Mysterious icy items have been identified for thousands of light years, with astronomers uncertain about their nature. The discovery was made through observations for many years, with initial detection associated with the data collected between 2006 and 2011. Recent results have deepened the mystery, researchers have noted that these items are not in line with well -known heavenly institutions. These structures appear to contain ice and gas, which are located in the outer region of the Akashganga, where the formation of the star is unusual. Their sizes, compounds and locations have raised questions about their originality and rating.

Observations and consequences

According to Study Along with Atsaki Sakin and Takashi Onaa from Nigata University, published at the University of Tokyo on Takshi Smundi, Aki Space Telescope and Alma Surrey data were analyzed in Chile. Both items were first recorded in infrared data, which was later followed by follow -up observations using Alma. Despite the additional results, their correct nature is not.

As if Reported Through the Phys.com, both items are estimated 10 times higher than the size of the solar system, which is considered as extraordinarily small for gas clouds. Infrared analysis depicts samples of absorption that are compatible with young strings or background stars that are vague with dense clouds. However, their position is far from the ordinary star maker regions.

To the dishonesty of distance and structure

Contradictory distance measurements have increased uncertainty. One data source keeps an item away from 6,500 light years, while the other recommends a distance of 30,000 light years. The second item is permanently measured at a distance of 43,700 light years. There are complex efforts to classify them in these contradictions.

The gas around the two structures has been identified primarily as silicon dioxide, which contains marks of carbon dioxide. This proportion is resembling young stars, but no final conclusion has been drawn. Researchers estimate that future observations using the James Webpace telescopes can provide more explanation on their formation and inception.