Io: Ground-Based Observations of Hot Spots
Abstract
Observations of Io in eclipse demonstrate conclusively that Io emits substantial amounts of radiation at 4.8 and 3.8 micrometers and a measurable amount at 2.2 micrometers. Color temperatures derived from the observations fit blackbody emission at 560 K. The required source area to yield the observed 4.8-micrometer flux is approximately 5 × 10-5 of the disk of Io and is most likely comprised of small hot spots in the vicinity of the volcanoes.
- Publication:
-
Science
- Pub Date:
- November 1980
- DOI:
- 10.1126/science.210.4473.1015
- Bibcode:
- 1980Sci...210.1015S
- Keywords:
-
- Infrared Astronomy;
- Io;
- Planetary Temperature;
- Ground Stations;
- Volcanoes;
- Lunar and Planetary Exploration; Jupiter;
- JUPITER;
- SATELLITES;
- IO;
- ECLIPSES;
- EARTH-BASED OBSERVATIONS;
- EMISSIONS;
- RADIATION;
- TEMPERATURES;
- VOLCANOES;
- PHOTOMETRY;
- BRIGHTNESS;
- MAGNITUDE;
- REFLECTANCE;
- RADIOMETERY;
- INFRARED SPECTROSCOPY;
- WAVELENGTHS;
- FLUX;
- SCATTERING;
- ABSORPTION