Members Can Post Anonymously On This Site
NASA Awards Contract for Infrared Telescope Facility Operations
-
Similar Topics
-
By NASA
1 min read
NASA Science Activation Teams Present at National Rural STEM Summit
NASA Science Activation (SciAct) teams participated in the National Rural STEM (Science, Technology, Engineering, & Mathematics) Summit held June 4-7, 2024 in Tucson, Arizona. Hosted by Kalman Mannis of the Rural Activation and Innovation Network (Arizona Science Center) and the SciTech Institute, the summit fostered learning and sharing among organizations dedicated to creating partnerships and pathways for authentic STEM learning in rural communities.
Participants included:
Matt Cass and Randi Neff from SciAct’s Smoky Mountains STEM Collaborative, who presented “A sense of place: Crafting authentic experiences for rural STEM learners”; Tina Harte from NASA (Science Systems and Applications, Inc), who presented “Nature explorations with NASA”; Kalman Mannis from the SciAct STEM Ecosystems project and the Rural Activation and Innovation Network, who presented “Building leaders in STEM through coaching, connections, and camaraderie”; and members of the SciAct Rural Committee. SciAct STEM Ecosystems is supported by NASA under cooperative agreement award number 80NSSC210007 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
Randi Neff of the NASA SciAct-funded Smoky Mountains STEM Collaborative presents at the National Rural STEM Learning Summit. Arizona Science Center Share
Details
Last Updated Jul 05, 2024 Editor NASA Science Editorial Team Related Terms
Astrophysics Biological & Physical Sciences Earth Science Heliophysics Planetary Science Science Activation Science-enabling Technology Explore More
4 min read NASA’s Webb Captures Celestial Fireworks Around Forming Star
Article
3 days ago
9 min read Behind the Scenes of a NASA ‘Moonwalk’ in the Arizona Desert
Article
4 days ago
3 min read NASA Selects 5 Proposals to Conduct Research Using Openly Available Data in the Physical Sciences Informatics System
Article
7 days ago
Keep Exploring Discover More Topics From NASA
James Webb Space Telescope
Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
Perseverance Rover
This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial…
Parker Solar Probe
On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona…
Juno
NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to…
View the full article
-
By NASA
Firefly Aerospace’s Alpha rocket leaves a glowing trail above the skies of Vandenberg Space Force Base in California on July 3, 2024. Firefly Aerospace/Trevor Mahlmann As part of NASA’s CubeSat Launch Initiative, Firefly Aerospace launched eight small satellites on July 3 aboard the company’s Alpha rocket. Named “Noise of Summer,” the rocket successfully lifted off from Space Launch Complex 2 at Vandenberg Air Force Base in California at 9:04 p.m. PDT.
The CubeSat missions were designed by universities and NASA centers and cover science that includes climate studies, satellite technology development, and educational outreach to students.
Firefly Aerospace completed its Venture-Class Launch Services Demonstration 2 contract with this launch. The agency’s venture-class contracts offer launch opportunities for new providers, helping grow the commercial launch industry and leading to cost-effective competition for future NASA missions.
NASA’s CubeSat Launch Initiative provides a low-cost way for universities, non-profits, science centers, and other researchers to conduct science and technology demonstrations in space.
Image Credit: Firefly Aerospace/Trevor Mahlmann
View the full article
-
By NASA
July 3, 2024
RELEASE: J24-011
Former Chief Astronaut Patrick Forrester NASA NASA astronaut Patrick G. Forrester retired June 29, after a career spanning 31 years of service and three spaceflights. He went on to become chief of NASA’s Astronaut Office, and most recently served as an advisor to the associate administrator for the Space Operations Mission Directorate at NASA Headquarters in Washington.
Forrester joined the agency in 1993 as an aerospace engineer at NASA’s Johnson Space Center in Houston and was selected to become an astronaut in 1996. He dedicated his early career to the assembly of the International Space Station, spending 40 days in space and completing four spacewalks totaling 25 hours and 30 minutes.
“Pat’s dedication and commitment to the advancement of human space exploration over the past three decades has been an inspiration, not just to the Johnson workforce, but the Artemis generation as well,” said NASA’s Johnson Space Center Director Vanessa Wyche. “I want to extend my sincere gratitude to Pat for his outstanding contributions. His legacy will continue to impact the agency and the next generation of explorers for many years to come. Many congratulations to Pat; I wish him all the best in his retirement.”
Forrester launched to the space station for the first time in August 2001 aboard space shuttle Discovery in support of STS-105. Forrester was the mission’s prime robotics operator, helping to install the Leonardo Multi-Purpose Logistics Module that would help deliver 2.7 metric tons of supplies to the station. He flew again with STS-117 in June 2007 aboard space shuttle Atlantis, delivering the orbiting laboratory’s second starboard truss and its third set of solar arrays. His final spaceflight, STS-128 aboard Discovery, launched in August 2009. As prime robotics officer, Forrester again installed Leonardo and the crew transferred 18,000 pounds of supplies.
Forrester continued to support the astronaut corps through numerous leadership positions, serving as technical assistant to the director of Flight Crew Operations. He was a crew representative of robotics development on the space station and shuttle training and onboard crew procedures. Forrester also held the role of spacecraft communicator, or CAPCOM, for both station and shuttle missions.
In 2017, Forrester became chief of the Astronaut Office, overseeing the first flights of NASA’s Commercial Crew Program and helping develop the initial architecture for the agency’s Artemis campaign. In 2020, he stepped down from his chief position, handing over to NASA astronaut Reid Wiseman.
“Pat’s leadership was instrumental during a time where NASA was just starting to launch our astronauts from American soil again,” said Norm Knight, director of flight operations at NASA Johnson. “I admire his courage, his tenacity, and his character during such a dynamic time in our history, and I thank him for laying a strong foundation, not just in his role as chief astronaut, but through his career in human spaceflight. To me, he is a mentor and a friend, and I wish him all the best.”
At the time of his retirement, Forrester supported the Space Operations Mission Directorate, serving as the director of the Cross-Directorate Technical Integration Office and an adviser to the directorate’s associate administrator and fellow NASA astronaut Ken Bowersox.
“Pat is an incredible leader who has provided invaluable service to NASA’s astronaut corps and human spaceflight during his career,” said Ken Bowersox, associate administrator for space operations at NASA. “In the Space Operations Mission Directorate, his influence will be felt long after his departure as we continue to work every day in low Earth orbit and prepare for the future near Earth, at the Moon, Mars and into the solar system.”
An El Paso, Texas, native, Forrester earned a bachelor of science degree in applied sciences and engineering from the U.S. Military Academy, West Point, New York, and a master of science in mechanical and aerospace engineering from the University of Virginia, Charlottesville. A retired colonel in the U.S. Army, Forrester logged more than 5,300 hours of flight time in over 50 different aircraft as an operational aviator and test pilot, retiring in 2005.
“It has been an honor to serve our nation as a member of the NASA family. Many of the stories I will tell for the rest of my life will be related to my experiences here,” said Forrester. “I look forward to watching my friends and colleagues circle the Moon and eventually land on its surface – with the help of all those serving faithfully on the ground. I am forever grateful.”
Read Forrester’s full biography at:
https://go.nasa.gov/45NnfUA
-end-
Chelsey Ballarte
Johnson Space Center, Houston
281-483-5111
chelsey.n.ballarte@nasa.gov
View the full article
-
By NASA
Credits: NASA NASA has selected Space Exploration Technologies Corporation (SpaceX) of Hawthorne, California, to provide launch services for the COSI (Compton Spectrometer and Imager) mission.
The firm-fixed-price contract has a value of approximately $69 million, which includes launch services and other mission related costs. The COSI mission currently is targeted to launch August 2027 on a SpaceX Falcon 9 rocket from Cape Canaveral Space Force Station.
This wide-field gamma-ray telescope will study energetic phenomena in the Milky Way and beyond, including the creation and destruction of matter and antimatter and the final stages of the lives of stars. NASA’s COSI mission will probe the origins of the Milky Way’s galactic positrons, uncover the sites of nucleosynthesis in our galaxy, perform studies of gamma-ray polarization, and find counterparts to multi-messenger sources. The compact Compton telescope combines improved sensitivity, spectral resolution, angular resolution, and sky coverage to facilitate groundbreaking science.
The mission is a collaboration between the University of California, Berkeley’s Space Sciences Laboratory, the University of California, San Diego, the Naval Research Laboratory, NASA’s Goddard Space Flight Center, and Northrop Grumman.
The COSI principal investigator-led project management team is located at the University of California, Berkeley. NASA’s Astrophysics Explorers Program at Goddard Space Flight Center in Greenbelt, Maryland, supports development of the project for the Astrophysics Division within NASA’s Science Mission Directorate. NASA’s Launch Services Program at the Kennedy Space Center in Florida is responsible for program management of the launch services.
For more information about COSI, visit:
https://science.nasa.gov/mission/cosi/
-end-
Tiernan Doyle
Headquarters, Washington
202-358-1600
tiernan.doyle@nasa.gov
Patti Bielling
Kennedy Space Center, Florida
321-501-7575
patricia.a.bielling@nasa.gov
Share
Details
Last Updated Jul 02, 2024 LocationNASA Headquarters Related Terms
COSI (Compton Spectrometer and Imager) Astrophysics Division Astrophysics Explorers Program Science Mission Directorate Space Operations Mission Directorate View the full article
-
By NASA
4 Min Read NASA’s Webb Captures Celestial Fireworks Around Forming Star
L1527, shown in this image from NASA’s James Webb Space Telescope’s MIRI (Mid-Infrared Instrument). The colors within this mid-infrared image reveal details about the central protostar’s behavior.
The cosmos seems to come alive with a crackling explosion of pyrotechnics in this new image from NASA’s James Webb Space Telescope. Taken with Webb’s MIRI (Mid-Infrared Instrument), this fiery hourglass marks the scene of a very young object in the process of becoming a star. A central protostar grows in the neck of the hourglass, accumulating material from a thin protoplanetary disk, seen edge-on as a dark line.
The protostar, a relatively young object of about 100,000 years, is still surrounded by its parent molecular cloud, or large region of gas and dust. Webb’s previous observation of L1527, with NIRCam (Near-Infrared Camera), allowed us to peer into this region and revealed this molecular cloud and protostar in opaque, vibrant colors.
Image A: L1527 – Webb/MIRI
L1527, shown in this image from NASA’s James Webb Space Telescope’s MIRI (Mid-Infrared Instrument), is a molecular cloud that harbors a protostar. It resides about 460 light-years from Earth in the constellation Taurus. The more diffuse blue light and the filamentary structures in the image come from organic compounds known as polycyclic aromatic hydrocarbons (PAHs), while the red at the center of this image is an energized, thick layer of gases and dust that surrounds the protostar. The region in between, which shows up in white, is a mixture of PAHs, ionized gas, and other molecules. This image includes filters representing 7.7 microns light as blue, 12.8 microns light as green, and 18 microns light as red.
Both NIRCam and MIRI show the effects of outflows, which are emitted in opposite directions along the protostar’s rotation axis as the object consumes gas and dust from the surrounding cloud. These outflows take the form of bow shocks to the surrounding molecular cloud, which appear as filamentary structures throughout. They are also responsible for carving the bright hourglass structure within the molecular cloud as they energize, or excite, the surrounding matter and cause the regions above and below it to glow. This creates an effect reminiscent of fireworks brightening a cloudy night sky. Unlike NIRCam, however, which mostly shows the light that is reflected off dust, MIRI provides a look into how these outflows affect the region’s thickest dust and gases.
The areas colored here in blue, which encompass most of the hourglass, show mostly carbonaceous molecules known as polycyclic aromatic hydrocarbons. The protostar itself and the dense blanket of dust and a mixture of gases that surround it are represented in red. (The sparkler-like red extensions are an artifact of the telescopes’s optics). In between, MIRI reveals a white region directly above and below the protostar, which doesn’t show as strongly in the NIRCam view. This region is a mixture of hydrocarbons, ionized neon, and thick dust, which shows that the protostar propels this matter quite far away from it as it messily consumes material from its disk.
As the protostar continues to age and release energetic jets, it’ll consume, destroy, and push away much of this molecular cloud, and many of the structures we see here will begin to fade. Eventually, once it finishes gathering mass, this impressive display will end, and the star itself will become more apparent, even to our visible-light telescopes.
The combination of analyses from both the near-infrared and mid-infrared views reveal the overall behavior of this system, including how the central protostar is affecting the surrounding region. Other stars in Taurus, the star-forming region where L1527 resides, are forming just like this, which could lead to other molecular clouds being disrupted and either preventing new stars from forming or catalyzing their development.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).
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.
Media Contacts
Laura Betz – laura.e.betz@nasa.gov, Rob Gutro – rob.gutro@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Hanna Braun hbraun@stsci.edu Christine Pulliam – cpulliam@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Related Information
ARTICLE/IMAGE: Webb’s previous observation of L1527, with NIRCam (Near-Infrared Camera)
VIDEO: Fly-through the star-forming Pillars of Creation
INTERACTIVE: Explore star formation via a multi-wavelength view of Herbig-Haro 46/47
POSTER: L1527 NIRCam poster
VIDEO: Science Snippets Video: Dust and the formation of Planetary Systems
More Webb News
More Webb Images
Webb Mission Page
Related For Kids
What is a nebula?
What is the Webb Telescope?
SpacePlace for Kids
En Español
¿Qué es una nebulosa?
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…
Galaxies
Stars
Universe
Share
Details
Last Updated Jul 02, 2024 Editor Stephen Sabia Contact Laura Betz laura.e.betz@nasa.gov Related Terms
Astrophysics James Webb Space Telescope (JWST) Nebulae Protostars Science & Research Star-forming Nebulae Stars The Universe
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.