Wednesday, August 28, 2024

Zooming on Western Wall of The Carina Nebula | NOIRLab

Zooming on Western Wall of The Carina Nebula | NOIRLab

A 50-trillion-km (33-trillion-mile, or 5 light-year) long section of the western wall in the Carina Nebula, as observed with adaptive optics on the Gemini South telescope. This mountainous section of the nebula reveals a number of unusual structures including a long series of parallel ridges that could be produced by a magnetic field, a remarkable almost perfectly smooth wave, and fragments that appear to be in the process of being sheared off the cloud by a strong wind. There is also evidence for a jet of material ejected from a newly-formed star. The exquisite detail seen in the image is in part due to a technology known as adaptive optics, which resulted in a ten-fold improvement in the resolution of the research team’s observations.

The International Gemini Observatory consists of twin 8.1-meter diameter optical/infrared telescopes located on two of the best observing sites on the planet. The Gemini South telescope is located on a mountain in the Chilean Andes called Cerro Pachón, where very dry air and negligible cloud cover make this another prime telescope location. Both of the Gemini telescopes have been designed to excel in a wide variety of optical and infrared capabilities. By incorporating technologies such as laser guide star adaptive optics and multi-object spectroscopy, astronomers in the Gemini partnership explore the universe in unprecedented depth and detail.


International Gemini Observatory/NOIRLab/NSF/AURA, NASA, D. Stover/ESO/S. Brunier/Digitized Sky Survey 2

Image Processing: Patrick Hartigan (Rice University), Travis Rector (University of Alaska Anchorage), Mahdi Zamani & Davide de Martin.

Duration: 26 seconds 

Release Date: Oct. 5, 2020


#NASA #Astronomy #Space #Science #Nebulae #Nebula #CarinaNebula #NGC3372 #Carina #Constellation #MilkyWayGalaxy #Cosmos #Universe #GeminiSouthTelescope #AdaptiveOptics #GeminiObservatory #CerroPachón #Chile #NOIRLab #AURA #NSF #UnitedStates #STEM #Education #HD #Video

The Carina Nebula: Western Wall | Gemini South Telescope

The Carina Nebula: Western Wall | Gemini South Telescope


A 50-trillion-km (33-trillion-mile, or 5 light-year) long section of the western wall in the Carina Nebula, as observed with adaptive optics on the Gemini South telescope. This mountainous section of the nebula reveals a number of unusual structures including a long series of parallel ridges that could be produced by a magnetic field, a remarkable almost perfectly smooth wave, and fragments that appear to be in the process of being sheared off the cloud by a strong wind. There is also evidence for a jet of material ejected from a newly-formed star. The exquisite detail seen in the image is in part due to a technology known as adaptive optics, which resulted in a ten-fold improvement in the resolution of the research team’s observations.

The International Gemini Observatory consists of twin 8.1-meter diameter optical/infrared telescopes located on two of the best observing sites on the planet. The Gemini South telescope is located on a mountain in the Chilean Andes called Cerro Pachón, where very dry air and negligible cloud cover make this another prime telescope location. Both of the Gemini telescopes have been designed to excel in a wide variety of optical and infrared capabilities. By incorporating technologies such as laser guide star adaptive optics and multi-object spectroscopy, astronomers in the Gemini partnership explore the universe in unprecedented depth and detail.


Credit: International Gemini Observatory / NOIRLab / NSF / AURA / P. Hartigan (Rice University)

Image Processing: Patrick Hartigan (Rice University), Travis Rector (University of Alaska Anchorage), Mahdi Zamani & Davide de Martin

Release Date: Oct. 5, 2020


#NASA #Astronomy #Space #Science #Nebulae #Nebula #CarinaNebula #NGC3372 #Carina #Constellation #MilkyWayGalaxy #Cosmos #Universe #GeminiSouthTelescope #AdaptiveOptics #GeminiObservatory #CerroPachón #Chile #NOIRLab #AURA #NSF #UnitedStates #STEM #Education

Discovering Earth’s Third Global Energy Field | NASA Goddard

Discovering Earth’s Third Global Energy Field | NASA Goddard

High above the Earth’s North and South Poles, a steady stream of particles escapes from our atmosphere into space. Scientists call this mysterious outflow the “polar wind,” and for almost 60 years, spacecraft have been flying through it as scientists have theorized about its cause. The leading theory was that a planet-wide electric field was drawing those particles up into space. But this so-called ambipolar electric field, if it exists, is so weak that all attempts to measure it have failed—until now.

In 2022, scientists traveled to Svalbard, a small archipelago in Norway, to launch a rocket in an attempt to measure Earth’s ambipolar electric field for the first time. This was NASA’s Endurance rocketship mission. Here is its story.

To learn more, visit: https://science.nasa.gov/science-research/heliophysics/nasa-discovers-long-sought-global-electric-field-on-earth/


Video Credit: NASA's Goddard Space Flight Center

Producer: Lacey Young (MORI Associates), Miles Hatfield (MORI Associates), Rachel Lense (ADNET Systems)

Editor: Lacey Young (MORI Associates)

Writer: Miles Hatfield (MORI Associates), Glyn Collinson (NASA), Rachel Lense (ADNET Systems)

Talent: Glyn Collinson (NASA)

Animator: Krystofer Kim (Rothe Enterprises, Inc.), Wes Buchanan (ARES Corporation)

Duration: 4 minutes, 21 seconds

Release Date: Aug. 28, 2024


#NASA #Space #Astronomy #Science #Sun #Heliophysics #SolarWind #SolarSystem #Planet #Earth #ElectricFields #AmbipolarElectricField #PolarWind #Atmosphere #NorthPole #Svalbard #Norway #Norge #SoundingRockets #SubOrbitalRockets #EnduranceMission #STEM #Education #HD #Video

Dim, Starry Mini-Galaxy Andromeda VI in Pegasus | Hubble

Dim, Starry Mini-Galaxy Andromeda VI in Pegasus | Hubble

A glittering collection of stars shines against a background of much more distant galaxies in this view from NASA’s Hubble Space Telescope of the Pegasus Dwarf spheroidal galaxy, also known as Andromeda VI. 

The Andromeda galaxy (Messier 31) is the Milky Way galaxy’s closest grand spiral galaxy neighbor, and is host to at least 13 dwarf galaxies that orbit around it. The Pegasus Dwarf spheroidal galaxy, also called Andromeda VI, is one of these mini-galaxies. Dwarf spheroidal galaxies are the dimmest and least massive galaxies known. They tend to have elliptical shapes and relatively smooth distributions of stars. Dwarf spheroidal galaxies are usually devoid of gas and dominated by old and intermediate-age stars, although some have experienced small amounts of recent star formation. 

The Pegasus Dwarf Spheroidal galaxy was discovered in 1998 and has been characterized as having a small amount of heavy elements and little of the gas needed  to form another generation of stars―though more than many of the dwarf spheroidal galaxies within our Local Group of galaxies. Researchers suspect that Andromeda’s gravitational field may have stripped the star-forming gases from it, leaving a dearth of material to build more than a few generations of stars. In comparison, there are dwarf spheroidal companion galaxies of the Milky Way found at comparable distances that do contain intermediate-age stars. However, this could be because Andromeda is so massive and extended that its gravitational effects extend farther.

The jury is still out on how dwarf spheroidal galaxies form. Theories include collisions between galaxies that break off small fragments, the gravitational influence of larger galaxies on small disk-shaped dwarf galaxies, and processes associated with the birth of small systems among collections of dark matter. Andromeda and the Milky Way are the only galaxies close enough for astronomers to view these dim satellite galaxies, so clues to their formation will have to come from close neighbors like this one.

Hubble studied this galaxy as part of an examination of the entire Andromeda system of satellites in order to investigate such critical matters as dark matter, reionization, and the growth of galactic ecosystems across cosmic time.


Image Credit: NASA, ESA, and D. Weisz (University of California – Berkeley); Processing: Gladys Kober (NASA/Catholic University of America)

Release Date: Aug. 27, 2024


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxies #Galaxy #AndromedaVI #PegasusDwarfSpheroidalGalaxy #Pegasus #Constellation #AndromedaGalaxy #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

The Milky Way Galaxy | International Space Station

The Milky Way Galaxy | International Space Station

The Milky Way is pictured from the International Space Station near the top of this long-duration photograph with a camera programmed for high sensitivity.


Expedition 71 Updates:

https://blogs.nasa.gov/spacestation/

Expedition 71 Crew
Station Commander: Oleg Kononenko (Russia)
Roscosmos (Russia): Nikolai Chub, Alexander Grebenkin (Russia)
NASA: Tracy Dyson, Matthew Dominick, Mike Barrett, Jeanette Epps
NASA’s Boeing Crew Flight Test astronauts Suni Williams and Butch Wilmore

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada. The ISS has been the most politically complex space exploration program ever undertaken.

Learn more about the important research being operated on Station:

https://www.nasa.gov/iss-science 

For more information about STEM on Station:

https://www.nasa.gov/stemonstation

Science, Technology, Engineering, Math (STEM)


Image Credit: NASA's Johnson Space Center (JSC)

Image Date: Aug. 7, 2024


#NASA #Space #ISS #Science #Moon #Planet #Earth #SolarSystem #Galaxies #MilkyWayGalaxy #Astronauts #AstronautPhotography #UnitedStates #SpaceLaboratory #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition71 #InternationalCooperation #SpaceExploration #STEM #Education

Tuesday, August 27, 2024

Perseid Meteors over Inyo National Forest in California

Perseid Meteors over Inyo National Forest in California


Astrophotographer Preston Dyches: "Four meteors was the best I could do with the cloudy skies I encountered for the Perseids this year. By the time I woke up at 4 a.m. to grab the camera, it was overcast and starting to drizzle. And so it is."

"This was a location in Inyo National Forest called Westgard Pass, not far from the Ancient Bristlecone Pine Forest. There's some pinkish glow from the aurora at left, and a little greenish skyglow on the right, which is kind of neat. Andromeda Galaxy appears at the top just left of center."

"This is a blend of stacked, low-level-lit foreground exposures and a single sky background exposure. The three fainter meteors are composited, after being rotated into the correct position with respect to the Perseids radiant."

Learn more about the Perseid meteor shower here:

https://science.nasa.gov/solar-system/meteors-meteorites/perseids/

Inyo National Forest is a United States National Forest covering parts of the eastern Sierra Nevada of California and the White Mountains of California and Nevada. The forest hosts several superlatives, including Mount Whitney—the highest point in the contiguous United States;

Inyo National Forest: https://www.fs.usda.gov/inyo/

Image Credit: Preston Dyches

Location: Inyo National Forest - near Zurich, California, United States

Image Date: Aug. 12, 2024


#NASA #Space #Astronomy #Science #Earth #Planet #Atmosphere #Airglow #AuroraBorealis #Meteors #PerseidMeteors #Perseids #Meteor #Fireballs #Perseus #Constellation #Astrophotography #PrestonDyches #Astrophotographer #CitizenScience #SolarSystem #WestguardPass #InyoNationalForest #California #UnitedStates #STEM #Education

Solar Array ‘Wings’ for NASA's Jupiter-Bound Europa Clipper Spacecraft

Solar Array ‘Wings’ for NASA's Jupiter-Bound Europa Clipper Spacecraft

NASA’s Europa Clipper spacecraft is getting ready for launch, and its massive solar arrays were recently installed. These “wings” are so large because Jupiter receives only 3% to 4% of the sunlight Earth gets. Thus, the arrays need to be able to collect enough sunlight to power the spacecraft throughout its mission. 

With the arrays deployed, the spacecraft spans more than 100 feet (30.5 meters). This is nearly the distance from the Statue of Liberty’s toes to her head. The arrays will help the spacecraft make its 1.8 billion-mile (2.6 billion-kilometer) journey to Jupiter and power science instruments, electronics, heaters, and other subsystems during the years orbiting Jupiter and flying by the moon Europa. They also support six antennas that stick out perpendicularly from the panels. These antennas are for the Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) instrument. It will probe for water within and beneath Europa’s ice. 

Both wings were installed at NASA’s Kennedy Space Center in Florida in collaboration with the John Hopkins University Applied Physics Laboratory and Airbus Netherlands. The solar arrays are so large only one can be installed and tested at a time. Both will be folded and stowed for launch. They will fully deploy in space. 

Scientists believe the moon Europa has an ocean under its icy crust that may have conditions suitable for supporting life. Europa Clipper is expected to launch in October 2024 from Kennedy Space Center and arrive in the Jovian system in 2030.

Europa Clipper Mission website: 

https://europa.nasa.gov/


Credit: NASA/JPL-Caltech/KSC/APL/Airbus

Duration: 1 minute, 27 seconds

Release Date: Aug. 27, 2024

#NASA #Astronomy #Space #Science #Jupiter #Europa #Moon #Ocean #Astrobiology #Biosignatures #Habitability #Radiation #EuropaClipper #EuropaClipperSpacecraft #SolarArrays #SolarSystem #SpaceExploration #JHUAPL #GSFC #MSFC #JPL #Caltech #KSC #Spaceport #Florida #UnitedStates #STEM #Education #HD #Video

Europe's Jupiter Probe: Lunar-Earth Flyby Timelapse | ESA

Europe's Jupiter Probe: Lunar-Earth Flyby Timelapse | ESA

Between August 19-20, 2024, the European Space Agency’s Jupiter Icy Moons Explorer (JUICE) spacecraft successfully completed a lunar-Earth flyby with flight controllers guiding it first past the Moon, then Earth. The gravity of the two changed JUICE’s speed and direction, sending it on a shortcut to Jupiter via Venus.

The closest approach to the Moon was at 23:15 CEST on August 19, deflecting JUICE towards a closest approach to Earth just over 24 hours later at 23:56 CEST on August 20. In the hours before and after both close approaches, JUICE’s two monitoring cameras captured photos, giving us a unique ‘JUICE eye view’ of our home planet.

JUICE’s two monitoring cameras provide 1024 x 1024 pixel snapshots that can be processed in color. Their main purpose is to monitor the spacecraft’s various booms and antennas, especially during the challenging period after launch. The photos they captured of the Moon and Earth during the lunar-Earth flyby are a bonus.

Follow the JUICE Mission: www.esa.int/juice

Learn more:

https://www.esa.int/Science_Exploration/Space_Science/Juice/Juice_s_lunar-Earth_flyby_all_you_need_to_know

https://www.esa.int/Enabling_Support/Operations/Juice_why_s_it_taking_sooo_long


Video Credit: ESA - European Space Agency

Acknowledgements: Simeon Schmauß & Mark McCaughrean

Duration: 1 minute, 31 seconds

Release Date: Aug. 27, 2024


#NASA #ESA #Space #Astronomy #Science #Moon #Planets #Earth #Jupiter #Moons #Europa #Callisto #Ganymede #JUICE #JUICEMission #Spacecraft #LunarEarth #GravitationalAssists #SolarSystem #SpaceExploration #Europe #Infographics #STEM #Education #Timelapse #HD #Video

Panning across Nebula NGC 1333: Stellar Nursery in Perseus | Webb Telescope

Panning across Nebula NGC 1333: Stellar Nursery in Perseus | Webb Telescope


This new mosaic of images from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope showcases the nearby star-forming cluster, NGC 1333. The nebula is in the Perseus molecular cloud, and located approximately 960 light-years away.

Webb’s superb sensitivity allows astronomers to investigate young objects with extremely low masses. The faintest ‘stars’ in the picture are in fact newly born free-floating brown dwarfs with masses comparable to those of giant planets.

The center of the image presents a deep peek into the heart of the NGC 1333 cloud. Across the image, we see large patches of orange that represent gas glowing in the infrared. These so-called Herbig-Haro objects form when ionized material ejected from young stars collides with the surrounding cloud. They are hallmarks of a very active site of star formation.

Many of the young stars in this image are surrounded by discs of gas and dust. These may eventually produce planetary systems. On the right hand side of the image, we can glimpse the shadow of one of these discs oriented edge-on—two dark cones emanating from opposite sides, seen against a bright background.

Similarly to the young stars in this mosaic, our own Sun and planets formed inside a dusty molecular cloud, 4.6 billion years ago. Our Sun did not form in isolation but as part of a cluster. It was perhaps even more massive than NGC 1333. The cluster in the mosaic, only 1–3 million years old, presents us with an opportunity to study stars like our Sun, as well as brown dwarfs and free-floating planets, in their nascent stages.


Credit: ESA/Webb, NASA & CSA, A. Scholz, K. Muzic, A. Langeveld, R. Jayawardhana

Duration: 30 seconds

Release Date: Aug. 27, 2024


#NASA #Space #Astronomy #Science #Stars #Nebula #DarkNebula #NGC1333 #StellarNursery #HerbigHaroObjects #Perseus #Constellation  #Cosmos #Universe #JWST #Infrared #SpaceTelescopes #ESA #CSA #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Nebula NGC 1333: Peeking into The Perseus Molecular Cloud | Webb Telescope

Nebula NGC 1333: Peeking into The Perseus Molecular Cloud | Webb Telescope

This new mosaic of images from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope showcases the nearby star-forming cluster, NGC 1333. The nebula is in the Perseus molecular cloud, and located approximately 960 light-years away.

Webb’s superb sensitivity allows astronomers to investigate young objects with extremely low masses. The faintest ‘stars’ in the picture are in fact newly born free-floating brown dwarfs with masses comparable to those of giant planets.

The center of the image presents a deep peek into the heart of the NGC 1333 cloud. Across the image, we see large patches of orange that represent gas glowing in the infrared. These so-called Herbig-Haro objects form when ionized material ejected from young stars collides with the surrounding cloud. They are hallmarks of a very active site of star formation.

Many of the young stars in this image are surrounded by discs of gas and dust. These may eventually produce planetary systems. On the right hand side of the image, we can glimpse the shadow of one of these discs oriented edge-on—two dark cones emanating from opposite sides, seen against a bright background.

Similarly to the young stars in this mosaic, our own Sun and planets formed inside a dusty molecular cloud, 4.6 billion years ago. Our Sun did not form in isolation but as part of a cluster. It was perhaps even more massive than NGC 1333. The cluster in the mosaic, only 1–3 million years old, presents us with an opportunity to study stars like our Sun, as well as brown dwarfs and free-floating planets, in their nascent stages.

The same cluster was featured as the 33rd anniversary image of the NASA/ESA Hubble Space Telescope in April 2023. Hubble’s image just scratched the surface of this region, because clouds of dust obscure much of the star formation process. Observing with a larger aperture and in the infrared part of the spectrum, Webb is capable of peering through the dusty veil to reveal newborn stars, brown dwarfs and planetary mass objects. 

Image Description: A nebula made up of cloudy gas and dust in the form of soft and wispy clouds and, in the center, thin and highly detailed layers pressed close together. Large, bright stars surrounded by six long points of light are dotted over the image, as well as small, point-like stars embedded in the clouds. The clouds are lit up in blue close to the stars; orange colors show clouds that glow in infrared light.


Credit: ESA/Webb, NASA & CSA, A. Scholz, K. Muzic, A. Langeveld, R. Jayawardhana

Release Date: Aug. 27, 2024


#NASA #Space #Astronomy #Science #Stars #Nebula #DarkNebula #NGC1333 #StellarNursery #HerbigHaroObjects #Perseus #Constellation  #Cosmos #Universe #JWST #Infrared #SpaceTelescopes #ESA #CSA #GSFC #STScI #UnitedStates #STEM #Education

The Sharpest Ground Observations for Black Holes Ever | ESO Chasing Starlight

The Sharpest Ground Observations for Black Holes Ever | ESO Chasing Starlight


The images of black holes released by the Event Horizon Telescope (EHT) Collaboration in 2019 and 2022 were the sharpest images of the cosmos ever obtained from Earth. They were captured using a virtual telescope the size of our planet. If we are already using the largest ground-based telescope we possibly can, are we able to take even sharper black hole images? 

In this episode of Chasing Starlight, European Southern Observatory astronomer Suzanna Randall reveals how a pilot experiment using telescopes that are part of the EHT was able to obtain the highest-resolution observations ever made from the ground, and what that means for future black hole images.


Credit: European Southern Observatory (ESO)

Directed by: L. Calçada, M. Wallner

Hosted by: S. Randall

Written by: L. Spillman

Videography: A. Tsaousis

Animations & footage: ESO, M. Kornmesser, L. Calçada, ALMA (ESO/NAOJ/NRAO)/Benisty et al., ALMA (ESO/NAOJ/NRAO)/M. Maercker et al.; N. R. Fuller/NSF

Scientific consultant: P. Amico, J. C. Munoz-Mateos

Acknowledgement: Eduardo Ros

Duration: 8 minutes

Release Date: Aug. 27, 2024


#NASA #NSF #ESO #Space #Astronomy #Science #BlackHoles #Galaxies #MilkyWayGalaxy #Astrophysics #Cosmos #Universe #EventHorizonTelescope #EHT #VLT #Telescope #Chile #ChasingStarlight #STEM #Education #HD #Video

The Large Magellanic Cloud Galaxy: A Close Galactic Neighbor

The Large Magellanic Cloud Galaxy: Our Close Galactic Neighbor

This image transports you to the most advanced visible-light astronomical observatory in the world—the Very Large Telescope (VLT), located at the European Southern Observatory’s Paranal Observatory in Chile. With an estimated 30 billion stars, the Large Magellanic Cloud, at over 160,000 light years away, is visible at the center of the frame, while Canopus, the brightest star in the constellation Carina (The Keel), watches over the starry scene to the upper right. At 2,635 meters above sea level in the Atacama Desert of Chile, ESO’s Paranal Observatory is one of the best astronomical observing sites in the world. It is the flagship facility for European ground-based astronomy. It hosts several world-class telescopes; among them are the Very Large Telescope and the Visible and Infrared Survey Telescope for Astronomy (VISTA).

The shadowy figure gazing at the dark skies is photographer Babak Tafreshi, as captured by his fellow ESO Photo Ambassador Petr Horálek. For a moment, place yourself in Babak’s—or indeed Petr’s —shoes. The site is silent, dark, still. You stare up at the pristine Chilean night sky, which, with its extremely low levels of light pollution and water vapor, offers spectacular nighttime scenery to delight any astrophotographer or stargazer. With your trusty camera on hand, a night of amazing photo opportunities lies ahead; you anticipate spending clear hour after clear hour documenting the heavens, with no fear of cloudy weather appearing, uninvited, to spoil the view.


Credit: P. Horálek/ESO

Release Date: June 27, 2016

#NASA #Astronomy #Space #Science #Planet #Earth #SolarSystem #Star #Canopus #MilkWayGalaxy #LargeMagellanicCloud #DwarfGalaxy #Constellations #Dorado #Mensa #Cosmos #Universe #Telescope #VLT #ParanalObservatory #AtacamaDesert #Chile #Europe #Astrophotographers #BabakTafreshi #PetrHorálek #Astrophotography #STEM #Education

Monday, August 26, 2024

Eye on The Cosmos: 25 Years of Discoveries | NASA's Chandra X-ray Observatory

Eye on The Cosmos: 25 Years of Discoveries NASA's Chandra X-ray Observatory

On July 23, 1999, NASA’s Chandra X-ray Observatory was launched aboard space shuttle Columbia. Its “First Light” operation on Aug. 26, 1999, delivered unprecedented X-ray images of the supernova remnant Cassiopeia A. Over the 25 years that followed, Chandra has delivered nearly 25,000 observations of black holes, galaxy clusters, and other high-energy cosmic phenomena – and this hardy observatory is still going strong. Founding Chandra project scientist Martin Weisskopf and other key Chandra team members at NASA’s Marshall Space Flight Center look back at the road to launch, Chandra’s landmark scientific achievements, and the down-to-Earth formula for its success. 


Video Credits: NASA 

Written by Rick Smith & Michael Allen 

Produced & Narrated by Joe Kuner (NASA)

Duration: 7 minutes, 50 seconds

Release Date: Aug. 26, 2024


#NASA #Astronomy #Space #Science #Stars #BlackHoles #CasA #SupernovaRemnant #Galaxies #GalaxyClusters #Cosmos #Universe #NASAChandra #Xray #SpaceTelescope #JPL #GSFC #UnitedStates #STEM #Education #History #HD #Video

Cosmic Evolution: Early Galaxies—"Not So Massive After All" | Webb Telescope

Cosmic Evolution: Early Galaxies—'Not So Massive After All' | Webb Telescope

This image shows a small portion of the field observed by NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) for the Cosmic Evolution Early Release Science (CEERS) survey. It is filled with galaxies. The light from some of them has traveled for over 13 billion years to reach the telescope. Hundreds of small galaxies against the black background of space. Several white spiral galaxies are near image center. Most of the galaxies are various shades of orange and red, and many are too tiny to discern a shape. A handful of foreground stars show Webb's six diffraction spikes.

There were galaxies that appeared to have grown so massive, so quickly, that simulations could not account for them. However, a new study finds that a great percentage of those early galaxies are in fact much less massive than they first appeared. Black holes in those galaxies make them appear much brighter and bigger than they really were.

It was called a crisis in cosmology. However, now astronomers can explain a number of surprising recent discoveries. Not long after the James Webb Space Telescope began science operations in July 2022, headlines proclaimed that observations of distant galaxies were “breaking theories of cosmic evolution.” Astronomers had found galaxies that appeared much brighter than expected. If all of that light came from stars, then those galaxies would have formed so many stars, so quickly, that the leading theory for the universe’s formation and evolution could not explain them.

New research finds that several of those early galaxies are in fact much less massive than they first appeared. Much of their light came, not from stars, but from a hot accretion disk surrounding a supermassive black hole.

When astronomers gained their first glimpses of galaxies in the early universe from NASA’s James Webb Space Telescope, they were expecting to find galactic pipsqueaks, but instead they found what appeared to be a bevy of Olympic 'bodybuilders'. Galaxies appeared to have grown so massive, so quickly, that simulations could not account for them. Researchers suggested this meant that something might be wrong with the theory that explains what the universe is made of and how it has evolved since the Big Bang, known as the standard model of cosmology.

According to a new study in the Astronomical Journal led by University of Texas at Austin graduate student Katherine Chworowsky, a significant portion of those early galaxies are in fact much less massive than they first appeared. Black holes in these galaxies make them appear much brighter and larger than they really were.

"Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4–8 from CEERS"

“We are still seeing more galaxies than predicted, although none of them are so massive that they ‘break’ the universe,” Chworowsky said.

The evidence was provided by Webb’s Cosmic Evolution Early Release Science (CEERS) Survey, led by Steven Finkelstein, a professor of astronomy at UT Austin and study co-author.

Black Holes Add to Brightness

According to this latest study, the galaxies that appeared overly massive likely host black holes rapidly consuming gas. Friction in the fast-moving gas emits heat and light, making these galaxies much brighter than they would be if that light emanated just from stars. This extra light can make it appear that the galaxies contain many more stars, and hence are more massive, than we would otherwise estimate. When scientists remove these galaxies, dubbed “little red dots” (based on their red color and small size), from the analysis, the remaining early galaxies are not too massive to fit within predictions of the standard model.

“So, the bottom line is there is no crisis in terms of the standard model of cosmology,” Finkelstein said. “Any time you have a theory that has stood the test of time for so long, you have to have overwhelming evidence to really throw it out. And that’s simply not the case.”

Efficient Star Factories

Although they have settled the main dilemma, a less thorny problem remains. There are still roughly twice as many massive galaxies in Webb’s data of the early universe than expected from the standard model. One possible reason might be that stars formed more quickly in the early universe than they do today. 

“Maybe in the early universe, galaxies were better at turning gas into stars,” Chworowsky said.

Star formation happens when hot gas cools enough to succumb to gravity and condense into one or more stars. But as the gas contracts, it heats up, generating outward pressure. In our region of the universe, the balance of these opposing forces tends to make the star formation process very slow. But perhaps, according to some theories, because the early universe was denser than today, it was harder to blow gas out during star formation, allowing the process to go faster.

More Evidence of Black Holes

Concurrently, astronomers have been analyzing the spectra of "little red dots" discovered with Webb, with researchers in both the CEERS team and others finding evidence of fast-moving hydrogen gas, a signature of black hole accretion disks. This supports the idea that at least part of the light coming from these compact, red objects comes from gas swirling around black holes, rather than stars—reinforcing Chworowsky and their team’s conclusion that they are probably not as massive as astronomers initially thought. However, further observations of these intriguing objects are incoming, and should help solve the puzzle about how much light comes from stars versus gas around black holes.

Often in science, when you answer one question, this leads to new questions. While Chworowsky and their colleagues have shown that the standard model of cosmology likely is not broken, their work points to the need for new ideas in star formation.

“And so there is still that sense of intrigue,” Chworowsky said. “Not everything is fully understood. That’s what makes doing this kind of science fun, because it’d be a terribly boring field if one paper figured everything out, or there were no more questions to answer.”

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).


Image Credit: NASA, ESA, CSA, Steve Finkelstein (UT Austin)

Release Date: Aug. 26, 2024


#NASA #Space #Astronomy #Science #Stars #Galaxies #BlackHoles #AccretionDiscs #CEERSSurvey #DeepField #Boötes #Constellation #BigBangModel #Cosmology #Astrophysics #Cosmos #Universe #JWST #Infrared #SpaceTelescope #ESA #CSA #GSFC #STScI #UnitedStates #STEM #Education

Listen to The Universe's Past | NASA Chandra X-ray Sonifications

Listen to The Universe's Past | NASA Chandra X-ray Sonifications

A quarter of a century ago, the “First Light” images from NASA’s Chandra X-ray Observatory were released to the public. This introduction to the world of Chandra’s high resolution X-ray imaging capabilities included an unprecedented view of Cassiopeia A, the remains of an exploded star located about 11,000 light-years from Earth. Over the years, Chandra’s views of Cassiopeia A are among the telescope’s best-known images.

To mark the anniversary of this milestone and celebrate what discoveries are to come, new sonifications of three images—including Cassiopeia A (Cas A)—are being released. Sonification is a process that translates astronomical data into sound, similar to how these digital data are more routinely turned into images. This translation process preserves the science of the data from its original digital state but provides an alternative pathway to experiencing the data.

This sonification of Cas A features data from Chandra as well as NASA’s James Webb and Hubble Space Telescopes. The scan starts at the neutron star at the center of the remnant, marked by a triangle sound, and moves outward. X-ray data from Chandra are mapped to modified piano sounds, while infrared data from JWST, which detects warmed dust embedded in the hot gas, have been assigned to various string and brass instruments. Stars that Hubble detects are played with small cymbals.

30 Doradus is one of the largest and brightest regions of star formation close to the Milky Way. This sonification again combines X-rays from Chandra with infrared data from JWST. X-rays from Chandra, which reveal gas that has been superheated by shock waves generated by the winds from massive stars, are heard as airy synthesizer sounds. Meanwhile, JWST’s infrared data show cooler gas that provides the raw ingredients for future stars.

The final member of this new sonification triumvirate is the large spiral galaxy called NGC 6872 that has two elongated arms stretching to the upper right and lower left. Just to the upper left of NGC 6872 appears another smaller spiral galaxy. These two galaxies, each of which likely has a supermassive black hole at the center, are being drawn toward one another. Chandra’s X-rays, represented in sound by a wind-like sound, show multimillion-degree gas that permeates the galaxies. Meanwhile Hubble data reveal the galaxy’s spiral arms and background stars as low drone sounds and soft plucks and cymbals.


Video Credit: NASA's Chandra X-ray Observatory

Duration: 3 minutes, 25 seconds

Release Date: Aug. 26, 2024


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China-France SVOM Astronomy Satellite Speeds Gamma-ray Burst Detections

China-France SVOM Astronomy Satellite Speeds Gamma-ray Burst Detections

How can we quickly capture and study gamma-ray bursts? Wei Jianyan, Chinese principal investigator of Space Variable Objects Monitor (SVOM), said the satellite jointly developed by China and France has a response time of about five minutes, breaking the previous record of about 20 minutes. The 930kg (2,050-pound) satellite took hundreds of scientists and engineers nearly two decades to develop. It orbits Earth at 625km (450 miles) above the ground to accurately measure the location and energy of distant, violent explosions known as gamma-ray bursts. The SVOM satellite was successfully launched from the Xichang Satellite Launch Center in southwest China's Sichuan Province on June 22, 2024.

China's primary responsibilities for the mission were launch, satellite and operations. It shared responsibility with France for the design and construction of the instruments and ground segment.

The French contribution was developed in partnership with research laboratories at the IRFU research institute at CEA, the French atomic energy and alternative energies commission, and at INSU, the national institute of universe science, and IN2P3, the national institute of nuclear and particle physics, both attached to the national scientific research centre CNRS.

It represents a milestone in international space collaboration. Developed jointly by Chinese and French scientists over nearly two decades, SVOM carries two French and two Chinese scientific payloads designed to detect distant space phenomena known as gamma-ray bursts (GRBs). Researchers from both countries believe the SVOM monitoring satellite will help advance their investigations in many fields of astrophysics, including the origins of the universe and of elements on Earth.

"The gamma-ray burst is a tool to observe the early universe. We can observe maybe the first stars. And this is very interesting because this is the only way to do that, said Bertrand Cordier, French lead researcher of the SVOM project.

Wei Jianyan, the Chinese principal investigator of SVOM, said the satellite can help researchers expand their collection of observed astronomical phenomena and better understand the Earth.

"We can discover some special types of gamma-ray bursts, as well as the relatively rare ones. We have already known some common types, as it has been studied for two or three decades. But there are still rare ones, high redshift gamma ray bursts, for example. And very interestingly, it helps us understand where some of the elements on earth come from, including gold and silver that we often wear," he said.

Researchers said the two countries' cooperation will lead to great progress in their research.

"We use China's BeiDou satellite system. If we on the ground see a very interesting target in space, we can tell our satellite to point at it in a matter of minutes. As far as I know, this process used to take 20 minutes in international practice. With the BeiDou system, we can respond in a few minutes, and that's a big step forward. This can be effective in detecting swift events," said Wei.

The BeiDou satellite navigation system is a space-based radio navigation service owned and operated by the China National Space Administration (CNSA).

"China, as you said, has developed several missions that are looking to gamma-ray burst, but we are working together. I'm also involved in the Einstein commission, and the idea is to have a very powerful system with many satellites; the idea is to have a way to work together in order to enhance the scientific study," said Cordier.

Both sides approved the SVOM mission in 2006. It is hoped it will run longer than the satellite's designed lifespan of 5 years into the next decade.

Learn more about the SVOM Mission: 

https://svom.cnes.fr/en/SVOM/index.htm


Video Credit: China Global Television Network (CGTN)

Duration: 1 minute, 51 seconds

Release Date: Aug. 26, 2024


#NASA #CNSA #Space #Astronomy #Science #China #中国 #SVOM #GammaRays #GammaRayBursts #GRB #Astrophysics #Cosmos #Universe #SpaceTechnology #SpaceExploration #InternationalCooperation #France #CNES #STEM #Education #History #HD #Video