Astrometry of Saturns Satellites from the Hubble Space Telescope WFPC2
A strong decrease in Saturns equatorial jet at cloud level
A strong vortex in Saturns South Pole
Cassini Imaging Science: Initial Results on Saturns Atmosphere
HST observations of azimuthal asymmetry in Saturns rings
HST observations of spokes in Saturns B ring
Interior properties of the inner Saturnian moons from space astrometry data
Near-infrared spectra of the leading and trailing hemispheres of Enceladus
No Hexagonal Wave around Saturns Southern Pole
Numerical modeling of atmospheric jet streams on Jupiter and Saturn: Their formation and stability
Saturns cloud structure and temporal evolution from ten years of Hubble Space Telescope images (1994 2003)
Saturns Rings at True Opposition
Saturns wayward shepherds: the peregrinations of Prometheus and Pandora
Short-term changes in the belt/zone structure of Saturns Southern Hemisphere (1996-2004)
The Bolometric Bond Albedo of Enceladus
The Gravity Field of the Saturnian System from Satellite Observations and Spacecraft Tracking Data
The opposition and tilt effects of Saturns rings from HST observations
The opposition surge of Enceladus: HST observations 338-1022 nm
The Orbits of Saturns Small Satellites Derived from Combined Historic and Cassini Imaging Observations
The Orbits of the Main Saturnian Satellites, the Saturnian System Gravity Field, and the Orientation of Saturns Pole
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2001-09-08T04:49:14Z/2002-01-31T11:43:15Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, French comma Richard G., 2003, 'Saturn's Rings and Small Moons', 1.0, European Space Agency, https://doi.org/10.5270/esa-fj981oh
