Conjunctions
Close approaches within 5 km between satellites in the portal catalog and other objects in orbit over the next seven days. The table is updated three times a day.
Last updated, UTC: 2026-10-11 16:30
Last updated, UTC: 2026-10-11 16:30
| Time of closest approach, UTC | Object 1 | Object 2 | Distance, km | Speed, km/s | Max. probability |
|---|---|---|---|---|---|
| 2026-10-15 19:48:47 |
STARLINK-1451
NORAD 45668 |
FLOCK 4H-15
NORAD 66718 |
3.473 | 14.12 | 5.4e-06 |
| 2026-10-15 12:24:21 |
STARLINK-6044
NORAD 56479 |
FLOCK 4H-15
NORAD 66718 |
4.777 | 9.31 | 4.8e-06 |
| 2026-10-12 12:43:21 |
SHIJIAN-26 (SJ-26)
NORAD 64199 |
FLOCK 4H-15
NORAD 66718 |
2.073 | 0.82 | 1.0e-06 |
| 2026-10-15 17:14:53 |
FLOCK 4H-15
NORAD 66718 |
CZ-4B R/B
NORAD 29507 |
2.222 | 3.57 | 8.7e-07 |
| 2026-10-14 11:16:50 |
FLOCK 4H-15
NORAD 66718 |
YAOGAN-47
NORAD 66988 |
2.440 | 0.18 | 7.4e-07 |
| 2026-10-15 11:43:54 |
SHIJIAN-6 01A (SJ-6 01A)
NORAD 28413 |
FLOCK 4H-15
NORAD 66718 |
2.667 | 5.67 | 5.8e-07 |
| 2026-10-12 23:44:46 |
OBJECT C
NORAD 63293 |
FLOCK 4H-15
NORAD 66718 |
3.375 | 8.58 | 3.3e-07 |
| 2026-10-16 06:27:18 |
YUNYAO-1 19
NORAD 58759 |
FLOCK 4H-15
NORAD 66718 |
3.315 | 9.50 | 3.3e-07 |
| 2026-10-17 09:37:27 |
SPACEMOBILE-001
NORAD 61047 |
FLOCK 4H-15
NORAD 66718 |
3.232 | 12.22 | 2.8e-07 |
| 2026-10-14 00:13:14 |
FLOCK 4H-15
NORAD 66718 |
COSMOS 2603
NORAD 67677 |
4.095 | 3.07 | 2.6e-07 |
| 2026-10-15 03:43:45 |
IRIDE-MS1-EAGLET 2-8
NORAD 66702 |
FLOCK 4H-15
NORAD 66718 |
4.238 | 0.01 | 2.4e-07 |
| 2026-10-15 14:50:56 |
OBJECT F
NORAD 63296 |
FLOCK 4H-15
NORAD 66718 |
4.221 | 8.61 | 2.1e-07 |
| 2026-10-16 17:44:24 |
FLOCK 4H-15
NORAD 66718 |
COSMO
NORAD 68460 |
3.891 | 12.73 | 1.8e-07 |
| 2026-10-12 00:39:22 |
FLOCK 4H-4
NORAD 66707 |
FLOCK 4H-15
NORAD 66718 |
4.549 | 0.00 | 1.7e-07 |
| 2026-10-14 02:34:26 |
FLOCK 4H-15
NORAD 66718 |
PEGASUS DEB
NORAD 24082 |
4.727 | 14.69 | 8.2e-08 |
Data: CelesTrak SOCRATES Plus, computed from TLEs of the public catalog. This is an estimate, not grounds for a manoeuvre: TLEs carry no covariance, and the maximum probability assumes a position error.