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.
6H63821
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 |
|---|---|---|---|---|---|
| 2026-08-07 06:10:19 UTC | 3 | 3 | W94 — MAPS, San Pedro de Atacama | 13.400′ | fitted |
| 2026-08-07 07:10:06 UTC | 3 | 6 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 0.660′ | fitted |
| 2026-08-07 23:38:33 UTC | 2 | 8 | M21 — Schiaparelli Southern Observatory, Hakos | 0.009′ | fitted |
| 2026-08-08 04:10:05 UTC | 3 | 11 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 0.003′ | fitted |
| 2026-08-08 06:25:05 UTC | 3 | 14 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 0.002′ | fitted |
| 2026-08-09 05:30:04 UTC | 6 | 20 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 0.002′ | fitted |
| 2026-08-09 06:50:17 UTC | 2 | 22 | M21 — Schiaparelli Southern Observatory, Hakos | 0.002′ | fitted |
| 2026-08-14 00:40:58 UTC | 1 | 23 | F52 — Pan-STARRS 2, Haleakala | 0.022′ | fitted |
| 2026-08-15 23:29:16 UTC | 2 | 25 | M21 — Schiaparelli Southern Observatory, Hakos | 0.003′ | fitted |
6H63K21
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.
6H74C22
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 |
|---|---|---|---|---|---|
| 2026-08-08 08:25:04 UTC | 3 | 3 | W94 — MAPS, San Pedro de Atacama | 14.967′ | fitted |
| 2026-08-08 08:55:04 UTC | 3 | 6 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 0.707′ | fitted |
| 2026-08-09 09:30:04 UTC | 3 | 9 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 0.016′ | fitted |
| 2026-08-14 00:43:15 UTC | 3 | 12 | F51 — Pan-STARRS 1, Haleakala | 0.020′ | fitted |
6HE2A22
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 |
|---|---|---|---|---|---|
| 2026-08-15 13:10:06 UTC | 3 | 3 | W94 — MAPS, San Pedro de Atacama | 768.000′ | fitted |
| 2026-08-15 13:20:05 UTC | 3 | 6 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 1.418′ | fitted |
| 2026-08-15 20:00:19 UTC | 2 | 8 | K88 — GINOP-KHK, Piszkesteto | 0.023′ | fitted |
| 2026-08-15 20:08:48 UTC | 4 | 12 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.019′ | fitted |
| 2026-08-15 20:20:04 UTC | 3 | 15 | L01 — Visnjan Observatory, Tican | 0.016′ | fitted |
| 2026-08-15 20:51:56 UTC | 2 | 17 | M49 — IAS Remote Observatory, Hakos | 0.005′ | fitted |
| 2026-08-15 21:01:17 UTC | 4 | 21 | 106 — Crni Vrh | 0.004′ | fitted |
| 2026-08-15 21:34:10 UTC | 3 | 24 | 595 — Farra d'Isonzo | 0.005′ | fitted |
| 2026-08-15 22:07:46 UTC | 2 | 26 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.004′ | fitted |
| 2026-08-15 22:11:45 UTC | 2 | 28 | L47 — Osservatorio Astronomico, Piobbico | 0.004′ | fitted |
| 2026-08-15 22:14:03 UTC | 2 | 30 | G34 — Oberfrauendorf | 0.004′ | fitted |
| 2026-08-15 22:15:05 UTC | 2 | 32 | 104 — San Marcello Pistoiese | 0.004′ | fitted |
| 2026-08-15 23:03:48 UTC | 2 | 34 | Z43 — Landehen | 0.004′ | fitted |
| 2026-08-15 23:05:05 UTC | 3 | 37 | K51 — Osservatorio del Celado, Castello Tesino | 0.003′ | fitted |
| 2026-08-15 23:21:57 UTC | 3 | 40 | J95 — Great Shefford | 0.003′ | fitted |
| 2026-08-15 23:48:42 UTC | 4 | 44 | L18 — QOS Observatory, Zalistsi | 0.003′ | fitted |
| 2026-08-16 01:40:30 UTC | 3 | 47 | I41 — Palomar Mountain--ZTF | 0.003′ | fitted |
| 2026-08-16 04:15:18 UTC | 5 | 52 | H21 — Astronomical Research Observatory, Westfield | 0.003′ | fitted |
| 2026-08-16 19:00:06 UTC | 3 | 55 | M75 — Online observatory, Peschany | 0.003′ | fitted |
| 2026-08-16 19:01:49 UTC | 2 | 57 | 204 — Schiaparelli Observatory | 0.003′ | fitted |
6HF2521
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 |
|---|---|---|---|---|---|
| 2026-08-16 04:55:05 UTC | 3 | 3 | W94 — MAPS, San Pedro de Atacama | 5.717′ | fitted |
| 2026-08-16 05:35:06 UTC | 3 | 6 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 1.363′ | fitted |
| 2026-08-16 06:39:54 UTC | 2 | 8 | 673 — Table Mountain Observatory, Wrightwood | 0.013′ | fitted |
| 2026-08-16 13:28:01 UTC | 4 | 12 | I41 — Palomar Mountain--ZTF | 0.178′ | fitted |
| 2026-08-16 14:04:34 UTC | 5 | 17 | 474 — Mount John Observatory, Lake Tekapo | 0.005′ | fitted |
A11FAuF
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.
E000011
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 |
|---|---|---|---|---|---|
| 2026-08-13 22:30:40 UTC | 2 | 2 | 151 — Eschenberg Observatory, Winterthur | — | insufficient-observations |
LA0Cq3L
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 |
|---|---|---|---|---|---|
| 2026-08-14 17:07:12 UTC | 4 | 4 | P07 — Space Surveillance Telescope, HEH Station | 1.700′ | fitted |
LA0Cq3M
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 |
|---|---|---|---|---|---|
| 2026-08-14 17:07:18 UTC | 5 | 5 | P07 — Space Surveillance Telescope, HEH Station | 1.700′ | fitted |
LA0Cq3N
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 |
|---|---|---|---|---|---|
| 2026-08-14 17:07:18 UTC | 5 | 5 | P07 — Space Surveillance Telescope, HEH Station | 4.100′ | fitted |
OP90566
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 |
|---|---|---|---|---|---|
| 2026-08-11 14:55:22 UTC | 3 | 3 | O18 — WFST, Lenghu | 473.000′ | fitted |
P12oO5R
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 |
|---|---|---|---|---|---|
| 2026-08-04 12:39:57 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.300′ | fitted |
| 2026-08-04 16:40:09 UTC | 2 | 6 | F52 — Pan-STARRS 2, Haleakala | 0.372′ | fitted |
| 2026-08-07 13:55:49 UTC | 4 | 10 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.023′ | fitted |
P12oVNR
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 |
|---|---|---|---|---|---|
| 2026-08-07 10:03:43 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 1.585′ | fitted |
P12oVRq
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 |
|---|---|---|---|---|---|
| 2026-08-07 11:16:13 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.198′ | fitted |
P12oVRt
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 |
|---|---|---|---|---|---|
| 2026-08-07 11:16:26 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 2.683′ | fitted |
P12oZg1
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.
P12oZh1
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 |
|---|---|---|---|---|---|
| 2026-08-08 12:39:04 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 2.117′ | fitted |
| 2026-08-08 16:41:00 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 0.507′ | fitted |
| 2026-08-09 06:14:58 UTC | 4 | 9 | H01 — Magdalena Ridge Observatory, Socorro | 0.020′ | fitted |
P12oZkE
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.
P12oZmo
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 |
|---|---|---|---|---|---|
| 2026-08-08 12:47:52 UTC | 2 | 2 | F51 — Pan-STARRS 1, Haleakala | — | insufficient-observations |
| 2026-08-08 13:49:15 UTC | 1 | 3 | F51 — Pan-STARRS 1, Haleakala | 6.867′ | fitted |
| 2026-08-08 16:47:11 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 0.725′ | fitted |
| 2026-08-14 01:06:27 UTC | 4 | 9 | F51 — Pan-STARRS 1, Haleakala | 2.750′ | fitted |
P12onNw
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 |
|---|---|---|---|---|---|
| 2026-07-14 19:17:30 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 2.567′ | fitted |
| 2026-07-15 10:47:07 UTC | 2 | 6 | Y05 — SONEAR Wykrota-CEAMIG, Serra da Piedade | 0.061′ | fitted |
| 2026-07-15 11:46:30 UTC | 3 | 9 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.002′ | fitted |
| 2026-07-15 20:37:36 UTC | 8 | 17 | I41 — Palomar Mountain--ZTF | 0.004′ | fitted |
| 2026-07-17 21:56:41 UTC | 3 | 20 | B74 — Santa Maria de Montmagastrell | 0.005′ | fitted |
| 2026-07-18 05:05:05 UTC | 3 | 23 | L06 — Sormano 2 Observatory, Bellagio Via Lattea | 0.003′ | fitted |
| 2026-07-18 22:03:01 UTC | 3 | 26 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.002′ | fitted |
| 2026-07-19 06:38:43 UTC | 2 | 28 | M21 — Schiaparelli Southern Observatory, Hakos | 0.003′ | fitted |
| 2026-07-20 05:06:52 UTC | 2 | 30 | 673 — Table Mountain Observatory, Wrightwood | 0.000′ | fitted |
| 2026-07-20 06:41:32 UTC | 2 | 32 | W62 — Comet Hunter Observatory2, New Ringgold | 0.005′ | fitted |
| 2026-07-20 14:40:05 UTC | 2 | 34 | Q62 — iTelescope Observatory, Siding Spring | 0.006′ | fitted |
| 2026-07-22 05:34:28 UTC | 3 | 37 | R59 — Camarasa Observatory, Astrocamp Nerpio | 0.003′ | fitted |
| 2026-07-22 13:43:44 UTC | 3 | 40 | T12 — University of Hawaii 88-inch telescope, Maunakea | 0.001′ | fitted |
| 2026-07-24 04:44:08 UTC | 3 | 43 | W62 — Comet Hunter Observatory2, New Ringgold | 0.003′ | fitted |
| 2026-07-24 22:30:05 UTC | 2 | 45 | G02 — KYSUCE Observatory, Kysucke Nove Mesto | 0.003′ | fitted |
| 2026-07-31 13:42:12 UTC | 6 | 51 | 658 — Dominion Astrophysical Observatory | 0.003′ | fitted |
| 2026-08-05 22:57:40 UTC | 3 | 54 | M57 — Wide-field Mufara Telescope, Isnello | 0.003′ | fitted |
| 2026-08-07 00:15:18 UTC | 3 | 57 | Z31 — Tenerife Observatory-LCO A, Tenerife | 0.002′ | fitted |
| 2026-08-07 05:50:20 UTC | 3 | 60 | R49 — Observatorio Villuercas-Navezuelas, Navezuelas | 0.002′ | fitted |
| 2026-08-07 20:39:02 UTC | 4 | 64 | F51 — Pan-STARRS 1, Haleakala | 0.002′ | fitted |
| 2026-08-07 23:08:53 UTC | 2 | 66 | 104 — San Marcello Pistoiese | 0.002′ | fitted |
| 2026-08-14 20:19:35 UTC | 2 | 68 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.004′ | fitted |
| 2026-08-16 10:44:10 UTC | 3 | 71 | G00 — AZM Martinsberg, Oed | 0.003′ | fitted |
P12p4AH
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.
P12p4HJ
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 |
|---|---|---|---|---|---|
| 2026-08-09 13:54:49 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 3.250′ | fitted |
P12p4Jx
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 |
|---|---|---|---|---|---|
| 2026-08-09 15:48:49 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 0.627′ | fitted |
| 2026-08-09 16:44:29 UTC | 1 | 5 | F51 — Pan-STARRS 1, Haleakala | 0.198′ | fitted |
| 2026-08-10 07:09:05 UTC | 3 | 8 | W62 — Comet Hunter Observatory2, New Ringgold | 0.024′ | fitted |
| 2026-08-12 06:08:29 UTC | 3 | 11 | L27 — 29PREMOTE Observatory, Dauban | 0.007′ | fitted |
| 2026-08-13 12:24:57 UTC | 3 | 14 | G00 — AZM Martinsberg, Oed | 0.045′ | fitted |
| 2026-08-13 22:52:48 UTC | 2 | 16 | 126 — Monte Viseggi L. Zannoni Observatory | 0.007′ | fitted |
| 2026-08-14 01:30:06 UTC | 2 | 18 | L01 — Visnjan Observatory, Tican | 0.005′ | fitted |
| 2026-08-14 01:40:05 UTC | 4 | 22 | Z24 — Tenerife Observatory-LCO B, Tenerife | 0.004′ | fitted |
| 2026-08-14 03:15:12 UTC | 2 | 24 | Q62 — iTelescope Observatory, Siding Spring | 0.003′ | fitted |
| 2026-08-14 04:17:51 UTC | 3 | 27 | L27 — 29PREMOTE Observatory, Dauban | 0.003′ | fitted |
| 2026-08-14 15:28:18 UTC | 2 | 29 | G00 — AZM Martinsberg, Oed | 0.004′ | fitted |
| 2026-08-14 23:01:30 UTC | 2 | 31 | K83 — Osservatorio Astronomico Beppe Forti, Montelupo | 0.004′ | fitted |
| 2026-08-16 18:16:39 UTC | 4 | 35 | V21 — Cewanee Observatory at DSNM | 0.004′ | fitted |
| 2026-08-16 19:25:36 UTC | 4 | 39 | I41 — Palomar Mountain--ZTF | 0.003′ | fitted |
P12p4s9
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 |
|---|---|---|---|---|---|
| 2026-08-08 21:32:05 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 944.000′ | fitted |
P12p4sf
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 |
|---|---|---|---|---|---|
| 2026-08-08 21:40:07 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 4.617′ | fitted |
P12p4zJ
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 |
|---|---|---|---|---|---|
| 2026-08-09 12:34:07 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 3.217′ | fitted |
| 2026-08-11 12:51:31 UTC | 4 | 8 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.060′ | fitted |
| 2026-08-14 07:30:52 UTC | 3 | 11 | M21 — Schiaparelli Southern Observatory, Hakos | 0.004′ | fitted |
P12p4zK
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.
P12paCn
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 |
|---|---|---|---|---|---|
| 2026-08-11 15:49:42 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.585′ | fitted |
| 2026-08-12 08:40:06 UTC | 3 | 7 | H21 — Astronomical Research Observatory, Westfield | 0.062′ | fitted |
| 2026-08-12 14:30:56 UTC | 3 | 10 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.021′ | fitted |
P12pap5
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.
P12papq
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 |
|---|---|---|---|---|---|
| 2026-08-11 09:37:37 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 25.717′ | fitted |
| 2026-08-11 20:09:06 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 7.983′ | fitted |
| 2026-08-11 21:23:07 UTC | 2 | 7 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.044′ | fitted |
P12patY
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.
P12patZ
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 |
|---|---|---|---|---|---|
| 2026-08-11 11:57:51 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 3.117′ | fitted |
| 2026-08-11 20:44:22 UTC | 2 | 5 | F52 — Pan-STARRS 2, Haleakala | 1.415′ | fitted |
| 2026-08-14 13:54:05 UTC | 3 | 8 | 474 — Mount John Observatory, Lake Tekapo | 0.002′ | fitted |
P12payP
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 |
|---|---|---|---|---|---|
| 2026-08-11 14:30:31 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 6.017′ | fitted |
| 2026-08-11 20:14:03 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 1.108′ | fitted |
| 2026-08-11 23:45:08 UTC | 3 | 8 | L01 — Visnjan Observatory, Tican | 0.011′ | fitted |
| 2026-08-12 06:30:05 UTC | 3 | 11 | H21 — Astronomical Research Observatory, Westfield | 0.008′ | fitted |
| 2026-08-12 06:35:21 UTC | 3 | 14 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.007′ | fitted |
| 2026-08-12 23:26:00 UTC | 4 | 18 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.009′ | fitted |
| 2026-08-13 00:40:05 UTC | 3 | 21 | I93 — St Pardon de Conques | 0.008′ | fitted |
| 2026-08-13 23:34:00 UTC | 4 | 25 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.006′ | fitted |
| 2026-08-16 00:20:10 UTC | 2 | 27 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.004′ | fitted |
| 2026-08-16 19:16:42 UTC | 4 | 31 | I41 — Palomar Mountain--ZTF | 0.003′ | fitted |
P12payW
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.
P12pb3b
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 |
|---|---|---|---|---|---|
| 2026-08-11 16:00:55 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 0.327′ | fitted |
| 2026-08-12 06:19:31 UTC | 3 | 7 | L27 — 29PREMOTE Observatory, Dauban | 0.023′ | fitted |
| 2026-08-12 14:35:44 UTC | 3 | 10 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.004′ | fitted |
| 2026-08-13 05:54:20 UTC | 4 | 14 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.009′ | fitted |
| 2026-08-13 11:45:10 UTC | 3 | 17 | G00 — AZM Martinsberg, Oed | 0.010′ | fitted |
| 2026-08-13 23:25:05 UTC | 4 | 21 | Z31 — Tenerife Observatory-LCO A, Tenerife | 0.020′ | fitted |
| 2026-08-14 03:15:12 UTC | 2 | 23 | Q62 — iTelescope Observatory, Siding Spring | 0.017′ | fitted |
| 2026-08-14 04:23:18 UTC | 3 | 26 | L27 — 29PREMOTE Observatory, Dauban | 0.010′ | fitted |
| 2026-08-14 07:11:28 UTC | 3 | 29 | R49 — Observatorio Villuercas-Navezuelas, Navezuelas | 0.008′ | fitted |
| 2026-08-14 12:45:27 UTC | 3 | 32 | K74 — Muensterschwarzach Observatory, Schwarzach | 0.010′ | fitted |
| 2026-08-14 15:47:15 UTC | 3 | 35 | G00 — AZM Martinsberg, Oed | 0.009′ | fitted |
| 2026-08-14 18:57:23 UTC | 3 | 38 | 900 — Moriyama | 0.006′ | fitted |
| 2026-08-15 05:42:11 UTC | 4 | 42 | G34 — Oberfrauendorf | 0.008′ | fitted |
| 2026-08-15 05:48:23 UTC | 3 | 45 | M49 — IAS Remote Observatory, Hakos | 0.006′ | fitted |
| 2026-08-16 02:20:07 UTC | 4 | 49 | L01 — Visnjan Observatory, Tican | 0.002′ | fitted |
| 2026-08-16 05:48:11 UTC | 3 | 52 | M49 — IAS Remote Observatory, Hakos | 0.002′ | fitted |
| 2026-08-16 06:17:09 UTC | 3 | 55 | L27 — 29PREMOTE Observatory, Dauban | 0.002′ | fitted |
P12pflz
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 |
|---|---|---|---|---|---|
| 2026-08-11 21:30:52 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 5.133′ | fitted |
P12pfnV
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 |
|---|---|---|---|---|---|
| 2026-08-11 23:01:03 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 471.000′ | fitted |
P12pfyU
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.
P12pfyW
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 |
|---|---|---|---|---|---|
| 2026-08-12 13:20:49 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 6.267′ | fitted |
| 2026-08-12 20:42:22 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 1.507′ | fitted |
| 2026-08-14 14:58:46 UTC | 4 | 9 | 474 — Mount John Observatory, Lake Tekapo | 0.006′ | fitted |
P12pfyX
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 |
|---|---|---|---|---|---|
| 2026-08-12 13:21:48 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 2.217′ | fitted |
P12pkQG
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.
P12pkRb
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 |
|---|---|---|---|---|---|
| 2026-08-12 18:24:23 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 452.000′ | fitted |
P12pkRc
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.
P12pkRg
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.
P12pkRh
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 |
|---|---|---|---|---|---|
| 2026-08-12 18:24:42 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 470.000′ | fitted |
| 2026-08-13 20:36:31 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 0.076′ | fitted |
| 2026-08-15 02:15:05 UTC | 3 | 9 | L01 — Visnjan Observatory, Tican | 0.002′ | fitted |
P12pkX8
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 |
|---|---|---|---|---|---|
| 2026-08-13 10:18:47 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 4.133′ | fitted |
| 2026-08-13 20:40:07 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 3.300′ | fitted |
| 2026-08-14 20:55:05 UTC | 3 | 8 | Z84 — Calar Alto-Schmidt | 0.203′ | fitted |
| 2026-08-16 07:29:25 UTC | 2 | 10 | M21 — Schiaparelli Southern Observatory, Hakos | 0.006′ | fitted |
P12pkXl
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 |
|---|---|---|---|---|---|
| 2026-08-13 11:54:39 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 3.850′ | fitted |
| 2026-08-14 20:45:05 UTC | 3 | 6 | Z84 — Calar Alto-Schmidt | 1.315′ | fitted |
| 2026-08-14 22:03:37 UTC | 3 | 9 | M21 — Schiaparelli Southern Observatory, Hakos | 2.600′ | fitted |
| 2026-08-14 22:22:05 UTC | 4 | 13 | F51 — Pan-STARRS 1, Haleakala | 2.717′ | fitted |
| 2026-08-15 03:01:52 UTC | 3 | 16 | Y05 — SONEAR Wykrota-CEAMIG, Serra da Piedade | 0.003′ | fitted |
| 2026-08-15 19:10:05 UTC | 3 | 19 | M21 — Schiaparelli Southern Observatory, Hakos | 0.011′ | fitted |
P12pkZx
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 |
|---|---|---|---|---|---|
| 2026-08-13 12:01:27 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 1.733′ | fitted |
| 2026-08-14 11:00:44 UTC | 4 | 8 | 474 — Mount John Observatory, Lake Tekapo | 0.034′ | fitted |
| 2026-08-16 11:18:40 UTC | 2 | 10 | M21 — Schiaparelli Southern Observatory, Hakos | 0.019′ | fitted |
| 2026-08-16 14:45:04 UTC | 3 | 13 | 474 — Mount John Observatory, Lake Tekapo | 0.004′ | fitted |
P12pl4l
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 |
|---|---|---|---|---|---|
| 2026-08-13 15:52:09 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 2.733′ | fitted |
| 2026-08-14 06:24:26 UTC | 3 | 7 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.100′ | fitted |
| 2026-08-15 01:05:07 UTC | 3 | 10 | L01 — Visnjan Observatory, Tican | 0.074′ | fitted |
P12pl4m
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 |
|---|---|---|---|---|---|
| 2026-08-13 15:52:12 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 3.417′ | fitted |
| 2026-08-14 06:13:57 UTC | 3 | 7 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.113′ | fitted |
| 2026-08-14 17:03:12 UTC | 4 | 11 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.011′ | fitted |
P12pl4n
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 |
|---|---|---|---|---|---|
| 2026-08-13 15:52:14 UTC | 3 | 3 | F51 — Pan-STARRS 1, Haleakala | 8.683′ | fitted |
P12ptHh
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 |
|---|---|---|---|---|---|
| 2026-08-14 16:57:10 UTC | 4 | 4 | F51 — Pan-STARRS 1, Haleakala | 33.917′ | fitted |
| 2026-08-14 22:58:47 UTC | 4 | 8 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.073′ | fitted |
| 2026-08-16 02:15:09 UTC | 2 | 10 | I41 — Palomar Mountain--ZTF | 0.054′ | fitted |
| 2026-08-16 05:40:20 UTC | 3 | 13 | H21 — Astronomical Research Observatory, Westfield | 0.025′ | fitted |
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 |
P22oVOy
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 |
|---|---|---|---|---|---|
| 2026-08-07 11:09:24 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.605′ | fitted |
| 2026-08-07 17:05:18 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 0.528′ | fitted |
| 2026-08-08 07:35:10 UTC | 2 | 7 | H21 — Astronomical Research Observatory, Westfield | 0.014′ | fitted |
| 2026-08-14 01:20:05 UTC | 4 | 11 | F52 — Pan-STARRS 2, Haleakala | 0.023′ | fitted |
P22oVTI
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 |
|---|---|---|---|---|---|
| 2026-08-07 12:39:47 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.662′ | fitted |
| 2026-08-07 17:07:46 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 0.457′ | fitted |
| 2026-08-08 08:15:05 UTC | 3 | 8 | H21 — Astronomical Research Observatory, Westfield | 0.014′ | fitted |
| 2026-08-15 09:25:03 UTC | 2 | 10 | 673 — Table Mountain Observatory, Wrightwood | 0.007′ | 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 |
P22oW3t
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 |
|---|---|---|---|---|---|
| 2026-08-07 14:02:08 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 3.100′ | fitted |
| 2026-08-07 17:10:35 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 0.915′ | fitted |
| 2026-08-08 11:42:47 UTC | 3 | 8 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.064′ | fitted |
| 2026-08-16 17:01:49 UTC | 4 | 12 | 474 — Mount John Observatory, Lake Tekapo | 0.001′ | fitted |
P22oY70
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 |
|---|---|---|---|---|---|
| 2026-08-07 16:09:16 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 1.382′ | fitted |
P22oZfK
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 |
|---|---|---|---|---|---|
| 2026-08-07 22:22:46 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 8.650′ | fitted |
P22oZgZ
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 |
|---|---|---|---|---|---|
| 2026-08-08 12:37:34 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.168′ | fitted |
| 2026-08-08 16:51:25 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 0.450′ | fitted |
| 2026-08-14 01:57:34 UTC | 4 | 10 | F51 — Pan-STARRS 1, Haleakala, F52 — Pan-STARRS 2, Haleakala | 3.267′ | fitted |
P22p4Fp
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.
P22p4Fq
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.
P22p4Jd
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 |
|---|---|---|---|---|---|
| 2026-08-09 15:42:52 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 1.247′ | fitted |
P22p4vP
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 |
|---|---|---|---|---|---|
| 2026-08-09 09:07:15 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 2.550′ | fitted |
| 2026-08-09 16:52:46 UTC | 2 | 5 | F52 — Pan-STARRS 2, Haleakala | 1.950′ | fitted |
| 2026-08-09 22:20:54 UTC | 2 | 7 | J95 — Great Shefford | 0.004′ | fitted |
| 2026-08-10 20:09:32 UTC | 4 | 11 | 106 — Crni Vrh | 0.001′ | fitted |
| 2026-08-10 22:00:05 UTC | 3 | 14 | L01 — Visnjan Observatory, Tican | 0.002′ | fitted |
| 2026-08-10 22:26:57 UTC | 4 | 18 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.002′ | fitted |
| 2026-08-11 20:28:20 UTC | 4 | 22 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.002′ | fitted |
| 2026-08-11 21:40:06 UTC | 3 | 25 | I93 — St Pardon de Conques | 0.001′ | fitted |
| 2026-08-12 20:51:26 UTC | 4 | 29 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.002′ | fitted |
| 2026-08-13 20:25:09 UTC | 3 | 32 | M75 — Online observatory, Peschany | 0.002′ | fitted |
| 2026-08-13 21:06:48 UTC | 3 | 35 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.002′ | fitted |
| 2026-08-13 22:40:50 UTC | 3 | 38 | J95 — Great Shefford | 0.003′ | fitted |
| 2026-08-14 04:00:11 UTC | 3 | 41 | H21 — Astronomical Research Observatory, Westfield | 0.003′ | fitted |
| 2026-08-14 20:15:46 UTC | 4 | 45 | 106 — Crni Vrh | 0.002′ | fitted |
| 2026-08-14 20:38:52 UTC | 2 | 47 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.003′ | fitted |
| 2026-08-14 22:50:46 UTC | 4 | 51 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.004′ | fitted |
| 2026-08-14 23:36:25 UTC | 2 | 53 | M21 — Schiaparelli Southern Observatory, Hakos | 0.002′ | fitted |
| 2026-08-15 00:18:23 UTC | 2 | 55 | 104 — San Marcello Pistoiese | 0.002′ | fitted |
| 2026-08-15 00:55:05 UTC | 3 | 58 | K51 — Osservatorio del Celado, Castello Tesino | 0.002′ | fitted |
| 2026-08-15 02:21:36 UTC | 3 | 61 | W62 — Comet Hunter Observatory2, New Ringgold | 0.002′ | fitted |
| 2026-08-16 03:00:06 UTC | 3 | 64 | H21 — Astronomical Research Observatory, Westfield | 0.002′ | fitted |
| 2026-08-16 19:31:07 UTC | 2 | 66 | I41 — Palomar Mountain--ZTF | 0.002′ | fitted |
P22p4wv
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.
P22p4xS
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.
P22papf
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.
P22paph
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 |
|---|---|---|---|---|---|
| 2026-08-11 09:23:24 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 3.883′ | fitted |
| 2026-08-11 20:28:19 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 1.032′ | fitted |
| 2026-08-12 11:42:16 UTC | 3 | 8 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.104′ | fitted |
| 2026-08-15 09:05:11 UTC | 2 | 10 | M21 — Schiaparelli Southern Observatory, Hakos | 0.008′ | fitted |
| 2026-08-16 02:50:05 UTC | 4 | 14 | H21 — Astronomical Research Observatory, Westfield | 0.002′ | fitted |
P22paxH
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 |
|---|---|---|---|---|---|
| 2026-08-11 13:12:12 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.173′ | fitted |
| 2026-08-11 20:38:03 UTC | 1 | 4 | F52 — Pan-STARRS 2, Haleakala | 1.610′ | fitted |
| 2026-08-12 02:05:05 UTC | 3 | 7 | L01 — Visnjan Observatory, Tican | 0.040′ | fitted |
| 2026-08-12 07:20:06 UTC | 3 | 10 | H21 — Astronomical Research Observatory, Westfield | 0.009′ | fitted |
| 2026-08-14 06:16:43 UTC | 4 | 14 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.007′ | fitted |
| 2026-08-14 21:10:05 UTC | 3 | 17 | Z84 — Calar Alto-Schmidt | 0.007′ | fitted |
P22paxQ
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 |
|---|---|---|---|---|---|
| 2026-08-11 13:13:27 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.260′ | fitted |
| 2026-08-11 20:31:56 UTC | 2 | 5 | F52 — Pan-STARRS 2, Haleakala | 0.587′ | fitted |
| 2026-08-12 07:55:43 UTC | 2 | 7 | H21 — Astronomical Research Observatory, Westfield | 0.015′ | fitted |
| 2026-08-16 06:43:06 UTC | 4 | 11 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.004′ | fitted |
P22pfCv
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.
P22pfnu
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 |
|---|---|---|---|---|---|
| 2026-08-11 22:28:29 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 462.000′ | fitted |
P22pfsJ
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 |
|---|---|---|---|---|---|
| 2026-08-12 11:52:24 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 1.250′ | fitted |
| 2026-08-12 20:47:48 UTC | 2 | 5 | F52 — Pan-STARRS 2, Haleakala | 1.367′ | fitted |
| 2026-08-13 01:55:05 UTC | 3 | 8 | L01 — Visnjan Observatory, Tican | 0.006′ | fitted |
| 2026-08-13 05:27:55 UTC | 4 | 12 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.019′ | fitted |
| 2026-08-13 07:05:07 UTC | 4 | 16 | H21 — Astronomical Research Observatory, Westfield | 0.006′ | fitted |
| 2026-08-14 05:45:05 UTC | 3 | 19 | H21 — Astronomical Research Observatory, Westfield | 0.008′ | fitted |
| 2026-08-15 00:52:36 UTC | 2 | 21 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.004′ | fitted |
P22pkRP
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 |
|---|---|---|---|---|---|
| 2026-08-12 18:26:05 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 438.000′ | fitted |
P22pl07
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 |
|---|---|---|---|---|---|
| 2026-08-13 12:03:36 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 3.333′ | fitted |
| 2026-08-13 20:55:22 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 1.630′ | fitted |
| 2026-08-14 16:37:33 UTC | 4 | 10 | 474 — Mount John Observatory, Lake Tekapo | 0.018′ | fitted |
| 2026-08-14 20:45:05 UTC | 3 | 13 | Z84 — Calar Alto-Schmidt | 0.010′ | fitted |
| 2026-08-14 23:55:06 UTC | 3 | 16 | L01 — Visnjan Observatory, Tican | 0.001′ | fitted |
| 2026-08-16 12:10:54 UTC | 3 | 19 | M21 — Schiaparelli Southern Observatory, Hakos | 0.001′ | fitted |
| 2026-08-16 13:31:15 UTC | 2 | 21 | I41 — Palomar Mountain--ZTF | 0.001′ | fitted |
P22pl08
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.
P22ppXD
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 |
|---|---|---|---|---|---|
| 2026-08-13 20:04:20 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 8.533′ | fitted |
| 2026-08-14 02:50:05 UTC | 3 | 6 | L01 — Visnjan Observatory, Tican | 0.067′ | fitted |
| 2026-08-14 17:09:36 UTC | 4 | 10 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.012′ | fitted |
| 2026-08-16 02:26:06 UTC | 3 | 13 | I41 — Palomar Mountain--ZTF | 0.005′ | fitted |
P22ppY2
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 |
|---|---|---|---|---|---|
| 2026-08-14 12:25:35 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.433′ | fitted |
| 2026-08-14 20:25:33 UTC | 4 | 8 | F51 — Pan-STARRS 1, Haleakala | 0.437′ | fitted |
| 2026-08-14 22:34:18 UTC | 4 | 12 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.010′ | fitted |
| 2026-08-15 22:27:50 UTC | 3 | 15 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.015′ | fitted |
| 2026-08-16 05:30:06 UTC | 3 | 18 | H21 — Astronomical Research Observatory, Westfield | 0.010′ | fitted |
P22ppYR
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 |
|---|---|---|---|---|---|
| 2026-08-14 12:30:13 UTC | 4 | 4 | F52 — Pan-STARRS 2, Haleakala | 0.015′ | fitted |
| 2026-08-14 20:28:37 UTC | 2 | 6 | F51 — Pan-STARRS 1, Haleakala | 0.393′ | fitted |
| 2026-08-15 08:07:28 UTC | 2 | 8 | 673 — Table Mountain Observatory, Wrightwood | 0.017′ | fitted |
| 2026-08-16 02:17:26 UTC | 2 | 10 | I41 — Palomar Mountain--ZTF | 0.059′ | fitted |
| 2026-08-16 06:35:11 UTC | 2 | 12 | H21 — Astronomical Research Observatory, Westfield | 0.005′ | fitted |
P22pq2q
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 |
|---|---|---|---|---|---|
| 2026-08-14 12:52:05 UTC | 3 | 3 | F52 — Pan-STARRS 2, Haleakala | 0.772′ | fitted |
| 2026-08-14 20:29:38 UTC | 2 | 5 | F51 — Pan-STARRS 1, Haleakala | 1.362′ | fitted |
| 2026-08-15 00:35:08 UTC | 3 | 8 | L01 — Visnjan Observatory, Tican | 0.006′ | fitted |
| 2026-08-15 02:10:02 UTC | 4 | 12 | 106 — Crni Vrh | 0.007′ | fitted |
| 2026-08-15 07:00:05 UTC | 3 | 15 | Z84 — Calar Alto-Schmidt | 0.004′ | fitted |
RMM2026
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 |
|---|---|---|---|---|---|
| 2026-07-17 00:32:02 UTC | 7 | 7 | 809 — European Southern Observatory, La Silla, X05 — Simonyi Survey Telescope, Rubin Observatory | 0.061′ | fitted |
| 2026-07-17 02:34:12 UTC | 7 | 14 | 705 — Apache Point | 0.006′ | fitted |
| 2026-07-17 20:17:38 UTC | 12 | 26 | F51 — Pan-STARRS 1, Haleakala | 0.003′ | fitted |
| 2026-07-18 01:20:04 UTC | 1 | 27 | J13 — La Palma-Liverpool Telescope | 0.002′ | fitted |
| 2026-07-18 11:27:15 UTC | 3 | 30 | T14 — Canada-France-Hawaii Telescope, Maunakea | 0.000′ | fitted |
| 2026-07-18 18:46:13 UTC | 2 | 32 | X05 — Simonyi Survey Telescope, Rubin Observatory | 0.000′ | fitted |
| 2026-07-20 03:20:17 UTC | 2 | 34 | Q62 — iTelescope Observatory, Siding Spring | 0.001′ | fitted |
| 2026-07-21 21:31:23 UTC | 5 | 39 | E10 — Siding Spring-Faulkes Telescope South | 0.002′ | fitted |
| 2026-07-27 21:40:21 UTC | 3 | 42 | E10 — Siding Spring-Faulkes Telescope South | 0.008′ | fitted |
| 2026-07-27 21:56:40 UTC | 3 | 45 | F65 — Haleakala-Faulkes Telescope North | 0.005′ | fitted |
| 2026-07-31 17:38:19 UTC | 3 | 48 | E10 — Siding Spring-Faulkes Telescope South | 0.002′ | fitted |
| 2026-07-31 20:25:20 UTC | 29 | 77 | F51 — Pan-STARRS 1, Haleakala, F52 — Pan-STARRS 2, Haleakala | 0.001′ | fitted |
Roc4012
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 |
|---|---|---|---|---|---|
| 2026-08-12 12:44:02 UTC | 3 | 3 | X89 — Rocca Observatory, Brasilia | 565.000′ | fitted |
SK000Zy
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 |
|---|---|---|---|---|---|
| 2026-08-16 12:37:30 UTC | 3 | 3 | U62 — TransAstra TKO at SkiesAway | 2,880.000′ | fitted |
ST26H33
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 |
|---|---|---|---|---|---|
| 2026-08-13 07:50:27 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H41
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 |
|---|---|---|---|---|---|
| 2026-08-15 10:31:52 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
STO1481
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 |
|---|---|---|---|---|---|
| 2026-08-14 12:30:07 UTC | 3 | 3 | X19 — Santel Observatory, El Leoncito | 2,520.000′ | fitted |
Sar2900
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 |
|---|---|---|---|---|---|
| 2026-08-14 00:45:04 UTC | 6 | 6 | K88 — GINOP-KHK, Piszkesteto | 4.133′ | fitted |
| 2026-08-14 01:15:18 UTC | 3 | 9 | K88 — GINOP-KHK, Piszkesteto | 1.238′ | fitted |
| 2026-08-14 01:29:39 UTC | 2 | 11 | J95 — Great Shefford | 0.041′ | fitted |
| 2026-08-14 02:00:32 UTC | 3 | 14 | L01 — Visnjan Observatory, Tican | 0.034′ | fitted |
| 2026-08-14 04:30:12 UTC | 3 | 17 | H21 — Astronomical Research Observatory, Westfield | 0.017′ | fitted |
| 2026-08-14 21:50:28 UTC | 3 | 20 | 106 — Crni Vrh | 0.006′ | fitted |
| 2026-08-14 22:10:03 UTC | 3 | 23 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.007′ | fitted |
| 2026-08-15 06:02:06 UTC | 3 | 26 | W62 — Comet Hunter Observatory2, New Ringgold | 0.004′ | fitted |
| 2026-08-15 06:42:22 UTC | 2 | 28 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.004′ | fitted |
| 2026-08-15 21:04:05 UTC | 4 | 32 | 033 — Karl Schwarzschild Observatory, Tautenburg | 0.005′ | fitted |
| 2026-08-16 00:25:05 UTC | 2 | 34 | K51 — Osservatorio del Celado, Castello Tesino | 0.003′ | fitted |
| 2026-08-16 02:18:02 UTC | 2 | 36 | I41 — Palomar Mountain--ZTF | 0.003′ | fitted |
TF26H65
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 |
|---|---|---|---|---|---|
| 2026-08-15 15:37:28 UTC | 2 | 2 | U74 — JPL SynTrack Robotic Telescope 2, Auberry | — | insufficient-observations |
X89913
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 |
|---|---|---|---|---|---|
| 2026-08-16 16:01:23 UTC | 3 | 3 | D29 — Purple Mountain Observatory, XuYi Station | 814.000′ | fitted |
X89940
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 |
|---|---|---|---|---|---|
| 2026-08-15 23:18:00 UTC | 3 | 3 | D29 — Purple Mountain Observatory, XuYi Station | 510.000′ | fitted |
| 2026-08-16 01:40:05 UTC | 3 | 6 | L01 — Visnjan Observatory, Tican | 0.062′ | fitted |
| 2026-08-16 13:28:57 UTC | 1 | 7 | I41 — Palomar Mountain--ZTF | 0.074′ | fitted |
ZTF10FL
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 |
|---|---|---|---|---|---|
| 2026-08-15 00:40:48 UTC | 4 | 4 | I41 — Palomar Mountain--ZTF | 2,940.000′ | fitted |
ZTF10FO
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 |
|---|---|---|---|---|---|
| 2026-08-15 22:17:43 UTC | 4 | 4 | I41 — Palomar Mountain--ZTF | 2,100.000′ | fitted |
ZTF10FQ
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 |
|---|---|---|---|---|---|
| 2026-08-16 09:09:11 UTC | 4 | 4 | I41 — Palomar Mountain--ZTF | 1,320.000′ | fitted |
orA4767
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 |
|---|---|---|---|---|---|
| 2026-08-16 06:32:16 UTC | 3 | 3 | J43 — Oukaimeden Observatory, Marrakech | 480.000′ | fitted |