Abstract
A novel method, called the crossover technique, has been devised for the remote determination of the surface temperature of planets, satellites, and asteroids having a negligible atmosphere. The method is discussed using new spectra of Mars as an example, and it is shown how it might be extended to other solar system objects. The accuracy of the method, both absolutely and in comparison to other methods, is also considered.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
