URGENT: We will run out of 5-digit catalog numbers at 69999 not 99999, which is estimated to occur around 2026‑07‑20 (we're currently at 68126). At that point, newly cataloged objects will have 6-digit catalog numbers of 100000+ and GP data will not be available for them using the TLE format. CelesTrak developed new formats that removed this limitation (and finally fixed the Y2K problem) in May 2020 and immediately began providing GP data in those formats for software developers. The same limitations apply to the legacy fixed-field SATCAT. Follow @TSKelso on Bluesky for the latest updates, tutorials, and changes as we approach this transition. Spread the word! ‑ TS

SOCRATES Plus

Search Results

CelesTrak

Search parameters:

  • NORAD Catalog Number(s): 25544
  • Order by NORAD Catalog Number
  • Return first 25 items


Data current as of 2026 Mar 10 04:05:40 UTC

Computation Interval: Start = 2026 Mar 10 04:00:00 UTC, Stop = 2026 Mar 17 04:00:00 UTC
Computation Threshold: 5.0 km
Considering: 14,654 Primaries, 30,077 Secondaries (119,788 Conjunctions)
11 SGP4 Propagation Errors
Computation run time: 09h 53m 04.702s

SOCRATES Format Documentation

See notes at bottom of page for data field descriptions

Data
&
Graphs
NORAD
Catalog
Number
Name [Ops Status] Days
Since
Epoch
TCA
(UTC)
Min
Range
(km)
Relative
Speed
(km/sec)
Max
Probability
Dilution
Threshold
(km)
GP Data 25544 ISS (ZARYA) [+] 3.071 2026-03-12 18:40:06.403 2.945 14.633
50 km All 48907 MANDRAKE 2 ABLE [+] 3.286 1.342E-05 1.597
GP Data 25544 ISS (ZARYA) [+] 6.141 2026-03-15 20:21:18.827 4.799 14.049
50 km All 48951 DEMO8 (TENZING) [+] 6.347 5.838E-06 2.253
GP Data 25544 ISS (ZARYA) [+] 0.961 2026-03-10 16:01:07.917 3.925 14.476
50 km All 52754 HAWK-5C [+] 0.749 7.842E-06 2.050
GP Data 25544 ISS (ZARYA) [+] 1.800 2026-03-11 12:10:26.965 4.341 14.548
50 km All 52756 HAWK-5B [+] 1.589 6.289E-06 2.312
GP Data 25544 ISS (ZARYA) [+] 0.831 2026-03-10 12:54:42.829 4.417 14.438
50 km All 52757 HAWK-5A [+] 0.620 6.256E-06 2.284
GP Data 25544 ISS (ZARYA) [+] 1.879 2026-03-11 14:04:11.448 0.953 7.082
50 km All 52908 YAOGAN-35 02B [+] 1.632 2.653E-04 0.250
GP Data 25544 ISS (ZARYA) [+] 2.041 2026-03-11 17:56:25.205 4.777 7.098
50 km All 52908 YAOGAN-35 02B [+] 1.793 1.055E-05 1.252
GP Data 25544 ISS (ZARYA) [+] 7.441 2026-03-17 03:32:36.388 4.972 13.524
50 km All 58823 OBJECT D [+] 7.194 6.008E-06 2.113
GP Data 25544 ISS (ZARYA) [+] 1.185 2026-03-10 21:23:59.510 4.009 14.310
50 km All 59112 SONATE-2 [+] 0.974 7.902E-06 1.992

9 records found

Data Fields:
  • Data: The GP Data button links to a page which provides the GP data used to generate the associated prediction.
  • NORAD Catalog Number: NORAD Catalog Numbers of the two conjuncting objects.
  • Name: SATCAT names of the two conjuncting objects. Operational status of each object is shown in brackets, using the standard CelesTrak SATCAT codes.
  • Days Since Epoch: The number of days from the epoch of the NORAD GP or SupGP (green) element set used to produce the prediction until the time of closest approach for the conjunction.
  • TCA (UTC): Time of closest approach.
  • Min Range (km): The distance between the two conjuncting objects at the time of closest approach.
  • Relative Speed (km/sec): Relative speed of the two conjuncting objects at the time of closest approach.
  • Max Probability: Given fixed spherical object radii and relative distance at the time of closest approach (TCA), the projected covariance ellipse is sized and oriented to produce the maximum probability. For these reports the ratio of major-to-minor axes of the projected covariance ellipse is set using radial, in-track, and cross-track values of 100 m, 300 m, 100 m, respectively. If the combined object radius is greater than the relative distance, the maximum probability will be one; such occurrences are not addressed here. For more details on the maximum probability method, see Dr. Sal Alfano's paper titled "Relating Position Uncertainty to Maximum Conjunction Probability".
  • Dilution Threshold (km): The standard deviation that produces the maximum probability defines the threshold of dilution. A smaller or larger standard deviation will produce a smaller probability. In the case of computing true probability with a smaller standard deviation, the data is of sufficient quality to associate low probability with low risk. For a larger standard deviation, this is not the case and the resulting true probability calculation becomes "diluted." If operating in this dilution region, the recommendation is to obtain better data and reassess the encounter. If time or resources do not permit, then the maximum probability should be used in place of the true probability.
  • SGP4 Propagation Errors: A list of objects which were not screened because their GP data shows they have already decayed (but haven't yet been reflected in the SATCAT) or will decay prior to the end of the computation interval.