25 Years Ago: STS-95, John Glenn Returns to Space

25 Years Ago: STS-95, John Glenn Returns to Space

On Oct. 29, 1998, NASA astronaut John H. Glenn made history again when he returned to space aboard space shuttle Discovery’s STS-95 mission, nearly 37 years after becoming the first American in orbit during his February 1962 Friendship 7 mission. The seven-member STS-95 crew consisted of Commander Curtis L. Brown, Pilot Steven W. Lindsey, Mission Specialists Stephen K. Robinson, Dr. Scott E. Parazynski, and Pedro F. Duque of the European Space Agency, and Payload Specialists Dr. Chiaki Mukai of the National Space Development Agency of Japan, now the Japan Aerospace Exploration Agency, and Glenn, who at age 77 became the oldest person to orbit the Earth, a record that stands to this day. During the nine-day mission, they conducted more than 80 experiments, many of them to study how exposure to weightlessness might relate to the aging process.

The STS-95 crew during their introductory press conference President William J. “Bill” Clinton introduces the STS-95 crew
Left: The STS-95 crew during their introductory press conference. Right: President William J. “Bill” Clinton introduces the STS-95 crew, including Senator John H. Glenn, during a ceremony at NASA’s Johnson Space Center in Houston.

Glenn, whom NASA essentially grounded after his historic 1962 mission for fear of losing a national hero in a spaceflight accident, had always dreamed of returning to space. Upon learning about the physiological changes that occur during spaceflight, and how they somewhat resemble those brought about by aging, now Senator Glenn began lobbying NASA Administrator Daniel S. Goldin for an opportunity to put that theory to the test, by volunteering himself as a subject. Goldin agreed in principle, providing Glenn passed the same physicals as all the other astronauts and that the flight included valuable peer-reviewed research. Glenn did, and teams at NASA working with the National Institutes of Health’s National Institute on Aging to put together a research program of experiments to study bone and muscle loss, balance disorders, sleep disturbances, and changes in the immune system. In addition, the mission conducted other experiments in fields such as materials processing, protein crystal growth, cell biology, and plant growth. Also part of the mission, the SPARTAN 201-5 free-flyer pallet carried instruments to study the Sun’s corona and the solar wind. On Jan. 16, 1998, NASA announced that Glenn would fly as a payload specialist on STS-95. On Feb. 13, the agency announced the rest of the STS-95 crew, who held a press conference at NASA’s Johnson Space Center (JSC) on Feb. 20, coincidentally the 36th anniversary of Glenn’s Friendship 7 flight. During a visit to JSC on April 14, President William J. “Bill” Clinton introduced the STS-95 astronauts.

STS-95 astronauts Steven W. Lindsey, seated left, and Curtis L. Brown; Scott E. Parazynski, standing left, Stephen K. Robinson, Chiaki Mukai of the National Space Development Agency of Japan, now the Japan Aerospace Exploration Agency, Pedro F. Duque of the European Space Agency, and John H. Glenn The STS-95 crew patch Liftoff of space shuttle Discovery on the STS-95 mission, returning Glenn to orbit
Left: STS-95 astronauts Steven W. Lindsey, seated left, and Curtis L. Brown; Scott E. Parazynski, standing left, Stephen K. Robinson, Chiaki Mukai of the National Space Development Agency of Japan, now the Japan Aerospace Exploration Agency, Pedro F. Duque of the European Space Agency, and John H. Glenn. Middle: The STS-95 crew patch. Right: Liftoff of space shuttle Discovery on the STS-95 mission, returning Glenn to orbit.

Space shuttle Discovery’s 25th liftoff took place at 2:19 p.m. EDT on Oct. 29, 1998, from Launch Pad 39B at NASA’s Kennedy Space Center (KSC) in Florida, carrying a double Spacehab module filled with scientific equipment. Brown, making his fifth trip into space and second as commander, and Pilot Lindsey on his second launch, monitored Discovery’s systems as they climbed into orbit, assisted by Mission Specialist Parazynski, a physician making his third trip into space, serving as the flight engineer. Mission Specialist Duque accompanied them on the flight deck. Mission Specialist Robinson, on his second mission, and Payload Specialists Mukai, also a physician and on her second trip to space, and Glenn experienced launch in the shuttle’s middeck.

View of the Spacehab module and the Canadian robotic arm in Discovery’s payload bay The crew’s first view of the interior of the Spacehab module Chiaki Mukai, left, and Stephen K. Robinson begin activating the Spacehab
Left: View of the Spacehab module and the Canadian robotic arm in Discovery’s payload bay. Middle: The crew’s first view of the interior of the Spacehab module. Right: Chiaki Mukai, left, and Stephen K. Robinson begin activating the Spacehab.

Upon reaching orbit, the crew opened the payload bay doors, thus deploying the shuttle’s radiators. Shortly after, the crew opened the hatch from the shuttle’s middeck, translated down the transfer tunnel, and entered Spacehab for the first time, activating the module and turning on the first experiments. These included the life sciences experiments that Glenn conducted to compare the effects of weightlessness and aging.

Physician astronaut Dr. Scott E. Parazynski, left, prepares to draw a blood sample from John H. Glenn Glenn, left, and Parazynski prepare to centrifuge the collected blood sample Glenn, instrumented for a sleep study, prepares to begin his sleep period
Left: Physician astronaut Dr. Scott E. Parazynski, left, prepares to draw a blood sample from John H. Glenn. Middle: Glenn, left, and Parazynski prepare to centrifuge the collected blood sample. Right: Glenn, instrumented for a sleep study, prepares to begin his sleep period.

The STS-95 astronauts use the Canadian-built Remote Manipulator system, or robotic arm, to release the SPARATAN 201-5 free flyer Stephen K. Robinson operates the RMS to retrieve the SPARTAN after its four-day autonomous flight Robinson places the SPARTAN back in the shuttle’s payload bay
Left: The STS-95 astronauts use the Canadian-built Remote Manipulator system, or robotic arm, to release the SPARATAN 201-5 free flyer. Middle: Stephen K. Robinson operates the RMS to retrieve the SPARTAN after its four-day autonomous flight. Right: Robinson places the SPARTAN back in the shuttle’s payload bay.

On the mission’s second day, the crew deployed the PANSAT, a small experimental communications satellite built by the Naval Postgraduate School in Monterey, California. Later in the day, Robinson used the Canadian-built Remote Manipulator System (RMS) or robotic arm to grapple the SPARTAN free flyer. He removed it from its cradle in the payload bay and deployed it for its four-day independent mission. It successfully completed its autonomous flight, traveling up to 30 miles from the shuttle. On flight day 6, Robinson used the RMS to capture SPARTAN and placed it back in its cradle in the payload bay.

Stephen K. Robinson processes a sample in the Advanced Gradient Heating Facility (AGHF) John H. Glenn operates the Osteoporosis Experiment in Orbit (OSTEO) payload investigating the behavior of bone cells in microgravity
Left: Stephen K. Robinson processes a sample in the Advanced Gradient Heating Facility (AGHF). Right: John H. Glenn operates the Osteoporosis Experiment in Orbit (OSTEO) payload investigating the behavior of bone cells in microgravity.

Scott E. Parazynski prepares an experiment in the Microgravity Science Glovebox Chiaki Mukai examines plants grown in the Biological Research in Canisters (BRIC) experiment
Left: Scott E. Parazynski prepares an experiment in the Microgravity Science Glovebox. Right: Chiaki Mukai examines plants grown in the Biological Research in Canisters (BRIC) experiment.

For the remainder of the mission, the seven-member crew busied itself with conducting the 80 experiments in the shuttle’s middeck, the Spacehab, and in the payload bay.

Chiaki Mukai operates the Vestibular Function Experiment Unit (VFEU) investigation the vestibular systems of toadfish John H. Glenn removes cartridges from the Advanced Separation (ADSEP) experiment Steven Lindsey operates the BIOBOX used to store biological samples
Left: Chiaki Mukai operates the Vestibular Function Experiment Unit (VFEU) investigation the vestibular systems of toadfish. Middle: John H. Glenn removes cartridges from the Advanced Separation (ADSEP) experiment. Right: Steven Lindsey operates the BIOBOX used to store biological samples.

Pedro F. Duque operates the Microencapsulation Electrostatic Processing System (MEPS) experiment Chiaki Mukai operates the high-definition camcorder provided by the Japanese company NHK John H. Glenn takes one of the 2,500 Earth observation images obtained during the STS-95 mission
Left: Pedro F. Duque operates the Microencapsulation Electrostatic Processing System (MEPS) experiment. Middle: Chiaki Mukai operates the high-definition camcorder provided by the Japanese company NHK. Right: John H. Glenn takes one of the 2,500 Earth observation images obtained during the STS-95 mission.

Photograph of the Hawaiian Islands  taken by the STS-95 crew Photograph of Houston taken by the STS-95 crew Photograph of Florida taken by the STS-95 crew Photograph of Yemen and the Horn of Africa taken by the STS-95 crew
A selection of the Earth observation photographs taken by the STS-95 crew. Left: The Hawaiian Islands. Middle left: Houston. Middle right: Florida. Right: Yemen and the Horn of Africa.

STS-95 astronauts, clockwise from lower left, Pedro F. Duque, Chiaki Mukai, Scott E. Parazynski, John H. Glenn, Curtis L. Brown, Steven W. Lindsey, and Stephen K. Robinson Brown, left, and Lindsey review entry checklists before donning their launch and entry suits in preparation for returning to Earth Mukai, left, and Duque help Glenn, center, put on his launch and entry suit for reentry
Left: STS-95 astronauts, clockwise from lower left, Pedro F. Duque, Chiaki Mukai, Scott E. Parazynski, John H. Glenn, Curtis L. Brown, Steven W. Lindsey, and Stephen K. Robinson. Middle: Brown, left, and Lindsey review entry checklists before donning their launch and entry suits in preparation for returning to Earth. Right: Mukai, left, and Duque help Glenn, center, put on his launch and entry suit for reentry.

On their last day in space, the crew finished the experiments, closed up the Spacehab module, donned their launch and entry suits, and strapped themselves into their seats to prepare for their return to Earth. They fired the shuttle’s Orbital Maneuvering System engines to begin the descent from orbit. Brown piloted Discovery to a smooth landing at KSC’s Shuttle Landing Facility on Nov. 7, after completing 134 orbits around the Earth in 8 days, 21 hours, and 44 minutes. The astronauts exited Discovery about one hour after landing and immediately began their postflight data collection to measure their immediate physiological responses after returning to a 1 g environment. Ground crews towed Discovery to the Orbiter Processing Facility to begin preparing it for its next mission, STS-96, the first shuttle docking to the International Space Station. The astronauts returned to Houston’s Ellington Field, where a large crowd of well-wishers, including government officials and the media, welcomed them home.

Space Shuttle Discovery lands at NASA’s Kennedy Space Center (KSC) in Florida to end the nine-day STS-95 mission sts-95 postlanding Dignitaries including Isao Uchida, president of Japan’s National Space
Left: Space Shuttle Discovery lands at NASA’s Kennedy Space Center (KSC) in Florida to end the nine-day STS-95 mission. Middle: Dignitaries including Isao Uchida, president of Japan’s National Space Development Agency, KSC Director Roy D. Bridges, and NASA Administrator Daniel S. Goldin greet the returning STS-95 crew after their landing. Right: Dignitaries including Houston Mayor Lee P. Brown, left, U.S. Representative Sheila Jackson Lee, U.S. Senator Kay Bailey Hutchison, Administrator Goldin, and Johnson Space Center Director George W.S. Abbey greet the STS-95 crew at Ellington Field in Houston.

U.S. Senator Kay Bailey Hutchison addresses the crowd at Ellington Field gathered to welcome the STS-95 crew back to Houston NASA Administrator Daniel S. Goldin addresses the crowd at Ellington as the STS-95 astronauts listen
Left: U.S. Senator Kay Bailey Hutchison addresses the crowd at Ellington Field gathered to welcome the STS-95 crew back to Houston. Right: NASA Administrator Daniel S. Goldin addresses the crowd at Ellington as the STS-95 astronauts listen.

Enjoy the crew-narrated video about the STS-95 mission.

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Kelli Mars

Daily Minor Planet Volunteers Spot an Asteroid Passing Close to Earth

Daily Minor Planet Volunteers Spot an Asteroid Passing Close to Earth

2 min read

Daily Minor Planet Volunteers Spot an Asteroid Passing Close to Earth

A starry night sky with a telescope in the foreground.
The Catalina Sky Survey telescope “G96” with the follow-up telescope “I52” in the background.
Credit: David Rankin

Volunteers working with The Daily Minor Planet have made the project’s first big discovery: an asteroid passing very near planet Earth. On the night of October 3rd, a telescope for the Catalina Sky Survey snapped four pictures of a far northern section of the sky. The next day, volunteers  H. N. DiRuscio, X. Liao, V. Gonano and E. Chaghafi spotted a clear streak moving through each image and quickly notified the Daily Minor Planet team.

Other telescopes from around the world went on the hunt for this space rock to find where it was heading. Observations of the asteroid came in from New Mexico and Croatia confirming the asteroid’s trajectory. It was found that the asteroid would pass by Earth about twice as far as the moon the next week and that it was about 50 meters (164 feet) in diameter! 

The Catalina Sky Survey is a NASA funded project to find dangerous Near Earth Asteroids (NEAs) based at the Lunar and Planetary Laboratory of the University of Arizona. The Daily Minor Planet is a citizen science project hosted by the Zooniverse that asks volunteers to review animated nightly images taken by this survey to determine if they are real asteroids or false detections. The Daily Minor Planet team has already submitted observations of over 1,000 main belt asteroids and a few dozen NEA candidates since it started in May of this year. This is the first one to be independently confirmed and published by the Minor Planet Center.

Fortunately, further observations of this object ruled out any possibility of this asteroid hitting the Earth. But the Daily Minor Planet volunteers continue to search! New data is uploaded after each clear night of observing, so there are always new discoveries to be made. To join the search, visit https://www.zooniverse.org/projects/fulsdavid/the-daily-minor-planet

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Accounts Receivable

Accounts Receivable

6 Min Read

Accounts Receivable

ACH Credit Payment

ACH Credit is a payment method that allows a payer to initiate payment through their financial institution through the ACH/Federal Reserve network. ACH Credit allows the payer to control the initiation and timing of payments as well as when the date the funds are sent. Please view the instructions by accessing ACH Credit Payment Instructions.

Payments to NASA

For your convenience and fast results, you have the following options to pay online:
Option 1: Pay Via Bank Account (ACH Direct Debit, also known as electronic check); or
Option 2: Pay Via Plastic Card (any credit or debit card with Visa, MasterCard, American Express or Discover, debit cards are accepted by Pay.gov).
For information on other payment, options please contact NASA Shared Services Center (NSSC) Customer Contact Center: 1.877.677.2123.

NSSC Accounts Receivable does not process checks for returned funds from Grantees.
Grantees should refer to Health and Human Services website for instructions on returning funds.

For other payment options, please contact the Customer Contact Center.

Check Payments
Make checks payable to: NSSC/For the account (s) of [applicable center]
Please include the bill number on your check.
Send all check payments to the following address:
NASA Shared Services Center (NSSC)
Building 1111, Jerry Hlass Road
Stennis Space Center, MS 39529

Credit/Debit Card Payments to NASA

To begin, please go to the Treasury Financial Manual at: https://tfm.fiscal.treasury.gov/v1/p5/c700.html.  
Please reference the following sections for more guidance on the following items: 

Credit Card

Section 7045—Limitations on Card Collection Transactions
Section 7045.10—Transaction Maximums

Debit Card

Section 7010—Scope, Applicability, and Network Rules
Section 7025—Honoring of Cards and Surcharges
Section 7025.10—Honoring of Cards
Section 7025.20—Surcharges

Testing
Agencies wishing to test the new credit card daily dollar value limits can do so using the Vanity emulator. Use the $1.72 amount. The return code will be V2. Please refer to section 10.10 and Appendix A of the Pay.gov Agency Guide to the Collections Service for additional information on using the Vanity emulator.  

Fedwire Payments for NASA

The Federal Reserve Banks provide the Fedwire Funds Service, a real-time gross settlement system that enables participants to initiate funds transfer that are immediate, final, and irrevocable once processed. Depository institutions and certain other financial institutions that hold an account with a Federal Reserve Bank are eligible to participate in the Fedwire Funds Services. There are approximately 7,300 participants who make Fedwire funds transfers. The Fedwire Funds Service is generally used to make large-value, time-critical payments. International and Domestic financial institutions can use Fedwire to send a wire transfer in United States dollars directly to the bank to the United States Treasury, which then forwards the payment to NASA.

The Fedwire Funds Service is a credit transfer service. Participants originate funds transfers by instructing a Federal Reserve Bank to debit funds from its own account and credit funds to the account of another participant. Participants may originate funds transfers online, by initiating a secure electronic message, or off line, via telephone procedures.

The Fedwire Funds Service business day begins at 9:00 p.m. Eastern Time (ET) on the preceding calendar day and ends at 6:30 p.m. ET, Monday through Friday, excluding designated holidays. For example, the Fedwire Funds Service opens for Monday at 9:00 p.m. on the preceding Sunday. The deadline for initiating transfers for the benefit of a third party (such as a bank’s customer) is 6:00 p.m. ET each business day. Under certain circumstances, Fedwire Funds Service operating hours may be extended by the Federal Reserve Banks.

For more information, please visit: https://frbservices.org/financial-services/wires/index.html

Sending A Fedwire


Payments can be made through your Financial Institution. Your Financial Institution may charge additional fees for this service which will be incurred by the customer. Please also include a point of contact for your business in case NASA has any questions about the payment once it is received. Include any other identifying information with the payment, such as the bill of collection number, reference numbers and identify where to apply the payment. Customers should use the following instructions that meet their payment requirements.
Note: NASA does not charge the Fedwire fee.

Pay.Gov Payments

Online payments to NASA can be made through Pay.Gov through NASA Online Payment link only. Customers should use the following instructions for Pay.Gov that meet their payment requirements:

1. Reimbursable Customers requesting to make an Advance Payment, please view instructions by accessing NASA Online Payments via Pay.Gov (Advances).
2. Direct Customers (Non-Reimbursable) requesting to make a payment on a Bill of Collection, please view instructions by accessing NASA Online Payments via Pay.Gov (Direct).

3. Solutions for Enterprise-Wide Procurement (SEWP) Customers requesting to make a payment on a SEWP Fee, please view instructions by accessing NASA Online Payments via Pay.Gov (SEWP).
4. Click to view a Pay.Gov Screen Shot Example.

SWIFT Payment

Society for Worldwide Interbank Financial Telecommunication (SWIFT) payment is an interbank communications system in which financial institutions worldwide can send and receive information about financial transactions in a secure, standardized and reliable environment. SWIFT does not facilitate funds transfer; rather, it sends payment orders, which must be settled by correspondent accounts that the institutions have with each other. 
 
Each financial institution, to exchange banking transactions, must have a banking relationship by either being a bank or affiliating itself with one or more. SWIFT is linked to more than 9,000 financial institutions in 209 countries and territories. For payments to NASA, the SWIFT message directs funds to a United States Treasury account, which then references and forwards the payment to a NASA Center. Please view the instructions by accessing SWIFT Payment Instructions.
 
Note: NASA does not charge the SWIFT fee.
 

Foreign Payments

International Treasury Service (ITS) or ITS.gov is a comprehensive payment and collection system.  ITS.gov is the federal government’s single portal for all types of international transactions, including payments and collections. Wire transfers allow for the individualized transmission of funds from single individuals or entities to others while still maintaining the efficiencies associated with the fast and secure movement of money. By using a wire transfer, people in different geographic locations can safely transfer money to locales and financial institutions around the globe.

International wire transfers are monitored by the Office of Foreign Assets Control (OFAC), and agency of the U.S. Treasury tasked with preventing money from going to or coming from countries that are the subject of sanctions by the U.S. government.

Please reference Foreign Currency Accounts and ITS Collection Instructions for more information.

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NASA

NASA X-ray Telescopes Reveal the “Bones” of a Ghostly Cosmic Hand

NASA X-ray Telescopes Reveal the “Bones” of a Ghostly Cosmic Hand

4 min read

NASA X-ray Telescopes Reveal the “Bones” of a Ghostly Cosmic Hand

This release features a composite image of a pulsar wind nebula, which strongly resembles a ghostly purple hand with sparkling fingertips. A pulsar is a highly magnetized collapsed star that rotates and creates jets of matter flowing away from its poles. These jets, along with intense winds of particles, form pulsar wind nebulae. Here, the pulsar wind nebula known as MSH 15-52 resembles a hazy purple cloud set against a black, starry backdrop. Both NASA's Chandra X-ray Observatory and the Imaging X-ray Polarimetry Explorer (IXPE) have observed MSH 15-52. Their observations revealed that the shape of this pulsar wind nebula strongly resembles a human hand, including five fingers, a palm and wrist. The bright white spot near the base of the palm is the pulsar itself. The three longest fingertips of the hand-shape point toward our upper right, or 1:00 on a clock face. There, a small, mottled, orange and yellow cloud appears to sparkle or glow like embers. This orange cloud is part of the remains of the supernova explosion that created the pulsar. The backdrop of stars was captured in infrared light.
Credit: X-ray: NASA/CXC/Stanford Univ./R. Romani et al. (Chandra); NASA/MSFC (IXPE); Infared: NASA/JPL-Caltech/DECaPS; Image Processing: NASA/CXC/SAO/J. Schmidt)

In 1895, Wilhelm Röntgen discovered X-rays and used them to image the bones in his wife’s hand, kicking off a revolutionary diagnostic tool for medicine. Now two of NASA’s X-ray space telescopes have combined their imaging powers to unveil the magnetic field “bones” of a remarkable hand-shaped structure in space. Together, these telescopes reveal the behavior of a dead collapsed star that lives on through plumes of particles of energized matter and antimatter. 

Around 1,500 years ago, a giant star in our Galaxy ran out of nuclear fuel to burn. When this happened, the star collapsed onto itself and formed an extremely dense object called a neutron star. 

Rotating neutron stars with strong magnetic fields, or pulsars, provide laboratories for extreme physics, with conditions that cannot be replicated on Earth. Young pulsars can create jets of matter and antimatter moving away from the poles of the pulsar, along with an intense wind, forming a “pulsar wind nebula”.

This release features a composite image of a pulsar wind nebula, which strongly resembles a ghostly white hand with sparkling fingertips
By combining data from Chandra and IXPE, astronomers are learning more about how a pulsar is injecting particles into space and shaping its environment. The X-ray data are shown along with infrared data from the Dark Energy Camera in Chile. Young pulsars can create jets of matter and antimatter moving away from the poles of the pulsar, along with an intense wind, forming a “pulsar wind nebula”. This one, known as MSH 15-52, has a shape resembling a human hand and provides insight into how these objects are formed.
Credit: X-ray: NASA/CXC/Stanford Univ./R. Romani et al. (Chandra); NASA/MSFC (IXPE); Infared: NASA/JPL-Caltech/DECaPS; Image Processing: NASA/CXC/SAO/J. Schmidt

In 2001, NASA’s Chandra X-ray Observatory first observed the pulsar PSR B1509-58 and revealed that its pulsar wind nebula (referred to as MSH 15-52) resembles a human hand. The pulsar is located at the base of the “palm” of the nebula. MSH 15-52 is located 16,000 light-years from Earth.

Now, NASA’s newest X-ray telescope, the Imaging X-ray Polarimetry Explorer (IXPE), has observed MSH 15-52 for about 17 days, the longest it has looked at any single object since it launched in December 2021.

“The IXPE data gives us the first map of the magnetic field in the ‘hand’,” said Roger Romani of Stanford University in California, who led the study. “The charged particles producing the X-rays travel along the magnetic field, determining the basic shape of the nebula, like the bones do in a person’s hand.”

IXPE provides information about the electric field orientation of X-rays, determined by the magnetic field of the X-ray source. This is called X-ray polarization. In large regions of MSH 15-52 the amount of polarization is remarkably high, reaching the maximum level expected from theoretical work. To achieve that strength, the magnetic field must be very straight and uniform, meaning there is little turbulence in those regions of the pulsar wind nebula. 

“We’re all familiar with X-rays as a diagnostic medical tool for humans,” said co-author Josephine Wong, also of Stanford. “Here we’re using X-rays in a different way, but they are again revealing information that is otherwise hidden from us.” 

One particularly interesting feature of MSH 15-52 is a bright X-ray jet directed from the pulsar to the “wrist” at the bottom of the image. The new IXPE data reveal that the polarization at the start of the jet is low, likely because this is a turbulent region with complex, tangled magnetic fields associated with the generation of high-energy particles. By the end of the jet the magnetic field lines appear to straighten and become much more uniform, causing the polarization to become much larger.

A ghostly looking purple hand in space.
Credit: X-ray: NASA/CXC/Stanford Univ./R. Romani et al. (Chandra); NASA/MSFC (IXPE); Infared: NASA/JPL-Caltech/DECaPS; Image Processing: NASA/CXC/SAO/J. Schmidt

These results imply that particles are given an energy boost in complex turbulent regions near the pulsar at the base of the palm, and flow to areas where the magnetic field is uniform along the wrist, fingers and thumb.

“We’ve uncovered the life history of super energetic matter and antimatter particles around the pulsar,” said co-author Niccolò Di Lalla, also of Stanford. “This teaches us about how pulsars can act as particle accelerators.”

IXPE has also detected similar magnetic fields for the Vela and Crab pulsar wind nebulae, which implies that they may be surprisingly common in these objects.

These results are published in a new paper in The Astrophysical Journal. 

IXPE is a collaboration between NASA and the Italian Space Agency with partners and science collaborators in 12 countries. IXPE is led by Marshall. Ball Aerospace, headquartered in Broomfield, Colorado, manages spacecraft operations together with the University of Colorado’s Laboratory for Atmospheric and Space Physics in Boulder.

NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.

Read more from NASA’s Chandra X-ray Observatory.

For more Chandra images, multimedia and related materials, visit:

https://www.nasa.gov/chandra

Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998

Jonathan Deal
Marshall Space Flight Center
Huntsville, Ala.
256-544-0034

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Beth Ridgeway

NASA, Partners Explore Sustainable Fuel’s Effects on Aircraft Contrails

NASA, Partners Explore Sustainable Fuel’s Effects on Aircraft Contrails

3 min read

NASA, Partners Explore Sustainable Fuel’s Effects on Aircraft Contrails

NASA Armstrong Flight Research Center’s DC-8 aircraft takes flight over the northwestern U.S. to monitor emissions from Boeing’s ecoDemonstrator Explorer aircraft.
NASA Armstrong’s DC-8 aircraft flies over the northwestern U.S. to monitor emissions from Boeing’s ecoDemonstrator Explorer aircraft.  As the largest flying science laboratory in the world, the DC-8 is equipped to collect crucial data about the sustainable aviation fuel and its effects on condensation trail formation.
NASA/Jim Ross

Contrails, the lines of clouds left by high-flying aircraft that crisscross the skies, are familiar sights, but they may have an unseen effect on the planet – trapping heat in the atmosphere. Working with Boeing, United Airlines, and other industry, government, and international partners, NASA researchers are collecting data to see how new, greener aviation fuels can help reduce the problem.

Throughout October, NASA has supported contrail research through Boeing’s ecoDemonstrator program, a multi-year effort to analyze sustainable aviation fuel its capacity to benefit the environment.

Boeing’s current ecoDemonstrator Explorer aircraft, a 737-10, has conducted test flights switching between tanks filled either with 100% sustainable aviation fuel or conventional fuel. NASA’s DC-8 aircraft, the world’s largest flying science laboratory, has followed, measuring emissions and contrail ice formation from each type of fuel. This data will help determine whether sustainable aviation fuels help reduce the formation of contrails.

“Contrails are believed to be a major source of pollution,” said Rich Moore, a research physical scientist in NASA’s Langley Aerosol Research Group Experiment. Moore was among the researchers who flew aboard the DC-8. “With this mission, we’re looking not so much at correcting contrails, but at preventing them.”

In addition to the DC-8, which is based at NASA’s Armstrong Flight Research Center in Edwards,

California, the agency contributed other critical capabilities, including a mobile laboratory for ground testing. Other collaborators for the ecoDemonstrator flights include General Electric Aerospace, the German Aerospace Center, National Research Council Canada, and the Federal Aviation Administration.

Within a year, the researchers will publish their results.

“One of the most amazing things about this collaboration is that this data will be released publicly with the world,” Moore said.

Contrail clouds form when aircraft operate in the cold temperatures at high altitudes and water vapor in engine exhaust condenses and freezes. Made up of ice particles, contrail clouds can have both a cooling and warming effect based on ambient conditions, timing, and persistence – but scientists estimate that their warming effect is greater on a global scale.

Over the past decade, NASA-funded research has shown that sustainable aviation fuels have significant benefits for reducing engine particle emissions that can influence local air quality near airports and contribute to the formation of contrails.

Efforts to develop and evaluate sustainable aviation fuels focus on delivering the performance of conventional jet fuel without releasing new carbon dioxide into the environment. These fuels can be derived from sustainable sources such as feedstocks and waste resources.

Flight testing remains the gold standard for understanding aerospace innovations and their environmental impacts, making partnerships like ecoDemonstrator and research aircrafts like NASA’s DC-8 important sources for data that can help make aviation more sustainable, protecting the environment and improving life on Earth.

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Last Updated

Oct 30, 2023

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Ryan M. Henderson

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Ryan M. Henderson