File:Brightness Variations in Saturn's Satellite 1995S5 (1995-31-324).jpg
Brightness_Variations_in_Saturn's_Satellite_1995S5_(1995-31-324).jpg (200 × 200 pixels, file size: 8 KB, MIME type: image/jpeg)
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Summary
[edit]DescriptionBrightness Variations in Saturn's Satellite 1995S5 (1995-31-324).jpg |
English: This sequence of 100 sec exposures taken with HST's Wide Field and Planetary Camera (WFPC2) in planetary mode on 10 August 1995 shows the newly discovered object 1995S5 (red arrows) moving in its orbit around the planet. As it moves further from Saturn, its brightness decreases appreciably. This brightness variation is more consistent with that expected for an elongated, opaque clump of ring material than for a satellite, leading to the suspicion that 1995S5 is in fact a ring arc rather than a previously undiscovered satellite. It is likely that it lies within the narrow, braided F Ring. |
Date | 11 August 1995 (upload date) |
Source | Brightness Variations in Saturn's Satellite 1995S5 |
Author | Phil Nicholson (Cornell University), Mark Showalter (NASA-Ames/Stanford) and NASA |
Keywords InfoField | Moons; Planets; Saturn; Solar System; Planetary Rings |
Licensing
[edit]Public domainPublic domainfalsefalse |
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org. For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag. |
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