Telescopio espacial James Webb revela Arp 220

Captada por el Telescopio Espacial James Webb, Arp 220, una galaxia compacta infrarroja ultraluminosa, muestra la luminosidad de un billón de soles, formación estelar masiva y clara evidencia de una danza galáctica en curso. Crédito: NASA, ESA, CSA, STScI, procesamiento de imágenes: Alyssa Pagan (STScI)

Una impresionante vista del nacimiento de una estrella capturada en infrarrojo

Un impresionante choque de dos galaxias espirales brilla en el infrarrojo con la luz de más de un billón de soles. Apodado Arp 220, las galaxias en colisión encendieron una explosión masiva de nacimiento de estrellas. Cada uno de los CGN está rodeado por un anillo giratorio de formación estelar que emite una luz brillante que Webb capturó en el infrarrojo. Esta luz brillante crea un estallido estelar prominente y puntiagudo.

El telescopio espacial James Webb capturó esta impresionante imagen de Arp 220, una galaxia infrarroja ultraluminosa (ULIRG) formada a partir de la fusión de dos galaxias espirales. Ubicado a 250 millones de años luz de distancia en la constelación Serpens, tiene una luminosidad superior a un billón de soles, en comparación con los 10 mil millones de la Vía Láctea. La colisión condujo a la formación de estrellas masivas, con alrededor de 200 cúmulos de estrellas masivas en una región compacta y polvorienta que contenía gas equivalente a toda la Vía Láctea. El telescopio reveló los núcleos de las galaxias madre, cada uno con un anillo giratorio de formación de estrellas responsable de golpear la luz infrarroja. La imagen también muestra tenues colas de marea y materia orgánica como evidencia de fusiones galácticas en curso. Crédito: NASA, ESA, CSA, STScI, procesamiento de imágenes: Alyssa Pagan (STScI)

El Telescopio Espacial Webb captura la increíble fusión de galaxias, Arp 220

Un faro brillante en medio de un mar de galaxias, Arp 220 brilla en el cielo nocturno en esta vista desde[{» attribute=»»>NASA’s James Webb Space Telescope. Actually, two spiral galaxies in the process of merging, Arp 220 glows brightest in infrared light, making it an ideal target for Webb. It is an ultra-luminous infrared galaxy (ULIRG) with a luminosity of more than a trillion suns. In comparison, our Milky Way galaxy has a much more modest luminosity of about ten billion suns.

Located 250 million light-years away in the constellation of Serpens, the Serpent, Arp 220 is the 220th object in Halton Arp’s Atlas of Peculiar Galaxies. It is the nearest ULIRG and the brightest of the three galactic mergers closest to Earth.

The collision of the two spiral galaxies began about 700 million years ago. It sparked an enormous burst of star formation. About 200 huge star clusters reside in a packed, dusty region about 5,000 light-years across (about 5 percent of the Milky Way’s diameter). The amount of gas in this tiny region is equal to all of the gas in the entire Milky Way galaxy. 

Image of Arp 220 captured by Webb’s Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI), with compass arrows, scale bar, and color key for reference.
The north and east compass arrows show the orientation of the image on the sky. Note that the relationship between north and east on the sky (as seen from below) is flipped relative to direction arrows on a map of the ground (as seen from above).
The scale bar is labeled in light-years, which is the distance that light travels in one Earth-year. (It takes 18,000 years for light to travel a distance equal to the length of the bar.) One light-year is equal to about 5.88 trillion miles or 9.46 trillion kilometers. The field of view shown in this image is approximately 120,000 light-years across.
This image shows invisible infrared wavelengths of light that have been translated into visible-light colors. The color key shows which filters were used when collecting the light. The color of each filter name is the visible-light color used to represent the infrared light that passes through that filter.
Credit: NASA, ESA, CSA, STScI, Image Processing: Alyssa Pagan (STScI)

Previous radio telescope observations revealed about 100 supernova remnants in an area of less than 500 light-years. NASA’s Hubble Space Telescope uncovered the cores of the parent galaxies 1,200 light-years apart. Each of the cores has a rotating, star-forming ring blasting out the dazzling infrared light so apparent in this Webb view. This glaring light creates diffraction spikes — the starburst feature that dominates this image. 

On the outskirts of this merger, Webb reveals faint tidal tails, or material drawn off the galaxies by gravity, represented in blue — evidence of the galactic dance that is occurring. Organic material represented in reddish-orange appears in streams and filaments across Arp 220.

Webb viewed Arp 220 with its Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI).

The James Webb Space Telescope is the world’s leading space science observatory is the James Webb Space Telescope, and was designed to unravel the mysteries of our solar system and explore distant worlds around other stars. Moreover, it aims to investigate the enigmatic structures and origins of our universe, and our position within it. This international program is spearheaded by NASA in collaboration with its partners, namely, the European Space Agency (ESA) and the Canadian Space Agency.