Comprehensive Photometry of the Rings and 16 Satellites of Uranus with the Hubble Space Telescope
Dynamics of cloud features on Uranus
Keck Adaptive Optics Images of Uranus and Its Rings
Near-IR photometry of the small Uranian satellites with Keck at phase angles 0-2deg
New Measurements of the Winds of Uranus
Probable detection of hydrogen sulphide (H2S) in Neptunes atmosphere
Spatially resolved cloud structure on Uranus: Implications of near-IR adaptive optics imaging
The haze and methane distributions on Uranus from HST-STIS spectroscopy
UV star-formation rates of GRB host galaxies
Instrument
NICMOS, NICMOS/NIC1, NICMOS/NIC2
Temporal Coverage
1998-08-05T01:26:05Z/1998-08-08T23:12:12Z
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, Hammel comma Heidi B., 1999, 'Uranus Nearing Equinox: Vertical Aerosol Distribution of Atmospheric Structure', 1.0, European Space Agency, https://doi.org/10.5270/esa-vepxt9w