Tag Archive for 'NGC 346'

This Hubble image shows a small region of the Small Magellanic Cloud near the center of the open cluster NGC 346. Image credit: NASA / ESA / Hubble / C. Murray.

Hubble Focuses on Star-Studded Region in Neighbor Galaxy

Mar 17, 2025 by Enrico de Lazaro

A new image taken with the NASA/ESA Hubble Space Telescope shows a small region of the Small Magellanic Cloud, one of the closest galaxies to the Milky...

This Webb image shows NGC 346, a massive star cluster in the Small Magellanic Cloud. Yellow circles overlaid on the image indicate the positions of the ten stars surveyed in the study. Image credit: NASA / ESA / CSA / STScI / Olivia C. Jones, UK ATC / Guido De Marchi, ESTEC / Margaret Meixner, USRA.

Protoplanetary Disks around Sun-Like Stars Appear to Live Longer in Early Universe

Dec 16, 2024 by News Staff

In 2003, Hubble provided evidence of a massive exoplanet around a very old star. Such stars possess only small amounts of heavier elements that are the...

This Hubble image shows NGC 346, an open star cluster some 210,000 light-years in the constellation of Tucana. Image credit: NASA / ESA / C. Murray, Space Telescope Science Institute / Gladys Kober, NASA & Catholic University of America.

Hubble Space Telescope Captures Ultraviolet Image of NGC 346

Sep 3, 2024 by Enrico de Lazaro

The Hubble team has released a striking new photo taken by the NASA/ESA Hubble Space Telescope of the open cluster NGC 346, which resides in one of our...

This Webb image of NGC 346 traces emission from cool gas and dust. Image credit: NASA / ESA / CSA / STScI / N. Habel, JPL / P. Kavanagh, Maynooth University.

Webb Captures Mid-Infrared Image of NGC 346

Oct 10, 2023 by Enrico de Lazaro

A new image taken with the Mid-Infrared Instrument (MIRI) onboard the NASA/ESA/CSA James Webb Space Telescope shows streamers of gas and dust studded with...

This composite image features four separate images that combine X-ray data from Chandra and infrared data from Webb, and some data from other telescopes like Hubble, Spitzer and XMM-Newton. Image credit: NASA / CXC / SAO / ESA / XMM-Newton / CSA / STScI / JPL / CalTech / ESO / L. Frattare / J. Major / K. Arcand.

Webb Captures Two Galaxies, Star-Forming Nebula, and Star Cluster

May 24, 2023 by Enrico de Lazaro

New images that combine data from the NASA/ESA/CSA James Webb Space Telescope and several space- and ground-based telescopes show spiral galaxies NGC 1672...

Optical (left) and infrared (right) image of NGC 346 in the Small Magellanic Cloud; the positions of the main ionizing sources of NGC 346, namely SSN 7 and SSN 9, are highlighted by red and green squares, respectively. Image credit: A. Nota, ESA & STScI / NASA / ESA / CSA / O. Jones, UK ATC / G. De Marchi, ESTEC / M. Meixner, USRA / A. Pagan, STScI / N. Habel, USRA / L. Lenkic, USRA / L. Chu, NASA’s Ames Research Center.

Two Massive Touching Stars Will Merge as Black Holes in 18 Billion Years, Astronomers Predict

Apr 27, 2023 by Enrico de Lazaro

SSN 7 is a so-called contact binary located in the Small Magellanic Cloud, a dwarf galaxy some 210,000 light-years away in the constellation of Tucana....

The left panel shows a three-color composite mosaic of NGC 346 combining Webb’s F277W (blue), F335M (green) and F444W (red) filters. The region is rich in structures of knots, arcs and filaments. Areas of bright pink and/or red emission are associated with clumpy star formation. The spatially resolved PAH emission excited by ultraviolet photons in green is brightest in regions corresponding to the edges of dense material, characteristic of a photodissociation region. Massive stars, stars belonging to the BS90 cluster (circled in green) and the Small Magellanic Cloud field population are also visible. The right panel shows a mosaic image from the F335M filter showing four different populations of stars: pre-main-sequence stars (blue circles), young stellar objects with Paα (orange diamonds), young stellar objects without Paα (red squares) and stars matched with the HST-PMS catalogue (purple stars). Image credit: Jones et al., doi: 10.1038/s41550-023-01945-7.

Webb Detects Planetary Ingredients in NGC 346

Apr 25, 2023 by Natali Anderson

Located in the Small Magellanic Cloud at a distance of roughly 200,000 light-years, NGC 346 is a prominent young cluster — roughly 3 million years...

The unusual shape of the open cluster NGC 346 is partly due to stars and gas spiraling into the center of the cluster in a river-like motion; the red spiral superimposed on NGC 346 traces the movement of stars and gas toward the center; this spiraling motion is the most efficient way to feed star formation from the outside toward the center of the cluster. Image credit: NASA / ESA / Andi James, STScI.

Astronomers Find Spiraling Stars in NGC 346

Sep 8, 2022 by News Staff

Astronomers using the Multi Unit Spectroscopic Explorer (MUSE) instrument on ESO’s Very Large Telescope (VLT) and the NASA/ESA Hubble Space Telescope...