Planetary observations at a wavelength of 1.32 MM

Details Planetary observations at a wavelength of 1.32 MM Planetary observations at a wavelength of 1.32 MM

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984icar...60..590u&link_type=abstract

Icarus (ISSN 0019-1035), vol. 60, Dec. 1984, p. 590-598. NASA-supported research.

Astronomy and Astrophysics

Astronomy

44

Callisto, Ceres Asteroid, Ganymede, Gas Giant Planets, Planetary Temperature, Radio Astronomy, Brightness Temperature, H Ii Regions, Jupiter (Planet), Millimeter Waves, Planetary Atmospheres

Scientific paper

Observations at a wavelength of 1.32 mm have been made of the Jovian planets, Ceres, the satellites Callisto and Ganymede, and the H II region DR 21. The observed brightness temperatures are presented. Those of the Jovian planets agree with the values expected from model atmosphere calculations, except that of Jupiter, which is lower than expected. Ceres and the satellites do not have atmospheres so their emission arised in their subsurface layers. The observed brightness temperatures are intermediate between those measured at infrared and centimeter wavelengths.

Affiliated with

Also associated with

No associations

Rating

Planetary observations at a wavelength of 1.32 MM does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Planetary observations at a wavelength of 1.32 MM, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Planetary observations at a wavelength of 1.32 MM will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-736615