Hubble’s Close-Up of the Spherical Cluster Messier 72

As part of Hubble’s 35th anniversary ceremony, astronomers have acquired a stunning new image of a rich collection of scattered stars. Messier 72.

This Hubble image shows the Messier 72, a spherical cluster about 50,000 light years away in the constellation of Aquarius. Image credits: NASA/ESA/Hubble/A. Sarajedini / G. Piotto / M. libralato.

Spherical clusters are a very old star system, coupled to a single structure, about 100-200 light-years by gravity.

They contain hundreds of thousands, or perhaps million stars. Large masses at the center of the rich stars in the cluster pull the stars inward to form a ball of stars.

Spherical clusters are one of the oldest known objects in the universe and are relics from the first era of the Galactic Layer.

It is believed that all galaxies have a population of spherical clusters. Our Milkyway Galaxy hosts at least 150 such objects, and could be hidden behind the thick disks of the Galaxy.

Messier 72 is It was located It is about 50,000 light years away from Earth, the constellation of Aquarius.

This spherical cluster, also known as the M72 or NGC 6981, is almost 9.5 billion years old.

Its apparent size is 9.4, and appears as a faint patch of light on a small telescope. The best time to observe it is September.

Messier 72 was the first one I discovered it In 1780, by Pierre Messine, a French astronomer and colleague of Charles Messier.

It is the first of the five-star clusters Mechine discovers while assisting Messier, and one of the most remote clusters in Messier’s catalog.

“Messier 72 is a particularly special target as it was the first image to be released in the Hubble Picture of the Week series on April 22, 2010,” Hubble Astronomers said in a statement.

“For 15 years, our team has been publishing new Hubble images every Monday for everyone to enjoy.”

“This has added nearly 800 images to the vast Hubble Image Archive over the years.”

“The impressive variety of star colours in the new Messier 72 images, especially compared to the original image, is the result of adding UV observations to previous visible light data,” they added.

“Colors indicate different types of stars.”

“The blue star is a cluster star originally larger, and after burning much of its hydrogen fuel, it now reaches a hotter temperature. The bright red object is a low-mass star that is now a red giant.”

“Studying these different groups will help you understand the spherical clusters and how the galaxies in which they were born were first formed.”

Source: www.sci.news

Hubble’s Spectacular Images of NGC 5530

NASA has released a beautiful new image snapped by the NASA/ESA Hubble Space Telescope on the “flocculent” Spiral Galaxy NGC 5530.



This Hubble image shows the NGC 5530, a spiral galaxy about 40 million light years away in the constellation of Lupus. Image credits: NASA/ESA/Hubble/D. Thilker.

NGC 5530 It is about 40 million light years away from the constellation of Lupus.

Also known as the IRAS 14152-4309 or ESO-LV 272-0030, this Galaxy has a diameter of approximately 60,000 light years.

First discovered by British astronomer John Herschel on April 7, 1837, the NGC 5530 is a key member of the NGC 5643 Galaxy Group.

“NGC 5530 is classified as a “coheterogeneous” spiral. This means that the spiral arm is patchy and obscure,” the statement said.

“Some galaxies have very bright centers that host ultra-high Massive black holes of feasts, but the bright source near the centre of NGC 5530 is not an active black hole, but a star
within our own galaxy, which is only 10,000 light years from Earth.”

“This chance alignment gives the star the appearance of the dense mind of the NGC 5530.”

2007, a labeled supernova event SN 2007it It occurred in this galaxy.

“If you had pointed to a backyard telescope on the NGC 5530 on the evening of September 13, 2007, you would have seen another bright spot of light adorned the galaxy,” the astronomer said.

“That night, Australian amateur astronomer Robert Evans discovered a supernova named SN 2007it by comparing the appearance of the NGC 5530 with a reference photograph of the galaxy from a telescope.”

“It’s worth noting that even one supernova can be discovered using this painstaking method, but Evans has actually discovered over 40 supernovaes like this.”

“This particular discovery was truly a coincidence. It is possible that light from the supernova completed its 40 million year journey to Earth a few days before the explosion was discovered.”

The color image of the NGC 5530 is Hubble Wide Field Camera 3 (WFC3) UV, near-infrared, and optical parts of the spectrum.

The image is based on data obtained through five filters. Colors are attributed to assigning different hue to each monochromatic image associated with an individual filter.

Source: www.sci.news

Hubble’s Stunning Photomosaic of the Andromeda Galaxy Unveils Countless Stars

A century ago, American astronomer Edwin Hubble was the first to prove that this so-called “spiral nebula” lies about 2.5 million light-years away from the Milky Way. To date, the NASA/ESA Hubble Space Telescope has achieved the most comprehensive survey of the Andromeda Galaxy. It took more than 10 years to collect the data. This colorful portrait which captures the glow of 200 million stars and was created from over 600 snapshots.

This is the largest photomosaic ever assembled from Hubble observations. A panoramic view of the neighboring Andromeda galaxy, 2.5 million light years away. Image credit: NASA/ESA/B. Williams, University of Washington.

The Andromeda Galaxy (Mesier 31) is located 2.5 million light-years away and is the closest large galaxy neighbor to the Milky Way.

Hubble's sharp imaging power can resolve more than 200 million stars in the galaxy and detect only those stars brighter than the Sun. They look like grains of sand on a beach. But that's just the tip of the iceberg.

Andromeda's total population is estimated to be 1 trillion stars, with many less massive stars falling below Hubble's sensitivity limit.

“Imaging the Andromeda Galaxy was a difficult task because it is a much larger target than the galaxies that Hubble regularly observes, often billions of light years away,” Washington said. said university astronomer Zhuo Chen and colleagues.

“The complete mosaic was performed under two Hubble observing programs. In total, it required more than 1,000 Hubble orbits spanning more than 10 years.”

“This panorama… Panchromatic Hubble Andromeda Treasury (PHAT) Program About ten years ago. ”

The Andromeda Galaxy is tilted 77 degrees to Earth's perspective and is seen almost head-on. Areas of interest include (a) a photobombing of bright blue clusters of stars embedded within the galaxy, background galaxies visible in the distance, and some bright foreground stars that are actually within the Milky Way; Masu. (b) NGC 206 is Andromeda's most prominent nebula. (c) A young population of newborn blue stars. (d) Satellite galaxy M32. This could be the remnant nucleus of a galaxy that once collided with Andromeda. (e) A dark dust band across countless stars. Image credit: NASA/ESA/B. Williams, University of Washington.

“Images were acquired at near-ultraviolet, visible, and near-infrared wavelengths. Hubble's advanced survey camera (ACS) and wide field camera 3 (WFC3) To photograph the northern half of Andromeda. ”

“The follow-up of this program is Panchromatic Hubble Andromeda Tropical Treasury (PHAST), added images of about 100 million stars in the southern half of Andromeda. ”

“This region is structurally unique and more sensitive to the history of galactic mergers than the northern disk mapped by the PHAT survey.”

“The combined program collectively covers Andromeda's entire disc, which is tilted 77 degrees to Earth's field of view and viewed almost head-on.”

“The galaxy is so large that the mosaic is assembled from about 600 separate fields of view.”

of result described in the paper. astrophysical journal.

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Zhuo Chen others. 2025. Fast. Panchromatic Hubble Andromeda Southern Treasury. I. Ultraviolet and optical photometry of over 90 million stars in M31. APJ 979, 35;doi: 10.3847/1538-4357/ad7e2b

Source: www.sci.news

Hubble’s Observation of a Spiral Galaxy Hosting a Supernova

NASA has released a beautiful photo of spiral galaxy LEDA 22057 taken by the NASA/ESA Hubble Space Telescope.

This Hubble image shows spiral galaxy LEDA 22057 about 650 million light-years away in the constellation Gemini. Image credits: NASA/ESA/Hubble/RJ Foley, University of California, Santa Cruz.

Leda 22057 It is located in the constellation Gemini, about 650 million light years away from Earth.

Also known as AGC 170923, MaNGA 11743-12703, or 2MASX J07524264+1450263, this galaxy is the site of a supernova explosion.

“This special supernova… SN2024piwas discovered by automated research in January 2024,” Hubble team members said in a statement.

“This survey covered the entire northern half of the night sky every two days and cataloged more than 10,000 supernovae.”

New images of LEDA 22057 consist of observations from. Hubble’s Wide Field Camera 3 (WCF3) Located in the infrared part of the spectrum.

“SN 2024pi is visible in this image,” the astronomers said.

“SN 2024pi’s pale blue dot, located just below and to the right of the galactic nucleus, stands out against the galaxy’s ghostly spiral arms.”

“This image was taken about a month and a half after the supernova was discovered, so the supernova appears many times fainter here than at its peak brightness.”

According to the researchers, SN 2024pi supernova belongs to type Ia.

“This type of supernova requires a remarkable object called a white dwarf, which is the crystallized core of a star with a mass less than about eight times the mass of the Sun,” the researchers said.

“When a star of this size runs out of hydrogen in its core, it expands into a red giant, becoming colder, swollen, and brighter.”

“Over time, pulsations and stellar winds strip away the star’s outer layers, leaving behind a white dwarf and a colorful planetary nebula.”

“White dwarfs can have surface temperatures of over 100,000 degrees Celsius and are extremely dense, packing almost the mass of the Sun into a sphere the size of Earth.”

“Nearly all stars in the Milky Way will someday evolve into white dwarfs, a fate that awaits our Sun in about 5 billion years, but not all of them will explode as Type Ia supernovae.”

“For that to happen, the white dwarf must be part of a binary star system.”

“If a white dwarf siphons material from its stellar partner, it could become too massive to support itself.”

“The resulting runaway fusion explosion destroys the white dwarf in a supernova explosion visible many galaxies away.”

Source: www.sci.news

Webb confirms Hubble’s calculations of distance

New observations by NASA/ESA/CSA’s James Webb Space Telescope confirm previous measurements by the NASA/ESA Hubble Space Telescope of the distances between nearby stars and galaxies, and confirm measurements of the universe’s mysterious expansion. Provide critical cross-checking to address discrepancies. This contradiction, known as the Hubble tension, remains unexplained by even the best cosmological models.

This artist’s impression shows the evolution of the universe, starting with the Big Bang on the left and continuing with the emergence of the Cosmic Microwave Background. The formation of the first stars ends the Dark Ages of the universe, followed by the formation of galaxies. Image credit: M. Weiss / Harvard-Smithsonian Center for Astrophysics.

“The discrepancy between the observed rate of expansion of the universe and the predictions of the Standard Model suggests that our understanding of the universe may be incomplete,” said Nobel laureate and Johns Hopkins University professor Adam Riess. “There is,” he said.

“Now that NASA’s two flagship telescopes are confirming each other’s discoveries, we must take this issue very seriously. It’s a challenge, but it’s a It’s also a great opportunity to learn more.”

The new research builds on Professor Rees’ Nobel Prize-winning discovery that the expansion of the universe is being accelerated by a mysterious dark energy that permeates the vast expanses of space between stars and galaxies.

The authors used the largest sample of Webb data collected during the first two years of the universe to test the Hubble telescope’s measure of the rate of expansion of the universe, a number known as the Hubble constant.

They used three different methods to measure the distance to the galaxy where the supernova occurred, using a method previously measured by the Hubble telescope and known to provide the most accurate “local” measurement of this number. We focused on the distance that is being

Observations from both telescopes were in close agreement, revealing that Hubble’s measurements were accurate and eliminating inaccuracies large enough to attribute the tension to Hubble’s errors.

Still, the Hubble constant remains a mystery. This is because measurements based on current telescopic observations of the universe produce higher values ​​compared to projections made using the standard model of cosmology. The Standard Model is a widely accepted framework for how the universe works, calibrated with cosmic microwave background data. Weak radiation left over from the Big Bang.

The Standard Model Hubble constant is approximately 67-68 km/sec per megaparsec, but measurements based on telescope observations typically yield higher values ​​of 70-76, with an average of 73 km/sec/megaparsec.

This discrepancy has puzzled cosmologists for more than a decade. A difference of 5 to 6 kilometers per second per megaparsec is too large to be explained solely by deficiencies in measurement and observation technology.

Webb’s new data eliminates significant bias in Hubble’s measurements, so the Hubble tension could be due to unknown factors or gaps in cosmologists’ understanding of physics that have yet to be discovered.

“Webb’s data represent the first high-definition view of the universe, greatly improving the signal-to-noise ratio of the measurements,” said Xiang Li, a graduate student at Johns Hopkins University. .

This image, taken with the Nicholas U. Mayall 4-meter telescope, shows the spiral galaxy Messier 106. Two dwarf galaxies (NGC 4248 in the lower right and UGC 7356 in the lower left) also appear in the image. Image credits: KPNO / NOIRLab / NSF / AURA / New Mexico State University MT Patterson / University of Alaska Anchorage TA Chancellor / M. Zamani & D. de Martin.

The astronomers used the known distance to the spiral galaxy Messier 106 (also known as M106 or NGC 4258) as a reference point to cover roughly one-third of Hubble’s total galaxy sample.

Despite the small dataset, they achieved impressive accuracy, showing less than 2% difference between measurements. This is much smaller than the approximately 8-9% size of the Hubble tension mismatch.

In addition to analyzing pulsating stars called Cepheid variable stars, the gold standard for measuring distances in the universe, they cross-checked measurements based on the brightest red giant stars in the same galaxy as carbon-rich stars. .

All galaxies observed by Webb with supernovae yielded a Hubble constant of 72.6 km per second per megaparsec. This is about the same as the 72.8 km per second per megaparsec that Hubble found for the very same galaxy.

“One possible explanation for the Hubble tension is that something was missing in our understanding of the early universe, such as a new component of matter that unexpectedly bombarded the universe after the Big Bang, nascent dark energy. I guess so,” Johns said. Mark Kamionkowski, a cosmologist at Hopkins University, was not involved in the study.

“And there are other ideas that might do the trick, like interesting dark matter properties, exotic particles, changing electron masses, or primordial magnetic fields. Theorists have a right to be pretty creative. It is.”

of result Published in astrophysical journal.

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Adam G. Reese others. 2024. JWST validates HST distance measurements: Supernova subsample selection explains differences in JWST estimates of local H0. APJ 977, 120; doi: 10.3847/1538-4357/ad8c21

Source: www.sci.news

Hubble’s Stunning Images of NGC 1672

The NASA/ESA Hubble Space Telescope took this photo of barred spiral galaxy NGC 1672, visible from the southern hemisphere.



This Hubble image shows NGC 1672, a barred spiral galaxy about 49 million light-years away in the constellation Sera. Color images were created from separate exposures taken in the ultraviolet, visible, and near-infrared regions of the spectrum using Hubble’s Advanced Survey Camera (ACS) and Wide Field Camera 3 (WFC3). Six filters were used to sample different wavelengths. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credits: ESA / Hubble / NASA / O. Fox / L. Jenkins / S. Van Dijk / A. Filipenko / J. Li / PHANGS-HST Team / D. De Martin / M. Zamani.

NGC1672 is located approximately 49 million light-years away in the constellation Sera.

This galaxy, also known as ESO 118-43, IRAS 04449-5920, LEDA 15941, or VV 826, has a diameter of 75,000 light years.

it was discovered It was proposed by Scottish astronomer James Dunlop on November 5, 1826.

NGC 1672 is a typical barred spiral galaxy, which differs from normal spiral galaxies in that its spiral arms do not twist all the way to the center.

Instead, they are attached to each end of the star’s straight rod that surrounds the core.

NGC 1672 is visible almost head-on and shows regions of intense star formation.

The highest concentrations of star-forming regions are near the edges of galaxies’ strong galactic bars.

NGC 1672 is Seyfert Galaxyis named after astronomer Carl Keenan Seifert, who extensively studied galaxies containing active nuclei in the 1940s. The energy output of these nuclei can exceed that of the host galaxy.

Active galaxies also include the exotically named quasars and blazars.

Each type has unique characteristics, and they are all thought to be powered by the same engine – a supermassive black hole – but seen from different angles.

“NGC 1672 is a versatile light show that showcases the impressive lights of a variety of celestial objects,” Hubble astronomers said in a statement.

“Like other spiral galaxies, its disk is filled with billions of bright stars, giving it a beautiful glow.”

“Along its two large arms, bubbles of hydrogen gas glow with a striking red light due to the powerful radiation of newly formed stars within.”

“There are some particularly spectacular stars near the center: newly formed, extremely hot stars that are embedded in a ring of hot gas and emit powerful X-rays,” the researchers said. added.

“And at its center lies an even brighter X-ray source, an active galactic nucleus produced by the heated accretion disk around NGC 1672’s supermassive black hole. This makes NGC 1672 a Seyfert galaxy. Masu.”

“But the highlight of the new photos is the most fleeting and ephemeral of these lights: supernovae. SN2017 GaxIt appears in only one of the six Hubble images that make up this composite image. ”

“this is Type I supernova Caused by the collapse of a core and the subsequent explosion of a giant star, it goes from invisible to new light in the sky in just a few days. ”

“In images taken later that year, the supernova was already fading, so it’s only visible here as a small green dot just below the bend of the spiral arm on the right.”

“In fact, this was intentional. We wanted to look for companion stars that the supernova progenitor might have had, something that would be impossible to find outside of a living supernova.”

Source: www.sci.news

Hubble’s Stunning Photo of NGC 4951

In this new image, the NASA/ESA Hubble Space Telescope captures the glow of spiral galaxy NGC 4951.



This Hubble image shows NGC 4951, a spiral galaxy about 49 million light-years away in the constellation Virgo. Image courtesy of NASA / ESA / Hubble / D. Thilker / M. Zamani, ESA and Hubble.

NGC 4951 is located about 49 million light-years from Earth in the constellation Virgo.

Also known as AGC 530015, IRAS 13025-0613, or LEDA 45246, the galaxy has a diameter of about 65,000 light-years.

It was discovered on April 17, 1784 by German-born British astronomer William Herschel.

The new image of NGC 4951 is Hubble’s Wide Field Camera 3 (WFC3) is in the ultraviolet, infrared, and optical parts of the spectrum.

It is based on data acquired through six filters: color is generated by assigning a different hue to each monochrome image associated with an individual filter.

“The data used to create this image was taken by Hubble as part of a program to study how matter and energy move in nearby galaxies,” Hubble astronomers said. statement.

“Galaxy undergoes continuous cycles of star formation: gas within galaxies forms molecular clouds, which collapse to form new stars, and then the formed clouds are dispersed by powerful radiation and stellar winds in a process called feedback.”

“The remaining gas will form new clouds elsewhere,” the researchers added.

“This cycle of matter and energy transfer determines how quickly a galaxy forms stars and how quickly it exhausts its supply of gas — in other words, how the galaxy evolves throughout its life.”

“To understand this evolution, we need to know the nebulae, stars and star clusters in our galaxy, when they formed and what their past behavior is.”

“The Hubble Telescope has always excelled at measuring stellar populations, and its work tracking gas and star formation in galaxies including NGC 4951 is no exception,” the astronomers noted.

NGC 4951 is also classified as a Seyfert galaxy, a type of galaxy that has a so-called active galactic nucleus.

“The image gives a good glimpse into how energetic the galaxy is and some of the dynamic galactic activity that transports matter and energy throughout the galaxy: a glowing core surrounded by swirling arms, pink-hued star-forming regions, and thick dust,” the researchers said.

Source: www.sci.news

Hubble’s Discovery: Dwarf Spiral Galaxy Found in the Coma Constellation

Astronomers using the NASA/ESA Hubble Space Telescope have captured stunning images of the dwarf spiral galaxy IC 3476 in the constellation of Coma.


This Hubble image shows IC 3476, a dwarf spiral galaxy located 54 million light-years away in the constellation Coma. This image consists of observations made by Hubble's Altitude Survey Camera (ACS) in the near-infrared and optical parts of the spectrum. This is based on data obtained through his two filters. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / M. Sun.

IC 3476 It is located in the constellation Coma, approximately 54 million light-years from Earth.

This galaxy is first discovered It was proposed by German astronomer Arnold Schwassmann on November 22, 1900.

IC 3476, also known as IRAS 12301+1419 or LEDA 41608, is a member of the Virgo Cluster.

On the other hand, new Hubble images of the galaxy don't look quite as dramatic. The actual physical events occurring in IC 3476 are highly energetic.

“IC 3476 is undergoing a process known as ram pressure stripping, which promotes unusually high levels of star formation within the region of the galaxy itself,” the Hubble astronomers said.

“We tend to associate the letter 'ram' with the acronym RAM, which refers to random access memory in computing.”

“But ram pressure has a perfectly clear definition in physics: it is the pressure exerted on an object by the overall resistance of the fluid as it moves through some form of fluid.”

“If the entire galaxy is under ram pressure, then the galaxy is a 'celestial body', and the intergalactic medium or the intracluster medium (dust and gas that permeates the space between galaxies, in the latter case the intergalactic space) becomes a “celestial body”. fluid'. “

“Lamb pressure stripping occurs when gas is stripped from a galaxy by ram pressure,” the astronomers explained.

“Gas is absolutely key to star formation, so removing this gas could lead to reduced levels of star formation or even a complete cessation.”

“But the ram's pressure could also compress other parts of the galaxy, which could actually promote star formation.”

“This is what appears to be happening in IC 3476: no star formation appears to be occurring at the edges of the galaxy, which are bearing the brunt of the ram pressure separation, but in deeper regions of the galaxy, the rate of star formation slows down. It seems to be clearly above average. ”

Source: www.sci.news

Hubble’s Close-Up of UGC 8091

The Hubble team has released a close-up image of UGC 8091, a dwarf irregular galaxy that resembles a glittering festive snow globe.



This Hubble image shows UGC 8091, a dwarf irregular galaxy about 7 million light-years away in the constellation Virgo. The color images were created from separate exposures taken with Hubble’s Advanced Survey Camera (ACS) and Wide Field Camera 3 (WFC3). Image credits: NASA / ESA / Hubble / Yumi Choi, NSF’s NOIRLab / Caroline Gilbert, STScI / Julien Dalcanton, Center for Computational Astrophysics and University of Washington Flatiron Institute.

UGC 8091 It is located in the constellation Virgo, about 7 million light years away from Earth.

Also known as GR 8, DDO 155, LEDA 44491, or TC 257, this galaxy discovered It was discovered by astronomers at Lick Observatory in the 1940s and 1950s.

“Unlike other galaxies whose stars appear more regular, UGC 8091 is classified as an irregular galaxy,” said the Hubble astronomer.

“It’s not hard to see why. The stars that make up this cluster look more like a tangle of bright string lights than a galaxy.”

“While some irregular galaxies are thought to have become entangled due to intense internal activity, others are known to have formed through interactions with neighboring galaxies.”

“The result is a class of galaxies with a wide range of sizes and shapes, including these galaxies with diffuse and scattered stars.”

UGC 8091, also classified as a dwarf irregular galaxy, contains about 1 billion stars.

“That’s a huge amount of light, but not for a galaxy. Our Milky Way galaxy is thought to contain more than 100 billion stars, and other galaxies have trillions. “There could be as many stars as possible,” the astronomers said.

“Dwarf galaxies often orbit around larger galaxies, and their lower masses make them vulnerable to interference and consumption from larger neighbors, and in the process they destroy twisted dwarfs like UGC 8091. A galaxy is generated.”

“This type of galaxy is thought to have characteristics similar to the very old and distant galaxies seen in deep-field images.”

“Investigating the composition of dwarf galaxies and their stars, particularly their low metal content, could help uncover evolutionary links between these ancient galaxies and more modern galaxies like ours. We hope it will be helpful.”

To do this, researchers have carefully examined UGC 8091’s colorful stars.

“By using filters that restrict the light entering Hubble’s instruments to very specific wavelength ranges, we can pick out different features of galaxies,” the researchers said.

“These filtered images can be recombined to create a full-color image. An astonishing 12 filters are combined to produce this image, capturing light from the mid-UV to the red end of the visible spectrum. Contributing.”

“The blooming red spots represent light emitted by excited hydrogen molecules in hot, energetic stars formed in recent starbursts.”

“The other sparks in this image are a mixture of older stars.”

Source: www.sci.news

Hubble’s remarkable clarity reveals ring-spoke phenomenon

This photo of Saturn was taken by NASA’s Hubble Space Telescope on , when the ringed planet was about 850 million miles from Earth. Hubble’s razor-sharp vision reveals a phenomenon called ring spokes.

Saturn’s spokes are temporary features that rotate with the rings. Their ghostly appearance only lasts for two or three revolutions around Saturn. During the active period, newly formed spokes continually add to the pattern.

Credit: NASA, ESA, STScI, Amy Simon (NASA-GSFC)

Floating Dust rides a merry-go-round around a huge ring world

However Saturn

Its unusual-looking “cup-handle” feature was first noted by Galileo in 1610, but it took another 45 years before it was described by Christian Huygens as a disk surrounding Saturn. Ground-based telescopes were then able to identify only four unique concentric circles, labeled A, B, C, and D. It could not be identified until the 1980s. NASA

The two Voyager spacecraft will fly close to Saturn and photograph thousands of concentric ringlets. An even bigger surprise for Voyager scientists was the dark, radial, spoke-like pattern on the ring’s surface that moved back and forth as it orbited Saturn.

Over the past 30 years, hubble space telescope Voyager picked up where it left off. Hubble’s ultra-clear vision is the next best thing to being there. Hubble follows a “merry-go-round” of ring spokes every year. The black spokes are believed to be dust particles suspended by static electricity above the ring surface. They seem to vary richly depending on the seasons of Saturn’s seven years. And this may be related to changes in Saturn’s magnetic field, which is influenced by the solar wind.

This is an annotated version of the image above. Credit: NASA, ESA, STScI, Amy Simon (NASA-GSFC)

Hubble Space Telescope observes Saturn’s ‘spokes season’

This photo of Saturn was taken by NASA’s Hubble Space Telescope on , when the ringed planet was about 850 million miles from Earth. Hubble’s razor-sharp vision reveals a phenomenon called ring spokes.

Saturn’s spokes are temporary features that rotate with the rings. Their ghostly appearance only lasts for two or three revolutions around Saturn. During the active period, newly formed spokes continually add to the pattern.

In , NASA’s Voyager 2 took the first photo of a ring spoke. NASA’s cassini The orbiter also sighted spokes during its 13-year mission, which ended in 2017.

Hubble continues to observe Saturn every year as its spokes come and go. This cycle is captured by Hubble’s Outer Planet Atmospheric Legacy (OPAL) program, which was launched nearly a decade ago to annually monitor weather changes on all four gas giants.

Hubble’s clear images show that the frequency of the spokes’ appearance is seasonal, and they appeared in the OPAL data for the first time in , but only on the morning (left) side of the ring. Long-term monitoring has shown that both the number and contrast of spokes change with Saturn’s seasons. Saturn’s axis is tilted like Earth’s, and its seasons last about seven years.

“We’re heading towards the Saturn equinox, when the spokes are expected to be at their most active, and will remain active for several years to come,” said Amy Simon, OPAL program principal scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “We expect higher frequencies and darker spokes to appear.” .

This year, these ephemeral structures will appear on both sides of the Earth simultaneously, rotating around the giant world. Although it appears small compared to Saturn, its length and width can extend to more than Earth’s diameter.

“The leading theory is that the spokes are connected to Saturn’s strong magnetic field, and that the Sun is somehow interacting with that field to create the spokes,” Simon said. As Saturn approaches its vernal equinox, Saturn and its rings tilt less away from the Sun. In this configuration, the solar wind could hit Saturn’s massive magnetic field even harder, promoting spoke formation.

Planetary scientists believe that the electrostatic forces generated by this interaction cause the dust and ice to float above the ring, forming the spokes, but even after decades, no theory can fully predict the spokes. . Continued Hubble observations may ultimately help solve the mystery.

The Hubble Space Telescope is an international cooperative project between NASA and ESA. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts science operations for Hubble and Webb. STScI is operated for NASA by the Association of Universities for Astronomical Research in Washington, DC.

Source: scitechdaily.com

Hubble’s Holiday Globe Reveals 1 Billion Stars, Says NASA

In this festive Hubble Space Telescope image from NASA and ESA (European Space Agency), the galaxy UGC 8091 resembles a sparkling snow globe filled with a billion stars. Credits: ESA/Hubble, NASA, ESA, Yumi Choi (NSF’s NOIRLab), Karoline Gilbert (STScI), Julianne Dalcanton (Center for Computational Astrophysics/Flatiron Institute, Washington)

Dwarf irregular galaxies are born and dazzling stars are born

Hubble’s colorful snapshots show that the universe always seems to be in the holiday spirit. The dwarf irregular galaxy UGC 8091 is a rich example. A dizzying interplay of matter and energy bubbles up to create a dazzling blue, newborn star that looks like a celebratory string of lights. They are encased in a glowing cocoon of hot pink hydrogen gas. A galaxy is a collection of about 1 billion stars. That sounds like a lot, but it’s one-hundredth of the number of stars in our adult bodies. milky way Galaxy.

This little galaxy came late to the party. The early universe was filled with dwarf galaxies, which eventually merged to form the magnificent spiral galaxies that surround us today. Seven million light-years away, UGC 8091 has only recently begun to display its glittering tapestry.

The Hubble Space Telescope is an iconic symbol of space exploration, launched into orbit in 1990. Hubble revolutionized astronomy by providing unprecedented clarity and deep views of the universe, far beyond the distortions of Earth’s atmosphere. Credit: NASA

Hubble Space Telescope presents a starry sky for Christmas

The billion stars of galaxy UGC 8091 resemble sparkling snow globes during this festival. hubble space telescope Images from NASA and ESA (European Space Agency).

The dwarf galaxy is located in the constellation Virgo, about 7 million light-years from Earth. It is considered an “irregular galaxy” because it does not have a regular spiral or elliptical appearance. Rather, the stars that make up this cluster look more like a tangle of bright string lights than a galaxy.

Some irregular galaxies are entangled due to tumultuous internal activity, while others are formed by interactions with neighboring galaxies. The result is a class of galaxies of varying size and shape, including those whose stars are diffuse and scattered.

A combination of 12 camera filters produced this image using light from the mid-ultraviolet to the red end of the visible spectrum. The red spots are likely interstellar hydrogen molecules, excited by the light from the hot, energetic star and glowing. The other sparkles you see in this image are old star combinations. A diverse array of distant galaxies appears in the background, captured by Hubble’s sharp field of view.

The data used in this image was taken by Hubble’s Wide Field Camera 3 and Advanced Survey Camera from 2006 to 2021.

Among other things, the observing program involved in this image sought to investigate the role that dwarf galaxies billions of years ago played in reheating hydrogen that had cooled after the universe expanded. big bang.

Astronomers are also studying the composition of dwarf galaxies and their stars to uncover evolutionary connections between these ancient galaxies and more modern galaxies like ours.

The Hubble Space Telescope is an international cooperation project between the two countries. NASA And ESA. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts science operations for Hubble and Webb. STScI is operated for NASA by the Association of Universities for Astronomical Research in Washington, DC.

Source: scitechdaily.com