GEO satellite tracking
Continuous or occasional observations to support orbit determination, catalogue maintenance and long-term monitoring.
OPTICAL SATELLITE TRACKING · GEO SSA / SST
A clearer view
of what’s in orbit.
Scientific-grade optical data for satellite tracking and space situational awareness. From detection to characterisation, turn observations into understanding.
From a point of light.
To a measurable trajectory.
THE SKY, MEASURED.ANGANA.SPACE / OPTICAL OBSERVATIONS
170
professional telescopes, observatories & facilities60 cm+
typical scientific-grade apertures18–19 mag
faint-object detection capability<1 arcsec
typical GEO precision per frame01 / CAPABILITIES
Keep sight of
the objects that matter.
Targeted observations for satellite operators, research teams and organisations working in space surveillance and tracking.
Object characterisation
Position and brightness measurements to investigate photometric variability, rotational signatures and the behaviour of satellites and orbital debris.
Follow-up & anomaly investigation
Global observing coverage for follow-up and variability monitoring, with cross-validation across independent sites and instruments.
02 / DATA PRODUCTS
Observations you
can put to work.
Gaia-referenced astrometry and calibrated photometry. Traceable measurements for orbit determination, object characterisation and monitoring.
01
Calibrated observation images
02
Detection reports and alerts
03
Astrometric measurements
04
Photometric measurements
05
Standardised light curves
Independent observing sites and instruments help cross-validate detections and increase confidence in results.
Every change in brightness tells a story.
Photometric variability reveals how an object changes over time.
03 / THE SCIENTIFIC DIFFERENCE
Fainter objects.
Sharper measurements.
Scientific-grade sensitivity
With typical apertures of 60 cm+ and 18–19 magnitude detection capability, observe faint satellites and orbital debris that demand sensitive optical measurements.
Precision with provenance
Gaia-referenced astrometry delivers typical sub-arcsecond GEO precision per frame. Calibrated photometry supports consistent brightness measurements and light curves.
A global perspective
Observations across a global network support follow-up and long-term monitoring, with resilience to local observing conditions.
LET’S DEFINE YOUR OBSERVATION
What do you need
to keep in sight?
Tell us your target, cadence and data requirements.
We’ll show you what we can deliver.
Dr. Elżbieta Łazarewicz-Wyrzykowska
CEO
Prof. Łukasz Wyrzykowski
CTO · Astronomical Observatory, University of Warsaw
National Centre for Nuclear Research