Jump to content
Join the Alien Search, login or register FREE on Aliens and Space Forum
Members Can Post Anonymously On This Site

NASA to Launch 8 Scientific Balloons From New Mexico

NASA

By NASA
in NASA

 Share

Recommended Posts

  • Publishers
NASA Mentor

NASA

Posted
  • Publishers
Posted

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A crane holds a science instrument as a large scientific balloon, tethered to the ground, inflates before liftoff in New Mexico.
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.

Share

Details

Last Updated
Aug 09, 2024
Editor
Olivia F. Littleton
Contact
Olivia F. Littleton
Location
Wallops Flight Facility

Related Terms

Explore More

sweden-balloon.jpeg?w=300
7 min read

NASA Balloons Head North of Arctic Circle for Long-Duration Flights

Article 3 months ago
gusto-launch-photo.jpg?w=300
4 min read

GUSTO Breaks NASA Scientific Balloon Record for Days in Flight

Article 6 months ago
balloons-mcmurdo.jpeg?w=300
6 min read

NASA Scientific Balloons Ready for Flights Over Antarctica

Article 9 months ago

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

×
 Share
Go to topic listing

  • Similar Topics

    • NASA
      NASA, SpaceX Invite Media to Watch Crew-11 Launch to Space Station
      By NASA
      The four crew members of NASA’s SpaceX Crew-11 mission to the International Space Station train inside a SpaceX Dragon spacecraft in Hawthorne, California. From left to right: Roscosmos cosmonaut Oleg Platonov, NASA astronauts Mike Fincke and Zena Cardman, and JAXA astronaut Kimiya Yui.Credit: SpaceX Media accreditation is open for the launch of NASA’s 11th rotational mission of a SpaceX Falcon 9 rocket and Dragon spacecraft carrying astronauts to the International Space Station for a science expedition. NASA’s SpaceX Crew-11 mission is targeted to launch in the late July/early August timeframe from Launch Complex 39A at the agency’s Kennedy Space Center in Florida.
      The mission includes NASA astronauts Zena Cardman, serving as commander; Mike Fincke, pilot; JAXA (Japan Aerospace Exploration Agency) astronaut Kimiya Yui, mission specialist; and Roscosmos cosmonaut Oleg Platonov, mission specialist. This is the first spaceflight for Cardman and Platonov, the fourth trip for Fincke, and the second for Yui, to the orbiting laboratory.
      Media accreditation deadlines for the Crew-11 launch as part of NASA’s Commercial Crew Program are as follows:
      International media without U.S. citizenship must apply by 11:59 p.m. EDT on Sunday, July 6. U.S. media and U.S. citizens representing international media organizations must apply by 11:59 p.m. on Monday, July 14. All accreditation requests must be submitted online at:
      https://media.ksc.nasa.gov
      NASA’s media accreditation policy is online. For questions about accreditation or special logistical requests, email: ksc-media-accreditat@mail.nasa.gov. Requests for space for satellite trucks, tents, or electrical connections are due by Monday, July 14.
      For other questions, please contact NASA Kennedy’s newsroom at: 321-867-2468.
      Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo: 321-501-8425, o Messod Bendayan: 256-930-1371.
      For launch coverage and more information about the mission, visit:
      https://www.nasa.gov/commercialcrew
      -end-
      Joshua Finch / Claire O’Shea
      Headquarters, Washington
      202-358-1100
      joshua.a.finch@nasa.gov / claire.a.o’shea@nasa.gov
      Steve Siceloff / Stephanie Plucinsky
      Kennedy Space Center, Florida
      321-867-2468
      steven.p.siceloff@nasa.gov / stephanie.n.plucinsky@nasa.gov
      Joseph Zakrzewski
      Johnson Space Center, Houston
      281-483-5111
      joseph.a.zakrzewski@nasa.gov
      Share
      Details
      Last Updated Jul 01, 2025 EditorJessica TaveauLocationNASA Headquarters Related Terms
      Commercial Crew Commercial Space Humans in Space International Space Station (ISS) ISS Research Space Operations Mission Directorate View the full article
    • NASA
      NASA Hosts ISRO Officials at Johnson, Kennedy
      By NASA
      NASA NASA astronaut Raja Chari and Dr. V. Narayanan, chairman of ISRO (Indian Space Research Organisation), interact outside the Orion spacecraft mockup at NASA’s Johnson Space Center in Houston. Narayanan and Indian officials visited NASA Johnson and NASA’s Kennedy Space Center in Florida, ahead of the Axiom Mission 4 launch to the International Space Station.

      As part of a collaboration between NASA and ISRO, Axiom Mission 4 delivers on a commitment highlighted by President Trump and Indian Prime Minister Narendra Modi to send the first ISRO astronaut to the station. The space agencies are participating in five joint science investigations and two in-orbit science, technology, engineering, and mathematics demonstrations. NASA and ISRO have a long-standing relationship built on a shared vision to advance scientific knowledge and expand space collaboration.
      Keep Exploring Discover More Topics From NASA
      Low Earth Orbit Economy
      Humans In Space
      Commercial Space
      Private Astronaut Missions
      View the full article
    • NASA
      A New Alloy is Enabling Ultra-Stable Structures Needed for Exoplanet Discovery
      By NASA
      7 min read
      A New Alloy is Enabling Ultra-Stable Structures Needed for Exoplanet Discovery
      A unique new material that shrinks when it is heated and expands when it is cooled could help enable the ultra-stable space telescopes that future NASA missions require to search for habitable worlds.
      Advancements in material technologies are needed to meet the science needs of the next great observatories. These observatories will strive to find, identify, and study exoplanets and their ability to support life. Credit: NASA JPL One of the goals of NASA’s Astrophysics Division is to determine whether we are alone in the universe. NASA’s astrophysics missions seek to answer this question by identifying planets beyond our solar system (exoplanets) that could support life. Over the last two decades, scientists have developed ways to detect atmospheres on exoplanets by closely observing stars through advanced telescopes. As light passes through a planet’s atmosphere or is reflected or emitted from a planet’s surface, telescopes can measure the intensity and spectra (i.e., “color”) of the light, and can detect various shifts in the light caused by gases in the planetary atmosphere. By analyzing these patterns, scientists can determine the types of gasses in the exoplanet’s atmosphere.
      Decoding these shifts is no easy task because the exoplanets appear very near their host stars when we observe them, and the starlight is one billion times brighter than the light from an Earth-size exoplanet. To successfully detect habitable exoplanets, NASA’s future Habitable Worlds Observatory will need a contrast ratio of one to one billion (1:1,000,000,000).
      Achieving this extreme contrast ratio will require a telescope that is 1,000 times more stable than state-of-the-art space-based observatories like NASA’s James Webb Space Telescope and its forthcoming Nancy Grace Roman Space Telescope. New sensors, system architectures, and materials must be integrated and work in concert for future mission success. A team from the company ALLVAR is collaborating with NASA’s Marshall Space Flight Center and NASA’s Jet Propulsion Laboratory to demonstrate how integration of a new material with unique negative thermal expansion characteristics can help enable ultra-stable telescope structures.
      Material stability has always been a limiting factor for observing celestial phenomena. For decades, scientists and engineers have been working to overcome challenges such as micro-creep, thermal expansion, and moisture expansion that detrimentally affect telescope stability. The materials currently used for telescope mirrors and struts have drastically improved the dimensional stability of the great observatories like Webb and Roman, but as indicated in the Decadal Survey on Astronomy and Astrophysics 2020 developed by the National Academies of Sciences, Engineering, and Medicine, they still fall short of the 10 picometer level stability over several hours that will be required for the Habitable Worlds Observatory. For perspective, 10 picometers is roughly 1/10th the diameter of an atom.

      NASA’s Nancy Grace Roman Space Telescope sits atop the support structure and instrument payloads. The long black struts holding the telescope’s secondary mirror will contribute roughly 30% of the wave front error while the larger support structure underneath the primary mirror will contribute another 30%.
      Credit: NASA/Chris Gunn
      Funding from NASA and other sources has enabled this material to transition from the laboratory to the commercial scale. ALLVAR received NASA Small Business Innovative Research (SBIR) funding to scale and integrate a new alloy material into telescope structure demonstrations for potential use on future NASA missions like the Habitable Worlds Observatory. This alloy shrinks when heated and expands when cooled—a property known as negative thermal expansion (NTE). For example, ALLVAR Alloy 30 exhibits a -30 ppm/°C coefficient of thermal expansion (CTE) at room temperature. This means that a 1-meter long piece of this NTE alloy will shrink 0.003 mm for every 1 °C increase in temperature. For comparison, aluminum expands at +23 ppm/°C.

      While other materials expand while heated and contract when cooled, ALLVAR Alloy 30 exhibits a negative thermal expansion, which can compensate for the thermal expansion mismatch of other materials. The thermal strain versus temperature is shown for 6061 Aluminum, A286 Stainless Steel, Titanium 6Al-4V, Invar 36, and ALLVAR Alloy 30.
      Because it shrinks when other materials expand, ALLVAR Alloy 30 can be used to strategically compensate for the expansion and contraction of other materials. The alloy’s unique NTE property and lack of moisture expansion could enable optic designers to address the stability needs of future telescope structures. Calculations have indicated that integrating ALLVAR Alloy 30 into certain telescope designs could improve thermal stability up to 200 times compared to only using traditional materials like aluminum, titanium, Carbon Fiber Reinforced Polymers (CFRPs), and the nickel–iron alloy, Invar.
      The hexapod assembly with six ALLVAR Alloy struts was measured for long-term stability. The stability of the individual struts and the hexapod assembly were measured using interferometry at the University of Florida’s Institute for High Energy Physics and Astrophysics. The struts were found to have a length noise well below the proposed target for the success criteria for the project. Credit: (left) ALLVAR and (right) Simon F. Barke, Ph.D. To demonstrate that negative thermal expansion alloys can enable ultra-stable structures, the ALLVAR team developed a hexapod structure to separate two mirrors made of a commercially available glass ceramic material with ultra-low thermal expansion properties. Invar was bonded to the mirrors and flexures made of Ti6Al4V—a titanium alloy commonly used in aerospace applications—were attached to the Invar. To compensate for the positive CTEs of the Invar and Ti6Al4V components, an NTE ALLVAR Alloy 30 tube was used between the Ti6Al4V flexures to create the struts separating the two mirrors. The natural positive thermal expansion of the Invar and Ti6Al4V components is offset by the negative thermal expansion of the NTE alloy struts, resulting in a structure with an effective zero thermal expansion.
      The stability of the structure was evaluated at the University of Florida Institute for High Energy Physics and Astrophysics. The hexapod structure exhibited stability well below the 100 pm/√Hz target and achieved 11 pm/√Hz. This first iteration is close to the 10 pm stability required for the future Habitable Worlds Observatory. A paper and presentation made at the August 2021 Society of Photo-Optical Instrumentation Engineers conference provides details about this analysis.
      Furthermore, a series of tests run by NASA Marshall showed that the ultra-stable struts were able to achieve a near-zero thermal expansion that matched the mirrors in the above analysis. This result translates into less than a 5 nm root mean square (rms) change in the mirror’s shape across a 28K temperature change.
      The ALLVAR enabled Ultra-Stable Hexapod Assembly undergoing Interferometric Testing between 293K and 265K (right). On the left, the Root Mean Square (RMS) changes in the mirror’s surface shape are visually represented. The three roughly circular red areas are caused by the thermal expansion mismatch of the invar bonding pads with the ZERODUR mirror, while the blue and green sections show little to no changes caused by thermal expansion. The surface diagram shows a less than 5 nanometer RMS change in mirror figure. Credit: NASA’s X-Ray and Cryogenic Facility [XRCF] Beyond ultra-stable structures, the NTE alloy technology has enabled enhanced passive thermal switch performance and has been used to remove the detrimental effects of temperature changes on bolted joints and infrared optics. These applications could impact technologies used in other NASA missions. For example, these new alloys have been integrated into the cryogenic sub-assembly of Roman’s coronagraph technology demonstration. The addition of NTE washers enabled the use of pyrolytic graphite thermal straps for more efficient heat transfer. ALLVAR Alloy 30 is also being used in a high-performance passive thermal switch incorporated into the UC Berkeley Space Science Laboratory’s Lunar Surface Electromagnetics Experiment-Night (LuSEE Night) project aboard Firefly Aerospace’s Blue Ghost Mission 2, which will be delivered to the Moon through NASA’s CLPS (Commercial Lunar Payload Services) initiative. The NTE alloys enabled smaller thermal switch size and greater on-off heat conduction ratios for LuSEE Night.
      Through another recent NASA SBIR effort, the ALLVAR team worked with NASA’s Jet Propulsion Laboratory to develop detailed datasets of ALLVAR Alloy 30 material properties. These large datasets include statistically significant material properties such as strength, elastic modulus, fatigue, and thermal conductivity. The team also collected information about less common properties like micro-creep and micro-yield. With these properties characterized, ALLVAR Alloy 30 has cleared a major hurdle towards space-material qualification.
      As a spinoff of this NASA-funded work, the team is developing a new alloy with tunable thermal expansion properties that can match other materials or even achieve zero CTE. Thermal expansion mismatch causes dimensional stability and force-load issues that can impact fields such as nuclear engineering, quantum computing, aerospace and defense, optics, fundamental physics, and medical imaging. The potential uses for this new material will likely extend far beyond astronomy. For example, ALLVAR developed washers and spacers, are now commercially available to maintain consistent preloads across extreme temperature ranges in both space and terrestrial environments. These washers and spacers excel at counteracting the thermal expansion and contraction of other materials, ensuring stability for demanding applications.
      For additional details, see the entry for this project on NASA TechPort.
      Project Lead: Dr. James A. Monroe, ALLVAR
      The following NASA organizations sponsored this effort: NASA Astrophysics Division, NASA SBIR Program funded by the Space Technology Mission Directorate (STMD).
      Share








      Details
      Last Updated Jul 01, 2025 Related Terms
      Technology Highlights Astrophysics Astrophysics Division Science-enabling Technology Explore More
      7 min read NASA Webb ‘Pierces’ Bullet Cluster, Refines Its Mass


      Article


      1 day ago
      2 min read Hubble Captures an Active Galactic Center


      Article


      4 days ago
      2 min read NASA Citizen Scientists Find New Eclipsing Binary Stars


      Article


      5 days ago
      View the full article
    • USH
      "We got it from them" - Former NASA flight surgeon breaks silence about alien technology
      By USH
      In 1992, Dr. Gregory Rogers a NASA flight surgeon and former Chief of Aerospace Medicine witnessed an event that would stay with him for more than three decades. Now, after years of silence, he’s finally revealing the details of a 15-minute encounter that shattered everything he thought he knew about aerospace technology. 

      With a distinguished career that includes support for 31 space shuttle launches, training as an F-16 pilot, and deep involvement in classified aerospace programs, Dr. Rogers brings unmatched credibility to the conversation. His firsthand account of observing what appeared to be a reverse-engineered craft, emblazoned with "U.S. Air Force" markings, raises profound questions about the true timeline of UAP development and disclosure. 
      The full interview spans nearly two hours. To help navigate the discussion, here’s a timeline so you can jump to the segments that interest you most. 
      00:00 Introduction and Dr. Rogers' Unprecedented Credentials 07:25 The 1992 Cape Canaveral Encounter Begins 18:45 Inside the Hangar: First Glimpse of the Craft 26:30 "We Got It From Them" - The Shocking Revelation 35:15 Technical Analysis: Impossible Flight Characteristics 43:40 Electromagnetic Discharges and Advanced Propulsion 52:20 The Cover Story and 33 Years of Silence 1:01:10 Why He's Speaking Out Now: Grush and Fravor's Influence 1:08:45 Bob Lazar Connections and Reverse Engineering Timeline 1:17:20 Flight Surgeon Stories: The Human Side of Classified Work 1:25:50 G-Force Brain Injuries: An Unreported Military Crisis 1:34:30 Columbia Disaster: When Safety Warnings Are Ignored 1:43:15 The Bureaucratic Resistance to Truth 1:50:40 Congressional Testimony and The Path Forward 1:58:25 Final Thoughts: Legacy vs. Truth
        View the full article
    • NASA
      NASA to Provide Coverage of Progress 92 Launch, Space Station Docking
      By NASA
      The Roscosmos Progress 90 cargo craft approaches the International Space Station for a docking to the Poisk module delivering nearly three tons of food, fuel, and supplies replenishing the Expedition 72 crew. Credit: NASA NASA will provide live coverage of the launch and docking of a Roscosmos cargo spacecraft delivering approximately three tons of food, fuel, and supplies to the Expedition 73 crew aboard the International Space Station.
      The unpiloted Roscosmos Progress 92 spacecraft is scheduled to launch at 3:32 p.m. EDT, Thursday, July 3 (12:32 a.m. Baikonur time, Friday, July 4), on a Soyuz rocket from the Baikonur Cosmodrome in Kazakhstan.
      Live launch coverage will begin at 3:10 p.m. on NASA+. Learn how to watch NASA content through a variety of platforms, including social media.
      After a two-day, in-orbit journey to the station, the spacecraft will dock autonomously to the space-facing port of the orbiting laboratory’s Poisk module at 5:27 p.m. on Saturday, July 5. NASA’s rendezvous and docking coverage will begin at 4:45 p.m. on NASA+.
      The Progress 92 spacecraft will remain docked to the space station for approximately six months before departing for re-entry into Earth’s atmosphere to dispose of trash loaded by the crew.
      Ahead of the spacecraft’s arrival, the Progress 90 spacecraft will undock from the Poisk module on Tuesday, July 1. NASA will not stream undocking.
      The International Space Station is a convergence of science, technology, and human innovation that enables research not possible on Earth. For nearly 25 years, NASA has supported a continuous U.S. human presence aboard the orbiting laboratory, through which astronauts have learned to live and work in space for extended periods of time. The space station is a springboard for developing a low Earth economy and NASA’s next great leaps in exploration, including missions to the Moon under Artemis and, ultimately, human exploration of Mars.
      Learn more about the International Space Station, its research, and crew, at:
      https://www.nasa.gov/station
      -end-
      Jimi Russell
      Headquarters, Washington
      202-358-1100
      james.j.russell@nasa.gov  
      Sandra Jones / Joseph Zakrzewski
      Johnson Space Center, Houston
      281-483-5111
      sandra.p.jones@nasa.gov / joseph.a.zakrzewski@nasa.gov
      Share
      Details
      Last Updated Jun 30, 2025 LocationNASA Headquarters Related Terms
      Humans in Space International Space Station (ISS) Johnson Space Center NASA Headquarters View the full article

  • Check out these Videos

×
×
  • Create New...