Polarimetry Probes Brown Dwarf

Polarimetry Probes Brown Dwarf Clouds which shows signs of cloud bands similar to those seen on Jupiter Currently Luhman 16 is the third-closest-known star/brown-dwarf system to the Sun after the triple Alpha Centauri system (4.37 ly) and Barnard's Star (5.98 ly), Luhman 16A is part of a binary system (Luhman 16) containing a second brown dwarf, Luhman 16B. This pair of brown dwarfs Luhman 16A and Luhman 16B orbit each other. Despite the fact that Luhman 16A and 16B have similar masses and temperatures and presumably formed at the same time, they show markedly different weather.
Luhman 16B shows no sign of stationary cloud bands, instead showing evidence of more irregular, patchy clouds
Polarimetry is the measurement and interpretation of the polarization of transverse waves, most notably electromagnetic waves, such as radio or light waves. Typically polarimetry is done on electromagnetic waves that have traveled through or have been reflectedrefracted, or diffracted by some material in order to characterize that object.

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