SeekSat

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Current satellite positions
SatelliteLatitudeLongitude
COSMOS 2524
SeekSat

COSMOS 2524

launched 2017low orbitNORAD 43032 · 2017-076A

Height
916.5 km
From center
7,277.2 km
Sunlight
Sunlit
Speed
7.398 km/s
Ground speed
6.287 km/s
Over
64.579° N, 111.904° W

Passes

Technical details

Mean elements

Elements are 10 hours old, from CelesTrak GP data (groups: active), fetched 3 h ago.How accurate is this?

Perigee
897 km
Apogee
905 km
Period
103.01 min
Inclination
67.14°
Eccentricity
0.0005547
Semi-major axis
7,279.1 km
Epoch
2026-11-15T13:04:18Z

Orbit check

The live speed and distance fit this orbit to within 0.097%.

Vis-viva: v²r/GM = 0.9993 and 2 − r/a = 1.0003

Raw elements

2LE

1 43032U 17076A   26319.54466205  .00000166  00000+0  17154-3 0  9999
2 43032  67.1449 184.1150 0005547 311.6541  48.4069 13.97443858456757

3LE

COSMOS 2524
1 43032U 17076A   26319.54466205  .00000166  00000+0  17154-3 0  9999
2 43032  67.1449 184.1150 0005547 311.6541  48.4069 13.97443858456757

OMM

{
  "OBJECT_NAME": "COSMOS 2524",
  "OBJECT_ID": "2017-076A",
  "EPOCH": "2026-11-15T13:04:18.801120",
  "MEAN_MOTION": 13.97443858,
  "ECCENTRICITY": 0.0005547,
  "INCLINATION": 67.1449,
  "RA_OF_ASC_NODE": 184.115,
  "ARG_OF_PERICENTER": 311.6541,
  "MEAN_ANOMALY": 48.4069,
  "EPHEMERIS_TYPE": 0,
  "CLASSIFICATION_TYPE": "U",
  "NORAD_CAT_ID": 43032,
  "ELEMENT_SET_NO": 999,
  "REV_AT_EPOCH": 45675,
  "BSTAR": 0.00017154,
  "MEAN_MOTION_DOT": 0.00000166,
  "MEAN_MOTION_DDOT": 0
}

How we compute these

Altitude
Height above the WGS84 ellipsoid, the standard model of Earth's shape, straight below the satellite.
Speed
The length of SGP4's velocity vector in the TEME frame: the inertial speed. It is not the speed over the ground.
Ground speed
How fast the point below the satellite moves across Earth's surface, with Earth's rotation taken out.
From Earth's center
Distance from Earth's center, from SGP4's position.
Latitude and longitude
The point on the WGS84 ellipsoid straight below the satellite, from SGP4's position turned into Earth-fixed coordinates.
Sunlight
How much sunlight reaches the satellite past Earth and its atmosphere. Light grazing Earth is dimmed by air and ozone, bent into the shadow by refraction, and blocked below 10 km (clouds and haze); the Sun's disc is darker at its edge. So the satellite fades over a few seconds in low orbit and a couple of minutes in geostationary orbit, reddening as it goes, rather than switching off. The atmosphere is a clear standard one: haze from a large volcanic eruption can make the real fade come a few seconds early.
Orbit check (vis-viva)
v²r/GM uses the live speed and distance above, with GM = 398,600.4418 km³/s². Vis-viva says it equals 2 − r/a, where a is the mean semi-major axis. They agree as closely as SGP4's mean elements allow, usually within 1%.
Mean elements
Perigee, apogee, period, eccentricity, inclination and semi-major axis are mean elements from the published set, not instantaneous values. Perigee and apogee heights are above Earth's equatorial radius (6,378 km).
Epoch
The epoch is the moment the element set describes. Positions get less accurate the further you are from it.
How accurate is this?
Positions are predictions from the published elements, not live tracking. Through SGP4 they are usually within a kilometre or two near the epoch and drift by a few km a day after it, more for low or manoeuvring satellites. The map shows ground positions, the point straight below the satellite, so dots that look close can be thousands of km apart in height. Good for passes and tracks; not for judging close approaches between objects.
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