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Hubble Sees a Celestial Cannonball
Hubble Sees a Celestial Cannonball
The spiral galaxy in this NASA/ESA Hubble Space Telescope image is IC 3225. It looks remarkably as if it was launched from a cannon, speeding through space like a comet with a tail of gas streaming from its disk behind it. The scenes that galaxies appear in from Earth’s point of view are fascinating; many seem to hang calmly in the emptiness of space as if hung from a string, while others star in much more dynamic situations!
Appearances can be deceiving with objects so far from Earth — IC 3225 itself is about 100 million light-years away — but the galaxy’s location suggests some causes for this active scene, because IC 3225 is one of over 1,300 members of the Virgo galaxy cluster. The density of galaxies in the Virgo cluster creates a rich field of hot gas between them, called ‘intracluster medium’, while the cluster’s extreme mass has its galaxies careening around its center in some very fast orbits. Ramming through the thick intracluster medium, especially close to the cluster’s center, places enormous ‘ram pressure’ on the moving galaxies that strips gas out of them as they go.
As a galaxy moves through space, the gas and dust that make up the intracluster medium create resistance to the galaxy’s movement, exerting pressure on the galaxy. This pressure, called ram pressure, can strip a galaxy of its star-forming gas and dust, reducing or even stopping the creation of new stars. Conversely, ram pressure can also cause other parts of the galaxy to compress, which can boost star formation. IC 3225 is not so close to the cluster core right now, but astronomers have deduced that it has undergone ram pressure stripping in the past. The galaxy looks compressed on one side, with noticeably more star formation on that leading edge (bottom-left), while the opposite end is stretched out of shape (upper-right). Being in such a crowded field, a close call with another galaxy may also have tugged on IC 3225 and created this shape. The sight of this distorted galaxy is a reminder of the incredible forces at work on astronomical scales, which can move and reshape entire galaxies!
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The Milky Way’s Supermassive Black Hole Photo Might Need a Retake
Remember that amazing “first image” of Sagittarius A* (Sgr A) black hole at the heart of the Milky Way? Well, it may not be completely accurate, according to researchers at the National Astronomical Observatory of Japan (NAOJ). Instead, the accretion disk around Sgr A* may be more elongated, rather than the circular shape we first saw in 2022.
Scientists at NAOJ applied different analysis methods to the data of Sgr A* first taken by the Event Horizon Telescope (EHT) team. The EHT data came from a network of eight ground-based radio telescopes. The original analysis showed a bright ring structure surrounding a dark central region. The re-analysis resulting in a different shape implies something about the motions and distribution of matter in the disk.
In fairness to both teams, radio interferometry data is notoriously complex to analyze. According to NAOJ astronomer Miyoshi Mikato, the rounded appearance may be due to the way the image was constructed. “We hypothesize that the ring image resulted from errors during EHT’s imaging analysis and that part of it was an artifact, rather than the actual astronomical structure,” Miyoshi suggested.
This is the first image of Sgr A*, the supermassive black hole at the center of our galaxy. A reanalysis of EHT data by NAOJ scientists suggests its accretion disk may be more elongated than circular. Credit: EHT Explaining the Black Hole AppearanceSo, what does Sgr A* look like in the NAOJ re-analysis? “Our image is slightly elongated in the east-west direction, and the eastern half is brighter than the western half,” said Miyoshi. “We think this appearance means the accretion disk surrounding the black hole is rotating at about 60 percent of the speed of light.”
The accretion disk is filled with superheated material “circling the drain” as it were. It’s funneling into the 4-million-solar-mass black hole. As it cycles through the accretion disk, friction and the action of magnetic fields heat the material. That causes it to glow, mostly in x-rays and visible light as well as giving off radio emissions.
Various factors also influence the shape of the accretion disk, including the spin of the black hole itself. In addition, the accretion rate (that is, how much material falls into the disk), as well as the angular momentum of the material, all affect the shape. The gravitational pull of the black hole also distorts our view of the accretion disk. That sort of “funhouse mirror” distortion makes it incredibly difficult to image. As it turns out, either view of the disk’s actual shape—the original EHT “circular” view or the NAOJ elongated view—could be accurate.
So, Why the Different Views of the Black Hole?How did the teams come up with two slightly different views of Sgr A* using the same data? “No telescope can capture an astronomical image perfectly,” Miyoshi pointed out. For the EHT observations, it turns out that interferometric data from the widely linked telescopes can have gaps. During data analysis, scientists have to use special techniques to construct a complete image. That’s what the EHT team did, resulting in the “round black hole” image.
Miyoshi’s team published a paper describing their results. In it, they propose that the “ring” structure in the 2022 image released by EHT is an artifact caused by the bumpy point-spread function (PSF) of the EHT data. The PSF describes how an imaging system deals with a point source in the region it’s looking at. It helps give a measure of the amount of blurring that occurs because of imperfections in the optics (or in this case, the gaps in the interferometric data). In other words, it had problems with “filling” in the gaps.
The NAOJ team reanalyzed the data and used a different mapping method to smooth over the gaps in the data. That resulted in an elongated shape for the Sgr A* accretion disk. One-half of the disk is brighter and they suggest it’s due to a Doppler boost as the disk rotates rapidly. They suggest that the newly analyzed data and elongated image shows a portion of the disk that lies a few Schwarzschild radii away from the black hole, rotating extremely fast, and viewed from an angle of 40°-45°.
What’s Next?This reanalysis should help contribute to a better understanding of what the Sgr A* accretion disk actually looks like. The EHT study of Sgr A* resulting in the 2022 image release was the first detailed attempt to map the region around the black hole. The EHT consortium is working on improvements to produce better and more detailed interferometry images of this and other black holes. Eventually, that should result in more accurate views. Follow-up studies should help fill in any gaps in the observations of the accretion disk. In addition, detailed studies of the near environment around the black hole should give more clues to the black hole hidden inside the disk. I
For More InformationFirst Picture of Milky Way Black Hole ‘May Not Be Accurate’
An Independent Hybrid Imaging of Sgr A* from the Data in EHT 2017 Observations
The post The Milky Way’s Supermassive Black Hole Photo Might Need a Retake appeared first on Universe Today.
Autumn Leaves – Call for Volunteers
3 min read
Autumn Leaves – Call for VolunteersThe Global Learning and Observations to Benefit the Environment (GLOBE) Program is calling on volunteers of all ages to help students and citizen scientists document seasonal change through leaf color and land cover. The data collection event will support students across North America, Latin America, Central America, and Europe, who are working together to document the seasonal changes taking place from September through December – see Figure. The observations will also provide vital data for GLOBE students creating student research projects for the GLOBE 2025 International Virtual Science Symposium (IVSS). The project is part of GLOBE’s Intensive Observation Period (IOP), which collects data during a focused period to assess how climate change is unfolding in different regions of the world.
Figure. Locations Green-Down observations being entered into the GLOBE database. Figure credit: GLOBE
Green down is the seasonal change when leaves change from green to brown and then fall to the ground. During green-down data collection, volunteers take regular, daily photos of trees to document the transition in color. Regular observations of land cover and tree height capture the broader changes happening around the tree.
By gathering this data, you can provide important information about when a single tree changes ahead of or behind the others in your region. When this data is paired with satellite observations, researchers gain a much stronger picture of how seasonal and climate variations impact the life cycles of plants and animals.
The GLOBE European Phenology Campaign has created materials to assist educators in these efforts. This includes a series of YouTube videos that volunteers can use to select a tree for the phenology project, estimate tree height, and assess land cover. In addition, volunteers can refer to the green-down protocol for guidance at the beginning of the survey. Educators can learn more about the importance of the green-down study by registering as a GLOBE Educator at the GLOBE “Create an Account” website.
GLOBE students have been collecting seasonal variability in plant and animal data for decades. This work will augment global databases to help students, educators, and scientists around the world study climate change.
These observations are taking place around the world. This IOP is being conducted in conjunction with the GLOBE North America Phenology Campaign and the European Phenology Campaign, which focus on monitoring and reporting of cycles in plants and animals to help validate the timing of changes in growing season and habitat. The work is also being conducted in conjunction with the Trees Within LAC Campaign, which is collecting information about tree species and their dynamics over time.
Share Details Last Updated Oct 25, 2024 Related Terms
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Kites in the Classroom: Training Teachers to Conduct Remote Sensing Missions
3 min read
Kites in the Classroom: Training Teachers to Conduct Remote Sensing MissionsThe NASA Science Activation program’s AEROKATS and ROVER Education Network (AREN), led by Wayne Regional Educational Service Agency (RESA) in Wayne County, MI, provides learners with hands-on opportunities to engage with science instruments & NASA technologies and practices in authentic, experiential learning environments. On July 25, 2024, the AREN team held a four-day virtual workshop: “Using Kites and Sensors to Collect Local Data for Science with the NASA AREN Project”. During this workshop, the team welcomed 35 K-12 educators and Science, Technology, Education, & Mathematics (STEM) enthusiasts from across the country to learn about the AREN project and how to safely conduct missions to gather remote sensing data in their classrooms.
Teachers were trained to use an AeroPod, an aerodynamically stabilized platform suspended from a kite line, in order to collect aerial imagery and introduce their students to topics like resolution, pixels, temporal and seasonal changes to landscape, and image classification of land cover types. Educators were also familiarized with safe operation practices borrowed from broader NASA mission procedures to ensure students in the field can enjoy experiential education safely. The AREN team will also meet with workshop participants during follow-up sessions to highlight next steps and new instrumentation that can be used to gather different data, help broaden the educators depth of understanding, and increase successful implementation in the classroom.
“This session has been very helpful and informative of the program and the possible investigations that we can conduct. The fact that it can connect hands on experiments, data analysis, and draw conclusions from the process is going to be a fantastic learning experience.” ~AREN Workshop Participant
The AREN project continually strives to provide low cost, user-friendly opportunities to engage in hands-on experiential education and increase scientific literacy. The versatility of the NASA patented AeroPod platform allows learners to investigate scientific questions that are meaningful to their community and local environment. Learn more about AREN and how to implement AREN technologies in the classroom: https://science.nasa.gov/sciact-team/resa/
AREN is supported by NASA under NASA Science Mission Directorate Science Education Cooperative Agreement Notice (CAN) Solicitation NNH15ZDA004C Award Number NNX16AB95A and is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn
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Paxi explores wind
English Paxi explores wind
Learn about wind, what causes it and how and why we study it in the latest Paxi adventure
Spanish Paxi explora el viento
Aprende sobre el viento, qué lo provoca y cómo y por qué lo estudiamos en la última aventura de Paxi.
Romanian Paxi explorează vântul
Aflați despre vânt, ce îl provoacă și cum și de ce îl studiem în cea mai recentă aventură Paxi.
Portuguese Paxi explora o vento
Aprende sobre o vento, o que o provoca e como e porquê o estudamos na mais recente aventura Paxi.
Polish Paxi bada wiatr
Dowiedz się więcej o wietrze, jego przyczynach oraz o tym, jak i dlaczego go badamy w najnowszej przygodzie Paxi.
Norwegian Paxi utforsker vind
Lær mer om vind, hva som forårsaker den og hvordan og hvorfor vi studerer den i det nyeste Paxi-eventyret.
Italian Paxi osserva il vento
Imparate a conoscere il vento, le sue cause e come e perché lo studiamo nell'ultima avventura di Paxi.
Greek Ο Πάξι εξερευνά τον άνεμο
Μάθετε για τον άνεμο, τι τον προκαλεί και πώς και γιατί τον μελετάμε στην τελευταία περιπέτεια του Paxi.
German Paxi erforscht den Wind
Erfahren Sie im neuesten Paxi-Abenteuer mehr über Wind, seine Ursachen und wie und warum wir ihn untersuchen.
French Paxi te fait découvrir le vent
Découvrez le vent, ce qui le provoque et comment et pourquoi nous l'étudions dans la dernière aventure de Paxi.
Swedish Paxi utforskar vind
Lär dig mer om vind, vad som orsakar den och hur och varför vi studerar den i det senaste Paxi-äventyret.
Dutch Paxi onderzoekt wind
Leer meer over wind, wat het veroorzaakt en hoe en waarom we het bestuderen in het nieuwste Paxi-avontuur.
Danish Paxi udforsker vind
Lær om vind, hvad der forårsager den, og hvordan og hvorfor vi studerer den i det seneste Paxi-eventyr.
Czech Paxi zkoumá vítr
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Finnish Paxi tutkii tuulta
Tutustu tuuleen, sen syihin sekä siihen, miten ja miksi sitä tutkitaan uusimmassa Paxi-seikkailussa.
Estonian Paxi avastab tuult
Tutvu tuulega, selle põhjustega ning sellega, kuidas ja miks me seda uurime Paxi viimases seikluses.
High-Altitude ER-2 Flights Get Down-to-Earth Data
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Francisco Rodriguez (aircraft mechanic) services liquid oxygen or LOX on the ER-2 during the Geological Earth Mapping Experiment (GEMx) research project. Experts like Rodriguez sustain a high standard of safety on airborne science aircraft like the ER-2 and science missions like GEMx. The ER-2 is based out of NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Steve Freeman
Operating at altitudes above 99% of the Earth’s atmosphere, NASA’s ER-2 aircraft is the agency’s highest-flying airborne science platform. With its unique ability to observe from as high as 65,000 feet, the ER-2 aircraft is often a platform for Earth science that facilitates new and crucial information about our planet, especially when the plane is part of collaborative and multidisciplinary projects.
“We’re deploying instruments and people everywhere from dry lakebeds in the desert to coastal oceans and from the stratosphere to marine layer clouds just above the surface,” said Kirk Knobelspiesse, an atmospheric scientist at NASA’s Goddard Space Flight Center. “We live on a changing planet, and it is through collaborative projects that we can observe and understand those changes.”
One mission that recently benefitted from the ER-2’s unique capabilities is the Plankton, Aerosol, Cloud, ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) project. The PACE-PAX mission uses the ER-2’s capabilities to confirm data collected from the PACE satellite, which launched in February 2024.
The PACE observatory is making novel measurements of the ocean, atmosphere, and land surfaces, noted Knobelspiesse, the mission scientist for PACE-PAX. This mission is all about checking the accuracy of those new satellite measurements.
Sam Habbal (quality inspector), Darick Alvarez (aircraft mechanic), and Juan Alvarez (crew chief) work on the network “canoe” on top of the ER-2 aircraft, which provides network communication with the pilot onboard. Experts like these sustain a high standard of safety while outfitting instruments onboard science aircraft like the ER-2 and science missions like the Plankton, Aerosol, Cloud, ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) mission. The ER-2 is based out of NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Genaro Vavuris
“The ER-2 is the ideal platform for PACE-PAX because it’s about the closest we can get to putting instruments in orbit without actually doing so,” Knobelspiesse said.
The collaborative project includes a diverse team of researchers from across NASA, plus the National Oceanic and Atmospheric Administration (NOAA), the Netherlands Institute for Space Research (SRON), the University of Maryland, Baltimore County, the Naval Postgraduate School, and other institutions.
Similarly, the Geological Earth Mapping eXperiment (GEMx) science mission is using the ER-2 over multiple years to collect observations of critical mineral resources across the Western United States.
“Flying at this altitude means the GEMx mission can acquire wide swaths of data with every overflight,” said Kevin Reath, NASA’s associate project manager for the GEMx mission, a collaboration between the United States Geological Survey (USGS) and NASA.
The ER-2 conducted over 80 flight hours in service of the Plankton, Aerosol, Cloud, ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) mission. The ER-2 is uniquely qualified to conduct the high-altitude scientific flights that this project required, and is based at NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Genaro Vavuris
The GEMx team collects visible, shortwave infrared, and thermal infrared data using instruments installed onboard the ER-2. Combining these instruments with the aircraft’s capability to fly at high altitudes bears promising results.
“The dataset being produced is the largest airborne surface mineralogy dataset captured in a single NASA campaign,” Reath said. “These data could help inform federal, tribal, state, and community leaders to make decisions that protect or develop our environment.”
Learn more about the ER-2 aircraft.
Learn more about the PACE-PAX mission.
Learn more about the GEMx mission.
Learn more about NASA’s Airborne Science Program.
Share Details Last Updated Oct 24, 2024 EditorDede DiniusContactErica HeimLocationArmstrong Flight Research Center Related Terms Explore More 3 min read Autumn Leaves – Call for VolunteersThe Global Learning and Observations to Benefit the Environment (GLOBE) Program is calling on volunteers…
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