Remote sensing analysis of solar-system objects

Details Remote sensing analysis of solar-system objects Remote sensing analysis of solar-system objects

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phst..130a4037e&link_type=abstract

Physica Scripta, Volume 130, Issue , pp. 014037 (2008).

Physics

Scientific paper

Most of our knowledge of solar-system objects has been achieved by remote sensing observations, and, in particular, by spectroscopy at all wavelengths. Solar-system spectra mainly show two components: a reflected solar component that peaks in the visible range, and a thermal component that extends in the infrared and millimetre range. Remote sensing observations of planets, satellites and comets have demonstrated the amazing variety of their atmospheric and surface properties; this variety is to be kept in mind when observations of extrasolar planets become available.

Affiliated with

Also associated with

No associations

Rating

Remote sensing analysis of solar-system objects 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 Remote sensing analysis of solar-system objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Remote sensing analysis of solar-system objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1807622