Members Can Post Anonymously On This Site
To The Stars - A Tribute To Starship and Test Flight 42
-
Similar Topics
-
By Space Force
A joint team of AFGSC Airmen and Vandenberg SFB Guardians launched an unarmed Minuteman III intercontinental ballistic missile equipped with a single telemetered joint test assembly re-entry vehicle from Vandenberg SFB.
View the full article
-
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).
Downloads
Right click any image to save it or open a larger version in a new tab/window via the browser’s popup menu.
View/Download all image products at all resolutions for this article from the Space Telescope Science Institute.
Read the research paper published in Nature.
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.
Related Information
More Webb News
More Webb Images
Webb Science Themes
Webb Mission Page
Article: Large-scale Structures
Article: Phoenix Galaxy Cluster’s black hole
Article: Spectroscopy 101
Related For Kids
What is the Webb Telescope?
SpacePlace for Kids
En Español
Ciencia de la NASA
NASA en español
Space Place para niños
Keep Exploring Related Topics
James Webb Space Telescope
Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
Stars
Galaxies
Hubble Space Telescope
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
View the full article
-
By NASA
1 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
A still image of a video that shows a plastic rod and cotton-fiberglass fabric being burned during a ground test of the Lunar-g Combustion Investigation (LUCI) experiment.Credit: Voyager Technologies An experiment studying how solid materials catch fire and burn in the Moon’s gravity was launched on Blue Origin’s New Shepard suborbital flight this month.
Developed by NASA’s Glenn Research Center in Cleveland together with Voyager Technologies, the Lunar-g Combustion Investigation (LUCI) will help researchers determine if conditions on the Moon – with reduced gravity – might be a more hazardous environment for fire safety.
The video shows a plastic rod and cotton-fiberglass fabric being burned during a ground test of the Lunar-g Combustion Investigation (LUCI) experiment. Scientists will compare the ground test video to the video recorded on the Blue Origin flight.
Credit: Voyager Technologies On this flight, LUCI tested flammability of cotton-fiberglass fabric and plastic rods, and once launched, the payload capsule rotated at a speed to simulate lunar gravity. NASA Glenn researchers will analyze data post-flight.
A plastic rod and cotton-fiberglass fabric that were burned during testing for the Lunar-g Combustion Investigation. New, unburned samples were lit on fire during the flight. Credit: Voyager Technologies LUCI’s findings will help NASA and its partners design safe spacecraft and spacesuits for future Moon and Mars missions.
For more information on LUCI and the mission, visit.
Return to Newsletter View the full article
-
By NASA
NASA Blue mach diamonds from the main engine nozzles and bright exhaust from the solid rocket boosters mark the successful launch of space shuttle Endeavour 25 years ago on Feb. 11, 2000. The STS-99 mission crew – including astronauts from NASA, the National Space Development Agency of Japan (NASDA), and the European Space Agency (ESA) – were aboard the shuttle.
This mission saw the deployment of the Shuttle Radar Topography Mission mast and the antenna turned to its operation position. After a successful checkout of the radar systems, mapping began less than 12 hours after launch. Crewmembers split into two shifts so they could work around the clock.
Also aboard Endeavour was a student experiment called EarthKAM, which took 2,715 digital photos during the mission through an overhead flight-deck window. The NASA-sponsored program lets middle school students select photo targets and receive the images via the Internet.
Image credit: NASA
View the full article
-
By NASA
Jesse Walsh helps to bring people together in his work with project formulation management. “I try to build trust between team members by understanding everyone’s incentives and making sure all team members understand the different incentives,” he said. “We may have different angles of approach, but we all have the same goal.”Credits: NASA’s Goddard Space Flight Center/William Hrybyk Name: Jesse Walsh
Formal Job Classification: Project Formulation Manager
Organization: Project Formulation and Development Office, Flight Projects Directorate (Code 401.0)
What do you do and what is most interesting about your role here at Goddard? How do you help support Goddard’s mission?
As a formulation manager, I am the project manager in the room as we are designing science space flight missions. We develop proposals to be competed on the agency level against other NASA centers, and outside institutions.
I am also our office’s representative on the Earth science line of business.
“I help everyone negotiate a balance that fits within the cost and schedule,” said Walsh. “The diversity between and among scientists, engineers, and financial experts is what creates NASA’s innovative solutions.”Credits: NASA’s Goddard Space Flight Center/William Hrybyk What is your background?
In 2000, I graduated from the U.S. Naval Academy with a B.S. in mechanical engineering. In the Navy I went to flight school in Pensacola, Florida, and became a naval flight officer. I was the “Goose,” not “Maverick,” in the P-3 Orion, a four-engine prop plane that primarily hunts for submarines. I was then stationed in Hawaii as part of Patrol Squadron 9, that deployed to the Far East and Middle East. Next, I worked at the Naval Research Lab in Washington, D.C., as a project officer for science experiments on P-3s from Patuxent River Naval Air Station in Patuxent River, Maryland.
I developed migraines that disqualified me from flying. In 2007, I got a master’s in civil engineering project management from the University of Maryland. I then worked in Bethesda, Maryland, constructing buildings around the beltway, as a physics teacher at our local high school, and as a project manager of secure facilities with the Army Corps of Engineers.
In 2016, I became the assistant branch head for facilities planning at Goddard. I later entered the Flight Projects Development Program, a two-year project manager training program, during which time I worked at the Flight Projects Development Office and as the payload manager for Space Infrastructure Dexterous Robot (SPIDER), a payload on OSAM-1. I had a proposal selected for a second step, and I came back to PFDO to work proposals.
Why is this your dream job?
We are on the cutting edge of what will fly. We are designing the missions and figuring out what the world of possible will be in space in five to seven years. Scientists come to the table with ideas and engineers make those ideas reality. I make sure the whole team is working together and that all these ideas and solutions fit within our budget and schedule. We make ideas realities.
How do you translate between scientists and engineers?
It is primarily about understanding incentives. Everyone is thinking differently with different solutions, but we have the same goal. Some scientists have had an idea for years, but the idea still has to be workable. If the resulting instrument or spacecraft fails, technical issues are often the first to be examined. I help the engineers push what they are comfortable making and help the scientists understand the limits of technology.
Please talk about the competing pressures of your job.
We are responsible for taxpayer’s money. If one thing goes wrong, even on a smaller mission, the monetary loss can run into many millions. The missions we build have cost limits. We fit cutting edge science into a cost-limited opportunity.
NASA is extremely thorough. We safeguard taxpayer funds, but also push cutting-edge science.
We are on a seesaw. The engineers are more focused on technical solutions while the scientists are more focused on scientific results. I help everyone negotiate a balance that fits within the cost and schedule. The diversity between and among scientists, engineers, and financial experts is what creates NASA’s innovative solutions.
“We are on the cutting edge of what will fly,” said Jesse Walsh about his work as a project formulation manager. “We are designing the missions and figuring out what the world of possible will be in space in five to seven years.”Credits: NASA’s Goddard Space Flight Center/William Hrybyk What are some of your negotiating techniques?
I try to build trust between team members by understanding everyone’s incentives and making sure all team members understand the different incentives. We may have different angles of approach, but we all have the same goal. People are more likely to compromise the means if they know we will end up at the same place.
What is your proudest accomplishment?
I am proudest of our Dorado proposal because it was cutting edge science. We were trying to discover where heavy metals like gold are created in the universe. We were trying to prove that we could do fundamental science on a very lean budget, $35 million.
We did not win the final proposal, but I was extremely proud of our team, a very small, high-functioning team, that made us feel like we could discover the world.
You recently transferred to support the Geospace Dynamics Constellation (GDC) mission. What do you most enjoy about your new role?
I am still learning what I don’t know about GDC. I am finding is fascinating to see how the plans that are made in early stages of formulation change and adapt as they run into unforeseen obstacles during implementation. I am really enjoying being part of a small, high performing team, that is mission focused.
“We fit cutting-edge science into a cost-limited opportunity,” said Jesse Walsh of his work in project formulation management.”NASA is extremely thorough. We safeguard taxpayer funds, but also push cutting-edge science.”Credits: Courtesy of Jesse Walsh Who is your favorite author?
I married a librarian, and books and stories are fundamental parts of our life. I love Hemingway because he portrays extremely complex, emotional scenarios in very simplistic terms.
Who is your science hero?
My high school physics teacher, Mr. Finkbeiner, who taught me that you understand science in your gut, not your head. Science is not memorizing equations; it is understanding how the world around you works.
What are your hobbies?
I love flyfishing on the Chesapeake’s tidal rivers and also on fresh water for trout. Flyfishing involves actively engaging with nature; reading the water and the tides, figuring out nature’s puzzle and trying to crack the code.
What is your “six-word memoir”? A six-word memoir describes something in just six words.
I can’t wait for what’s next!
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.
View the full article
-
-
Check out these Videos
Recommended Posts
Join the conversation
You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.