Given the increasing number of active satellites and space debris in the Geostationary Earth Orbit (GEO) ring, a continuous and accurate monitoring of these objects is strictly necessary and increasingly important. By accurately determining their orbits, Space Surveillance and Tracking (SST) services play a critical role in ensuring the safety and sustainability of space operations in the GEO region. Optical measurements are a key source of data for the Orbit Determination (OD) of GEO objects. In this paper, the research team from Sapienza Space Systems and Space Surveillance Laboratory (S5Lab) suggests a method for the correlation of optical measurements and a precise anglesonly OD technique that can be used to compute an accurate orbit of observed space objects. S5Lab owns a network of telescopes and observations systems for both Space Situational Awareness (SSA) activities and Space Traffic Management (STM), among which two persistent monitoring wide field-of-view observation systems for monitoring the GEO ring: SURGE (located in Italy) and Mini-SURGE (located in Australia). The optical data used in the context of this paper were gathered using these two observation systems. Every night tens of thousands of uncorrelated optical measurements, in terms of Right Ascension (RA) and Declination (Dec), are acquired. Processing this amount of data is a challenging task that involves identifying and matching optical measurements of an object over time. One approach to correlation of optical measurements is to use catalogue-based methods. This involves comparing the observed position of an object to a catalogue of known objects in the field of view. When catalogue-based methods are unsuccessful, another approach is provided that can be used in place of or in addition to them. This might be the case of newly detected objects that have not been included in public catalogues. Finally, an accurate orbit for each observed space object is computed using a non-linear least squares differential-correction technique. Both the correlation and the OD procedure are validated with reference satellites having known high accuracy ephemerides.
GEO Optical Measurements Correlation and Angles-Only Orbit Determination / Varanese, Simone; Mariani, Lorenzo; Zarcone, Gaetano; Bucciarelli, Mascia; Cimino, Lorenzo; Rossetti, Matteo; Kelecy, Thomas M.. - (2023). (Intervento presentato al convegno 74th International Astronautical Congress tenutosi a Baku; Azerbaijan).
GEO Optical Measurements Correlation and Angles-Only Orbit Determination
Simone Varanese
;Lorenzo Mariani;Gaetano Zarcone;Mascia Bucciarelli;Lorenzo Cimino;Matteo Rossetti;
2023
Abstract
Given the increasing number of active satellites and space debris in the Geostationary Earth Orbit (GEO) ring, a continuous and accurate monitoring of these objects is strictly necessary and increasingly important. By accurately determining their orbits, Space Surveillance and Tracking (SST) services play a critical role in ensuring the safety and sustainability of space operations in the GEO region. Optical measurements are a key source of data for the Orbit Determination (OD) of GEO objects. In this paper, the research team from Sapienza Space Systems and Space Surveillance Laboratory (S5Lab) suggests a method for the correlation of optical measurements and a precise anglesonly OD technique that can be used to compute an accurate orbit of observed space objects. S5Lab owns a network of telescopes and observations systems for both Space Situational Awareness (SSA) activities and Space Traffic Management (STM), among which two persistent monitoring wide field-of-view observation systems for monitoring the GEO ring: SURGE (located in Italy) and Mini-SURGE (located in Australia). The optical data used in the context of this paper were gathered using these two observation systems. Every night tens of thousands of uncorrelated optical measurements, in terms of Right Ascension (RA) and Declination (Dec), are acquired. Processing this amount of data is a challenging task that involves identifying and matching optical measurements of an object over time. One approach to correlation of optical measurements is to use catalogue-based methods. This involves comparing the observed position of an object to a catalogue of known objects in the field of view. When catalogue-based methods are unsuccessful, another approach is provided that can be used in place of or in addition to them. This might be the case of newly detected objects that have not been included in public catalogues. Finally, an accurate orbit for each observed space object is computed using a non-linear least squares differential-correction technique. Both the correlation and the OD procedure are validated with reference satellites having known high accuracy ephemerides.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.