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  • NASA adds Chandra information to Webb observations, unveils spectacular new photos
  • NASA unveils spectacular new photos combining information from various telescopes. See the breathtaking benefits of this cosmic collaboration

    This image of the Eagle Nebula was produced employing information from various telescpoes. (Image credit: NASA)Listen to this short article
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    NASA on Tuesday released 4 photos that combine information from the space agency’s Chandra X-ray Observatory and the James Webb Space Telescope. Every image combines the infrared information from previously released Webb photos with X-ray information from Chandra.

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    Each the higher power X-ray light and low-power infrared light are invisible to the naked eye but when they are translated into visible light, it benefits in some spectacular photos. The space agency says it also utilized optical light information from the Hubble telescope, infrared light from the Spitzer Space Telescope, optical information from the European Southern Observator’s New Technologies Telescope and X-ray information from the European Space Agency’s XMM-Newton telescope.

    Verify out the spectacular benefits from this mixture of information under.

    A composite image of the Eagle Nebula. (Image credit: NASA)

    Eagle Nebula or Messier 16 (M16)

    Messier 16, or the Eagle Nebula, is the popular area of the sky that is also referred to as the Pillars of Creation in NASA’s initially photos from the Webb telescope. In the new image, the dark columns of gas shrouding the young stars are displayed from Webb information. The light detected by Chandra, which appears like dots, are these young stars providing off X-ray light.

    Composite image of Messier 74. (Image credit: NASA)

    M74, the Phantom Galaxy

    Messier 74 or M74 is a spiral galaxy just like our Milky Way. It is nicknamed the Phantom Galaxy simply because it is pretty dim, creating it extra tricky to observe compared to other galaxies in Charles Messier’s popular catalogue.

    The Webb information outlines gas and dust in infrared though Chandra’s X-ray information shows higher-power activity from stars. Along with this, Hubble optical information displays further stars and dust along dust lanes.

    Composite image of NGC 346. (Image credit: NASA)

    NGC 346

    NGC 346 is a star cluster in the Tiny Magellanic Cloud, which is a galaxy about 200,000 light-years away from our planet. The plumes and arcs of gas and dust that type stars and planets are observed in the Webb information. The young, hot and huge stars that send out strong stellar winds shaping the gas and dust are visible from the Chandra information. This image also contains further information from the Hubble and Spitzer telescopes, along with supporting information from XMM-Newton and the New Technologies Telescope.

    Composite image of NGC 1672. (Image credit:

    NGC 1672

    NGC 1672 is a different spiral galaxy but astronomers categorise it as a barred spiral. In the regions close to their centres, the arms of barred spiral galaxies are visible as straight bars of stars that enclose the cores. Run-of-the-mill spiral galaxies have arms that twist all the way to the core.

    Information from Chandra reveals compact objects like neutron stars or black holes pulling in material from companion stars and also, the remnants of exploded stars. Researchers utilized optical information from Hubble to fill out the spiral arms with gas and dust though Webb information was utilized to show gas and dust in NGC 1672’s spiral arms.

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    Very first published on: 27-05-2023 at ten:19 IST

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