Surfing NASA’s Internet of Animals: Satellites Study Ocean Wildlife

Surfing NASA’s Internet of Animals: Satellites Study Ocean Wildlife

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

An aerial view of Palmyra Atoll, where animal tracking data now being studied by NASA’s Internet of Animals project was collected using wildlife tags by partners at The Nature Conservancy, the U.S. Geological Survey, the National Oceanic and Atmospheric Administration, and several universities.
An aerial view of Palmyra Atoll, where animal tracking data now being studied by NASA’s Internet of Animals project was collected using wildlife tags by partners at The Nature Conservancy, the U.S. Geological Survey, the National Oceanic and Atmospheric Administration, and several universities.
The Nature Conservancy/Kydd Pollock

Anchoring the boat in a sandbar, research scientist Morgan Gilmour steps into the shallows and is immediately surrounded by sharks. The warm waters around the tropical island act as a reef shark nursery, and these baby biters are curious about the newcomer. They zoom close and veer away at the last minute, as Gilmour slowly makes her way toward the kaleidoscope of green sprouting from the island ahead.

Gilmour, a scientist at NASA’s Ames Research Center in California’s Silicon Valley, conducts marine ecology and conservation studies using data collected by the U.S. Geological Survey (USGS) from animals equipped with wildlife tags. Palmyra Atoll, a United States marine protected area, provides the perfect venue for this work.

A juvenile blacktip reef shark swims toward researchers in the shallow waters around Palmyra Atoll.
A juvenile blacktip reef shark swims toward researchers in the shallow waters around Palmyra Atoll.
The Nature Conservancy/Kydd Pollock

A collection of roughly 50 small islands in the tropical heart of the Pacific Ocean, the atoll is bursting with life of all kinds, from the reef sharks and manta rays circling the shoreline to the coconut crabs climbing palm branches and the thousands of seabirds swooping overhead. By analyzing the movements of dolphins, tuna, and other creatures, Gilmour and her collaborators can help assess whether the boundaries of the marine protected area surrounding the atoll actually protect the species they intend to, or if its limits need to shift.

Launched in 2020 by The Nature Conservancy and its partners – USGS, NOAA (National Oceanic and Atmospheric Administration), and several universities – the project team deployed wildlife tags at Palmyra in 2022, when Gilmour was a scientist with USGS.

Now with NASA, she is leveraging the data for a study under the agency’s Internet of Animals project. By combining information transmitted from wildlife tags with information about the planet collected by satellites – such as NASA’s Aqua, NOAA’s GOES (Geostationary Operational Environmental Satellite) satellites, and the U.S.-European Jason-3 – scientists can work with partners to draw conclusions that inform ecological management.

A satellite image shows a a collection of islands in various shades of green, stretching roughly in two parallel lines from left to right. On the top line, a thin layer of whitewater denotes where the reefs are. Bright teal surrounds the islands where the water is shallowest, fading quickly into the deep blue ocean water composing the majority of the image.
The Palmyra Atoll is a haven for biodiversity, boasting thriving coral reef systems, shallow waters that act as a shark nursery, and rich vegetation for various land animals and seabirds. In the Landsat image above, a small white square marks the research station, where scientists from all over the world come to study the many species that call the atoll home.
NASA/Earth Observatory Team

“Internet of Animals is more than just an individual collection of movements or individual studies; it’s a way to understand the Earth at large,” said Ryan Pavlick, then Internet of Animals project scientist at NASA’s Jet Propulsion Laboratory in Southern California, during the project’s kickoff event.

The Internet of Animals at Palmyra

“Our work at Palmyra was remarkably comprehensive,” said Gilmour. “We tracked the movements of eight species at once, plus their environmental conditions, and we integrated climate projections to understand how their habitat may change. Where studies may typically track two or three types of birds, we added fish and marine mammals, plus air and water column data, for a 3D picture of the marine protected area.”

Tagged Yellowfin Tuna, Grey Reef Sharks, and Great Frigatebirds move in and out of a marine protected area (blue square), which surrounds the Palmyra Atoll (blue circle) in the tropical heart of the Pacific. These species are three of many that rely on the atoll and its surrounding reefs for food and for nesting.
NASA/Lauren Dauphin

Now, the NASA team has put that data into a species distribution model, which combines the wildlife tracking information with environmental data from satellites, including sea surface temperature, chlorophyll concentration, and ocean current speed. The model can help researchers understand how animal populations use their habitats and how that might shift as the climate changes.

Preliminary results from Internet of Animals team show that the animals tracked are moving beyond the confines of the Palmyra marine protected area. The model identified suitable habitats both in and around the protected zone – now and under predicted climate change scenarios – other researchers and decisionmakers can utilize that knowledge to inform marine policy and conservation.

Research scientist Morgan Gilmour checks on a young great frigatebird in its nest. The marine protected area around Palmyra Atoll protects these birds' breeding grounds.
Research scientist Morgan Gilmour checks on a young great frigatebird in its nest. The marine protected area around Palmyra Atoll protects these birds’ breeding grounds.
UC Santa Barbara/Devyn Orr

Following a 2023 presidential memorandum, NOAA began studying and gathering input on whether to expand the protected areas around Palmyra and other parts of the Pacific Remote Islands Marine National Monument. Analysis from NASA’s Internet of Animals could inform that and similar decisions, such as whether to create protected “corridors” in the ocean to allow for seasonal migrations of wildlife. The findings and models from the team’s habitat analysis at Palmyra also could help inform conservation at similar latitudes across the planet.

Beyond the Sea: Other Internet of Animals Studies

Research at Palmyra Atoll is just one example of work by Internet of Animals scientists.

Claire Teitelbaum, a researcher with the Bay Area Environmental Research Institute based at NASA Ames, studies avian flu in wild waterfowl, investigating how their movement may contribute to transmission of the virus to poultry and other domestic livestock.

Teams at Ames and JPL are also working with USGS to create next-generation wildlife tags and sensors. Low-power radar tags in development at JPL would be lightweight enough to track small birds. Ames researchers plan to develop long-range radio tags capable of maximizing coverage and transmission of data from high-flying birds. This could help researchers take measurements in hard-to-reach layers of the atmosphere.

With the technology brought together by the Internet of Animals, even wildlife can take an active role in the study of Earth’s interacting systems, helping human experts learn more about our planet and how best to confront the challenges facing the natural world.

To learn more about the Internet of Animals visit: https://www.nasa.gov/nasa-earth-exchange-nex/new-missions-support/internet-of-animals/

The Internet of Animals project is funded by NASA and managed at NASA’s Jet Propulsion Laboratory in Southern California. The team at NASA’s Ames Research Center in California’s Silicon Valley is part of the NASA Earth Exchange, a Big Data initiative providing unique insights into Earth’s systems using the agency’s supercomputers at the center. Partners on the project include the U.S. Geological Survey, The Nature Conservancy, the National Oceanic and Atmospheric Administration, the Yale Center for Biodiversity and Global Change, Stanford University, University of Hawaii, University of California Santa Barbara, San Jose State University, University of Washington, and the Max Planck Institute for Animal Behavior.

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Media Contacts

Members of the news media interested in covering this topic should reach out to the NASA Ames newsroom.

About the Author

Milan Loiacono

Milan Loiacono

Science Communication Specialist

Milan Loiacono is a science communication specialist for the Earth Science Division at NASA Ames Research Center.

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Milan Loiacono

A Midsummer Red Sprite Seen from Space

A Midsummer Red Sprite Seen from Space

A line of bright blue lightning storms shines against a black background. Above the largest storm small wisps of red sprites stretch up. Along the left side, small yellow lights shine from an illuminated city.
Several transient luminous events illuminate pockets of Earth’s upper atmosphere. A line of thunderstorms off the coast of South Africa powers the rare phenomena.
NASA/Matthew Dominick

NASA astronaut Matthew Dominick photographed red sprites in Earth’s upper atmosphere from the International Space Station on June 3, 2024. The bright red flashes (more easily seen by clicking on the photo to see a larger version) are a less understood phenomena associated with powerful lightning events and appear high above the clouds in the mesosphere. Transient Luminous Events (TLEs), including red sprites, are colorful bursts of energy that appear above storms as a result of lightning activity occurring in and below storms on Earth.

Crew members typically capture TLEs with wide focal lengths during Earth timelapses. Instruments mounted outside station, like Atmosphere-Space Interactions Monitor (ASIM), can capture a range of data for researchers on Earth using cameras, photometers, X-ray and gamma-ray detectors. Learn more about seeing storms from space. 

While space station crew hunt for TLEs from space, you can help right here on Earth: send your photographs of sprites and other TLEs to NASA’s citizen science project, Spritacular, to contribute to a crowdsourced database that professional scientists can use for research.

Image Credit: NASA/Matthew Dominick

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Andrea Lloyd

NASA Deputy Administrator Strengthens Ties in Japan, Republic of Korea

NASA Deputy Administrator Strengthens Ties in Japan, Republic of Korea

NASA Deputy Administrator Pam Melroy gives keynote remarks during the 37th Space Symposium in Colorado Springs, Colorado.
NASA Deputy Administrator Pam Melroy gives keynote remarks during the 37th Space Symposium, April 5, 2022, in Colorado Springs, Colorado.
Credits: NASA/Bill Ingalls

NASA Deputy Administrator Pam Melroy will visit Japan and the Republic of Korea beginning Thursday, July 11, to underscore the critical role of international cooperation in advancing space exploration and technology development.

During her week-long visit to the region, Melroy will engage with ministers and other senior government officials in both countries, including leaders from JAXA (Japan Aerospace Exploration Agency) and KASA (Korea AeroSpace Administration) to strengthen partnerships and highlight civil space cooperation.

In Tokyo, Melroy will participate in the Secure World Foundation’s 6th Summit for Space Sustainability, highlighting NASA’s leadership in responsible and sustainable operations amid rapid technological advancements, many of them championed by the agency.

NASA and JAXA are working to advance sustainable human exploration of the Moon. NASA announced in April that Japan will design, develop, and operate a pressurized rover for exploration of the lunar surface. The activity is part of a shared goal for a Japanese national to be the first non-American to land on the Moon as part of a future Artemis mission, assuming important benchmarks are achieved. In addition, NASA and JAXA are advancing goals in climate research and space science missions to benefit humanity.

Melroy also will speak alongside other space agency leaders at the 45th Scientific Assembly of the Committee on Space Research in Busan, Korea, emphasizing opportunities for international and commercial collaboration in space research.

The visit to Korea coincides with the recent establishment of KASA and builds upon decades of collaboration with NASA in exploration, Earth and space science, and aeronautics.

For more information about NASA’s international partnerships, visit:

https://www.nasa.gov/oiir

-end-

Amber Jacobson
Headquarters, Washington
202-358-1600
amber.c.jacobson@nasa.gov

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Tiernan P. Doyle

Sols 4239-4240: ‘Vuggin’ Out’

Sols 4239-4240: ‘Vuggin’ Out’

2 min read

Sols 4239-4240: ‘Vuggin’ Out’

On a Martian surface covered in fine, powdery, brownish-orange soil, a large pockmarked rock – resembling a natural sponge – dominates half of the frame, extending from the upper-right corner to the center.
NASA’s Mars rover Curiosity acquired this image of a target named “Glacier Notch” on July 6, 2024, Sol 4236 of the Mars Science Laboratory Mission, at 16:55:06 UTC. Curiosity used its Mars Hand Lens Imager (MAHLI), located on the turret at the end of the rover’s robotic arm, capturing the image from 32 centimeters (about 13 inches) away.

Earth planning date: Monday, July 8, 2024

And just like we planned, Curiosity successfully drove about 11 meters (about 36 feet) after a 27-sol drill campaign at Mammoth Lakes! Not so fast, though, these rocks are just too interesting to leave behind so quickly. Instead of high-tailing it uphill like we usually do after a drill campaign, we’re staying put for another plan to get as much contact science on these diversely-toned rocks with mysterious origins and vugs (geologic term for the cavities in the rock) galore. It’s been a high priority to get as much color documentation of the clasts in the area, so a plan like this has kept my team busy commanding the Mastcams!

The first sol of this plan includes a long, 90-minute remote science block including about 50 minutes of ChemCam LIBS and RMI, about 32 minutes of Mastcam images, and a six-minute dust devil movie taken by Navcam. ChemCam is using its one-LIBS-per-sol on a conglomeratic block target named “Mount  Baxter,” and an RMI of Echo Ridge to the south. Mastcam is taking a 12-image mosaic of Mount Baxter after the LIBS work is done, and a huge 54-image mosaic to the east of Echo Ridge called “Stubblefield Canyon.” After the mast instruments are done, our rover will take about a four-hour long nap and wake up to unstow our arm. Arm activities this plan include two vug-tastic targets named “Lake Dorothy” and “Palisade Glacier,” both imaged by MAHLI and investigated by APXS. Curiosity is back to sleep by about 22:50, which sounds like my perfect sleep schedule.

The second sol of this plan includes a 60-minute remote science block containing about 45 minutes of ChemCam LIBS and RMI, only about six minutes of Mastcam images, and a whopping two hours of dust devil and environmental monitoring by Navcam. With 27 sols at our last location, we noticed significant wind motion between repeated images, and Navcam monitoring helps us keep track of how windy it is. Our rover will take another midday nap and wake up in the evening for a bonus APXS integration on Lake Dorothy, helping raise the signal-to-noise ratio and uncover more secrets (and questions) these Martian rocks have been keeping for millions of years.

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

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NASA’s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri

NASA’s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri

4 Min Read

NASA’s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri

A Hubble image of the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space.
This NASA Hubble Space Telescope image features the globular star cluster, Omega Centauri.
Credits:
ESA/Hubble, NASA, Maximilian Häberle (MPIA)

Most known black holes are either extremely massive, like the supermassive black holes that lie at the cores of large galaxies, or relatively lightweight, with a mass of under 100 times that of the Sun. Intermediate-mass black holes (IMBHs) are scarce, however, and are considered rare “missing links” in black hole evolution.

Now, an international team of astronomers has used more than 500 images from NASA’s Hubble Space Telescope — spanning two decades of observations — to search for evidence of an intermediate-mass black hole by following the motion of seven fast-moving stars in the innermost region of the globular star cluster Omega Centauri.

A Hubble image of the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space.
Omega Centauri is about 10 times as massive as other big globular clusters – almost as massive as a small galaxy – and consists of roughly 10 million stars that are gravitationally bound.
ESA/Hubble, NASA, Maximilian Häberle (MPIA)

These stars provide new compelling evidence for the presence of the gravitational pull from an intermediate-mass black hole tugging on them. Only a few other IMBH candidates have been found to date.

Omega Centauri consists of roughly 10 million stars that are gravitationally bound. The cluster is about 10 times as massive as other big globular clusters — almost as massive as a small galaxy.

Among the many questions scientists want to answer: Are there any IMBHs, and if so, how common are they? Does a supermassive black hole grow from an IMBH? How do IMBHs themselves form? Are dense star clusters their favored home?

The astronomers have now created an enormous catalog for the motions of these stars, measuring the velocities for 1.4 million stars gleaned from the Hubble images of the cluster. Most of these observations were intended to calibrate Hubble’s instruments rather than for scientific use, but they turned out to be an ideal database for the team’s research efforts.

The central region of the globular star cluster Omega Centauri. It appears as a collection of myriad stars colored red, white, and blue on the black background of space.
This image shows the central region of the Omega Centauri globular cluster, where NASA’s Hubble Space Telescope found strong evidence for an intermediate-mass black hole candidate.
ESA/Hubble, NASA, Maximilian Häberle (MPIA)

“We discovered seven stars that should not be there,” explained Maximilian Häberle of the Max Planck Institute for Astronomy in Germany, who led this investigation. “They are moving so fast that they would escape the cluster and never come back. The most likely explanation is that a very massive object is gravitationally pulling on these stars and keeping them close to the center. The only object that can be so massive is a black hole, with a mass at least 8,200 times that of our Sun.”

Several studies have suggested the presence of an IMBH in Omega Centauri. However, other studies proposed the mass could be contributed by a central cluster of stellar-mass black holes, and had suggested the lack of fast-moving stars above the necessary escape velocity made an IMBH less likely in comparison.

This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image, middle, zooms in on details of the central region of this cluster, with a closer view of the individual stars. The third image, at right, zooms in further to show the location of the intermediate-mass black hole candidate in the cluster. A dark region is circled and labeled
An international team of astronomers used more than 500 images from NASA’s Hubble Space Telescope – spanning two decades of observations – to detect seven fast-moving stars in the innermost region of Omega Centauri, the largest and brightest globular cluster in the sky. These stars provide compelling new evidence for the presence of an intermediate-mass black hole (IMBH) tugging on them. Only a few other IMBH candidates have been found to date. This image shows the location of the IMBH in Omega Centauri. If confirmed, at its distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, which is 26,000 light-years away. Besides the Galactic center, it would also be the only known case of a number of stars closely bound to a massive black hole. This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image shows the details of the central region of this cluster, with a closer view of the individual stars. The third image shows the location of the IMBH candidate in the cluster.
ESA/Hubble, NASA, Maximilian Häberle (MPIA)

“This discovery is the most direct evidence so far of an IMBH in Omega Centauri,” added team lead Nadine Neumayer of the Max Planck Institute for Astronomy in Germany, who initiated the study, together with Anil Seth from the University of Utah, Salt Lake City. “This is exciting because there are only very few other black holes known with a similar mass. The black hole in Omega Centauri may be the best example of an IMBH in our cosmic neighborhood.”

If confirmed, at a distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, located 26,000 light-years away.

Omega Centauri is visible from Earth with the naked eye and is one of the favorite celestial objects for stargazers living in the southern hemisphere. Located just above the plane of the Milky Way, the cluster appears almost as large as the full Moon when seen from a dark rural area. It was first listed in Ptolemy’s catalog nearly 2,000 years ago as a single star. Edmond Halley reported it as a nebula in 1677. In the 1830s the English astronomer John Herschel was the first to recognize it as a globular cluster.

The discovery paper led by Häberle et al. is published online today in the journal Nature.

Scientists think a massive object is gravitationally pulling on the stars within Omega Centauri, keeping them close to its center. Credit: NASA’s Goddard Space Flight Center, Lead Producer: Paul Morris

The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, Colorado, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, Maryland, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.

Media Contacts:

Claire Andreoli
NASA’s Goddard Space Flight CenterGreenbelt, MD
claire.andreoli@nasa.gov

Ray Villard
Space Telescope Science Institute, Baltimore, MD

Bethany Downer
ESA/Hubble.org

Science Contact:
Maximilian Häberle
Max Planck Institute for Astronomy, Heidelberg, Germany

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