SeekSat

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Current satellite positions
SatelliteLatitudeLongitude
TOM-3
SeekSat

TOM-3

launched 2026low orbitNORAD 69906 · 2026-156AP

Height
603.7 km
From center
6,961.9 km
Sunlight
Sunlit
Speed
7.566 km/s
Ground speed
6.974 km/s
Over
75.043° N, 146.953° E

Passes

Technical details

Mean elements

Elements are 1.3 days old, from CelesTrak GP data (groups: active), fetched 18 h ago.How accurate is this?

Perigee
588 km
Apogee
595 km
Period
96.51 min
Inclination
97.74°
Eccentricity
0.0005509
Semi-major axis
6,969.7 km
Epoch
2026-11-14T16:05:26Z

Orbit check

The live speed and distance fit this orbit to within 0.12%.

Vis-viva: v²r/GM = 0.9999 and 2 − r/a = 1.0011

Raw elements

2LE

1 69906U 26156AP  26318.67044356  .00001564  00000+0  16336-3 0  9992
2 69906  97.7368 216.6413 0005509  63.6479 296.5304 14.91093707 19425

3LE

TOM-3
1 69906U 26156AP  26318.67044356  .00001564  00000+0  16336-3 0  9992
2 69906  97.7368 216.6413 0005509  63.6479 296.5304 14.91093707 19425

OMM

{
  "OBJECT_NAME": "TOM-3",
  "OBJECT_ID": "2026-156AP",
  "EPOCH": "2026-11-14T16:05:26.324448",
  "MEAN_MOTION": 14.91093707,
  "ECCENTRICITY": 0.00055088,
  "INCLINATION": 97.7368,
  "RA_OF_ASC_NODE": 216.6413,
  "ARG_OF_PERICENTER": 63.6479,
  "MEAN_ANOMALY": 296.5304,
  "EPHEMERIS_TYPE": 0,
  "CLASSIFICATION_TYPE": "U",
  "NORAD_CAT_ID": 69906,
  "ELEMENT_SET_NO": 999,
  "REV_AT_EPOCH": 1942,
  "BSTAR": 0.00016335814,
  "MEAN_MOTION_DOT": 0.00001564,
  "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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