Ever Restless Mount Dukono Erupts

Ever Restless Mount Dukono Erupts

An ash-rich plume streams northwest from the volcano amidst scattered puffy, white clouds.
An ash-rich volcanic plume streams from the volcano on May 13, 2026, in this image captured by the OLI (Operational Land Imager) on Landsat 9.  
NASA Earth Observatory / Lauren Dauphin

In May 2026, the Global Volcanism Program reported nine actively erupting volcanoes in Indonesia—more than any other country at the time. Such activity is typical for the Southeast Asian archipelago, where eruptions have occurred at 55 volcanoes since the 1960s—the highest total for any country. Japan ranks second with eruptions at 40 volcanoes over that time period, followed by the United States with 39, according to Global Volcanism Program data.

Even for such an eruption-prone country, the persistence of activity at Mount Dukono stands out. The remote stratovolcano, located at the northern end of Halmahera Island, has been erupting nearly continuously since 1933, with near-daily rumbles and frequent emissions of ash and volcanic gases. The volcano routinely flings hunks of semi-molten rock, known as volcanic bombs, hundreds of meters from its vent.

This sort of activity at Dukono turned deadly on May 8, 2026, when ash and volcanic bombs rained down on a group of hikers. In the days following the tragedy, the mountain remained highly active. Indonesia’s volcanological survey reported an average of 52 eruptive events per day between May 9 and 16, with ash plumes rising 400 to 4,300 meters (1,300 feet to 14,000 feet) above the summit.

NASA and other U.S. government satellites detected thermal anomalies, ash plumes, and sulfur dioxide emissions in recent days. Indonesian authorities have set the alert level at 2 (on a scale of 4) and warned the public to stay at least 4 kilometers (2 miles) from the crater.

NASA Earth Observatory image by Lauren Dauphin, using Landsat data from the U.S. Geological Survey. Story by Adam Voiland.

References & Resources

You may also be interested in:

Stay up-to-date with the latest content from NASA as we explore the universe and discover more about our home planet.

Home Reef Adds On

3 min read

The Tongan volcano expanded its mid-Pacific real estate during its latest eruptive phase.

Article

A Volcanic Medley Near Mammoth Lakes 

4 min read

A massive, old caldera and more recently formed craters shape the landscape in the eastern Sierra Nevada.

Article

Scoria Cones on Earth and Mars

7 min read

The hill-shaped features are a sign of explosive volcanic activity—a rarity on the Red Planet.

Article

Powered by WPeMatico

Get The Details…

Robotics, Science Underway as Cosmonauts Prep for Wednesday Spacewalk

Robotics, Science Underway as Cosmonauts Prep for Wednesday Spacewalk

Roscosmos cosmonauts Sergey Kud-Sverchkov (left) and Sergei Mikaev (right), Expedition 74 commander and flight engineer respectively, are pictured inside the Poisk module's airlock trying on their Orlan spacesuits as NASA flight engineer Jessica Meir assists them. The duo was preparing for a spacewalk to install a solar radiation experiment and remove biological exposure hardware on the outside of the International Space Station.
Cosmonauts Sergey Kud-Sverchkov (left) and Sergei Mikaev (right) are pictured inside the Poisk module’s airlock trying on their Orlan spacesuits as NASA flight engineer Jessica Meir (center) assists them.
Sophie Adenot/ESA (European Space Agency)

Robotics controllers wrapped up a weekend of swapping scientific hardware packed inside the SpaceX Dragon cargo spacecraft’s trunk for installation on the International Space Station. Meanwhile, the Expedition 74 crew is continuing its biotechnology and botany research while getting ready for a spacewalk scheduled for Wednesday, May 27.

The orbital outpost hosts a new Earth-observing research facility, the CLARREO Pathfinder, designed to improve satellite imagery and research data accuracy. CLARREO was delivered on May 17 inside Dragon’s unpressurized trunk. It was removed with the Canadarm2 robotic arm, remotely controlled by engineers on Earth, over the Memorial Day weekend and installed on the station’s port side truss structure. Early last week, another research payload, the Space Test Program-Houston 11, was robotically removed from Dragon and installed on the outside of the Columbus laboratory module. The multi-experiment facility will test new space technologies, measure the space environment, and support a variety of research.

A multitude of experiments is also underway inside the orbiting lab with Tuesday’s science schedule packed with biotechnology and space botany to improve health on and off the Earth.

NASA flight engineer Jessica Meir opened up the Life Science Glovebox in the Kibo laboratory module and nourished cartilage-forming cells. The cells are growing into tiny pieces of cartilage tissue to help doctors understand how cartilage develops and repairs itself in microgravity. Results may improve astronaut fitness regimens and promote the development of advanced implants on Earth.

NASA flight engineers Chris Williams and Jack Hathaway each had a unique photography session for two different botany investigations on Tuesday. Williams took pictures of white clover seeds that will be returned to Earth so students can plant them for studying. Hathaway watered and photographed alfalfa plants growing inside the Columbus laboratory module’s Veggie facility for the Veg-06 study to help plants thrive in microgravity and promote food production in space.

Flight engineer Sophie Adenot of ESA (European Space Agency) spent her shift servicing a variety of advanced research hardware. Adenot first connected the Echo Finder-2 ultrasound device to a computer tablet then configured the biomedical device’s performance and wi-fi connectivity. Next, she installed experiment containers, or modules that house biological samples, inside the BioLab that enables microbiology research in weightlessness. Afterward, she checked out the functionality of a portable DNA sequencer and updated the device’s software to support an anti-bacterial investigation.

Cosmonauts Sergey Kud-Sverchkov and Sergei Mikaev are ready for a spacewalk to install a solar radiation experiment and remove other scientific hardware on the outside of the space station. The Roscosmos duo will exit the Poisk module’s airlock at 10:15 a.m. EDT on Wednesday in their Orlan spacesuits with live NASA+ coverage beginning at 9:45 a.m. The pair’s main task will be installing a new experiment that will observe the Sun’s terahertz electromagnetic during events such as solar flares and coronal mass ejections. The cosmonaut duo completed a spacewalk task review and finalized the configuration of their spacewalking tools on Tuesday.

Roscosmos flight engineer Andrey Fedyaev will assist his spacewalking crewmates on Wednesday as he controls the European robotic arm (ERA) from inside the Nauka science module. Fedyaev will use the ERA to help retrieve the Biorisk experiment container housing biological samples exposed to the harsh external microgravity environment. Fedyaev readied the ERA for service positioning it in its pre-spacewalk configuration on Tuesday.

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

Get the latest from NASA delivered every week. Subscribe here.

Powered by WPeMatico

Get The Details…

Mark A. Garcia

NASA to Announce Artemis III Crew, Provide Mission Progress Update

NASA to Announce Artemis III Crew, Provide Mission Progress Update

NASA meatball
NASA meatball

NASA will provide an update on the agency’s Artemis III mission and announce the astronauts assigned to the test flight during a live event at 11 a.m. EDT on Tuesday, June 9, at the agency’s Johnson Space Center in Houston.

The event will stream on NASA+ and on the agency’s YouTube channel. Learn how to watch NASA content through a variety of online platforms, including social media.

Following the event, the Artemis III crew will be available for limited in-person and virtual interviews.

Interview requests must be submitted to the NASA Johnson newsroom by 5 p.m. on June 4. International media interested in attending must contact the NASA Johnson newsroom at jsccommu@mail.nasa.gov by 5 p.m., Thursday, May 28. U.S. media must contact the newsroom by 5 p.m., Thursday, June 4. Registered media will receive confirmation and additional event details by email. NASA’s media accreditation policy is available online.

Artemis III will launch four astronauts from NASA’s Kennedy Space Center in Florida aboard the Orion spacecraft on the SLS (Space Launch System) rocket. The mission will test critical rendezvous and docking capabilities between Orion and commercial human landing systems needed to deliver astronauts to the lunar surface. Building on the successful Artemis II crewed test flight in April, Artemis III will pave the way for future surface missions.

As part of the Golden Age of innovation and exploration, NASA will send Artemis astronauts on increasingly complex missions to explore more of the Moon for scientific discovery, economic benefits, establish an enduring human presence on the lunar surface, and to build on our foundation for the first crewed missions to Mars.

Learn more about NASA’s Artemis program:

https://www.nasa.gov/artemis

-end-

Rachel Kraft
Headquarters, Washington
202-358-1600
rachel.h.kraft@nasa.gov  

Anna Schneider
Johnson Space Center, Houston
281-483-5111
anna.c.schneider@nasa.gov

Share

Details

Last Updated

May 26, 2026

Editor
Jennifer M. Dooren

Powered by WPeMatico

Get The Details…
Jennifer M. Dooren

Chennai City Lights

Chennai City Lights

A view of Chennai at night from the International Space Station shows a sprawling city along the water (upper right). City lights make the city shine while also highlighting roadways. The surrounding area is mostly dark.
NASA/Chris Williams

Chennai, on India’s southern coast along the Bay of Bengal and with a metropolitan population of about 8.7 million, shines with white LED streetlights in this photograph taken at approximately 9:13 p.m. local time on May 2, 2026, from the International Space Station.

Earth observations from the space station let us see how our planet changes over time. In combination with NASA-developed technologies, these observations provide the foundation needed to explore and sustain human life on the Moon, Mars, and beyond.

Image credit: NASA/Chris Williams

Powered by WPeMatico

Get The Details…
HQ Web Team

New Instrument Used Antarctic Ice Sheet to Probe Extreme Universe

New Instrument Used Antarctic Ice Sheet to Probe Extreme Universe

A white balloon with a long tether hovering above the icy ground
This image shows PUEO at the Long Duration Balloon Facility in Antarctica, immediately after balloon release.
Credit: NASA/Scott Battaion

The Payload for Ultrahigh Energy Observations (PUEO) is a NASA Astrophysics Pioneers Program mission designed to detect the most energetic particles in the universe. The PUEO mission flew high above Antarctica on a Long Duration Balloon (LDB) and used the Antarctic ice sheet as an enormous detection volume to look for radio signals generated by the interactions of extremely energetic astrophysical neutrinos as they passed through the ice. In addition to searching for the highest energy neutrinos, PUEO could also detect radio signals from high energy cosmic rays showering in Earth’s atmosphere (a.k.a. air showers), either as the signals entered directly into the instrument or reflected off the ice below. The sensitivity achieved with the PUEO instrument was a result of technology advancements and careful optimization of the experimental design to enable accommodation within the balloon platform’s launch volume. 

The ultra-high energy neutrinos that PUEO was searching for carry information from the most extreme places in the universe, including supermassive black holes that accrete matter at the centers of galaxies, neutron star mergers, and other powerful cosmic accelerators. Because these particles travel large distances along straight lines without being absorbed, they provide a unique view of the distant, most energetic universe. Not only will data collected by PUEO reveal the origin and composition of the highest-energy cosmic rays, it will also test fundamental physics at energies far beyond those achievable in human-made particle accelerators on Earth. 

The PUEO mission built on heritage from the NASA-sponsored Antarctic Impulsive Transient Antenna (ANITA) mission, which had four successful flights from 2006-2016. Like ANITA, PUEO consisted of an array of radio-frequency antennas, an onboard data acquisition system that is triggered by neutrino-like signals and processes and saves the data, and a navigation and command and control system. From its 120,000-foot altitude, PUEO monitored an extremely large volume of Antarctic ice, looking for signals from very rare, high-energy neutrino interactions.  

The first of NASA’s Astrophysics Pioneers missions to launch, PUEO took off Dec. 20, 2025, from NASA’s Long Duration Balloon Facility near McMurdo Station, Antarctica, and flew for 23 days before landing approximately 120 miles (200 km) from the South Pole. The full payload has been recovered, including the data drives. The PUEO team is currently analyzing the data collected—an undertaking that may take up to a year due to the complex nature of the task. 

Two rows of people in front of a tall structure consisting of rows of white components placed in a circle, topped by metallic containers and an additional circular layer of white structures supported by a tower.
The PUEO mission’s on-ice integration team is seen here in front of the fully constructed instrument.
Credit: Cosmin Deaconu

The significant improvement in sensitivity achieved with the PUEO instrument compared to that of ANITA was due to a variety of technology advancements and careful optimization of the experimental design to enable accommodation within the balloon platform’s constrained launch volume. 

Lowering detection threshold with interferometric triggering 

At the heart of PUEO’s technology advancement was a new type of trigger called an interferometric phased array trigger. The PUEO trigger coherently summed signals from multiple antennas in real time, enabling the instrument to detect weaker signals than previously possible. By lowering the trigger threshold, PUEO could dig further into the noise, and find weaker neutrino and cosmic-ray signals than previous experiments. 

More channels in a physically constrained space 

The PUEO antenna collecting area for frequencies above 300 MHz was doubled compared to ANITA, improving the sensitivity to radio emission from particle interactions. To ensure the PUEO payload remained within the allowable launch volume, the team increased the low-frequency cutoff of the PUEO antennas, which enabled them to be even smaller than those used on ANITA. 

Low-frequency instrument for air shower characterization 

To improve sensitivity to extensive air showers produced by cosmic rays and potentially neutrinos, PUEO incorporated a new low-frequency instrument that deployed once the payload reached float altitude (it would have been much too large to fit in the allowable launch volume in its flight configuration). This new low-frequency instrument incorporated antennas that are sensitive down to 50 MHz, and extended PUEOs sensitivity to air showers.  

A rectangular structure containing components attached with wires on top of a workbench
This photo shows the inside of PUEO’s Main Instrument Enclosure, where many of PUEO’s electronics are housed.
Credit: Eric Oberla

Many of the technology advancements that were developed for PUEO may also be applicable for mission concepts under development that would use the lunar regolith as a detector for ultra-high energy cosmic rays, and other potential future radio missions on the moon.

Project Lead: Dr. Abigail Vieregg, David N. Schramm Director of the Kavli Institute for Cosmological Physics and professor of Physics, Astronomy & Astrophysics, and the Enrico Fermi Institute, University of Chicago, assisted by graduate student, Rachel Scrandis 

Sponsoring Organization(s): NASA Astrophysics Division Pioneers Program 

Powered by WPeMatico

Get The Details…