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Since molecules and dimers absorb different frequencies of light, studying the spectrum of starlight that has passed through a planetary atmosphere could reveal its atmospheric pressure.
The Lorentz force, acting on an electrostatically charged spacecraft as it moves through a planetary magnetic field, provides a new propellantless method for orbital maneuvers.
Refraction due to gradients in ionospheric electron density, Ne, and neutral number density, nn, can shift the frequency of radio signals propagating through a planetary atmosphere.
We then calculate the colors using our simulated spectra (Section 2.4) that account for the effects of viewing a surface through a planetary atmosphere.
We have also shown that pigmented organisms do not occupy a unique region of visible broadband color-color space and that the broadband colors of biological and abiotic surfaces are altered significantly when viewed through a planetary atmosphere.
Second, we generate synthetic spectra with a 1-D radiative transfer model that simulates ideal cases where single surface types dominate planetary surfaces and are viewed through a planetary atmosphere.
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This includes eccentric orbits, which could be fixed, for example, through interactions with a planetary companion (Van Laerhoven et al., 2014).
So called because the smaller varieties almost resemble planetary disks when viewed through a telescope, planetary nebulae represent a stage at the end of the stellar life cycle rather than one at the beginning.
But in an age when anyone can make a planetary discovery through a $400 telescope then instantly share it with the world — hey, check out my cool Jupiter shots on Flickr!
We are through our intelligence and communication a planetary equivalent of a nervous system.
There is some indication of a local time dependence in the occurrence of the clouds in the northern hemisphere which may arise from the passage of a planetary wave through the regions available for observation from geostationary orbit.
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