An international team of researchers has found that the red supergiant star Antares is even more gigantic than initially thought, reports.

Previous research found that Antares, which is located about 550 light-years away in the Scorpius constellation, is about 700 times larger than the Sun — but that number increases dramatically when mapped in a different spectrum.

"The size of a star can vary dramatically depending on what wavelength of light it is observed with," Eamon O’Gorman, astronomer at the Dublin Institute for Advanced Studies and lead author of a new study about the project published in the journal Astronomy & Astrophysics this week, said in a statement.

"The longer wavelengths of the [Very Large Array] revealed the supergiant’s atmosphere out to nearly 12 times the star’s radius," O'Gorman added.

The team used the latest readings from both the Very Large Array combined with the Atacama Large Millimeter/submillimeter Array to study Antares' atmosphere — and, in the process assembled the most detailed map in existence of any star besides our Sun.

Supergiant red stars are the largest stars found in the universe in terms of volume, but not mass. They're relatively cool and form from stars that start to collapse in on themselves. Once their time is up, they collapse into a supernova.

The region just above red supergiant's surface, the chromosphere, is cooler than the Sun's. Its chromosphere is also far more extensive, stretching to 2.5 times that of its radius, compared to the Sun's chromosphere, which extends to only 0.5 percent of its radius.

“We found that the chromosphere is ‘lukewarm’ rather than hot, in stellar temperatures,” O’Gorman explained. "The difference can be explained because our radio measurements are a sensitive thermometer for most of the gas and plasma in the star’s atmosphere, whereas past optical and ultraviolet observations were only sensitive to very hot gas and plasma."

By scrutinizing the star's chromosphere, they could even tell where winds on its surface start from.

"Knowing the actual sizes and temperatures of the atmospheric zones gives us a clue of how these huge winds start to form and how much mass is being ejected," co-author Graham Harper of the University of Colorado said in the statement.

READ MORE: New map reveals just how enormous the supergiant star Antares really is []

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