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|    Message 7,819 of 8,931    |
|    ScienceDaily to All    |
|    Webb Telescope captures rarely seen prel    |
|    14 Mar 23 22:30:30    |
      MSGID: 1:317/3 641149eb       PID: hpt/lnx 1.9.0-cur 2019-01-08       TID: hpt/lnx 1.9.0-cur 2019-01-08        Webb Telescope captures rarely seen prelude to supernova                Date:        March 14, 2023        Source:        NASA/Goddard Space Flight Center        Summary:        The rare sight of a Wolf-Rayet star -- among the most luminous,        most massive, and most briefly detectable stars known -- was one of        the first observations made by NASA's James Webb Space Telescope in        June 2022. Webb shows the star, WR 124, in unprecedented detail with        its powerful infrared instruments. The star is 15,000 light-years        away in the constellation Sagittarius.                      Facebook Twitter Pinterest LinkedIN Email       FULL STORY       ==========================================================================       The rare sight of a Wolf-Rayet star -- among the most luminous, most       massive, and most briefly detectable stars known -- was one of the       first observations made by NASA's James Webb Space Telescope in June       2022. Webb shows the star, WR 124, in unprecedented detail with its       powerful infrared instruments. The star is 15,000 light-years away in       the constellation Sagittarius.                     ==========================================================================       Massive stars race through their lifecycles, and only some of       them go through a brief Wolf-Rayet phase before going supernova,       making Webb's detailed observations of this rare phase valuable to       astronomers. Wolf-Rayet stars are in the process of casting off their       outer layers, resulting in their characteristic halos of gas and dust. The       star WR 124 is 30 times the mass of the Sun and has shed 10 Suns' worth of       material -- so far. As the ejected gas moves away from the star and cools,       cosmic dust forms and glows in the infrared light detectable by Webb.              The origin of cosmic dust that can survive a supernova blast and       contribute to the universe's overall "dust budget" is of great interest       to astronomers for multiple reasons. Dust is integral to the workings       of the universe: It shelters forming stars, gathers together to help       form planets, and serves as a platform for molecules to form and clump       together -- including the building blocks of life on Earth. Despite       the many essential roles that dust plays, there is still more dust       in the universe than astronomers' current dust-formation theories can       explain. The universe is operating with a dust budget surplus.              Webb opens up new possibilities for studying details in cosmic dust, which       is best observed in infrared wavelengths of light. Webb's Near-Infrared       Camera (NIRCam) balances the brightness of WR 124's stellar core and       the knotty details in the fainter surrounding gas. The telescope's       Mid-Infrared Instrument (MIRI) reveals the clumpy structure of the gas and       dust nebula of the ejected material now surrounding the star. Before Webb,       dust-loving astronomers simply did not have enough detailed information       to explore questions of dust production in environments like WR 124,       and whether the dust grains were large and bountiful enough to survive       the supernova and become a significant contribution to the overall dust       budget. Now those questions can be investigated with real data.              Stars like WR 124 also serve as an analog to help astronomers understand       a crucial period in the early history of the universe. Similar dying stars       first seeded the young universe with heavy elements forged in their cores       -- elements that are now common in the current era, including on Earth.              Webb's detailed image of WR 124 preserves forever a brief, turbulent time       of transformation, and promises future discoveries that will reveal the       long- shrouded mysteries of cosmic dust.               * RELATED_TOPICS        o Space_&_Time        # Stars # Nebulae # Cosmology # Astronomy # NASA #        Galaxies # Big_Bang # Astrophysics        * RELATED_TERMS        o Blue_supergiant_star o Spitzer_space_telescope o Supernova o        Alpha_Centauri o Stellar_evolution o Star_cluster o Milky_Way        o Star_Trek              ==========================================================================       Story Source: Materials provided by       NASA/Goddard_Space_Flight_Center. Note: Content may be edited for style       and length.                     ==========================================================================       Related Multimedia:        * The_luminous,_hot_star_Wolf-Rayet_124_(WR_124)       ==========================================================================                     Link to news story:       https://www.sciencedaily.com/releases/2023/03/230314205347.htm              --- up 1 year, 2 weeks, 1 day, 10 hours, 50 minutes        * Origin: -=> Castle Rock BBS <=- Now Husky HPT Powered! (1:317/3)       SEEN-BY: 15/0 106/201 114/705 123/120 153/7715 226/30 227/114 229/110       SEEN-BY: 229/111 112 113 307 317 400 426 428 470 664 700 292/854 298/25       SEEN-BY: 305/3 317/3 320/219 396/45       PATH: 317/3 229/426           |
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