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Current satellite positions
SatelliteLatitudeLongitude
STARLINK-4667
SeekSat

STARLINK-4667

Starlinklaunched 2022low orbitNORAD 53707 · 2022-107H

Height
467.7 km
From center
6,833.4 km
Sunlight
Sunlit
Speed
7.639 km/s
Ground speed
6.839 km/s
Over
49.844° N, 167.856° E

Passes

Technical details

Mean elements

Elements are 17 hours old, from CelesTrak GP data (groups: active), fetched 11 h ago.How accurate is this?

Perigee
462 km
Apogee
464 km
Period
93.85 min
Inclination
53.16°
Eccentricity
0.0001119
Semi-major axis
6,841.1 km
Epoch
2026-11-15T06:14:56Z

Orbit check

The live speed and distance fit this orbit to within 0.074%.

Vis-viva: v²r/GM = 1.0004 and 2 − r/a = 1.0011

Raw elements

2LE

1 53707U 22107H   26319.26037501  .00000444  00000+0  24264-4 0  9992
2 53707  53.1577 160.7001 0001119  63.2843 296.8274 15.34392425233212

3LE

STARLINK-4667
1 53707U 22107H   26319.26037501  .00000444  00000+0  24264-4 0  9992
2 53707  53.1577 160.7001 0001119  63.2843 296.8274 15.34392425233212

OMM

{
  "OBJECT_NAME": "STARLINK-4667",
  "OBJECT_ID": "2022-107H",
  "EPOCH": "2026-11-15T06:14:56.401728",
  "MEAN_MOTION": 15.34392425,
  "ECCENTRICITY": 0.00011193,
  "INCLINATION": 53.1577,
  "RA_OF_ASC_NODE": 160.7001,
  "ARG_OF_PERICENTER": 63.2843,
  "MEAN_ANOMALY": 296.8274,
  "EPHEMERIS_TYPE": 0,
  "CLASSIFICATION_TYPE": "U",
  "NORAD_CAT_ID": 53707,
  "ELEMENT_SET_NO": 999,
  "REV_AT_EPOCH": 23321,
  "BSTAR": 0.000024264443,
  "MEAN_MOTION_DOT": 0.00000444,
  "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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