Nearly two years have passed since the momentous launch of the James Webb Space Telescope, a remarkable instrument that has the remarkable ability to capture images of the cosmos with unparalleled clarity. This innovative technology is invaluable to scientists and astronomers, providing invaluable data. Distinguishing itself from conventional ground-based telescopes, the Webb telescope transcends the limitations imposed by Earth's gravitational pull, magnetic field, and atmosphere. Furthermore, unlike its predecessor, the Hubble telescope, Webb does not orbit our planet. Instead, it maintains a stable position 1,5 million kilometers away, between the Earth and the Sun.
What the James Webb Space Telescope has managed to capture
In Baltimore, images taken by the James Webb Space Telescope are processed to remove any factors that might hinder scientific objectives. To make these images attractive and easily understandable to the general public, a small amount of color enhancement, approximately 5%, is applied. In addition, in recent months, Webb has allowed scientists to unravel the mysteries of ancient black holes and better understand galaxy formation in the early stages of the universe, as explained in the article on .
As an example, The ghost galaxy, also known as M74, is photographed in monochrome using four different filters on the Webb Telescope's MIRI instrument. Upon arrival at the operations center in Baltimore, these images undergo meticulous processing to remove any imperfections or artifacts caused by the instrument, resulting in pristine images that scientists can directly use in their research.
For some time now, scientists have been aware of the existence of smaller black holes in the early stages of the universe; However, it was only through Webb's observations that they were finally able to definitively detect them.
By capturing spectra of celestial objects such as planets, stars and galaxies, the telescope enables a comprehensive understanding of their composition. The Webb spectrograph plays a crucial role in this process by separating infrared light into various components., thus revealing a spectrum that reveals the existence of various chemical elements and molecules. What is the telescope for? and how it helps in the exploration of the cosmos.
Using spectral analysis, astronomers successfully identified the presence of sulfur dioxide, sodium, potassium, water vapor, carbon dioxide and carbon monoxide on the exoplanet WASP-39 b. This technique also allows us to observe celestial objects obscured by dust and gas, thus significantly expanding our view of the cosmos.
Black hole depths
NASA's publication of the image of the galaxy CEERS 1019 and its supermassive black hole, captured by the James Webb Telescope on July 6, 2023, has attracted significant attention from the scientific and astronomical community. This remarkable image reveals the most remote active supermassive black hole ever identified, located within a galaxy that was born just over 570 million years after the Big Bang. What sets this black hole apart is its relatively modest mass, weighing in at around nine million solar masses, which is considerably smaller compared to most supermassive black holes in the early universe, which typically number over a billion. times the mass of our Sun.
The presence of a black hole in CEERS 1019, despite its relatively smaller size, has sparked investigations into its formation during the early stages of the universe. Scientists were aware of the likelihood that smaller black holes existed in the early cosmos, but it was not until observations by Webb that they were able to conclusively confirm their existence.
After a full year of traversing the vast expanse of space, the NASA, ESA, and CSA collaborative effort known as the James Webb Space Telescope continues to amaze us with its stunning images. It recently revealed two stunning photographs showcasing the immense beauty of NGC 604, a magnificent galaxy filled with approximately 200 celestial bodies. These captivating images offer a glimpse into the intricate details of this stellar phenomenon, leaving us in awe.
Image by NIRCam
NGC 604, a galaxy that is about half the size of our Milky Way, is captured in two new images taken by NIRCam (Near Infrared Camera) and MIRI (Middle Infrared Instrument). These images reveal an intricate and complete depiction of the star formation process, showing expanding gas-filled bubbles and spreading filaments. The level of detail surpasses previous observations and presents a vivid tapestry of the celestial birth.
The image captured by the near-infrared camera provides confirmation of the existence of two young stars located above the central nebula. In addition, vibrant red bubble-shaped structures are observed within the nebula, which NASA attributes to the influence of the winds generated by the most intense and luminous stars in NGC 604. The image also reveals striking orange streaks, which indicate the presence of carbon-based compounds called polycyclic aromatic hydrocarbons (PAHs). These substances are important components of the interstellar medium and play a crucial role in the formation of celestial bodies, although their origin remains enigmatic. Furthermore, the image shows the remarkable ability of the two young, radiant stars to excavate openings in the dust above the central nebula.
MIRI image
The MIRI image shows a notable reduction in the number of stars, particularly supergiants, which are a million and a hundred times brighter and larger than our Sun, respectively. This decrease can be attributed to the fact that these hot stars emit significantly less light in the wavelengths captured by MIRI. Furthermore, in these observations, The Webb telescope has explored the atmosphere of Uranus and how this influences the formation of new stars in NGC 604. The presence of cooler clumps of gas and dust radiate a luminous glow, and the same star formation process is detected in these areas as in other regions of the universe.
NASA has identified distinct blue formations that resemble tendrils, indicating the probable existence of polycyclic aromatic hydrocarbons. As we mentioned earlier, these hydrocarbons are crucial in the formation of celestial bodies such as planets and stars. NGC 604, whose age is estimated at about 3,5 million years, features a luminous cloud of gas that extends an impressive diameter of 1.300 light years.
