Rotating-drift-scan observation and orbit determination of near-Earth asteroids
- Autores
- Tang, K.; Pomazan, A.; Maigurova, N.; Song, Y.; Yu, Y.; Mao, Y.; Tang, Z.
- Año de publicación
- 2025
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- Precise observations of near-Earth asteroids (NBAs) are critical for ex tending observational arcs, refining their orbits, and ensuring Earth’s safety through accurate impact prediction. However, their high apparent motion during close Earth encounters presents a significant challenge to precise ob servation. The rotating-drift-scan (RDS) charge-coupled device (CCD) tech nique offers a promising solution for observing these fast-moving NBAs during close approaches. By rotating the telescope camera, time delay integration is enabled, allowing the NBA to be imaged as a point source despite long exposure times.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Asteroids
Impact prediction
Monitoring system - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-nd/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/192131
Ver los metadatos del registro completo
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Rotating-drift-scan observation and orbit determination of near-Earth asteroidsTang, K.Pomazan, A.Maigurova, N.Song, Y.Yu, Y.Mao, Y.Tang, Z.Ciencias AstronómicasAsteroidsImpact predictionMonitoring systemPrecise observations of near-Earth asteroids (NBAs) are critical for ex tending observational arcs, refining their orbits, and ensuring Earth’s safety through accurate impact prediction. However, their high apparent motion during close Earth encounters presents a significant challenge to precise ob servation. The rotating-drift-scan (RDS) charge-coupled device (CCD) tech nique offers a promising solution for observing these fast-moving NBAs during close approaches. By rotating the telescope camera, time delay integration is enabled, allowing the NBA to be imaged as a point source despite long exposure times.Facultad de Ciencias Astronómicas y Geofísicas2025-08info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionResumenhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/192131enginfo:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/190232info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-nd/4.0/Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2026-03-31T12:42:01Zoai:sedici.unlp.edu.ar:10915/192131Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-03-31 12:42:01.933SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Rotating-drift-scan observation and orbit determination of near-Earth asteroids |
| title |
Rotating-drift-scan observation and orbit determination of near-Earth asteroids |
| spellingShingle |
Rotating-drift-scan observation and orbit determination of near-Earth asteroids Tang, K. Ciencias Astronómicas Asteroids Impact prediction Monitoring system |
| title_short |
Rotating-drift-scan observation and orbit determination of near-Earth asteroids |
| title_full |
Rotating-drift-scan observation and orbit determination of near-Earth asteroids |
| title_fullStr |
Rotating-drift-scan observation and orbit determination of near-Earth asteroids |
| title_full_unstemmed |
Rotating-drift-scan observation and orbit determination of near-Earth asteroids |
| title_sort |
Rotating-drift-scan observation and orbit determination of near-Earth asteroids |
| dc.creator.none.fl_str_mv |
Tang, K. Pomazan, A. Maigurova, N. Song, Y. Yu, Y. Mao, Y. Tang, Z. |
| author |
Tang, K. |
| author_facet |
Tang, K. Pomazan, A. Maigurova, N. Song, Y. Yu, Y. Mao, Y. Tang, Z. |
| author_role |
author |
| author2 |
Pomazan, A. Maigurova, N. Song, Y. Yu, Y. Mao, Y. Tang, Z. |
| author2_role |
author author author author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Asteroids Impact prediction Monitoring system |
| topic |
Ciencias Astronómicas Asteroids Impact prediction Monitoring system |
| dc.description.none.fl_txt_mv |
Precise observations of near-Earth asteroids (NBAs) are critical for ex tending observational arcs, refining their orbits, and ensuring Earth’s safety through accurate impact prediction. However, their high apparent motion during close Earth encounters presents a significant challenge to precise ob servation. The rotating-drift-scan (RDS) charge-coupled device (CCD) tech nique offers a promising solution for observing these fast-moving NBAs during close approaches. By rotating the telescope camera, time delay integration is enabled, allowing the NBA to be imaged as a point source despite long exposure times. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
Precise observations of near-Earth asteroids (NBAs) are critical for ex tending observational arcs, refining their orbits, and ensuring Earth’s safety through accurate impact prediction. However, their high apparent motion during close Earth encounters presents a significant challenge to precise ob servation. The rotating-drift-scan (RDS) charge-coupled device (CCD) tech nique offers a promising solution for observing these fast-moving NBAs during close approaches. By rotating the telescope camera, time delay integration is enabled, allowing the NBA to be imaged as a point source despite long exposure times. |
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2025 |
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2025-08 |
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http://sedici.unlp.edu.ar/handle/10915/192131 |
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eng |
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info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/190232 |
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