Depict the knowledge that volcanoes in Venus have been active: the new 3D proportional model records that Venus is agitated indoors

A new studio identifies 37 volcanic structures relatively active in Venus. The study of the proportions of the best interests is that now that Venus is a geologically active planet. An investigation work on the work carried out by investigators from the University of Maryland and the ETH Institute of Geophysics of Zurich, Switzerland, published in the journal Geography of nature July 20, 2020

“It is the first time that we can design specific structures and decide on Mira, it is not an ancient volcano that is one that is active, but inactive, but not dead,” says Laurent Montési, professor of degeology at UMD and co-author of the UMD. investigation work. “This study changed significantly the vision of Venus from a planet in its inactivity to a single interior, which is agitated and can be eaten by many active volcanoes.”

The scientific questions from here are always the time that Venus has an area that has the planets like Mars and Mercury, which shade the interiors of the fries. The evidence of a cold interior and geological activity spans the surface of the planet in the form of structures in the form of a colonized colonized anchovy, which is created when the columns of material in the interior of the planet rise above the cross and the cross section of the manto. It is similar to the form in which the plumas del manto formaron las islas volcánicas de Hawaii.

Pero thought that the coronas in Venus probably had signs of antigenic activity, and that Venus would normally suffer as sufficient to develop geological activity in the interior of the planet and endorse the cortse that would cure the material of the fund in no way. . Users who processed exact texts from Los Cuales the plumas del manto formaron coronas en Venus y las razones para la variación entre coronas han sido temas de debata.

In the new studio, investigators use numerical models of thermomechanical activity to discuss the surface area of ​​Venus to create 3D simulations of another resolution of the crown formation. See more information on the details of the process processed from ammunition.

The results of the loss of ayudaron in Montési y sus colegas to identify the characteristics that are presented solo in the coronas activas recientemente. The equipment can therefore be associated with observations in the area of ​​Venus, revealing that part of the variation in the coronas in this planet represents different stages of geological development. The study is proportionate to the first evidence that the crowns in Venus are evolving, indicating that the interior of the planet is agitated.

“The degree of improvement in reality in these models with Respect to the Studies allowed to identify various stages in the evolution of the corona and to define the geological characteristics of the diagnostic present only in the crowns currently active”, says Montési. “We can decide that less than 37 crowns are very active”

The active crowns in Venus are aggregated into a place of location, where suggesting areas around the planet are more active, proportionating pistons to the functioning of the interior of the planet. These results can help to identify the objective objectives of geological instruments that must be included in the future futures of Venus, as EnVision of Europe, which will be available in 2032.

Source history:

Materials proportional por University of Maryland . Note: The content can be edited by style and length.

Source link