NASA Analysis Shows Irreversible Sea Level Rise for Pacific Islands

NASA Analysis Shows Irreversible Sea Level Rise for Pacific Islands

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Overhead view of Pacific Island nation Kiribati
Pacific Island nations such as Kiribati — a low-lying country in the southern Pacific Ocean — are preparing now for a future of higher sea levels.
NASA Earth Observatory

Climate change is rapidly reshaping a region of the world that’s home to millions of people.

In the next 30 years, Pacific Island nations such as Tuvalu, Kiribati, and Fiji will experience at least 8 inches (15 centimeters) of sea level rise, according to an analysis by NASA’s sea level change science team. This amount of rise will occur regardless of whether greenhouse gas emissions change in the coming years.

The sea level change team undertook the analysis of this region at the request of several Pacific Island nations, including Tuvalu and Kiribati, and in close coordination with the U.S. Department of State.

In addition to the overall analysis, the agency’s sea level team produced high-resolution maps showing which areas of different Pacific Island nations will be vulnerable to high-tide flooding — otherwise known as nuisance flooding or sunny day flooding — by the 2050s. Released on Sept. 23, the maps outline flooding potential in a range of emissions scenarios, from best-case to business-as-usual to worst-case.

“Sea level will continue to rise for centuries, causing more frequent flooding,” said Nadya Vinogradova Shiffer, who directs ocean physics programs for NASA’s Earth Science Division. “NASA’s new flood tool tells you what the potential increase in flooding frequency and severity look like in the next decades for the coastal communities of the Pacific Island nations.”

Team members, led by researchers at the University of Hawaii and in collaboration with scientists at the University of Colorado and Virginia Tech, started with flood maps of Kiribati, Tuvalu, Fiji, Nauru, and Niue. They plan to build high-resolution maps for other Pacific Island nations in the near future. The maps can assist Pacific Island nations in deciding where to focus mitigation efforts.

“Science and data can help the community of Tuvalu in relaying accurate sea level rise projections,” said Grace Malie, a youth leader from Tuvalu who is involved with the Rising Nations Initiative, a United Nations-supported program led by Pacific Island nations to help preserve their statehood and protect the rights and heritage of populations affected by climate change. “This will also help with early warning systems, which is something that our country is focusing on at the moment.”

Future Flooding

The analysis by the sea level change team also found that the number of high-tide flooding days in an average year will increase by an order of magnitude for nearly all Pacific Island nations by the 2050s. Portions of the NASA team’s analysis were included in a sea level rise report published by the United Nations in August 2024.  

Areas of Tuvalu that currently see less than five high-tide flood days a year could average 25 flood days annually by the 2050s. Regions of Kiribati that see fewer than five flood days a year today will experience an average of 65 flood days annually by the 2050s.

“I am living the reality of climate change,” said Malie. “Everyone (in Tuvalu) lives by the coast or along the coastline, so everyone gets heavily affected by this.” 

Flooding on island nations can come from the ocean inundating land during storms or during exceptionally high tides, called king tides. But it can also result when saltwater intrudes into underground areas and pushes the water table to the surface. “There are points on the island where we will see seawater bubbling from beneath the surface and heavily flooding the area,” Malie added.

Matter of Location

Sea level rise doesn’t occur uniformly around the world. A combination of global and local conditions, such as the topography of a coastline and how glacial meltwater is distributed in the ocean, affects the amount of rise a particular region will experience.

“We’re always focused on the differences in sea level rise from one region to another, but in the Pacific, the numbers are surprisingly consistent,” said Ben Hamlington, a sea level researcher at NASA’s Jet Propulsion Laboratory in Southern California and the agency’s sea level change science team lead.

The impacts of 8 inches (15 centimeters) of sea level rise will vary from country to country. For instance, some nations could experience nuisance flooding several times a year at their airport, while others might face frequent neighborhood flooding equivalent to being inundated for nearly half the year.

Researchers would like to combine satellite data on ocean levels with ground-based measurements of sea levels at specific points, as well as with better land elevation information. “But there’s a real lack of on-the-ground data in these countries,” said Hamlington. The combination of space-based and ground-based measurements can yield more precise sea level rise projections and improved understanding of the impacts to countries in the Pacific.  

“The future of the young people of Tuvalu is already at stake,” said Malie. “Climate change is more than an environmental crisis. It is about justice, survival for nations like Tuvalu, and global responsibility.”

To explore the high-tide flooding maps for Pacific Island nations, go to:

https://sealevel.nasa.gov

News Media Contacts

Jane J. Lee / Andrew Wang
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-0307 / 626-379-6874
jane.j.lee@jpl.nasa.gov / andrew.wang@jpl.nasa.gov

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Sep 25, 2024

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Anthony Greicius

­­Robotic Moving ‘Crew’ Preps for Work on Moon 

­­Robotic Moving ‘Crew’ Preps for Work on Moon 

4 Min Read

­­Robotic Moving ‘Crew’ Preps for Work on Moon 

The LANDO system works by using onboard sensors to scan encoded markers (similar to a QR code) on a payload, which will reveal critical information about its position and orientation relative to the LSMS. This information is used to calculate where the robotic arm exists in space and plan the motion path to pick up and move payloads.

Credits:
NASA/David C. Bowman

As NASA moves forward with efforts to establish a long-term presence on the Moon as part of the Artemis campaign, safely moving cargo from landers to the lunar surface is a crucial capability.  

Whether the cargo, also known as payloads, are small scientific experiments or large technology to build infrastructure, there won’t be a crew on the Moon to do all the work, which is where robots and new software come in. 

A team at NASA’s Langley Research Center in Hampton, Virginia, spent the last couple of years infusing existing robotic hardware with a software system that makes the robot operate autonomously. Earlier this month, that team, led by researcher Dr. Julia Cline of NASA Langley’s Research Directorate, ran demonstrations of their system called LANDO (Lightweight Surface Manipulation System AutoNomy capabilities Development for surface Operations and construction). 

LANDO prepares to move its payload to a safe spot on the simulated lunar surface.
NASA/David C. Bowman

The demos took place in an area set up to look like the Moon’s surface, complete with fake boulders and a model lunar lander. During the first demo, the team placed the payload, a small metal box, on a black pedestal. The robotic arm stretched over the scene, with its dangling hook poised to grasp the box.

As the team huddled nearby around computers, sensors on the arm scanned the surrounding area, looking for the metal box, which was outfitted with encoded markers — similar to QR codes — that revealed critical information about its position and orientation relative to the arm. Using a graphic user interface, team member Amelia Scott also chose a location for LANDO to place the payload.

During a series of slow, methodical movements, LANDO transports a payload from a pedestal to a simulated lunar surface.
NASA/Angelique Herring

After locating the metal box and computing a safe path to move it, the arm began a slow, deliberate movement toward its target, coming in at a precise angle that allowed the hook to select a capture point on the payload. Once engaged, the arm slowly lifted the payload from the pedestal, moved right, and gently lowered the payload to the simulated lunar surface. With the payload safely on the surface, the system carefully disengaged the hook from the capture point and returned to its home position. The entire process took a few minutes. Shortly after the first demo was complete, the team did it again, but with a small model rover.  

“What we demonstrated was the repeatability of the system,moving multiple payloads to show that we’re consistently and safely able to get them from point A to point B,” said Cline. “We also demonstrated the Lightweight Surface Manipulation System hardware – the ability to control the system through space and plan a path around obstacles.” 

The system’s successful performance during the September demonstration marks the end of this project, but the first step in developing a larger system to go to the Moon. 

Now that the team has determined how the system should function, Cline believes the next natural step would be to develop and test an engineering design unit on one of the landers going to the Moon as part of NASA’s Commercial Lunar Payload Services (CLPS) initiative. The team is actively looking for industry partners who want to commercialize the capability. 

Through CLPS, NASA is working with commercial companies to deliver science and technology demonstrations to the Moon.  

The work behind LANDO could be directly infused into much larger versions of a lightweight surface manipulation system.

The LANDO team, back row, left to right: Dominic Bisio, Joshua Moser, Walter Waltz, Jacob Martin, Ryan Bowers, Brace White and Iok Wong. And kneeling, left to right: Amelia Scott, Matthew Vaughan, Julia Cline, Jessica Friz and Javier Puig-Navarro.
NASA/Ryan Hill

“The overall control system we’ve developed would apply to larger versions of the technology,” said Cline. “When you think about the payloads we’ll have to offload for on the Moon, like habitats and surface power systems, this is the kind of general-purpose tool that could be used for those tasks.” 

The LANDO system was funded through the Early Career Initiative in NASA’s Space Technology Mission Directorate (STMD). Through STMD, NASA supports and develops transformative space technologies to enable future missions. As NASA embarks on its next era of exploration with the Artemis campaign, STMD is helping advance technologies, developing new systems, and testing capabilities at the Moon that will be critical for crewed missions to Mars. 

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Sep 25, 2024

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Joe Atkinson

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Julia L. Bradshaw

In Odd Galaxy, NASA’s Webb Finds Potential Missing Link to First Stars

In Odd Galaxy, NASA’s Webb Finds Potential Missing Link to First Stars

4 Min Read

In Odd Galaxy, NASA’s Webb Finds Potential Missing Link to First Stars

A black background sprinkled with small, colorful galaxies in orange, blue, and white. On the left, a third of the way down from the top of the image, a very faint dot of a galaxy is outlined with a white square and pulled out in a graphic to be shown magnified. In the pullout square to the right, the galaxy is a hazy white dot edged in orange, with faint blue projections opposite each other at the 11 o’clock and 5 o’clock positions.
What appears as a faint dot in this James Webb Space Telescope image may actually be a groundbreaking discovery. Full image and details below.
Credits:
NASA, ESA, CSA, STScI, Alex Cameron (Oxford)

Looking deep into the early universe with NASA’s James Webb Space Telescope, astronomers have found something unprecedented: a galaxy with an odd light signature, which they attribute to its gas outshining its stars. Found approximately one billion years after the big bang, galaxy GS-NDG-9422 (9422) may be a missing-link phase of galactic evolution between the universe’s first stars and familiar, well-established galaxies.

Image A: Galaxy GS-NDG-9422 (NIRCam Image)

A black background sprinkled with small, colorful galaxies in orange, blue, and white. On the left, a third of the way down from the top of the image, a very faint dot of a galaxy is outlined with a white square and pulled out in a graphic to be shown magnified. In the pullout square to the right, the galaxy is a hazy white dot edged in orange, with faint blue projections opposite each other at the 11 o’clock and 5 o’clock positions.
What appears as a faint dot in this James Webb Space Telescope image may actually be a groundbreaking discovery. Detailed information on galaxy GS-NDG-9422, captured by Webb’s NIRSpec (Near-Infrared Spectrograph) instrument, indicates that the light we see in this image is coming from the galaxy’s hot gas, rather than its stars. Astronomers think that the galaxy’s stars are so extremely hot (more than 140,000 degrees Fahrenheit, or 80,000 degrees Celsius) that they are heating up the nebular gas, allowing it to shine even brighter than the stars themselves.
NASA, ESA, CSA, STScI, Alex Cameron (Oxford)

“My first thought in looking at the galaxy’s spectrum was, ‘that’s weird,’ which is exactly what the Webb telescope was designed to reveal: totally new phenomena in the early universe that will help us understand how the cosmic story began,” said lead researcher Alex Cameron of the University of Oxford.

Cameron reached out to colleague Harley Katz, a theorist, to discuss the strange data. Working together, their team found that computer models of cosmic gas clouds heated by very hot, massive stars, to an extent that the gas shone brighter than the stars, was nearly a perfect match to Webb’s observations.

“It looks like these stars must be much hotter and more massive than what we see in the local universe, which makes sense because the early universe was a very different environment,” said Katz, of Oxford and the University of Chicago.

In the local universe, typical hot, massive stars have a temperature ranging between 70,000 to 90,000 degrees Fahrenheit (40,000 to 50,000 degrees Celsius). According to the team, galaxy 9422 has stars hotter than 140,000 degrees Fahrenheit (80,000 degrees Celsius).

The research team suspects that the galaxy is in the midst of a brief phase of intense star formation inside a cloud of dense gas that is producing a large number of massive, hot stars. The gas cloud is being hit with so many photons of light from the stars that it is shining extremely brightly.

Image B: Galaxy GS-NDG-9422 Spectrum (NIRSpec)

Infographic titled Galaxy GS-NDG-9422, Nebular light outshines starlight. Graphic is divided horizontally with one spectrum on top, labeled Webb Data, and one on bottom, labeled Model Spectrum. A portion of both spectrums about an inch wide is highlighted with a vertical column labeled Slope Feature. There is a clear similarity between the top and bottom graphs, thought the top has more angular lines and the bottom is smoother and rounded. See extended description for more.
This comparison of the data collected by the James Webb Space Telescope with a computer model prediction highlights the same sloping feature that first caught the eye of astronomer Alex Cameron, lead researcher of a new study published in Monthly Notices of the Royal Astronomical Society.

The bottom graphic compares what astronomers would expect to see in a “typical” galaxy, with its light coming predominantly from stars (white line), with a theoretical model of light coming from hot nebular gas, outshining stars (yellow line). The model comes from Cameron’s collaborator, theoretical astronomer Harley Katz, and together they realized the similarities between the model and Cameron’s Webb observations of galaxy GS-NDG-9422 (top). The unusual downturn of the galaxy’s spectrum, leading to an exaggerated spike in neutral hydrogen, is nearly a perfect match to Katz’s model of a spectrum dominated by super-heated gas.

While this is still only one example, Cameron, Katz, and their fellow researchers think the conclusion that galaxy GS-NDG-9422 is dominated by nebular light, rather than starlight, is their strongest jumping-off point for future investigation. They are looking for more galaxies around the same one-billion-year mark in the universe’s history, hoping to find more examples of a new type of galaxy, a missing link in the history of galactic evolution.

NASA, ESA, CSA, Leah Hustak (STScI)

In addition to its novelty, nebular gas outshining stars is intriguing because it is something predicted in the environments of the universe’s first generation of stars, which astronomers classify as Population III stars.

“We know that this galaxy does not have Population III stars, because the Webb data shows too much chemical complexity. However, its stars are different than what we are familiar with – the exotic stars in this galaxy could be a guide for understanding how galaxies transitioned from primordial stars to the types of galaxies we already know,” said Katz.

At this point, galaxy 9422 is one example of this phase of galaxy development, so there are still many questions to be answered. Are these conditions common in galaxies at this time period, or a rare occurrence? What more can they tell us about even earlier phases of galaxy evolution? Cameron, Katz, and their research colleagues are actively identifying more galaxies to add to this population to better understand what was happening in the universe within the first billion years after the big bang.

“It’s a very exciting time, to be able to use the Webb telescope to explore this time in the universe that was once inaccessible,” Cameron said. “We are just at the beginning of new discoveries and understanding.”

The research paper is published in Monthly Notices of the Royal Astronomical Society.

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.

View/Download the research results from the Monthly Notices of the Royal Astronomical Society.

Media Contacts

Laura Betz – laura.e.betz@nasa.gov, Rob Gutrorob.gutro@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Christine Pulliamcpulliam@stsci.edu, Leah Ramsaylramsay@stsci.edu
Space Telescope Science Institute, Baltimore, Md.

Related Information

Read more: “What Were the First Stars Like?”

Watch:Massive Stars: Engines of Creation

Learn about spectroscopy:Spectroscopy 101 – Introduction

Star Lifecycle

More Webb News

More Webb Images

Webb Science Themes

Webb Mission Page

Related For Kids

What is a galaxy?

What is the Webb Telescope?

SpacePlace for Kids

En Español

Ciencia de la NASA

NASA en español 

Space Place para niños

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Sep 24, 2024
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Marty McCoy
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September 2024 Transformer of the Month: Lori Arnett

September 2024 Transformer of the Month: Lori Arnett

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Portrait of Lori Arnett

Lori Arnett approaches her work at NASA with a simple motto: think big, start small, act fast. As the Associate Director for Digital Transformation for the Aerosciences Evaluation and Test Capabilities (AETC) within the Aeronautics Research Mission Directorate (ARMD), she helps manage the capability portfolio for wind tunnels across the agency. In this role and in the many ways she champions digital transformation at NASA, she is unapologetic about the ambitious mindset she brings to the table. “I know that I have a lot of passion around the work I do, and that can sometimes be seen as intimidating to others,” she says. “But I’m going to drive to something. I want to make progress.”

Lori’s approach to achieving big goals and true transformation at NASA begins with small, quantifiable steps. With this strategy, she has significantly impacted the agency’s ability to deliver on its aerospace missions. In response to AETC releasing its strategic plan in June 2022, Lori and her team created a data governance board and strategy for quantifying and measuring success, positioning her mission directorate to achieve its goals on schedule.

Her team successfully defined and captured data on customer data and service quality, reliability, timeliness, and other attributes for operational and maintenance costs for the wind tunnels to create a quantifiable performance metric. To complement performance, they also defined and captured data on the tunnels’ mission relevancy, future demand, test usage, adaptability, and uniqueness for a quantifiable value metric. Together, these metrics create a real-time view of progress toward agency goals for everyone from headquarters program managers to customers to wind tunnel operators. Other NASA capability portfolios have copied the construct, further demonstrating its value.

By making various data available with access controls, Lori and her team drive toward agency-wide transparency and standardization. They created the first-ever integrated view of availability and access data for NASA’s wind tunnels and increased data discoverability by expanding the ARMD Test Data Portal to include ground test data in addition to flight data. Her team is currently working to bring ground and flight test data together with computational data sets—a feat that would provide unprecedented data integration and interoperability in enabling future missions.

To achieve such quick turnaround with minimal budgeting needs, the team partnered with the Office of the Chief Information Officer (OCIO) to leverage existing enterprise-wide services when building the data application ADAPT (AETC Data & Analytics Portfolio Transformation). “I’m all about leveraging and collaborating. I don’t want to reinvent the wheel,” says Lori. Her act-fast mentality drives her toward interoperable architectures, common tools, and inclusive teaming, leveraging existing solutions to help her directorate achieve increasingly complex missions. In return, Lori embraces any opportunity to share her work and enable other teams in their digital transformation journeys. “If anything I do can help somebody else, please reuse it. I don’t do this only for my organization. I’m doing this for the greater good of NASA and for this nation.”

Lori believes that NASA’s ability to drive innovation hinges on how the agency maximizes the impact of its data, specifically in achieving FAIRUST principles. By 2032, AETC strives for 100% of its strategic data assets to be FAIRUST (Findable, Accessible, Interoperable, Reusable, Understandable, Secure, and Trustworthy). The strategic plan also outlines requirements for a 50% return on investment; to achieve this, Lori and her team developed a construct for quantifying ROI that they shared with multiple other teams, including the Digital Transformation Working Group. By creating ways of defining performance and value, Lori drives strategic investments and data-informed business outcomes. 

Her motivation for delivering quantifiable value stems from her years of experience in the aerospace industry. Growing up in the suburbs of Cleveland, Ohio not far from Glenn Research Center (GRC), Lori knew she wanted to become an aerospace engineer from a young age. She went on to receive an undergraduate degree in aerospace engineering and a master’s in mechanical engineering from Case Western Reserve University. Prior to joining NASA as a test engineer at GRC in 2007 and a civil servant in 2010, she worked for ten years designing aerospace products and technologies. Her background influences her commitment to freeing up time for the working level through digital transformation solutions. 

When asked what she enjoys most about working with Digital Transformation, Lori says, “For me, it’s all about sharing and collaborating so we can innovate for the benefit of all.” She recognizes that large-scale transformation requires many smaller parts contributing their diverse skillsets to the common goal. Of her various responsibilities and achievements, this is what excites and motivates her to continue impacting the agency as a digital transformer. “I just love collaborating with others that have this same mindset.”

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Maya L. Kikuchi

Astronaut José Hernández Boards Discovery

Astronaut José Hernández Boards Discovery

Astronaut José Hernández, a Hispanic man, smiles broadly at the camera while waiting to board space shuttle Discovery. He wears an orange escape suit that has an American flag patch on the left shoulder. Behind him are mission specialists Patrick Forrester (left) and Christer Fuglesang (back to camera).
NASA/Jim Grossmann

In this photo from Aug. 7, 2009, Jose Hernandez, mission specialist, smiles at the camera as he waits for his turn to enter the space shuttle Discovery as part of STS-128. It was the 128th Shuttle mission and the 30th mission to the International Space Station. While at the orbital lab, the STS-128 crew conducted three spacewalks.

Hernandez joined NASA’s Johnson Space Center in Houston in 2001. There, he was a materials research engineer in the Materials & Processes branch; eventually, he became branch chief. In 2004, he was selected as an astronaut candidate, and in 2009, he became a crew member of STS-128.

Get to know some of our Hispanic colleagues, past and present, during Hispanic Heritage Month.

Image credit: NASA/Jim Grossmann

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Monika Luabeya