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Showing posts from March, 2024

Hubble's three-year study under the ULLYSES program enters a new chapter.

  The ULLYSES program embarked on a comprehensive investigation into the diverse population of young stars, focusing on two distinct categories: the scorching super-hot, massive, blue stars, and their cooler, redder counterparts, which are less massive than our Sun. Illustrating this stellar diversity, the top panel presents a captivating Hubble Space Telescope image capturing a star-forming enclave within 30 Doradus, the Tarantula Nebula. Situated amidst the ethereal expanse of the Large Magellanic Cloud, this celestial crucible teems with the brilliance of massive, youthful blue stars, serving as a prime target for ULLYSES' probing gaze. In contrast, the bottom panel offers an artist's rendition of a cooler, redder, young star, characterized by its subtle hues and serene demeanor. Despite its lesser mass compared to our Sun, this stellar entity is in the midst of an evolutionary ballet, as it steadily accrues material from its surrounding planetary disk, sculpting the cosmic ...

Was SNR 1181 really the surprising echo of an 800-year-old explosion?

In the year 1181 a rare supernova explosion appeared in the night sky, staying visible for 185 consecutive days. In the annals of astronomical history, the year 1181 marked an extraordinary event—a rare supernova explosion that captivated the night sky for 185 consecutive days. This cosmic spectacle, resembling a temporary ‘star’ in the constellation Cassiopeia shining as brightly as Saturn, left an indelible mark on humanity's collective memory.  For centuries, scientists endeavored to unravel the enigma of this ancient supernova's remnant. Initially, speculation pointed towards 3C 58, a nebula enveloping a pulsar. However, meticulous investigations revealed the pulsar predates the supernova event, dismissing it as the potential remnant. Enter Pa 30, a circular nebula with a central star discovered in Cassiopeia—a newfound contender in the quest for Supernova 1181's remnants. Through a composite image derived from various telescopic observations across the electromagnetic ...

Webb's unveiling of A duo of starbursts in I Zwicky 18.

  The NASA/ESA/CSA James Webb Space Telescope has recently unveiled a captivating portrait of the galaxy I Zwicky 18 (I Zw 18), originally identified by Swiss astronomer Fritz Zwicky in the 1930s. Situated approximately 59 million light-years away from Earth, this galaxy serves as a celestial time capsule, offering insights into the early stages of cosmic evolution. I Zw 18, classified as a dwarf irregular galaxy, epitomizes the primitive structures that populated the nascent universe. Characterized by abrupt surges in stellar birth, this diminutive galaxy harbors two prominent starburst regions nestled within its core. These regions, adorned with wispy brown filaments, bear witness to the transformative forces of stellar winds and intense ultraviolet radiation emitted by youthful, luminous stars. A neighboring companion galaxy, captured in the wider-field image, hints at a potential interaction that may have catalyzed I Zw 18's recent bout of star formation. Moreover, the faint or...

NASA's Hubble Captures FS Tau's Spectacular Jet Formation.

  NASA's Hubble Space Telescope unveils the enigmatic FS Tau star system in its latest image capture. Jets of vibrant energy streak across the cosmos as FS Tau, a newly forming star system, takes center stage in NASA's latest Hubble Space Telescope image.  Situated within the stellar nursery of FS Tau, FS Tau A and FS Tau B (Haro 6-5B) stand as celestial siblings amidst a tapestry of gas and dust. FS Tau A, a luminous beacon at the image's core, contrasts with FS Tau B, veiled by a dense shroud of dust to the far right. At a mere 2.8 million years old, FS Tau is a youthful ensemble compared to our mature Sun, which boasts an age of approximately 4.6 billion years. FS Tau B, a protostar in the making, is ensconced within a protoplanetary disk—a precursor to planetary formation—its silhouette delineated by a thick dust lane. The evolutionary journey of FS Tau B is illuminated by its transformation into a T Tauri star, a phase marked by fluctuations in brightness as nuclear fu...

Unveiling the Enigmatic Beauty of Spider Galaxy UGC 5829 by hubble.

  A captivating image captured by the NASA/ESA Hubble Space Telescope unveils the enigmatic beauty of the irregular galaxy UGC 5829. The celestial canvas captured by the NASA/ESA Hubble Space Telescope reveals the mesmerizing visage of UGC 5829, an irregular galaxy ensconced approximately 30 million light-years from Earth. Despite its elusive nature, this faint yet captivating cosmic entity has earned the moniker "the Spider Galaxy," evoking images of celestial arachnids with its ethereal allure. In this captivating image, the intricate tapestry of UGC 5829 unfolds, showcasing its enigmatic features and captivating charm. The galaxy's asymmetrical form, characterized by distorted galactic arms adorned with luminous, star-forming tips, evokes a semblance to the sinuous legs of an arachnid, weaving a cosmic web of intrigue and fascination. The genesis of this captivating portrait lies in the collaborative efforts of two pioneering Hubble observing programs. The first progra...

NASA's Chandra X-ray has identified a black hole that has very little impact on the surrounding environment.

NASA's Chandra X-ray Observatory has unveiled the underperformance of a black hole, contrary to astronomers' expectations. Dubbed H1821+643, this quasar, a rapidly growing supermassive black hole located approximately 3.4 billion light-years away from Earth, exhibits characteristics that challenge conventional understanding. Quasars, distinguished by their vigorous material consumption and consequent radiation emissions, typically wield significant influence over their host galaxies. However, H1821+643 defies this norm, as evidenced by data from Chandra and the NSF’s Karl G. Jansky’s Very Large Array. Unlike non-quasar black holes, which moderate star growth in their vicinity by regulating intergalactic hot gas temperature, quasars like H1821+643 manifest a lesser impact. Despite their heightened activity, quasars may play a diminished role in steering the fate of their host galaxies and clusters. Through meticulous analysis facilitated by Chandra, researchers dissected the in...

Why do brown dwarf stars move apart from each other?

Brown dwarfs, enigmatic objects residing in the Twilight Zone between stars and planets, have captured the attention of astronomers yet again. Despite their name, which seems to suggest a dull hue, these celestial beings are anything but ordinary. Unlike stars, they lack the mass needed to sustain hydrogen fusion, marking them as failed stars or super-sized planets, depending on one's perspective. A recent survey conducted by NASA's Hubble Space Telescope unveils a poignant truth about these cosmic wanderers: as they age, they grow increasingly solitary. Born sometimes in pairs, akin to stellar siblings, these brown dwarfs eventually part ways, drifting apart over hundreds of millions of years. The culprit? The gravitational influence of passing stars, which gradually weakens the bond between these stellar loners. Led by Clémence Fontanive of the Trottier Institute for Research on Exoplanets at the Université de Montréal, Canada, the study scrutinized a sample of aging brown dw...

Could the mysterious orbit of Betelgeuse be a cosmic illusion due to its huge 'boiling' surface.

  Recent simulations have shed light on the intriguing behavior of Betelgeuse, revealing the dynamic nature of its surface as blobs of plasma rise and fall, akin to a celestial boiling cauldron. The colossal star Betelgeuse, potentially on the brink of a cataclysmic explosion, has confounded scientists with its apparent rapid rotation, a phenomenon now attributed to the dynamic nature of its surface rather than true spinning. Betelgeuse, a red supergiant towering around 1,000 times the mass of our sun, holds the distinction of being one of the universe's largest stars. Its sheer enormity is such that if it were to replace the sun, its vast expanse would engulf the orbit of Jupiter, consigning inner planets like Earth, Mercury, Venus, and Mars to oblivion. Despite its youth of merely 10 million years, a mere fraction of our sun's age, Betelgeuse stands precariously on the threshold of celestial demise, having depleted its hydrogen reserves due to its intense heat and mass. This ...

Hubble Observes Galaxy LEDA 42160 Battling intergalactic gas Pressure in Virgo Cluster.

  This Hubble image shows dwarf galaxy, LEDA 42160. NASA/ESA's Hubble Space Telescope recently captured a striking image of LEDA 42160, a diminutive galaxy situated approximately 52 million light-years away in the Virgo constellation. Despite its small stature, this galaxy finds itself in the midst of a cosmic struggle within the dense environment of the massive Virgo cluster of galaxies. The image unveils LEDA 42160 as it contends with the formidable force known as ram pressure, exerted by the intergalactic gas permeating the cluster. Ram pressure, a consequence of the galaxy's motion through space, imposes significant effects on the galaxy's star formation processes. As LEDA 42160 traverses through the Virgo cluster, the relentless pressure from surrounding gas and dust threatens to strip the galaxy of its star-forming materials. This stripping action can hinder or even halt the birth of new stars within the galaxy. Paradoxically, however, ram pressure can also compress g...

Space Butterfly Nursery: Where Hundreds of Baby Stars Take Flight.

  W40, the cosmic "Space Butterfly," is a nebula—a colossal cloud of gas and dust—with its "wings" formed by massive stars expelling gas outward. In a mesmerizing display of cosmic artistry, NASA's Spitzer Space Telescope unveils the celestial spectacle of Westerhout 40 (W40), affectionately dubbed the "Space Butterfly." This infrared image captures the essence of a stellar nursery, where hundreds of infant stars take shape within the expansive confines of a nebula—a vast expanse of gas and dust in the cosmos primed for the birth of new stellar entities. W40's ethereal form, reminiscent of a crimson butterfly in flight, belies its true nature as a crucible for stellar genesis. Its majestic "wings" represent colossal bubbles of searing interstellar gas propelled by the radiant vigor of the region's most luminous and massive stars. Yet, amidst its breathtaking beauty, W40 also illustrates the paradoxical interplay between star formation...

Multiple NASA spacecraft tell the story of a giant solar storm that occurred on April 17, 2021.

  On April 17, 2021, the Solar Terrestrial Relations Observatory (STEREO) spacecraft provided a captivating glimpse of a coronal mass ejection, skillfully revealing solar features by obscuring the Sun with a black disk at the center of the image. On April 17, 2021, the Sun unexpectedly unleashed a formidable display of solar activity, launching a massive cloud of solar material into space. While solar eruptions are not uncommon, this particular event stood out for its unprecedented scale, propelling solar energetic particles (SEPs) – high-speed protons and electrons – toward multiple spacecraft across the inner solar system. Remarkably, it marked the first instance of such SEPs being observed simultaneously by spacecraft at five distinct locations, including those positioned between the Sun and Earth and others orbiting Mars. These diverse perspectives are shedding light on the varied origins and trajectories of potentially hazardous SEPs, emphasizing the complexity of solar phenom...

NASA's Juno mission provides an insight into Europa's oxygen production.

This view of Jupiter's icy moon Europa was skillfully captured by the JunoCam imager aboard NASA's Juno spacecraft. The snapshot was taken during the spacecraft's close flyby on September 29, 2022, providing a unique perspective on the enigmatic features that characterize Europa's icy surface. Beneath its icy exterior, Jupiter's moon Europa serves as a prolific oxygen factory, churning out an impressive 1,000 tons of oxygen every 24 hours. Scientists from NASA's Juno mission to Jupiter have recently recalibrated the rate of oxygen production on Europa, revealing a more conservative estimate compared to earlier studies. Published on March 4 in Nature Astronomy, these findings stem from measuring hydrogen outgassing from Europa's surface. The spacecraft's Jovian Auroral Distributions Experiment (JADE) instrument played a crucial role in collecting the data that led to this insightful discovery. In their published paper, the authors project the production o...

In 2024, the Great Lakes reach historic lows.

  In late February or early March each year, the Great Lakes typically witness their annual peak in ice coverage. However, the year 2024 marked an anomaly as the lakes were notably devoid of ice during this period. Unusually warm winter conditions and above-average surface water temperatures contributed to this phenomenon, resulting in historically low ice cover. Satellite-based measurements, dating back to 1973, have consistently recorded an average winter extent exceeding 40 percent ice coverage. Yet, by late February 2024, the ice cover reached only about one-tenth of this average maximum. The VIIRS (Visible Infrared Imaging Radiometer Suite) sensor aboard the Suomi NPP satellite captured this striking image of the lakes on February 24, 2024, highlighting the significant departure from the norm. The freezing patterns of the Great Lakes exhibit considerable variability, with instances like 2014 witnessing coverage exceeding 80 percent. Nevertheless, a discernible trend has emer...

NGC 1841 is a densely populated globular cluster of stars.

  Within the cosmic tapestry, NGC 1841 stands as a densely populated globular cluster nestled within the Large Magellanic Cloud (LMC). Situated about 162,000 light-years away, the LMC is a satellite galaxy gracefully orbiting the Milky Way, our cosmic host. While the Andromeda Galaxy often claims the title of our nearest galactic companion, a more accurate portrayal reveals a multitude of satellites encircling our home galaxy. Among these, the LMC shines as the largest and brightest, casting its celestial glow visible to the naked eye in the southern hemisphere, though the encroachment of light pollution dims its luminosity. Nestled within the confines of the LMC, numerous globular clusters, including NGC 1841, grace the cosmic landscape. These enigmatic celestial bodies, positioned between open clusters and compact galaxies in density, harbor diverse stellar populations. The intricacies of their formation remain elusive, yet common threads persist. Globular clusters, marked by sta...