004′ | fitted |
| 2026-09-15 18:59:25 UTC | 2 | 99 | M38 — Harsona Observatory, Nyiregyhaza | 0.004′ | fitted |
| 2026-09-15 19:27:38 UTC | 4 | 103 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.001′ | fitted |
| 2026-09-15 19:30:05 UTC | 4 | 107 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-09-15 19:32:43 UTC | 2 | 109 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-09-15 20:00:26 UTC | 3 | 112 | M54 — Observatoire Albireo de Biot | 0.004′ | fitted |
| 2026-09-15 20:01:12 UTC | 3 | 115 | 126 — Monte Viseggi L. Zannoni Observatory | 0.004′ | fitted |
| 2026-09-15 20:09:06 UTC | 3 | 118 | K19 — PASTIS Observatory, Banon | 0.004′ | fitted |
| 2026-09-15 20:17:56 UTC | 3 | 121 | B74 — Santa Maria de Montmagastrell | 0.004′ | fitted |
| 2026-09-15 21:12:47 UTC | 4 | 125 | 151 — Eschenberg Observatory, Winterthur | 0.000′ | fitted |
| 2026-09-15 21:18:33 UTC | 2 | 127 | 970 — Chelmsford | 0.000′ | fitted |
| 2026-09-15 21:33:58 UTC | 2 | 129 | 204 — Schiaparelli Observatory | 0.000′ | fitted |
| 2026-09-15 22:30:03 UTC | 2 | 131 | D31 — Osservatorio Aldebaran, Rivalba | 0.002′ | fitted |
| 2026-09-15 22:47:59 UTC | 2 | 133 | 104 — San Marcello Pistoiese | 0.001′ | fitted |
| 2026-09-16 00:35:33 UTC | 2 | 135 | Z80 — Northolt Branch Observatory | 0.001′ | fitted |
| 2026-09-16 10:50:52 UTC | 3 | 138 | G40 — Slooh.com Canary Islands Observatory | 0.003′ | fitted |
| 2026-09-16 11:10:06 UTC | 4 | 142 | A71 — Stixendorf | 0.003′ | fitted |
| 2026-09-16 11:35:06 UTC | 2 | 144 | L85 — BiAnto Observatory, Lauria | 0.005′ | fitted |
| 2026-09-16 13:45:06 UTC | 4 | 148 | P87 — Hirao Observatory, Yamaguchi | 0.053′ | fitted |
| 2026-09-16 18:56:56 UTC | 2 | 150 | M38 — Harsona Observatory, Nyiregyhaza | 0.003′ | fitted |
| 2026-09-16 19:22:32 UTC | 2 | 152 | C82 — Osservatorio Astronomico Nastro Verde, Sorrento | 0.002′ | fitted |
| 2026-09-16 19:31:42 UTC | 2 | 154 | C82 — Osservatorio Astronomico Nastro Verde, Sorrento | 0.002′ | fitted |
| 2026-09-16 19:54:55 UTC | 2 | 156 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.002′ | fitted |
| 2026-09-16 20:10:25 UTC | 5 | 161 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-09-16 20:34:53 UTC | 4 | 165 | L18 — QOS Observatory, Zalistsi | 0.001′ | fitted |
| 2026-09-16 20:35:05 UTC | 3 | 168 | I93 — St Pardon de Conques | 0.001′ | fitted |
| 2026-09-16 20:37:44 UTC | 3 | 171 | K83 — Osservatorio Astronomico Beppe Forti, Montelupo | 0.001′ | fitted |
| 2026-09-16 21:33:57 UTC | 3 | 174 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.001′ | fitted |
| 2026-09-16 23:20:05 UTC | 2 | 176 | 950 — La Palma | 0.001′ | fitted |
| 2026-09-17 03:23:05 UTC | 2 | 178 | 970 — Chelmsford | 0.001′ | fitted |
| 2026-09-17 06:40:22 UTC | 2 | 180 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.002′ | fitted |
| 2026-09-17 07:38:39 UTC | 2 | 182 | G40 — Slooh.com Canary Islands Observatory | 0.002′ | fitted |
| 2026-09-17 08:44:01 UTC | 3 | 185 | R49 — Observatorio Villuercas-Navezuelas, Navezuelas | 0.002′ | fitted |
| 2026-09-17 11:49:52 UTC | 3 | 188 | 900 — Moriyama | 0.002′ | fitted |
| 2026-09-17 19:52:12 UTC | 3 | 191 | M35 — PS Observatory, Parjol | 0.002′ | fitted |
| 2026-09-17 20:45:05 UTC | 2 | 193 | G18 — ALMO Observatory, Padulle | 0.002′ | fitted |
| 2026-09-17 21:20:17 UTC | 4 | 197 | J95 — Great Shefford | 0.001′ | fitted |
| 2026-09-18 00:48:18 UTC | 3 | 200 | Z80 — Northolt Branch Observatory | 0.001′ | fitted |
| 2026-09-18 03:09:50 UTC | 3 | 203 | X04 — MCD Observatory, Saint-Anaclet | 0.001′ | fitted |
| 2026-09-18 06:35:05 UTC | 3 | 206 | 718 — Tooele | 0.001′ | fitted |
| 2026-09-18 16:27:08 UTC | 2 | 208 | D63 — G. Pascoli Observatory, Barga (since June 2023) | 0.002′ | fitted |
| 2026-09-18 18:50:04 UTC | 3 | 211 | K88 — GINOP-KHK, Piszkesteto | 0.002′ | fitted |
| 2026-09-18 19:10:06 UTC | 5 | 216 | M32 — Sunny Transcarpathian, Mukachevo | 0.002′ | fitted |
| 2026-09-18 19:16:38 UTC | 3 | 219 | A71 — Stixendorf | 0.001′ | fitted |
| 2026-09-18 19:56:59 UTC | 3 | 222 | K19 — PASTIS Observatory, Banon | 0.001′ | fitted |
| 2026-09-18 21:09:52 UTC | 3 | 225 | G34 — Oberfrauendorf | 0.001′ | fitted |
| 2026-09-18 21:58:45 UTC | 3 | 228 | I81 — Tarbatness Observatory, Portmahomack | 0.001′ | fitted |
| 2026-09-18 23:46:11 UTC | 4 | 232 | I41 — Palomar Mountain--ZTF | 0.001′ | fitted |
| 2026-09-18 23:54:58 UTC | 2 | 234 | Q14 — Goto Astronomical Observatory in Yatsugatake | 0.001′ | fitted |
| 2026-09-19 01:04:42 UTC | 3 | 237 | W62 — Comet Hunter Observatory2, New Ringgold | 0.001′ | fitted |
| 2026-09-19 01:46:07 UTC | 4 | 241 | H36 — Sandlot Observatory, Scranton | 0.001′ | fitted |
| 2026-09-19 03:53:26 UTC | 4 | 245 | 703 — University of Arizona Catalina Sky Survey | 0.001′ | fitted |
| 2026-09-19 05:13:55 UTC | 10 | 255 | L27 — 29PREMOTE Observatory, Dauban | 0.001′ | fitted |
| 2026-09-19 05:25:31 UTC | 6 | 261 | V16 — Dark Sky New Mexico, Animas | 0.001′ | fitted |
| 2026-09-19 08:21:44 UTC | 6 | 267 | V21 — Cewanee Observatory at DSNM | 0.001′ | fitted |
| 2026-09-19 15:20:06 UTC | 3 | 270 | Y87 — Trevinca Skies-Amalthea, Trevinca | 0.002′ | fitted |
| 2026-09-19 19:01:14 UTC | 2 | 272 | M38 — Harsona Observatory, Nyiregyhaza | 0.002′ | fitted |
| 2026-09-19 20:05:22 UTC | 5 | 277 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-09-19 21:01:45 UTC | 4 | 281 | L18 — QOS Observatory, Zalistsi | 0.001′ | fitted |
| 2026-09-19 21:45:00 UTC | 3 | 284 | A77 — Observatoire Chante-Perdrix, Dauban | 0.001′ | fitted |
| 2026-09-20 02:23:52 UTC | 3 | 287 | I81 — Tarbatness Observatory, Portmahomack | 0.001′ | fitted |
| 2026-09-20 05:21:49 UTC | 3 | 290 | V21 — Cewanee Observatory at DSNM | 0.001′ | fitted |
| 2026-09-20 08:10:24 UTC | 3 | 293 | G00 — AZM Martinsberg, Oed | 0.002′ | fitted |
| 2026-09-20 09:10:05 UTC | 3 | 296 | 718 — Tooele | 0.002′ | fitted |
| 2026-09-20 16:28:10 UTC | 2 | 298 | 213 — Observatorio Montcabre | 0.002′ | fitted |
| 2026-09-20 17:05:05 UTC | 3 | 301 | P87 — Hirao Observatory, Yamaguchi | 0.002′ | fitted |
| 2026-09-20 17:37:16 UTC | 3 | 304 | U95 — USA1/HCRO, Pie Town | 0.002′ | fitted |
| 2026-09-20 18:12:16 UTC | 4 | 308 | L18 — QOS Observatory, Zalistsi | 0.002′ | fitted |
| 2026-09-20 18:13:32 UTC | 3 | 311 | M35 — PS Observatory, Parjol | 0.001′ | fitted |
| 2026-09-20 19:06:04 UTC | 3 | 314 | L99 — Novosilky | 0.001′ | fitted |
| 2026-09-20 19:16:20 UTC | 4 | 318 | C23 — Olmen | 0.001′ | fitted |
| 2026-09-20 19:30:04 UTC | 3 | 321 | C40 — Kuban State University Astrophysical Observatory | 0.001′ | fitted |
| 2026-09-20 20:19:22 UTC | 3 | 324 | 213 — Observatorio Montcabre | 0.001′ | fitted |
| 2026-09-20 20:48:01 UTC | 3 | 327 | 204 — Schiaparelli Observatory | 0.001′ | fitted |
| 2026-09-20 21:20:05 UTC | 4 | 331 | C43 — Hoyerswerda | 0.001′ | fitted |
| 2026-09-20 22:35:36 UTC | 3 | 334 | 970 — Chelmsford | 0.001′ | fitted |
| 2026-09-21 00:05:42 UTC | 2 | 336 | Z80 — Northolt Branch Observatory | 0.001′ | fitted |
| 2026-09-21 04:10:35 UTC | 4 | 340 | 703 — University of Arizona Catalina Sky Survey | 0.001′ | fitted |
| 2026-09-21 06:25:22 UTC | 3 | 343 | 718 — Tooele | 0.001′ | fitted |
| 2026-09-21 07:18:29 UTC | 6 | 349 | 193 — Sanglok | 0.001′ | fitted |
| 2026-09-21 07:43:12 UTC | 3 | 352 | V21 — Cewanee Observatory at DSNM | 0.001′ | fitted |
| 2026-09-21 10:55:34 UTC | 3 | 355 | D28 — Escaldarium Observatory,Caldes de Montbui | 0.001′ | fitted |
| 2026-09-21 19:28:48 UTC | 4 | 359 | C23 — Olmen | 0.001′ | fitted |
| 2026-09-21 21:20:09 UTC | 2 | 361 | 970 — Chelmsford | 0.001′ | fitted |
| 2026-09-21 22:02:04 UTC | 3 | 364 | I81 — Tarbatness Observatory, Portmahomack | 0.001′ | fitted |
| 2026-09-21 22:22:27 UTC | 3 | 367 | 213 — Observatorio Montcabre | 0.001′ | fitted |
| 2026-09-22 07:24:20 UTC | 6 | 373 | B96 — Brixiis Observatory, Kruibeke | 0.001′ | fitted |
| 2026-09-22 11:06:37 UTC | 3 | 376 | 900 — Moriyama | 0.001′ | fitted |
| 2026-09-22 11:07:38 UTC | 3 | 379 | Q06 — Tarui Observatory, Tarui | 0.001′ | fitted |
| 2026-09-22 11:34:04 UTC | 2 | 381 | Z80 — Northolt Branch Observatory | 0.001′ | fitted |
| 2026-09-22 19:40:13 UTC | 3 | 384 | L65 — Bredenkamp Observatory, Bremen | 0.001′ | fitted |
| 2026-09-22 20:14:45 UTC | 3 | 387 | R63 — Observatorio Sureste Estelar, Fuente Alamo | 0.001′ | fitted |
| 2026-09-22 20:27:27 UTC | 3 | 390 | 185 — Observatoire Astronomique Jurassien-Vicques | 0.001′ | fitted |
| 2026-09-22 20:35:53 UTC | 3 | 393 | 126 — Monte Viseggi L. Zannoni Observatory | 0.001′ | fitted |
| 2026-09-23 05:54:05 UTC | 5 | 398 | L27 — 29PREMOTE Observatory, Dauban | 0.001′ | fitted |
| 2026-09-23 06:08:28 UTC | 3 | 401 | 213 — Observatorio Montcabre | 0.001′ | fitted |
| 2026-09-23 06:46:27 UTC | 3 | 404 | K87 — Dettelbach Vineyard Observatory | 0.001′ | fitted |
| 2026-09-23 11:50:05 UTC | 3 | 407 | 903 — Fukuchiyama and Kannabe | 0.001′ | fitted |
| 2026-09-23 17:01:24 UTC | 4 | 411 | U94 — iTelescope Observatory, Beryl Junction | 0.001′ | fitted |
| 2026-09-23 17:55:05 UTC | 3 | 414 | C40 — Kuban State University Astrophysical Observatory | 0.001′ | fitted |
| 2026-09-23 18:22:55 UTC | 3 | 417 | A71 — Stixendorf | 0.001′ | fitted |
| 2026-09-23 19:24:01 UTC | 3 | 420 | A71 — Stixendorf | 0.001′ | fitted |
| 2026-09-23 19:38:02 UTC | 3 | 423 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-09-23 19:55:08 UTC | 5 | 428 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-09-24 00:38:26 UTC | 2 | 430 | Z80 — Northolt Branch Observatory | 0.001′ | fitted |
| 2026-09-24 04:56:04 UTC | 3 | 433 | G58 — Chabot Space and Science Center, Oakland | 0.001′ | fitted |
| 2026-09-24 07:25:04 UTC | 3 | 436 | 718 — Tooele | 0.001′ | fitted |
| 2026-09-24 12:55:35 UTC | 2 | 438 | 900 — Moriyama | 0.001′ | fitted |
| 2026-09-24 13:36:45 UTC | 5 | 443 | 658 — Dominion Astrophysical Observatory | 0.001′ | fitted |
| 2026-09-24 17:36:22 UTC | 4 | 447 | C53 — NEOSSat | 0.001′ | fitted |
| 2026-09-24 19:00:35 UTC | 4 | 451 | K74 — Muensterschwarzach Observatory, Schwarzach | 0.001′ | fitted |
| 2026-09-24 19:35:59 UTC | 3 | 454 | R59 — Camarasa Observatory, Astrocamp Nerpio | 0.001′ | fitted |
| 2026-09-24 20:43:08 UTC | 3 | 457 | J95 — Great Shefford | 0.001′ | fitted |
| 2026-09-25 00:43:07 UTC | 2 | 459 | Z80 — Northolt Branch Observatory | 0.001′ | fitted |
| 2026-09-25 05:09:10 UTC | 3 | 462 | X04 — MCD Observatory, Saint-Anaclet | 0.001′ | fitted |
| 2026-09-25 18:20:05 UTC | 5 | 467 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-09-25 18:46:37 UTC | 2 | 469 | L47 — Osservatorio Astronomico, Piobbico | 0.001′ | fitted |
| 2026-09-25 19:32:39 UTC | 2 | 471 | L47 — Osservatorio Astronomico, Piobbico | 0.001′ | fitted |
| 2026-09-25 19:39:21 UTC | 4 | 475 | C23 — Olmen | 0.001′ | fitted |
| 2026-09-25 20:47:21 UTC | 2 | 477 | R64 — Steyning Observatory | 0.001′ | fitted |
| 2026-09-26 01:15:05 UTC | 3 | 480 | P87 — Hirao Observatory, Yamaguchi | 0.001′ | fitted |
| 2026-09-26 04:55:06 UTC | 3 | 483 | 695 — Kitt Peak | 0.001′ | fitted |
| 2026-09-26 08:35:15 UTC | 3 | 486 | R92 — Osterholz-Scharmbeck | 0.001′ | fitted |
| 2026-09-26 11:02:12 UTC | 3 | 489 | D28 — Escaldarium Observatory,Caldes de Montbui | 0.001′ | fitted |
| 2026-09-26 17:50:05 UTC | 3 | 492 | M18 — Koeditz | 0.001′ | fitted |
| 2026-09-26 19:02:45 UTC | 3 | 495 | L47 — Osservatorio Astronomico, Piobbico | 0.001′ | fitted |
| 2026-09-26 21:04:39 UTC | 4 | 499 | L18 — QOS Observatory, Zalistsi | 0.001′ | fitted |
| 2026-09-26 22:05:05 UTC | 4 | 503 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-09-27 06:13:48 UTC | 3 | 506 | L99 — Novosilky | 0.001′ | fitted |
| 2026-09-27 15:15:05 UTC | 3 | 509 | M18 — Koeditz | 0.002′ | fitted |
| 2026-09-27 19:03:25 UTC | 2 | 511 | 160 — Castelmartini | 0.002′ | fitted |
| 2026-09-27 19:23:17 UTC | 3 | 514 | 595 — Farra d'Isonzo | 0.001′ | fitted |
| 2026-09-27 19:23:55 UTC | 3 | 517 | S03 — Stierlingwald, Buermoos | 0.001′ | fitted |
| 2026-09-27 19:28:22 UTC | 2 | 519 | M14 — Schiaparelli Gallarate Station | 0.001′ | fitted |
| 2026-09-27 19:36:22 UTC | 11 | 530 | B67 — Sternwarte Mirasteilas, Falera | 0.001′ | fitted |
| 2026-09-27 19:55:33 UTC | 3 | 533 | G19 — Immanuel Kant Observatory,Limbach | 0.001′ | fitted |
| 2026-09-28 01:25:11 UTC | 3 | 536 | W42 — Mind's Eye Observatory, Vero Beach | 0.001′ | fitted |
| 2026-09-28 08:23:32 UTC | 3 | 539 | A77 — Observatoire Chante-Perdrix, Dauban | 0.001′ | fitted |
| 2026-09-28 18:16:22 UTC | 2 | 541 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-09-28 18:26:34 UTC | 4 | 545 | G34 — Oberfrauendorf | 0.001′ | fitted |
| 2026-09-28 18:29:37 UTC | 2 | 547 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-09-28 18:43:49 UTC | 3 | 550 | A71 — Stixendorf | 0.001′ | fitted |
| 2026-09-28 18:55:05 UTC | 5 | 555 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-09-29 13:55:06 UTC | 3 | 558 | 367 — Yatsuka | 0.001′ | fitted |
| 2026-09-29 17:32:04 UTC | 3 | 561 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.001′ | fitted |
| 2026-09-29 19:03:27 UTC | 3 | 564 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-09-29 20:30:06 UTC | 2 | 566 | G18 — ALMO Observatory, Padulle | 0.001′ | fitted |
| 2026-09-29 22:41:10 UTC | 2 | 568 | Y05 — SONEAR Wykrota-CEAMIG, Serra da Piedade | 0.001′ | fitted |
| 2026-09-30 06:05:06 UTC | 3 | 571 | 718 — Tooele | 0.001′ | fitted |
| 2026-09-30 06:55:06 UTC | 3 | 574 | 585 — Kyiv comet station | 0.001′ | fitted |
| 2026-09-30 10:56:52 UTC | 2 | 576 | 900 — Moriyama | 0.001′ | fitted |
| 2026-09-30 17:25:56 UTC | 3 | 579 | U52 — Shasta Valley Observatory, Grenada | — | fit-error |
| 2026-09-30 18:38:35 UTC | 3 | 582 | L47 — Osservatorio Astronomico, Piobbico | 0.001′ | fitted |
| 2026-09-30 19:04:06 UTC | 3 | 585 | 160 — Castelmartini | 0.001′ | fitted |
| 2026-09-30 19:23:54 UTC | 3 | 588 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-09-30 19:54:06 UTC | 3 | 591 | K74 — Muensterschwarzach Observatory, Schwarzach | — | fit-error |
| 2026-09-30 19:54:44 UTC | 3 | 594 | L49 — VEGA-Sternwarte, Dorfleiten | 0.001′ | fitted |
| 2026-09-30 22:18:43 UTC | 2 | 596 | Z80 — Northolt Branch Observatory | 0.001′ | fitted |
| 2026-10-01 01:30:05 UTC | 5 | 601 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-10-01 05:50:05 UTC | 3 | 604 | 718 — Tooele | 0.001′ | fitted |
| 2026-10-01 07:01:08 UTC | 2 | 606 | G40 — Slooh.com Canary Islands Observatory | 0.001′ | fitted |
| 2026-10-01 07:26:30 UTC | 2 | 608 | Z24 — Tenerife Observatory-LCO B, Tenerife | 0.001′ | fitted |
| 2026-10-01 07:35:05 UTC | 2 | 610 | L07 — Osservatorio Salvatore di Giacomo, Agerola | 0.001′ | fitted |
| 2026-10-01 11:55:32 UTC | 3 | 613 | Q06 — Tarui Observatory, Tarui | 0.001′ | fitted |
| 2026-10-01 12:54:32 UTC | 3 | 616 | P13 — Baihuashan Observatory, Beijing | 0.001′ | fitted |
| 2026-10-01 14:10:07 UTC | 3 | 619 | P87 — Hirao Observatory, Yamaguchi | 0.001′ | fitted |
| 2026-10-01 18:16:36 UTC | 4 | 623 | L18 — QOS Observatory, Zalistsi | 0.001′ | fitted |
| 2026-10-01 18:58:50 UTC | 2 | 625 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-10-01 20:35:07 UTC | 2 | 627 | L07 — Osservatorio Salvatore di Giacomo, Agerola | 0.001′ | fitted |
| 2026-10-02 02:35:53 UTC | 4 | 631 | V16 — Dark Sky New Mexico, Animas | 0.001′ | fitted |
| 2026-10-02 03:00:08 UTC | 4 | 635 | 703 — University of Arizona Catalina Sky Survey | 0.001′ | fitted |
| 2026-10-02 09:31:05 UTC | 6 | 641 | A98 — Observatory Mazzarot-1, Baran' | 0.001′ | fitted |
| 2026-10-02 12:21:46 UTC | 3 | 644 | U52 — Shasta Valley Observatory, Grenada | 0.001′ | fitted |
| 2026-10-02 16:15:06 UTC | 5 | 649 | 349 — Ageo | 0.001′ | fitted |
| 2026-10-02 20:02:27 UTC | 3 | 652 | G17 — BAS Observatory, Scandicci | 0.001′ | fitted |
| 2026-10-03 02:30:27 UTC | 4 | 656 | V16 — Dark Sky New Mexico, Animas | 0.001′ | fitted |
| 2026-10-03 05:25:05 UTC | 3 | 659 | P87 — Hirao Observatory, Yamaguchi | 0.001′ | fitted |
| 2026-10-03 08:55:05 UTC | 3 | 662 | M18 — Koeditz | 0.001′ | fitted |
| 2026-10-03 10:24:36 UTC | 3 | 665 | Q06 — Tarui Observatory, Tarui | 0.001′ | fitted |
| 2026-10-03 13:45:05 UTC | 3 | 668 | Q23 — Sukagawa | 0.001′ | fitted |
| 2026-10-03 16:52:43 UTC | 3 | 671 | R92 — Osterholz-Scharmbeck | 0.001′ | fitted |
| 2026-10-03 17:28:02 UTC | 2 | 673 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-10-03 18:40:06 UTC | 3 | 676 | S45 — Station name unavailable | 0.001′ | fitted |
| 2026-10-03 18:45:09 UTC | 3 | 679 | B72 — Soerth Observatory | 0.001′ | fitted |
| 2026-10-03 18:50:04 UTC | 5 | 684 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-10-03 21:55:49 UTC | 3 | 687 | 160 — Castelmartini | 0.001′ | fitted |
| 2026-10-04 08:39:07 UTC | 2 | 689 | Q14 — Goto Astronomical Observatory in Yatsugatake | 0.001′ | fitted |
| 2026-10-04 13:15:23 UTC | 3 | 692 | P87 — Hirao Observatory, Yamaguchi | 0.001′ | fitted |
| 2026-10-04 17:49:07 UTC | 3 | 695 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-10-04 18:48:13 UTC | 3 | 698 | D56 — Osservatorio Sideris Oculus, San Pietro in Gu | 0.001′ | fitted |
| 2026-10-04 19:35:52 UTC | 6 | 704 | G19 — Immanuel Kant Observatory,Limbach | 0.001′ | fitted |
| 2026-10-04 19:50:05 UTC | 3 | 707 | M75 — Online observatory, Peschany | 0.001′ | fitted |
| 2026-10-04 20:27:47 UTC | 3 | 710 | 160 — Castelmartini | 0.001′ | fitted |
| 2026-10-05 09:45:58 UTC | 3 | 713 | R92 — Osterholz-Scharmbeck | 0.001′ | fitted |
| 2026-10-05 18:50:09 UTC | 5 | 718 | M32 — Sunny Transcarpathian, Mukachevo | 0.001′ | fitted |
| 2026-10-05 18:55:41 UTC | 4 | 722 | C23 — Olmen | 0.001′ | fitted |
| 2026-10-05 20:03:28 UTC | 10 | 732 | L27 — 29PREMOTE Observatory, Dauban | 0.001′ | fitted |
| 2026-10-05 20:05:44 UTC | 3 | 735 | B50 — Corner Observatory, Durmersheim | 0.001′ | fitted |
| 2026-10-05 20:24:30 UTC | 2 | 737 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
C46MLP1
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
C46MYX1
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
CEUDMR2
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 05:24:38 UTC | 4 | 4 | G96 — University of Arizona Mt. Lemmon Survey | 3.250′ | fitted |
| 2026-10-04 07:32:47 UTC | 4 | 8 | I52 — Steward Observatory, Mt. Lemmon Station | 0.958′ | fitted |
| 2026-10-04 07:57:13 UTC | 2 | 10 | H36 — Sandlot Observatory, Scranton | 0.059′ | fitted |
| 2026-10-05 05:19:08 UTC | 3 | 13 | G96 — University of Arizona Mt. Lemmon Survey | 0.005′ | fitted |
| 2026-10-05 05:49:22 UTC | 2 | 15 | 673 — Table Mountain Observatory, Wrightwood | 0.006′ | fitted |
| 2026-10-05 06:25:52 UTC | 4 | 19 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.004′ | fitted |
CEUEYH2
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 05:50:44 UTC | 4 | 4 | G96 — University of Arizona Mt. Lemmon Survey | 3.100′ | fitted |
| 2026-10-04 08:09:11 UTC | 4 | 8 | I52 — Steward Observatory, Mt. Lemmon Station | 0.783′ | fitted |
| 2026-10-05 05:13:29 UTC | 3 | 11 | G96 — University of Arizona Mt. Lemmon Survey | 0.008′ | fitted |
CEUKDC2
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 06:33:56 UTC | 3 | 3 | G96 — University of Arizona Mt. Lemmon Survey | 2.250′ | fitted |
| 2026-10-04 08:22:07 UTC | 3 | 6 | I52 — Steward Observatory, Mt. Lemmon Station | 0.657′ | fitted |
| 2026-10-05 05:00:07 UTC | 4 | 10 | H21 — Astronomical Research Observatory, Westfield | 0.020′ | fitted |
CEUPDC2
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 07:30:28 UTC | 3 | 3 | G96 — University of Arizona Mt. Lemmon Survey | 3.567′ | fitted |
CEUU5W2
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 09:04:13 UTC | 4 | 4 | G96 — University of Arizona Mt. Lemmon Survey | 1.917′ | fitted |
| 2026-10-04 09:12:45 UTC | 4 | 8 | G96 — University of Arizona Mt. Lemmon Survey | 0.917′ | fitted |
| 2026-10-05 05:40:05 UTC | 5 | 13 | H21 — Astronomical Research Observatory, Westfield | 0.053′ | fitted |
CEUY7A2
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
CEUZQ12
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:18:03 UTC | 3 | 3 | G96 — University of Arizona Mt. Lemmon Survey | 14.067′ | fitted |
| 2026-10-05 10:30:01 UTC | 4 | 7 | G96 — University of Arizona Mt. Lemmon Survey | 3.967′ | fitted |
| 2026-10-05 11:18:51 UTC | 3 | 10 | G96 — University of Arizona Mt. Lemmon Survey | 0.665′ | fitted |
CEUZW22
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
CEV09N2
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 11:41:55 UTC | 3 | 3 | G96 — University of Arizona Mt. Lemmon Survey | 19.417′ | fitted |
K000001
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 13:10:47 UTC | 10 | 10 | U62 — TransAstra TKO at SkiesAway | 14.517′ | fitted |
P12pwoA
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-02 10:25:01 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.800′ | fitted |
| 2026-09-05 11:27:53 UTC | 3 | 7 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.074′ | fitted |
| 2026-09-06 00:05:40 UTC | 3 | 10 | 807 — Cerro Tololo Observatory, La Serena | 0.004′ | fitted |
| 2026-09-09 03:15:05 UTC | 2 | 12 | Q62 — iTelescope Observatory, Siding Spring | 0.006′ | fitted |
P12qGDR
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P12qGDT
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-02 11:57:50 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 0.922′ | fitted |
| 2026-10-02 20:57:17 UTC | 2 | 6 | F52 — Pan-STARRS 2, Haleakala | 0.697′ | fitted |
| 2026-10-03 12:25:37 UTC | 3 | 9 | 691 — Steward Observatory, Kitt Peak-Spacewatch | 0.048′ | fitted |
P12qGGE
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-02 14:39:31 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.217′ | fitted |
| 2026-10-03 06:45:05 UTC | 4 | 8 | H21 — Astronomical Research Observatory, Westfield | 0.068′ | fitted |
| 2026-10-04 05:32:19 UTC | 2 | 10 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.021′ | fitted |
| 2026-10-04 08:40:04 UTC | 3 | 13 | H21 — Astronomical Research Observatory, Westfield | 0.006′ | fitted |
P12qMrz
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-03 13:51:44 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.117′ | fitted |
| 2026-10-03 19:19:11 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 1.260′ | fitted |
| 2026-10-03 22:57:06 UTC | 2 | 8 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.026′ | fitted |
| 2026-10-04 08:05:05 UTC | 3 | 11 | H21 — Astronomical Research Observatory, Westfield | 0.027′ | fitted |
| 2026-10-05 08:40:06 UTC | 3 | 14 | H21 — Astronomical Research Observatory, Westfield | 0.007′ | fitted |
P12qRD2
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 12:30:53 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 3.017′ | fitted |
| 2026-10-04 15:39:17 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 0.972′ | fitted |
| 2026-10-05 06:05:06 UTC | 2 | 8 | H21 — Astronomical Research Observatory, Westfield | 0.031′ | fitted |
P12qRD3
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 12:30:58 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 5.183′ | fitted |
| 2026-10-04 15:40:33 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 0.783′ | fitted |
| 2026-10-05 05:50:05 UTC | 2 | 7 | H21 — Astronomical Research Observatory, Westfield | 0.023′ | fitted |
P12qRD4
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 12:31:32 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 0.967′ | fitted |
| 2026-10-04 15:42:00 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 1.055′ | fitted |
| 2026-10-05 06:25:04 UTC | 3 | 9 | H21 — Astronomical Research Observatory, Westfield | 0.031′ | fitted |
P12qRD5
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 12:31:42 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 4.533′ | fitted |
| 2026-10-04 15:43:32 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 1.398′ | fitted |
| 2026-10-05 07:30:06 UTC | 2 | 7 | H21 — Astronomical Research Observatory, Westfield | 0.016′ | fitted |
P12qRQV
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 13:37:32 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.468′ | fitted |
| 2026-10-04 15:44:45 UTC | 2 | 6 | F52 — Pan-STARRS 2, Haleakala | 1.042′ | fitted |
| 2026-10-05 08:10:10 UTC | 3 | 9 | H21 — Astronomical Research Observatory, Westfield | 0.039′ | fitted |
P12qRQW
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 13:37:35 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.933′ | fitted |
| 2026-10-04 15:45:49 UTC | 2 | 6 | F52 — Pan-STARRS 2, Haleakala | 0.595′ | fitted |
| 2026-10-05 07:55:06 UTC | 4 | 10 | H21 — Astronomical Research Observatory, Westfield | 0.030′ | fitted |
P12qRUu
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 15:08:11 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 0.492′ | fitted |
P12qZCA
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 21:36:33 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 92.650′ | fitted |
P12qZDO
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P12qZDP
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 22:16:37 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 760.000′ | fitted |
P12qZLd
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P12qZLf
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:36:29 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 2.183′ | fitted |
P12qZLl
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:37:36 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.365′ | fitted |
P12qfMj
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-16 11:20:18 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 0.720′ | fitted |
| 2026-09-16 20:50:18 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 0.500′ | fitted |
| 2026-09-20 08:20:30 UTC | 3 | 9 | I52 — Steward Observatory, Mt. Lemmon Station | 0.019′ | fitted |
| 2026-09-20 18:18:06 UTC | 10 | 19 | F51 — Pan-STARRS 1, Haleakala, F52 — Pan-STARRS 2, Haleakala | 0.001′ | fitted |
| 2026-09-21 12:02:38 UTC | 3 | 22 | T14 — Canada-France-Hawaii Telescope, Maunakea | 8.300′ | fitted |
| 2026-09-22 02:00:26 UTC | 2 | 24 | Q62 — iTelescope Observatory, Siding Spring | 0.000′ | fitted |
| 2026-10-05 19:53:06 UTC | 3 | 27 | T12 — University of Hawaii 88-inch telescope, Maunakea | 0.001′ | fitted |
P12qz2H
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-29 15:11:52 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 2.150′ | fitted |
| 2026-10-01 04:09:26 UTC | 3 | 7 | 807 — Cerro Tololo Observatory, La Serena | 0.088′ | fitted |
| 2026-10-03 16:11:16 UTC | 4 | 11 | 474 — Mount John Observatory, Lake Tekapo | 0.009′ | fitted |
| 2026-10-04 05:47:32 UTC | 3 | 14 | M49 — IAS Remote Observatory, Hakos | 0.001′ | fitted |
| 2026-10-04 21:37:27 UTC | 2 | 16 | M21 — Schiaparelli Southern Observatory, Hakos | 0.003′ | fitted |
P12qzuD
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-01 11:40:07 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 7.900′ | fitted |
| 2026-10-02 21:00:24 UTC | 2 | 5 | F52 — Pan-STARRS 2, Haleakala | 0.630′ | fitted |
| 2026-10-03 04:55:05 UTC | 5 | 10 | H21 — Astronomical Research Observatory, Westfield | 0.029′ | fitted |
P12r01e
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 12:46:19 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 4.000′ | fitted |
P12r01f
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P12r01o
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 12:47:42 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 1.410′ | fitted |
P12r02P
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 14:01:51 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 4.067′ | fitted |
P12r02Q
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 14:02:41 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 4.100′ | fitted |
P12r02R
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 14:02:52 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 6.367′ | fitted |
P12r02S
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P22oLCM
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-08-03 12:10:42 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.500′ | fitted |
| 2026-08-04 00:13:24 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 0.640′ | fitted |
| 2026-08-04 06:10:06 UTC | 2 | 8 | H21 — Astronomical Research Observatory, Westfield | 0.017′ | fitted |
| 2026-08-04 13:05:52 UTC | 4 | 12 | F52 — Pan-STARRS 2, Haleakala | 0.007′ | fitted |
| 2026-08-06 13:55:01 UTC | 3 | 15 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.000′ | fitted |
| 2026-08-08 16:49:06 UTC | 2 | 17 | F51 — Pan-STARRS 1, Haleakala | 0.003′ | fitted |
| 2026-08-14 03:15:12 UTC | 2 | 19 | Q62 — iTelescope Observatory, Siding Spring | 0.005′ | fitted |
| 2026-09-04 21:19:35 UTC | 3 | 22 | M57 — Wide-field Mufara Telescope, Isnello | 0.003′ | fitted |
| 2026-09-06 05:10:02 UTC | 3 | 25 | G00 — AZM Martinsberg, Oed | 0.002′ | fitted |
| 2026-09-25 12:24:47 UTC | 7 | 32 | F51 — Pan-STARRS 1, Haleakala | 0.009′ | fitted |
| 2026-10-01 05:47:24 UTC | 3 | 35 | 691 — Steward Observatory, Kitt Peak-Spacewatch | 0.004′ | fitted |
| 2026-10-05 20:00:57 UTC | 3 | 38 | T12 — University of Hawaii 88-inch telescope, Maunakea | 0.002′ | fitted |
P22oVrz
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-08-06 18:42:50 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 14.117′ | fitted |
| 2026-08-07 13:04:03 UTC | 3 | 6 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.042′ | fitted |
| 2026-08-07 19:05:05 UTC | 2 | 8 | L01 — Visnjan Observatory, Tican | 0.017′ | fitted |
| 2026-08-07 19:26:28 UTC | 2 | 10 | J95 — Great Shefford | 0.006′ | fitted |
| 2026-08-07 19:38:57 UTC | 4 | 14 | F51 — Pan-STARRS 1, Haleakala | 0.005′ | fitted |
| 2026-08-08 12:15:51 UTC | 3 | 17 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.008′ | fitted |
| 2026-08-15 16:10:06 UTC | 2 | 19 | Q62 — iTelescope Observatory, Siding Spring | 0.004′ | fitted |
| 2026-09-04 11:32:33 UTC | 3 | 22 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.001′ | fitted |
| 2026-09-25 12:38:29 UTC | 3 | 25 | F51 — Pan-STARRS 1, Haleakala | 0.070′ | fitted |
P22pKXS
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-05 17:35:01 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 5.200′ | fitted |
| 2026-09-06 06:45:37 UTC | 3 | 6 | 807 — Cerro Tololo Observatory, La Serena | 0.042′ | fitted |
| 2026-09-07 05:05:05 UTC | 3 | 9 | H21 — Astronomical Research Observatory, Westfield | 0.002′ | fitted |
| 2026-09-11 06:46:50 UTC | 3 | 12 | R48 — Centro Astronomico Alto Turia 2 | 0.003′ | fitted |
| 2026-09-15 11:50:06 UTC | 2 | 14 | Q62 — iTelescope Observatory, Siding Spring | 0.013′ | fitted |
| 2026-09-25 12:40:32 UTC | 4 | 18 | F51 — Pan-STARRS 1, Haleakala | 0.192′ | fitted |
| 2026-10-05 20:05:59 UTC | 3 | 21 | T12 — University of Hawaii 88-inch telescope, Maunakea | 0.014′ | fitted |
P22qGC1
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-01 23:45:22 UTC | 5 | 5 | K88 — GINOP-KHK, Piszkesteto | 6.083′ | fitted |
| 2026-10-02 02:20:05 UTC | 6 | 11 | K88 — GINOP-KHK, Piszkesteto | 0.428′ | fitted |
| 2026-10-02 11:35:19 UTC | 2 | 13 | F52 — Pan-STARRS 2, Haleakala | 0.006′ | fitted |
| 2026-10-02 11:55:22 UTC | 1 | 14 | F52 — Pan-STARRS 2, Haleakala | 0.006′ | fitted |
| 2026-10-02 19:45:05 UTC | 3 | 17 | K88 — GINOP-KHK, Piszkesteto | 0.004′ | fitted |
| 2026-10-02 21:09:06 UTC | 2 | 19 | F51 — Pan-STARRS 1, Haleakala | 0.006′ | fitted |
| 2026-10-02 22:41:16 UTC | 2 | 21 | J95 — Great Shefford | 0.004′ | fitted |
| 2026-10-03 04:15:05 UTC | 3 | 24 | H21 — Astronomical Research Observatory, Westfield | 0.004′ | fitted |
| 2026-10-03 19:23:15 UTC | 2 | 26 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.005′ | fitted |
| 2026-10-03 20:10:04 UTC | 3 | 29 | K88 — GINOP-KHK, Piszkesteto | 0.004′ | fitted |
| 2026-10-03 20:31:32 UTC | 3 | 32 | S45 — Station name unavailable | 0.004′ | fitted |
| 2026-10-03 22:17:11 UTC | 2 | 34 | 703 — University of Arizona Catalina Sky Survey | 0.004′ | fitted |
| 2026-10-03 22:23:02 UTC | 2 | 36 | D63 — G. Pascoli Observatory, Barga (since June 2023) | 0.003′ | fitted |
| 2026-10-04 12:01:49 UTC | 2 | 38 | F52 — Pan-STARRS 2, Haleakala | 0.004′ | fitted |
P22qGG2
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-02 13:45:10 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 1.950′ | fitted |
| 2026-10-02 21:04:10 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 0.508′ | fitted |
| 2026-10-03 02:50:05 UTC | 5 | 10 | H21 — Astronomical Research Observatory, Westfield | 0.039′ | fitted |
| 2026-10-03 22:04:17 UTC | 2 | 12 | J95 — Great Shefford | 0.008′ | fitted |
P22qGG4
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-02 13:45:17 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 2.017′ | fitted |
| 2026-10-02 21:04:55 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 0.497′ | fitted |
| 2026-10-03 05:20:05 UTC | 4 | 9 | H21 — Astronomical Research Observatory, Westfield | 0.014′ | fitted |
P22qGGJ
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-02 15:38:28 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 3.417′ | fitted |
P22qGnU
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-01 21:09:17 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 26.683′ | fitted |
P22qMeV
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P22qMlB
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-03 11:18:30 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 4.683′ | fitted |
| 2026-10-03 15:39:24 UTC | 4 | 7 | 474 — Mount John Observatory, Lake Tekapo | 0.110′ | fitted |
| 2026-10-03 19:22:10 UTC | 2 | 9 | F52 — Pan-STARRS 2, Haleakala | 0.080′ | fitted |
| 2026-10-03 20:14:20 UTC | 2 | 11 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.006′ | fitted |
| 2026-10-05 00:40:05 UTC | 2 | 13 | L01 — Visnjan Observatory, Tican | 0.004′ | fitted |
P22qRPP
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 13:25:13 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.390′ | fitted |
| 2026-10-04 15:48:10 UTC | 2 | 5 | F52 — Pan-STARRS 2, Haleakala | 0.452′ | fitted |
| 2026-10-04 16:01:03 UTC | 4 | 9 | 474 — Mount John Observatory, Lake Tekapo | 0.014′ | fitted |
| 2026-10-05 08:25:05 UTC | 2 | 11 | H21 — Astronomical Research Observatory, Westfield | 0.002′ | fitted |
P22qRQt
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 13:26:07 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.262′ | fitted |
| 2026-10-04 15:50:07 UTC | 2 | 6 | F52 — Pan-STARRS 2, Haleakala | 0.253′ | fitted |
| 2026-10-04 23:45:05 UTC | 2 | 8 | L01 — Visnjan Observatory, Tican | 0.023′ | fitted |
| 2026-10-05 00:39:31 UTC | 2 | 10 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.023′ | fitted |
| 2026-10-05 07:40:05 UTC | 2 | 12 | H21 — Astronomical Research Observatory, Westfield | 0.025′ | fitted |
P22qRQu
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 13:26:12 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.121′ | fitted |
| 2026-10-04 15:51:12 UTC | 2 | 6 | F52 — Pan-STARRS 2, Haleakala | 0.160′ | fitted |
| 2026-10-05 08:55:05 UTC | 3 | 9 | H21 — Astronomical Research Observatory, Westfield | 0.018′ | fitted |
P22qRk5
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-03 21:08:48 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 806.000′ | fitted |
P22qRk6
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P22qRmB
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 08:29:10 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 1.015′ | fitted |
| 2026-10-04 15:54:00 UTC | 3 | 6 | F52 — Pan-STARRS 2, Haleakala | 0.685′ | fitted |
| 2026-10-05 04:25:05 UTC | 3 | 9 | H21 — Astronomical Research Observatory, Westfield | 0.039′ | fitted |
P22qRmb
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P22qRra
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 11:29:47 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 1.043′ | fitted |
| 2026-10-04 15:57:24 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 0.365′ | fitted |
| 2026-10-05 06:33:26 UTC | 2 | 8 | 673 — Table Mountain Observatory, Wrightwood | 0.002′ | fitted |
P22qZFD
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P22qZL4
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 09:20:58 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 1.275′ | fitted |
P22qZNR
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:44:39 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.056′ | fitted |
P22qZNT
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:44:48 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.240′ | fitted |
P22qZNU
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:44:58 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.215′ | fitted |
P22qZNV
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:45:01 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.557′ | fitted |
P22qZNW
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:45:04 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.153′ | fitted |
P22qZSN
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:53:30 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 1.817′ | fitted |
P22qZSU
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
P22qZSn
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 10:49:34 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 10.550′ | fitted |
P22qZTc
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 11:54:52 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.190′ | fitted |
P22qZVl
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 11:57:20 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.312′ | fitted |
P22qZZr
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 12:28:40 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.242′ | fitted |
P22qZZs
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 12:28:53 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.678′ | fitted |
P22qZZt
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 12:30:18 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.697′ | fitted |
P22qz1V
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-28 18:25:24 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 4.600′ | fitted |
P22qzx6
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-01 11:52:06 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 1.588′ | fitted |
| 2026-10-02 02:40:22 UTC | 3 | 7 | 807 — Cerro Tololo Observatory, La Serena | 0.066′ | fitted |
| 2026-10-03 23:40:25 UTC | 4 | 11 | T12 — University of Hawaii 88-inch telescope, Maunakea | 0.007′ | fitted |
P22r47C
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 18:39:38 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 1.288′ | fitted |
SWAN26Q
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-09-05 02:39:20 UTC | 8 | 8 | 249 — SOHO | — | fit-error |
| 2026-09-06 01:55:49 UTC | 4 | 12 | 247 — Roving Observer | — | fit-error |
| 2026-09-06 17:58:14 UTC | 4 | 16 | 314 — Station name unavailable | — | fit-error |
| 2026-09-06 18:11:58 UTC | 3 | 19 | 311 — Station name unavailable | — | fit-error |
| 2026-09-06 18:50:16 UTC | 5 | 24 | C49 — STEREO-A | — | fit-error |
| 2026-09-06 20:14:18 UTC | 33 | 57 | 335 — PUNCH | — | fit-error |
| 2026-09-08 00:10:33 UTC | 2 | 59 | 247 — Roving Observer | — | fit-error |
| 2026-09-16 18:19:49 UTC | 25 | 84 | 335 — PUNCH | — | fit-error |
Sar2932
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-04 19:55:05 UTC | 3 | 3 | K88 — GINOP-KHK, Piszkesteto | 17.183′ | fitted |
| 2026-10-04 20:15:06 UTC | 2 | 5 | K88 — GINOP-KHK, Piszkesteto | 5.833′ | fitted |
| 2026-10-04 20:30:05 UTC | 4 | 9 | L01 — Visnjan Observatory, Tican | 0.212′ | fitted |
| 2026-10-04 21:11:38 UTC | 2 | 11 | 126 — Monte Viseggi L. Zannoni Observatory | 0.407′ | fitted |
| 2026-10-04 21:22:26 UTC | 2 | 13 | J95 — Great Shefford | 0.058′ | fitted |
| 2026-10-04 21:30:22 UTC | 2 | 15 | M38 — Harsona Observatory, Nyiregyhaza | 0.009′ | fitted |
| 2026-10-04 21:44:06 UTC | 2 | 17 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.013′ | fitted |
| 2026-10-04 21:56:41 UTC | 3 | 20 | 595 — Farra d'Isonzo | 0.007′ | fitted |
| 2026-10-04 22:15:04 UTC | 2 | 22 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.013′ | fitted |
| 2026-10-04 23:03:25 UTC | 3 | 25 | Z43 — Landehen | 0.007′ | fitted |
| 2026-10-05 00:46:17 UTC | 3 | 28 | W13 — Star Quarry Observatory, Bedford | 0.010′ | fitted |
| 2026-10-05 01:30:05 UTC | 3 | 31 | K88 — GINOP-KHK, Piszkesteto | 0.004′ | fitted |
| 2026-10-05 01:38:34 UTC | 2 | 33 | H36 — Sandlot Observatory, Scranton | 0.004′ | fitted |
| 2026-10-05 01:55:05 UTC | 4 | 37 | H21 — Astronomical Research Observatory, Westfield | 0.004′ | fitted |
| 2026-10-05 06:38:15 UTC | 3 | 40 | 703 — University of Arizona Catalina Sky Survey | 0.001′ | fitted |
| 2026-10-05 12:28:24 UTC | 2 | 42 | M21 — Schiaparelli Southern Observatory, Hakos | 0.004′ | fitted |
| 2026-10-05 13:36:38 UTC | 4 | 46 | P13 — Baihuashan Observatory, Beijing | 0.003′ | fitted |
| 2026-10-05 18:10:19 UTC | 3 | 49 | M35 — PS Observatory, Parjol | 0.004′ | fitted |
| 2026-10-05 19:55:06 UTC | 3 | 52 | I93 — St Pardon de Conques | 0.004′ | fitted |
| 2026-10-05 20:34:33 UTC | 3 | 55 | K74 — Muensterschwarzach Observatory, Schwarzach | 0.004′ | fitted |
| 2026-10-05 20:34:51 UTC | 3 | 58 | G34 — Oberfrauendorf | 0.004′ | fitted |
Sar2936
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 00:20:05 UTC | 3 | 3 | K88 — GINOP-KHK, Piszkesteto | 6.500′ | fitted |
| 2026-10-05 00:30:05 UTC | 2 | 5 | K88 — GINOP-KHK, Piszkesteto | 1.230′ | fitted |
| 2026-10-05 01:35:05 UTC | 3 | 8 | L01 — Visnjan Observatory, Tican | 0.257′ | fitted |
| 2026-10-05 02:01:37 UTC | 2 | 10 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.103′ | fitted |
| 2026-10-05 03:09:43 UTC | 2 | 12 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.121′ | fitted |
| 2026-10-05 03:30:05 UTC | 2 | 14 | H21 — Astronomical Research Observatory, Westfield | 0.010′ | fitted |
| 2026-10-05 06:10:02 UTC | 2 | 16 | 673 — Table Mountain Observatory, Wrightwood | 0.003′ | fitted |
| 2026-10-05 06:56:13 UTC | 3 | 19 | H36 — Sandlot Observatory, Scranton | 0.003′ | fitted |
Sar2937
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 20:15:05 UTC | 3 | 3 | K88 — GINOP-KHK, Piszkesteto | 1.563′ | fitted |
W000001
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
X90690
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 19:29:34 UTC | 3 | 3 | D29 — Purple Mountain Observatory, XuYi Station | 7.233′ | fitted |
X90801
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 20:46:29 UTC | 3 | 3 | D29 — Purple Mountain Observatory, XuYi Station | 4.500′ | fitted |
XAanmXA
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-05 13:26:39 UTC | 3 | 3 | N94 — Altay Astronomical Observatory | 799.000′ | fitted |
ZTF10GW
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
| Submission UTC | New observations | Cumulative observations | Stations | Uncertainty at submission | Fit status |
|---|---|---|---|---|---|
| 2026-10-03 06:23:58 UTC | 4 | 4 | I41 — Palomar Mountain--ZTF | 2,940.000′ | fitted |
ZTF10Gb
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.
ec0001
Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.