Near-infrared spectrophotometry of the satellites and rings of Uranus
โ Scribed by B.T. Soifer; G. Neugebauer; K. Matthews
- Publisher
- Elsevier Science
- Year
- 1981
- Tongue
- English
- Weight
- 391 KB
- Volume
- 45
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
## Using the CoCo Cold Coronagraph at NASA's Infrared Telescope Facility on Mauna Kea, we observed the uranian satellites Miranda, Puck, Portia, and Rosalind and the neptunian satellite Proteus in the near infrared (JHK) to determine the albedos of those faint satellites. In V-J, all of Puck, Port
We have observed the leading and trailing hemispheres of Phobos from 1.65 to 3.5 ยตm and Deimos from 1.65 to 3.12 ยตm near opposition. We find the trailing hemisphere of Phobos to be brighter than its leading hemisphere by 0.24 ยฑ 0.06 magnitude at 1.65 ยตm and brighter than Deimos by 0.98 ยฑ 0.07 magnit