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CelesTrak

Search parameters:

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


Data current as of 2023 Mar 30 08:19:34 UTC

Computation Interval: Start = 2023 Mar 30 09:00:00 UTC, Stop = 2023 Apr 06 09:00:00 UTC
Computation Threshold: 5.0 km
Considering: 7,450 Primaries, 24,764 Secondaries (55,103 Conjunctions)
23 SGP4 Propagation Errors
Computation run time: 04h 27m 00.116s

SOCRATES Format Documentation

See notes at bottom of page for data field descriptions

Re-sort by: Maximum Probability|Minimum Range|Time of Closest Approach|Relative Speed|NORAD Catalog Number

Data NORAD
Catalog
Number
Name [Ops Status] Days
Since
Epoch
TCA
(UTC)
Min
Range
(km)
Relative
Speed
(km/sec)
Max
Probability
Dilution
Threshold
(km)
25544 ISS (ZARYA) [+] 2.979 2023-04-02 03:37:42.754 0.217 3.840
49469 GLOBAL-14 [+] 3.277 5.476E-03 0.053
25544 ISS (ZARYA) [+] 5.491 2023-04-04 15:54:04.430 0.981 14.483
47717 OBJECT T [-] 6.441 1.259E-04 0.511
25544 ISS (ZARYA) [+] 6.232 2023-04-05 09:41:05.904 1.488 14.533
46300 SPACEBEE-21 [+] 6.750 5.411E-05 0.783
25544 ISS (ZARYA) [+] 6.475 2023-04-05 15:30:33.242 1.693 7.498
41459 E-ST@R-II [+] 6.859 8.293E-05 0.450
25544 ISS (ZARYA) [+] 1.356 2023-03-31 12:39:17.294 2.148 14.763
48256 OBJECT J [-] 1.277 2.433E-05 1.208
25544 ISS (ZARYA) [+] 6.846 2023-04-06 00:25:44.774 3.324 14.310
49814 OBJECT C [?] 7.012 1.146E-05 1.657
25544 ISS (ZARYA) [+] 2.837 2023-04-02 00:12:03.913 3.410 14.743
49515 RESURS O1 DEB [-] 28.597 9.709E-06 1.906
25544 ISS (ZARYA) [+] 3.612 2023-04-02 18:48:21.197 3.755 14.753
44080 FLOCK 4A-2 [+] 3.610 7.981E-06 2.106
25544 ISS (ZARYA) [+] 5.229 2023-04-04 09:36:23.437 3.794 14.718
40301 QSAT-EOS [+] 5.520 7.881E-06 2.111
25544 ISS (ZARYA) [+] 1.237 2023-03-31 09:48:14.673 4.048 14.355
41558 NUSAT-2 (BATATA) [+] 1.261 7.641E-06 2.041

10 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.