NASA Data Helps Map Tiny Plankton That Feed Giant Right Whales

NASA Data Helps Map Tiny Plankton That Feed Giant Right Whales

6 min read

NASA Data Helps Map Tiny Plankton That Feed Giant Right Whales

A North Atlantic right whale, partially submerged, swims in dark blue ocean water, creating white foam around its head and back.
This North Atlantic right whale, named “Bowtie,” was spotted feeding in southern Maine waters in January 2025. A new technique aims to use NASA satellite data to see the plankton these whales depend on from space.
Credit: New England Aquarium, taken under NMFS permit # 25739

In the waters off New England, one of Earth’s rarest mammals swims slowly, mouth agape. The North Atlantic right whale filters clouds of tiny reddish zooplankton — called Calanus finmarchicus — from the sea. These zooplankton, no bigger than grains of rice, are the whale’s lifeline. Only about 370 of these massive creatures remain.

For decades, tracking the tiny plankton meant sending research vessels out in the ocean, towing nets and counting samples by hand. Now, scientists are looking from above instead.

Using NASA satellite data, researchers found a way to detect Calanus swarms at the ocean surface in the Gulf of Maine, picking up on the animals’ natural red pigment. This early-stage approach, described in a new study, may help researchers better estimate where the copepods gather, and where whales might follow.

Tracking the zooplankton from space could aid both the whales and maritime industries. By predicting where these mammals are likely to feed, researchers and marine resource managers hope to reduce deadly vessel strikes and fishing gear entanglements — two major threats to the species. Knowing the feeding patterns could also help shipping and fishing industries operate more efficiently.

A magnified view of a nearly translucent Calanus finmarchicus zooplankton, showing its segmented body, antennae, and internal structures.
Calanus finmarchicus, a tiny zooplankton powering North Atlantic food webs, fuels right whale populations with its energy-rich lipid reserves.
Credit: Cameron Thompson

“NASA invests in this kind of research because it connects space-based observation with real-world challenges,” said Cynthia Hall, a support scientist at NASA headquarters in Washington. She works with the Early Career Research Program, which partly funded the work. “It’s yet another a way to put NASA satellite data to work for science, communities, and ecosystems.”

Revealing the Ocean’s Hidden Patterns

The new approach uses data from the Moderate Resolution Imaging Spectroradiometer (MODIS) aboard NASA’s Aqua satellite. The MODIS instrument doesn’t directly see the copepods themselves. Instead, it reads how the spectrum of sunlight reflected from the ocean surface changes in response to what’s in the water.

When large numbers of the zooplankton rise to the surface, their reddish pigment — astaxanthin, the same compound that gives salmon its pink color — subtly alters how photons, or particles of light, from the sun are absorbed or scattered in the water. The fate of these photons in the ocean depends on the mix of living and non-living matter in seawater, creating a slight shift in color that MODIS can detect.

“We didn’t know to look for Calanus before in this way,” said Catherine Mitchell, a satellite oceanographer at Bigelow Laboratory for Ocean Sciences in East Boothbay, Maine. “Remote sensing has typically focused on smaller things like phytoplankton. But recent research suggested that larger, millimeter-sized organisms like zooplankton can also influence ocean color.”

A few years ago, researchers piloted a satellite method for detecting copepods in Norwegian waters. Now, some of those same scientists — along with Mitchell’s team — have refined the approach and applied it to the Gulf of Maine, a crucial feeding ground for right whales during their northern migration. By combining satellite data, a model, and field measurements, they produced enhanced images that revealed Calanus swarms at the sea surface, and were able to estimate numbers of the tiny animals.

“We know the right whales are using habitats we don’t fully understand,” said Rebekah Shunmugapandi, also a satellite oceanographer at Bigelow and the study’s lead author. “This satellite-based Calanus information could eventually help identify unknown feeding grounds or better anticipate where whales might travel.”

Tracking Elusive Giants

Despite decades of study, North Atlantic right whales remain remarkably enigmatic to scientists. Once fairly predictable in their movements along the Eastern Seaboard of North America, these massive mammals began abandoning some traditional feeding grounds in 2010-2011. Their sudden shift to unexpected areas like the Gulf of Saint Lawrence caught people off guard, with deadly consequences.

“We’ve had whales getting hit by ships and whales getting stuck in fishing gear,” said Laura Ganley, a research scientist in the Anderson Cabot Center for Ocean Life at the New England Aquarium in Boston, which conducts aerial and boat surveys of the whales.  

In 2017, the National Oceanic and Atmospheric Administration designated the situation as an “unusual mortality event” in an effort to address the whales’ decline. Since then, 80 North Atlantic right whales have been killed or sustained serious injuries, according to NOAA.

Map showing estimated concentrations of the copepod Calanus finmarchicus in the Gulf of Maine, with the highest densities (up to 150,000 individuals per cubic meter) marked in dark red. Areas with no data are shaded in a blue crosshatch pattern.
NASA satellite imagery from June 2009 was used to test a new method for detecting the copepod Calanus finmarchicus in the Gulf of Maine and estimating their numbers from space.
Credit: NASA Earth Observatory image by Wanmei Liang, using data from Shunmugapandi, R., et al. (2025)

In the Gulf of Maine, there’s less shipping activity, but there can be a complex patchwork of lobster fishing gear, said Sarah Leiter, a scientist with the Maine Department of Marine Resources. “Each fisherman has 800 traps or so,” Leiter explained. “If a larger number of whales shows up suddenly, like they just did in January 2025, it is challenging. Fishermen need time and good weather to adjust that gear.”

What excites Leiter the most about the satellite data is the potential to use it in a forecasting tool to help predict where the whales could go. “That would be incredibly useful in giving us that crucial lead time,” she said.

PACE: The Next Generation of Ocean Observer

For now, the Calanus-tracking method has limitations. Because MODIS detects the copepods’ red pigment, not the animals themselves, that means other small, reddish organisms can be mistaken for the zooplankton. And cloud cover, rough seas, or deeper swarms all limit what satellites can spot.

MODIS is also nearing the end of its operational life. But NASA’s next-generation PACE (Plankton, Aerosol, Cloud, ocean Ecosystem) satellite — launched in 2024 — is poised to make dramatic improvements in the detection of zooplankton and phytoplankton.

Swirling green phytoplankton blooms in the Gulf of Maine are seen in a satellite image taken by NASA’s PACE mission.
NASA’s Ocean Color Instrument on the PACE satellite captured these swirling green phytoplankton blooms in the Gulf of Maine in April 2024. Such blooms fuel zooplankton like Calanus finmarchicus.
Credit: NASA

“The PACE satellite will definitely be able to do this, and maybe even something better,” said Bridget Seegers, an oceanographer and mission scientist with the PACE team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

The PACE mission includes the Ocean Color Instrument, which detects more than 280 wavelengths of light. That’s a big jump from the 10 wavelengths seen by MODIS. More wavelengths mean finer detail and better insights into ocean color and the type of plankton that the satellite can spot.

Local knowledge of seasonal plankton patterns will still be essential to interpret the data correctly. But the goal isn’t perfect detection, the scientists say, but rather to provide another tool to inform decision-making, especially when time or resources are limited.

By Emily DeMarco
NASA Headquarters

Powered by WPeMatico

Get The Details…

NASA Langley Participates in Air Power Over Hampton Roads

NASA Langley Participates in Air Power Over Hampton Roads

NASA Langley highlights its Cirrus Design SR22 during Air Power Over Hampton Roads STEM Day.
NASA Langley highlights its Cirrus Design SR22 during Air Power Over Hampton Roads STEM Day.
NASA/Angelique Herring

NASA Langley Research Center’s integral role in the past, present, and future of flight was on full display April 25-27 during the Air Power Over Hampton Roads air show.

The air show, held at Joint Base Langley-Eustis (JBLE), which neighbors NASA Langley in Hampton, Virginia, attracted thousands of spectators throughout the weekend.

The weekend kicked off with a STEM Day on April 25. Langley’s Office of STEM Engagement (OSTEM) offered educational and engaging activities, exhibits, and displays to share NASA missions and encourage K-12 students from local schools to explore the possibilities that science, technology, engineering, and math offer.

“Participation in the air show allows us to share NASA’s work in aeronautics with the public and provides an opportunity for Langley researchers and engineers to work directly with students and families to share the exciting work they do,” said Bonnie Murray, Langley OSTEM Student Services manager.

NASA Langley personnel inspire young minds during Air Power Over Hampton Roads STEM Day.
NASA Langley personnel inspire young minds during Air Power Over Hampton Roads STEM Day.
NASA/Angelique Herring

Langley OSTEM’s participation continued throughout the weekend as a part of the air show’s STEM Expo, where visitors to the NASA booths tested a paper helicopter in a small-scale wind tunnel to explore flight dynamics, learned how NASA uses X-planes for research and designed their own X-plane, and tested experimental paper airplanes of various designs. By observing flight of the plane designs and making improvements to each one, students participated in the engineering design process. NASA subject matter experts in attendance guided students through these activities, inspired young minds by sharing some of their innovations, and promoted a variety of STEM career paths.

“Through engagement in the NASA STEM Zone activities, students had an opportunity to see themselves in the role of a NASA researcher,” Murray said. “Authentic learning experiences such as these help build children’s STEM identity, increasing the likelihood of them pursuing STEM careers in the future.”

A child enjoys NASA STEM activities during Air Power Over Hampton Roads STEM Day.
A child enjoys NASA STEM activities during Air Power Over Hampton Roads STEM Day.
NASA/Angelique Herring

The air show’s static aircraft displays included NASA Langley’s Cirrus Design SR22, a research aircraft used to support NASA’s airborne science program, the science community, and aeronautics research.

“Reflective of our strong, long-standing partnership with JBLE, NASA Langley was proud to participate in this year’s Air Power Over Hampton Roads air show,” said Glenn Jamison, director of Langley’s Research Services Directorate. “Our relationship spans back to 1917 when NACA and Langley Field evolved together over formative years in aerodynamic research, sharing the airspace and facilities here in Hampton. Today, we continue our collaboration with JBLE in pursuing shared interests and finding innovative solutions to complex problems.”

The displays also featured several small Unmanned Aircraft Systems (sUAS) and NASA’s P-3 Orion, a research aircraft based at NASA’s Wallops Flight Facility on Wallops Island, Virginia.

Air show visitors could explore a picture display that highlighted NASA Langley’s rich aviation legacy, from its founding in 1917 to Langley’s work today to accelerate advancements in aeronautics, science, and space technology and exploration. Spacey Casey, a crowd favorite, greeted and took pictures with educators, students, and guests throughout the weekend, bringing out-of-this-world smiles to their faces. Members of Langley’s Office of the Director also represented the center at the event.

Brittny McGraw
NASA Langley Research Center

Powered by WPeMatico

Get The Details…
Joseph Scott Atkinson

NASA’s Webb Lifts Veil on Common but Mysterious Type of Exoplanet

NASA’s Webb Lifts Veil on Common but Mysterious Type of Exoplanet

6 Min Read

NASA’s Webb Lifts Veil on Common but Mysterious Type of Exoplanet

Illustration showing a large fuzzy blue planet in the foreground, and an orange-yellow star in the background. The side of the planet facing the star is lit, and the side facing away is dark. The boundary between the lit and dark sides is fuzzy. The atmosphere is almost homogeneous in color and texture, with extremely subtle variations and no sign of a surface. The star is slightly more orange than the Sun. The black background of space is scattered with white points of light.
This artist’s concept shows what the hot sub-Neptune exoplanet TOI-421 b could look like. It is based on spectroscopic data gathered by Webb, as well as previous observations from other telescopes on the ground and in space.
Credits:
Illustration: NASA, ESA, CSA, Dani Player (STScI)

Though they don’t orbit around our Sun, sub-Neptunes are the most common type of exoplanet, or planet outside our solar system, that have been observed in our galaxy. These small, gassy planets are shrouded in mystery…and often, a lot of haze. Now, by observing exoplanet TOI-421 b, NASA’s James Webb Space Telescope is helping scientists understand sub-Neptunes in a way that was not possible prior to the telescope’s launch.

“I had been waiting my entire career for Webb so that we could meaningfully characterize the atmospheres of these smaller planets,” said principal investigator Eliza Kempton of the University of Maryland, College Park. “By studying their atmospheres, we’re getting a better understanding of how sub-Neptunes formed and evolved, and part of that is understanding why they don’t exist in our solar system.”

Image A: Artist’s Concept of TOI-421 b

Illustration showing a large fuzzy blue planet in the foreground, and an orange-yellow star in the background. The side of the planet facing the star is lit, and the side facing away is dark. The boundary between the lit and dark sides is fuzzy. The atmosphere is almost homogeneous in color and texture, with extremely subtle variations and no sign of a surface. The star is slightly more orange than the Sun. The black background of space is scattered with white points of light.
This artist’s concept shows what the hot sub-Neptune exoplanet TOI-421 b could look like. It is based on spectroscopic data gathered by Webb, as well as previous observations from other telescopes on the ground and in space.
Illustration: NASA, ESA, CSA, Dani Player (STScI)

Small, Cool, Shrouded in Haze

The existence of sub-Neptunes was unexpected before they were discovered by NASA’s retired Kepler space telescope in the last decade. Now, astronomers are trying to understand where these planets came from and why are they so common.

Before Webb, scientists had very little information on them. While sub-Neptunes are a few times larger than Earth, they are still much smaller than gas-giant planets and typically cooler than hot Jupiters, making them much more challenging to observe than their gas-giant counterparts.

A key finding prior to Webb was that most sub-Neptune atmospheres had flat or featureless transmission spectra. This means that when scientists observed the spectrum of the planet as it passed in front of its host star, instead of seeing spectral features – the chemical fingerprints that would reveal the composition of the atmosphere – they saw only a flat-line spectrum. Astronomers concluded from all of those flat-line spectra that at least certain sub-Neptunes were probably very highly obscured by either clouds or hazes.

Image B: Spectrum of TOI-421 b

Graphic titled “Exoplanet TOI-421 b Hot Sub-Neptune, NIRISS Single Object Slitless Spectroscopy, NIRSpec Bright Object Time-Series Spectroscopy” shows a graph of amount of light blocked on the y-axis versus wavelength of light on the x-axis.
A transmission spectrum captured by NASA’s James Webb Space Telescope reveals chemicals in the atmosphere of the hot sub-Neptune exoplanet TOI-421 b.
Illustration: NASA, ESA, CSA, Joseph Olmsted (STScI)

A Different Kind of Sub-Neptune?

“Why did we observe this planet, TOI-421 b? It’s because we thought that maybe it wouldn’t have hazes,” said Kempton. “And the reason is that there were some previous data that implied that maybe planets over a certain temperature range were less enshrouded by haze or clouds than others.”

That temperature threshold is about 1,070 degrees Fahrenheit. Below that, scientists hypothesized that a complex set of photochemical reactions would occur between sunlight and methane gas, and that would trigger the haze. But hotter planets shouldn’t have methane and therefore perhaps shouldn’t have haze.

The temperature of TOI-421 b is about 1,340 degrees Fahrenheit, well above the presumed threshold. Without haze or clouds, researchers expected to see a clear atmosphere – and they did!

A Surprising Finding

“We saw spectral features that we attribute to various gases, and that allowed us to determine the composition of the atmosphere,” said the University of Maryland’s Brian Davenport, a third-year Ph.D. student who conducted the primary data analysis. “Whereas with many of the other sub-Neptunes that had been previously observed, we know their atmospheres are made of something, but they’re being blocked by haze.”

The team found water vapor in the planet’s atmosphere, as well as tentative signatures of carbon monoxide and sulfur dioxide. Then there are molecules they didn’t detect, such as methane and carbon dioxide. From the data, they can also infer that a large amount of hydrogen is in TOI-421 b’s atmosphere.

The lightweight hydrogen atmosphere was the big surprise to the researchers. “We had recently wrapped our mind around the idea that those first few sub-Neptunes observed by Webb had heavy-molecule atmospheres, so that had become our expectation, and then we found the opposite,” said Kempton. This suggests TOI-421 b may have formed and evolved differently from the cooler sub-Neptunes observed previously.

Is TOI-421 b Unique?

The hydrogen-dominated atmosphere is also interesting because it mimics the composition of TOI-421 b’s host star. “If you just took the same gas that made the host star, plopped it on top of a planet’s atmosphere, and put it at the much cooler temperature of this planet, you would get the same combination of gases. That process is more in line with the giant planets in our solar system, and it is different from other sub-Neptunes that have been observed with Webb so far,” said Kempton.

Aside from being hotter than other sub-Neptunes previously observed with Webb, TOI-421 b orbits a Sun-like star. Most of the other sub-Neptunes that have been observed so far orbit smaller, cooler stars called red dwarfs.

Is TOI-421b emblematic of hot sub-Neptunes orbiting Sun-like stars, or is it just that exoplanets are very diverse? To find out, the researchers would like to observe more hot sub-Neptunes to determine if this is a unique case or a broader trend. They hope to gain insights into the formation and evolution of these common exoplanets.

“We’ve unlocked a new way to look at these sub-Neptunes,” said Davenport. “These high-temperature planets are amenable to characterization. So by looking at sub-Neptunes of this temperature, we’re perhaps more likely to accelerate our ability to learn about these planets.”

The team’s findings appear on May 5 in the Astrophysical Journal Letters.

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

Click any image to open a larger version.

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
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Ann Jenkinsjenkins@stsci.edu
Space Telescope Science Institute, Baltimore, Md.

Hannah Braunhbraun@stsci.edu
Space Telescope Science Institute, Baltimore, Md.

Related Information

Webb Blog: Reconnaissance of Potentially Habitable Worlds with NASA’s Webb

Video: How to Study Exoplanets

Article: Webb’s Impact on Exoplanet Research

Video: How do we learn about a planet’s Atmosphere?

Learn more about exoplanets

More Webb News

More Webb Images

Webb Science Themes

Webb Mission Page

Related For Kids

What is the Webb Telescope?

SpacePlace for Kids

En Español

Ciencia de la NASA

NASA en español 

Space Place para niños

Share

Details

Last Updated
May 04, 2025
Editor
Marty McCoy
Contact

Powered by WPeMatico

Get The Details…

GSFC Office of the Chief Knowledge Officer – Case Studies

GSFC Office of the Chief Knowledge Officer – Case Studies

The Goddard OCKO has a large collection of case studies covering a wide range of missions and technical topics, including launch decision making, project management, procurement, instrument development, risk management, systems engineering and more. These case studies can be used to facilitate learning of critical knowledge and lessons that enable mission success.

Click Here to Access the Case Studies (Internal NASA Only).

Powered by WPeMatico

Get The Details…
Alysha Bayens

Sols 4527-4528: ‘Boxwork Ahoy!’

Sols 4527-4528: ‘Boxwork Ahoy!’

2 min read

Sols 4527-4528: ‘Boxwork Ahoy!’

A grayscale photograph of the Martian surface from the Curiosity rover shows a field of rough and jagged rocks covering the surface from the foreground extending to hills in the background, all medium to dark gray. The hills appear smoother overall, but have horizontal folds on their sides leading up to their peaks.
NASA’s Mars rover Curiosity acquired this image looking directly west and showing a first ground view of the boxwork structures the rover is driving toward. The boxwork structures are visible in the distance as smoother terrain criss-crossed by ridges, just below the hilltops. Curiosity acquired this image using its Left Navigation Camera on April 30, 2025 – Sol 4526, or Martian day 4,526 of the Mars Science Laboratory mission – at 14:10:41 UTC.
NASA/JPL-Caltech

Written by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems

Earth planning date: Wednesday, April 30, 2025

We’re back in our standard “touch and go” plan regime today, where we sandwich a midday remote science block between morning-APXS and afternoon-MAHLI contact science arm blocks. We had our first late-slide 9 a.m. PDT start in quite a while due to our “isolated nominal” plan on Monday! This meant the whole team was ready and “patiently” (read: not-so-patiently) waiting for our drive data to come down around 8:40 this morning. Thankfully, everything we were waiting for came down to Earth and told us Curiosity was right where we wanted her to be! The planning begins…

Sol 4527 contains most of our activities in this plan. We start off about 10:00 local Gale time with a DRT and APXS analysis of contact science target “Tamarack Valley,” a rough but brushable bedrock target in our workspace. We leave the arm unstowed (and out of the way) for our remote science block spanning the hours of about 12:35-13:45. That block starts with a large, 76-frame stereo Mastcam mosaic covering the boxwork structures to the west while ChemCam’s instrument cools down to allow for LIBS.

After Mastcam is done, ChemCam shoots their LIBS on a rougher bedrock target named “Aguanga,” and an RMI mosaic of the boxwork structures included in the Mastcam mosaic. About 14:00 local time, MAHLI finishes the contact science with a full suite of Tamarack Valley (25-centimeter, 5-centimeter stereo, and 1-centimeter images). Then we drive! Hopefully about 30 meters closer (about 98 feet) to the boxwork structures for our weekend plan. 

Curiosity takes the second sol easier with some Navcam dust-devil and horizon movies, along with a rover-decided LIBS target at our new location to start off science decisions for Friday.

Share

Details

Last Updated
May 04, 2025

Related Terms

Powered by WPeMatico

Get The Details…