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By NASA
JPL is a research and development lab federally funded by NASA and managed by Caltech. NASA/JPL-Caltech Workforce statement and memo to employees
JPL statement issued on Nov. 12, 2024:
While we have taken various measures to meet our current FY’25 budget allocation, we have reached the difficult decision to reduce the JPL workforce through layoffs. This reduction affects approximately 325 of our colleagues, an impact of about 5% of our workforce. The impacts are occurring across technical, business, and support areas of the Laboratory. These are painful but necessary adjustments that will enable us to adhere to our budget while continuing our important work for NASA and our nation.
The following is a memo sent earlier today from JPL Director Laurie Leshin to employees:
Dear Colleagues,
This is a message I had hoped not to have to write. I’m reaching out to share the difficult news that JPL will be taking a workforce action tomorrow, Nov. 13, resulting in a layoff of approximately 325 of our colleagues, or ~5% of our workforce. Despite this being incredibly difficult for our community, this number is lower than projected a few months ago thanks in part to the hard work of so many people across JPL. The workforce assessment conducted as part of this process has been both extensive and thorough, and although we can never have perfect insight into the future, I sincerely believe that after this action we will be at a more stable workforce level moving forward.
How we got here:
During our last town hall, I discussed our continued funding challenges and projections of what the potential impact on our workforce could look like. I shared that we had been working through multiple workforce scenarios to address the dynamic funding environment, and that we have been doing everything we can, in partnership with our colleagues at NASA and elsewhere, to minimize adverse effects on JPL’s capabilities and team.
Unfortunately, despite all these efforts, we need to make one further workforce reduction to meet the available funding for FY’25. This reduction is spread across essentially all areas of the Lab including our technical, project, business, and support areas. We have taken seriously the need to re-size our workforce, whether direct-funded (project) or funded on overhead (burden). With lower budgets and based on the forecasted work ahead, we had to tighten our belts across the board, and you will see that reflected in the layoff impacts.
As part of our workforce assessment and determining where reductions are being made, we have taken time to complete a full review of our competencies, future mission needs, and we have established guidance for our core capabilities across the Laboratory. We have worked closely with the Executive Council, division managers, project leadership and others to ensure we maintain the appropriate levels of technical expertise, capacity for innovation, and ability to deliver on an exciting future for JPL. Our focus will continue to be on empowering managers to support their teams through this action and equipping all of us with a variety of resources as we move forward together.
Here are the details about what will happen tomorrow:
Unless notified otherwise, all employees are required to work from home tomorrow Nov. 13, regardless of their telework status. Tomorrow you will be invited to a short, virtual, Lab-wide meeting with myself and Deputy Director Leslie Livesay at 9:30 a.m. We will relay the details of where we are in the process and what to expect. Please look out for the meeting notification that will follow this memo. There will not be organization-level notification meetings as in February. This one meeting will provide the information needed for the entire Lab at once.
Our approach is to prioritize notifying everyone via email as quickly as possible whether their role is being affected by the layoff or not. Then we can rapidly shift to providing personalized support to our laid-off colleagues who are part of the workforce reduction, including offering dedicated time to discuss their benefits, and several other forms of assistance. Because of system limitations, the individual email notifications will take place over several hours tomorrow. A schedule of the notifications, which will occur by organization, will be shared in the virtual briefing tomorrow morning and also posted on JPL Space, the JPL HR Website, and Slack. You can also find answers to Frequently Asked Questions (FAQs) on our website here.
Our JPL Community:
I know the absence of our colleagues will be acutely felt, especially after a very challenging year for the Lab. To those leaving JPL as a result of this action, we are grateful for your many vital contributions to JPL and to NASA. We will be here to support you during this time to ensure this transition is as smooth as possible.
To reiterate to you all, I believe this is the last cross-Lab workforce action we will need to take in the foreseeable future. After this action, we will be at about 5,500 JPL regular employees. I believe this is a stable, supportable staffing level moving forward. While we can never be 100% certain of the future budget, we will be well positioned for the work ahead. This may not help much in this difficult moment, but I do want to be crystal clear with my thoughts and perspective. If we hold strong together, we will come through this, just as we have done during other turbulent times in JPL’s nearly 90-year history. Finally, even though the coming leadership transition at NASA may introduce both new uncertainties and new opportunities, this action would be happening regardless of the recent election outcome.
While I know many of us are feeling anger or disappointment with this news, I encourage everyone to act with grace and empathy toward one another, and to lean on each other for support. I will be speaking with you again very soon to discuss our path ahead. Until then, know that we are an incredibly strong organization – our dazzling history, current achievements, and relentless commitment to exploration and discovery position us well for the future.
Laurie
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Last Updated Nov 12, 2024 Related Terms
Jet Propulsion Laboratory Explore More
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By NASA
MuSat2 at Vandenberg Air Force Base, prior to launch. MuSat2 leverages a dual-frequency science antenna developed with support from NASA to measure phenomena such as ocean wind speed. Muon Space A science antenna developed with support from NASA’s Earth Science Technology Office (ESTO) is now in low-Earth orbit aboard MuSat2, a commercial remote-sensing satellite flown by the aerospace company Muon Space. The dual-frequency science antenna was originally developed as part of the Next Generation GNSS Bistatic Radar Instrument (NGRx). Aboard MuSat2, it will help measure ocean surface wind speed—an essential data point for scientists trying to forecast how severe a burgeoning hurricane will become.
“We’re very interested in adopting this technology and pushing it forward, both from a technology perspective and a product perspective,” said Jonathan Dyer, CEO of Muon.
Using this antenna, MuSat2 will gather signals transmitted by navigation satellites as they scatter off Earth’s surface and back into space. By recording how those scattered navigation signals change as they interact with Earth’s surface, MuSat2 will provide meteorologists with data points they can use to study severe weather.
“We use the standard GPS signals you know—the navigation signals that work for your car and your cell phone,” explained Chris Ruf, director of the University of Michigan Space Institute and principal investigator for NGRx.
Ruf designed the entire NGRx system to be an updated version of the sensors on NASA’s Cyclone Global Navigation Satellite System (CYGNSS), another technology he developed with support from ESTO. Since 2016, data from CYGNSS has been a critical resource for people dedicated to forecasting hurricanes.
The science antenna aboard MuSat2 enables two key improvements to the original CYGNSS design. First, the antenna allows MuSat2 to gather measurements from satellites outside the U.S.-based GPS system, such as the European Space Agency’s Galileo satellites. This capability enables MuSat2 to collect more data as it orbits Earth, improving its assessments of conditions on the planet’s surface.
Second, whereas CYGNSS only collected cross-polar radar signals, the updated science antenna also collects co-polar radar signals. This additional information could provide improved information about soil moisture, sea ice, and vegetation. “There’s a whole lot of science value in looking at both polarization components scattering from the Earth’s surface. You can separate apart the effects of vegetation from the effects of surface, itself,” explained Ruf.
Hurricane Ida, as seen from the International Space Station. NASA-developed technology onboard MuSat2 will help supply the U.S. Air Force with critical data for producing reliable weather forecasts. NASA For Muon Space, this technology infusion has been helpful to the company’s business and science missions. Dallas Masters, Vice President of Muon’s Signals of Opportunity Program, explains that NASA’s investments in NGRx technology made it much easier to produce a viable commercial remote sensing satellite. According to Masters, “NGRx-derived technology allowed us to start planning a flight mission early in our company’s existence, based around a payload we knew had flight heritage.”
Dyer agrees. “The fact that ESTO proves out these measurement approaches – the technology and the instrument, the science that you can actually derive, the products from that instrument – is a huge enabler for companies like ours, because we can adopt it knowing that much of the physics risk has been retired,” he said.
Ultimately, this advanced antenna technology for measuring ocean surface wind speed will make it easier for researchers to turn raw data into actionable science products and to develop more accurate forecasts.
“Information is absolutely precious. When it comes to forecast models and trying to understand what’s about to happen, you have to have as good an idea as you can of what’s already happening in the real world,” said oceanographer Lew Gramer, an Associate Scientist with the Cooperative Institute For Marine And Atmospheric Studies and NOAA’s Hurricane Research Division.
Project Lead: Chris Ruf, University of Michigan
Sponsoring Organizations: NASA’s Earth Science Technology Office and Muon Space
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Last Updated Nov 12, 2024 Related Terms
CYGNSS (Cyclone Global Navigation Satellite System) Earth Science Earth Science Division Earth Science Technology Office Oceans Science-enabling Technology Technology Highlights Explore More
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By NASA
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Preparations for Next Moonwalk Simulations Underway (and Underwater)
Candeska Cikana Community College uses selective laser sintering, a type of 3D-printing in which heat and pressure form specific structures using layers of powdered material. Shown here, a student works to remove excess material, in this case a powdered form of nylon with carbon fibers, to reveal a prototype of the “Mapi Hapa,” or “sky shoe.” Candeska Cikana Community College Human exploration on the lunar surface is no small feat. It requires technologists and innovators from all walks of life to tackle many challenges, including feet.
From designing astronaut boots, addressing hazardous Moon dust, and researching new ways to land on Mars, NASA is funding valuable research through M-STAR (Minority University Research and Education Project’s (MUREP) Space Technology Artemis Research). The M-STAR program provides opportunities for students and faculty at Minority Serving Institutions to participate in space technology development through capacity building and research grants. With more than $11.5 million awarded since 2020, M-STAR aims to ensure NASA isn’t leaving any potential solution behind.
Best Foot Forward
Nicholas Bitner from Candeska Cikana Community College, left, and Jesse Rhoades from the University of North Dakota (UND), right, are pictured in UND’s BiPed lab, where their students test and capture motion data for the Mapi Hapa. Walter Criswell, UND Today Supportive boots are required for astronauts who will perform long duration Artemis missions on the Moon. With astronaut foot health in mind, students and faculty of North Dakota’s Candeska Cikana Community College in Fort Totten and the University of North Dakota in Grand Forks are designing a solution for extravehicular activity Moon boots. The project, called Mapi Hapa, proposes a 3D printed device that helps astronauts achieve the range of motion that takes place in the ankle when you draw your toe back towards the shin.
Candeska Cikana Community College is a tribal college that serves the Spirit Lake Nation, including the Dakota, Lakota, Sisseton, Wahpeton, and Yanktonai peoples.
Nicholas Bitner, an instructor at Candeska Cikana and graduate student at the University of North Dakota, notes the unique skills that tribal students possess. “Their perspective, which is unlike that of any other student body, thrives on building with their hands and taking time to make decisions.”
Bitner also attributes many opportunities and successes of their program to M-STAR and its partnership which exemplifies the dire importance of consistent funding.
“Given the relationships, we have been able to expand our capabilities and our lab, but it has also given us funding. We were able to hire all our students in the engineering department as lab technicians. So, they get paid to do the research that they are a part of, and not only do they have that psychological ownership, but they also have a good paying job that looks nice on their resumes.”
In addition to addressing astronaut foot health, M-STAR funding is helping develop solutions to combat lunar regolith, or Moon dust, which can damage landers, spacesuits, and human lungs, if inhaled.
Lunar Dust Development
With M-STAR, New Mexico State University in Las Cruces developed affordable, reliable lunar regolith simulants to help test lunar surface technologies. The team also designed testing facilities that mimic environmental conditions on the Moon.
New Mexico State has already started sharing their simulants, including with a fellow M-STAR awardee. An M-STAR project selected in 2023 from the University of Maryland Eastern Shore in Princess Anne uses the simulants to help test their experience in smart agriculture to test applications for crop production on the Moon.
University of Maryland, Eastern Shore explores the possibility of growing crops in lunar regolith by mixing varying proportions of lunar regolith simulant, horse manure, and potting soil. The lunar regolith simulant was provided by fellow M-STAR awardee at New Mexico State University in in Las Cruces.Stephanie Yeldell/NASA Douglas Cortez, associate professor in civil engineering at New Mexico State, believes different perspectives are essential to maximizing solutions.
“There are hundreds of people working at Minority Serving Institutions that are used to looking at the world in a completely different way,” said Cortez. “When they start looking at the same problem and parameters, they come up with very different solutions.”
As we look to sustainable presence on the Moon, NASA also has its sights set on Mars and M-STAR is helping develop technologies to inform crewed Martian exploration.
Stick the Landing
San Diego State University in California was awarded funding for research on Mars entry, descent, and landing technologies. The team aims to achieve optimal trajectory by developing onboard algorithms that guide vehicles to descent autonomously.
The M-STAR research opportunities have been invaluable to students like Chris Davami and his teammates working to develop improved methods to land on Mars.
Christopher Davami, who supported San Diego State University’s 2021 M-STAR project, is pictured here at NASA’s Langley Research Center, where he was selected for internships supporting research in aeroelasticity, atmospheric flight, and entry systems research.NASA “I would definitely not have been able to have these opportunities with NASA if it weren’t for M-STAR,” said Davami. “M-STAR helped pay for my education, which helped me save a lot in student loans. I probably wouldn’t be going to graduate school right now if I did not have this opportunity. This program enabled me to keep pursuing my research and continue doing what I love.”
Following his contributions to the M-STAR-funded project, Davami was awarded a NASA Space Technology Graduate Research Opportunity in 2023 on his work in autonomous end-to-end trajectory planning and guidance constrained entry and precision power decent.
Through efforts like M-STAR, NASA aims to seed the future workforce and prepare colleges and universities to win other NASA research opportunities. When it comes to the advancement of space technology, people of different backgrounds and skillsets are needed to achieve what was once known as impossible. Not only can the diversification of ideas spark fundamental innovations in space, but it can also help students apply these technological advancements to solving problems here on Earth.
To learn more about M-STAR visit:
https://go.nasa.gov/442k76s
by: Gabrielle Thaw, NASA’s Space Technology Mission Directorate
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Last Updated Nov 05, 2024 EditorLoura Hall Related Terms
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By NASA
In August, the Association for Advancing Participatory Sciences (AAPS) announced a fellowship opportunity in partnership with the NASA Citizen Science Leaders Series. Fifty-five people applied! The applications came from graduate students and early career professionals in diverse disciplines, including astronomy, ecology, engineering, nursing, policy, and zoology, to name a few.
Sadie Coffin, AAPS-NASA Cit Sci Leaders Fellow. (Credit: Olivia Schlichtkrull)
We are delighted to announce that Sadie Coffin, PhD student and co-lead (alongside her advisor, Dr. Jeyhan Kartaltepe) of the Redshift Wrangler project, will serve as the AAPS-NASA Cit Sci Leaders Fellow. Sadie’s task is to curate resources, advice, and best practices on topics of common interest from four years of NASA Cit Sci Leaders events. Sadie will dig into our recordings to find the moments, speakers, advice, and resources that offer the best guidance for project leaders starting or managing projects. She’ll help package the best elements of the recordings into usable formats for busy scientists and project leaders interested in creating, managing, and improving participatory science projects.
“This fellowship offers a unique opportunity to gain the mentorship and expertise I need to build a career that not only advances research but also fosters public engagement and inclusivity in science,” said Sadie.
The enthusiasm, talent, and passion in the applications we received revealed the broad appeal, utility, and growing acceptance of participatory research. One applicant commented, “Working in the participatory sciences is how I find meaning in my career as a researcher.” Many others commented that they were eager to connect with mentors and colleagues who were as invested in this work as they were.
Thank you to everyone who applied for this fellowship and to all of the early career professionals working in this field. You are inspiring, and we can’t wait to see what big ideas you contribute to the growth of this field! AAPS will announce additional fellowships focused on different projects in the coming months. Please watch for upcoming calls, consider applying yourself, and share them with the inspiring early career individuals in your networks!
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Last Updated Nov 04, 2024 Related Terms
Astrophysics Biological & Physical Sciences Citizen Science Earth Science Heliophysics Planetary Science Explore More
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Preparations for Next Moonwalk Simulations Underway (and Underwater)
Francisco Rodriguez (aircraft mechanic) services liquid oxygen or LOX on the ER-2 during the Geological Earth Mapping Experiment (GEMx) research project. Experts like Rodriguez sustain a high standard of safety on airborne science aircraft like the ER-2 and science missions like GEMx. The ER-2 is based out of NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Steve Freeman Operating at altitudes above 99% of the Earth’s atmosphere, NASA’s ER-2 aircraft is the agency’s highest-flying airborne science platform. With its unique ability to observe from as high as 65,000 feet, the ER-2 aircraft is often a platform for Earth science that facilitates new and crucial information about our planet, especially when the plane is part of collaborative and multidisciplinary projects.
“We’re deploying instruments and people everywhere from dry lakebeds in the desert to coastal oceans and from the stratosphere to marine layer clouds just above the surface,” said Kirk Knobelspiesse, an atmospheric scientist at NASA’s Goddard Space Flight Center. “We live on a changing planet, and it is through collaborative projects that we can observe and understand those changes.”
One mission that recently benefitted from the ER-2’s unique capabilities is the Plankton, Aerosol, Cloud, ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) project. The PACE-PAX mission uses the ER-2’s capabilities to confirm data collected from the PACE satellite, which launched in February 2024.
The PACE observatory is making novel measurements of the ocean, atmosphere, and land surfaces, noted Knobelspiesse, the mission scientist for PACE-PAX. This mission is all about checking the accuracy of those new satellite measurements.
Sam Habbal (quality inspector), Darick Alvarez (aircraft mechanic), and Juan Alvarez (crew chief) work on the network “canoe” on top of the ER-2 aircraft, which provides network communication with the pilot onboard. Experts like these sustain a high standard of safety while outfitting instruments onboard science aircraft like the ER-2 and science missions like the Plankton, Aerosol, Cloud, ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) mission. The ER-2 is based out of NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Genaro Vavuris “The ER-2 is the ideal platform for PACE-PAX because it’s about the closest we can get to putting instruments in orbit without actually doing so,” Knobelspiesse said.
The collaborative project includes a diverse team of researchers from across NASA, plus the National Oceanic and Atmospheric Administration (NOAA), the Netherlands Institute for Space Research (SRON), the University of Maryland, Baltimore County, the Naval Postgraduate School, and other institutions.
Similarly, the Geological Earth Mapping eXperiment (GEMx) science mission is using the ER-2 over multiple years to collect observations of critical mineral resources across the Western United States.
“Flying at this altitude means the GEMx mission can acquire wide swaths of data with every overflight,” said Kevin Reath, NASA’s associate project manager for the GEMx mission, a collaboration between the United States Geological Survey (USGS) and NASA.
The ER-2 conducted over 80 flight hours in service of the Plankton, Aerosol, Cloud, ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) mission. The ER-2 is uniquely qualified to conduct the high-altitude scientific flights that this project required, and is based at NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Genaro Vavuris The GEMx team collects visible, shortwave infrared, and thermal infrared data using instruments installed onboard the ER-2. Combining these instruments with the aircraft’s capability to fly at high altitudes bears promising results.
“The dataset being produced is the largest airborne surface mineralogy dataset captured in a single NASA campaign,” Reath said. “These data could help inform federal, tribal, state, and community leaders to make decisions that protect or develop our environment.”
Learn more about the ER-2 aircraft.
Learn more about the PACE-PAX mission.
Learn more about the GEMx mission.
Learn more about NASA’s Airborne Science Program.
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Last Updated Oct 24, 2024 EditorDede DiniusContactErica HeimLocationArmstrong Flight Research Center Related Terms
Armstrong Flight Research Center Airborne Science Earth Science Earth's Atmosphere ER-2 PACE (Plankton, Aerosol, Cloud, Ocean Ecosystem) Science Mission Directorate Explore More
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