• 15 Նոյեմբերի, 2024
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ՆԱՍԱ-ն հրապարակել է պարուրաձև գալակտիկաների լուսանկարները

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ԱՄՆ-ի ազգային ավիատիեզերական գործակալությունը (ՆԱՍԱ) հրապարակել է գալակտիկաների լուսանկարներ, որոնք ստացվել են գերհզոր «Ջեյմս Ուեբ» տիեզերական աստղադիտակի միջոցով։

Ըստ ՆԱՍԱ-ի կայքի՝ գիտնականները, որոնք աշխատում են Physics at High Resolution in Nearby Galaxies (PHANGS) ծրագրի շրջանակում, լուսանկարել են 19 պարուրաձև գալակտիկա:Դրանցից ամենամոտը մեզնից 15 միլիոն լուսային տարի հեռավորության վրա է, ամենահեռավորը՝ 60:

Galaxy IC 5332 was observed as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, a large project that includes observations from several space- and ground-based telescopes of many galaxies to help researchers study all phases of the star formation cycle, from the formation of stars within dusty gas clouds to the energy released in the process that creates the intricate structures revealed by Webb’s new images. IC 5332 is 30 million light-years away in the constellation Sculptor. Learn more about what can be seen in this vast collection of Webb images here. [Image description: Webb’s image of IC 5332 shows a densely populated face-on spiral galaxy anchored by a central region that has a light blue haze. Spine-like spiral orange arms extend to the edges and rotate clockwise.]
Galaxy IC 5332 was observed as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, a large project that includes observations from several space- and ground-based telescopes of many galaxies to help researchers study all phases of the star formation cycle, from the formation of stars within dusty gas clouds to the energy released in the process that creates the intricate structures revealed by Webb’s new images. IC 5332 is 30 million light-years away in the constellation Sculptor. Learn more about what can be seen in this vast collection of Webb images here. [Image description: Webb’s image of IC 5332 shows a densely populated face-on spiral galaxy anchored by a central region that has a light blue haze. Spine-like spiral orange arms extend to the edges and rotate clockwise.]
This spiral galaxy was observed as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, a large project that includes observations from several space- and ground-based telescopes of many galaxies to help researchers study all phases of the star formation cycle, from the formation of stars within dusty gas clouds to the energy released in the process that creates the intricate structures revealed by Webb’s new images. NGC 628 is 32 million light-years away in the constellation Pisces. Learn more about what can be seen in this vast collection of Webb images here. [Image description: Webb’s image of NGC 628 shows a densely populated face-on spiral galaxy anchored by a central region that has a light blue haze. Spine-like f spiral orange arms extend to the edges and rotate counterclockwise.]
This spiral galaxy was observed as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, a large project that includes observations from several space- and ground-based telescopes of many galaxies to help researchers study all phases of the star formation cycle, from the formation of stars within dusty gas clouds to the energy released in the process that creates the intricate structures revealed by Webb’s new images. NGC 1087 is 80 million light-years away in the constellation Cetus. Learn more about what can be seen in this vast collection of Webb images here. [Image description: Webb’s image of NGC 1087 shows a densely populated face-on spiral galaxy anchored by a central region that takes the shape of a short line. Its filamentary orange spiral arms appear muddled together and it is difficult to pick out individual spiral arms. The arms extend to the edges and rotate clockwise.]
This spiral galaxy was observed as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, a large project that includes observations from several space- and ground-based telescopes of many galaxies to help researchers study all phases of the star formation cycle, from the formation of stars within dusty gas clouds to the energy released in the process that creates the intricate structures revealed by Webb’s new images. NGC 1385 is 30 million light-years away in the constellation Fornax. Learn more about what can be seen in this vast collection of Webb images here. [Image description: Webb’s image of NGC 1385 shows a messy face-on spiral galaxy with filamentary structures in shades of white, yellow, orange, and red. At the centre are some light blue regions.]
This spiral galaxy was observed as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, a large project that includes observations from several space- and ground-based telescopes of many galaxies to help researchers study all phases of the star formation cycle, from the formation of stars within dusty gas clouds to the energy released in the process that creates the intricate structures revealed by Webb’s new images. NGC 1512 is 30 million light-years away in the constellation Horologium. Learn more about what can be seen in this vast collection of Webb images here. [Image description: Webb’s image of NGC 1512 shows a face-on barred spiral galaxy anchored by its central region, which is circular and shows a bright white point at the center with blue and yellow circles around it. The galaxy’s large bar is crossed by filamentary dust lanes that extend diagonally to the top left and bottom right. The bar is connected to a dense oval-shaped ring of orange spiral arms that start at the edges of the bar.]
This spiral galaxy was observed as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, a large project that includes observations from several space- and ground-based telescopes of many galaxies to help researchers study all phases of the star formation cycle, from the formation of stars within dusty gas clouds to the energy released in the process that creates the intricate structures revealed by Webb’s new images. NGC 4254 is 50 million light-years away in the constellation Coma Berenices. Learn more about what can be seen in this vast collection of Webb images here. [Image description: Webb’s image of NGC 4254 shows a densely populated face-on spiral galaxy anchored by its central region, which is right of centre. Spiral orange arms sweep out to the edges and rotate counterclockwise.]
This spiral galaxy was observed as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, a large project that includes observations from several space- and ground-based telescopes of many galaxies to help researchers study all phases of the star formation cycle, from the formation of stars within dusty gas clouds to the energy released in the process that creates the intricate structures revealed by Webb’s new images. NGC 7496 is 24 million light-years away in the constellation Grus. Learn more about what can be seen in this vast collection of Webb images here. [Image description: The central core of Webb’s image of the galaxy NGC 7496 begins as a bright white dot that melts into bright oranges. Eight prominent diffraction spikes emanate from the centre. A bright orange arc that looks like a thin, backward S forms the bar and two of the face-on spiral galaxy’s arms.]
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ԼՐԱՀՈՍ

Տնտեսական լուրեր 14.11.2024

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