A telescope in Chile captured an unbelievable 'butterfly' 2,500 light years away.

A telescope in Chile captured an unbelievable 'butterfly' 2,500 light years away.
A "butterfly" in deep space: the latest photo from Gemini South
porEditorial Team
Argentina

The Gemini South Telescope celebrated its 25th anniversary with a detailed image of the Butterfly Nebula, located 2,500 light-years away

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The Gemini South Telescope, located in Chile, captured one of the most striking images of deep space. The well-known Butterfly Nebula (NGC 6302 or Caldwell 69), a bipolar astronomical object located between 2,500 and 3,800 light-years away in the constellation of Scorpius. The photograph was released by the International Gemini Observatory.

The image was selected to celebrate the 25th anniversary of the telescope. The image stands out for the precision with which it shows the turbulent flows of gas surrounding its central star.

El Telescopio Gemini Sur obtuvo una de las imágenes más llamativas del espacio profundo
El Telescopio Gemini Sur obtuvo una de las imágenes más llamativas del espacio profundo

A "butterfly" formed by the violent death of a star

The image displays the complexity of NGC 6302, whose shape resembles the open wings of a butterfly. This appearance is the result of a violent process that occurs when a massive star approaches the end of its life cycle.

At the center of this nebula is a white dwarf, the ultra-dense remnant of a star similar to the Sun. It has approximately two-thirds of its mass and is one of the hottest stars known, with a surface temperature exceeding 250,000 °C (482,000 °F).

From red giant to blazing remnant

Before becoming a white dwarf, it went through the red giant phase, expanding to a diameter a thousand times greater than that of the Sun. During that period, it expelled layers of gas and dust, forming a "barrier" that would determine the final shape of the nebula.

Una “mariposa” formada por la muerte violenta de una estrella
Una “mariposa” formada por la muerte violenta de una estrella

That residual material caused a dense belt that later channeled the gas ejections in perpendicular directions, giving rise to the bipolar morphology now recorded by the telescope.

The solar wind as a cosmic sculptor

The solar wind collided with the pre-existing dust and gas, shaping the "wings" of this cosmic butterfly. The chromatic analysis from Gemini South makes it possible to distinguish key components: red reveals energized hydrogen and blue indicates highly excited oxygen.

 


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