The Umov Effect: Space Dust Clouds and The Mysteries of The Universe

The methodology under development is based on the Umov effect – an inverse correlation between the reflectivity of a body and the degree of linear polarization of light scattered by it. The brighter is an object, the lower polarization it produces. This relation was first formulated by the Russian physicist Nikolay Umov in 1905.

According to Evgenij Zubko, previously the Umov effect was studied only for surfaces, such as regolite (Moon surface) and the surfaces of asteroids. The explanation of this effect given in 1960-1970s, excluded its application to single dust particles that comprise the regolite. However, the team concluded that the Umov effect is almost equally applicable to individual particles and surfaces in general.

Previously the researchers concluded that the Umov effect holds in a homogenous sparse cloud of space dust. In the article published in the July 11, 2018 print issue of Monthly Notices of the Royal Astronomical Society the scientists suggested that this physical effect could be also applicable to clouds consisting of two types of dust particles which is characteristic of comae and tails of comets. The Umov effect is also expected to be observed in a three-component clouds of cosmic dust that is more typical for protoplanetary disks.

This is Comet Garradd and the Coat Hanger.

Credit: Rogelio Bernal Andreo

After studying the degree of linear polarization acquired by sunlight when it is scattered by cometary dust particles, scientists are able to give reliable estimation of the particles’ albedo or reflectivity. This characteristic is an extremely important for retrieval the total volume of dust expelled from a comet. The latter parameter allows the scientists to improve the existing methods of estimation of the dust-to-gas volume ratio in cometary comae. This is one of the most important characteristic of a cometary evolution – for example, it could indicate the place in the Solar System in which the comet was formed.

“Knowing the ratio between the volumes of ejected dust and gas, we can better understand the evolutionary stages passed by different comets and the circumstances of the Solar-System formation. However, while it is easy to calculate the volume of gas in a comet, in case of dust particles this is much more complicated,” said Evgenij Zubko. “When we measure the sunlight reflected by the coma, we need to understand the number of dust particles that contribute to the sunlight scattering. Their albedo or reflectivity is the key data we require to answer this question. However, different dust particles also behave differently, and the difference in the reflectivity of dark and bright particles in comets may exceed ten times. This is a common issue nowadays that also arises in other areas of astrophysics, such as the evaluation of matter volumes in protoplanetary disks around other stars.

We strive to understand the value of this albedo and use additional methods to do so – in particular, polarimetry to measure the degree of linear polarization and, thus, retrieve the reflectivity of cometary dust particles based on the Umov effect.”

There is still a lot to be discovered in the course of this work. “We are literally chasing a ghost,” says the scientist. He also pointed out that to achieve a breakthrough in this area of studies, groups of astrophysicists from different parts of the world had to extensively collaborate.

The analysis methodology based on the Umov effect may be further used in other areas besides the studies of comets. It may serve as a key to understanding the processes of formation and evolution of other planetary systems and therefore the Solar System as well.

According to Evgenij Zubko, the value of the Umov effect for the science in general is as high as the importance of the spectral analysis method developed by Gustav Kirchhoff. While the spectral analysis helps us understand the chemical composition of distant bodies based on the light reflected from them, the Umov effect allows to evaluate their size even if they appear like a point to an observer.

School of Natural Sciences, Far Eastern Federal University

Space Science Institute, USA

Finnish Geospatial Research Institute, Geodeetinrinne 2, FI-02430 Masala, Finland

Institute of Astronomy, V.N. Karazin Kharkov National University, 35 Sumskaya Street, Kharkov UA-61022, Ukraine

 

 

Alexander Zverev