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.

引用

页码：189 / 194

页数：6

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