NEAR-ULTRAVIOLET IMAGING OF JUPITER SATELLITE IO WITH THE HUBBLE SPACE TELESCOPE

被引：0

作者：

PARESCE, F

SARTORETTI, P

ALBRECHT, R

BARBIERI, C

BLADES, JC

BOKSENBERG, A

CRANE, P

DEHARVENG, JM

DISNEY, MJ

JAKOBSEN, P

KAMPERMAN, TM

KING, IR

MACCHETTO, F

MACKAY, CD

WEIGELT, G

BAXTER, D

GREENFIELD, P

JEDRZEJEWSKI, R

NOTA, A

SPARKS, WB

机构：

[1] EUROPEAN SPACE AGCY, DEPT SPACE SCI, DIV ASTROPHYS, F-75738 PARIS 15, FRANCE

[2] OSSERV ASTRON PADOVA, I-35122 PADUA, ITALY

[3] ROYAL GREENWICH OBSERV, CAMBRIDGE CB3 0EZ, ENGLAND

[4] EUROPEAN SO OBSERV, W-8046 GARCHING, GERMANY

[5] CNRS, ASTRON SPATIALE LAB, F-13012 MARSEILLE, FRANCE

[6] UNIV COLLEGE CARDIFF, DEPT PHYS, CARDIFF CF1 3TH, WALES

[7] EUROPEAN SPACE AGCY, EUROPEAN SPACE RES & TECHNOL CTR, DEPT SPACE SCI, DIV ASTROPHYS, 2200 AG NOORDWIJK, NETHERLANDS

[8] SPACE RES INST, SPACE RES LAB, 3584 CA UTRECHT, NETHERLANDS

[9] UNIV CALIF BERKELEY, DEPT ASTRON, BERKELEY, CA 94720 USA

[10] UNIV CAMBRIDGE, INST ASTRON, CAMBRIDGE CB3 0HA, ENGLAND

[11] MAX PLANCK INST RADIOASTRON, W-5300 BONN 1, GERMANY

来源：

ASTRONOMY & ASTROPHYSICS | 1992年 / 262卷 / 02期

关键词：

UV RADIATION; PLANETS AND SATELLITES; SATELLITES;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The surface of Jupiter's Galilean satellite Io has been resolved for the first time in the near ultraviolet at 2850 angstrom by the Faint Object Camera (FOC) on the Hubble Space Telescope (HST). The restored images reveal significant surface structure down to the resolution limit of the optical system corresponding to approximately 250 km at the sub-earth point.

引用

页码：617 / 620

页数：4

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