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Hot Shadows of Jupiter

Wildey, Robert L. (1965) Hot Shadows of Jupiter. Science, 147 (3661). pp. 1035-1036. ISSN 0036-8075. http://resolver.caltech.edu/CaltechAUTHORS:20151209-155238142

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Abstract

On the evenings of 26 October and 15 December 1962, while the disk of Jupiter was being scanned for thermal emission in the 8- to 14-micron wavelength region, a large enhancement was discovered in the emission from shadows cast on Jupiter by the Jovian satellites Ganymede and Europa. However, on the evening of 14 December 1964, the shadow of satellite Io was observed and no enhancement was detected. The effect is thus variable with time.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1126/science.147.3661.1035DOIArticle
http://www.sciencemag.org/content/147/3661/1035PublisherArticle
http://www.jstor.org/stable/1715236JSTORArticle
Additional Information:© 1965 American Association for the Advancement of Science. Received 1 February 1965.
Record Number:CaltechAUTHORS:20151209-155238142
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20151209-155238142
Official Citation:Hot Shadows of Jupiter Robert L. Wildey Science 26 February 1965: 147 (3661), 1035-1036. [DOI:10.1126/science.147.3661.1035]
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:62758
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:10 Dec 2015 20:43
Last Modified:10 Dec 2015 20:43

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