COSMOS 2041, 20235
Orbit data source: Space-Track
COSMOS 2041, 20235 is a payload satellite owned by UNKS (CIS) in LEO that was launched on Thu, 14 Sep 1989 UTC via a TSIKLON-3 launch vehicle from the Plesetsk Missile And Space Complex (PKMTR). Payload-class satellites include a variety of spacecraft equipped with specific instruments for various scientific and technological missions. These include communications satellites like Starlink; space stations such as the ISS; scientific satellites like the Hubble; Earth observation satellites from companies like Planet Labs, Umbra, and HawkEye 360; GPS; miniature CubeSats for education and research; and military/defense satellites.
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20235 intel report (Beta)
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Identifier
Orbit
Country
CISRelated business
Manufacturer
NPO PM
Mission
Defense Communications
Bus & Motor
STRELA-3, Unknown motor
Mass
225 kg wet, 225 kg dry
Launch date (UTC)
Launch vehicle
Launch site
Object type
Shape & HBR
Cyl + 1 Ant, 3.5 m
Radar Cross Section
1.583 m², Large (>1 m²)
Expand to show TLE details & historyLast TLE update: 13 hours ago
TLE from 13 hours ago
0 COSMOS 2041
1 20235U 89074D 26122.11388118 .00000015 00000-0 20711-4 0 9995
2 20235 82.5840 239.1531 0008437 194.0044 340.1574 12.64845447690687Epoch: 2026-05-02T02:43Z
TLE epoch observation values (Epoch: 2026-05-02T02:43:59.333Z)
Latitude
5.74631°
Longitude
157.37267°
Altitude
1,399.006 km
Speed
7.164 km/s
True Right ascension
03h 53m 37s
True Declination
5° 42' 54"
Sunlit
Visualization orbit readout
Latitude
Unknown
Longitude
Unknown
Altitude
Unknown
Speed
Unknown
Apparent Right ascension
Unknown
Apparent Declination
Unknown
Sunlit
Visualization observer readout
Local Sidereal Time
23:22:51
Azimuth
Unknown
Elevation
Unknown
Doppler factor
Unknown
Orbital elements
Apogee altitude
1,406.888 km
Perigee altitude
1,393.763 km
Semi-major axis
7,778.462 km
Eccentricity
0.00084
Inclination
82.584°
RAAN
239.1531°
Arg. of periapsis
194.0044°
True anomaly
340.12455°
Mean anomaly
340.1574°
Eccentric anomaly
340.14098°
Mean motion
3.16375 °/min
Orbital period
113.79 mins
BSTAR
0.000020711
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Other satellites on launch #74 in the year 1989 (1989-09-14 UTC)
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You can import UDL-sourced sensor .json files into the Sandbox to generate a visibility chart that accounts for multi-vendor sensor geometry.COSMOS 2041 Visibility forecast
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Span | Click to sort rows by Start time (UTC) header in descending order | Start Az. | Max El. time (UTC) | Max El. Az. | Max El. | End time (UTC) | End Az. |
|---|---|---|---|---|---|---|---|
| 8 mins | 2026-05-02 17:38:03.397Z | 31.393° NE | 2026-05-02 17:42:03.397Z | 61.771° ENE | 14.638° | 2026-05-02 17:46:03.397Z | 92.009° ESE |
| 15 mins | 2026-05-02 19:31:03.397Z | 355.206° N | 2026-05-02 19:38:03.397Z | 69.939° E | 44.575° | 2026-05-02 19:46:03.397Z | 169.565° S |
| 9 mins | 2026-05-02 21:28:03.397Z | 312.525° NW | 2026-05-02 21:32:03.397Z | 279.392° WNW | 18.121° | 2026-05-02 21:37:03.397Z | 240.951° WSW |
| 5 mins | 2026-05-03 06:29:03.397Z | 88.858° E | 2026-05-03 06:31:03.397Z | 73.444° E | 13.227° | 2026-05-03 06:34:03.397Z | 51.44° ENE |
| 15 mins | 2026-05-03 08:17:03.397Z | 179.101° S | 2026-05-03 08:24:03.397Z | 96.698° ESE | 44.546° | 2026-05-03 08:32:03.397Z | 10.108° NNE |
| 10 mins | 2026-05-03 10:15:03.397Z | 255.739° W | 2026-05-03 10:20:03.397Z | 297.216° NW | 19.425° | 2026-05-03 10:25:03.397Z | 336.951° NNW |
Co-orbital & Co-planar RSOs
Thresholds — Semi-major Axis: ±100 km, RAAN: ±3°, Inclination: ±5°
TCA is derived from TLE conjunctions
Click to sort rows by RSO header in ascending order | Click to sort rows by Country header in ascending order | Click to sort rows by Type header in ascending order | Click to sort rows by Inclination Δ header in ascending order | Click to sort rows by RAAN Δ header in ascending order | Click to sort rows by Coplanar Angle header in ascending order | Click to sort rows by SMA Δ header in ascending order | Click to sort rows by Orbital period header in ascending order | Click to sort rows by <5km Md TCA header in descending order |
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CAUTION: Conjunctions in this section are generated from low-fidelity TLE screenings
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