APOD: 2026 September 17 – A Treasure Chest in the Carina Nebula

APOD

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

A colorful nebula resembles an open treasure chest on a field of stars

A Treasure Chest in the Carina Nebula

Explanation: This treasure chest is full of stars. The featured image was obtained with NASA‘s James Webb Space Telescope and shows a dust pillar in the Carina Nebula inside our Galaxy, roughly 7500 light-years away. It is formed by interstellar gas and dust, and shaped by powerful stellar winds and radiation from neighboring stars like the nearby Eta Carinae stellar system which is more luminous than 5 million suns. The star formation inside the pillar is excavating its head, creating the open lid of the chest. Astronomers estimate that there are about 70 stars in a compact cluster inside the pillar. This cluster is now thought to be only around 1.3 million years old. Its bounty of young stars includes a massive star approximately 19 times as massive as the Sun. More massive stars are rarer, shine brighter and evolve faster than less massive stars. They are the shiniest jewels in the treasure chest.

APOD’s main NASA site is moving : From apod.nasa.gov to science.nasa.gov/apod
Tomorrow’s picture: what’s next?

Date September 17, 2026
Credit ESA/Webb, NASA & CSA, M. Reiter; Acknowledgement: M. H. Özsaraç
Authors & editors: Cecilia Chirenti, Robert Nemiroff, Jerry Bonnell, Keighley Rockcliffe
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

Source: science.nasa.gov

Indonesia’s Anak Krakatau

A white volcanic plume streams left over a tan ash cloud that fills most of the image. A small green island and blue water are visible in the upper right.
NASA/Michala Garrison

Anak Krakatau erupts ash and volcanic gases in this Sept. 5, 2026, image acquired with the OLI (Operational Land Imager) on Landsat 8. Eruptions are a regular occurrence at Anak Krakatau, a small volcano between the Indonesian islands of Java and Sumatra. Much of its activity remains relatively mild, but it occasionally puts on more impressive and hazardous shows of force. In early September 2026, a booming eruption lasting more than 24 hours sent gas and ash high into the atmosphere, disrupting thousands of flights and degrading air quality in parts of the country, including the capital city of Jakarta.

Learn more about the recent eruption.

Image credit: NASA/Michala Garrison

Source: www.nasa.gov

NASA Watches Earth’s Weight, Finds Center of Mass

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A 3D digital illustration of Earth with a slice cut away to reveal its internal layers. The exterior shows a realistic view of the globe, focusing on Europe, Asia, and Africa with visible geographic features and grid lines.
Water sloshing between the land and oceans shifts Earth’s center of mass relative to its geometric center. NASA scientists have developed a new technique using ultraprecise satellite tracking to estimate the displacement to within fractions of inches.
NASA’s Scientific Visualization Studio

Seasonal changes redistribute enough water around Earth to shift the planet’s center of mass back and forth by fractions of an inch relative to its geometric center. NASA scientists are on the case, tracking the oscillations because Earth’s center of mass is a crucial reference point for satellite navigation and elevation measurements.

A team, led by NASA’s Jet Propulsion Laboratory in Southern California, has proposed a way to calculate the seasonal swings with extreme precision. The technique and findings are detailed in a new study published in Geophysical Journal International. The authors paint a vivid picture of springtime thaws, churning oceans, and dense winter air shifting massive surface loads from season to season.

The study isn’t the first attempt to pin down Earth’s center of mass. Scientists over the decades have pioneered several space-based techniques to define and locate it. But it’s a moving goalpost. If Earth were a hard blue marble, its center of mass would simply overlap its geometric center. In reality, the planet is sloshing and sagging under the weight of water, ice, and air. Because of this, Earth’s center of mass continually swivels around its geometric center by as much as several millimeters.

NASA’s Space Geodesy Project currently uses a variety of space- and land-based techniques to track Earth’s center of mass (also called the geocenter) moving up and down and side to side. This animation traces the millimeter-scale motion from 1993 to 2017.
NASA’s Scientific Visualization Studio

How accurate are existing methods to measure the size of the swivel? The last two international estimates, made in 2017 and 2023, differ by 0.27 inches (7 millimeters), about the height of three stacked nickels. The difference is almost as large as the motion itself.

To reduce uncertainty, JPL geoscientist Donald Argus led the development of a new technique based on ultraprecise satellite tracking.

Driven by gravity, satellites naturally orbit Earth’s center of mass, as if bound by invisible tethers. Tiny changes in the distance between satellites and ground stations reflect Earth’s shifting center of mass.

Using satellites to locate Earth’s center of mass is not a new idea. In fact, dense metal satellites, launched in 1976 and 1992, are dedicated exclusively to this purpose. Resembling 900-pound (408-kilogram) disco balls, both Laser Geodynamics Satellites (LAGEOS 1 and 2) are studded with reflective prisms and tracked with laser precision via ground stations globally distributed across more than 20 countries.

However, one limitation of satellite laser ranging is the uneven distribution of ground stations around Earth. The new technique improves accuracy in two ways: It adds GPS tracking into the mix along with orbital data from several satellites in low Earth orbit to provide a diverse array of targets. And it considers how the weight of water and ice deforms Earth’s crust, taking ground stations along for the ride.

The technique was developed by Argus along with researchers from JPL’s satellite orbit determination team, the University of Nevada, University of Montana, and the Helmholtz Centre for Geosciences in Germany.

“We’re now estimating the size of the movement of Earth’s mass center back and forth each year to be about half of what we believed it to be eight years ago,” said Argus. “Our findings suggest that the mass of Earth’s water and air moving between the hemisphere is smaller than previously thought.”

Felix Landerer, one of the study’s coauthors at JPL, noted that “while these movements might appear tiny, our modern world relies on extremely accurate positioning measurements. By unraveling and understanding the mechanisms that change reference systems, we can build better reference systems that ultimately benefit mapping and navigation — from global shipping logistics to precision agriculture.”

What they found

The study authors tracked Earth’s center of mass oscillating seasonally and attributed the cause to three categories: oceans, atmosphere, and continental water (made up of land ice, snow, lake and river water, soil moisture, and groundwater).

They found that snow accumulation in North America and Eurasia reaches a maximum in March and shifts Earth’s center of mass about 3 millimeters toward the North Pole. A month later, in April, rainwater in the Amazon River basin peaks at 2,400 gigatons, swinging Earth’s center of mass 2.2 millimeters toward South America. Monsoon water in southeast Asia attains a maximum of 600 gigatons six months later in November, adding slightly to the annual oscillation.

Between August and October, the oceans swell with meltwater and rain, and Earth’s center of mass shifts toward the South Pacific Ocean. The Pacific Ocean is so large that mass changes there overshadow the loss or gain in other oceans, though seasonal dynamics in the Mediterranean, Red, North, Baltic, and Barents seas all help shift Earth’s center of mass in their own small way.

The researchers used a model developed by the European Centre for Medium-Range Weather Forecasts to estimate how atmospheric changes affect Earth’s center of mass throughout the seasons. They found that cold, dense, winter air helps tip the scales over Arabia, Asia, and northern Africa around Dec. 21 each year, and over South America and South Africa around June 21.

The mass calculations in the study are consistent with observations made by the Gravity Recovery and Climate Experiment Follow-On (GRACE-FO) mission. Launched in 2018, the mission is made up of twin satellites that map monthly fluctuations in Earth’s gravitational pull due primarily to the mass movement of water above and below ground. The two satellites fly in precise formation, and when the lead satellite passes over a dense body, like a swollen river basin, the extra gravitational tug changes the distance between its twin by a small but measurable amount.

The GRACE-FO mission is a joint partnership between NASA and the German Research Centre for Geosciences (GFZ). The next-generation GRACE-Continuity (GRACE-C) mission is targeting a launch in late 2028 to extend the nearly 25-year GRACE-series data record.

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Written by Sally Younger

2026-061

Source: www.nasa.gov

NASA Visits Schools Strengthening Florida’s Skilled Workforce

NASA recently awarded $10.5 million to seven organizations nationwide through its new State Hubs initiative. Space Florida was selected for Project ORBIT, which aims to expand opportunities for middle and high school students, boost enrollment in key career and technical programs, and create a statewide portal connecting skilled workers with aerospace employers.

Two people looking at a computer screen
Elaine Ho, right, associate administrator for NASA’s Office of STEM Engagement, discusses training software with a student at Lyman High School in Longwood, Florida on on Aug. 27, 2026.
Credit: NASA/Clayton Rougelot

Elaine Ho, associate administrator for NASA’s Office of STEM Engagement, joined local leaders and industry partners recently to see Space Florida Academy students in action at three Central Florida schools. Students at Lyman High School in Longwood, Florida, demonstrated their skills in aerospace engineering, robotics, building trades, welding, and more. Later, in Merritt Island, Florida, Ho and the other leaders stopped by the Aeronautics & Flight Exploration (AFEX) program and cloud computing classrooms at Merritt Island High School and the robotics lab at nearby Edgewood Junior/Senior High School.

Since its launch in August 2024, the Space Florida Academy has expanded from 23 to 42 participating school districts, preparing students for careers in aviation and aerospace, advanced manufacturing, construction, cybersecurity, logistics, and semiconductors.

A group of students posing with Elaine Ho wearing matching t-shirts
Elaine Ho, center, poses for a photo with Space Florida representatives, public school officials, aerospace industry partners, and students at Edgewood Junior/Senior High School in Merritt Island, Florida on Aug. 27, 2026.
Credit: NASA/Clayton Rougelot

“It’s all about showing students what’s possible and then giving them the tools to achieve it,” said Dean Cuke, Merritt Island High School AFEX astronautics and aviation flight instructor. “There are far more possible pathways to be part of the space industry than I think they realize. We’re showing them ways that they can attain that, through learning, through motivation and chasing after their dreams. I’m excited for them.”

Merritt Island High School juniors and student pilots Olivia Street and Troy Wallenburg have both benefited from the program.

“It makes you feel like you’re a part of something way bigger than just a high school class. I learned what I want to do when I grow up – to be a pilot,” Street said.

“My entire life, I’ve just loved space,” Wallenburg said. “It’s great knowing that I’m actually somewhat involved in it, too.”

Elaine Ho sitting in a chair with her hands on controller with a student helping set up the simulator
A student in the Merritt Island High School Aeronautics and Flight Exploration program shows Elaine Ho, left, how to use a flight simulator on Aug. 27, 2026.
Credit: NASA/Clayton Rougelot

“I’m so impressed by how this region holds so many opportunities for our students, who are incredibly capable of solving hard problems, who can build our hardware, who want to be part of something bigger than themselves,” Ho said. “NASA is really focused on ensuring that those opportunities are easier to reach.”

Source: www.nasa.gov

NASA Celebrates Restoration of Guam Station Damaged by Typhoon Mawar 

NASA celebrated the full restoration of its Guam Remote Station with a ribbon-cutting on Sept. 10, closing out more than three years of recovery after Super Typhoon Mawar devastated the site in 2023. Engineers from across the agency completed the final and most complex step of the rebuild on July 1, when they returned the station’s central antenna to service.

Three large white spherical radio antennas at the repaired Guam Remote Station stand behind a security fence on a grassy field. A rainbow arcs through the partly cloudy blue sky behind the antennas.
A rainbow arcs over the newly repaired Guam Remote Station antennas.
NASA

For nearly three decades, the Guam Remote Station has been one of three ground stations supporting NASA’s Tracking and Data Relay Satellites, or TDRS, a critical part of the Near Space Network. From 22,000 miles above Earth, the relays link spacecraft in low Earth orbit with the ground, allowing flight controllers to communicate with astronauts, command spacecraft, and receive mission data. The Guam station alone closes the “Zone of Exclusion,” a stretch of orbit beyond the relays’ line of sight. Without it, the International Space Station can lose contact with Earth for up to 20 minutes of every 90-minute orbit, an unacceptable risk for crewed missions.

On May 24, 2023, the Category 4 super typhoon struck Guam with 185 mph winds and more than 28 inches of rain, destroying two 16.5-meter antennas and damaging an 11-meter north antenna and the Inter Facility Link building at NASA’s station. The Zone of Exclusion reopened for the first time since 1998, cutting TDRS coverage to about 85% of a spacecraft’s orbit.

NASA made emergency repairs to the least-damaged antenna and borrowed two mobile terminals from the U.S. Army to expand coverage. The patchwork restored partial service within months, in time for a November 2023 spacewalk.

In early 2025, Congress dedicated disaster-relief funding to rebuild the ground station and harden the network against future storms. Construction began that summer and finished in summer 2026, when the rebuilt central antenna rejoined TDRS operations and the Zone of Exclusion closed once more. The same appropriation funded critical upgrades at three additional Near Space Network ground stations.

The return to service of the Guam Remote Station’s central antenna represents far more than the restoration of a critical piece of infrastructure — it is a testament to the dedication, resilience, and ingenuity of the people who made it possible.

Jena Garrahy

Jena Garrahy

SCaN Deputy Program Manager for Network Operations

At the ribbon-cutting, representatives from NASA’s SCaN (Space Communications and Navigation) Division joined the station’s workforce and local leaders to mark the central antenna’s return to service. The Guam team, which led debris removal, site security, and on-island recovery, was recognized for its  work to keep NASA connected to its missions through the outage and rebuild. A companion ceremony at NASA’s White Sands Complex in Las Cruces, New Mexico, honored the engineers and specialists across SCaN who supported the recovery off island.

“The return to service of the Guam Remote Station’s central antenna represents far more than the restoration of a critical piece of infrastructure — it is a testament to the dedication, resilience, and ingenuity of the people who made it possible,” said Jena Garrahy, Deputy Program Manager for Network Operations. “Through long days, challenging conditions, and unexpected obstacles, this team remained focused on the missions that depend on these critical assets every day.”

The Near Space Network is funded by SCaN, a division of NASA’s Research and Technology Mission Directorate, at the agency’s Headquarters in Washington. The network is operated out of NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Repairs of the Guam Remote Station were managed out of NASA’s Glenn Research Center in Cleveland.

About the Author

Korine Powers

Korine Powers

Lead Writer and Communications Strategist

Korine Powers, Ph.D. is a writer for NASA's SCaN (Space Communications and Navigation) Program office and covers emerging technologies, commercialization efforts, exploration activities, and more.

Source: www.nasa.gov

Summer Goes Out With a Heat Dome

Air temperatures in the United States are depicted in white to light blue (cooler) and orange to red (warmer). An area of red, indicating temperatures around 100 degrees Fahrenheit, covers Texas and several states to the east and northeast.
An area of high pressure over the south-central U.S. produced unseasonable and, in some places, record-breaking warmth on September 15, 2026, as shown in this map of modeled air temperatures from GEOS (Goddard Earth Observing System).
NASA Earth Observatory/Michala Garrison

While the calendar indicated that astronomical summer was winding down, a swath of the south-central United States was sweltering under a heat dome in mid-September 2026.

This map shows air temperatures in the contiguous U.S. on September 15, 2026, at 4 p.m. Central Time (21:00 Universal Time), modeled at 2 meters (6.5 feet) above the ground. It was produced by combining satellite observations with temperatures predicted by a version of the GEOS (Goddard Earth Observing System) model, which uses mathematical equations to represent physical processes in the atmosphere. The darkest reds indicate areas where temperatures approached or exceeded 40 degrees Celsius (104 degrees Fahrenheit).

More than 41 million people in the U.S.—about 12 percent of the population—were under a National Weather Service extreme heat advisory, extreme heat watch, or extreme heat warning on September 15. The high temperatures spanned large portions of several states, such as Texas, Oklahoma, Arkansas, Missouri, and Tennessee. Meteorologists warned that high humidity, limited cloud cover, and light winds could make temperatures feel higher than thermometer readings and increase the risk of heat-related illnesses.

Several locations set new daily high temperature records on September 15. These included Dallas, Texas, at 101ºF (38ºC), Memphis, Tennessee, at 99ºF (37ºC), and Nashville, Tennessee, at 100ºF (38ºC). The cities were all at least 12ºF warmer than normal that day, with Nashville breaking its daily-high record from 1927. The day before, Nashville also set a record-high minimum temperature of 75ºF (24ºC).

A weather phenomenon meteorologists call a heat dome was responsible for driving temperatures up across the region. A heat dome develops when an area of high pressure in the upper atmosphere pushes hot air toward the surface and traps it there. Heat domes put the brakes on convection and suppress clouds and precipitation. This allows sunlight to reach Earth’s surface relatively unhindered and further elevate air temperatures.

The stretch of unseasonable temperatures follows the warmest June through August in the contiguous United States in a 132-year record, according to NOAA. The three-month period in 2026 was 0.4ºF warmer than the previous records, set in 1936 and 2021.

NASA Earth Observatory image by Michala Garrison, using GEOS-FP data from the Global Modeling and Assimilation Office at NASA GSFC. Story by Lindsey Doermann.

References & Resources

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Heat Dome Broils the Western U.S.

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Source: science.nasa.gov

Curiosity Postcard Celebrates Rover’s 5,000th Day on Mars

2 Min Read

Curiosity Postcard Celebrates Rover’s 5,000th Day on Mars

NASA’s Curiosity rover traverses the rocky, desert landscape of Mars beneath a soft sky. The scene is captured in striking blue and yellow hues.

PIA26700

Credits:
NASA/JPL-Caltech

Description

While parked at a sand ridge nicknamed “Chocolatal,” NASA’s Curiosity Mars rover used its black-and-white navigation cameras to capture panoramas at two times of day. The first was taken on Aug. 30, 2026, at 9:56 a.m. local Mars time; the second was taken on Sep. 2, 2026, at 5:39 p.m. local Mars time. Those dates correspond to the 5,000th and 5,003rd Martian days, or sols, of the mission.

After being sent back to Earth, the two images were merged together. Color was added for an artistic interpretation of the scene, with blue representing the morning panorama and yellow representing the afternoon one. The resulting “postcard” is similar to past examples created with rover images, such as one taken in November 2021.

The rover’s deck can be seen in the foreground, including its can-shaped UHF antenna, used for sending data to orbiting spacecraft, and its finned Multi-Mission Radioisotope Thermoelectric Generator (MMRTG), a nuclear power source, at its rear. The rover’s tracks can be seen trailing off in the distance. 

Curiosity is in the lower foothills of Mount Sharp, a 3-mile-tall (5-kilometer-tall) mountain that sits within Gale Crater. This image looks down toward the crater floor, with the crater rim barely perceptible on the horizon.

Curiosity was built by NASA’s Jet Propulsion Laboratory, which is managed by Caltech in Pasadena, California. JPL leads the mission on behalf of NASA’s Science Mission Directorate in Washington as part of NASA’s Mars Exploration Program portfolio.

To learn more about Curiosity, visit:

https://science.nasa.gov/mission/msl-curiosity/

Source: science.nasa.gov

NASA Astronaut Reid Wiseman to Join NFL Fans in Baltimore

Reid Wiseman looks toward supporters, smiling, wearing an orange spacesuit with his name and a NASA meatball patch.
NASA astronaut Reid Wiseman prepares to depart the Neil A. Armstrong Operations and Checkout Building for Launch Complex 39B at the agency’s Kennedy Space Center in Florida to board NASA’s Artemis II SLS (Space Launch System) rocket and Orion spacecraft for the agency’s Artemis II launch on April 1, 2026.
Credit: NASA/John Kraus

As part of NASA’s new Inspiration Tour, Reid Wiseman, NASA astronaut and commander of the agency’s Artemis II mission, will highlight America’s strengths in space exploration and aeronautics innovation at the Baltimore Ravens vs. New Orleans Saints game in Baltimore on Sunday, Sept. 20.

A Baltimore native, Wiseman is a 27-year Navy veteran and NASA astronaut who spent 175 days in space over two missions. On April 1, Wiseman launched from NASA’s Kennedy Space Center in Florida on a SLS (Space Launch System) rocket as part of the Artemis II mission. Wiseman and his fellow Artemis II crew members completed a historic lunar flyby, marking humanity’s return to the vicinity of the Moon for the first time in more than 50 years.

Wiseman also will be available for media interviews inside the stadium at 12:20 p.m. To RSVP for the media availability, please contact Shaneequa Vereen at: [email protected].

NASA team members will engage with fans at the agency’s Experience Zone, located outside the stadium from 10 a.m. to 1 p.m. before the game. Fans can learn more about NASA’s return to the Moon through the agency’s Artemis program, enjoy interactive games, and capture photos at a selfie station and with a large, inflatable NASA logo.

With stops across the nation, NASA’s Inspiration Tour convenes academic, industry, and public sector stakeholders to connect the agency with the people, technologies, and organizations that drive American leadership in space.

The tour will culminate in MAX POWER, a public exposition of American air and space innovation, Saturday, Nov. 7, and Sunday, Nov. 8, on and near the agency’s Kennedy Space Center in Florida. Held in honor of America’s historic 250th anniversary, the multi-day, family-friendly event will showcase the next-generation aircraft, spacecraft, autonomous vehicles, and technologies that will help define the future of transportation in air and space.

For more information about MAX POWER and the agency’s missions, visit:

https://www.nasa.gov/maxpower

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Camille Gallo / Jessica Taveau
Headquarters, Washington
202-358-1600
[email protected] / [email protected]

Details

Last Updated

Sep 16, 2026

Editor
Jessica Taveau

Source: www.nasa.gov

Travel

5 Min Read

Travel

The NSSC provides travel reimbursement services for all authorized Agency travel including: domestic, foreign, local, ETDY, and Change of Station (COS).

References

Federal Travel Regulations (FTR)
Traveler Extended TDY and Taxes
Domestic Per Diem Rates
Foreign Per Diem Rates

Change of Station

NSSC Travel now has another way that a transferee Traveler may submit his or her vouchers. Please see, submitting Change of Station Process Steps

If traveling CONUS, review: NASA’s Guide to a Successful Move (CONUS)

If traveling OCONUS, review: NASA’s Guide to a Successful Move (OCONUS)

Change of Station References

Change of Station Voucher Information And Samples

Allegiance POC Information

GSA Smart Pay State Tax Information

Change of Station and RITA

Change of Station ServiceNow Instructions

Change of Station Forms

NSSC Change of Station Form

OF 1012 Travel Voucher 

SF 1038 Advance of Funds Application and Account

NF420  Service Agreement-First Duty Station Appointment

NF513 Service Agreement and Duplicate Reimbursement Disclosure Statement OCONUS Employment

NF1204 Employee’s Claim for Damage to, or Loss of, Personal Property Incident to Service

NF1337 Service Agreement-Transferred Employee

NF1338 Employee Application for Reimbursement of Expenses Incurred upon Sale or Purchase (or both) of Residence upon Change of Station

NF1449C  CONUS-Information Covering Persons Transferred or Appointed to First Duty Station

NF1449O OCONUS-Information Covering Persons Transferred or Appointed to First Duty Station

NF1450C CONUS Change of Station Authorization

NF1450O OCONUS Change of Station Authorization

NF1500 Claim for Temporary Quarters Subsistence Expense/Temporary Quarters Subsistence Allowance Reimbursement

NF1807 Househunting Trip Binding Decision

NF1808 Property Management Binding Decision

NF1810 Employee Agreement to Repay Withholding Tax Allowance (WTA)

NF 1811 Temporary Quarters Subsistence Allowance (TQSA)

NF1812 Temporary Quarters Subsistence Allowance (TQSA) Preceding Final Departure

NF1813 Temporary Change of Station (TCS) Duplicate Reimbursement Disclosure Statement

NF1814 Temporary Quarters Subsistence Allowance (TQSA) Predeparture Binding Decision

Related Tax Information:

Check out the latest Taxability Change Notice for Change of Station travelers.
To learn more, see: Relocation Income Tax Allowance Information

Domestic Travel

POV Mileage for NASA Travelers
For Privately Owned Vehicle (POV) Mileage Reimbursement Rates for TDY and ETDY Travel please refer to the GSA Web site: http://www.gsa.gov/mileage   

NASA Domestic Travel: Day that Travel Ends
For the day travel ends (the day a traveler returns to the PDS, home, or other authorized point), the per diem allowance is 75% of M&IE. 

NASA Domestic Travel Rental Car Liability

When making a reservation for a rental car, please remember the Government is only responsible to pay for rental car charges for official travel time.  If a traveler decides to take annual leave in conjunction with official travel and keeps the rental car during annual leave, the portion of the rental rate applicable to annual leave is the responsibility of the traveler.  Please refer to 41 CFR 301-10.453

What is my liability for unauthorized use of a rental automobile obtained with Government funds?

You are responsible for any additional cost resulting from the unauthorized use of a commercial rental automobile for other than official travel-related purposes.

NASA Domestic Travel: Tax Exemption

Prior to traveling, refer to the GSA State Tax Information webpage: https://smartpay.gsa.gov/smarttax. Select your State/US territory of interest to see the exemption status and download the appropriate form, if required.

Extended Temporary Duty (ETDY)

Reduced Per Diem rate

NASA’s standard reduced per diem rate for ETDY travel is 65 percent under the current policy as defined in the NASA Procedural Requirements (NPR) 9750.1-3.1.2.

     a.   Consistent with 41 CFR 301-11.200, an ETDY authorization can include reasonable further reductions from this standard rate or limitations on approved lodging for unique circumstances, to the extent it can be  determined in advance that such will substantially lower costs without mission impact.  For example, if lodging is obtained at 50 percent per diem, the ETDY authorization should be adjusted to authorize a lower rate. 

    b.   The reduced rate of reimbursement begins on the first day of travel regardless of the mode of transportation, except as noted in 3.1.3.  Allowances are covered by the reduced per diem rate; therefore, NASA will authorize the employee a per diem rate (up to 65 percent) to reasonably cover expenses for a one bedroom furnished apartment.  For ETDY greater than 90 days, first consideration should be given to long-term lodging facilities.  Long-term lodging facilities are available on the GSA schedule at http://www.gsa.gov.  If a long-term facility is not selected, proper justification should be provided. 

Find more about Allowable ETDY Expenses Included in Reduced Per Diem Rate, please see the following document: 

Allowable ETDY Expenses Included in Reduced Per Diem Rate

GSA Long-term Lodging (Schedule 48)

GSA’s Schedule 48 is designed for lodging needs of 30 days or more. This program provides housing accommodations for temporary or permanent relocation. Typical facilities include apartment or condominium type properties that may be furnished with all the amenities of a regular home. The current list of vendors is available by clicking on the link above. Most of these properties will accommodate NASA Extended TDY travelers within the 65% reduce per diem rate and will allow use of the government charge card.

Foreign Travel

Please consult the Code of Federal Regulations (CFR), NPR 9710.1, and NPR 9750.1. Please call the NSSC Contact Center using this form for additional information.

Source: www.nasa.gov

NASA’s Webb Reveals Dynamic Panorama of Star Formation

5 Min Read

NASA’s Webb Reveals Dynamic Panorama of Star Formation

A star-forming region. The left two thirds of the image is blanketed in thick clouds of green and yellow gas and dust that form swirling patterns. Some of the gas is spread into thin, thready wisps. The right third of the image is the black background speckled with stars and multi-colored dots that represent distant galaxies. Bright stars are scattered throughout the clouds, with the densest cluster situated in the center of the scene. Each is crowned with six long spikes and two shorter spikes created by the optics of the telescope’s mirrors. In the upper right, a couple of hidden stars blast out long, glowing jets of material that glow in blue.

NASA’s James Webb Space Telescope recently observed IC 348, a star-forming region just 1,000 light-years away from Earth. Webb’s sharp vision revealed tiny brown dwarfs, some just twice Jupiter’s mass, and young stars ejecting powerful jets crashing into surrounding gas and dust.

Credits:
Image: NASA, ESA, CSA, Kevin Luhman (PSU), Catarina Alves de Oliveira (ESA), Mahdi Zamani (ESA/Webb)

This starry view of the nearby star-forming region IC 348 is one of the largest images released to date from NASA’s James Webb Space Telescope. Using Webb, astronomers searched IC 348 for brown dwarfs, which are less massive than the smallest stars. The researchers discovered brown dwarfs just twice the mass of Jupiter, bringing the study of these curious objects into a new mass range and revealing new insights about the star formation process.

The star-forming region IC 348 is located just 1,000 light-years away in the constellation Perseus. In regions like IC 348, cold clouds of molecular hydrogen gas collapse to form new stars, creating glowing, sculpted scenes like this one. The star-formation process can create widely varied objects, from massive stars that expire after only a few million years in core-collapse supernova explosions to the smallest and most common stars, which are long lived and produce powerful stellar storms.

IC 348 (NIRCam Image)

A star-forming region. The left two thirds of the image is blanketed in thick clouds of green and yellow gas and dust that form swirling patterns. Some of the gas is spread into thin, thready wisps. The right third of the image is the black background speckled with stars and multi-colored dots that represent distant galaxies. Bright stars are scattered throughout the clouds, with the densest cluster situated in the center of the scene. Each is crowned with six long spikes and two shorter spikes created by the optics of the telescope’s mirrors. In the upper right, a couple of hidden stars blast out long, glowing jets of material that glow in blue.
NASA’s James Webb Space Telescope recently observed IC 348, a star-forming region just 1,000 light-years away from Earth. Webb’s sharp vision revealed tiny brown dwarfs, some just twice Jupiter’s mass, and young stars ejecting powerful jets crashing into surrounding gas and dust.
Image: NASA, ESA, CSA, Kevin Luhman (PSU), Catarina Alves de Oliveira (ESA), Mahdi Zamani (ESA/Webb)

The smallest stars weigh in at around 8 percent of the Sun’s mass. Below this mass lies a strange class of objects called brown dwarfs. Brown dwarfs form in the same way stars do, through the collapse of molecular clouds. However, unlike stars, the cores of brown dwarfs never become hot enough to fuse ordinary hydrogen into helium (though many briefly fuse deuterium, or heavy hydrogen, early in their lives).

What’s still not clear, and what researchers hoped to learn by using Webb’s sensitive instruments to study IC 348, is how small the smallest objects created by the star-formation process are. In other words, how small is the smallest brown dwarf?

Researchers seeking to answer this question first used Webb to study IC 348 in 2022, when they discovered brown dwarfs with masses as low as three to four times the mass of Jupiter. Now, the same research team has used Webb to probe even deeper into this region in search of even smaller brown dwarfs. 

The team used Webb’s NIRCam (Near-Infrared Camera) in 2024 to capture the warm glow of young brown dwarfs and newborn stars seen in this new image of IC 348. After selecting candidate brown dwarfs based on their colors and brightness, they followed up with Webb’s NIRSpec (Near-Infrared Spectrograph) in 2025 to conduct spectroscopic observations to study the masses of the brown dwarfs.

These deep Webb observations revealed something remarkable to the researchers: brown dwarfs with masses as low as just twice the mass of Jupiter or only 0.19 percent of the Sun’s mass — far smaller than theory predicts brown dwarfs should be. These are the least massive brown dwarfs known and their existence poses a challenge to models of how stars form.

In addition to the discovery of these unexpectedly lightweight brown dwarfs, the Webb observations contained even more surprises. One of the lightest newfound brown dwarfs showed signs of a disk, suggesting that small planets could be forming around an object that is itself only the mass of a planet.

While inspecting the spectra of IC 348’s brown dwarfs, the research team also found a feature they attributed to an unidentified hydrocarbon — molecules made only of hydrogen and carbon atoms. This specific feature has only been seen in the atmospheres of the lowest-mass brown dwarfs, suggesting that these extreme objects might exist in a spectral class of their own.

The stars and brown dwarfs of IC 348 aren’t the only attractions in this image. A brilliantly detailed collection of protostars occupies the upper right corner. Several of these protostars are accompanied by Herbig-Haro objects, which are luminous regions that form when jets from growing newborn stars crash into the gas and dust around the star.

The long, narrow feature that is oriented horizontally in this corner is the Herbig-Haro object HH 797. Upon close inspection, this source is revealed to be two protostars with nearly parallel outflows. Just to the right of HH 797 is the propeller-shaped source HH 211, which features both narrow jets and broader outflows.

IC 348 Collage

A collage, with three large panels along the top and four smaller ones on the bottom. The middle panel on top shows star-forming region IC 348, which has a blanket of thick clouds of yellow and green dust blanketing most of the image. Six boxes are drawn around features in the region, numbered 1–6. The other six panels are numbered and show these features enlarged. They include bright stars throughout the nebula, protostars shooting jets of gas, a distant spiral galaxy, and a gravitational lens.
This collage features a collection of insets from NASA’s James Webb Space Telescope’s image of star-forming region IC 348: embedded stars, a central star cluster, faint outflows, Herbig-Haro objects, gravitational lensing, and spiral galaxies.
Image: NASA, ESA, CSA, Kevin Luhman (PSU), Catarina Alves de Oliveira (ESA), Mahdi Zamani (ESA/Webb)

The data used to create this image comes from the Webb General Observer Program 4866. In addition to studying the lowest-mass objects created through the star-formation process, this program also seeks to understand how the populations of planetary-mass objects like brown dwarfs vary between star-forming regions, as well as the origins of the hydrocarbon feature in the lowest-mass brown dwarfs.

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).

To learn more about Webb, visit:

https://science.nasa.gov/webb

Downloads & Related Information

The following sections contain links to download this article’s images and videos in all available resolutions followed by related information links, media contacts, and if available, research paper and Spanish translation links.

Read more: NASA’s Webb Identifies Tiniest Free-Floating Brown Dwarf

View more: Star cluster IC 348

View more: Brown Dwarfs in IC 348

Read more: Webb Science: Star Lifecycle

View more: Chandra and Webb composite of the star-forming region IC 348

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Details

Last Updated

Sep 15, 2026

Contact

Media

Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
[email protected]

Bethany Downer
ESA/Webb
Baltimore, Maryland

Christine Pulliam
Space Telescope Science Institute
Baltimore, Maryland

Source: science.nasa.gov