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.
6HJ4621
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 |
|---|---|---|---|---|---|
| 2026-08-20 05:55:06 UTC | 3 | 3 | W94 — MAPS, San Pedro de Atacama | 0.908′ | fitted |
6HK2621
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.
6HM3721
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 |
|---|---|---|---|---|---|
| 2026-08-23 03:40:07 UTC | 3 | 3 | W94 — MAPS, San Pedro de Atacama | 5.367′ | fitted |
| 2026-08-23 04:30:06 UTC | 3 | 6 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 0.214′ | fitted |
| 2026-08-23 05:25:05 UTC | 3 | 9 | W97 — Atacama Desert Observatory, San Pedro de Atacama | 1.850′ | 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 |
A11FVo2
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 |
|---|---|---|---|---|---|
| 2026-08-22 05:39:35 UTC | 4 | 4 | M22 — ATLAS South Africa, Sutherland | 8.017′ | fitted |
ABC0149
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 |
|---|---|---|---|---|---|
| 2026-08-23 13:22:37 UTC | 3 | 3 | 122 — Pises Observatory | 932.000′ | fitted |
C1FP4X5
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 |
|---|---|---|---|---|---|
| 2026-08-21 09:15:17 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 2.600′ | fitted |
C1FP8U5
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 |
|---|---|---|---|---|---|
| 2026-08-21 09:20:02 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 2.750′ | fitted |
C1FPQP5
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.
C1FQ9Y5
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.
C1FQCU5
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 |
|---|---|---|---|---|---|
| 2026-08-22 12:01:42 UTC | 3 | 3 | V00 — Kitt Peak-Bok | 1.767′ | fitted |
C1FQUM5
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.
C1FQZ45
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 |
|---|---|---|---|---|---|
| 2026-08-22 08:43:34 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 2.633′ | fitted |
C1FRE35
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 |
|---|---|---|---|---|---|
| 2026-08-22 09:14:38 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 5.517′ | fitted |
| 2026-08-22 21:29:04 UTC | 2 | 6 | 291 — LPL/Spacewatch II | 5.617′ | fitted |
| 2026-08-23 08:25:04 UTC | 4 | 10 | V00 — Kitt Peak-Bok | 0.027′ | fitted |
| 2026-08-24 15:37:39 UTC | 3 | 13 | I41 — Palomar Mountain--ZTF | 0.027′ | fitted |
C1FRLU5
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 |
|---|---|---|---|---|---|
| 2026-08-22 09:24:44 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 10.250′ | fitted |
C1FT295
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 |
|---|---|---|---|---|---|
| 2026-08-22 09:38:37 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 8.850′ | fitted |
C1FVG05
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 |
|---|---|---|---|---|---|
| 2026-08-23 06:12:08 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 0.177′ | fitted |
| 2026-08-24 07:25:07 UTC | 3 | 7 | H21 — Astronomical Research Observatory, Westfield | 0.030′ | fitted |
| 2026-08-25 05:00:06 UTC | 3 | 10 | H21 — Astronomical Research Observatory, Westfield | 0.001′ | fitted |
| 2026-08-25 05:25:07 UTC | 3 | 13 | 695 — Kitt Peak | 0.001′ | fitted |
C1FVTC5
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.
C1FVXQ5
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 |
|---|---|---|---|---|---|
| 2026-08-23 07:39:02 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 6.217′ | fitted |
| 2026-08-23 10:42:14 UTC | 3 | 7 | 291 — LPL/Spacewatch II | 0.562′ | fitted |
| 2026-08-24 07:00:05 UTC | 2 | 9 | H21 — Astronomical Research Observatory, Westfield | 0.081′ | fitted |
| 2026-08-24 14:11:17 UTC | 1 | 10 | I41 — Palomar Mountain--ZTF | 0.148′ | fitted |
| 2026-08-25 06:00:05 UTC | 3 | 13 | H21 — Astronomical Research Observatory, Westfield | 0.016′ | fitted |
| 2026-08-25 08:20:05 UTC | 3 | 16 | 695 — Kitt Peak | 0.012′ | fitted |
| 2026-08-25 10:05:53 UTC | 2 | 18 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.010′ | fitted |
C1FW5R5
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.
C1FW9G5
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.
C1FWHY5
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 |
|---|---|---|---|---|---|
| 2026-08-23 08:18:14 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 5.283′ | fitted |
C1FX255
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.
C1FXP05
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.
C1FYW35
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 |
|---|---|---|---|---|---|
| 2026-08-23 11:07:01 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 6.167′ | fitted |
| 2026-08-23 19:23:32 UTC | 3 | 7 | 291 — LPL/Spacewatch II | 1.783′ | fitted |
| 2026-08-24 07:55:05 UTC | 2 | 9 | H21 — Astronomical Research Observatory, Westfield | 0.048′ | fitted |
| 2026-08-25 06:50:05 UTC | 3 | 12 | H21 — Astronomical Research Observatory, Westfield | 0.010′ | fitted |
| 2026-08-25 07:45:06 UTC | 3 | 15 | 695 — Kitt Peak | 0.009′ | fitted |
C1FZHE5
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 |
|---|---|---|---|---|---|
| 2026-08-23 12:06:02 UTC | 4 | 4 | V00 — Kitt Peak-Bok | 2.683′ | fitted |
| 2026-08-24 08:50:07 UTC | 3 | 7 | H21 — Astronomical Research Observatory, Westfield | 0.021′ | fitted |
| 2026-08-25 07:10:06 UTC | 3 | 10 | H21 — Astronomical Research Observatory, Westfield | 0.008′ | fitted |
| 2026-08-25 09:05:08 UTC | 3 | 13 | 695 — Kitt Peak | 0.006′ | fitted |
LA0Cr6m
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 |
|---|---|---|---|---|---|
| 2026-08-18 19:27:46 UTC | 6 | 6 | P07 — Space Surveillance Telescope, HEH Station | 0.152′ | fitted |
MQM9799
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 |
|---|---|---|---|---|---|
| 2026-08-24 14:42:11 UTC | 6 | 6 | O18 — WFST, Lenghu | 0.009′ | fitted |
OCA1666
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 |
| 2026-08-17 01:30:07 UTC | 3 | 58 | C40 — Kuban State University Astrophysical Observatory | 0.003′ | fitted |
| 2026-08-17 12:01:37 UTC | 2 | 60 | G40 — Slooh.com Canary Islands Observatory | 0.003′ | fitted |
| 2026-08-17 18:54:47 UTC | 2 | 62 | E42 — AUSTRALIA1/SRI, Swan Reach | 0.004′ | fitted |
| 2026-08-18 05:54:26 UTC | 3 | 65 | M49 — IAS Remote Observatory, Hakos | 0.003′ | fitted |
| 2026-08-18 07:41:03 UTC | 3 | 68 | S15 — Station name unavailable | 0.003′ | fitted |
| 2026-08-18 10:05:33 UTC | 2 | 70 | G40 — Slooh.com Canary Islands Observatory | 0.003′ | fitted |
| 2026-08-18 18:05:55 UTC | 4 | 74 | K92 — Sutherland-LCO B | 0.004′ | fitted |
| 2026-08-18 18:07:21 UTC | 3 | 77 | K91 — Sutherland-LCO A | 0.003′ | fitted |
| 2026-08-19 02:18:50 UTC | 3 | 80 | B74 — Santa Maria de Montmagastrell | 0.002′ | fitted |
| 2026-08-19 04:40:35 UTC | 3 | 83 | M49 — IAS Remote Observatory, Hakos | 0.002′ | fitted |
| 2026-08-19 08:19:10 UTC | 3 | 86 | W62 — Comet Hunter Observatory2, New Ringgold | 0.002′ | fitted |
| 2026-08-19 13:17:29 UTC | 5 | 91 | V21 — Cewanee Observatory at DSNM | 0.001′ | fitted |
| 2026-08-21 00:55:07 UTC | 3 | 94 | C40 — Kuban State University Astrophysical Observatory | 0.002′ | fitted |
| 2026-08-21 02:14:15 UTC | 2 | 96 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.002′ | fitted |
| 2026-08-21 07:32:15 UTC | 2 | 98 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.002′ | fitted |
| 2026-08-22 00:25:05 UTC | 3 | 101 | M75 — Online observatory, Peschany | 0.002′ | fitted |
| 2026-08-22 07:45:26 UTC | 3 | 104 | M49 — IAS Remote Observatory, Hakos | 0.002′ | fitted |
| 2026-08-22 10:27:48 UTC | 3 | 107 | M45 — Starhopper Observatory, Sfantu Gheorghe | 0.002′ | fitted |
| 2026-08-22 11:20:19 UTC | 4 | 111 | X03 — Observatoire SADR, Poroto | 0.001′ | fitted |
| 2026-08-22 14:37:30 UTC | 3 | 114 | L34 — Galhassin Robotic Telescope, Isnello | 0.001′ | fitted |
| 2026-08-23 00:50:29 UTC | 5 | 119 | X25 — UBC Southern Observatory | 0.002′ | fitted |
| 2026-08-23 02:08:26 UTC | 2 | 121 | L04 — ROASTERR-1 Observatory, Cluj-Napoca | 0.001′ | fitted |
| 2026-08-24 04:05:05 UTC | 3 | 124 | L06 — Sormano 2 Observatory, Bellagio Via Lattea | 0.002′ | fitted |
| 2026-08-24 14:15:03 UTC | 4 | 128 | K35 — Huenfelden | 0.002′ | fitted |
| 2026-08-24 14:30:50 UTC | 3 | 131 | 215 — Buchloe | 0.002′ | fitted |
| 2026-08-24 15:03:55 UTC | 2 | 133 | G40 — Slooh.com Canary Islands Observatory | 0.002′ | fitted |
| 2026-08-24 15:39:02 UTC | 2 | 135 | G40 — Slooh.com Canary Islands Observatory | 0.002′ | fitted |
| 2026-08-24 15:55:36 UTC | 3 | 138 | X07 — iTelescope Deep Sky Chile, Rio Hurtado | 0.001′ | fitted |
| 2026-08-24 22:30:29 UTC | 4 | 142 | V21 — Cewanee Observatory at DSNM | 0.001′ | fitted |
| 2026-08-25 01:19:50 UTC | 2 | 144 | Q21 — Southern Utsunomiya | 0.001′ | fitted |
| 2026-08-25 10:55:05 UTC | 4 | 148 | G40 — Slooh.com Canary Islands Observatory | 0.002′ | 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.
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 |
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 |
ST26H52
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 |
|---|---|---|---|---|---|
| 2026-08-17 07:12:42 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H72
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 |
|---|---|---|---|---|---|
| 2026-08-22 08:00:01 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H75
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 |
|---|---|---|---|---|---|
| 2026-08-22 15:39:29 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H76
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 |
|---|---|---|---|---|---|
| 2026-08-22 15:40:46 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H78
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 |
|---|---|---|---|---|---|
| 2026-08-22 15:43:33 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H83
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 |
|---|---|---|---|---|---|
| 2026-08-23 10:10:20 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H84
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 |
|---|---|---|---|---|---|
| 2026-08-23 10:11:56 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H89
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 |
|---|---|---|---|---|---|
| 2026-08-24 16:00:07 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H92
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 |
|---|---|---|---|---|---|
| 2026-08-25 08:33:00 UTC | 2 | 2 | U68 — JPL SynTrack Robotic Telescope, Auberry | — | insufficient-observations |
ST26H93
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.
TF26HC9
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 |
|---|---|---|---|---|---|
| 2026-08-24 06:55:20 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 |
X90000
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 |
|---|---|---|---|---|---|
| 2026-08-23 09:07:26 UTC | 3 | 3 | D29 — Purple Mountain Observatory, XuYi Station | 2,100.000′ | fitted |
XAaiiXA
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 18:24:08 UTC | 3 | 3 | N94 — Altay Astronomical Observatory | 4.683′ | fitted |
| 2026-08-19 19:59:36 UTC | 3 | 6 | N88 — Xingming Observatory #3, Nanshan | 0.285′ | fitted |
| 2026-08-20 02:00:05 UTC | 2 | 8 | L01 — Visnjan Observatory, Tican | 0.052′ | 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.
ZTF10FV
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.
ZTF10FX
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 |
|---|---|---|---|---|---|
| 2026-08-21 15:03:07 UTC | 4 | 4 | I41 — Palomar Mountain--ZTF | 1,320.000′ | fitted |
ZTF10Fc
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 |
|---|---|---|---|---|---|
| 2026-08-25 17:31:24 UTC | 4 | 4 | I41 — Palomar Mountain--ZTF | 498.000′ | fitted |
orA5076
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 |
|---|---|---|---|---|---|
| 2026-08-22 06:37:40 UTC | 3 | 3 | J43 — Oukaimeden Observatory, Marrakech | 2.850′ | fitted |