Physical studies of asteroids .30. The asteroid 153 Hilda

被引：1
|
作者：
Lagerkvist, CI
DiMartino, M
Blanco, C
Dahlgren, M
Erikson, A
Lahulla, JF
Lazzarin, M
Lumme, K
Pohjolainen, S
Riccioli, D
机构：
[1] OSSERV ASTRON TORINO,I-10025 PINO TORINESE,ITALY
[2] UNIV CATANIA,IST ASTRON,I-95125 CATANIA,ITALY
[3] GERMAN AEROSP RES ESTAB,D-12489 BERLIN,GERMANY
[4] ASTRON OBSERV,E-28014 MADRID,SPAIN
[5] UNIV PADUA,DIPARTIMENTO FIS,I-35131 PADUA,ITALY
[6] HELSINKI UNIV OBSERV,SF-00014 HELSINKI,FINLAND
[7] HELSINKI UNIV TECHNOL,METSAHOVI RADIO RES STN,SF-02150 ESPOO,FINLAND
来源：
EARTH MOON AND PLANETS | 1995年 / 71卷 / 03期
关键词：
D O I：
10.1007/BF00612956
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The asteroid 153 Kilda was studied by photometric, spectroscopic and polarimetric observations during the apparition in 1992. The rotation period was determined to 5.11 hours with a lightcurve amplitude of 0.05 magnitudes. From our spectrum we find 153 Hilda to be of taxonomic type P. The polarization value of -0.23 at a phase angle of 3.2 degrees seems normal for a P-type asteroid. Long term integrations of the orbit shows that it is stable over time intervals of several million years.
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收藏
页码：189 / 194
页数：6
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