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By NASA
AMS-02 mounted on the outside of the space station.NASA Visible matter in the form of stars and planets adds up to about five percent of the total known mass of the Universe. The rest is either dark matter, antimatter, or dark energy. The exact nature of these substances is unknown, but the International Space Station’s Alpha-Magnetic Spectrometer or AMS-02 is helping to solve the mystery.
AMS-02 collects data on charged particles from cosmic ray events, which helps scientists understand the origin of those rays and could ultimately reveal whether dark matter and antimatter exist.
To date, the instrument has collected data on about 573 events per second on average – just over 18 billion per year. This high volume of data enables highly precise statistical analyses, and multiple groups of researchers independently process the raw data to ensure accurate results.
Learn more about astrophysics research on the space station.
This view shows the core of AMS-02, a massive magnet that bends particles from space to reveal whether their charge is positive or negative.NASA AMS-02 is the hexagonal shape visible on one of the space station’s trusses, just to the right of the center.NASA Keep Exploring Discover More Topics
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By NASA
NASA/CXC/M.Weiss By using new data from NASA’s Chandra X-ray Observatory and Neil Gehrels Swift Observatory as well as ESA’s XMM-Newton, a team of researchers have made important headway in understanding how — and when — a supermassive black hole obtains and then consumes material, as described in our latest press release.
This artist’s impression shows a star that has partially been disrupted by such a black hole in the system known as AT2018fyk. The supermassive black hole in AT2018fyk — with about 50 million times more mass than the sun — is in the center of a galaxy located about 860 million light-years from Earth.
Astronomers have determined that a star is on a highly elliptical orbit around the black hole in AT2018fyk so that its point of farthest approach from the black hole is much larger than its closest. During its closest approach, tidal forces from the black hole pull some material from the star, producing two tidal tails of “stellar debris”.
The illustration shows a point in the orbit soon after the star is partially destroyed, when the tidal tails are still in close proximity to the star. Later in the star’s orbit, the disrupted material returns to the black hole and loses energy, leading to a large increase in X-ray brightness occurring later in the orbit (not shown here). This process repeats each time the star returns to its point of closest approach, which is approximately every 3.5 years. The illustration depicts the star during its second orbit, and the disk of X-ray emitting gas around the black hole that is produced as a byproduct of the first tidal encounter.
Researchers took note of AT2018fyk in 2018 when the optical ground-based survey ASAS-SN detected that the system had become much brighter. After observing it with NASA’s NICER and Chandra, and XMM-Newton, researchers determined that the surge in brightness came from a “tidal disruption event,” or TDE, which signals that a star was completely torn apart and partially ingested after flying too close to a black hole. Chandra data of AT2018fyk is shown in the inset of an optical image of a wider field-of-view.
X-ray: NASA/SAO/Kavli Inst. at MIT/D.R. Pasham; Optical: NSF/Legacy Survey/SDSS When material from the destroyed star approached close to the black hole, it got hotter and produced X-ray and ultraviolet (UV) light. These signals then faded, agreeing with the idea that nothing was left of the star for the black hole to digest.
However, about two years later, the X-ray and UV light from the galaxy got much brighter again. This meant, according to astronomers, that the star likely survived the initial gravitational grab by the black hole and then entered a highly elliptical orbit with the black hole. During its second close approach to the black hole, more material was pulled off and produced more X-ray and UV light.
Based on what they had learned about the star and its orbit, a team of astronomers predicted that the black hole’s second meal would end in August 2023 and applied for Chandra observing time to check. Chandra observations on August 14, 2023, indeed showed the telltale sign of the black hole feeding coming to an end with a sudden drop in X-rays. The researchers also obtained a better estimate of how long it takes the star to complete an orbit, and predicted future mealtimes for the black hole.
A paper describing these results appears in the August 14, 2024 issue of The Astrophysical Journal and is available online. The authors are Dheeraj Passam (Massachusetts Institute of Technology), Eric Coughlin (Syracuse University), Muryel Guolo (Johns Hopkins University), Thomas Wevers (Space Telescope Science Institute), Chris Nixon (University of Leeds, UK), Jason Hinkle (University of Hawaii at Manoa), and Ananaya Bandopadhyay (Syracuse).
NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science from Cambridge Massachusetts and flight operations from Burlington, Massachusetts.
Read more from NASA’s Chandra X-ray Observatory.
For more Chandra images, multimedia and related materials, visit:
https://www.nasa.gov/mission/chandra-x-ray-observatory/
Visual Description:
In this digital illustration, a star sheds stellar debris as it orbits a supermassive black hole. This artist’s impression represents the center of a galaxy about 860 million light-years from Earth.
The supermassive black hole sits at our upper left. It resembles an irregular, pitch-black sphere at the heart of an almond-shaped pocket of swirling sand and dirt. Though gritty in texture, the swirling brown and grey pocket is actually a disk of hot gas.
Near our lower right is the orbiting star. In this illustration, the star is relatively close to us, with the black hole far behind it. The star is a blue-white ball that, from this perspective, appears slightly larger than the distant black hole.
Two tapered streaks peel off of the glowing star like the pulled-back corners of a smile. These streaks represent tidal tails of stellar debris; material pulled from the surface of the star by the gravity of the black hole. This partial destruction of the star occurs every 3.5 years, when the star’s orbit brings it closest to the supermassive black hole.
During the orbit, the stellar debris from the tidal tails is ingested by the black hole. A byproduct of this digestion is the X-ray gas which swirls in a disk around the black hole.
At the upper left of the grid is an image of the distant galaxy cluster known as MACS J0416. Here, the blackness of space is packed with glowing dots and tiny shapes, in whites, purples, oranges, golds, and reds, each a distinct galaxy. Upon close inspection (and with a great deal of zooming in!) the spiraling arms of some of the seemingly tiny galaxies are revealed in this highly detailed image. Gently arched across the middle of the frame is a soft band of purple; a reservoir of superheated gas detected by Chandra.
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By NASA
Bindu Rani had childhood dreams of flight. Today she lifts her gaze even higher, helping researchers study stars, planets beyond our solar system, and black holes billions of times more massive than our Sun.
Name: Bindu Rani
Title: Astrophysicist, Neil Gehrels Swift Observatory Guest Investigator Program Lead Scientist
Organization: Astroparticle Physics Laboratory, Science Directorate (Code 661)
Bindu Rani is an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Md.Photo credit: NASA/Jay Friedlander What do you do and what is most interesting about your role here at Goddard?
I study supermassive black holes using both space-based and ground-based observations. I love trying to understand the dynamics and nature of physical processes that happen in the vicinity of a black hole.
Why did you become an astrophysicist?
When I was a little girl, I wanted to fly way up in the sky and be a pilot. When I was doing my master’s, I got interested in black holes and neutron stars. I was so fascinated that I decided to pursue this field.
What is your educational background?
In 2005, I got a bachelor’s degree in science from Government College Bahadurgarh, India. In 2007, I got a master’s degree in in physics from the Department of Physics and Astrophysics, Delhi University, India. In 2013, I got a doctorate in astrophysics from the Max Planck Institute for Radio Astronomy, Bonn, Germany. From 2014 to 2016, I was a post-doctoral fellow at Max Plank.
How did you come to Goddard?
In 2016, I came to Goddard through NASA’s Postdoctoral Fellowship program.
From 2020 to 2022, I worked at the Korea Astronomy and Space Science Institute in South Korea as a staff scientist. I can say please and thank you in Korean, but everyone in the lab and the young students spoke English and loved practicing English.
In September 2022, I returned to Goddard as the Swift Guest Investigator Program lead scientist.
You have lived in India, South Korea, Germany, and now the United States. What are your favorite aspects of each country?
The best thing about India is that my family is there, and I deeply miss them. All my happy memories are in one small town along with my parents, siblings, and friends. I deeply miss Indian food too. My family and I visit India whenever we can.
I love South Korean food. What motivated me in the mornings was their delicious coffee and cafeteria food. I miss their culture, so warm and welcoming. When I left, there was a hole in my heart.
Life in Germany is amazing. They have the best work life balance. Also, I miss German bread and beer.
What are your goals as the Swift Guest Investigator Program lead?
I lead the program, including managing the proposals, staffing the program, conducting reviews, and supporting the users. Swift is an amazing mission because it provides X-rays and ultraviolet to optical observations of all different kinds of astronomical objects including exoplanets, stars, dwarf stars, and black holes up to millions to billions of solar masses.
How do you keep your people motivated?
Our work is super interesting which itself is motivating. My idea is that if you want the best out of people, you have to make them comfortable. I try to apply this both at work and at home.
“Most of my inspiration comes from my own curiosity and from the fact that I am very determined,” said Bindu.Photo courtesy of Bindu Rani How do you feel when you discover a black hole?
Swift observes radiation from many black holes ranging in size from a few solar masses (that is, a few times the mass of our Sun) to billions of solar masses. In the vicinity of black holes, infalling material heats up and emits radiation. In some cases, black holes consuming dust and gas at the center of galaxies produce jets — a laser-like beam of light that we observe with our telescopes.
When we have a new discovery, it is very exciting, and many observations follow using many different ground and space telescopes. For example, the brightest of all time gamma-ray burst (BOAT GRB), which is likely the birth cry of a new black hole, was jointly discovered by Swift and the Fermi Gamma-ray Space Telescope on Oct. 9, 2022. It was subsequently observed by about 50 space- and ground-based telescopes.
What is the most amazing observation you have seen from a black hole?
Black holes are extremely fascinating astronomical objects to study and to test our theoretical models in extreme gravity environments. I believe the most amazing observation is the first image of a black hole itself. In 2019, the first direct image of a black hole at the center of galaxy M87 confirmed the existence of black holes, marking a historic milestone in astrophysics.
Who inspires you?
Most of my inspiration comes from my own curiosity and from the fact that I am very determined. My family is my true inspiration, especially my parents. They were motivating in many different ways. My parents are really hard working. They are very proud of me.
What do you say to the people you mentor?
I tell them to keep learning, to enjoy what they are doing even if it feels hard. I them to stay curious. I also tell them to strengthen their speaking, writing and coding skills to become a good scientists. As my doctorate advisor told me, you have to learn how to sell yourself.
As an avid reader, who is your favorite author?
Books bring me peace. I enjoy reading books in Hindi, by an Indian author called Munsi Prem Chand, who wrote about social fiction. I am currently reading Laura Markam’s “Peaceful Parents, Happy Kids” because I have a young child.
What else do you do to relax?
I like to run and practice yoga. Mostly either I work or spend time with my child.
What is it like for both you and your husband to both work at Goddard?
My husband, Pankaj Kumar, is a heliophysicist in the Space Weather Laboratory (Code 674). We met in India, and both found jobs at Goddard. It is so wonderful to be at the same working institute. At home, we try not to discuss work. But our child is very curious and asks us a lot of questions about our research. Our child wants to become a NASA scientist, which he calls a NASA professor.
What do you value most about working at Goddard?
Goddard has the best work culture. Everyone is so open and friendly. I can just knock on any door and will be able to talk. The open communication puts you at ease.
Also, Goddard has a lot of women researchers in lead positions. Goddard values women.
How do you describe yourself?
I am a girl who came from a small village in India and am now at Goddard. I dreamed about going to space one day and now I am doing research at Goddard. My family’s support mattered. My own strong-willed nature helped too. At this stage, my curiosity and love of challenges continues to motivate me. Several factors in my life got me to where I am.
Who do you want to thank?
I am grateful to the people who believed in me (my family, friends, and colleagues) as well as those who tried to hinder me.
What’s your “big dream”?
I want to be an astronaut. When I was doing my master’s, I became interested in being an astronaut.
By Elizabeth M. Jarrell
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Conversations With Goddard is a collection of Q&A profiles highlighting the breadth and depth of NASA’s Goddard Space Flight Center’s talented and diverse workforce. The Conversations have been published twice a month on average since May 2011. Read past editions on Goddard’s “Our People” webpage.
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Last Updated Aug 06, 2024 EditorMadison OlsonContactRob Garnerrob.garner@nasa.govLocationGoddard Space Flight Center Related Terms
People of Goddard Goddard Space Flight Center People of NASA Explore More
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By NASA
4 Min Read NASA’s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri
This NASA Hubble Space Telescope image features the globular star cluster, Omega Centauri. Credits:
ESA/Hubble, NASA, Maximilian Häberle (MPIA) Most known black holes are either extremely massive, like the supermassive black holes that lie at the cores of large galaxies, or relatively lightweight, with a mass of under 100 times that of the Sun. Intermediate-mass black holes (IMBHs) are scarce, however, and are considered rare “missing links” in black hole evolution.
Now, an international team of astronomers has used more than 500 images from NASA’s Hubble Space Telescope — spanning two decades of observations — to search for evidence of an intermediate-mass black hole by following the motion of seven fast-moving stars in the innermost region of the globular star cluster Omega Centauri.
Omega Centauri is about 10 times as massive as other big globular clusters – almost as massive as a small galaxy – and consists of roughly 10 million stars that are gravitationally bound. ESA/Hubble, NASA, Maximilian Häberle (MPIA)
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These stars provide new compelling evidence for the presence of the gravitational pull from an intermediate-mass black hole tugging on them. Only a few other IMBH candidates have been found to date.
Omega Centauri consists of roughly 10 million stars that are gravitationally bound. The cluster is about 10 times as massive as other big globular clusters — almost as massive as a small galaxy.
Among the many questions scientists want to answer: Are there any IMBHs, and if so, how common are they? Does a supermassive black hole grow from an IMBH? How do IMBHs themselves form? Are dense star clusters their favored home?
The astronomers have now created an enormous catalog for the motions of these stars, measuring the velocities for 1.4 million stars gleaned from the Hubble images of the cluster. Most of these observations were intended to calibrate Hubble’s instruments rather than for scientific use, but they turned out to be an ideal database for the team’s research efforts.
This image shows the central region of the Omega Centauri globular cluster, where NASA’s Hubble Space Telescope found strong evidence for an intermediate-mass black hole candidate. ESA/Hubble, NASA, Maximilian Häberle (MPIA)
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“We discovered seven stars that should not be there,” explained Maximilian Häberle of the Max Planck Institute for Astronomy in Germany, who led this investigation. “They are moving so fast that they would escape the cluster and never come back. The most likely explanation is that a very massive object is gravitationally pulling on these stars and keeping them close to the center. The only object that can be so massive is a black hole, with a mass at least 8,200 times that of our Sun.”
Several studies have suggested the presence of an IMBH in Omega Centauri. However, other studies proposed the mass could be contributed by a central cluster of stellar-mass black holes, and had suggested the lack of fast-moving stars above the necessary escape velocity made an IMBH less likely in comparison.
An international team of astronomers used more than 500 images from NASA’s Hubble Space Telescope – spanning two decades of observations – to detect seven fast-moving stars in the innermost region of Omega Centauri, the largest and brightest globular cluster in the sky. These stars provide compelling new evidence for the presence of an intermediate-mass black hole (IMBH) tugging on them. Only a few other IMBH candidates have been found to date. This image shows the location of the IMBH in Omega Centauri. If confirmed, at its distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, which is 26,000 light-years away. Besides the Galactic center, it would also be the only known case of a number of stars closely bound to a massive black hole. This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image shows the details of the central region of this cluster, with a closer view of the individual stars. The third image shows the location of the IMBH candidate in the cluster. ESA/Hubble, NASA, Maximilian Häberle (MPIA)
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“This discovery is the most direct evidence so far of an IMBH in Omega Centauri,” added team lead Nadine Neumayer of the Max Planck Institute for Astronomy in Germany, who initiated the study, together with Anil Seth from the University of Utah, Salt Lake City. “This is exciting because there are only very few other black holes known with a similar mass. The black hole in Omega Centauri may be the best example of an IMBH in our cosmic neighborhood.”
If confirmed, at a distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, located 26,000 light-years away.
Omega Centauri is visible from Earth with the naked eye and is one of the favorite celestial objects for stargazers living in the southern hemisphere. Located just above the plane of the Milky Way, the cluster appears almost as large as the full Moon when seen from a dark rural area. It was first listed in Ptolemy’s catalog nearly 2,000 years ago as a single star. Edmond Halley reported it as a nebula in 1677. In the 1830s the English astronomer John Herschel was the first to recognize it as a globular cluster.
The discovery paper led by Häberle et al. is published online today in the journal Nature.
Scientists think a massive object is gravitationally pulling on the stars within Omega Centauri, keeping them close to its center. Credit: NASA’s Goddard Space Flight Center, Lead Producer: Paul Morris
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The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, Colorado, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, Maryland, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contacts:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov
Ray Villard
Space Telescope Science Institute, Baltimore, MD
Bethany Downer
ESA/Hubble.org
Science Contact:
Maximilian Häberle
Max Planck Institute for Astronomy, Heidelberg, Germany
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Last Updated Jul 10, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
Astrophysics Astrophysics Division Black Holes Goddard Space Flight Center Hubble Space Telescope Missions Stars The Universe Keep Exploring Discover More Topics From Hubble
Hubble Space Telescope
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
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By European Space Agency
An international team of astronomers has used more than 500 images from the NASA/ESA Hubble Space Telescope spanning two decades to detect seven fast-moving stars in the innermost region of Omega Centauri, the largest and brightest globular cluster in the sky. These stars provide compelling new evidence for the presence of an intermediate-mass black hole.
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