TY - JOUR
T1 - Practical method to identify orbital anomaly as spacecraft breakup in the geostationary region
AU - Uetsuhara, Masahiko
AU - Hanada, Toshiya
N1 - Funding Information:
The authors wish to acknowledge Mr. Yoshitaka Nakaniwa of Kyushu University for his dedicated assistance in data analyses. A part of this research is supported by Grant-in-Aid for JSPS Fellows Grant Number 243000.
PY - 2013/9/15
Y1 - 2013/9/15
N2 - Identifying spacecraft breakup events is an essential issue for better understanding of the current orbital debris environment. This paper proposes an observation planning approach to identify an orbital anomaly, which appears as a significant discontinuity in archived orbital history, as a spacecraft breakup. The proposed approach is applicable to orbital anomalies in the geostationary region. The proposed approach selects a spacecraft that experienced an orbital anomaly, and then predicts trajectories of possible fragments of the spacecraft at an observation epoch. This paper theoretically demonstrates that observation planning for the possible fragments can be conducted. To do this, long-term behaviors of the possible fragments are evaluated. It is concluded that intersections of their trajectories will converge into several corresponding regions in the celestial sphere even if the breakup epoch is not specified and it has uncertainty of the order of several weeks.
AB - Identifying spacecraft breakup events is an essential issue for better understanding of the current orbital debris environment. This paper proposes an observation planning approach to identify an orbital anomaly, which appears as a significant discontinuity in archived orbital history, as a spacecraft breakup. The proposed approach is applicable to orbital anomalies in the geostationary region. The proposed approach selects a spacecraft that experienced an orbital anomaly, and then predicts trajectories of possible fragments of the spacecraft at an observation epoch. This paper theoretically demonstrates that observation planning for the possible fragments can be conducted. To do this, long-term behaviors of the possible fragments are evaluated. It is concluded that intersections of their trajectories will converge into several corresponding regions in the celestial sphere even if the breakup epoch is not specified and it has uncertainty of the order of several weeks.
UR - http://www.scopus.com/inward/record.url?scp=84883448680&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84883448680&partnerID=8YFLogxK
U2 - 10.1016/j.asr.2013.06.003
DO - 10.1016/j.asr.2013.06.003
M3 - Article
AN - SCOPUS:84883448680
SN - 0273-1177
VL - 52
SP - 1072
EP - 1077
JO - Advances in Space Research
JF - Advances in Space Research
IS - 6
ER -