Hubble Seeks Clusters in Lost Galaxy

Hubble Seeks Clusters in Lost Galaxy

Handout Photo shows NASA/ESA Hubble Space Telescope image features the spiral galaxy NGC 4535, which is situated about 50 million light-years away in the constellation Virgo (the Maiden). Through a small telescope, this galaxy appears extremely faint, giving it the nickname ‘Lost Galaxy’. With a mirror spanning nearly eight feet (2.4 meters) across and its location above Earth’s light-obscuring atmosphere, Hubble can easily observe dim galaxies like NGC 4535 and pick out features like its massive spiral arms and central bar of stars. This image features NGC 4535’s young star clusters, which dot the galaxy’s spiral arms. Glowing-pink clouds surround many of these bright-blue star groupings. These clouds, called H II (‘H-two’) regions, are a sign that the galaxy is home to especially young, hot, and massive stars that blaze with high-energy radiation. Such massive stars shake up their surroundings by heating their birth clouds with powerful stellar winds, eventually exploding as supernovae. The image incorporat

  • Product Code
  • ILEA004955002
  • Registered date
  • 2025/12/04 00:00:00
  • Credit
  • Abaca Press / Kyodo News Images
  • Media source
  • ABACA
  • Media size
  • 4101 × 3902 pixel
  • Resolution
  • 1 dpi
  • Deployment size
  • 1.89(MB)*
  • Special instruction

*File size when opened in Photoshop, etc.

Similar Images & Videos
    Star Explosion Reveals New Space Ingredients

    Star Explosion Reveals New Space Ingredients

    Handout - Scientists have spotted chlorine and potassium hiding inside the remains of a blown-up star for the first time. Using Japan’s XRISM space telescope, they found these elements inside the giant cloud of debris left behind by the supernova called Cassiopeia A. The explosion happened about 11,000 light-years from Earth, but it is still giving up new secrets today. The find shows how stars don’t just light up the sky, they also make many of the elements that help build planets and life. Even long after a star explodes, it can still teach us something new about the universe. This discovery was published in a scientific paper on December 4 this year, and the image was released on January 28, 2024, using data from NASA’s Chandra telescope along with Hubble, Webb and Spitzer. Photo by Image credit: X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. Arcand via ABACAPRESS.COM
      Hubble Seeks Clusters in ‘Lost Galaxy’

      Hubble Seeks Clusters in ‘Lost Galaxy’

      NASA/ESA Hubble Space Telescope image features the spiral galaxy NGC 4535, which is situated about 50 million light-years away in the constellation Virgo (the Maiden). Through a small telescope, this galaxy appears extremely faint, giving it the nickname ‘Lost Galaxy’. With a mirror spanning nearly eight feet (2.4 meters) across and its location above Earth’s light-obscuring atmosphere, Hubble can easily observe dim galaxies like NGC 4535 and pick out features like its massive spiral arms and central bar of stars. This image features NGC 4535’s young star clusters, which dot the galaxy’s spiral arms. Glowing-pink clouds surround many of these bright-blue star groupings. These clouds, called H II (‘H-two’) regions, are a sign that the galaxy is home to especially young, hot, and massive stars that blaze with high-energy radiation. Such massive stars shake up their surroundings by heating their birth clouds with powerful stellar winds, eventually exploding as supernovae. The image incorporates data from an obse
        Red Spider Nebula

        Red Spider Nebula

        Handout photo dated on October 26, 2025 shows Red Spider Nebula. Using its Near-InfraRed Camera (NIRCam), NASA’s James Webb Space Telescope captured never-before-seen details of the Red Spider Nebula, a planetary nebula, in this image released on Oct. 26, 2025. NIRCam is Webb’s primary near-infrared imager, providing high-resolution imaging and spectroscopy for a wide variety of investigations. Webb’s new view of the Red Spider Nebula reveals for the first time the full extent of the nebula’s outstretched lobes, which form the ‘legs’ of the spider. These lobes, shown in blue, are traced by light emitted from H2 molecules, which contain two hydrogen atoms bonded together. Stretching over the entirety of NIRCam’s field of view, these lobes are shown to be closed, bubble-like structures that each extend about 3 light-years. Outflowing gas from the center of the nebula has inflated these massive bubbles over thousands of years. Photo by ESA/Webb, NASA & CSA, J. H. Kastner (Rochester Institute of Technolo via ABAC
          Webb Reveals Sombrero Galaxy's Hidden Details

          Webb Reveals Sombrero Galaxy's Hidden Details

          Handout photo dated November 25, 2024 shows NASA’s James Webb Space Telescope recently imaged the Sombrero Galaxy with its MIRI (Mid-Infrared Instrument), resolving the clumpy nature of the dust along the galaxy’s outer ring. NASA’s James Webb Space Telescope captures the Sombrero Galaxy (Messier 104) in stunning mid-infrared detail. This oblong galaxy, named for its resemblance to a wide-brimmed hat, reveals intricate clumps of dust along its outer ring, illuminated in shades of blue and white. Speckles of stars scatter its inner disk, while distant galaxies dot the black cosmic canvas in the background. The new image, taken with Webb's MIRI instrument, offers unprecedented insight into the galaxy’s structure and the faint traces of young star-forming regions. November 25, 2024. Photo by NASA via ABACAPRESS.COM
            Webb Reveals Sombrero Galaxy's Hidden Details

            Webb Reveals Sombrero Galaxy's Hidden Details

            Handout photo dated November 25, 2024 shows the view of the famous Sombrero Galaxy in mid-infrared light (top) and visible light (bottom). The James Webb Space Telescope’s MIRI (Mid-Infrared Instrument) reveals the smooth inner disk of the galaxy, while the Hubble Space Telescope’s visible-light image shows the large and extended glow of the central bulge of stars. NASA’s James Webb Space Telescope captures the Sombrero Galaxy (Messier 104) in stunning mid-infrared detail. This oblong galaxy, named for its resemblance to a wide-brimmed hat, reveals intricate clumps of dust along its outer ring, illuminated in shades of blue and white. Speckles of stars scatter its inner disk, while distant galaxies dot the black cosmic canvas in the background. The new image, taken with Webb's MIRI instrument, offers unprecedented insight into the galaxy’s structure and the faint traces of young star-forming regions. November 25, 2024. Photo by NASA via ABACAPRESS.COM
              Hubble Spots the Little Dumbbell Nebula

              Hubble Spots the Little Dumbbell Nebula

              Handout - In celebration of the 34th anniversary of the launch of NASA’s Hubble Space Telescope, astronomers took a snapshot of the Little Dumbbell Nebula, also known as Messier 76, or M76, located 3,400 light-years away in the northern circumpolar constellation Perseus. The name ‘Little Dumbbell’ comes from its shape that is a two-lobed structure of colorful, mottled, glowing gases resembling a balloon that’s been pinched around a middle waist. Like an inflating balloon, the lobes are expanding into space from a dying star seen as a white dot in the center. Blistering ultraviolet radiation from the super-hot star is causing the gases to glow. The red color is from nitrogen, and blue is from oxygen. Photo by NASA, ESA, STScI via ABACAPRESS.COM
                NASA's Webb Reveals New Features in Heart of Milky Way

                NASA's Webb Reveals New Features in Heart of Milky Way

                Handout photo - The latest image from NASA's James Webb Space Telescope shows a portion of the dense center of our galaxy in unprecedented detail, including never-before-seen features astronomers have yet to explain. The star-forming region, named Sagittarius C (Sgr C), is about 300 light-years from the Milky Way's central supermassive black hole, Sagittarius A. Approximate outlines help to define the features in the Sagittarius C (Sgr C) region. Astronomers are studying data from NASA’s James Webb Space Telescope to understand the relationship between these features, as well as other influences in the chaotic galaxy center. The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.
                  NASA's Webb Reveals New Features in Heart of Milky Way

                  NASA's Webb Reveals New Features in Heart of Milky Way

                  Handout photo - The latest image from NASA's James Webb Space Telescope shows a portion of the dense center of our galaxy in unprecedented detail, including never-before-seen features astronomers have yet to explain. The star-forming region, named Sagittarius C (Sgr C), is about 300 light-years from the Milky Way's central supermassive black hole, Sagittarius A. The NIRCam (Near-Infrared Camera) instrument on NASA's James Webb Space Telescope's reveals a portion of the Milky Way’s dense core in a new light. An estimated 500,000 stars shine in this image of the Sagittarius C (Sgr C) region, along with some as-yet unidentified features. A large region of ionized hydrogen, shown in cyan, contains intriguing needle-like structures that lack any uniform orientation. The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and o
                    NASA's Webb Reveals New Features in Heart of Milky Way

                    NASA's Webb Reveals New Features in Heart of Milky Way

                    Handout photo - The latest image from NASA's James Webb Space Telescope shows a portion of the dense center of our galaxy in unprecedented detail, including never-before-seen features astronomers have yet to explain. The star-forming region, named Sagittarius C (Sgr C), is about 300 light-years from the Milky Way's central supermassive black hole, Sagittarius A. The NIRCam (Near-Infrared Camera) instrument on NASA's James Webb Space Telescope's reveals a portion of the Milky Way’s dense core in a new light. An estimated 500,000 stars shine in this image of the Sagittarius C (Sgr C) region, along with some as-yet unidentified features. A large region of ionized hydrogen, shown in cyan, contains intriguing needle-like structures that lack any uniform orientation. The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and o
                      Stunning First Full-Colour Images From Euclid Telescope

                      Stunning First Full-Colour Images From Euclid Telescope

                      HANDOUT - Irregular galaxy NGC 6822. The European Space Agency's (ESA) Euclid space mission unveiled its first five full-colour images of the cosmos on Tuesday, November 7, 2023. Launched in July, Euclid is a cutting-edge telescope tasked with mapping a third of the extragalactic sky, shedding light on how dark matter and dark energy shape our universe. This ambitious mission is unique in its ability to capture razor-sharp astronomical images across a vast expanse of the sky, offering unprecedented insights into the far reaches of the universe. The initial set of images serves as a testament to Euclid's unparalleled capability to construct the most extensive 3D map of the universe to date. Among the images, the most captivating is a panoramic view of the Horsehead Nebula, also known as Barnard 33, situated in the Orion constellation approximately 1,375 light-years away. The nebula, with its striking equine shape, stands as the nearest giant star-forming region to Earth. Positioned just south of the prominent