samedi 12 mai 2018

Mars Helicopter to Fly on NASA's Next Red Planet Rover Mission












NASA - Mars Rover Mission logo.

May 12, 2018


Image above: The Mars Helicopter, a small, autonomous rotorcraft, will travel with NASA's Mars 2020 rover, currently scheduled to launch in July 2020, to demonstrate the viability and potential of heavier-than-air vehicles on the Red Planet. Image Credits: NASA/JPL-Caltech.

NASA is sending a helicopter to Mars.

The Mars Helicopter, a small, autonomous rotorcraft, will travel with the agency's Mars 2020 rover mission, currently scheduled to launch in July 2020, to demonstrate the viability and potential of heavier-than-air vehicles on the Red Planet.

"NASA has a proud history of firsts," said NASA Administrator Jim Bridenstine. "The idea of a helicopter flying the skies of another planet is thrilling. The Mars Helicopter holds much promise for our future science, discovery, and exploration missions to Mars."

NASA Mars Helicopter Technology Demonstration

Video above: The Mars Helicopter is a technology demonstration that will travel to the Red Planet with the Mars 2020 rover. It will attempt controlled flight in Mars' thin atmosphere, which may enable more ambitious missions in the future.

U.S. Rep. John Culberson of Texas echoed Bridenstine's appreciation of the impact of American firsts on the future of exploration and discovery.

"It's fitting that the United States of America is the first nation in history to fly the first heavier-than-air craft on another world," Culberson said. "This exciting and visionary achievement will inspire young people all over the United States to become scientists and engineers, paving the way for even greater discoveries in the future."

Started in August 2013 as a technology development project at NASA's Jet Propulsion Laboratory, the Mars Helicopter had to prove that big things could come in small packages. The result of the team's four years of design, testing and redesign weighs in at little under four pounds (1.8 kilograms). Its fuselage is about the size of a softball, and its twin, counter-rotating blades will bite into the thin Martian atmosphere at almost 3,000 rpm -- about 10 times the rate of a helicopter on Earth.

"Exploring the Red Planet with NASA's Mars Helicopter exemplifies a successful marriage of science and technology innovation and is a unique opportunity to advance Mars exploration for the future," said Thomas Zurbuchen, Associate Administrator for NASA's Science Mission Directorate at the agency headquarters in Washington. "After the Wright Brothers proved 117 years ago that powered, sustained, and controlled flight was possible here on Earth, another group of American pioneers may prove the same can be done on another world."

The helicopter also contains built-in capabilities needed for operation at Mars, including solar cells to charge its lithium-ion batteries, and a heating mechanism to keep it warm through the cold Martian nights. But before the helicopter can fly at Mars it has to get there. It will do so attached to the belly pan of the Mars 2020 rover.

"The altitude record for a helicopter flying here on Earth is about 40,000 feet. The atmosphere of Mars is only one percent that of Earth, so when our helicopter is on the Martian surface, it's already at the Earth equivalent of 100,000 feet up," said Mimi Aung, Mars Helicopter project manager at JPL. "To make it fly at that low atmospheric density, we had to scrutinize everything, make it as light as possible while being as strong and as powerful as it can possibly be."

Once the rover is on the planet's surface, a suitable location will be found to deploy the helicopter down from the vehicle and place it onto the ground. The rover then will be driven away from the helicopter to a safe distance from which it will relay commands. After its batteries are charged and a myriad of tests are performed, controllers on Earth will command the Mars Helicopter to take its first autonomous flight into history.

NASA's Mars 2020 Rover Artist's Concept. Image Credits: NASA/JPL

"We don't have a pilot and Earth will be several light minutes away, so there is no way to joystick this mission in real time," said Aung. "Instead, we have an autonomous capability that will be able to receive and interpret commands from the ground, and then fly the mission on its own."

The full 30-day flight test campaign will include up to five flights of incrementally farther flight distances, up to a few hundred meters, and longer durations as long as 90 seconds, over a period. On its first flight, the helicopter will make a short vertical climb to 10 feet (3 meters), where it will hover for about 30 seconds.

As a technology demonstration, the Mars Helicopter is considered a high-risk, high-reward project. If it does not work, the Mars 2020 mission will not be impacted. If it does work, helicopters may have a real future as low-flying scouts and aerial vehicles to access locations not reachable by ground travel.

"The ability to see clearly what lies beyond the next hill is crucial for future explorers," said Zurbuchen. "We already have great views of Mars from the surface as well as from orbit. With the added dimension of a bird's-eye view from a 'marscopter,' we can only imagine what future missions will achieve."

Mars 2020 will launch on a United Launch Alliance (ULA) Atlas V rocket from Space Launch Complex 41 at Cape Canaveral Air Force Station in Florida, and is expected to reach Mars in February 2021.

The rover will conduct geological assessments of its landing site on Mars, determine the habitability of the environment, search for signs of ancient Martian life, and assess natural resources and hazards for future human explorers. Scientists will use the instruments aboard the rover to identify and collect samples of rock and soil, encase them in sealed tubes, and leave them on the planet's surface for potential return to Earth on a future Mars mission.

The Mars 2020 Project at JPL in Pasadena, California, manages rover development for the Science Mission Directorate at NASA Headquarters in Washington. NASA's Launch Services Program, based at the agency's Kennedy Space Center in Florida, is responsible for launch management.

For more information about NASA's Mars missions, go to: https://www.nasa.gov/mars

Mars 2020 rover mission: https://www.nasa.gov/mars2020

Images (mentioned), Video, Text, Credits: NASA/Dwayne Brown/JoAnna Wendel/JPL/DC Agle.

Greetings, Orbiter.ch

vendredi 11 mai 2018

SpaceX - Bangabandhu Satellite-1 Mission Success












SpaceX - Falcon 9 / Bangabandhu-1 Mission patch.

May 11, 2018

Falcon 9 carrying Bangabandhu Satellite-1 launch

SpaceX successfully launched the Bangabandhu Satellite-1 on Friday, May 11 from Launch Complex 39A (LC-39A) at NASA’s Kennedy Space Center, Florida. Liftoff occurred at 4:14 p.m. EDT and Bangabandhu Satellite-1 was deployed into a geostationary transfer orbit (GTO) approximately 33 minutes after launch.

Bangabandhu Satellite-1 Mission

The Bangabandhu Satellite-1 mission served as the first flight of Falcon 9 Block 5, the final substantial upgrade to SpaceX’s Falcon 9 launch vehicle. Falcon 9 Block 5 is designed to be capable of 10 or more flights with very limited refurbishment as SpaceX continues to strive for rapid reusability and extremely high reliability. Following stage separation, SpaceX successfully landed Falcon 9’s first stage on the “Of Course I Still Love You” droneship in the Atlantic Ocean. This will be the first launch of the upgraded Block 5 version of SpaceX’s Falcon 9 rocket.

Bangabandhu 1 communications satellite

Bangabandhu 1 communications satellite for the Bangladesh Telecommunication Regulatory Commission. The spacecraft will provide broadcasting and telecommunication services to rural areas and introduce direct-to-home television programming across Bangladesh and neighboring countries. The Bangabandhu 1 satellite was built by Thales Alenia Space.

For more information about SpaceX, visit: http://www.spacex.com/

Images, Video, Text, Credits: SpaceX/Günter Space Page/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch

Station to Orbit Higher Before Spacewalk and Crew Landing











ISS - Expedition 55 Mission patch.

May 11, 2018

The International Space Station will be orbiting a little higher this weekend to prepare for the departure of three Expedition 55 crew members and the arrival of a new Russian cargo craft. The docked Russian Progress 69 resupply ship will fire its engines Saturday at 6:07 p.m. EDT for two minutes and 52 seconds slightly boosting the orbital lab’s altitude.


Image above: The six-member Expedition 55 crew poses inside the Harmony module which links both the Japanese Kibo and the European Columbus laboratory modules. In the bottom row from left, are Soyuz MS-08 crew members Drew Feustel, Ricky Arnold and Oleg Artemyev. In the top row from left, are Soyuz MS-07 crew members Anton Shkaplerov, Scott Tingle and Norishige Kanai. Image Credit: NASA.

This orbital reboost sets up the proper phasing trajectory for the Soyuz MS-07 spacecraft when it undocks June 3.  The Soyuz will carry Commander Anton Shkaplerov and Flight Engineers Scott Tingle and Norishige Kanai back to Earth after six-and-a-half month mission in space. The reboost will also enable a two-orbit launch to docking opportunity for Russia’s next resupply ship the Progress 70 in July.

Overnight and early Friday morning robotics controllers from the Japan Aerospace Exploration Agency supported the deployment of small satellites from outside the Kibo laboratory module. The Japanese robotic arm attached to Kibo ejected several small satellites to support a series of technology demonstrations.


Image above: Flying over North Pacific Ocean, seen by EarthCam on ISS, speed: 27'615 Km/h, altitude: 404,49 Km, image captured by Roland Berga (on Earth in Switzerland) from International Space Station (ISS) using ISS-HD Live application with EarthCam's from ISS on May 10, 2018 at 22:22 UTC. Image Credits: Orbiter.ch Aerospace/Roland Berga.

Two spacewalkers and a pair of Flight Engineers continued more computer training and procedure reviews today ahead of next week’s spacewalk. NASA astronauts Ricky Arnold and Drew Feustel will go outside in their U.S. spacesuits Wednesday for about 6.5 hours to swap out thermal control gear that cools external station systems. Tingle and Kanai will assist the duo in and out of the Quest airlock and help choreograph the spacewalk tasks.

Related links:

NASA TV: https://www.nasa.gov/multimedia/nasatv/index.html

Expedition 55: https://www.nasa.gov/mission_pages/station/expeditions/expedition55/index.html

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Images (mentioned), Text, Credits: NASA/Mark Garcia/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

Hubble Spies Glowing Galaxies in Massive Cluster











NASA - Hubble Space Telescope patch.

May 11, 2018


In the darkness of the distant universe, these galaxies resemble glowing fireflies, flickering candles, charred embers floating up from a bonfire, and light bulbs softly shining. This image, captured by the NASA/ESA Hubble Space Telescope, shows a massive group of galaxies bound together by gravity: a cluster named RXC J0032.1+1808.

This image was taken by Hubble’s Advanced Camera for Surveys and Wide Field Camera 3 as part of an observing program called RELICS (Reionization Lensing Cluster Survey). RELICS imaged 41 massive galaxy clusters with the aim of finding the brightest distant galaxies for the forthcoming James Webb Space Telescope to study.

Hubble Space Telescope (HST)

Expected to launch in 2020, the Webb telescope is designed to see in infrared wavelengths, which is exceedingly useful for observing distant objects. As a result of the expansion of the universe, very distant objects are highly redshifted (their light is shifted toward the redder end of the spectrum), and so infrared telescopes are needed to study them. While Hubble currently has the ability to peer billions of years into the past to see “toddler” galaxies, the Webb telescope will have the capability to study “baby” galaxies, the first galaxies that formed in the universe.

Related link:

RELICS (Reionization Lensing Cluster Survey): https://relics.stsci.edu/

For more information about Hubble, visit:

http://hubblesite.org/
http://www.nasa.gov/hubble
http://www.spacetelescope.org/

Image, Animation, Text, Credits: ESA/Hubble & NASA, RELICS/Text: European Space Agency/NASA/Karl Hille.

Greetings, Orbiter.ch

Space Station Science Highlights: Week of May 7, 2018











ISS - Expedition 55 Mission patch.

May 11, 2018

This week, the crew members aboard the International Space Station continued scientific operations and spacewalk preparation as tons of science and hardware returned to Earth aboard the SpaceX Dragon capsule on Saturday, May 5.

International Space Station (ISS). Image Credit: NASA

NASA astronauts Ricky Arnold and Drew Feustel will conduct the 210th spacewalk at the space station beginning Wednesday, May 16. The veteran spacewalkers will work to swap thermal control gear that controls the circulation of ammonia to keep external station systems cool. NASA TV begins its live coverage at 6:30 a.m.

Here is a look at some of the science that happened this week aboard your orbiting laboratory:

Crew member examines blood vessels and heart

Cardiac and Vessel Structure and Function with Long-Duration Space Flight and Recovery (Vascular Echo) examines changes in blood vessels and the heart, both in space and on Earth. The results may provide insight into potential countermeasures to help maintain crewmember health, and quality of life for those on Earth.


Animation above: NASA astronaut Scott Tingle works within the CIR as a part of the ACME E-FIELD Flames investigation. Animation Credit: NASA.

This week, a crewmember attached Electrocardiogram (ECG) electrodes to himself, marked his femoral artery and then performed an ultrasound scan with remote guidance from the ground team.

Imagery contributes to study of Intracranial Pressure

The Non-invasive Assessment of Intracranial Pressure for Spaceflight and Related Visual Impairment (IPVI) investigation studies changes to crewmembers’ eyes and optic nerves by analyzing arterial blood pressure and blood flow to the brain before and after spaceflight. This investigation uses non-invasive methods to measure intracranial pressure, rather than commonly used more invasive methods.


Image above: The SpaceX Dragon capsule, pictured above, returned to Earth Saturday full of science and hardware. Image Credit: NASA.

This week, a crewmember took front and side photographs to check for any facial swelling, followed by a conference with ground experts.

Studying crew culture

The Culture, Values, and Environmental Adaptation in Space (At Home in Space) investigation, sponsored by the Canadian Space Agency, looks at changes in perceptions about home in space and the ways a unique culture may develop aboard the station during a mission.


Animation above: The SpaceX Dragon capsule departs the International Space Station, carrying with it samples and hardware from research conducted aboard the orbiting laboratory. Animation Credit: NASA.

Participants answer a series of questionnaires before, during and after flight, enabling researchers to see whether perceptions and the relative importance of values change over the course of a mission. Questions explore individual and culturally related differences, family functioning and relationships, personal values and coping with stress. This week, a crew member completed the questionnaire prior to his midday meal.

Space to Ground: Ready for a Walk: 05/11/2018

Other work was done on these investigations: Crew Earth Observations, Veggie PONDS, CBEF, CIR, Multi-Use Variable-g platform (MVP), MERLIN, Probiotics, Radi-N2, ELF, Microbial Tracking-2, J-SSOD #8, and Food Acceptability.

Related links:

NASA TV: https://www.nasa.gov/multimedia/nasatv/index.html

Vascular Echo: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1664

At Home in Space: https://www.nasa.gov/mission_pages/station/research/at_home_in_space

Crew Earth Observations: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=84

Veggie PONDS: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7581

CBEF: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=333

CIR: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=317

Multi-Use Variable-g platform (MVP): https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=1777

MERLIN: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=29

Probiotics: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=2047

Radi-N2: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=874

ELF: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1738

Microbial Tracking-2: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1663

J-SSOD: http://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=883

Food Acceptability: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7562

Spot the Station: https://spotthestation.nasa.gov/

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Images (mentioned), Animations (mentioned), Video, Text, Credits: NASA/Michael Johnson/Yuri Guinart-Ramirez, Lead Increment Scientist Expeditions 55 & 56.

Best regards, Orbiter.ch

jeudi 10 mai 2018

Virtual Reality Training and Global Robotics Work Before Spacewalk











ISS - Expedition 55 Mission patch.

May 10, 2018

Two Expedition 55 Flight Engineers are using virtual reality and computer training today to prepare for next week’s spacewalk at the International Space Station. Robotics controllers from Houston and Japan are also maneuvering a pair of robotic arms for the upcoming spacewalk and satellite deployments.


Image above: The Kibo laboratory module from the Japan Aerospace Exploration Agency was pictured as the International Space Station orbited over the southern Pacific Ocean east of New Zealand. Image Credit: NASA.

NASA astronauts Ricky Arnold and Drew Feustel will conduct the 210th spacewalk at the space station beginning Wednesday, May 16 at 8:10 a.m. EDT. The veteran spacewalkers will work for about 6.5 hours swapping thermal control gear that controls the circulation of ammonia to keep external station systems cool. NASA TV begins its live coverage at 6:30 a.m.

The veteran spacewalkers checked the functionality a pair of jet packs that will be attached to their U.S. spacesuits next week. The jet packs, known as Simplified Aid For EVA Rescue (SAFER), provide mobility for spacewalkers in the unlikely event they become untethered from the station. The duo also wore virtual reality goggles to practice maneuvering their SAFER jet packs and reviewed their spacewalk procedures.


Image above: Flying over North Pacific Ocean, seen by EarthCam on ISS, speed: 27'615 Km/h, altitude: 404,49 Km, image captured by Roland Berga (on Earth in Switzerland) from International Space Station (ISS) using ISS-HD Live application with EarthCam's from ISS on May 10, 2018 at 22:22 UTC. Image Credits: Orbiter.ch Aerospace/Roland Berga.

Robotics controllers from opposite sides of the world maneuvered a pair of robotic arms independently of each other today. Canada’s 57.7-foot-long robotic arm, nicknamed Canadarm2, was remotely positioned today by engineers in Houston in advance of next week’s spacewalk activities. Controllers from the Japan Aerospace Exploration Agency remotely operated the Kibo laboratory module’s robotic arm to prepare for the deployment of small satellites Friday morning.

Related links:

Canadarm2: https://www.nasa.gov/mission_pages/station/structure/elements/mss.html

Kibo laboratory module: https://www.nasa.gov/mission_pages/station/structure/elements/jem.html

NASA TV: https://www.nasa.gov/multimedia/nasatv/index.html

Expedition 55: https://www.nasa.gov/mission_pages/station/expeditions/expedition55/index.html

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Images (mentioned), Text, Credits: NASA/Mark Garcia/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

NASA’s NICER Mission Finds an X-ray Pulsar in a Record-fast Orbit















ISS - Neutron star Interior Composition Explorer (NICER) patch.

May 10, 2018

Scientists analyzing the first data from the Neutron star Interior Composition Explorer (NICER) mission have found two stars that revolve around each other every 38 minutes — about the time it takes to stream a TV drama. One of the stars in the system, called IGR J17062–6143 (J17062 for short), is a rapidly spinning, superdense star called a pulsar. The discovery bestows the stellar pair with the record for the shortest-known orbital period for a certain class of pulsar binary system.

The data from NICER also show J17062’s stars are only about 186,000 miles (300,000 kilometers) apart, less than the distance between Earth and the Moon. Based on the pair’s breakneck orbital period and separation, scientists involved in a new study of the system think the second star is a hydrogen-poor white dwarf.

“It’s not possible for a hydrogen-rich star, like our Sun, to be the pulsar’s companion,” said Tod Strohmayer an astrophysicist at Goddard and lead author on the paper. “You can’t fit a star like that into an orbit so small.”

NICER Finds X-ray Pulsar in Record-fast Orbit

Video above: The stars of IGR J17062–6143, illustrated here, circle each other every 38 minutes, the fastest-known orbit for a binary system containing an accreting millisecond X-ray pulsar. As they revolve, a superdense pulsar pulls gas from a lightweight white dwarf. The two stars are so close they would fit between Earth and the Moon. Video Credits: NASA’s Goddard Space Flight Center.

A previous 20-minute observation by the Rossi X-ray Timing Explorer (RXTE) in 2008 was only able to set a lower limit for J17062’s orbital period. NICER, which was installed aboard the International Space Station last June, has been able to observe the system for much longer periods of time. In August, the instrument focused on J17062 for more than seven hours over 5.3 days. Combining additional observations in October and November, the science team was able to confirm the record-setting orbital period for a binary system containing what astronomers call an accreting millisecond X-ray pulsar (AMXP).

When a massive star goes supernova, its core collapses into a black hole or a neutron star, which is small and superdense — around the size of a city but containing more mass than the Sun. Neutron stars are so hot the light they radiate passes red-hot, white-hot, UV-hot and enters the X-ray portion of the electromagnetic spectrum. A pulsar is a rapidly spinning neutron star.

The 2008 RXTE observation of J17062 found X-ray pulses recurring 163 times a second. These pulses mark the locations of hot spots around the pulsar’s magnetic poles, so they allow astronomers to determine how fast it’s spinning. J17062’s pulsar is rotating at about 9,800 revolutions per minute. 

Hot spots form when a neutron star’s intense gravitational field pulls material away from a stellar companion — in J17062, from the white dwarf — where it collects into an accretion disk. Matter in the disk spirals down, eventually making its way onto the surface. Neutron stars have strong magnetic fields, so the material lands on the surface of the star unevenly, traveling along the magnetic field to the magnetic poles where it creates hot spots.

Neutron Star Interior Composition Explorer (NICER). Image Credit: NASA

The constant barrage of in-falling gas causes accreting pulsars to spin more rapidly. As they spin, the hot spots come in and out of the view of X-ray instruments like NICER, which record the fluctuations. Some pulsars rotate over 700 times per second, comparable to the blades of a kitchen blender. X-ray fluctuations from pulsars are so predictable that NICER’s companion experiment, the Station Explorer for X-ray Timing and Navigation Technology (SEXTANT), has already shown they can serve as beacons for autonomous navigation by future spacecraft.

Over time, material from the donor star builds up on the surface of the neutron star. Once the pressure of this layer builds up to the point where its atoms fuse, a runaway thermonuclear reaction occurs, releasing the energy equivalent of 100 15-megaton bombs exploding over every square centimeter, explained Strohmayer. X-rays from such outbursts can also be captured by NICER, although one has yet to be seen from J17062.

The researchers were able to determine that J17062’s stars revolve around each other in a circular orbit, which is common for AMXPs. The white dwarf donor star is a “lightweight,” only around 1.5 percent of our Sun’s mass. The pulsar is much heavier, around 1.4 solar masses, which means the stars orbit a point around 1,900 miles (3,000 km) from the pulsar. Strohmayer said it’s almost as if the donor star orbits a stationary pulsar, but NICER is sensitive enough to detect a slight fluctuation in the pulsar’s X-ray emission due to the tug from the donor star.

“The distance between us and the pulsar is not constant,” Strohmayer said. “It’s varying by this orbital motion. When the pulsar is closer, the X-ray emission takes a little less time to reach us than when it’s further away. This time delay is small, only about 8 milliseconds for J17062's orbit, but it’s well within the capabilities of a sensitive pulsar machine like NICER.”

The results of the study were published May 9 in The Astrophysical Journal Letters.


Image above: Artist's illustration of The stars of IGR J17062–6143, illustrated here, circle each other every 38 minutes, the fastest-known orbit for a binary system containing an accreting millisecond X-ray pulsar. Image Credit: NASA’s Goddard Space Flight Center.

NICER’s mission is to provide high-precision measurements to further study the physics and behavior of neutron stars. Other first-round results from the instrument have provided details about one object’s thermonuclear bursts and explored what happens to the accretion disk during these events.

“Neutron stars turn out to be truly unique nuclear physics laboratories, from a terrestrial standpoint,” said Zaven Arzoumanian, a Goddard astrophysicist and lead scientist for NICER. “We can’t recreate the conditions on neutron stars anywhere within our solar system. One of NICER’s key objectives is to study subatomic physics that isn’t accessible anywhere else.”

NICER is an Astrophysics Mission of Opportunity within NASA's Explorer program, which provides frequent flight opportunities for world-class scientific investigations from space utilizing innovative, streamlined, and efficient management approaches within the heliophysics and astrophysics science areas. NASA's Space Technology Mission Directorate supports the SEXTANT component of the mission, demonstrating pulsar-based spacecraft navigation.

Related links:

Neutron star Interior Composition Explorer (NICER): https://www.nasa.gov/nicer

Rossi X-ray Timing Explorer (RXTE): https://heasarc.gsfc.nasa.gov/docs/xte/xhp_geninfo.html

Station Explorer for X-ray Timing and Navigation Technology (SEXTANT): https://gameon.nasa.gov/projects/deep-space-x-ray-navigation-and-communication/

The Astrophysical Journal Letters: http://iopscience.iop.org/article/10.3847/2041-8213/aabf44

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Images (mentioned), Video (mentioned), Text, Credits: NASA/Rob Garner/Goddard Space Flight Center, by Jeanette Kazmierczak.

Greetings, Orbiter.ch