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By NASA
5 Min Read Webb Maps Full Picture of How Phoenix Galaxy Cluster Forms Stars
Spectroscopic data collected from NASA’s James Webb Space Telescope is overlayed on an image of the Phoenix cluster that combines data from NASA’s Hubble Space Telescope, Chandra X-ray Observatory and the Very Large Array (VLA) radio telescope. Credits:
NASA, CXC, NRAO, ESA, M. McDonald (MIT), M. Reefe (MIT), J. Olmsted (STScI) Discovery proves decades-old theory of galaxy feeding cycle.
Researchers using NASA’s James Webb Space Telescope have finally solved the mystery of how a massive galaxy cluster is forming stars at such a high rate. The confirmation from Webb builds on more than a decade of studies using NASA’s Chandra X-ray Observatory and Hubble Space Telescope, as well as several ground-based observatories.
The Phoenix cluster, a grouping of galaxies bound together by gravity 5.8 billion light-years from Earth, has been a target of interest for astronomers due to a few unique properties. In particular, ones that are surprising: a suspected extreme cooling of gas and a furious star formation rate despite a roughly 10 billion solar mass supermassive black hole at its core. In other observed galaxy clusters, the central supermassive black hole powers energetic particles and radiation that prevents gas from cooling enough to form stars. Researchers have been studying gas flows within this cluster to try to understand how it is driving such extreme star formation.
Image A: Phoenix Cluster (Hubble, Chandra, VLA Annotated)
Spectroscopic data collected from NASA’s James Webb Space Telescope is overlayed on an image of the Phoenix cluster that combines data from NASA’s Hubble Space Telescope, Chandra X-ray Observatory and the Very Large Array (VLA) radio telescope. Webb’s powerful sensitivity in the mid-infrared detected the cooling gas that leads to a furious rate of star formation in this massive galaxy cluster. Credit: NASA, CXC, NRAO, ESA, M. McDonald (MIT), M. Reefe (MIT), J. Olmsted (STScI) “We can compare our previous studies of the Phoenix cluster, which found differing cooling rates at different temperatures, to a ski slope,” said Michael McDonald of the Massachusetts Institute of Technology in Cambridge, principal investigator of the program. “The Phoenix cluster has the largest reservoir of hot, cooling gas of any galaxy cluster — analogous to having the busiest chair lift, bringing the most skiers to the top of the mountain. However, not all of those skiers were making it down the mountain, meaning not all the gas was cooling to low temperatures. If you had a ski slope where there were significantly more people getting off the ski lift at the top than were arriving at the bottom, that would be a problem!”
To date, in the Phoenix cluster, the numbers weren’t adding up, and researchers were missing a piece of the process. Webb has now found those proverbial skiers at the middle of the mountain, in that it has tracked and mapped the missing cooling gas that will ultimately feed star formation. Most importantly, this intermediary warm gas was found within cavities tracing the very hot gas, a searing 18 million degrees Fahrenheit, and the already cooled gas around 18,000 degrees Fahrenheit.
The team studied the cluster’s core in more detail than ever before with the Medium-Resolution Spectrometer on Webb’s Mid-Infrared Instrument (MIRI). This tool allows researchers to take two-dimenstional spectroscopic data from a region of the sky, during one set of observations.
“Previous studies only measured gas at the extreme cold and hot ends of the temperature distribution throughout the center of the cluster,” added McDonald. “We were limited — it was not possible to detect the ‘warm’ gas that we were looking for. With Webb, we could do this for the first time.”
Image B: Phoenix Cluster (Hubble, Chandra, VLA)
This image of the Phoenix cluster combines data from NASA’s Hubble Space Telescope, Chandra X-ray Observatory, and the Very Large Array radio telescope. X-rays from Chandra depict extremely hot gas in purple. Optical light data from Hubble show galaxies in yellow, and filaments of cooler gas where stars are forming in light blue. Outburst generated jets, represented in red, are seen in radio waves by the VLA radio telescope. NASA, CXC, NRAO, ESA, M. McDonald (MIT). A Quirk of Nature
Webb’s capability to detect this specific temperature of cooling gas, around 540,000 degrees Fahrenheit, is in part due to its instrumental capabilities. However, the researchers are getting a little help from nature, as well.
This oddity involves two very different ionized atoms, neon and oxygen, created in similar environments. At these temperatures, the emission from oxygen is 100 times brighter but is only visible in ultraviolet. Even though the neon is much fainter, it glows in the infrared, which allowed the researchers to take advantage of Webb’s advanced instruments.
“In the mid-infrared wavelengths detected by Webb, the neon VI signature was absolutely booming,” explained Michael Reefe, also of the Massachusetts Institute of Technology, lead author on the paper published in Nature. “Even though this emission is usually more difficult to detect, Webb’s sensitivity in the mid-infrared cuts through all of the noise.”
The team now hopes to employ this technique to study more typical galaxy clusters. While the Phoenix cluster is unique in many ways, this proof of concept is an important step towards learning about how other galaxy clusters form stars.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
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Hannah Braun hbraun@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Christine Pulliam – cpulliam@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
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By NASA
Ambiguity.
That’s the word that comes to mind when documentary photographers start each day at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
PACE mission photographer Denny Henry and lead documentary photographer Desiree Stover pose for selfies in the clean room.Credits: NASA “You walk in and think one thing is happening,” said OCI’s lead documentary photographer Desiree Stover. “But in an instant things change – maybe goes wrong –- and you need to be ready to capture it.”
From build to testing to launch, one figure is always present in the background capturing the story of each Goddard mission – the documentary photographer.
In honor of #WorldPhotoDay, follow along as two of our documentarians share what it’s like to capture the story of Goddard’s latest mission build PACE.
PACE or Plankton, Aerosol, Cloud, ocean Ecosystem, is set to launch in early 2024. Its goal is to see ocean and atmosphere features in unparalleled detail. By measuring the intensity of the color that reflects from Earth’s ocean surface, PACE will capture fine details about tiny plant-like organisms and algae that live in the ocean, called phytoplankton, that are the basis of the marine food web and generate half of Earth’s oxygen.
Crafting the Story
For Stover and her partner Denny Henry, PACE’s lead mission photographer, the story starts with the smallest details.
“I think one of the first things I photographed was the outside of a circuit port box. It was literally an empty metal box,” said Henry, who started photographing PACE in 2020, right before the pandemic. “It might be small, but it’s part of a system that’s going to do big things.”
Mark Walter, David Kim, Melyane Ortiz-acosta, and Ariel Obaldo discuss plans for testing the PACE flight Solar Array Panels.Credits: NASA’s Goddard Space Flight Center/Denny Henry A typical day for these photographers usually starts with a morning meeting, assignments and getting ready. By the end of the day, the original plan has likely been changed, multiple times.
“Some days we might shoot eight photos, other days it might be hundreds or more,” Stover said.
PACE, or Plankton, Aerosol, Cloud, ocean Ecosystem, is set to launch in early 2024. Its goal is to see ocean and atmosphere features in unparalleled detail.Credits: NASA Images captured during shoots are used for a variety of things, especially technical components of the mission. This includes documenting builds, spotting mistakes and testing.
Stover got her start at Goddard by photographing NASA’s James Webb Space Telescope before switching to capturing imagery of Goddard’s small instruments, including PACE’s Ocean Color Instrument, or OCI. This advanced sensor will enable continuous measurement of light throughout the ultraviolet to shortwave infrared spectrum to better understand Earth’s ocean and atmosphere.
She says she’s still in awe that her teammates trust her “eye.”
“One of the most fascinating things about working here is that we have a specific job,” she said. “And even though engineers can pick up a camera and take photos, they don’t. They know we’re the experts at it. They trust our eyes to tell and capture the story.”
Henry said one of the most memorable days he’s documented so far was watching the PACE team integrate the SPEXone instrument into the spacecraft.
“All the partners were there as I photographed. It was a big deal,” he said. “I captured every bolt all the way to the mounting. It’s important to get these details. Six months from now someone who wasn’t there might want to see what was done in what order.”
Henry said that capturing images is only part of the job. For every hour of shooting, there’s also an hour spent processing and working with partners to ensure things were documented correctly.
Playing Detective
While telling the story is important, Stover says that part of the job is speaking up, especially when you notice something wrong.
During one assignment documenting vibration testing, Stover noticed that OCI’s Earth shade looked different.
“We took the bagging off and could see tape peeling off the radiator panels, possibly loose wires in certain places,” she said. “When I saw this, I thought back to what it was like when we shot this the first time.”
Physical Science Technician Kristen Washington performs a contamination inspection of the OCI Flight Fold Flat Mirror optic.Credits: Desiree Stover, NASA Goddard It’s common for the photographers to shoot things twice to examine how things might change when in testing. When Stover saw the tape, she got to work ensuring her hunch was right.
She sent a series of images to the thermal team lead letting him know what she found. Plans were already underway to change the design.
The unexpected
Stover and Henry agree that documenting missions has come with some interesting experiences.
Both had to undergo fall protection harness training in the event they had to climb around one of Goddard’s cleanrooms, something that happened to Stover during one assignment.
“Once I was up in Building 29’s high bay. Like up at the very top in the crane rafters shooting. I never thought I was afraid of heights until that moment,” she said. “But I focused on the image and what task I was accomplishing and completed the assignment without issue.”
Henry said adjusting to Covid-19 required a lot of flexibility, especially with sudden changes.
“This is not a job you can do from home,” he said. “After a few months, we adapted.”
Radio Frequency testing of the PACE Earth Coverage Antenna in the Electromagnetic Anechoic Chamber at Goddard Space Flight Center.Credits: NASA’s Goddard Space Flight Center/Denny Henry Henry said that many times mission teams will find that engineering drawings won’t match up with what was actually built. With the pandemic restrictions, PACE heavily relied on his images to note how things changed and why issues occurred.
As PACE heads toward big milestones in the next year, both Stover and Henry are excited to see their work come together, including the day of launch.
They both agreed that photographing the teams involved in each aspect of PACE’s build is especially rewarding as they help create mementos that go along with their mission’s story.
By: Sara Blumberg
NASA’s Goddard Space Flight Center, Greenbelt, Md.
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By European Space Agency
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By European Space Agency
The European Space Agency’s Milky Way-mapper Gaia has completed the sky-scanning phase of its mission, racking up more than three trillion observations of about two billion stars and other objects over the last decade to revolutionise the view of our home galaxy and cosmic neighbourhood.
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