Brown Dwarfs

This article was published in the Science Daily on December 23. This is two brown dwarfs discovered by scientists Alex Wolszczan, Evan Pugh, and Penn State. A brown dwarf is an object in the space between a star and a planet. In the early stages of Dwarf life, it is difficult to distinguish this goal from low quality stars. They start with the usual stars, so they are often called stars that failed. However, at some stage, they simply do not have enough mass to produce the fusion energy of the stars.

Scholz's Star is actually a low-quality binary system consisting of a red dwarf and a brown dwarf. The red dwarf is the most common type of star in the universe, but the brown dwarf is lower than that. They are sometimes called "failed stars" because they do not have enough mass to fuse hydrogen and become a "real star". As they may incorporate other elements, you can think of them as a very big and warm Jupiter. When a team of astronomers computed their course, we for the first time hinted at the star of Scholz living in the solar system in 2015. A pair of two objects moves quickly through the universe and analyzes the path projected through the edge of the solar system.

The team of astronomers led by UC Santa Cruz has published a report on the brown dwarf WISE 0 855, which is the darkest object ever imaged within its spectral range. Their results confirm the existing hypothesis that brown dwarfs should be able to support enough water to create water - cloudlike phenomena. The frustration about external embryology (except for strangers who convince you that you really have a job) is a tug of war between visibility and fever. The most obvious thing when looking for a planet is a star - they have no life. The next obvious thing is usually a gas giant, which is also considered to be unlikely to contain life. After that, things are basically decomposed by heat and light. The brighter the object is, the easier it is to see the earth, the warmer it will rise, the warnings that water will feel unpleasant are some.