All articles tagged with #sombrero galaxy
Astronomers using the 570-megapixel Dark Energy Camera in Chile captured a vast, diffuse halo around the Sombrero Galaxy (M104), extending far beyond its dusty disk and revealing a faint stellar stream that suggests past interactions with a smaller satellite galaxy. The image showcases both the bright central bulge and the faint outer structures in one frame, thanks to the camera’s sensitivity to extremely faint light.
A new 570-megapixel image from the Dark Energy Camera at Cerro Tololo reveals an enormous, diffuse halo around the Sombrero Galaxy (M104) that extends beyond the bright disk by more than three times, plus a faint stellar stream suggesting past interactions with a smaller satellite. The image also sharpens the central bulge and dust lanes, highlighting star formation regions and the galaxy’s distinctive hat-like shape, thanks to NOIRLab’s deep-sky imaging capabilities, building on recent JWST mid-infrared observations.
Space.com spotlights Messier 104, the Sombrero Galaxy, a spiral galaxy about 28 million light-years away in Virgo whose distinctive wide, hat-like disk earns it its nickname. The image was captured with the Dark Energy Camera (DECam) on the Blanco 4-meter telescope at Cerro Tololo, part of NOIRLab, and the galaxy hosts roughly 2,000 globular clusters. It’s too faint to see with the naked eye, though binoculars or a small telescope reveal its silhouette. This piece marks Space photo of the day for April 29, 2026.
The NSF’s 570‑megapixel Dark Energy Camera on the Victor M. Blanco 4‑meter telescope in Chile captured an ultra‑high‑resolution image of Messier 104 (the Sombrero Galaxy), detailing its dusty disk, extensive halo, thousands of globular clusters, and a tidal stellar stream that hints at a past merger, enabling deeper study of its structure and star formation.
A newly released image from NSF's NOIRLab captures Messier 104, the Sombrero galaxy, in an edge-on view that highlights its bright central bulge and dusty disk, illustrating the galaxy's distinctive silhouette about 28 million light-years from Earth.
Spring skies reveal a lineup of galaxies visible from the northern hemisphere, including the Leo Triplet and bright targets like the Sombrero and Whirlpool galaxies. The piece guides readers on star-hopping to locate these faint objects in regions such as Leo, Virgo, and Canes Venatici, and notes that a telescope (6 inches or more) or large binoculars is typically needed for rewarding views under dark skies.
The James Webb Space Telescope captured its most detailed image yet of the Sombrero Galaxy, revealing new features such as interstellar dust clouds and red giant stars, enhancing our understanding of this peculiar galaxy's structure and history.
NASA's James Webb Space Telescope has captured detailed near-infrared images of the Sombrero Galaxy, revealing its dense star bulge, dust lanes, and evidence of a turbulent past involving galaxy mergers, while also showcasing individual stars and distant galaxies in unprecedented detail.
NASA's James Webb Space Telescope has captured new near-infrared images of the Sombrero Galaxy, revealing details about its core, dust, and past mergers, enhancing our understanding of galaxy evolution.
The James Webb Space Telescope has provided a new perspective on the Sombrero galaxy, revealing its smooth inner disk and complex outer ring through mid-infrared imaging. This view contrasts with the visible light images from the Hubble Space Telescope, which highlight the galaxy's glowing core. The new imagery suggests the presence of star-forming regions and reveals carbon-containing molecules in the dust ring. Despite its quiet star formation activity, the Sombrero galaxy hosts a supermassive black hole and numerous globular clusters, offering rich opportunities for astronomical study.
NASA's James Webb Space Telescope has captured a detailed mid-infrared image of the Sombrero Galaxy, revealing a clumpy dust structure in its outer ring, unlike the smooth appearance seen in previous observations. This new perspective highlights the distribution of dust, a key component in star formation, although the Sombrero Galaxy is not a major site for star creation. The galaxy, located 30 million light-years away in Virgo, also hosts a supermassive black hole and numerous globular clusters, offering rich opportunities for astronomical study.
The James Webb Space Telescope (JWST) has provided new insights into the Sombrero galaxy, revealing its outer dust ring as turbulent and clumpy, and highlighting a sparse, dust-depleted inner disk. The galaxy, which combines features of both spiral and elliptical galaxies, contains a supermassive black hole and forms only one solar mass of new stars annually. JWST's advanced capabilities have unveiled details previously unseen, including numerous background galaxies, suggesting the Sombrero galaxy may represent a galactic end-state after consuming its neighbors.
The James Webb Space Telescope (JWST) has captured a new image of the Sombrero Galaxy, revealing its dust rings in unprecedented detail at mid-infrared wavelengths. This view highlights clumps in the outer ring, suggesting young star-forming regions, despite the galaxy's low star production rate compared to others like the Cigar Galaxy. The image also showcases a backdrop of distant galaxies, underscoring JWST's role in advancing astronomical research. Demand for JWST observation time is high, with a nine-to-one oversubscription rate for upcoming cycles.
NASA's James Webb Space Telescope has captured a detailed mid-infrared image of the Sombrero galaxy, revealing clumpy dust in its outer ring and multiple inner rings, which were not visible in previous images by the Hubble and Spitzer telescopes. This new view provides insights into the galaxy's structure and star-forming regions, despite its relatively low star formation rate and inactive supermassive black hole.
The James Webb Space Telescope has captured a new image of the Sombrero Galaxy, revealing unexpected details. Unlike previous images from the Hubble Telescope, the JWST's Mid-Infrared Instrument shows that the galaxy's dust ring is not a significant site for star formation, and the central region features a flat disk rather than a halo of stars. The galaxy's active black hole is also less luminous than anticipated. These findings suggest the Sombrero Galaxy is more unusual than previously thought, with future studies likely focusing on its numerous globular clusters.