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By European Space Agency
Hera asteroid mission launch kit
Everything you'd ever want to know about ESA's first planetary defence mission
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By NASA
5 Min Read NASA’s Webb Reveals Distorted Galaxy Forming Cosmic Question Mark
The galaxy cluster MACS-J0417.5-1154. Full image below. Credits:
NASA, ESA, CSA, STScI, V. Estrada-Carpenter (Saint Mary’s University). It’s 7 billion years ago, and the universe’s heyday of star formation is beginning to slow. What might our Milky Way galaxy have looked like at that time? Astronomers using NASA’s James Webb Space Telescope have found clues in the form of a cosmic question mark, the result of a rare alignment across light-years of space.
“We know of only three or four occurrences of similar gravitational lens configurations in the observable universe, which makes this find exciting, as it demonstrates the power of Webb and suggests maybe now we will find more of these,” said astronomer Guillaume Desprez of Saint Mary’s University in Halifax, Nova Scotia, a member of the team presenting the Webb results.
Image A: Lensed Question Mark (NIRCam)
The galaxy cluster MACS-J0417.5-1154 is so massive it is warping the fabric of space-time and distorting the appearance of galaxies behind it, an effect known as gravitational lensing. This natural phenomenon magnifies distant galaxies and can also make them appear in an image multiple times, as NASA’s James Webb Space Telescope saw here. Two distant, interacting galaxies — a face-on spiral and a dusty red galaxy seen from the side — appear multiple times, tracing a familiar shape across the sky. Active star formation, and the face-on galaxy’s remarkably intact spiral shape, indicate that these galaxies’ interaction is just beginning. NASA, ESA, CSA, STScI, V. Estrada-Carpenter (Saint Mary’s University). While this region has been observed previously with NASA’s Hubble Space Telescope, the dusty red galaxy that forms the intriguing question-mark shape only came into view with Webb. This is a result of the wavelengths of light that Hubble detects getting trapped in cosmic dust, while longer wavelengths of infrared light are able to pass through and be detected by Webb’s instruments.
Astronomers used both telescopes to observe the galaxy cluster MACS-J0417.5-1154, which acts like a magnifying glass because the cluster is so massive it warps the fabric of space-time. This allows astronomers to see enhanced detail in much more distant galaxies behind the cluster. However, the same gravitational effects that magnify the galaxies also cause distortion, resulting in galaxies that appear smeared across the sky in arcs and even appear multiple times. These optical illusions in space are called gravitational lensing.
The red galaxy revealed by Webb, along with a spiral galaxy it is interacting with that was previously detected by Hubble, are being magnified and distorted in an unusual way, which requires a particular, rare alignment between the distant galaxies, the lens, and the observer — something astronomers call a hyperbolic umbilic gravitational lens. This accounts for the five images of the galaxy pair seen in Webb’s image, four of which trace the top of the question mark. The dot of the question mark is an unrelated galaxy that happens to be in the right place and space-time, from our perspective.
Image B: Hubble and Webb Side by Side
Image Before/After In addition to producing a case study of the Webb NIRISS (Near-Infrared Imager and Slitless Spectrograph) instrument’s ability to detect star formation locations within a galaxy billions of light-years away, the research team also couldn’t resist highlighting the question mark shape. “This is just cool looking. Amazing images like this are why I got into astronomy when I was young,” said astronomer Marcin Sawicki of Saint Mary’s University, one of the lead researchers on the team.
“Knowing when, where, and how star formation occurs within galaxies is crucial to understanding how galaxies have evolved over the history of the universe,” said astronomer Vicente Estrada-Carpenter of Saint Mary’s University, who used both Hubble’s ultraviolet and Webb’s infrared data to show where new stars are forming in the galaxies. The results show that star formation is widespread in both. The spectral data also confirmed that the newfound dusty galaxy is located at the same distance as the face-on spiral galaxy, and they are likely beginning to interact.
“Both galaxies in the Question Mark Pair show active star formation in several compact regions, likely a result of gas from the two galaxies colliding,” said Estrada-Carpenter. “However, neither galaxy’s shape appears too disrupted, so we are probably seeing the beginning of their interaction with each other.”
“These galaxies, seen billions of years ago when star formation was at its peak, are similar to the mass that the Milky Way galaxy would have been at that time. Webb is allowing us to study what the teenage years of our own galaxy would have been like,” said Sawicki.
The Webb images and spectra in this research came from the Canadian NIRISS Unbiased Cluster Survey (CANUCS). The research paper is published in the Monthly Notices of the Royal Astronomical Society.
Image C: Wide Field – Lensed Question Mark (NIRCam)
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, ESA (European Space Agency) and CSA (Canadian Space Agency).
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Media Contacts
Laura Betz – laura.e.betz@nasa.gov, Rob Gutro – rob.gutro@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Christine Pulliam – cpulliam@stsci.edu , Leah Ramsey – lramsey@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
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Last Updated Sep 04, 2024 Editor Stephen Sabia Contact Laura Betz laura.e.betz@nasa.gov Related Terms
Astrophysics Galaxies Galaxies, Stars, & Black Holes Galaxy clusters Goddard Space Flight Center Gravitational Lensing James Webb Space Telescope (JWST) Science & Research The Universe View the full article
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By NASA
Learn Home New TEMPO Cosmic Data Story… Astrophysics Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Stories Science Activation Highlights Citizen Science 3 min read
New TEMPO Cosmic Data Story Makes Air Quality Data Publicly Available
On May 30th, 2024, NASA and the Center for Astrophysics | Harvard & Smithsonian announced the public release of “high-quality, near real-time air quality data” from NASA’s TEMPO (Tropospheric Emissions: Monitoring of Pollution) mission. The NASA Science Activation program’s Cosmic Data Stories team, led by Harvard University in Cambridge, MA, has since released a new “Data Story” – an interactive, digital showcase of new science imagery, including ideas for exploration and scientific highlights shared in a brief video and narrative text – that provides a quick and easy way for the public to visualize this important, large data set from TEMPO.
TEMPO allows unprecedented monitoring of air quality down to neighborhood scales, with its hourly daytime scans over North America. Air pollutants like NO2, produced, for example, by the burning of fossil fuels, can trigger significant health issues, especially among people with pre-existing illnesses such as asthma. The interactive views in the TEMPO Data Story provide public access to the same authentic data that scientists use and invite the public to explore patterns in their local air quality. For example, how do NO2 emissions vary in our area throughout the day and week? What are possible sources of NO2 in our community? How does our air quality compare with that of other communities with similar population densities, or with nearby urban or rural communities? TEMPO’s hyper-localized data will allow communities to make informed decisions and take action to improve their air quality.
The Cosmic Data Story team is grateful to TEMPO scientists, Xiong Liu and Caroline Nowlan, for providing the team with early access to the data and guidance on NO2 phenomena that learners can explore in the data. The TEMPO Data Story, featured on TEMPO’s webpage for the public, adds Earth science data to the portfolio of Cosmic Data Stories that is already making astrophysics data accessible to the public.
TEMPO Team Atmospheric Physicist from the Harvard-Smithsonian Center for Astrophysics, Caroline Nowlan, had this to say: “TEMPO produces data that are really useful for scientists, but are also important for the general public and policy makers. We are thrilled that the Cosmic Data Stories team has made a tool that allows everyone to explore TEMPO data and learn about pollution across North America and in their own communities.”
The Cosmic Data Stories project is supported by NASA under cooperative agreement award number 80NSSC21M0002 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
A view from the TEMPO Data Story, shows TEMPO’s NO2 data overlaid on a map of North America. A large plume of NO2, caused by large wildfires, arcs from Northern California all the way to Idaho. Other “hot spots” of NO2 are seen over cities across the US, Canada, and Mexico. Users can view any available date, as well as explore some featured dates and locations that describe phenomena of interest that are visible in the data. Share
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Last Updated Aug 13, 2024 Editor NASA Science Editorial Team Related Terms
Astrophysics Earth Science Science Activation Tropospheric Emissions: Monitoring of Pollution (TEMPO) Explore More
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By NASA
4 min read
Repair Kit for NASA’s NICER Mission Heading to Space Station
NASA will deliver a patch kit for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station, on the agency’s Northrop Grumman 21st commercial resupply mission. Astronauts will conduct a spacewalk to complete the repair.
Located near the space station’s starboard solar array, NICER was damaged in May 2023. The mission team delivered the patch kit to NASA’s Johnson Space Center in Houston in May 2024 so it could be prepped and packed for the upcoming resupply mission.
“It’s incredible that in just one year, we were able to diagnose the problem and then design, build, test, and deliver a solution,” said Steve Kenyon, NICER’s mechanical lead at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “We’re so excited to see the patches installed during a future spacewalk, return to a more regular operating schedule, and keep doing groundbreaking science.”
This image, obtained June 8, 2018, shows NASA’s NICER (Neutron star Interior Composition Explorer) on the International Space Station, where it studies neutron stars and other X-ray sources. NICER is about the size of a washing machine. The sunshades of its X-ray concentrators are visible as an array of circular features. NASA UAE (United Arab Emirates) astronaut Sultan Alneyadi captured this view of NICER from a window in the Poisk Mini-Research Module 2 on the space station in July 2023. Photos like this one helped the mission team map the damage to the thermal shields over NICER’s X-ray concentrators. NASA/Sultan Alneyadi Some of NICER’s damaged thermal shields (circled) are visible in this photograph. NASA/Sultan Alneyadi
From its perch on the station, the washing machine-sized NICER studies the X-ray sky. It has precisely measured superdense stellar remnants called neutron stars, which contain the densest matter scientists can directly observe. It has also investigated mysterious fast radio bursts, observed comets in our solar system, and collected data about Earth’s upper atmosphere.
But in May 2023, NICER developed a “light leak,” where unwanted sunlight began entering the telescope.
Photos taken aboard the station revealed several areas of damage to NICER’s thermal shields. The shields are 500 times thinner than a human hair and filter out infrared, ultraviolet, and visible light while allowing X-rays to pass through. They cover each of NICER’s 56 X-ray concentrators, sets of 24 nested circular mirrors designed to skip X-rays into corresponding detectors. A sunshade tops each concentrator and shield assembly, with a slight gap in between. The sunshades are segmented by six internal struts, resembling a sliced pie.
The largest damage to the shields is around the size of a typical U.S. postage stamp. The other areas are closer in size to pinheads. During the station’s daytime, the damage allows sunlight to reach the detectors, saturating sensors and interfering with NICER’s measurements. The mission team altered their daytime observing strategy to mitigate the effect. The damage does not impact nighttime observations.
“NICER wasn’t designed to be serviced or repaired,” said Keith Gendreau, the mission’s principal investigator at Goddard. “It was installed robotically, and we operate it remotely. When we decided to investigate the possibility of patching the largest damaged areas on the thermal shields, we had to come up with a method that would use the existing parts of the telescope and station toolkits. We couldn’t have done it without all the support and collaboration from our colleagues at Johnson and throughout the space station program.”
NICER’s patches are made from aluminum and anodized, or coated, black. Each is about 2 inches tall. “LCK” indicates the lock position for a tab at the bottom that will hold the patch in place. NASA is sending 12 of these patches to the International Space Station. During a spacewalk, astronauts will insert five into sunshades on the telescope to cover the most significant areas of damage. NASA/Sophia Roberts NICER’s patches will be inserted into its sunshades, as shown here. The small tab that locks the patch into place is visible beneath it. The carbon composite sunshades cover each of NICER’s 56 X-ray concentrators. Each sunshade is supported by three gold-colored fiberglass mounting feet. NASA/Sophia Roberts NICER’s thermal shields — the silver film shown here — cover each of the mission’s 56 X-ray concentrators. They block ultraviolet, infrared, and visible light while allowing X-rays to pass through to the mirrors underneath. Each shield is only about 160 nanometers thick, or 500 times thinner than a human hair. The fragile shield is supported by a stainless-steel frame which consists of a pattern of 1/8 inch (3 millimeter) squares in each of the wedges. NASA/Sophia Roberts NICER has 56 individual X-ray focusing elements, called concentrators, that each contain 24 nested mirrors. Every concentrator delivers X-rays to its own detector. The concentrator shown here is tilted on its side, so the camera is looking into the nested mirrors. X-rays are high-energy light, so they can pass through the atoms of telescope mirrors like those for NASA’s Hubble and James Webb space telescopes. Instead, X-ray observatories use grazing incidence mirrors, where the surfaces are turned on their sides. X-rays skip across their surfaces and into detectors. NASA/Sophia Roberts
The solution, in the end, was simple. The team designed patches, each shaped like a piece of pie, that will slide into the sunshades. A tab at the bottom of each patch will turn into the space between the bottom of the sunshade and the top of the thermal shield, keeping it in place.
Astronauts will install five patches during the spacewalk. They’ll cover the most significant areas of damage and block the sunlight affecting NICER’s X-ray measurements.
The repair kit contains 12 patches in total, allowing for spares if needed. Astronauts will carry the patches in a caddy, a rectangular frame containing two spare sunshades with the patches held inside.
“NICER will be the first X-ray telescope in orbit to be serviced by astronauts and only the fourth science observatory to be repaired overall — joining the ranks of missions like NASA’s Hubble Space Telescope,” said Charles Baker, the NICER project systems engineer at Goddard. “It’s been amazing to watch the patch kit come together over the last year. NICER has taught us so many wonderful things about the cosmos, and we’re really looking forward to this next step of its journey.”
The NICER caddy is an aluminum box containing two of the mission’s spare sunshades, which are attached to the bottom. Inside the sunshades, 12 patches are locked into place. Astronauts will take the complete caddy assembly with them during a future spacewalk to address damage to NICER’s thermal shields. They’ll insert five of the patches over the largest areas of damage, which will allow the mission to return to a normal operating status during the station’s daytime. The NICER telescope is an Astrophysics Mission of Opportunity within NASA’s Explorers Program, which provides frequent flight opportunities for world-class scientific investigations from space utilizing innovative, streamlined, and efficient management approaches within the heliophysics and astrophysics science areas. NASA’s Space Technology Mission Directorate supported the SEXTANT component of the mission, demonstrating pulsar-based spacecraft navigation.
Download high-resolution NICER images and videos
By Jeanette Kazmierczak
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Media Contact:
Claire Andreoli
301-286-1940
claire.andreoli@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
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Last Updated Jul 30, 2024 Related Terms
Astrophysics Goddard Space Flight Center International Space Station (ISS) ISS Research Johnson Space Center Neutron Stars NICER (Neutron star Interior Composition Explorer) Pulsars The Universe View the full article
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