La lumière proche infrarouge révèle de grandes constellations d’étoiles constituantes, dont beaucoup sont encore entourées de poussière

Hubble Space Telescope in 1995 and followed up in 2014, and many other telescopes have deeply gazed at this scene. However, this is the first time an observatory has delivered such detailed data in near-infrared light. Newly formed stars pop out in shades of pink, red, and crimson. Still-forming stars that remain hidden deep in dusty pillars resemble molten lava, and fully-formed blue and yellow stars sprinkle the scene.

Where are the galaxies that often “photobomb” Webb’s images? The pillars are located directly in front of our Milky Way galaxy’s disk, which blocks our view of the galaxies that lie behind it. It is also lit up by the collective light from the packed “party” of stars. With these new data, researchers will be able to update complex models of star formation with even more precise star counts and dust quantities. It is clear that we are about to learn a whole lot more about how stars form.

NASA’s Webb Takes Star-Filled Portrait of Pillars of Creation

In exquisite detail, NASA’s James Webb Space Telescope has captured a lush, intricate landscape – the iconic Pillars of Creation. This is a region where new stars are forming within dense clouds of gas and dust. The three-dimensional pillars resemble majestic rock formations, but are far more permeable. These columns are made up of cool interstellar gas and dust that appear – at times – semi-transparent in near-infrared light.

Webb’s new view of the Pillars of Creation, which were first made famous when imaged by NASA’s Hubble Space Telescope in 1995, will help astronomers revamp their models of star formation by identifying far more precise counts of newly formed stars, along with the quantities of gas and dust in the region. Over time, they will begin to build a clearer understanding of how stars form and burst out of these dusty clouds over millions of years.

NASA’s Hubble Space Telescope made the Pillars of Creation famous with its first image in 1995, but revisited the scene in 2014 to reveal a sharper, wider view in visible light, shown above at left. A new, near-infrared-light view from NASA’s James Webb Space Telescope, at right, helps us peer through more of the dust in this star-forming region. The thick, dusty brown pillars are no longer as opaque and many more red stars that are still forming come into view. Credit: NASA, ESA, CSA, STScI; Joseph DePasquale (STScI), Anton M. Koekemoer (STScI), Alyssa Pagan (STScI).

Newly formed stars are the scene-stealers in this stunning image from Webb’s Near-Infrared Camera (NIRCam). These are the bright red orbs that typically have diffraction spikes and lie outside one of the dusty pillars. When knots with sufficient mass form within the pillars of gas and dust, they begin to collapse under their own gravity, slowly heat up, and eventually form new stars.

What about those wavy lines that look like lava at the edges of some pillars? These are ejections from stars that are still forming within the gas and dust. Young stars periodically shoot out supersonic jets that collide with clouds of material, like these thick pillars. This sometimes also results in bow shocks, which can form wavy patterns like a boat does as it moves through water. The crimson glow comes from the energetic hydrogen molecules that result from jets and shocks. This is evident in the second and third pillars from the top – the NIRCam image is practically pulsing with their activity. These young stars are estimated to be only a few hundred thousand years old.

Faites une visite vidéo de l’image proche infrarouge de Webb des piliers de la création. Crédits : NASA, ESA, ASC, STScI ; Joseph DePasquale (STScI), Anton M. Coquemore (STScI), Alyssa Pagan (STScI); Daniel Kirchenblatt (STScI).

Bien qu’il semble que la lumière proche infrarouge ait permis au Webb de « pénétrer » les nuages ​​pour révéler de grandes distances cosmiques derrière les panaches, il n’y a pas de galaxies dans cette vue. Au lieu de cela, un mélange de gaz transparents et de poussière connu sous le nom de milieu interstellaire dans la partie la plus dense du disque de notre Voie lactée obscurcit notre vision de l’univers intérieur. (Le milieu interstellaire est le gaz et la poussière dispersés entre les étoiles de la galaxie. Il se compose principalement d’atomes d’hydrogène, de molécules et de particules solides.)

Cette scène a d’abord été filmée par Hubble en 1995 Et le Révisé en 2014, mais de nombreux autres observatoires regardaient profondément dans cette zone. Chaque outil avancé fournit aux chercheurs de nouveaux détails sur cette région qui grouille pratiquement d’étoiles.

Cette image recadrée est bien placée dans la vaste nébuleuse de l’Aigle, qui se trouve à 6 500 années-lumière.

Le Télescope spatial James Webb Est-ce que tu Le télescope spatial le plus puissant jamais construit et le Le premier observatoire des sciences spatiales au monde. Ce sera Résolvez les énigmes Dans notre système solaire, regardez au-delà Des mondes lointains autour d’autres étoilesexplorez des structures mystérieuses et L’origine de notre univers Et où nous sommes. Webb est un programme international dirigé par Nasa avec ses partenaires, ESA (Agence spatiale européenne) et ASC (Agence spatiale canadienne).