Newly Minted Ph.D. Studies Phytoplankton with NASA’s FjordPhyto Project

Newly Minted Ph.D. Studies Phytoplankton with NASA’s FjordPhyto Project

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Newly Minted Ph.D. Studies Phytoplankton with NASA’s FjordPhyto Project

A group of eight people wearing red and black cold-weather gear with neon yellow hoods are seated in a black inflatable boat in a polar environment. They are smiling and holding scientific equipment, including a plankton net, a mug, and an orange device. Snow-covered mountains and an icy ocean surround them under an overcast sky.
Adventurous travellers aboard the Viking Octantis ship, sampling phytoplankton from  Danco Island in the Errera Channel for the FjordPhyto project.
Allison Cusick

FjordPhyto is a collective effort where travelers on tour expedition vessels in Antarctica help scientists at Scripps Institution of Oceanography and Universidad Nacional de La Plata study phytoplankton. Now project leader Dr. Allison Cusick has a Ph.D.! . Dr. Cusick studies how melting glaciers influence phytoplankton in the coastal regions. She wrote her doctoral dissertation based on the data collected by FjordPhyto volunteers.

“Travelers adventure to the wild maritime climate of Antarctica and help collect samples from one of the most data-limited regions of the world,” said Cusick.  “While on vacation, they can volunteer to join a FjordPhyto science boat experience where they spend an hour collecting water measurements like salinity, temperature, chlorophyll-a, turbidity, as well as physical samples for molecular genetics work, microscopy identification, and carbon biomass estimates. It’s a full immersion into the ecosystem and the importance of polar research!”

Cusick successfully defended her thesis on December 18, 2024, earning a Ph.D. in Oceanography from the Scripps Institution of Oceanography. Hers is the second Ph.D.  based on data from the FjordPhyto project. Martina Mascioni from FjordPhyto team earned her Ph.D. from the National University of La Plata (Argentina) in 2018.

The project is a hit with travelers, too.

“It’s incredibly inspiring to be part of a program like this that’s open to non-specialist involvement,” said one volunteer, a retired biology teacher aboard the Viking Octantis ship, who continued to say, “Thank you for letting us be a part of the science and explaining so clearly why it matters to the bigger picture.”

If you would like to get involved, go to www.fjordphyto.org and reach out to the team!

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Last Updated
Feb 10, 2025

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Euclid Discovers Einstein Ring in Our Cosmic Backyard

Euclid Discovers Einstein Ring in Our Cosmic Backyard

A sea of colorful stars and galaxies appear to swim in the vast blackness of space around a hazy halo at centre stage. In the middle of the image, the fuzzy-looking bulb of light in a warm shade of yellow extends around a small bright spot, nestled within a thin light circle that appears to be drawn closely around it. As we follow the central halo’s rim outwards, its brightness dims and blends smoothly into its surroundings. Here, extended discs of shades ranging from a warm purple to golden yellow, and piercing dots of light with sharp diffraction spikes are spread evenly across the image.
The ring of light surrounding the center of the galaxy NGC 6505, captured by ESA’s Euclid telescope, is an example of an Einstein ring. NGC 6505 is acting as a gravitational lens, bending light from a galaxy far behind it.
ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre, G. Anselmi, T. Li; CC BY-SA 3.0 IGO or ESA Standard Licence

Euclid, an ESA (European Space Agency) mission with NASA contributions, has made a surprising discovery in our cosmic backyard: a phenomenon called an Einstein ring.

An Einstein ring is light from a distant galaxy bending to form a ring that appears aligned with a foreground object. The name honors Albert Einstein, whose general theory of relativity predicts that light will bend and brighten around objects in space.

In this way, particularly massive objects like galaxies and galaxy clusters serve as cosmic magnifying glasses, bringing even more distant objects into view. Scientists call this gravitational lensing.

Euclid Archive Scientist Bruno Altieri noticed a hint of an Einstein ring among images from the spacecraft’s early testing phase in September 2023.

“Even from that first observation, I could see it, but after Euclid made more observations of the area, we could see a perfect Einstein ring,” Altieri said. “For me, with a lifelong interest in gravitational lensing, that was amazing.”

The ring appears to encircle the center of a well-studied elliptical galaxy called NGC 6505, which is around 590 million light-years from Earth in the constellation Draco. That may sound far, but on the scale of the entire universe, NGC 6505 is close by. Thanks to Euclid’s high-resolution instruments, this is the first time that the ring of light surrounding the galaxy has been detected.  

Light from a much more distant bright galaxy, some 4.42 billion light-years away, creates the ring in the image. Gravity distorted this light as it traveled toward us. This faraway galaxy hasn’t been observed before and doesn’t yet have a name. 

“An Einstein ring is an example of strong gravitational lensing,” explained Conor O’Riordan, of the Max Planck Institute for Astrophysics, Germany, and lead author of the first scientific paper analyzing the ring. “All strong lenses are special, because they’re so rare, and they’re incredibly useful scientifically. This one is particularly special, because it’s so close to Earth and the alignment makes it very beautiful.” 

Einstein rings are a rich laboratory for scientists to explore many mysteries of the universe. For example, an invisible form of matter called dark matter contributes to the bending of light into a ring, so this is an indirect way to study dark matter. Einstein rings are also relevant to the expansion of the universe because the space between us and these galaxies — both in the foreground and the background — is stretching. Scientists can also learn about the background galaxy itself.

“I find it very intriguing that this ring was observed within a well-known galaxy, which was first discovered in 1884,” said Valeria Pettorino, ESA Euclid project scientist. “The galaxy has been known to astronomers for a very long time. And yet this ring was never observed before. This demonstrates how powerful Euclid is, finding new things even in places we thought we knew well. This discovery is very encouraging for the future of the Euclid mission and demonstrates its fantastic capabilities.” 

A close-up view of the center of the NGC 6505 galaxy, with the bright Einstein ring aligned with it, captured by ESA’s Euclid space telescope.
ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre, G. Anselmi, T. Li; CC BY-SA 3.0 IGO or ESA Standard Licence

By exploring how the universe has expanded and formed over its cosmic history, Euclid will reveal more about the role of gravity and the nature of dark energy and dark matter. Dark energy is the mysterious force that appears to be causing the universe’s expansion. The space telescope will map more than a third of the sky, observing billions of galaxies out to 10 billion light-years. It is expected to find around 100,000 strong gravitational lenses.  

“Euclid is going to revolutionize the field with all this data we’ve never had before,” added O’Riordan.  

Although finding this Einstein ring is an achievement, Euclid must look for a different, less visually obvious type of gravitational lensing called “weak lensing” to help fulfil its quest of understanding dark energy. In weak lensing, background galaxies appear only mildly stretched or displaced. To detect this effect, scientists will need to analyze billions of galaxies.

Euclid launched from Cape Canaveral, Florida, July 1, 2023, and began its detailed survey of the sky Feb. 14, 2024. The mission is gradually creating the most extensive 3D map of the universe yet. The Einstein ring find so early in its mission indicates Euclid is on course to uncover many more secrets of the universe. 

More About Euclid

Euclid is a European mission, built and operated by ESA, with contributions from NASA. The Euclid Consortium — consisting of more than 2,000 scientists from 300 institutes in 15 European countries, the United States, Canada, and Japan — is responsible for providing the scientific instruments and scientific data analysis. ESA selected Thales Alenia Space as prime contractor for the construction of the satellite and its service module, with Airbus Defence and Space chosen to develop the payload module, including the telescope. Euclid is a medium-class mission in ESA’s Cosmic Vision Programme.

Three NASA-supported science teams contribute to the Euclid mission. In addition to designing and fabricating the sensor-chip electronics for Euclid’s Near Infrared Spectrometer and Photometer (NISP) instrument, NASA’s Jet Propulsion Laboratory led the procurement and delivery of the NISP detectors as well. Those detectors, along with the sensor chip electronics, were tested at NASA’s Detector Characterization Lab at Goddard Space Flight Center in Greenbelt, Maryland. The Euclid NASA Science Center at IPAC (ENSCI), at Caltech in Pasadena, California, will archive the science data and support U.S.-based science investigations. JPL is a division of Caltech.

Media Contacts

Elizabeth Landau
Headquarters, Washington
202-358-0845
elandau@nasa.gov

Calla Cofield
Jet Propulsion Laboratory, Pasadena, Calif.
626-808-2469
calla.e.cofield@jpl.nasa.gov

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Elizabeth R. Landau

Relaxation, Housekeeping Wrap Up Work Week Aboard the Station

Relaxation, Housekeeping Wrap Up Work Week Aboard the Station

Astronaut Suni Williams rides the Canadarm2 robotic arm while being maneuvered to her worksite 264 miles above the Earth during a spacewalk on Jan. 30, 2025.
Astronaut Suni Williams rides the Canadarm2 robotic arm while being maneuvered to her worksite 264 miles above the Earth during a spacewalk on Jan. 30, 2025.

The Expedition 72 crew wrapped up the work week with housekeeping duties and relaxation following several days of spacewalk cleanup activities and advanced research aboard the International Space Station.

Station Commander Suni Williams and Flight Engineer Butch Wilmore, both NASA astronauts, were off duty on Friday after stowing spacewalk tools and deconfiguring spacesuits earlier in the week. The duo used the tools and wore the suits during a five hour and 26-minute spacewalk on Jan. 30 for science and maintenance. Williams and Wilmore also worked throughout the week on robotics research, computer updates, and life support maintenance.

NASA Flight Engineers Nick Hague and Don Pettit took turns at the end of the week measuring the airflow in their crew quarters ensuring a safe breathing environment inside the orbital lab. Hague first checked his overhead crew quarters then Pettit checked his starboard crew quarters, both in the Harmony module, measuring the airflows at different locations and at different speeds. Hague earlier collected biological samples for processing while Pettit conducted a photographic inspection of stowage areas inside the Columbus laboratory module.

Roscosmos Flight Engineer Aleksandr Gorbunov spent his day on variety of science activities. He first prepared drives to capture research data collected from a plasma crystal study, swapped a lens on a student-controlled Earth observation camera, then checked video recording gear. Flight Engineers Alexey Ovchinin and Ivan Vagner spent their day on life support maintenance tasks throughout the orbital outpost’s Roscosmos segment.


Learn more about station activities by following the space station blog@space_station and @ISS_Research on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark Garcia

February’s Night Sky Notes: How Can You Help Curb Light Pollution?

February’s Night Sky Notes: How Can You Help Curb Light Pollution?

5 min read

February’s Night Sky Notes: How Can You Help Curb Light Pollution?

Light pollution has long troubled astronomers, who generally shy away from deep sky observing under full Moon skies. The natural light from a bright Moon floods the sky and hides views of the Milky Way, dim galaxies and nebula, and shooting stars. In recent years, human-made light pollution has dramatically surpassed the interference of even a bright full Moon, and its effects are now noticeable to a great many people outside of the astronomical community. Harsh, bright white LED streetlights, while often more efficient and long-lasting, often create unexpected problems for communities replacing their old street lamps. Some notable concerns are increased glare and light trespass, less restful sleep, and disturbed nocturnal wildlife patterns. There is increasing awareness of just how much light is too much light at night. You don’t need to give in to despair over encroaching light pollution; you can join efforts to measure it, educate others, and even help stop or reduce the effects of light pollution in your community. 

This image compares an urban street at night under two lighting types: warm, yellow sodium-vapor lights (left) and cool, white LED or metal-halide lights (right). The left appears hazy with muted colors, while the right is clearer, highlighting details and enhancing visibility.
Before and after pictures of replacement lighting at the 6th Street Bridge over the Los Angeles River. The second picture shows improvements in some aspects of light pollution, as light is not directed to the sides and upwards from the upgraded fixtures, reducing skyglow. However, it also shows the use of brighter, whiter LEDs, which is not generally ideal, along with increased light bounce back from the road. 
City of Los Angeles

Amateur astronomers and potential citizen scientists around the globe are invited to participate in the Globe at Night (GaN) program to measure light pollution. Measurements are taken by volunteers on a few scheduled days every month and submitted to their database to help create a comprehensive map of light pollution and its change over time. GaN volunteers can take and submit measurements using multiple methods ranging from low-tech naked-eye observations to high-tech sensors and smartphone apps.

Globe at Night citizen scientists can use the following methods to measure light pollution and submit their results:

  • Their own smartphone camera and dedicated app
  • Manually measure light pollution using their own eyes and detailed charts of the constellations
  • A dedicated light pollution measurement device called a Sky Quality Meter (SQM).
  • The free GaN web app from any internet-connected device (which can also be used to submit their measurements from an SQM or printed-out star charts)

Night Sky Network members joined a telecon with Connie Walker of Globe at Night in 2014 and had a lively discussion about the program’s history and how they can participate. The audio of the telecon, transcript, and links to additional resources can be found on their dedicated resource page.

This image of Milan was acquired after the transition to LED technology in the centre. The illumination levels appear to be similar or even brighter in the centre than the suburbs, and the amount of blue light is now much higher, which suggests a greater impact on the ability to see the stars, human health and the environment. Since the European Space Agency’s NightPod device was installed on the ISS in 2012, astronauts have been taken systematic night images. It incorporates a motorised tripod that compensates for the station’s speed and the motion of the Earth below. Before that motion could blur images even though astronauts compensated with high-speed films and manual tracking. In 2003, NASA astronaut Don Pettit’s “barn door tracker” — a lower-tech precursor to NightPod using a motorised drill and assorted parts he accumulated on station — enabled the first motion-compensated night time imagery from the ISS. This image was taken by Samantha Cristoforetti.
Light pollution has been visible from space for a long time, but new LED lights are bright enough that they stand out from older street lights, even from orbit. The above photo was taken by astronaut Samantha Cristoforetti from the ISS cupola in 2015. The newly installed white LED lights in the center of the city of Milan are noticeably brighter than the lights in the surrounding neighborhoods.
NASA/ESA

DarkSky International has long been a champion in the fight against light pollution and a proponent of smart lighting design and policy. Their website (at darksky.org)  provides many resources for amateur astronomers and other like-minded people to help communities understand the negative impacts of light pollution and how smart lighting policies can not only help bring the stars back to their night skies but make their streets safer by using smarter lighting with less glare. Communities and individuals find that their nighttime lighting choices can help save considerable sums of money when they decide to light their streets and homes “smarter, not brighter” with shielded, directional lighting, motion detectors, timers, and even choosing the proper “temperature” of new LED light replacements to avoid the harsh “pure white” glare that many new streetlamps possess. Their pages on community advocacy and on how to choose dark-sky-friendly lighting are extremely helpful and full of great information. There are even local chapters of the IDA in many communities made up of passionate advocates of dark skies.

DarkSky International has notably helped usher in “Dark Sky Places“, areas around the world that are protected from light pollution. “Dark Sky Parks“, in particular, provide visitors with incredible views of the Milky Way and are perfect places to spot the wonders of a meteor shower. These parks also perform a very important function, showing the public the wonders of a truly dark sky to many people who may have never before even seen a handful of stars in the sky, let alone the full, glorious spread of the Milky Way. 

More research into the negative effects of light pollution on the health of humans and the environment is being conducted than ever before. Watching the nighttime light slowly increase in your neighborhood, combined with reading so much bad news, can indeed be disheartening! However, as awareness of light pollution and its negative effects increases, more people are becoming aware of the problem and want to be part of the solution. There is even an episode of PBS Kid’s SciGirls where the main characters help mitigate light pollution in their neighborhood!

Astronomy clubs are uniquely situated to help spread awareness of good lighting practices in their local communities in order to help mitigate light pollution. Take inspiration from Tucson, Arizona, and other dark sky-friendly communities that have adopted good lighting practices. Tucson even reduced its skyglow by 7% after its own citywide lighting conversion, proof that communities can bring the stars back with smart lighting choices.

Originally posted by Dave Prosper: November 2018
Last Updated by Kat Troche: January 2025

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Golden Moon over the Superdome

Golden Moon over the Superdome

The full moon (top right) rises over buildings in New Orleans, Louisiana, including the Superdome. The Superdome has a white rounded top. Billboards and ads can be seen around and on some of the buildings.
NASA/Michael DeMocker

The full moon rises over the Superdome and the city of New Orleans, Louisiana on Monday evening, January 13, 2025.

New Orleans is home to NASA’s Michoud Assembly Facility where several pieces of hardware for the SLS (Space Launch system) are being built. For more than half a century, NASA Michoud has been “America’s Rocket Factory,” the nation’s premiere site for manufacturing and assembly of large-scale space structures and systems.

See more photos from NASA Michoud.

Image credit: NASA/Michael DeMocker

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Monika Luabeya