Skip to main content

The a barred spiral galaxy NGC 1559 has been observed by the Webb telescope.

 


This image features the barred spiral galaxy galaxy NGC 1559 as seen by the NASA/ESA/CSA James Webb Space Telescope.


Captured by the NASA/ESA/CSA James Webb Space Telescope, this image showcases the barred spiral galaxy NGC 1559. Situated approximately 35 million light-years away in the seldom-explored southern constellation Reticulum (The Reticule), the galaxy exhibits a visible central region and distinctive, loosely-wound spiral arms. Utilizing two of Webb's instruments, the Mid-InfraRed Instrument (MIRI) captures the glow of interstellar dust grains, outlining the interstellar medium crucial for future star formation. Simultaneously, the Near-InfraRed Camera (NIRCam) reveals starlight, including that from young stars concealed behind extensive dust, and captures emissions from ionized nebulae surrounding these youthful celestial bodies.


The PHANGS team collected the data featured in this image as part of an extensive observing program, where the James Webb Space Telescope (Webb) observes 55 galaxies previously mapped by the Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope and the NASA/ESA Hubble Space Telescope. Webb's unparalleled perspective on dust and stars, combined with data from these other instruments, aims to provide an exceptionally detailed understanding of the life cycle of stars in galaxies throughout the Universe. As a Treasury program, the data is accessible immediately to the scientific community and the public, allowing for more rapid and extensive research applications.


NGC 1559, with its expansive spiral arms teeming with star formation, is in a state of recession, moving away from us at a velocity of approximately 1300 kilometers per second. Despite the optical illusion that places NGC 1559 near one of our apparent neighbors, the Large Magellanic Cloud (LMC), this is merely a trick of perspective. In reality, NGC 1559 exists in isolation, devoid of any nearby galaxies or affiliation with a galaxy cluster. Although it may be a cosmic loner, the James Webb Space Telescope allows us to appreciate NGC 1559 from a distance, offering a unique glimpse into its solitary celestial existence.

Comments

Popular posts from this blog

James Webb Space Telescope Opens New Frontiers in the Search for Life Beyond Earth.

  This image illustrates a science-based artist’s impression of K2-18 b, a potentially habitable exoplanet 120 light-years away, orbiting a cool dwarf star in its habitable zone. NASA’s James Webb Space Telescope (JWST) is revolutionizing the search for life beyond our solar system, offering humanity its most detailed look yet at distant, potentially habitable worlds. With its extraordinary infrared capabilities, Webb is not only detecting atmospheres on small rocky exoplanets but also probing their chemical makeup in search of biosignatures—clues that could hint at the presence of life. However, scientists caution that context is everything. Atmospheric data alone is not enough to confirm life; understanding a planet’s surface, interior, and broader environment is essential. Even detecting a potential biosignature, such as a gas possibly produced by biological processes, doesn’t equate to discovery. Multiple, independent lines of evidence would be needed to confirm such a find. “F...

Webb Telescope Reveals Tangled Rings and Dusty Chaos in Dying Star System NGC 1514.

  NASA’s James Webb Space Telescope has captured the most detailed image yet of planetary nebula NGC 1514, revealing clumpy dust rings and clear holes in its vibrant pink core using mid-infrared light. A dying star’s final performance has been brought into sharp focus by NASA’s James Webb Space Telescope, revealing a cosmic display of tangled rings, drifting dust, and mysterious holes in the planetary nebula NGC 1514. This mesmerizing structure lies about 1,500 light-years away in the constellation Taurus and has been evolving for at least 4,000 years. At the heart of the nebula are two tightly bound stars, orbiting each other every nine years, their light diffracted in Webb’s images like a celestial jewel. While the stars appear as one in mid-infrared light, they are central to the nebula’s complex architecture. One of these stars, once several times the mass of our Sun, ejected its outer layers in a slow, dense stellar wind as it aged. The other star’s close approach may have twi...

Astronomers have discovered a 'Death Star' black hole in action.

A team of astronomers has studied 16 supermassive black holes that are firing powerful beams into space, tracking where these beams, or jets, are pointing now and where they were aimed in the past, as reported in our latest press release. Using NASA’s Chandra X-ray Observatory and the U.S. National Science Foundation (NSF) National Radio Astronomical Observatory’s (NRAO) Very Large Baseline Array (VLBA), they found that some of the beams have changed directions by large amounts. These two Chandra images show hot gas in the middle of the galaxy cluster Abell 478 (left) and the galaxy group NGC 5044 (right). The center of each image contains one of the sixteen black holes firing beams outwards. Each black hole is located in the center of a galaxy embedded in the hot gas. In the images below, labels and the radio images appear. Ellipses show a pair of cavities in the hot gas for Abell 478 (left), while ellipses indicate two pairs of cavities for NGC 5044 (right). These cavities were carve...