Skip to main content

Astronomers Discover "Firefly Sparkle," a Forming Galaxy in the Early Universe.

 



For the first time, astronomers have identified a still-forming galaxy that weighs about the same as our Milky Way would have when it was in its infancy. This newly discovered galaxy, nicknamed the Firefly Sparkle, is in the process of assembling and forming stars, existing just 600 million years after the Big Bang.


The galaxy’s stretched and warped appearance is the result of gravitational lensing, a natural effect that magnifies distant objects. This phenomenon allowed researchers to gather unprecedented details about the galaxy’s structure, with some parts of the galaxy appearing over 40 times larger.


The Firefly Sparkle galaxy shines brightly with star clusters in a range of infrared colors, which indicate that the stars are forming at different stages, rather than all at once. This provides a rare glimpse into the evolutionary stages of a galaxy as it forms.


“I didn’t think it would be possible to resolve a galaxy that existed so early in the universe into so many distinct components, let alone discover a Milky Way-mass galaxy in the process of forming,” said Lamiya Mowla, lead author of the study and an assistant professor at Wellesley College in Massachusetts.


The researchers were able to identify 10 distinct star clusters in the galaxy. The galaxy itself is elongated due to gravitational lensing, which allowed for detailed study of its structure. Unlike other distant galaxies where stars appear as a single mass, the Firefly Sparkle allows astronomers to see the "building blocks" of a galaxy forming, star by star.


Adding to the complexity, two companion galaxies are located nearby—just 6,500 and 42,000 light-years away from the Firefly Sparkle. These galaxies may play a significant role in shaping the galaxy’s development over billions of years. The close proximity of these companions suggests they may eventually merge, with interactions that could trigger new star formations.


“This discovery is significant because it supports the long-standing theory that galaxies in the early universe formed through successive interactions and mergers with smaller galaxies,” explained Yoshihisa Asada, a co-author of the study and a doctoral student at Kyoto University.


The Firefly Sparkle exists in the galaxy cluster MACS J1423, which was previously studied by the Hubble Space Telescope as part of the Cluster Lensing And Supernova Survey with Hubble (CLASH) program. While Hubble was the first to image the galaxy, the James Webb Space Telescope provided new insights, resolving additional star clusters and detecting the two companion galaxies.


Mowla and her team discovered the Firefly Sparkle while analyzing Webb’s Canadian NIRISS Unbiased Cluster Survey (CANUCS), which includes infrared images and spectra from Webb's NIRCam and NIRSpec instruments. The team was drawn to the galaxy's sparkling star clusters, leading them to nickname it the Firefly Sparkle, resembling a swarm of glowing fireflies in the dark.


This discovery offers a remarkable opportunity to study the early stages of galaxy formation, providing valuable insight into how galaxies like the Milky Way may have formed in the distant past.


Comments

Popular posts from this blog

NASA/ESA Hubble Space Telescope Reveals New Details of the Orion Nebula’s Star Formation.

  This NASA/ESA Hubble Space Telescope image captures the Orion Nebula (Messier 42, M42), the nearest star-forming region to Earth, located about 1,500 light-years away. A captivating new image captured by the NASA/ESA Hubble Space Telescope offers an extraordinary look into the Orion Nebula, the nearest massive star-forming region to Earth. Located just 1,500 light-years away, this nebula is visible to the naked eye below the three stars forming Orion's "belt." The region is home to hundreds of newborn stars, including two protostars featured in the image: HOPS 150 and HOPS 153. Named after the Herschel Orion Protostar Survey, conducted with ESA’s Herschel Space Observatory, the protostars HOPS 150 and HOPS 153 provide key insights into the early stages of star formation. HOPS 150, visible in the upper-right corner of the image, is a binary star system, with two young stars orbiting one another. These protostars are surrounded by small dusty disks, where material from th...

New Method Detects Small Asteroids in Main Belt, Offering Insight for Planetary Defense.

  An international team of physicists, led by MIT researchers, has developed a groundbreaking method to detect small asteroids, as small as 10 meters in diameter, within the main asteroid belt. These space rocks, ranging from the size of a bus to several stadiums wide, were previously undetectable using traditional methods. The team's discovery, detailed in a paper published in Nature, could significantly improve tracking of potential asteroid impactors, aiding planetary defense efforts. The main asteroid belt, located between Mars and Jupiter, is home to millions of asteroids, but until now, scientists could only detect objects roughly a kilometer in diameter. The new detection technique, which utilizes the "shift and stack" method, is able to identify much smaller asteroids, even those far from Earth, enabling more precise orbital tracking. This breakthrough is crucial for planetary defense, allowing scientists to spot near-Earth objects that may pose a threat in the fu...

XSPECT Payload Successfully Validates Performance through Cas A Observation.

  The XSPECT instrument captures a detailed spectrum of the supernova remnant Cassiopeia A (Cas A), encompassing both the Galactic Cosmic Ray (GCR) background and the Cosmic X-ray Background (CXB). The flux observed above 8 keV predominantly results from the combined contributions of CXB and GCR. The presented spectrum, depicted in the figure, is derived from a cumulative integration time of 20 ksec, collected across multiple orbits, providing valuable insights into the X-ray emissions associated with Cas A. XPoSat, India's inaugural X-ray polarimetric mission, has achieved a significant as the XSPECT instrument captures its initial observations from the Cassiopeia A (Cas A) supernova remnant. Launched on January 1, 2024, XPoSat is equipped with two co-aligned instruments, namely the POLarimeter Instrument in X-rays (POLIX) and X-ray SPECtroscopy and Timing (XSPECT). This mission is designed to unravel the mysteries of cosmic X-ray sources. While POLIX focuses on examining X-ray po...