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Impressive activity around and above the Popocatépetl volcano, Mexico
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By NASA
Hubble Space Telescope Home NASA’s Hubble Sees a… Hubble Space Telescope Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Hubble News Archive Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts E-books Lithographs Fact Sheets Glossary Posters Hubble on the NASA App More Online Activities 3 Min Read NASA’s Hubble Sees a Stellar Volcano
NASA’s Hubble Space Telescope captures a spectacular view the star R Aquarii. Credits:
NASA, ESA, Matthias Stute , Margarita Karovska , Davide De Martin (ESA/Hubble), Mahdi Zamani (ESA/Hubble) NASA’s Hubble Space Telescope has provided a dramatic and colorful close-up look at one of the most rambunctious stars in our galaxy, weaving a huge spiral pattern among the stars.
Located approximately 700 light-years away, a binary star system called R Aquarii undergoes violent eruptions that blast out huge filaments of glowing gas. The twisted stellar outflows make the region look like a lawn sprinkler gone berserk. This dramatically demonstrates how the universe redistributes the products of nuclear energy that form deep inside stars and jet back into space.
R Aquarii belongs to a class of double stars called symbiotic stars. The primary star is an aging red giant and its companion is a compact burned-out star known as a white dwarf. The red giant primary star is classified as a Mira variable that is over 400 times larger than our Sun. The bloated monster star pulsates, changes temperature, and varies in brightness by a factor of 750 times over a roughly 390-day period. At its peak the star is blinding at nearly 5,000 times our Sun’s brightness.
This NASA Hubble Space Telescope image features the binary star system R Aquarii. NASA, ESA, Matthias Stute , Margarita Karovska , Davide De Martin (ESA/Hubble), Mahdi Zamani (ESA/Hubble) When the white dwarf star swings closest to the red giant along its 44-year orbital period, it gravitationally siphons off hydrogen gas. This material accumulates on the dwarf star’s surface until it undergoes spontaneous nuclear fusion, making that surface explode like a gigantic hydrogen bomb. After the outburst, the fueling cycle begins again.
This outburst ejects geyser-like filaments shooting out from the core, forming weird loops and trails as the plasma emerges in streamers. The plasma is twisted by the force of the explosion and channeled upwards and outwards by strong magnetic fields. The outflow appears to bend back on itself into a spiral pattern. The plasma is shooting into space over 1 million miles per hour – fast enough to travel from Earth to the Moon in 15 minutes! The filaments are glowing in visible light because they are energized by blistering radiation from the stellar duo.
Hubble first observed the star in 1990. R Aquarii was resolved into two very bright stars separated by about 1.6 billion miles. The ESA/Hubble team now has made a unique timelapse of R Aquarii’s dynamic behavior, from observations spanning from 2014 to 2023. Across the five images, the rapid and dramatic evolution of the binary star and its surrounding nebula can be seen. The binary star dims and brightens due to strong pulsations in the red giant star.
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This video features five frames spanning from 2014 to 2023 of R Aquarii. These frames show the brightness of the central binary changing over time due to strong pulsations in the red giant star. The central structures spiral outward due to their interaction with material previously ejected by the binary. This timelapse highlights the value of Hubble’s high resolution optical observations in the changing universe, known as time-domain astronomy. NASA, ESA, Matthias Stute , Margarita Karovska , Davide De Martin , Mahdi Zamani , N. Bartmann (ESA/Hubble) The scale of the event is extraordinary even in astronomical terms. Space-blasted material can be traced out to at least 248 billion miles from the stars, or 24 times our solar system’s diameter. Images like these and more from Hubble are expected to revolutionize our ideas about such unique stellar “volcanoes” as R Aquarii.
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.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov
Ray Villard
Space Telescope Science Institute, Baltimore, MD
Bethany Downer
ESA/Hubble
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Last Updated Oct 16, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
Astrophysics Astrophysics Division Binary Stars Goddard Space Flight Center Hubble Space Telescope Science Mission Directorate Stars The Universe Keep Exploring Discover More Topics From Hubble
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By NASA
NASA/Wanmei Liang, USGS On June 10, 2023, the Operational Land Imager on Landsat 8 acquired this image of Mount Taranaki, a snow-capped mountain in New Zealand that is ringed by a dark green forest. Two older and extinct volcanoes, Kaitake and Pouakai, lie to the northwest of its peak.
Learn more about Mount Taranaki.
Image Credit: NASA/Wanmei Liang, USGS
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By NASA
Ruidoso, New Mexico lay in an unusual hush on June 20, 2024. During any normal summer day, the village in the southern part of the state lives up to the Spanish translation of its name — noisy.
But the bustle of this vacation hotspot, which attracts nearly 2 million visitors each year, was stifled by a mandatory evacuation order issued as wildfires raged unchecked across Lincoln County and the Mescalero Apache Reservation. After four days of fires, news of the disaster began spreading to surrounding communities.
Wildfires cast an orange haze over the Sierra Blanca mountain range in Ruidoso, New Mexico, on June 20, 2024. Image courtesy of James Herrera At NASA’s White Sands Test Facility (WSTF), Fire Department Deputy Chief James Herrera and his team were on high alert from the moment the blaze began.
“There were so many rumors, so many things going on,” Herrera said. “People were saying the town was completely burning down. We were expecting the worst before we even got there.”
Herrera’s expectations were realistic.
Tinderbox conditions, rough terrain, and winds reaching more than 70 miles per hour fueled the flames raging at the South Fork area west of Ruidoso, devouring nearly 5,000 acres just hours after the fire started.
As first responders expended every resource available to them both on the ground and in the air, a second fire — the Salt Fire — broke out on tribal land south of the village.
Now the twin infernos closed in on Ruidoso like a set of jaws poised to snap shut.
Gov. Michelle Lujan Grisham quickly declared a state of emergency and the early whispers crescendoed into an urgent plea for aid from anyone who would listen.
There was no doubt in Herrera’s mind: WSTF, based 150 miles from Ruidoso in Las Cruces, New Mexico, would answer the call.
“Never once did [WSTF leadership] say ‘Sorry, we can’t help,’” he said. “They asked, ‘What can we do to help? How can we get there as soon as possible?’”
Shift changes made for an earliest possible departure at dawn on June 20. The WSTF Fire Department spent the night preparing their truck, gathering their belongings, and bracing for the uncertain.
“We didn’t know where we were going to sleep, there were no hotels, everything was closed,” Herrera said. “More than likely, we were going to end up sleeping in our engine.”
For the moment, rest was off the table.
“I’m not going to lie, we probably didn’t even sleep. I know I didn’t,” Herrera said. “I closed my eyes, and it was two o’clock in the morning. Time to get going.”
After checking in at the Incident Command Post, Herrera and the WSTF team — Lieutenant Gary Sida, firefighters Steven Olsson and Gabriel Rodriguez, and driver and engineer Tommy Montoya — were deployed to Ruidoso’s Casino Apache Travel Center off Highway 70.
Deputy Chief James Herrera (far left) and his crew (L-R) Driver/Operator Tommy Montoya, Firefighter Gabe Rodriguez (top), Lieutenant Gary Sida, and Firefighter Stephen Olsson return to a hero’s welcome at White Sands Test Facility in Las Cruces, New Mexico. NASA/Anthony Luis Quiterio When Herrera and his four-man crew reached the edge of the deserted mountain town, the silence was more than unusual. It was unsettling, as heavy as the smoke suffocating the Sierra Blanca Peak.
“You could not see more than 100 feet,” Herrera said. “The only sign of life was all the fire agencies that were there. It was an eerie feeling.”
NASA’s arrival on scene brought a shift from anxiety to optimism and relief.
“There were tears in some of their eyes because we were showing up to help,” he said. “I could hear people saying, ‘What’s NASA doing here?’” He added, “One gentleman asked us how we got there. I joked that we drove the whole line from Kennedy Space Center.”
By the afternoon, the light-heartedness among comrades was extinguished as escalating winds charged the situation to a fever pitch. The fire, once perched atop the mountains, began hurling down in a landslide of embers, leaping across Highway 70, and forming a nearly complete ring of danger.
Breathing grew difficult as ground crews, with aerial units roaring overhead, battled a relentless assault of heat. WSTF Fire Department’s assignment evolved into an effort to protect anything and everything within reach. “It makes you realize how fast something can be taken away from you,” Herrera said.
The NASA WSTF Fire Department makes engine preparations along U.S. Route 70 at the Ruidoso border. Image courtesy of James Herrera Though disaster descended in an instant, the day itself had been long. Herrera and his team were released from duty after a grueling 12 hours spent providing critical support to wildland units and successfully protecting nearby buildings.
“Once it starts to calm down, you can feel your hands start to shake a little bit because this thing was getting out of control really fast,” Herrera said.
By the weekend, containment efforts were gaining ground thanks to the efforts of a combined 780-strong emergency response force. Eager to rebuild, Ruidoso residents trickled back in, but the village soon encountered another challenge: rain.
Following the South Fork and Salt fires — which claimed an estimated 25,000 acres, 1,400 structures, and two lives — monsoons battered Ruidoso. Throughout July, deluges washed over the region’s burn scars in an ironic insult to injury leaving people trapped in vehicles and homes underwater. As recently as Aug. 7, evacuations continued as the Ruidoso Police Department worked to preemptively clear the Cherokee Mobile Village due to past flash flooding in the area.
In this harsh landscape of crisis and aftermath, Herrera views mutual aid as more than a tactical response, but a vital investment.
“Building goodwill with the community is akin to cultivating fertile ground for growth and success,” he said. “I strongly feel it strengthens the bond between us and our community.”
With the wet season expected to continue through the end of September, Ruidoso’s forecast remains uncertain. Even as storm clouds gather, one thing is clear: if the call comes again, the WSTF Fire Department will always be ready to answer.
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By NASA
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
A scientific balloon is inflated for the Salter Test Flight before being released during NASA’s 2023 fall balloon campaign. The test flight returns for the 2024 campaign in Fort Sumner, New Mexico, carrying several smaller payloads.NASA/Andrew Hynous NASA’s Scientific Balloon Program has kicked off its annual fall balloon campaign at the agency’s balloon launch facility in Fort Sumner, New Mexico. Eight balloon flights carrying scientific experiments and technology demonstrations are scheduled to launch from mid-August through mid-October.
The flights will support 16 missions, including investigations in the fields of astrophysics, heliophysics, and atmospheric research.
“The annual Fort Sumner campaign is the cornerstone of the NASA Balloon Program operations,” said Andrew Hamilton, acting chief of NASA’s Balloon Program Office. “Not only are we launching a large number of missions, but these flights set the foundation for follow-on missions from our long-duration launch facilities in Antarctica, New Zealand, and Sweden. The Fort Sumner campaign is also a strong focus for our student-based payloads and is an excellent training opportunity for our up-and-coming scientists and engineers.”
Returning to the fall lineup is the EXCITE (Exoplanet Climate Infrared Telescope) mission led by Peter Nagler, principal investigator, NASA’s Goddard Space Flight Center in Greenbelt, Maryland. EXCITE features an astronomical telescope developed to study the atmospheric properties of Jupiter-type exoplanets from near space. EXCITE’s launch was delayed during the 2023 campaign due to weather conditions.
“The whole EXCITE team is looking forward to our upcoming field campaign and launch opportunity from Fort Sumner,” said Nagler. “We’re bringing a more capable instrument than we did last year and are excited to prove EXCITE from North America before we bring it to the Antarctic for our future long-duration science flight.”
Some additional missions scheduled to launch include:
Salter Test Flight: The test flight aims to verify system design and support several smaller payloads on the flight called piggyback missions. HASP 1.0 (High-Altitude Student Platform): This platform supports up to 12 student payloads and assists in training the next generation of aerospace scientists and engineers. It is designed to flight test compact satellites, prototypes, and other small payloads. HASP 2.0 (High-Altitude Student Platform 2): This engineering test flight of the upgraded gondola and systems for the HASP program aims to double the carrying capability of student payloads. DR-TES (mini-Dilution Refrigerator and a Transition Edge Sensor): This flight will test a cooling system and a gamma-ray detector in a near-space environment. TIM Test Flight (Terahertz Intensity Mapper): This experiment will study galaxy evolution and the history of cosmic star formation. THAI-SPICE (Testbed for High-Acuity Imaging – Stable Photometry and Image-motion Compensation Experiment): The goal of this project is to build and demonstrate a fine-pointing system for stratospheric payloads with balloon-borne telescopes. TinMan (Thermalized Neutron Measurement Experiment): This hand-launch mission features a 60-pound payload designed to help better understand how thermal neutrons may affect aircraft electronics. An additional eight piggyback missions will ride along on flights to support science and technology development. Three of these piggyback missions are technology demonstrations led by the balloon program team at NASA’s Wallops Flight Facility in Virginia. Their common goal is to enhance the capabilities of NASA balloon missions. CASBa (Comprehensive Avionics System for Balloons) aims to upgrade the flight control systems for NASA balloon missions. DINGO (Dynamics INstrumentation for GOndolas) and SPARROW-5 (Sensor Package for Attitude, Rotation, and Relative Observable Winds – Five) are technology maturation projects designed to provide new sensing capabilities to NASA balloon missions.
Zero-pressure balloons, used in this campaign, are in thermal equilibrium with their surroundings as they fly. They maintain a zero-pressure differential with ducts that allow gas to escape to prevent an increase in pressure from inside the balloons as they rise above Earth’s surface. This zero-pressure design makes the balloons very robust and well-suited for short, domestic flights, such as those in this campaign. The loss of lift gas during the day-to-night cycle affects the balloon’s altitude after repeated day-to-night cycles; however, this can be overcome by launching from the polar regions, such as Sweden or Antarctica, where the Sun does not set on the balloon in the summer.
To follow the missions in the 2024 Fort Sumner fall campaign, visit NASA’s Columbia Scientific Balloon Facility website for real-time updates of balloons’ altitudes and locations during flight.
NASA’s Wallops Flight Facility in Virginia manages the agency’s scientific balloon flight program with 10 to 15 flights each year from launch sites worldwide. Peraton, which operates NASA’s Columbia Scientific Balloon Facility (CSBF) in Palestine, Texas, provides mission planning, engineering services, and field operations for NASA’s Scientific Balloon Program. The CSBF team has launched more than 1,700 scientific balloons over some 40 years of operations. NASA’s balloons are fabricated by Aerostar. The NASA Scientific Balloon Program is funded by the Science Mission Directorate’s Astrophysics Division at NASA Headquarters in Washington.
For more information on NASA’s Scientific Balloon Program, visit: https://www.nasa.gov/scientificballoons
By Olivia Littleton
NASA’s Wallops Flight Facility, Wallops Island, Va.
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Last Updated Aug 09, 2024 EditorOlivia F. LittletonContactOlivia F. Littletonolivia.f.littleton@nasa.govLocationWallops Flight Facility Related Terms
Scientific Balloons Astrophysics Goddard Space Flight Center Wallops Flight Facility Explore More
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