


The most famous of these is the Trapezium Cluster, a group of several hundred young stars that are just a few million years old and are surrounded by a bright, glowing cloud of gas.The Trapezium Cluster also has a radius that measures 10 light-years.


The Carina Nebula is also a source of many interesting objects, including planetary nebulae, supernova remnants, and young stellar clusters. The intense radiation and strong winds from these massive stars have shaped the nebula’s appearance, carving out huge cavities and sculpting intricate patterns of gas and dust. The Carina Nebula is home to some of the most massive and luminous stars in the galaxy, including Eta Carinae, which is one of the most luminous stars known and has a mass that is estimated to be around 100 times that of the Sun. The Carina Nebula harbors some of the brightest stars in the Milky Way The nebula is also one of the largest and most active star-forming regions in our Milky Way galaxy, with a size that is roughly four times that of the Orion Nebula. It has a radius that reaches 230 light-years. The Carina Nebula is also huge, as you’ve probably already guessed. We now have the possibility to admire the so-called “cosmic cliffs” of the nebula in 4K footage, meaning “a region at the edge of a gigantic, gaseous cavity within the star cluster NGC 3324,” as NASA/ESA reveals. One of the images shows the Carina Nebula in all its glory, meaning a beautiful cosmic structure that’s placed 7,500 light-years away from Earth. Webb, who served as the second administrator of NASA from 1961 to 1968 and played a key role in the Apollo program.īack in July, the JWST revealed the first full-color images of the Universe during an event that was awaited by the entire community of astronomers. It is a joint project of NASA, the European Space Agency (ESA), and the Canadian Space Agency (CSA). The James Webb Space Telescope is a state-of-the-art space telescope designed to observe the most distant objects in the Universe, as well as provide images and spectra of objects in our own solar system.
